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Home • [Police Standing Up] John Thomson – Former QLD Police
[Police Standing Up] John Thomson – Former QLD Police
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QLD Senior Sergeant John Thomson explains the bizarre experiences on the QLD Border during the pandemic and changed his view from very concerned to – what's going on here? "How does the virus know that you've got that permit? How does a permit protect you from a deadly virus?" Many examples like that just didn't make sense. Vaccinated people not being allowed to cross the border to see a dying family member but the whole National Rugby League could cross including their families and kids. He said that being a police officer, you investigate crime, and he has an objective opinion about the criminal history of J&J, Pfizer, and AstraZeneca and compares them to conmen.
Senior Sergeant John Thomson
Rumble | Vimeo
14 Oct 2021 – QLD Police officer Senior Sergeant John Thomson gives his testimony on why he will not take the vax.
Brisbane, Australia. 19 Year Career that I loved.
At the start, I was concerned about Covid, but after a few months of being on the border, my attitude started to change about the virus and the whole covid.
I was there at the border for 18 months, no mask, unvaccinated, and was having people coming from all over from Victoria & New South Wales and I started recognize that if you "had a piece of paper, a permit issued by the CHO – that protected you from the virus"
One evening I remember that certain areas were designated hot spots and they couldn't cross the border. So this guy turns up to the border 24 hours later from one of those locations and I said you can't cross – and he pulled out all this paperwork – a letter from the CHO – objectively, I was like "How does the virus know that you've got that permit? How does it protect you?" Many, many, many examples like that just didn't make sense.
The other example – you hear on the news that the QLD govt wouldn't allow people to come into Queensland from New South Wales to see a dying family member – but then the whole National Rugby League could come up to Queensland – and their families – and their kids.
Then you'd have your lockdowns but if State of Origins was on, you can go "as long as you have your mask to enter the football stadium, but when you sit down, you take the mask off"? I mean – objectively it doesn't make any sense, "does the virus know when you're standing up and sitting down?" – It's bizarre.
On top of that, people coming in from Overseas – Tom Hanks came in back in early 2020 – off he goes, staying in the Hinterland on the Gold Coast, and didn't have to stay in quarantine like all us plebs – if it's as deadly as what you make it out it is – then one rule fits all, period.
Being a police officer, you investigate crime, and one of the things that stand out in my mind is that these companies J&J, Pfizer, AstraZeneca – they've all got criminal history.
J&J had to pay out 5 billion this year, 2021 in criminal fines
AstraZeneca, 1.5 Billion.
Pfizer 4.5 Billion.
These guys don't have a good track record, they're not the most outstanding businessmen and women on the planet. If you have a known con-artist, let's say the famous Australian, Peter Foster I think it is – and he goes "Oh I've got some insurance to sell you" – what are you going to say? You're gonna say "Um, get stuffed mate, not interested". That's what you're going to say – that's normal – that's how anyone will react, and yet these people have got a rapt sheet of that sort of behaviour, and you come to realize – they're a bunch of grubs
Point 2 – they are exempt! Exempt from litigation. So if you have an adverse reaction to the vax, a leg gets chopped off or whatever it may be – you got nothing – can't sue them because they're exempt from litigation. Would you buy a brand new fridge from the Good Guys if you had no warranty? Would you buy a brand new car from Ford if you had no warranty? Of course you wouldn't – and yet, we've got that happening here.
Point 3 – This is the biggest one. It's not time-tested. Scientists, doctors, you can all bang on til the cows come home – we've spent all this money and this is the best, and its tested safe and blah, blah – it's not time-tested. You can't give it time. You can throw billions of dollars into it – but you can't give it time. That's my biggest issue – I don't know what the long-term effects of this is going to be – NOBODY does. That's the point!
Do we have any examples of that in history? Yes we do. Drug was used for morning sickness, many women went and used it and 12-15 months later, children being born with missing arms and missing legs and thousands of kids died. We have history of things that are not time-tested.
Thalidomide Documentary (Telegram)
How long was Polio tested before it came out? 30 years?
Before you say "he's an antivaxxer" – I take offence to that – it's like me calling you some rude word – no substance to it. but it's offensive – that is offensive. I was vaxxed when I was a kid, and went to countries where I had to be vaxxed, ok? So please, don't be lazy and tell me that I'm antivax – that's B.S.
These are not time-tested and that is my concern – it does my head in, trying to say – it's a legitimate concern… my body, my choice, right? Isn't it? It's my body – it's not the governments body – it's mine. I have that right, or I certainly should be able to make a decision without fear or favour. I should be able to make a decision without coercion, or threats, and yet here we are.
We're living in interesting times people, we're living in interesting times Australia.
Like when you're hearing politicians like Dan Andrews in Victoria talking about the vaccine "passport" – what's that all about? If you've got the vax, free-reign, and if you don't have it, you're restricted; they're starting to talk about this concept – I went to China, and there's a 2-tier society over there. If you're a party member you have privileges, if you're not a party member you're stuffed. What I see with this whole thing at the moment, is some type of Medical Communism. If you don't follow the medical procedure, then you're discriminated against.
Senior Constable John Thomson was stood down by the Queensland Police Service (QPS) in December 2021 for not taking the COVID Vaccination. Here are some follow-up videos:
Millions March v1 – John Thomson Speech
Nov 2021 – This speech is so good but I can't download or embed it. Please see it on Vimeo
Vaccinations – do they even work?
Vimeo | Rumble
Jan 2022 – Quick Update, what's been going on in the state last few days – just had a quick look on the news there, apparently the watch house at Ipswich had been shut for several hours and emails sent to staff to avoid arresting people due to covid outbreaks. We've got approx 49 officers at Beenleigh that had to Isolate about 2 weeks ago due to a Covid-Positive down there. We've got 52 officers at the Gold Coast that had to stand-down and isolate because of covid-positives down there.
I was mandated to get the vaccine and chose not to, and the reason they mandated the vaccine was so that we didn't have the reduction in the 'thin blue line' that's already thin. And yet, all these officers are fully-vaccinated and some have had their 3rd jab, and they've got to isolate because they've come in contact with a covid-positive? Or they've tested positive – I thought the whole concept, the whole reason for getting the vaccine was to prevent this from happening, and here we are seeing covid-positive officers having to go home and not work, emails being sent telling them not to arrest anyone where possible because of Covid… How does that work? Please explain that to me?
I just wanted to remind everybody that covid-19 has a survival-rate of 99.7% More people died in 2021 of falling-over in Australia, than they did of covid.
The average age of a person that passed-away was 86.
The average age of mortality rate in Australia was 83.
I want you to think long and hard about those ages and the survival rate, and ask yourself is it justifiable to mandate the entire country to receive a vaccine that clearly does not do what it's supposed to.
Canberra Update
Feb 2022 – "As a cop, we've been told to be impartial, not to take sides, be neutral, but you know what? I'm partial to "Freedom", and because I'm partial to freedom, that means I can't be impartial anymore. So now, we stand with the people. We want our freedoms back – we've had enough. God bless you guys! Australia Rocks!"
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Life is short, and if we remember to really appreciate it instead of taking it for granted, we can infuse every moment with joy.
— https://pennybutler.com/4things/


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\section{}

\section{Introduction}

The general method of constructing spacetime by generating manifolds of revolution around a given curve was recently formulated to study curved traversable wormholes \cite{Vee2013,Vee2012} \footnote{The original motivation that led to this formulation came from trying to helicalise a given curve \cite{Vee2013b}, i.e. replacing the given curve by another curve which winds around it.}. This follows from the ideas of Morris and Thorne \cite{Kip} that in finding solutions to general relativity, a spacetime geometry is first constructed and the Einstein field equations are subsequently used to determine the required materials to support it. Following the publication of Morris and Thorne's work, there has been intense research in the area of traversable wormholes, with a major result being the necessity of exotic matter to be present \cite{Vis2}. A useful application of the general method in \cite{Vee2013,Vee2012} is the construction of curved traversable wormholes which does not assume spherical symmetry. This led to the finding that by carefully engineering the shape and curvature of curved wormholes, it is possible for such wormholes to admit safe geodesics through them, i.e. freely-falling trajectories which are locally supported by ordinary matter, thereby avoiding the need for travellers to get into direct contact with exotic matter.

Here is how (3+1)-d spacetimes are constructed using that method. Given a smooth curve $\psi(v)$ embedded in a 4-d Euclidean space, a 3-manifold of revolution is:
\begin{eqnarray}\label{genmanifold}
\vec{\sigma}(u,v,w)=\psi(v)+Z(v)\cos{u}\ \vec{n}_1(v)+Z(v)\sin{u}\cos{w}\ \vec{n}_2(v)+Z(v)\sin{u}\sin{w}\ \vec{n}_3(v),
\end{eqnarray}
where $Z(v)$ is the radial function and $\vec{n}_1(v),\vec{n}_2(v),\vec{n}_3(v)$ are three orthonormal vectors. The metric of this 3-manifold can be calculated, and then extended to a (3+1)-d spacetime metric. This method can also be used to build dynamical spacetimes, as \cite{Vee2013} explicitly illustrated how an inflating wormhole can be constructed by letting the given curve $\psi(v)$ and the radial function $Z(v)$ depend on time.

In this paper, we would like to explore how the general method can be used to construct a rotating spacetime, and identify the essential attributes of the matter which produce this phenomenon. To investigate this in a simple model, extending a static traversable wormhole to a rotating one would not be ideal since it requires matter (exotic in some region) to already be present. It is instead advantageous to extend from an originally vacuum spacetime, since the matter that would be present is solely responsible for the rotational effects of the spacetime. Apart from the trivially flat Minkowski geometry, a Schwarzschild geometry is also vacuum (excluding the black hole, of course). We would hereby construct a rotating universe outside (the event horizon of) a black hole, where the spacetime itself rotates, and obtain the Minkowski version as the special case of zero black hole mass. To take full advantage of the spherical symmetry of the Schwarzschild geometry, the universe is prescribed to rotate in layers of rigid spherical shells. However, these shells of various radii need not be rotating with the same angular velocity (see Fig. 1), so the universe as a whole would not be rigidly rotating. This would be interesting, as we can compare such a non-uniformly rotating universe to an expanding universe which is isotropic and homogeneous (the FLRW solution), expanding in all directions whilst carrying the matter (or galaxies) along with it \cite{Gra}. Note also that we are going to assume that the mass-energy is static, unlike the van Stockum \cite{Stockum}, Tipler \cite{Tip} or Kerr \cite{VisserKerr} solutions which describe rotating matter. This helps to simplify the metric, since those examples necessarily contain a non-zero $g_{t\phi}$ cross-term which would lead to significantly arduous calculations and possibly obfuscate the interpretations of the matter properties, if incorporated into our model \footnote{As seen in the next section, the spatial 3-manifold representing a non-uniformly rotating universe would itself contain a $g_{v\phi}$ spatial cross-term.}.

\begin{figure}
\centering
\includegraphics[width=10cm]{fig1.png}
\caption{Each spherical shell rigidly rotates, but spherical shells of different radii may be rotating with different angular velocities.}
\label{fig1}
\end{figure}

In the next section, we construct the metric that describes a non-uniformly rotating spacetime around a Schwarzschild black hole by generating a 3-manifold of revolution around a straight line. In section 3, we decide on the choice of parametrisation for the straight line and the radial function, showing how the freedom in parametrisation leads to various coordinate systems that describe the Schwarzschild metric. Section 4 is devoted to the physical properties of the mass-energy fluid that give rise to such a rotating spacetime, with a discussion section following after. Section 6 concludes this paper. We shall be working in units where $G=c=1$.

\section{The metric construction}

Consider the following time-dependent 3-manifold of revolution around a straight line embedded into a 4-d Euclidean space:
\begin{eqnarray}\label{rotmanifold}
\vec{\sigma}(t,v,\theta,\phi)=
\left(
\begin{array}{c}
r(v)\cos{\theta}\\
r(v)\sin{\theta}\cos{(\phi+\chi(v)\omega t)}\\
r(v)\sin{\theta}\sin{(\phi+\chi(v)\omega t)}\\
z(v)
\end{array}
\right),
\end{eqnarray}
where $t$ is the time coordinate as measured by a faraway observer, $r$, $\theta$ and $\phi$ being the usual spherical coordinates for 3-d Euclidean space, and $z$ is the fourth spatial coordinate \footnote{A useful lower-dimensional analogue for visualisation is to think of embedding a 2-d surface into ordinary 3-d Euclidean space using cylindrical coordinates $r$, $\phi$ and $z$ so that $r$ and $\phi$ are the usual plane polar coordinates with $z$ being the third spatial coordinate. The general framework for generating surfaces of revolution by adding circles or 1-spheres to a given curve is described in \cite{Vee2012}.}. The symbol $\omega$ is a constant, with $v$ parametrising the radial coordinate $r(v)$ and the fourth spatial coordinate $z(v)$, so it can be thought of that one is a function of the other, viz. $z(r)$ or $r(z)$. This effectively determines the shape of the manifold of revolution around the straight line.

Disregarding the $\chi(v)\omega t$ term, this 3-manifold of revolution obtained by adding spheres of radii $r(v)$ along the straight line $\vec{L}(v)=(0,0,0,z(v))$ is a special case of the general method used in \cite{Vee2013} to construct static curved traversable wormholes \footnote{Note that in \cite{Vee2013}, the coordinates $u$ and $w$ were used in place of $\theta$ and $\phi$, with the radial function denoted as $Z(v)$ (see Eq. (\ref{genmanifold})). The reason such general symbols were used was because they were not the usual spherical coordinates as the given curve (which was not necessarily a straight line since curved wormholes were to be constructed) would naturally induce a more general coordinate system. Here, the focus is on manifolds of revolution around a straight line (in fact rotating about that line) so we are indeed working with the three usual spherical coordinates $r,\theta,\phi$ plus the fourth spatial coordinate $z$.}. The time-dependence built in here by replacing $\phi\rightarrow \phi+\chi(v)\omega t$ from the static version in Eq. (\ref{genmanifold}) to yield Eq. (\ref{rotmanifold}) represents the fact that a spherical shell of radius $r(v)$ is rotating about the fourth coordinate axis $z$ (or the line $\vec{L}$) with constant angular velocity $\chi(v)\omega$. This can be seen by choosing any particular point on the 3-manifold i.e. fixing some values of $v,\theta,\phi$, and noting that as $t$ evolves this point would be rotated by an angle of $\chi(v)\omega t$ about $\vec{L}$. The $v$-dependence on $\chi$ implies that spheres of different radii $r(v)$ which are added at different points on $\vec{L}(v)$ may in general be rotating with different angular velocities, although we would require that this variation is smooth with $v$.

For physical interest that we would like to consider here in this study, the following conditions are imposed:
\begin{enumerate}[(i)]
\item
$\chi\rightarrow0$ as $v\rightarrow\infty$ so that when extended to a (3+1)-d spacetime manifold, a faraway observer would be sitting on an asymptotically flat manifold which is non-rotating. Physical observations shall be discussed with respect to this inertial frame.
\item
$\chi(v_0)$ is normalised to 1 at some reference point where the parameter is $v_0$. This reference spherical shell of radius $r(v_0)$ would then be rotating with angular velocity $\omega$.
\item
$\chi(v)$ monotonically decreases as $v$ goes from $v_0$ to $\infty$.
\end{enumerate}
The first two are boundary conditions that prohibit $\chi$ from being a constant (since it has to be 1 at $v_0$ and 0 at $\infty$), so the universe is rotating non-uniformly in contrast to being in a rigid rotation. This means that there is no observer that would see the universe as being globally static. Any observer that may be locally static would necessarily see at least one other spherical shell rotating. The third condition would demand that the bulk of the mass-energy be concentrated near the axis of rotation, diminishing away from it. Some kind of mass-energy distribution in the universe whose properties are to be found through the Einstein field equations would cause the universe itself to behave like a swirling fluid with maximum rate of swirling at the centre, and dissipating with essentially little or no swirling towards the outer edge. Note that this is not the same as the mass-energy being the said fluid that is rotating, rather it is the universe itself that is non-uniformly rotating \footnote{Like an expanding universe, the spacetime itself is expanding as opposed to the galaxies themselves moving away from each other.}.

The spatial metric $ds^2_{\textrm{space}}$ for the 3-manifold given by Eq. (\ref{rotmanifold}) can be computed as follows: the components are $g_{ij}=\vec{\sigma}_i\cdot\vec{\sigma}_j$, where $i,j\in\{v,\theta,\phi\}$, and $\vec{\sigma}_i$ denotes partial derivative with respect to $i$. This gives
\begin{eqnarray}
ds^2_{\textrm{space}}&=&(z'^2+r'^2+\chi'^2\omega^2t^2r^2\sin^2{\theta})dv^2+r^2d\theta^2+r^2\sin^2{\theta}\ d\phi^2\nonumber\\
&\ &+2\chi'\omega tr^2\sin^2{\theta}\ dvd\phi,
\end{eqnarray}
where explicit dependence on $v$ for $z(v),r(v),\chi(v)$ are suppressed for conciseness.
This spatial metric can also be written as,
\begin{eqnarray}
ds^2_{\textrm{space}}&=&(z'^2+r'^2)dv^2+r^2d\theta^2+r^2\sin^2{\theta}(\chi'\omega t\ dv+d\phi)^2,
\end{eqnarray}
indicating how the time-dependence term leads to the $dvd\phi$ cross-term, viz. $\phi\rightarrow\phi+\chi\omega t$ for the static to rotating manifold's parametric equations corresponds to $d\phi\rightarrow d(\phi+\chi\omega t)=d\phi+\chi'\omega t\ dv$ for their metrics. It is clear that a constant $\chi$ just gives the usual spherically symmetric metric (see section 7.2 in \cite{Vee2012}). Our boundary conditions however, forbid this for the non-uniform rotation case.

We can extend this to a spacetime metric of the form:
\begin{eqnarray}
ds^2&=&g_{tt}dt^2+(z'^2+r'^2)dv^2+r^2d\theta^2+r^2\sin^2{\theta}(\chi'\omega t\ dv+d\phi)^2,
\end{eqnarray}
where $g_{tt}<0$. Since we are chiefly concerned with the geometry outside a Schwarzschild black hole, $g_{tt}$ is a function of only $v$. We would not bother with the $g_{tj}$ ($j$ being any of the spatial coordinates $v,\theta,\phi$) cross-terms, taking them to be zero and impose the mass-energy to be static. This would greatly reduce the algebraic technicalities in calculating the Einstein tensor especially as the spatial metric itself already contains the $g_{v\phi}$ cross-term.

\section{Parametrisation of $z(v)$ and $r(v)$}

We should decide on the choice of parametrisation of $z(v)$ and $r(v)$, before proceeding with further computations. For the sake of discussion, let us consider the static spacetime so that $\omega=0$:
\begin{eqnarray}\label{staticmet}
ds^2&=&g_{tt}dt^2+(z'^2+r'^2)dv^2+r^2d\theta^2+r^2\sin^2{\theta}\ d\phi^2.
\end{eqnarray}
Amongst many possible parametrisations, two simple ones are linearly parametrising $r(v)=v$, or to linearly parametrise $z(v)=v$. The former is to treat the actual radial coordinate $r$ as the parameter itself, so that $z$ becomes a function of $r$ and the metric in Eq. (\ref{staticmet}) becomes
\begin{eqnarray}
ds^2&=&g_{tt}(r)dt^2+(z'(r)^2+1)dr^2+r^2d\theta^2+r^2\sin^2{\theta}\ d\phi^2.
\end{eqnarray}
If one goes on to calculate the Einstein tensor and solve the vacuum field equations, one would find that $z(r)=2\sqrt{R_s(r-R_s)}$ and $g_{tt}(r)=-(1-R_s/r)$, where $R_s$ is the Schwarzschild radius. This is the usual static spherically symmetric vacuum solution expressed in Schwarzschild coordinates and $z(r)=2\sqrt{R_s(r-R_s)}$ is recognised as Flamm's paraboloid.

If the latter parametrisation is used instead (which can also be thought of as linearly parametrising the line $\vec{L}$), then the metric in Eq. (\ref{staticmet}) becomes
\begin{eqnarray}
ds^2&=&g_{tt}(z)dt^2+(1+r'(z)^2)dz^2+r(z)^2d\theta^2+r(z)^2\sin^2{\theta}\ d\phi^2.
\end{eqnarray}
Solving the vacuum field equations gives $r(z)=z^2/4R_s+R_s$ and $g_{tt}(z)=-z^2/(z^2+4R_s^2)$. This is actually equivalent to the Einstein-Rosen coordinates if one rescales $z=2u\sqrt{R_s}$ \footnote{Matt Visser provides an excellent description on these various coordinate systems that cover only certain regions of the Schwarzschild geometry, which played a part in leading Einstein and Rosen to deduce the Einstein-Rosen bridge from their coordinates in \cite{EinRos}. The Einstein-Rosen coordinates are $ds^2=-u^2/(u^2+R_s)dt^2+4(u^2+R_s)du^2+(u^2+R_s)^2(d\theta^2+\sin^2{\theta}\ d\phi^2)$. See for instance chapter five in \cite{Vis2}.}. It is hereby obvious that they would have naturally interpreted from such coordinates that this represents a wormhole, since spheres of radii $r(z)=z^2/4R_s+R_s$ are added to the line $\vec{L}(z)=(0,0,0,z)$. With the radial function $r(z)>0$ for all $z\in{\mathbb R}$ and having a minimum value of $R_s$ at $z=0$, the geometrical picture of the spatial 3-manifold is a ``3-d straight tube'' with minimum radius $R_s$ at $z=0$ that grows into two asymptotically flat ends.

Those two parametrisations were rather effortless, i.e. setting either $r(v)=v$ or $z(v)=v$. As a third and perhaps not so straightforward example, isotropic coordinates can be obtained by the parametrisation $r(v)=v(1+R_s/4v)^2$ and $z(v)=(4v-R_s)\sqrt{R_s/4v}$ \footnote{The logical flow to arrive at this choice of parametrisation would be as follows: In isotropic coordinates, a spacetime metric takes the general form $ds^2=g_{tt}(v)dt^2+A(v)(dv^2+v^2d\theta^2+v^2\sin^2{\theta}\ d\phi^2)$. By comparing with our generic form in Eq. (\ref{staticmet}), we see that $z$ and $r$ has to satisfy $z'^2=r^2/v^2-r'^2$. By eliminating $z'^2$ in place of $r$ and $r'$, the vacuum field equation $G_{tt}=0$ reduces to $2v^2rr''=(r-vr')^2$, where $r(v)=v(1+R_s/4v)^2$ is a solution. It then follows that $z(v)=(4v-R_s)\sqrt{R_s/4v}$. Finally $g_{tt}(v)$ can be solved from other components of the vacuum field equations to give $g_{tt}(v)=-[(1-R_s/4v)/(1+R_s/4v)]^2$. The metric is hence $ds^2=-[(1-R_s/4v)/(1+R_s/4v)]^2dt^2+(1+R_s/4v)^4(dv^2+v^2d\theta^2+v^2\sin^2{\theta}\ d\phi^2)$, as anticipated. (See chapter 2.3.9 in \cite{Vis2}, for instance. Look out for the typo in Eq. (2.42) where $(1+r_s/4\rho)^2$ should be $(1+r_s/4\rho)^4$.)}. Fig. 2 shows how the same shape function is described by the three different parametrisations of $z(v)$ and $r(v)$ that are discussed here. It is thus intriguing that the various coordinate systems for the Schwarzschild geometry can be seen as arising from the freedom in parametrising $z(v)$ and $r(v)$ in the general method of constructing spacetime by generating manifolds of revolution around a given curve (in this case a straight line), as formulated in \cite{Vee2012,Vee2013} \footnote{In \cite{Vee2012,Vee2013} where static curved traversable wormholes were constructed, the parametrisations were essentially chosen from the beginning when the curve $\vec{\psi}(v)$ and the radial function $Z(v)$ were defined.}.

In our subsequent analysis of the rotating universe outside a Schwarzschild black hole, we shall adopt the parametrisation $r(v)=v$ which is the Schwarzschild coordinates.

\begin{figure}
\centering
\includegraphics[width=16cm]{fig2.png}
\caption{The same curve (with $R_s=1$) as described by (from left) Schwarzschild coordinates ($r$ is linearly parametrised), Einstein-Rosen coordinates ($z$ is linearly parametrised), and isotropic coordinates. Each dot on the curve represents an increment of $v$ by 1, beginning from $(r,z)=(R_s,0)$.}
\label{fig2}
\end{figure}

\section{Physical properties of a non-uniformly rotating universe outside a Schwarzschild black hole}

Let us return to describing a non-uniformly rotating universe outside a Schwarzschild black hole with Schwarzschild radius $R_s$. In Schwarzschild coordinates, the spacetime metric would be
\begin{eqnarray}\label{Schmet1}
ds^2&=&-\left(1-\frac{R_s}{r}\right)dt^2+\frac{1}{1-R_s/r}dr^2+r^2d\theta^2+r^2\sin^2{\theta}(\chi'(r)\omega t\ dr+d\phi)^2\\\label{Schmet2}
&=&-\left(1-\frac{R_s}{r}\right)dt^2+\left(\frac{1}{1-R_s/r}+\chi'(r)^2\omega^2t^2r^2\sin^2{\theta}\right)dr^2+r^2d\theta^2+r^2\sin^2{\theta}\ d\phi^2\nonumber\\&\ &+2\chi'(r)\omega tr^2\sin^2{\theta}\ drd\phi,
\end{eqnarray}
where $r\geq R_s$ is the region of interest. The Einstein tensor $G^{\mu\nu}=R^{\mu\nu}-Rg^{\mu\nu}/2$ can be calculated, with the following non-zero terms \footnote{It is obvious that $\omega=0$ gives $G^{\mu\nu}=0$, so that a non-rotating Schwarzschild geometry is Ricci flat.}:
\begin{eqnarray}
G^{tt}&=&-\frac{\chi'^2\omega^2r^3\sin^2{\theta}}{4(r-R_s)}\\
G^{rr}&=&\frac{1}{4}\chi'^2\omega^2r(r-R_s)\sin^2{\theta}\\
G^{\theta\theta}&=&-\frac{1}{4}\chi'^2\omega^2\sin^2{\theta}\\
G^{\phi\phi}&=&\frac{1}{4}\chi'^2\omega^2\left(\chi'^2\omega^2t^2r(r-R_s)\sin^2{\theta}-3\right)\\
G^{r\phi}&=&G^{\phi r}=-\frac{1}{4}\chi'^3\omega^3tr(r-R_s)\sin^2{\theta}\\
G^{t\phi}&=&G^{\phi t}=-\frac{\omega}{2r}(4\chi'+r\chi'')
\end{eqnarray}
A particularly interesting quick observation is that $G^{t\phi}=G^{\phi t}$ can be made to be identically zero if $\chi$ satisfies $4\chi'+r\chi''=0$. A solution to this is $\chi(r)=P/r^3+Q$ where $P,Q$ are arbitrary constants. The two boundary conditions for $\chi$ (see section 2) would be met if $P=R_s^3$ and $Q=0$, with the reference spherical shell being the horizon of the black hole $\chi(R_s)=1$ since the region observable by a faraway observer is $r\geq R_s$. The third condition is also met by $\chi(r)=(R_s/r)^3$. This leaves the non-zero components of $G^{\mu\nu}$ as
\begin{eqnarray}
G^{tt}&=&-\frac{9R_s^6\omega^2\sin^2{\theta}}{4r^5(r-R_s)}\\
G^{rr}&=&\frac{9R_s^6\omega^2(r-R_s)\sin^2{\theta}}{4r^7}\\
G^{\theta\theta}&=&-\frac{9R_s^6\omega^2\sin^2{\theta}}{4r^8}\\
G^{\phi\phi}&=&\frac{27}{4}R_s^6\omega^2\left(\frac{3R_s^6\omega^2t^2(r-R_s)\sin^2{\theta}-r^7}{r^{15}}\right)\\
G^{r\phi}&=&G^{\phi r}=\frac{27R_s^9\omega^3t(r-R_s)\sin^2{\theta}}{4r^{11}}.
\end{eqnarray}

The physics of the mass-energy that would result in such a non-uniformly rotating universe is given by the Einstein field equations $G^{\mu\nu}=8\pi T^{\mu\nu}$. With $\chi=(R_s/r)^3$, the $T^{t\phi}=T^{\phi t}$ terms are zero, so the simplest kind of mass-energy does not involve any heat transfer. In full, the non-zero components of $T^{\mu\nu}$ are:
\begin{eqnarray}\label{genTbegin}
T^{tt}&=&-\frac{9R_s^6\omega^2\sin^2{\theta}}{32\pi r^5(r-R_s)}\leq0\\
T^{rr}&=&\frac{9R_s^6\omega^2(r-R_s)\sin^2{\theta}}{32\pi r^7}\geq0\\
T^{\theta\theta}&=&-\frac{9R_s^6\omega^2\sin^2{\theta}}{32\pi r^8}\leq0\\
T^{\phi\phi}&=&\frac{27}{32\pi}R_s^6\omega^2\left(\frac{3R_s^6\omega^2t^2(r-R_s)\sin^2{\theta}-r^7}{r^{15}}\right)\\\label{genTend}
T^{r\phi}&=&T^{\phi r}=\frac{27R_s^9\omega^3t(r-R_s)\sin^2{\theta}}{32\pi r^{11}}\geq0\textrm{\ for\ }t\geq0.
\end{eqnarray}

A reassuring fact that can be inferred regarding the nature of the mass-energy density $T^{tt}$ is its time-independence. Note the contrast when compared to an expanding universe which dilutes the static material as it carries it along in the expansion. Here, there is no increase in volume since spherical shells of the universe are rotating but not expanding. The material density is naturally expected to be constant with time, lest mass-energy conservation be violated to produce the rotation.

As seen from the frame of a faraway observer, the mass-energy density $T^{tt}$ is negative and gets enormously large towards the horizon as $\displaystyle \lim_{r^+\rightarrow R_s}T^{tt}=-\infty$, though the $T^{rr}$ and $T^{r\phi}=T^{\phi r}$ stresses vanish at $r=R_s$. There are two (independent) components of the stress-energy tensor which are time-dependent, viz. $T^{\phi\phi}$ and $T^{r\phi}=T^{\phi r}$, where the former depends quadratically with time and linearly for the latter. The other two stresses $T^{rr}$ and $T^{\theta\theta}$ are time-independent. The field equations therefore reveal the astonishing effect of a mass-energy fluid whose stresses possess this directional dependence on time: Such static fluid, with time-dependent properties of $T^{\phi\phi}$ and $T^{r\phi}=T^{\phi r}$ would remarkably cause the universe to rotate, carrying the fluid along with it.

\begin{figure}
\centering
\includegraphics[width=8cm]{fig3.png}
\caption{The time-dependent stresses on a fluid element $T^{\phi\phi}$ (quadratic with time) and $T^{r\phi}=T^{\phi r}$ (linear with time) in the $\theta=\pi/2$ plane. The frame of a faraway observer would see the dotted circle trajectory of the static fluid element being carried along by the universe which rotates about a black hole. The time-independent stresses along the radial and $\theta$-directions are not shown.}
\label{fig3}
\end{figure}

Although a free particle cannot remain at rest outside a black hole (since the gravity of the black hole would attract the particle towards it), it is not difficult to imagine some kind of cosmological event where perhaps a red giant exploded and began collapsing into a black hole. During the explosion, the red giant would expel material outwards, eventually leading to a transient equilibrium state where the material is static outside the resulting black hole's event horizon for a period of time. The sign of $T^{\phi\phi}$ is negative for small $t$, indicating that the material is initially under tension along the $\phi$-direction. Over time, the sign of $T^{\phi\phi}$ changes to positive such that the material would be under increasing pressure. An example of a material whose pressure increases would be a nuclear process, whereby mass is converted into thermal energy which builds up the pressure over time, though in this situation the pressure increase only takes place along the $\phi$-direction and the $r\phi$-shears. A realistic scenerio of this non-uniformly rotating phenomenon would only be temporary, since the increase cannot go unbounded forever. Fig. 3 depicts the time-dependent stresses on a fluid element with increasing pressure along the $\phi$-direction and $r\phi$-shear forces.

Finally, consider the covariant null vector $k_\mu=((\sqrt{-g^{tt}})^{-1},0,0,(\sqrt{g^{\phi\phi}})^{-1})$. For $\theta\neq\pi/2$,
\begin{eqnarray}
T^{\mu\nu}k_\mu k_\nu=T^{tt}(k_t)^2+T^{\phi\phi}(k_\phi)^2=-\frac{9R_s^6\omega^2r\sin^2{\theta}}{8\pi[r^7+9R_s^6\omega^2(r-R_s)t^2\sin^2{\theta}]}<0,
\end{eqnarray}
implying that the null energy condition is violated \footnote{The null energy condition asserts that for any null vector, $T^{\mu\nu}k_\mu k_\nu\geq0$. This can be found in page 115 of \cite{Vis2}.}. This kind of mass-energy is therefore exotic in order to produce this non-uniformly rotating universe. The negativity of $T^{\mu\nu}k_\mu k_\nu$ for this null vector however, decreases with time.

\subsection{Minkowski spacetime ($R_s=0$)}

A non-uniformly rotating Minkowski spacetime can be thought of as the special case when the mass of the black hole is zero, or equivalently $R_s=0$. We cannot however, directly substitute $R_s=0$ into the stress-energy tensor because we chose $P=R_s^3$ to satisfy our two boundary conditions for $\chi$. To obtain the correct $T^{\mu\nu}$, we let $\chi=(R_0/r)^3$ with $R_0$ being a positive constant and only consider the region where $r\geq R_0$. The non-zero components of $T^{\mu\nu}$ corresponding to Eqs. (\ref{genTbegin}-\ref{genTend}) are
\begin{eqnarray}
T^{tt}&=&-\frac{9R_0^6\omega^2\sin^2{\theta}}{32\pi r^6}\leq0\\
T^{rr}&=&\frac{9R_0^6\omega^2\sin^2{\theta}}{32\pi r^6}\geq0\\
T^{\theta\theta}&=&-\frac{9R_0^6\omega^2\sin^2{\theta}}{32\pi r^8}\leq0\\
T^{\phi\phi}&=&\frac{27}{32\pi}R_0^6\omega^2\left(\frac{3R_0^6\omega^2t^2\sin^2{\theta}-r^6}{r^{14}}\right)\\
T^{r\phi}&=&T^{\phi r}=\frac{27R_0^9\omega^3t\sin^2{\theta}}{32\pi r^{10}}\geq0\textrm{\ for\ }t\geq0.
\end{eqnarray}

As in the universe outside a Schwarzschild black hole, the null energy condition is violated since a null vector $k_\mu=((\sqrt{-g^{tt}})^{-1},0,0,(\sqrt{g^{\phi\phi}})^{-1})$ gives (for $\theta\neq\pi/2$)
\begin{eqnarray}
T^{\mu\nu}k_\mu k_\nu=T^{tt}(k_t)^2+T^{\phi\phi}(k_\phi)^2=-\frac{9R_0^6\omega^2\sin^2{\theta}}{8\pi(r^6+9R_0^6\omega^2t^2\sin^2{\theta})}<0.
\end{eqnarray}

The results for the non-uniformly rotating Minkowski spacetime are therefore similar to that for Schwarzschild. Note however that unlike Schwarzschild where $r\geq R_s$ is the observable universe, here the entire spacetime should be observable. This ostensibly leads to a problem, because $r\geq R_0\neq0$ otherwise $\chi=(R_0/r)^3$ would then be identically zero. Nevertheless the form of $\chi=P/r^3+Q$ was a solution to $G^{t\phi}=G^{\phi t}=0$ such that $T^{t\phi}=T^{\phi t}=0$ which gives a stress-energy tensor that does not involve heat conduction. It is certainly possible to choose a different $\chi$ which is 1 at $r=0$ and monotonically decreases to 0 as $r\rightarrow\infty$, like $\chi=1/(1+r^3)$ but requires that $T^{t\phi}=T^{\phi t}\neq0$. This is thus a difference between a non-uniformly rotating Minkowski and a non-uniformly rotating Schwarzschild universe. Furthermore, the mass-energy for the Minkowski one is naturally static since there is no black hole to gravitationally attract it towards the centre \footnote{If $R_s=0$, then from Eqs. (\ref{Schmet1}) or (\ref{Schmet2}) the metric for a non-uniformly rotating Minkowski spacetime has $g_{tt}=-1$, which implies no tidal force.}.

\section{Further Discussion}

We began by constructing the geometry of a non-uniformly rotating universe around a Schwarzschild black hole in section 2, and subsequently showed that this is caused by a static mass-energy with time-dependent stress along the $\phi$-direction and $r\phi$-shear forces. The frame of a faraway observer sees that the mass-energy is negative, and violates the null energy condition. The exotic nature of the material may render this phenomenon as unphysical, notwithstanding the fact that there are known solutions in general relativity (like traversable wormholes \cite{Vis2}, and warp drive \cite{Alc}) which demand such physics. Whilst it is arguable that the Casimir effect \cite{Exo1,Exo2,Exo3} is a well-regarded example of exotic matter to support these kind of so-called unphysical solutions, it is certainly important to be critical and discrimate any artificially thought up spacetime with highly obscure and inordinate physical requirements.

In spite of the possibility of being classified into the undesirable category, the purpose of our study here is not to propose an arbitrary metric and just accept whatever stress-energy tensor that follows from the field equations. It is actually quite the contrary as we do not demand that there must exist a particular kind of mass-energy in nature to produce our desired spacetime. Instead, our motivation lies in figuring out the properties of such material and uncover their key characteristics. If such properties are deemed drastically preposterous, then it may perhaps be interpreted as an explanation to why we do not observe such rotational effects in our universe.

The Einstein field equations are notoriously complicated non-linear partial differential equations, and a repercussion is the difficulty to solve it exactly. They are nevertheless meant to be read both ways:
\begin{enumerate}[(i)]
\item
Given the physics, here is the resulting spacetime geometry.
\item
Given a spacetime geometry, here is the necessary physics.
\end{enumerate}
Even though our approach is based on the unorthodox direction of specifying the spacetime geometry to figure out the necessary physics, our results can be read from the more conventional direction to reveal the effect of a static mass-energy with time-dependent $\phi$-stress (quadratic with time) and $r\phi$-shear forces (linear with time): \emph{This causes the universe to rotate, i.e. shift along the $\phi$-direction.} Putting it in another way, the stress-energy time-dependence for a particular direction ($T^{\phi\phi}$, $T^{r\phi}=T^{\phi r}$) results in a spacetime translation along that direction ($\phi$). This may indicate that more complicated dynamical evolution of the universe can be decomposed into the respective directional time-dependence of the stress-energy tensor ($T^{rr}(t),T^{\theta\theta}(t)$, etc.). Our success in pinning down the precise conditions for this particular case owes to the fact that we constructed such a rotating spacetime first and then use the field equations to decipher the physics. We therefore already have an exact solution, for what may appear to be a strange (or highly fine-tuned) specification of the stress-energy tensor. Surely, one may begin instead with a physically constructed stress-energy tensor with the time-dependent properties of $T^{\phi\phi}$ and $T^{r\phi}=T^{\phi r}$. The major weakness in this usual approach is that unless the stress-energy is of a particularly nice form, it may be nearly impossible to analytically solve the field equations. An important lesson is thus had we remained obdurate and refused to be avant-garde with the field equations, we might not have discovered such properties that lead to a rotating universe.

Our results also show the difference between a non-uniformly rotating universe and an expanding universe as described by the FLRW solution. The latter assumes homogeneity and isotropicity, so it does not pick out any preferred spatial direction. The resulting Friedmann equations govern the change in the material density with time as it causes the universe to expand. Our non-uniformly rotating universe on the other hand has a fixed density and it is the increase in a directional stress with time that produces the rotation.

For future research, it would be interesting to investigate if the purported exotic nature of the material to produce the rotation is mandatory. One may attempt to adapt the key time-dependent features that we have found here to specify certain stress-energy tensors (perhaps with no or less severe violation of the null energy condition), and solve the field equations numerically to simulate the rotational evolution of the universe. Our model assumes a constant angular velocity for simplicity to glean the crucial physical insights. It would be desirable to study more exhaustively how the rotation may originate, and how it would end via numerical computations. Another possible extension would be to let the material orbit the black hole on a circular geodesic, although care is to be taken in distinguishing between the particle's own orbital motion with the rotation of the universe itself.

This simple model presented here is based on Einstein's theory of general relativity, without any quantum effects involved. Recent frontier research in quantum gravity has pushed the debate on what happens near the horizon of a black hole to unprecedented heights, following the black hole information paradox \cite{BHW,Haw1,Susskinda,Hooft,Susskindb} to firewalls near a black hole horizon \cite{nature,Firewall1}, with the latest update from Stephen Hawking suggesting that ADS-CFT supports the notion that black holes do not have event horizons \cite{Hawkinglatest}. It would be exciting to extend the formulation of a non-uniformly rotating universe around a black hole to the realm of such theories where quantum mechanics plays its part as well.

\section{Concluding remarks}

This study of a non-uniformly rotating universe around a Schwarzschild black hole is perhaps a paramount example of how the approach of constructing the spacetime metric based on its desired geometrical properties and then using the field equations to find out the physics of it has led to the discovery of a new kind of solution in general relativity. The key properties of the mass-energy for this spacetime have been carefully examined and discussed.

We have also illustrated how our general method of constructing spacetime by generating manifolds of revolution around a curve \cite{Vee2012,Vee2013} leads to the various coordinate systems for describing the Schwarzschild solution, when the given curve is a straight line. These different coordinate systems can be attributed to the freedom in parametrising the straight line and the radial function.

\begin{acknowledgments}
The author is grateful for the efforts by Meng Lee Leek from Nanyang Technological University in participating in useful discussions that aided towards the coherent formulation of this work, as well as reviewing the final draft of this manuscript.
\end{acknowledgments}

\bibliographystyle{spphys}

redpajama_set_name: RedPajamaArXiv


Cross for eastern people 3rd class with swords in bronze. Zink construction with ring. Unmarked, supposedly made by Rudolf Wächtler & Lange, Mittweida. Excellent condition with all bronze finish intact. Comes with its original green ribbon and attachment device. No repairs, no damage.


Gujarat PSC Recruitment 2017 Latest research officer 04 Posts – Gujarat Public service commission (GPSC) invites application for the position of 04 research officer class-I vacancies of general state service under Narmada water resources / water supply and Kalpasar department. Apply online before 31st May 2017.
Qualification/ Eligibility Criteria:- Eligible applicants applying for the position of research officer should have possess post-graduate degree with first class in civil engineering or technology or geo-physics or geology obtained from any of the universities and have about five year research experience.
Age Limit (In yrs.):- The age of the eligible applicant applying for the position of research officer should not be less than 21 years and not be more than 42 years. The age of the applicant should be as on 31st May 2017.
Mode of Selection:- The selection of the eligible applicant applying for the position of research officer will be on the basis of personal interview.
Application fee:- Interested and eligible applicants applying for the position of research officer are required to pay application fee Rs 100/- plus postal service charges. Fee can be pay through Indian postal order / online payment.
How to apply:- Interested and eligible applicants applying for the position of research officer may apply online through official website of Gujarat public service commission (GPSC) http://gpsc-ojas.guj.nic.in from 15th May 2017 to 31st May 2017.
Starting date for the submission of online application is 15th May 2017.
Last date for the submission of online application is 31st May 2017.


text:
Charles Korvin (Kárpáthy Korvin Géza) – the blacklisted Hungarian American film star
May 2, 2019 1:48 pm·
As part of our series on lesser known Hungarian Americans we introduce Hollywood star Charles Korvin. The very good looking Hungarian was a popular star of the screen in the 1940s.
Charles Korvin
Géza Kárpáthy Korvin was born in 1907 in Pöstyén, Hungarian Kingdom (today Piešťany, Slovakia) in a Hungarian speaking family with a noble lineage. Géza was fascinated with photography and filmmaking as a young man and moved to Paris to study at the Sorbonne. There he got involved in anti-Franco film projects supporting the Republicans of the Spanish Civil War.
Kárpáthy's political views were on the left and later he was even accused of Communist sympathies. In 1940 he moved to the US to study acting and successfully debuted on Broadway using the name, Geza Korvin. Universal Studio soon discovered the photogenic actor and offered him a contract he couldn't refuse. In 1945 he starred as a French thief in Enter Arsene Lupin under his new name, Charles Korvin.
French Poster of Enter Arsene Lupin
In 1947, Universal suspended stubborn the Korvin after he refused to play the role of a villain in Black Velvet. Korvin became independent and had no problem getting contracts. The major studios– Columbia, Paramount and 20th Century Fox–loved his athletic, chiseled looks.
Along with many other Hollywood actors Korvin was blacklisted in 1951 after he refused to cooperate with Senator Joseph McCarthy's House Un-American Activities Committee. With his family, he left the US to live in Klosters, Switzerland, where he maintained a second home during his life. Although he continued to make appearances on American television, it would not be until 1965 that he could return to the big screen in director Stanley Kramer's star-studded film, Ship of Fools. (In the early 1950s the infamous Hollywood blacklist denied employment to actors, screenwriters, film directors, musicians who believed to be or to have been Communists or leftist sympathizers.)
Korvin's studio postcard
Later Korvin appeared in television series, among them Zorro and an episode of The Honeymooners, in which he played a Latin dance instructor! Many say that early in his career Korvin was typecast by the Hollywood studios. The New York Times wrote in his obituary that he "made a career playing gentleman thieves and philandering husbands."
Romantic lead with his regular co-star, the exotic beauty Merle Oberon.
Korvin died in 1998 at Lenox Hill Hospital in Manhattan. His wish was to be cremated and his ashes spread over the Atlantic Ocean.
György Lázár
Tags: Charles Korvin, Film, United States
Author: György Lázár György Lázár came to the US in 1980 on a UNESCO fellowship to complete his Ph.D. at the University of North Carolina. He later moved to California where he became mesmerized by the entrepreneurial spirit of Silicon Valley and spent the next 25 years in high-tech consulting focusing on the financial aspects of technology. In the last couple of years he became a contributor to several Hungarian and English language publications. He and his wife enjoy spending time in Hungary, they try to go to Europe as often as they can.

redpajama_set_name: RedPajamaCommonCrawl


text:
Three people injured after car crashed on Swine Lane at Nostell near Wakefield
Friends and colleagues show their support for former Wakefield prison dog handler Paul Bailey by walking 73 miles
Watersplash Final to feature on BBC1's Inside Out show
A look back at the famous '˜Watersplash Final' of 1968 is to be screened on television next week.
Friday, 2nd February 2018, 3:23 pm
Updated Friday, 2nd February 2018, 3:26 pm
The cameras visited Sharlston Rovers RLFC's ground last month where fans and former players gathered to watch and reminisce about the Challenge Cup Final at Wembley between Wakefield and Leeds from 50 years ago.
The feature will be part of BBC1 North's Inside Out show to be screened on Monday, February 5 at 7.30pm.
The game is remembered for being played in atrocious conditions with torrential rain making it almost unplayable.
It also produced a nail-biting finale, with Wakefield's Don Fox missing a last-minute conversion to hand the trophy to Leeds with an 11-10 victory.
Former Wakefield MP and rugby fanatic, David Hinchliffe, was at the Sharlston Rovers screening and said: "The hall was pretty full, people who saw that game will not forget it as long as they live.
"It was an incredible game, right to the last minute, and it's right it should be remembered."
Meanwhile, David's book about the final, called 'They Walked on Water' is to be re-published this month to coincide with the 50th anniversary, with all cash going towards the Rugby League Benevolent Fund.
A commemorative event if the final is also planned at Huddersfield University on the morning of May 12, with film clips of the match, speakers, Q&As and an opportunity to see archive material relating to the match.
There will also be the play, written buy lifelong Trinity fan Peter Hirst, performed about the final. The event will free to attend.
'I had to pay £360 just to leave my estate': Wakefield Council concern over 'scandalous' land maintenance charges
City centre cannabis farm found after police call out
'If we were in leafy Harrogate this wouldn't be happening': Pontefract and Knottingley fury as Northern slashes rail services
Heating grants made available for Wakefield residents after £153,000 windfall
Barges banned on canal over concerns about rising fish deaths


A new year workplace challenge that started to help motivate colleagues into getting active in 2019 has turned into a fundraiser that has already raised in excess of £4,000 for charity.
Almost 90 colleagues entered the event and by the end of January well over 4,000 miles were recorded.
And to make it more worthwhile, Nisa's charity Making a Difference Locally (MADL) has pledged to match miles with money and will donate £1 per mile completed to Alzheimer's Society.
Steve Portess (pictured), Nisa IT analyst and the brains behind the initiative, said: "I've been totally overwhelmed by how many colleagues have got on board. There are people who previously were barely walking a few miles a month who have walked, jogged or run miles and miles, hitting their target and setting new ones throughout the month.
Head of Charity at Nisa Kate Carroll said: "We wanted to recognise everybody's efforts and matching miles with pounds seemed like a brilliant way to do it.


text:
<!doctype html>
<html lang="en">
<head>
  <meta charset="utf-8">
  <title>test.</title>
  <!-- bower:css -->
  <link rel="stylesheet" href="../bower_components/codecode/dist/codecode.css" />
  <link rel="stylesheet" href="../bower_components/bootstrap/dist/css/bootstrap.css" />
  <!-- endbower -->
</head>
<body>

  <!-- bower:js -->
  <script src="../bower_components/jquery/jquery.js" class="yay"></script>
  <script src="../bower_components/modernizr/modernizr.js" class="yay"></script>
  <script src="../bower_components/codecode/dist/codecode.js" class="yay"></script>
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redpajama_set_name: RedPajamaGithub


25 oKnow therefore and understand that pfrom the going out of the word to restore and qbuild Jerusalem to the coming of an ranointed one, a sprince, there shall be seven weeks. Then for sixty-two weeks it shall be built again1 with squares and moat, tbut in a troubled time.
8 And he said, i"See that you are not led astray. For jmany will come in my name, saying, k'I am he!' and, l'The time is at hand!' Do not go after them.


Ferritin is one of the above non-haem adamant accumulator proteins in animals, plants, and microorganisms. It is a multisubunit protein with a alveolate interior, which contains a mineral amount of hydrated adamant oxide, thereby ensuring its solubility in an aqueous environment. Each subunit consists of a closed, four-helical array with a awkward aberration and one crossover connection.
This access represents the ferritin-like superfamily. Proteins with this anatomy cover ferritin and added ferritin-like proteins such as bacterioferritin (cytochrome b1) that binds haem amid two subunits, non-haem ferritin, dodecameric ferritin homologue (DPS) that binds to and protects DNA, and the N-terminal area of rubrerythrin that is begin in abounding air-sensitive bacilli and archaea . In addition, ribonucleotide reductase-like proteins appearance a agnate anatomy to the ferritin-like fold; these di-iron carboxylate proteins aggregate a assorted chic of non-haem adamant enzymes assuming a aggregation of redox reactions. The superfamily aswell includes the alpha and beta subunits of methane monooxygenase hydrolase, basin 9-stearoyl-acyl carrier protein desaturase and manganese catalase.


text:
Q: Simple Breadcrumb Issue I've been trying to figure out how to make the last item in my breadcrumb have H1 tags in it. Here is a sample code without the H1.
// Each tree item has a URL and name. Some may have extra_before and extra_after.
foreach ($context['lateral_navigation'] as $link_num => $tree)
{
    echo '

';

    // Show something before the link?
    if (isset($tree['extra_before']))
        echo $tree['extra_before'];

    // Show the link, including a URL if it should have one.
    echo $settings['lateral_navigation_link'] && isset($tree['url']) ? '
            ' . $tree['name'] . '
            ' : '' . $tree['name'] . '';

    // Show something after the link...?
    if (isset($tree['extra_after']))
        echo $tree['extra_after'];

    echo '

';

I'm not a PHPer, and I've tried experimenting with it code on this line:

';

Because it shows the "last" only on the last item of the breadcrumb.
I tired this below, but obviously it didn't work:
// Each tree item has a URL and name. Some may have extra_before and extra_after.
foreach ($context['lateral_navigation'] as $link_num => $tree)
{
    echo '

' : '', '>';

    // Show something before the link?
    if (isset($tree['extra_before']))
        echo $tree['extra_before'];

    // Show the link, including a URL if it should have one.
    echo $settings['lateral_navigation_link'] && isset($tree['url']) ? '
            ' . $tree['name'] . '

            ' : '' . $tree['name'] . '';

    // Show something after the link...?
    if (isset($tree['extra_after']))
        echo $tree['extra_after'];

    // Don't show a separator for the last one.
    if ($link_num != count($context['lateral_navigation']) - 1)
        echo '';

    echo '

';
}

Any help with this?

A: Try this:
$count = count($context['lateral_navigation']); // get count

// Each tree item has a URL and name. Some may have extra_before and extra_after.
foreach ($context['lateral_navigation'] as $link_num => $tree)
{
    $count--; // decrement by 1
    echo ($count == 0) // if zero (last)
        ? '

'
        : '
';

    // Show something before the link?
    if (isset($tree['extra_before']))
        echo $tree['extra_before'];

    // Show the link, including a URL if it should have one.
    echo $settings['lateral_navigation_link'] && isset($tree['url']) ? '
            ' . $tree['name'] . '

            ' : '' . $tree['name'] . '';

    // Show something after the link...?
    if (isset($tree['extra_after']))
        echo $tree['extra_after'];

    // Don't show a separator for the last one.
    if ($link_num != count($context['lateral_navigation']) - 1)
        echo '';

    echo ($count == 0) // if zero (last)
        ? '

'
        : '
';
}

redpajama_set_name: RedPajamaStackExchange


English winger Patrick Roberts, 21, who is on loan at Girona from Manchester City -- would need permission to live and work in the country.
Real Madrid a better fit for Diaz?
The 30 most recent news articles written at Eyefootball.com about Girona.


There are several typical places to walk your dog out there. The first that will spring to mind are in the street or at the park, but there are some other venues around your areas that will work just as well – if not better –and provide both you and your canine with a change of pace and scenery. If you don't want to just stick to the tried and tested – and would like to try out some new places for you and your pet to enjoy some good exercise at, then look no further than these handy pointers.
If you are blessed not to live in a landlocked area, and have an ocean to get to, then this is just for you. The sand between your toes and the water gushing at your heels is just the treat for you and your dog. Make sure you clean up after your animal, though, if it does make a mess – as many signs will show that you could be hit in the pocket if you don't do this. Take some friends and their dogs – which among them might be a friendly Cocker Spaniel – with you, too, to make the fun all that more community-based and even better.
Granted, this won't work for everyone, but if you live on a high rise that has a decked out rooftop, with a greenhouse – an is spacious enough for doing more than just hanging your laundry, then this cold work for you. The air up there should be at its freshest – and the views will be amazing. Of course, stay away from the edges, and make sure your dog doesn't get too excited and also steers clear from enduring a nasty fall. Again, as with on the beach, you can do this with friends and other pets.
If not the ocean, then a river or related body of water, even a dam, could suffice for your and your dog. There is just something quite refreshing about having a body of water in sight when you are doing some physical exercise. Even if you can't get into the water, like you could at the ocean or river, the embankments of a natural or man-made dam would work nicely. If this is not to your liking or perhaps your dog doesn't show an abundance of excitement for this venue, the move along swiftly.
We don't all have mates with vast open spaces in their house backyards, but some of us do, and can invite ourselves around for a run in their green area. Even if you have to do laps, and make up circuits of sorts to make the space feel all the more large, then do so – you won't regret it. As a plus, unlike at the beach, you won't have to wash sand off your feet in the end – and your dog should be pretty clean for the ride home later. The physical exercising can be followed by a quiet drink with your friends – and some special treats for your dog.


text:
Michel Thomas Beginner Russian, Lesson 2
著者: Natasha Bershadski
ナレーター: Natasha Bershadski
What is the Michel Thomas Method?
The Michel Thomas Method teaches everyday conversational language that will allow you to communicate in a wide variety of situations, empowered by the ability to create your own sentences and use the language instinctively, having absorbed the vocabulary and grammatical structures. These all-audio courses were perfected over 25 years by gifted linguist and teacher Michel Thomas, and provide an accelerated method for language learning that is truly revolutionary.
Lessons 1-8, the Beginner course: This course makes no assumption of knowledge of any language other than English and gives the beginner practical and functional use of the spoken language. It is also appropriate for anyone who has studied Russian before, but has forgotten much of it or does not have confidence in speaking. The Beginner course is designed to take you from complete beginner to intermediate level.
Lessons 9-12, the Intermediate course: This course is for those with an intermediate-level foundation in Russian, or those who have completed lessons 1-8 and want to take their learning to an advanced level and speak Russian proficiently and easily.
Unlike most language courses that focus around topics or grammar forms, the Michel Thomas Method works by breaking a language down into its component parts, enabling you to reconstruct the language yourself - to form your own sentences, to say what you want, when you want. Within the first 10 minutes of the course, you will be generating complete sentences on your own. It is important that you complete the lessons in order. The Method is successful because it builds on the language you learn in each lesson and 'recycles' language taught in earlier lessons, allowing you to build ever-more complicated sentences. Because the Method is based on understanding, not memorisation, there is no set limit to the length of time that you should study each lesson. Once you feel you have a good grasp of the language taught in one lesson, you can move on to the next.
In lesson 2 of the Russian Beginner course, you'll be able to use the verb endings for 'I' and 'you', translate 'I have', and make polite requests with…
Verbs: 'to understand', 'to think', 'to find out', 'I want', 'to eat', 'to drink', 'to do', 'you know', 'to be'
Nouns: 'airport', 'address', 'café', 'things', 'mum', 'plan', 'idea', 'allergy', 'doctor', 'flu', 'computer'
Phrases: 'I'm hungry/thirsty' (= 'I want to eat/drink')
Asking politely
Verb endings for 'I' and 'you'
Pronouns: 'me', 'you' (object form: 'I understand you')
Question word: 'how?'
Social communications: 'how are things?', 'what do you think?', 'what do I do?'
Translating 'I have': 'by me (there is)'
Adverb: 'normal/OK'
Words ending in ' ture' and ' y' are similar in Russian
In the next lesson you'll be able to speak about the future and use impersonal verbs ('I need', 'I am interested') and the verbs endings for 'he', 'she', and 'we'.
PLEASE NOTE: When you purchase this title, the accompanying reference material will be available in your My Library section along with the audio.
©2013 Michel Thomas (P)2013 Hodder & Stoughton
Michel Thomas Method
Michel Thomas Beginner Russian, Lesson 2に寄せられたリスナーの声
Audible.com.au
Mr. I. E. Andrews
The course is dramatically let down !
The organisers really gave to sort this out !! I purchased the introductory course which was excellent. I then purchased lesion one which was the logical progression which turned out to be the same as chapter 1 in the introductory course. As every sample is exactly the same as the first there is no way of telling which is the follow on course. This is basic stuff and when you get going you do not want to run into childish errors like this! I've just purchased lesson two but again this turned out to be the same content as the introductory course. Why can't you just label it clearly. Like 1-2-3-4 and so on! I am more than dissatisfied with this as it greatly distracts from what is a well made course !!
Sigmund Do Cestra
Incorrect Pronunciation
I have listened to many Russian courses and found this one one of the most annoying because of the incorrect pronunciation and the old-school demeanor of the tutor. Also, IMO having two bad students pronouncing the sentences incorrectly and making mistakes does not work at all. I found it so irritating I did not go past minute 20 or so.
Great course, but buy CDs instead
What would have made Michel Thomas Beginner Russian, Lesson 2 better?
I am a great fan of Michel Thomas language courses, so the problem is not the content. However, since language courses are all available on CD it is far better value to buy the CD's load into itunes and then resell the CDs on ebay.
Leslie Brown
I'd rather not listen to students fumbling...
The speakers kept using rising intonation because they were not fully confident in what they were saying. it's almost as if they were asking "Is this right? Am I saying it right?" It becomes tiring listening to the instructor's continual corrections. This is akin to throwing you in the deep end on your first swimming lesson, or a ski instructor taking you down a black ski run on your first day. It's awkward. Better to learn the basics first, then you will automatically be a more confident speaker. She exercises the part of your brain to construct new sentences. But the vocabulary is very limited. What will happen is that the students won't understand anything that they are told in real life. It feels like a very superficial knowledge to learn 95% cognate words in another language... So far I have only listen to 2.5 hours, but she does not set you up to say very basic things like "the book is on the table". If you're going to teach or learn that way, better to know how to ask "How do you say xyz?" in Russian, then simply copy what is said. I think "behind the wheel" Russian is more fun. It's a much more comprehensive course (especially if you listen to it three times or more). And always with native speakers whom you can copy for perfect pronunciation! But not this! By contrast, I cannot imagine listening to this ever again. I won't. It feels more like quasi-Russian elocution lessons than foreign language learning.


Under the direction of the Director of Nutritional Programs, the Regional Nutrition Manager is responsible for the overall guidance, leadership, management, and implementation of Dietitian Services to assure quality nutritional programs across the region. Performs duties and responsibilities in a cost and effective manner consistent with our mission, vision, values, and Mercy Service Standards.
Assesses and improves regional performance through established quality improvements procedures and continuously seeks improvement opportunities for the quality of nutrition care.
Effective written and verbal communications skills with peers, patients/families, interdisciplinary team members.
Maintains state dietetics licensure and CDR registration with the Academy of Nutrition and Dietetics.
2.1 Supervises daily and monthly staffing levels across the region to assure levels are within targeted guidelines to efficiently utilize allocated resources.
2.2 Assesses through the hiring process basic qualifications, competencies of coworkers, and continuously assure that co-workers model the Mercy mission, vision, values, and Mercy Service Standards.
2.3 Implement and continuously monitor nutritional programs across the region to ensure quality goals align for achievement within Ministry Quality & Safety goals.
Education: Bachelor's degree from a regionally accredited university. Successful completion of a didactic program in dietetics and supervised practice experience, approved or accredited by The Commission on Dietetic Registration of the Academy of Nutrition and Dietetics.
Licensure: Registered Dietitian (RD) and Licensed in the State of Missouri.
Experience: Minimum of 5 years of clinical dietetics experience beyond completion of clinical training. A majority of the clinical work experience must have taken place in a large acute care hospital. Majority of work experience in a large hospital and in area of specialization (e.g. pediatrics, adult critical care, ambulatory specialty, general rehabilitation or medicine/surgery area). Experience supervising dietetic interns or other students. Evidence of mentoring other dietitians. Strong academic & applied background in clinical nutrition for outpatient, acute and post-acute care setting. Expertise and knowledge in application of medical nutrition therapy principles.
Preferred Education: Master's degree in Healthcare Administration, Business Administration, Clinical Nutrition, or other health care field.
Preferred Experience: Supervisor or Leadership experience preferred, Program implementation experience preferred.


text:
package org.mashti.jetson;

import io.netty.channel.ChannelInboundHandler;
import io.netty.channel.ChannelInitializer;
import io.netty.channel.ChannelOutboundHandler;
import io.netty.channel.socket.SocketChannel;
import io.netty.handler.codec.LengthFieldBasedFrameDecoder;
import io.netty.handler.codec.LengthFieldPrepender;
import io.netty.handler.logging.LogLevel;
import io.netty.handler.logging.LoggingHandler;
import io.netty.handler.timeout.ReadTimeoutHandler;
import io.netty.handler.timeout.WriteTimeoutHandler;
import java.util.concurrent.TimeUnit;
import org.slf4j.Logger;
import org.slf4j.LoggerFactory;

abstract class BaseChannelInitializer extends ChannelInitializer<SocketChannel> {

    private static final int DEFAULT_LENGTH_FIELD_LENGTH = 2;
    private static final int DEFAULT_MAX_FRAME_LENGTH = 0xFFFF;
    private static final Logger LOGGER = LoggerFactory.getLogger(BaseChannelInitializer.class);
    private static final long DEFAULT_READ_TIMEOUT_IN_SECONDS = 30;
    private static final long DEFAULT_WRITE_TIMEOUT_IN_SECONDS = DEFAULT_READ_TIMEOUT_IN_SECONDS;
    private static final LengthFieldPrepender DEFAULT_FRAME_ENCODER = new LengthFieldPrepender(DEFAULT_LENGTH_FIELD_LENGTH);
    private static final LoggingHandler LOGGING = new LoggingHandler(LogLevel.INFO);
    private volatile long read_timeout;
    private volatile TimeUnit read_timeout_unit;
    private volatile long write_timeout;
    private volatile TimeUnit write_timeout_unit;

    BaseChannelInitializer() {

        setReadTimeout(DEFAULT_READ_TIMEOUT_IN_SECONDS, TimeUnit.SECONDS);
        setWriteTimeout(DEFAULT_WRITE_TIMEOUT_IN_SECONDS, TimeUnit.SECONDS);
    }

    @Override
    public void initChannel(final SocketChannel channel) throws Exception {

        if (LOGGER.isDebugEnabled()) {
            channel.pipeline().addLast(LOGGING);
        }
        channel.pipeline().addLast("write_timeout", createWriteTimeoutHandler());
        channel.pipeline().addLast("read_timeout", createReadTimeoutHandler());
        channel.pipeline().addLast("frame_decoder", getFrameDecoder());
        channel.pipeline().addLast("frame_encoder", getFrameEncoder());
    }

    void setReadTimeout(final long timeout, final TimeUnit unit) {

        read_timeout = timeout;
        read_timeout_unit = unit;
    }

    void setWriteTimeout(final long timeout, final TimeUnit unit) {

        write_timeout = timeout;
        write_timeout_unit = unit;
    }

    ChannelOutboundHandler getFrameEncoder() {

        return DEFAULT_FRAME_ENCODER;
    }

    ChannelInboundHandler getFrameDecoder() {

        return new LengthFieldBasedFrameDecoder(DEFAULT_MAX_FRAME_LENGTH, 0, DEFAULT_LENGTH_FIELD_LENGTH, 0, DEFAULT_LENGTH_FIELD_LENGTH);
    }

    private WriteTimeoutHandler createWriteTimeoutHandler() {

        return new WriteTimeoutHandler(write_timeout, write_timeout_unit);
    }

    private ReadTimeoutHandler createReadTimeoutHandler() {

        return new ReadTimeoutHandler(read_timeout, read_timeout_unit);
    }
}


Travel Hanger was designed to make your life easier. It folds up for easy storage while travelling abroad to tropical waters, or even on the road to a local site.
The compact dimensions of the product are 5.4" x 8" x 2.5" (13.7 x 20.3 x 6.4 cm), while the unfolded dimensions are 15.75" x 8" x 6.25" (40 x 20.3 x 15.9 cm). Quick drainage and drying are made easy with the Travel Hanger! It is built to hold your BCD, regulator and other accessories with the additional folding arms. The Hanger has special shoulders, meant specifically to hold your BCD, so you don't find it on the ground next time you check. X-beam non-corrosive plastic will ensure longevity, as well as feel lightweight for travel!


Before long it was time to be unleashed.
With the Line up of Roy, John and bass player Alan Gilbert, Beyond Eternal was born.
Alan's tenure in the band would be short lived as he soon moved out of province but the wheels were set in motion.
In the spring of 2015 Rhtyhm guitarist Ryan Bernard parted ways with the band to be replaced by former Darkcide Axe man Steve Henry and After a brief hiatus Trevor Hickey temporarily returned to his rightful place behind the thunder. Work and other commitments saw Chris Deveau step in as the 4 string rager while Trevor stepped down from his duties. Plethora of shows later saw one last departure as Steve stepped down from his duties as 2nd axeman. Leaving the core more solid than ever, 2017 would see Trevor return on a permanent basis taking up the bass mantle while Chris assumed 2nd guitar duties.
This was not to last however, as both Trevor and Chris made the tough decision to step down from the band to focus on personal and family matters. After John had to step down from his drum throne due to a physical condition a new drummer in Mike Prevost was found, Trevor made his return to the fold permanently and work continued on a crushing album number 2.
The mission statement is simple: To create TRUE Heavy Metal without borders, without limitations. With a sound, that is both varied and unique.
Drawing from a multitude of influences from Metallica and Annihilator, Pantera and Dethklok, Iron Maiden and Sabbath (just to name a few) the band refuses to compromise in its quest to unleash its brand of metal to the masses.


Through her richly detailed paintings featuring imagery drawn from advertisements, New York–based artist Julia Jacquette addresses the challenges of navigating the contemporary media landscape that so directly influences our sense of personal identity and self-worth. Exposing our seemingly insatiable longing for a life that is purely a construct of the advertising industry, Jacquette's work focuses on commercialized objects of desire: prepared meals drawn from 1950s cookbook illustrations, ornate interiors of the wealthy sampled from contemporary lifestyle magazines, shimmering swimming pools extracted from luxury ad campaigns. These material trappings are presented, often close up, in works that convey the pervasiveness of such evocative imagery.
TRACY L. ADLER is the Johnson-Pote Director of the Ruth and Elmer Wellin Museum of Art at Hamilton College in Clinton, New York.


text:
Publish: 23 Jan 2023, 02:20 pm
6 Sentenced to Death for War Crimes in Mymensingh
Published: 23 Jan 2023, 02:20 pm
The International Crimes Tribunal on Monday sentenced six fugitive criminals of Mymensingh to death for their crimes against humanity during the Liberation War in 1971, reports UNB.
The condemned convicts are Mokhleshur Rahman Mukul, Saidur Rahman Ratan, Shamsul Haque Fakir, Nurul Haque Fakir, Sultan Mahmud Fakir and Naqib Hossain Adil Sarkar. All were tried in absentia.
The tribunal headed by Justice Md Shahinur Islam handed down the punishment to the six after holding them guilty of murder, torture and kidnapping.
Public prosecutor barrister Tapas Kanti Ball represented the state in the court.
"There were total nine accused in this case. Two of them were behind the bars. Three people died, including two who were in prison and a fugitive accused, said barrister Tapas Kanti.
According to the prosecution, the investigation of this case started on January 26 in 2017. On December 31 of that year, the investigation agency submitted its report after the investigation.
In July 12 in 2018, a chargesheet was submitted to the court against the convicts. Later, the trial started on December 5 of the same year through charge framing.
The testimonies of 19 people were taken in this case. At the end of arguments, the tribunal kept the case pending for judgment on December 5 last.
Subscribe Shampratik Deshkal Youtube Channel
Topic : Bangladesh Mymensingh War Crimes sentence Death for War Crimes the Liberation War fugitive criminals
More From Bangladesh


text:
(function(){
'use strict';

angular.module('omolumeter.sidenav', [])
.component('omolumeterSideNav', {
  templateUrl: 'components/sidenav/sidenav.html', //'sidenav!',
  controllerAs: 'vm',
  require:{
    omolumeter: "^omolumeter"
    },
  bindings: { $router: '<' },
  controller: ['$mdMedia', '$mdSidenav', '$log', '$rootRouter', function($mdMedia, $mdSidenav, $log, $rootRouter){
    var vm = this;

    vm.toggleMainNav = function (){
      console.log('sidenav.toggleMainNav(): DOES NOTHINGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGG');
      //$mdSidenav('mainNav').toggle();
      };

    vm.closeMainNav = function(){
      if($mdSidenav('mainNav').isLockedOpen()){
        $mdSidenav('mainNav').then(function(){

	});
        }
      $mdSidenav('mainNav').close();
      };

    vm.isSideNavLockedOpen = $mdMedia('gt-sm');

    vm.navigate = function(aRouteName){
      //hackOutletsHeight();
      $mdSidenav('mainNav').close();
      $rootRouter.navigate([aRouteName]);
      $log.log('navigated');
      //$rootRouter.navigate(['Informational']);
      //vm.$router.navigate(['Informational']);
    };

    function hackOutletsHeight(){
	var desiredHeight = '10000px'; //(window.getComputedStyle(document.getElementById('theNgOutlet'),null).getPropertyValue("height"));
      console.log('hackOutletsHeight(): ' + desiredHeight);
      document.getElementById('theNgOutlet').style.height =  desiredHeight;
      }

    vm.isSidenavToBeLockedOpen = $mdMedia('gt-sm');
  }]
  });
})();


Having the technical ability to write code is one of the most desired skills in today's job market. The amount of jobs in this sector has increased yearly, so learning to write code can be a great career for people fresh out of school as well as those looking to change careers. It is also a popular career for people who prefer to work remotely.
There is a misconception that learning how to code is difficult. However, it actually isn't as tough as people think, especially for problem solvers who enjoy finding the solution to difficult puzzles. One of the most popular methods of learning this skill is to attend a coding bootcamp of which there are numerous ones to choose from. The following are some of the careers in coding to consider that will enable you to work remotely.
A web developer is a one size fits all description for anyone who writes code as their primary job. Writing code is generally what developers, and that is what powers every website found on the internet. A web developer typically works with a website designer to turn their envisioned design into a functioning website.
However, some plugins that enable these things to work may be developed by someone else. Front end developers work with back end engineers to create apps and websites that are user-friendly and work as in ways that are intuitive for users. People in this career can make upwards of the high five figures in salary, meaning this is a very in-demand job.
Backend engineers or developers are responsible for the server side of coding that enables a website to work. They integrate code written by front end developers with the backend code, which is where data like user accounts, content, or anything kept in databases is stored for access.
An app developer is someone who builds applications for websites and mobile devices. The specific languages and skills they need depend on the platform the app is meant for like Windows, Android or iOS.
Basically, a website designer designs a prototype and user interface. The app developer makes this website function on mobile and tablet devices. Developers who work on the most popular apps can earn well into the mid-six figures, which makes this among the most popular careers for coders.
With the tech industry booming, it makes sense to pursue a career in coding. The careers can be quite lucrative, and they cater toward people who prefer to work remotely. This is why writing code is a job skill so in demand and should continue to be as long as technology keeps improving.
Samsung has Officially announced the brand new 2019 Galaxy A50 and Galaxy A30 with Infinity U Display for the Global markets.
Samsung hasn't said anything about the availability and pricing. Here are the Specifications for the Galaxy A30 and A50.


Will it fit standard fg baja? Maybe someone have? Is there some difference between 50 teeth and 48 Teeth ?
And how to mount this fg rain,dirt protection -pics?
RE: fg Steel Gearwheel Big 50 Teeth?/and rain dirt protection?


Put on your parka! This eye-catching Holiday dog leash features outdoor winter scenes that will make you shiver!
This leash is made to last, won't rust or fade and is machine washable. Your leash will last for years, it's machine washable and fade resistant. 100% Guaranteed even against chew damage.
All our dog leashes feature sturdy non-rusting snaps and quality nylon webbing in beautiful colors. Choose from 6 sizes of leash depending on the size of your dog. Small leashes are light weight and great for tiny dogs. Large leashes for big dogs feature strong snaps and durable webbing.
Faster shipping options are available for the holiday season. Matching Christmas collars, holiday collar bows and Christmas martingale dog collars are available. We even have holiday cat collars!
Go on and spread some holiday cheer. Order yours today!


text:
MAHER, MARY FRANCES
Mary Frances Maher, 74, of West Hartford, formerly of New Britain, died Saturday (Dec. 12, 1998) at a local convalescent home. Born in Hartford, daughter of the late James and Helen (McAloon) Maher, she lived in New Britain for many years before moving to West Hartford. She retired from Aetna Life Insurance Co. and Shawmut Bank. A Mass of Christian Burial will be Thursday (Dec. 17), 9 a.m. at St. Maurice Church, 100 Whiteman Rd., New Britain. Interment will be in St. Mary Cemetery, New Britain. Memorial donations may be made to St. Maurice Church, 100 Whiteman Rd., New Britain, 06052. The Burritt Hill Funeral Home, 332 Burritt St., New Britain is serving the family.
Copyright © 2023, Hartford Courant


I was blessed to have a private tour/photo session at the brand new pop up HideSeek! With so many rooms its a must see. It was instagram goals and here are some of my fav pics we captured!!
Hide from reality and seek a world of childlike wonder.
feel like a kid again.
you'll want to show and tell.
We're popping up at 1305 Dundas St. West. Toronto, ready or not, here we come!
We're easy to tag – @gohideseek. We like being it.
Posted in toronto, UncategorizedTagged art, hideseek, instagram, popup, torontoBookmark the permalink.


Fuel markets are changing. Consumer expectations are evolving. And the nation's G&T cooperatives are on the front lines.
With some 1.5 GW of co-op coal capacity expected to be shuttered by 2030, G&Ts are pushing to diversify and innovate.
While markets, fleet economics, and environmental performance drive the transition to cleaner, more efficient natural-gas-fired generation and renewable resources, generation co-ops are also investing in emerging sectors like advanced clean coal technology to preserve coal's role in power production while protecting existing plant investments.
As costs for solar and wind technology decline, G&Ts are contracting for more renewable energy, primarily through power-purchase agreements.
Electric co-ops have about 9.2 GW of owned and purchased renewable capacity—not including about 10 GW of annual federal hydropower—and at least 1.1 GW more is planned by 2020.
Analysts project continued renewable generation growth due to improving economics, the extension of federal tax incentives, and the likely adoption or expansion of renewable portfolio standards in several states.
The addition of renewables has also been driven by consumers. Recent member surveys by several distribution co-ops indicate widespread interest in environmental stewardship, as well as affordable, reliable power. As the primary power suppliers of distribution co-ops (79 percent of distribution co-ops are members of G&Ts), G&Ts have become more innovative in addressing consumer-member concerns and business demands.
For Wabash Valley Power Association, headquartered in Indianapolis, diversification has also meant savings for members. The G&T began investing in landfill gas generation in 2002, wherein plants capture methane from decaying trash and use it to produce electricity. Wabash Valley Power owns and operates 16 landfill plants that provide 53 MW of baseload capacity, making it a Midwest leader in utility-scale landfill gas generation.
Above ground, a 1.7-MW community solar program launched by the G&T in the fall of 2017 is already being expanded because of rapid adoption. The G&T also just inked two solar projects totaling 198 MW of utility-scale solar and, by 2020, will have 210 MW of wind energy in its power supply portfolio.
Rather than claiming these renewables in its generation portfolio, the G&T sells the environmental credits to other businesses seeking to achieve their compliance goals, which supports the growth of renewables in the marketplace.
"As a result of our flexible portfolio, we've capitalized on market opportunities, and our average wholesale rate has dropped for four consecutive years," says Lee Wilmes, Wabash Valley Power's executive vice president of risk and resource management.
While power generation options evolve, co-ops are advancing the reliability side of the business too. After a systemwide review of network schematics and identification of local transmission issues, Wabash Valley Power began an infrastructure upgrade of its existing SCADA system that will be complete this year. The initiative included a buildout of fiber-optic communication to each of its distribution co-ops' headquarters and additional equipment to aid in enhanced monitoring of power grid health.
In Texas, Golden Spread Electric Cooperative takes advantage of operating in both the Southwest Power Pool and the Electric Reliability Council of Texas. That unique position allows it to switch more than 550 MW of generation between the two regional transmission grids within one hour's notice.
The Amarillo-based G&T serves 16 distribution co-ops in a vast territory stretching from the South Texas plains north of the Rio Grande to the Texas Panhandle. Golden Spread member co-ops also serve portions of the Oklahoma Panhandle, southwestern Kansas, and southern Colorado.
Golden Spread employs a new load-forecasting process that enables it to incorporate water table studies, the impact on irrigation, and member feedback related to agricultural and industrial demand.
"This allows for a faster, more accurate energy and demand forecast that has been utilized for power supply optimization," says J. Jolly Hayden, Golden Spread's chief operating officer. He notes that it's also improved overall member satisfaction.
Since 2016, Golden Spread has upgraded software technology to forecast generation output, margins, and ancillary service revenue. The technology is also used to compile annual financials and budgeting, saving time and improving accuracy.


Africa Hunt Lodge allows the opportunity to hunt and harvest Monster South African Giraffe. The Limpopo Province of South Africa is the premier destination in the World to hunt the Giraffe. Year round, we offer hunts for awesome Trophy Giraffe. There are no seasonal restrictions on hunting the Giraffe in South Africa, which makes it a suitable trophy year round.
Our hunters typically hunt the South African Giraffe in conjunction with a 7-10 day African Safari. One of our Experienced and Licensed Professional Hunters will be your guide during your Giraffe Hunt. We typically hunt Giraffe Safari Style, Spot and Stalk, or by Still Hunting if you are a Bow Hunter. We can accommodate all methods of Hunting for Giraffe including Rifle, Bow, Black Powder, Crossbow or Handgun. We can accommodate hunters of any age and experience level.
The Giraffe which we hunt on our South Africa Concession are the biggest in the World. You can expect a 20+ foot Giraffe Bull on average when hunting with us.
Below are some of the trophies taken from our Giraffe hunts over the years.


Delivering an inconvenient truth will not be pleasant. People will accuse you of raining on their parade. You're not trying to ruin a good time; you're simply trying to avoid disaster. Anybody with an ounce of perception will see the wisdom of your warning and shut down a dangerous project. Many of your colleagues will blame you for the troubles that result. Let their complaints bounce off your skin as if it were armour. Ignoring the problem will only make it worse.


text:
Robbie Hunter-Paul
Experience makes all the difference says Sharp
HUDDERSFIELD Giants are just 80 minutes away from a Challenge Cup final!
Victory over Leeds Rhinos in Sunday's semi-final at the Grattan Stadium, Bradford (3.00) would book the Giants a place in the Twickenham final on Saturday, August 26.
Huddersfield start the tie as underdogs, with the experienced Rhinos appearing in their seventh semi-final in the last eight seasons.
The Giants, on the other hand, are featuring in only their second last-four clash in 35 years.
Their last appearance was just two years ago when they were heavily beaten 46-6 by eventual winners St Helens at Warrington.
But much has changed since then.
Huddersfield now have a much more experienced squad, with far more players having competed at the very highest level.
That's made head coach Jon Sharp a lot more confident this time around.
He admitted his players suffered the big freeze against Saints, with the squad failing to do themselves justice.
It's something the Giants have addressed since then, with players brought in specifically because of their big-match experience.
The time has now come for this experience to come to the fore, with Sharp confident he has the perfect blend of youth and experience.
"Before the start of the season, I spoke about bringing in players with the `X factor'," said Sharp.
"These are the players who know what it is all about to play in the bigger games and have shown they can rise to the occasion.
"That was the reason why we brought in the likes of Robbie Paul from Bradford Bulls and Martin Aspinwall and Stephen Wild from Wigan.
"They have obviously played in big games for their previous clubs and know what it takes to win on the big stage.
"These players, along with top Australians Michael De Vere and Brad Drew, are the sort of players we were lacking two years ago.
"So we know we head to Bradford on Sunday far better equipped to deal with games of this importance.
"The side that plays on Sunday will be at least 75% different from that which was in our last semi-final side. We were all a little naive and wet behind the ears, and I know I've learned a lot since then.
"I'm sure we'll see a completely different Giants performance this time around."
Sharp will keep changes to his semi-final side to an absolute minimum.
The only confirmed switch to the side that stormed to a 34-10 Super League triumph over Castleford Tigers on Sunday will be at centre.
On-loan Wigan utility back Kevin Brown is Cup-tied and is likely to be replaced in the three-quarters by Stephen Wild, although Sharp also has the option of starting with Chris Nero out in the backs.
Brown's absence also means an expected call to the bench for back-rower Paul Smith, who was 18th man against the Tigers.
But Sharp has not ruled out a return ahead of schedule for former Leeds prop Wayne McDonald.
He suffered a knee injury in the game against Leeds at the Galpharm at the start of the month and was expected to be sidelined for up to eight weeks.
But he is recovering well and could be a shock inclusion.
"For this stage of the season, we're in pretty good nick," added Sharp.
"It's obviously disappointing we won't have Kevin available, because he's been fantastic for us and is really enjoying life at the Giants.
"So, it's up to the others to make sure we don't miss him.
"We certainly have the players available to cover for his absence, and I expect everyone to rise to the occasion."
Huddersfield Giants RLFC
Stobart Super League


Watch No Offence Season 3 Episode 1 Online. Best and Free Online streaming for No Offence TV Show. We picked the best sites to stream s03e01. Simply pick a site below and click "Watch Now!" button next to it. Some of the links may be broken, please upvote the working and good links so other users see those links for No Offence Season 3 Episode 1 s03e01 at the top of the list.


When asked why I (Reginald Metts) want to be involved in helping churches, my answer is simple. I've been around Churches all of my life. I was raised in a Christian family that has produced Ministers that knows what it takes to run a church financially. I've always been interested in finding a way to help churches get the financing they need. God has provided me to work with a good company to help churches' pivotal growth of their ministry. It would be an honor to help your ministry get financing.
As for my personal involvement with churches; I am a part of two choirs, the cleaning ministry, and when called upon, I help the Deacons with the praise services. I also enjoy attending Bible Classes and Sunday School.
I attended Henry Ford Community College and Studied Computer Information and Radio Television Production. I also attended SER Metro and received Certification in Business Financing, Computer Office Skills, and Customer Services. Besides school, I've held the position as an ISO with different companies that provided funding to businesses.
Griffin Capital Funding is able to provide church loans anywhere in the United States. If you are in need of church financing, we can assist with loans for property acquisitions, refinancing, renovations, expansions and church loan consolidation.
Call now! I look forward to working with you and your church to help you achieve your goals.


Buffalo, NY – Erie County Sheriff Timothy B. Howard reports that while Deputies were investigating a one vehicle crash on Transit Road in the Town of Clarence Thursday night, a passing vehicle nearly struck the Deputies and patrol vehicles.
Deputy Rozycki responded to a call about a vehicle in a ditch around 9 p.m. and when the Deputy arrived the vehicle was unoccupied. A brief search found the operator nearby and standard field sobriety tests were administered. Anthony Remsen, 47, of Lockport, was arrested on felony DWI charges for having a previous conviction within ten years, drinking alcohol in the vehicle and other vehicle and traffic infractions.
While Deputies Rozycki, Nati, and Francis were investigating Anthony Remsen, a passing vehicle operated by Patricia Mount nearly struck the patrol vehicle. Deputies Nati and Francis pursued the vehicle and attempted to initiate a traffic stop, but she only slowed down and moved to the shoulder of the roadway. When the vehicle finally stopped, Patricia Mount, 40, of Lockport, was administered field sobriety tests; during the process, she became argumentative and confrontational with the Deputies. Mount was taken to the Clarence Substation were a chemical test revealed a BAC of .19%. Subsequent to the tests, Mount was charged with DWI, failure to use due care for a stopped emergency vehicle, and improper passing on the right. The defendant was released to a sober third party and issued tickets.
Defendant Remsen was transported to the Erie County Holding Center pending his arraignment.


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GTA 6 Next-Gen Technology Teased by Rockstar Games – ComicBook.com
According to most reports, GTA 6's release date is several years out, and given how long Red Dead Redemption 2 took Rockstar Games to make, this isn't very surprising. Rockstar Games used to release games at a rapid-fire rate, releasing GTA 3, GTA Vice City, and GTA San Andreas between 2001 and 2004. Present-day Rockstar Games now needs more time than this just to ship a single game. Why? Well, because its games now push design limits and the hardware they run on, which is why they are held as the premier developer of the industry.
To this end, during a recent GDC 2021 presentation, Rockstar Games teased that it's exploring machine learning approaches. What exactly this will mean for GTA 6 and future releases is tough to say, but judging by the presentation, it sounds like Rockstar Games is predominately investigating this technology in relationship to AI, an area of video game development that hasn't seen a ton of meaningful improvement lately.
To put this investigation into perspective, Rockstar Games revealed during the same presentation that horses have over 3,000 animations across 23 unique movement styles. That's a ton of work by the animation team, yet it sounds like it's not the peak for Rockstar Games, but the tip of the iceberg, which is why it's exploring machine learning, because there's no way it will ever be able to field an animation team capable of taking the work done on horses in RDR2 and apply it to the entire game.
I'm hyped. Apprently they're looking into machine learning approaches according to their GDC presentation. The next title is going to be insane pic.twitter.com/r2alxZaTr4
— Ben (@videotech_) August 12, 2021
For now, what the implications of this are for GTA 6 remain to be seen, but it sounds like Rockstar Games is looking to raise the bar again after raising it in 2018 with Red Dead Redemption 2, which remains the bar for game design and technical achievement. That said, this is assuming GTA 6 will be the developer's next game. Of course, this is a very safe assumption, but it's an assumption nonetheless. For all we know Rockstar Games is about to revive Table Tennis.
Until Rockstar Games revives Table Tennis with advanced machine learning, be sure to catch up on all of the latest news involving the developer and its games by clicking right here or by checking out the links right below:
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