text:
Patrick Cournot - Owner/Beverage Director
Patrick is Greenwich Village born and raised. He spent five years honing his skills at elite restaurants Bouley, Artisanal, and Tabla and went on to manage Blaue Gans, Osteria Resto & The Cannibal, Bar Henry and Lelabar. He completed his first sommelier courses while working at Danny Meyer's and Floyd Cardoz' Indian restaurant Tabla. Pairing Indian food with wines encouraged him to focus on some lesser known classic wines – graceful whites from Northern France, Germany and Austria, full and spicy reds like Bandol and Cahors, the orange wines of Italy and the amber wines from the Republic of Georgia. Outside of restaurants, Patrick spends his time with his wife Elena and daughter Lila.
Elena Hull Cournot - Designer/Owner
Elena is a painter and creative arts therapist with a private practice in the West Village. She is the designer of Ruffian's interior as well as the artist of Ruffian's horse painting, signage, and individually painted menu covers. Elena loves the intermix of culture, design, fashion, art, and personal story. She made her design choices for Ruffian in communion with Patrick's desire to illuminate the colors and variations of the wine in a warm and unpretentious setting. Her time in San Francisco, New York, Taos, and the west coast of Ireland have influenced her aesthetic. Elena lives in Brooklyn with her husband Patrick and daughter Lila.
Alexis Percival - Beverage Director/Partner
Alexis is a sommelier, event planner, an artist who puts the art in party. In addition to being certified by the Court of Master Sommeliers and WSET Level 3 certified, her wine experience covers a broad spectrum of the hospitality business. She was the owner of a Chilean wine importing company and longtime bartender at Lelabar in the West Village. Alexis has organized wine classes and produced themed wine and food dinners for a decade. Her primary objective is providing her guests with an adventure that takes them a step out of their everyday life. And Champagne...she really loves Champagne.
Josh Ochoa - Chef/Partner
Originally from small-town California, Josh Ochoa, grew up cooking Mexican influenced cuisine with his mother and grandmother. After starting his career in New Mexico, Josh moved to New York City in 2006 and worked at established restaurants like Porterhouse New York, Spice Market, and Tabla. After Tabla closed in 2010, he took the post as Sous Chef at Dressler and OTB. When not at Ruffian Josh can be found at the Library.
Andy Alexandre - Chef/Partner
Originating from Haiti, Andy Alexandre, found a profound love for cooking and sharing food in the midst of his childhood—whether it was eating the food that was being prepared at home, seeing women from farmer families make their way to the local market, or the street hawkers selling their prepared specialties. After moving to New York City in 1999, it was unclear how those memorable experiences from his adolescent years would translate to his young adult life in a new country. But in 2005 he attended culinary school while working at an ice cream shop, and two years later, he went to work at Tabla where he learned about the disciplines of the French brigade system, and the techniques of using Indian spices, which had a significant impact on his approach to cooking. Andy has also worked at North End Grill, Falai Restaurant, and most recently at Marlow and Sons.
Moshe Schulman - Director of PR/Partner
Moshe has worked in the hospitality industry for over a decade -- from mom and pop pizzerias to restaurants like Tabla, The Breslin, and Mailaino. Along with his restaurant experience, he's also a writer, filmmaker, and book publicist, which brings a strong skill set to all facets of the publicity and marketing process. He has written for The Rumpus, Orange Quarterly, Volume 1 Brooklyn, The Jewish Daily Forward, Tablet Magazine, Ravishly, Chicago Tribune, and elsewhere. He has been a featured storyteller on The Moth Radio Hour, The Moth Podcast, and NPR. His story "Then You Will Know" is featured in the New York Times Bestselling anthology "All These Wonders."
Ruffian, 125 E 7th St, New York, NY, 10009, United States


We are located in Calgary's Beltline and offer art exhibits, events, and a venue to create.
This gallery is a lifelong passion of mine. Our artistic concept in this space is to showcase Canada's best artists in all mediums while providing a space for Calgarians to host their own events.
We are conveniently located just outside Downtown Calgary in the heart of the Beltline Art District.
Featuring artistic creations of all different mediums, we curate and display some of Canada's best artists.
At over 5,000 square feet, we offer a fully stocked bar, a kitchen to handle catered events, and art lining the walls for a first-rate experience.
From art/fashion shows, private/corporate events, to weddings, The Gerry Thomas Gallery's offers bookings for all-ages social occasions.


Our two sister companies are having giveaway contests on Facebook to win a t-shirt and a mala. To enter visit the Facebook contest pages for JapaMalaBeads and YogaBasicsRetreats, read the rules and leave your comment!
On YogaBasics.com we have 4 copies of Donna DeLory's Sactuary CD to giveaway too! To enter the CD giveaway contest, simply leave a comment to this post and we will randomly select 4 comment authors on August 20th.
Offer good for U.S. Residents only, 18 years or older, 1 comment per person, multiple comments per person will be disqualified. Contest prizes provided by YogaBasics.com.
Contest ends at 11pm EST on August 20th, 2010. If you are chosen, you will be notified by email. Winners must respond within three days of the end of the contest. If you do not respond within that period, another winner will be chosen so please check your email (and spam box!) after the contest ends.
I am so excited to finally find this site! I am a new person to Yoga and I am just beginning to learn all about it as well. Hopefully I will learn alot from this site and possibly from a prize from this contest. Have a great day!
I have found that my yoga practice has greatly helped my flexibility. 8/20 is my birthday, so maybe I will win a prize too!
I just purchased a yoga studio in Westminster, MD and I'm so excited to see that your website offers so much. I'll pass it along to my teachers and students! Thank so much!
I love this site and all the yoga information and guidance it provides instructors like myself. I absolutely love Donna's music. She has the voice of an angel. In gratitude for this opportunity.
I also love this site and especially appreciate your clear and simple instructions for meditation and pranayama as well as the wide variety of yoga pose sequences that there are to try out at home. Thank You!
I would love to win a CD – teach in a variety of spaces -a traveling yogini from little ones to the senior st and always looking for good music! Love yur site!
I just attended my first class training to be a yoga instructor yesterday and I'm excited! This site has a ton of info that will help me along! Thanks!
Hi! I am elated to find this site. I have been interrested in yoga and meditation for a while now but never got the guts to start. I still havent but I found Jane's House and I plan to go check it out soon. I thought I could maybe try it out at home first. So they prize would be perfect! :) I've been having some problems lately and I don't sleep and my mind just wanders all over the place, no concentration, etc. So I was told that maybe yoga and meditation will help me? I'm hoping so! This site is great with all the information I'm finding out. I love it!
I hope I win the CD because I cannot seem to find the right yoga music.
Ok, the winning numbers are: 8, 3, 12 and 11. Check your email for notifications!


In August, the Star Tribune reported that the Eden Prairie city council had reached an agreement with the Metropolitan Council to begin the design efforts on the Town Center station on the proposed Southwest Light Rail Transit (SW LRT) line. This is the station that had been deferred two years ago when the costs of the SW LRT exceeded budget.
Hasn't funding for SW LRT been denied by the Minnesota legislature and dropped from the 2018 federal budget proposal? Why are plans going forward to design a station on a light rail line that will not be built?
The Town Center station on the proposed Southwest Light Rail line is estimated to cost $7.7M.
In January, at the end of the Obama administration, $6.1M of federal funds were provided to the Met Council to build the Town Center light rail station.
Eden Prairie needs to match 20% of that ($1.2M).
The Eden Prairie city council struck a deal with the Met Council such that Eden Prairie only needs to come up with $0.5M. The Met Council and Hennepin County will provide "their financial assistance" to fund the other $0.7M.
It is not clear from the article who will pay the other $1.6M for the station. One can only assume that this additional funding will also be coming from metro area residents and taxpayers.
Why the Eden Prairie city council even approved the $0.5M at this point is unclear. As the article points out, "full funding from the Federal Transit Administration for Southwest and other transit projects nationwide were not included in President Donald Trump's budget proposal." Maybe they believe that Congress will add that funding back into the 2018 budget.


text:
Q: How to make input field on full screan on position absolute In header i have search field, which should have with same lice container.
Some how i need to make biger input, example:
[![enter image description here][1]][1]
My code jsFiddle
$(".search-input").on("mousedown", function () {
    $(this).addClass('active');
    $('.search_container').addClass('test')
});

$(".cancel-icon").on("mousedown", function () {
    $('#search-content').hide();
    $('.search-input').removeClass('active');
    $('.search-input').val('');
    $('.search_container').removeClass('test')
});

For some reason input don't wanna go biger -_-

A: create one more class of your name. I just call it as .some and it to div.search-field when input is active and remove it when cancel-icon is clicked.
.some{
  flex-shrink: 0;
  width: 100%;
  transition: width 1s;
}

.search-field{
  ...
  width: 50%;
  ...
}

$(".search-input").on("mousedown", function () {
    ...
    $('.search-field').addClass('some');
});

$(".cancel-icon").on("mousedown", function () {
    ...
    $('.search-field').removeClass('some');
});

display: flex making the .search-field shrink. In order to avoid that I added flex-shrink: 0
Updated
Added transition: width 1s to animate a width of .search-field and added an extra style width: 50% to an existing .search-field which doesn't change the existing size but it will make impact in transition.

redpajama_set_name: RedPajamaStackExchange


Dingle was definitely the highlight of our time in Ireland. It's a little town on the west coast of Ireland in County Kerry and it's the capital of traditional music. We had three nights booked at John Benny's pub in the middle of town and stayed in an apartment out the back.
The first night in town we had a walk around and stopped in a few venues. The first had traditional music, the second had a guy with a guitar who played covers and used a loop machine. The third place was the hotel we were staying at and had a duo comprising of a young woman who sang and a man playing the guitar. They mainly sang covers and their own songs, not Irish songs. I'd expected every place to be doing trad music but the variety we encountered was good.
On the second night Jess booked us tickets for a concert in the local music shop, only a few doors down from where we were staying.
The show was mainly the man who'd played guitar at our hotel the night before (he was very good, he also sang) and a woman who sang and played the accordion. They explained a bit about trad music and the show was great plus it included half-time Irish coffees!
Luke and Jess went to another concert the next night which they said was even better. I stayed by the fire and read my kindle.
We didn't just listen to music though. We took a drive around the Dingle Peninsula and were lucky to get great weather.
The views were absolutely spectacular. There were also lots of hills that looked like great walking and made me wish we had more time to explore.
We took at look at some 'famine cottages'. While the layout was basic there was a lot of information displayed about the history of the area and the inhabitants of the cottages and what happened to them as a result of the potato famine.
Of course we also spent time in Dingle shopping and eating. I looked longingly at several pairs of Hunter boots but in the end decided I could order them online rather than lug them around Thailand.
As we left Dingle we stopped off at a very scenic little lough where took a bunch of photos and enjoyed the serenity.


Designed exclusively for active adults, this 55+ community in Lancaster, South Carolina is located just 30 minutes south of Charlotte, North Carolina. Outdoor enthusiasts and adventure seekers will enjoy fishing and kayaking on the community's 10-acre lake, bird watching at the rookery, and sightseeing on miles of walking trails. Resort-style amenities include a clubhouse with fitness center, swimming pool, tennis and pickleball. Homes priced from $275,000s to the $440,000s.


text:
(Episode 256) "Midnight Mass" Actor: Crystal Balint.
Episode 256.
"Midnight Mass"
Actor: Crystal Balint.
Welcome to Monday Morning Critic Podcast!
Crystal Balint is an award-winning actor with a career that spans more than 20 years, working extensively in both television, film and theatre in Canada and abroad. Born & raised a small town in the Rocky Mountains, Crystal has had a passion for the arts since childhood, singing and acting with her local community theatre while still in elementary school. She's followed that passion to build a career that has brought her many successes, both on the stage and the small screen.
Based in Vancouver, BC and appearing on many renown productions over the span of her career, Crystal has worked alongside some of North America's finest talent, with notable credits including sci-fi favorites like CW's The 100, Disney's Mech-X4, Supernatural, Arrow and Continuum, and dramatic series such as ABC's The Good Doctor, Prison Break, Get Shorty, The L-Word and Arctic Air. In 2019, Crystal's leading role as Iris Bearden in Britbox's spin-off series The Bletchley Circle: San Francisco won her a Best Actress Leo Award.
In addition to a recurring guest appearance in the upcoming final season of Supergirl, Crystal will next appear as a series regular in the highly anticipated Netflix original series Midnight Mass by writer/director Mike Flanagan. She will also appear in The Midnight Club, the forthcoming Mike Flanagan created series for Netflix, which is set to air in 2022.
Instagram: Monday Morning Critic Podcast.
Facebook: Monday Morning Critic Podcast.
Twitter: @DarekThomas or @mdmcritic
Website: www.mmcpodcast.com
Contact: Mondaymorningcritic@gmail.com
Welcome, Crystal Balint!

redpajama_set_name: RedPajamaCommonCrawl


The Greater Ontario Junior Hockey League's Western Conference final resumed in London Saturday night.
The Leamington Flyers now find themselves down 2-0 in the best-of-seven series with the Nationals after a 5-2 loss.
Rory DiNiro and Zach Taylor were the goal scorers for Leamington.
The Flyers will try to make up some ground as the teams return to Leamington for game three Sunday night.


We would like to invite you to the next presentation in our series of free online CIDER sessions. This session features a presentation and discussion with Dr. Rita Kop and Dr. Helene Fournier of the National Research Council, Canada.
After speculation in the literature about the nature of possible Personal Learning Environments, research in the design and development of a PLE is now in progress. The researchers will report on the educational research involved in the National Research Council of Canada, Institute for Information Technology's Personal Learning Environment project. This presentation will highlight important components, applications and tools in a PLE as identified through surveys of potential end users. The learner experience and the minimum set of components required to facilitate quality learning will be placed at the forefront.
This entry was tagged cider videoconference research distance_learning. Bookmark the permalink.


text:
\section{\textbf{Introduction}}

Numerous cosmological observations of type Ia supernova, cosmic microwave
background anisotropies measured with WMAP and large scale structure,
suggest that our universe is undergoing in an accelerated expansion possibly
due to the presence of dark energy which possesses negative pressure \cit
{1}. In the astrophysics community, the nature of such mysterious
form of energy is still a matter of debate. In cosmology, several
candidates responsible for this expansion have been proposed namely,
Chaplygin gas, modified gravity, scalar tensor theory, tachyon and
braneworld model, to a name a few \cite{2}. Despite the fact that
the cosmological constant is the most obvious candidate that offers
a solution to the dark energy problem, yet it has several drawbacks
like fine-tuning and coincidence problems.

In order to soften the cosmic coincidence and fine tuning problems,
models of dark energy interacting with dark matter have been
proposed \cite{3}. It is generally asked that if the universe
evolves from the earlier quintessence ($\omega >-1$) to late
accelerating universe with phantom regime ($\omega <-1$), then why
$\omega =-1$ crossing occurs at the present time, where
 $\omega={p}/{\rho }$. The equation of state (EoS) parameter $\omega $
changes at different cosmic epoch which supports the evolving dark
energy \cite{4}. In the cosmological model explaining dark energy,
the ratio of energy densities of dark matter and dark energy
$\mathit{r}_{m}$ is of order unity, while observations suggest that
in pure dark energy model, this ratio must decrease. It may implies
the transfer of energy occurs between these two entities to keep a
subtle balance at the current time. The interaction between these
entities involves a coupling constant that determines the strength
of this interaction. Besides Einstein gravity, this study of
interaction can also be extended to $f(R)$, Brans-Dicke, braneworld,
Horava-Lifshitz and Gauss-Bonnet gravities \cite{5}.

In recent times, considerable interest has been stimulated to explain the
observed dark energy (dominant force in cosmos) with the help of holographic
dark energy model \cite{6}. According to holographic principle, the number
of degrees of freedom in a bounded physical system should be finite and has
relationship with the area of its boundary rather than with its volume \cit
{7}. It is commonly believed that the holographic principle is a
fundamental principle of quantum gravity which is used to explain
the events involving high energy scale. It is motivated from an
observation that in quantum field theory, the ultra-violet cut-off
$\Lambda $ could be related to the infrared cut-off $L$ due to the
limit set by forming a black hole i.e. the quantum zero-point energy
of a system with size $L$ should not exceed the mass of a black hole
with the same size, i.e. $L^{3}\Lambda ^{3}\leq (M_{p}L)^{3/2}$
\cite{8}$.$ This last expression can be re-written as $L^{3}\rho
_{\Lambda }\leq LM_{p}^{2},$ where $\rho _{\Lambda }\backsim \Lambda
^{4}$ is the energy density corresponding to the zero point energy
and cut-off $\Lambda .$ Now the last inequality takes the form $\rho
_{\Lambda }\leq M_{p}^{2}L^{-2}$ or $\rho _{\Lambda
}=3n^{2}M_{p}^{2}L^{-2}.$ Here $3n^{2}$ is a constant and attached
for convenience. A sufficient literature is available on the study
of interaction between the holographic dark energy and the matter
\cite{9}. We are interested in studying the dynamics of entropy
corrected holographic dark energy (ECHDE) when it interacts with
some exotic type fluids. The entropy
corrected holographic dark energy is given by \cite{10
\begin{equation}
\rho _{\Lambda }=3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln
(m_{p}^{2}L^{2})+\beta L^{-4},
\end{equation
where the first term on right hand side is the usual holographic
dark energy while the other two appeared are mainly due to quantum
corrections in the loop quantum gravity (LQG). The correction term
play crucial role in early universe when L is small. When L gets
large, ECHDE reduces to HDE. The expression for the corrected
entropy of the black hole is given by $S=\frac{A}{4G}+\gamma \ln
(\frac{A}{4G})+\beta $ is
mainly arise due to the thermal equilibrium and quantum fluctuation \cite{11
. The parameters $n^{2},$ $\gamma $ and $\beta $ constant of order unity. If
we choose $\gamma $ and $\beta $ to be zero we arrive at the usual
holographic dark energy model. The parameter $n$ can be a function of time
\cite{12}, but in our discussion it is purely a constant quantity.

The plane of the paper is as follows: In section 2, the model of
Friedmann-Robertson-Walker (FRW) universe and the relevant equations are
presented. In section 3, we discuss a correspondence between ECHDE and
different Chaplygin gas forms including the modified variable Chaplygin gas
(MVCG) and new modified Chaplygin gas (NMCG) and the viscous generalized
Chaplygin gas (VGCG). In each case, we reconstruct the potentials and the
dynamics of the scalar field which describe the entropy corrected
holographic Chaplygin cosmology. The final section is devoted to the
conclusion.

\section{The model}

We start by assuming the background spacetime to be spatially
homogeneous and isotropic FRW spacetime given by
\begin{equation}
ds^{2}=-dt^{2}+a^{2}(t)\left[ \frac{dr^{2}}{1-kr^{2}}+r^{2}(d\theta
^{2}+\sin ^{2}\theta d\varphi ^{2})\right] .
\end{equation
Here $a(t)$ is the dimensionless scale factor which is an arbitrary function
of time and $k$ is defined to be the curvature parameter which has
dimensions of \emph{length}$^{-2}$ and its different values describe the
spatial geometry. For instance, for $k=-1,0,1,$ the above metric (2)
represents the spatially open, flat and closed FRW spacetimes respectively.
The Friedmann equation is given b
\begin{equation}
H^{2}+\frac{k}{a^{2}}=\frac{1}{3m_{p}^{2}}[\rho _{\Lambda }+\rho _{m}],
\end{equation
where $m_{p}^{2}=(8\pi G)^{-1}$ is modified Planck mass. Here $H=\dot{a}/a$
is the Hubble parameter while $\rho _{\Lambda }$ and $\rho _{m}$ are the
energy densities of dark energy and matter respectively. In dimensionless
form, Eq. (3) can be written a
\begin{equation}
1+\Omega _{k}=\Omega _{\Lambda }+\Omega _{m}.
\end{equation
The dimensionless density parameters corresponding to matter, dark energy
and curvature ar
\begin{equation}
\Omega _{m}=\frac{\rho _{m}}{\rho _{cr}}=\frac{\rho _{m}}{3H^{2}m_{p}^{2}}
\text{ }\Omega _{\Lambda }=\frac{\rho _{\Lambda }}{\rho _{cr}}=\frac{\rho
_{\Lambda }}{3H^{2}m_{p}^{2}},\text{ }\Omega _{k}=\frac{k}{(aH)^{2}}.
\end{equation
Here $\rho _{cr}=3H^{2}m_{p}^{2}$ is the critical density. The energy
conservation equations for dark energy and dark matter ar
\begin{eqnarray}
\dot{\rho}_{\Lambda }+3H(\rho _{\Lambda }+p_{\Lambda }) &=&-Q, \\
\dot{\rho}_{m}+3H\rho _{m} &=&Q.
\end{eqnarray
Here overdot represents the differentiation with respect to cosmic
co-moving time $t$. Eq. (6) and (7) show that if there is an
interaction between dark energy and dark matter, the energy
conservation for dark energy and matter would not hold independently
but for the total interacting system. In explicit form, we have
$p_{\Lambda }=\omega _{\Lambda }\rho _{\Lambda }$ and $p_{m}=0.$
During the energy transfer, local energy conservation will not hold
in general but for the whole interacting system. Naturally if two
species are present in dominant form, it is obvious that they will
interact. If the quantity $Q$ is positive, it shows the transfer of
energy from dark matter to dark energy and vice versa in the case
when $Q$ is negative. The importance of interacting dark energy and
dark matter model also emerges since it is the best fit for the data
we obtain from the physical observations for instance SN Ia and
cosmic microwave background \cite{1}.

Defining the effective equation of state for dark energy and dark matter as
\cite{13
\begin{equation}
\omega _{\Lambda }^{\text{eff}}=\omega _{\Lambda }+\frac{\Gamma }{3H},\text{
}\omega _{m}^{\text{eff}}=-\frac{1}{r_{m}}\frac{\Gamma }{3H},
\end{equation
where the term $\Gamma =Q/\rho _{\Lambda }$ represents the decay
rate. After employing Eq. (8) in (6) and (7), we obtain the
following pair of
continuity equation
\begin{eqnarray}
\dot{\rho}_{\Lambda }+3H(1+\omega _{\Lambda }^{\text{eff}})\rho _{\Lambda }
&=&0 \\
\dot{\rho}_{m}+3H(1+\omega _{m}^{\text{eff}})\rho _{m} &=&0.
\end{eqnarray
If we take $L$ as the Hubble scale $H^{-1}$ i.e. $L=H^{-1}$ at the present
epoch $H=H_{0}\backsim 10^{-33}eV,$ then the energy density $\rho _{\Lambda }
$ is comparable with the observed dark energy density $\backsim
10^{-10}eV^{4}.$ The second option for the infra-red cut-off is the particle
horizon. Hsu \cite{14} showed that under this scenario the resulting EoS
becomes zero and does not lead to an accelerated universe. So to get an
accelerated expansion of the observable universe, Li \cite{15} proposed that
the IR cut-off $L$ should be taken as the future event horizon and he
defined it a
\begin{equation}
L=a(t)r(t),
\end{equation
here $r(t)$ is related to the future event horizon of the observable
universe. Using the FRW metric, we can obtain \cite{15}
\begin{equation}
L=a(t)\frac{\text{sinn}(\sqrt{|k|}y)}{\sqrt{|k|}},\ \ \ y=\frac{R_{h}}{a(t)},
\end{equation
where $R_{h}$ is the size of the future event horizon defined as
\begin{equation}
R_{h}=a(t)\int\limits_{t}^{\infty }\frac{dt^{\prime }}{a(t^{\prime })
=a(t)\int\limits_{0}^{r_{1}}\frac{dr}{\sqrt{1-kr^{2}}}.
\end{equation
The last integral has the explicit form as
\begin{equation}
\int\limits_{0}^{r_{1}}\frac{dr}{\sqrt{1-kr^{2}}}=\frac{1}{\sqrt{|k|}}\text
sinn}^{-1}(\sqrt{|k|}r_{1})=\begin{cases}\text{sin}^{-1}(r_1) , & \,
\,k=+1,\\ r_1, & \, \, k=0,\\ \text{sinh}^{-1}(r_1), & \, \,k=-1.\\
\end{cases}
\end{equation
Using the definition of $\rho _{\Lambda }$ and $\rho _{cr},$ we obtain the
following relation
\begin{equation}
HL=\sqrt{\frac{3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2
}{3m_{p}^{2}\Omega _{\Lambda }}}.
\end{equation
Differentiate eq. (12) with respect to time $t$\ and using Eq. (16), we hav
\begin{equation}
\dot{L}=\sqrt{\frac{3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2}}{3m_{p}^{2}\Omega _{\Lambda
}}}-\text{cosn}(\sqrt{|k|}y),
\end{equation
wher
\begin{equation}
\text{cosn}(\sqrt{|k|}y)=\begin{cases} \text{cos}y , \, \,k=+1,\\ 1, \, \,
k=0,\\ \text{cosh}y, \, \,k=-1,\\ \end{cases}
\end{equation
After taking derivative of (1) with respect to $t,$ we ge
\begin{eqnarray}
\dot{\rho}_{\Lambda } &=&(2\gamma L^{-5}-4\gamma L^{-5}\ln
(m_{p}^{2}L^{2})-4\beta L^{-5}-6n^{2}m_{p}^{2}L^{-3})  \nonumber \\
&&\times \left[ \sqrt{\frac{3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2}}{3m_{p}^{2}\Omega _{\Lambda }}}-\text{cosn}
\sqrt{|k|}y)\right] .
\end{eqnarray
Using Eq. (18) in (6), we arrive at
\begin{eqnarray}
w_{\Lambda } &=&-1-\Big(\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln
(m_{p}^{2}L^{2})-4\beta L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma
L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2})}\Big)  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right] -\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }}.
\end{eqnarray
Now making use of Eq. (19) in (8) yield
\begin{eqnarray}
w_{\Lambda }^{\text{eff}} &=&-1-\Big(\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln
(m_{p}^{2}L^{2})-4\beta L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma
L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2})}\Big)  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right] .
\end{eqnarray}

\section{Correspondence between ECHDE and Chaplygin gas variants}

Since there are several candidates of dark energy, so it is
essential to develop a correspondence and the relationships between
them. Kamenshchik et al \cite{16} studied a homogenous model based
on a single fluid obeying the EoS $p=-\frac{A_{0}}{\rho }$ called
the Chaplygin gas, where $p$ and $\rho $ represent the pressure and
energy density of the fluid and $A_{0}$ is some positive constant.
Possessing many physically interesting features, several authors
have used it to model the accelerated expansion of universe
\cite{17}. But it does not satisfactorily address the problems like
structure formation and cosmological perturbation power spectrum
\cite{18}. Subsequently, this equation was modified to the form
$p=-\frac{A_{0}}{\rho ^{\alpha }}$ called generalized Chaplygin gas
(GCG) to construct viable cosmological models. Two free parameters
involved in it: one is $A_{0}$ and the other $0\leq \alpha \leq 1.$
The GCG fluid behaves like dust for small size of the universe while
it acts as cosmological constant when universe gets sufficiently
large. The GCG equation has been further modified to $p=B\rho -\frac{A_{0}}
\rho ^{\alpha }}$ with $0\leq \alpha \leq 1,$ which is called
modified Chaplygin gas (MCG) \cite{19} and it involves \ three
parameters. An interesting feature connected with MCG equation of
state is that it shows radiations era in the early universe. At the
late time it behaves as cosmological constant which can be fitted to
a $\Lambda $CDM model. Late on, Guo and Jhang \cite{20} first
proposed a model $p=B\rho -\frac{A_{0}}{\rho ^{\alpha }}$ by taking
$A_{0}$ as a function of the cosmological scale factor $a(t)$ i.e.
$A_{0}=A_{0}(a(t)),$ which is known as modified variable Chaplygin
gas (MVCG) \cite{21}. This assumption seems to be reasonable since
$A_{0}(a(t))$ is related to scalar potential if we interpret
Chaplygin gas via Born-Infeld scalar field.

\subsection{Modified variable Chaplygin gas and ECHDE}

Suppose we have two species i.e. dark matter and dark energy. The later is
specified by the MVCG which is given by
\begin{equation}
p=B\rho _{\Lambda }-\frac{B_{0}a^{-\delta }}{\rho _{\Lambda
}^{\alpha }}.
\end{equation
The evolution of the energy density of MVCG is
\begin{equation}
\rho _{\Lambda }=\Big[\frac{3(\alpha +1)B_{0}}{[3(\alpha +1)(B+1)-\delta ]
\frac{1}{a^{\delta }}-\frac{C}{a^{3(\alpha +1)(B+1)}}\Big]^{\frac{1}{\alpha
+1}},
\end{equation
where $B_{0}$ and $C$ are some constants.

We now reconstruct expressions of the potential and the dynamics of the
scalar field in the presence of ECHDE. So for this, consider a time
dependent scalar field $\phi (t)$ with potential $V(\phi ),$ which are
directly related with the energy density and pressure of MVCG a
\begin{eqnarray}
\rho _{\Lambda } &=&\frac{1}{2}\dot{\phi}^{2}+V(\phi ), \\
p_{\Lambda } &=&\frac{1}{2}\dot{\phi}^{2}-V(\phi ).
\end{eqnarray
Since the kinetic terms are positive hence it means that MVCG is of
quintessence type. Adding Eqs. (23) and (24), we get the kinetic ter
\begin{eqnarray}
\dot{\phi}^{2} &=&(1+B)\Big[\frac{3(\alpha +1)B_{0}}{[3(\alpha
+1)(B+1)-\delta ]}\frac{1}{a^{\delta }}-\frac{C}{a^{3(\alpha +1)(B+1)}}\Big
^{\frac{1}{\alpha +1}}  \nonumber \\
&&-\frac{B_{0}a^{-\delta }}{\Big[\frac{3(\alpha +1)B_{0}}{[3(\alpha
+1)(B+1)-\delta ]}\frac{1}{a^{\delta }}-\frac{C}{a^{3(\alpha +1)(B+1)}}\Big
^{\frac{\alpha }{\alpha +1}}}.
\end{eqnarray
Subtraction of Eqs. (23) and (24) yields the potential ter
\begin{eqnarray}
2V(\phi ) &=&(1-B)\Big[\frac{3(\alpha +1)B_{0}}{[3(\alpha +1)(B+1)-\delta ]
\frac{1}{a^{n}}-\frac{C}{a^{3(\alpha +1)(B+1)}}\Big]^{\frac{1}{\alpha +1}}
\nonumber \\
&&+\frac{B_{0}a^{-\delta }}{\Big[\frac{3(\alpha +1)B_{0}}{[3(\alpha
+1)(B+1)-\delta ]}\frac{1}{a^{\delta }}-\frac{C}{a^{3(\alpha +1)(B+1)}}\Big
^{\frac{\alpha }{\alpha +1}}}.
\end{eqnarray
To see the correspondence between the ECHDE and MVCG energy density, we use
Eqs. (1) and (22) to get
\begin{equation}
C=a^{3(\alpha +1)(B+1)}\Big[\frac{3(\alpha +1)B_{0}}{[3(\alpha
+1)(B+1)-\delta ]}\frac{1}{a^{\delta }}-(3n^{2}m_{p}^{2}L^{-2}+\gamma
L^{-4}\ln (m_{p}^{2}L^{2})+\beta L^{-4})^{\alpha +1}\Big].
\end{equation
Writing Eq. (21) in an alternate for
\begin{equation}
B_{0}=a^{\delta }(B-w_{\Lambda })\rho _{\Lambda }^{\alpha +1}.
\end{equation
Therefore in view of Eq. (19), the above equation (28) gives the value of
the parameter $B_{0}$ a
\begin{eqnarray}
B_{0} &=&a^{\delta }(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln
(m_{p}^{2}L^{2})+\beta L^{-4})^{\alpha +1}\Big[1+B  \nonumber \\
&&+\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln (m_{p}^{2}L^{2})-4\beta
L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2})}  \nonumber \\
&&\times \left( 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right) +\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }}\Big].
\end{eqnarray
Now to determine the other parameter $C$ substitute the value of $B_{0}$ in
Eq. (27), we hav
\begin{eqnarray}
C &=&a^{3(\alpha +1)(A+1)}(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln
(m_{p}^{2}L^{2})+\beta L^{-4})^{\alpha +1}\Big(\frac{3(\alpha +1)}{[3(\alpha
+1)(B+1)-\delta ]}  \nonumber \\
&&\times (B+1+\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln (m_{p}^{2}L^{2})-4\beta
L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2})})  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right] -1\Big)
\end{eqnarray
Now we can re-write the kinetic energy and scalar potential terms as
\begin{eqnarray}
\dot{\phi}^{2} &=&-(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln
(m_{p}^{2}L^{2})+\beta L^{-4})  \nonumber \\
&&\Big(\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln (m_{p}^{2}L^{2})-4\beta
L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2})}  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right] +\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }}\Big),
\end{eqnarray
an
\begin{eqnarray}
2V(\phi ) &=&(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln (m_{p}^{2}L^{2})+\beta
L^{-4})  \nonumber \\
&&\times \Big(2+\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln
(m_{p}^{2}L^{2})-4\beta L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma
L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2})}  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right] +\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }}\Big)
\end{eqnarray
Using the relation $x=\ln a,$ we get $\dot{\phi}=\phi ^{\prime }H,$ where
^{\prime }$ represents the derivative with respect to e-folding time
parameter $\ln a.$ After putting the value of $\dot{\phi}$ and applying
integration, we obtai
\begin{eqnarray}
\phi (a)-\phi (a_{0}) &=&\frac{1}{H}\int_{0}^{\ln
a}[-(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln (m_{p}^{2}L^{2})+\beta L^{-4})
\nonumber \\
&&\times \Big(\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln (m_{p}^{2}L^{2})-4\beta
L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2})}  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right] \Big)+\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }
]^{1/2}d\ln a,  \nonumber \\
&&
\end{eqnarray
where $a_{0}$ is the present value of the scale factor.

\subsection{New modified Chaplygin gas model and ECHDE}

The model that represents the dark energy is now the new modified Chaplygin
gas (NMCG) given by \cite{22
\begin{equation}
p_{\Lambda }=B\rho _{\Lambda }-\frac{K(a)}{\rho _{\Lambda }^{\alpha }},\text{
\ \ where }B>0\text{ and }0\leq \alpha \leq 1.
\end{equation
Here $K(a)$ is a function of scale factor of the universe. Taking $K(a)$ in
the form $K(a)=-\omega _{\Lambda }A_{1}a^{-3(w_{\Lambda }+1)(\alpha +1)}$ as
introduced by the authors in \cite{23}, we ge
\begin{equation}
p_{\Lambda }=B\rho _{\Lambda }+\frac{w_{\Lambda }A_{1}}{\rho _{\Lambda
}^{\alpha }}a^{-3(w_{\Lambda }+1)(\alpha +1)}.
\end{equation
The energy density of the NMCG can be expressed a
\begin{equation}
\rho _{\Lambda }=\Big[\frac{w_{\Lambda }}{w_{\Lambda }-B}A_{1}a^{-3(w_
\Lambda }+1)(\alpha +1)}+B_{1}a^{-3(B+1)(\alpha +1)}\Big]^{\frac{1}{\alpha +
}},
\end{equation
where $B_{1}$ is a constant of integration. Following the previous
section we establish the correspondence between the ECHDE and NMCG
energy density.
Comparing Eqs. (36) and (1), we ge
\begin{eqnarray}
B_{1} &=&a^{3(B+1)(\alpha +1)}\Big((3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln
(m_{p}^{2}L^{2})+\beta L^{-4})^{\alpha +1}  \nonumber \\
&&-\frac{1+\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln (m_{p}^{2}L^{2})-4\beta
L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2})}\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega
_{\Lambda }}{3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}
\text{cosn}(\sqrt{|k|}y)\right] }{1+B+\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln
(m_{p}^{2}L^{2})-4\beta L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma
L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2})}\times \left[ 1-\sqrt{\frac
3m_{p}^{2}\Omega _{\Lambda }}{3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}(\sqrt{|k|}y)\right] }  \nonumber
\\
&&\times \Big(A_{1}a^{3(\alpha +1)\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln
(m_{p}^{2}L^{2})-4\beta L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma
L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2})}\times \left[ 1-\sqrt{\frac
3m_{p}^{2}\Omega _{\Lambda }}{3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}(\sqrt{|k|}y)\right] }\Big)\Big).
\end{eqnarray
With the use of $p_{\Lambda }=\omega _{\Lambda }\rho _{\Lambda },$ Eq. (35)
gives an expression for $A_{1}$ i.e
\begin{eqnarray}
A_{1} &=&(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln (m_{p}^{2}L^{2})+\beta
L^{-4})^{\alpha +1}  \nonumber \\
&&\times a^{-3(\alpha +1)\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln
(m_{p}^{2}L^{2})-4\beta L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma
L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2})}\times \Big(1-\sqrt{\frac
3m_{p}^{2}\Omega _{\Lambda }}{3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}(\sqrt{|k|}y)\Big)}  \nonumber \\
&&\times \left[ \frac{B+1+\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln
(m_{p}^{2}L^{2})-4\beta L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma
L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2})}\times \left[ 1-\sqrt{\frac
3m_{p}^{2}\Omega _{\Lambda }}{3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}(\sqrt{|k|}y)\right] }{1+\frac
2\gamma L^{-2}-4\gamma L^{-2}\ln (m_{p}^{2}L^{2})-4\beta
L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2})}\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega
_{\Lambda }}{3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}
\text{cosn}(\sqrt{|k|}y)\right] }\right] .  \nonumber \\
&&
\end{eqnarray
So we have found the expressions for the constants $A_{1}$ and $B_{1}.$
Employing Eqs. (23) and (24), the kinetic and potential terms are found to b
\begin{eqnarray}
\dot{\phi}^{2} &=&(B+1)\Big[\frac{w_{\Lambda }}{w_{\Lambda }-B
A_{1}a^{-3(w_{\Lambda }+1)(\alpha +1)}+B_{1}a^{-3(B+1)(\alpha +1)}\Big]^
\frac{1}{\alpha +1}}  \nonumber \\
&&+\frac{A_{1}w_{\Lambda }a^{-3(w_{\Lambda }+1)(\alpha +1)}}{[\frac
w_{\Lambda }}{w_{\Lambda }-B}A_{1}a^{-3(w_{\Lambda }+1)(\alpha
+1)}+B_{1}a^{-3(B+1)(\alpha +1)}]^{\frac{\alpha }{\alpha +1}}},
\end{eqnarray
and
\begin{eqnarray}
2V(\phi ) &=&(1-B)[\frac{w_{\Lambda }}{w_{\Lambda }-B}A_{1}a^{-3(w_{\Lambda
}+1)(\alpha +1)}+B_{1}a^{-3(B+1)(\alpha +1)}]^{\frac{1}{\alpha +1}}
\nonumber \\
&&-\frac{A_{1}w_{\Lambda }a^{-3(w_{\Lambda }+1)(\alpha +1)}}{[\frac
w_{\Lambda }}{w_{\Lambda }-B}A_{1}a^{-3(w_{\Lambda }+1)(\alpha
+1)}+B_{1}a^{-3(B+1)(\alpha +1)}]^{\frac{\alpha }{\alpha +1}}},
\end{eqnarray
where $A_{1}$ and $B_{1}$ are given in (38) and (37) respectively.
In all Eqs. (35), (36), (39) and (40) the value of $ w_{\Lambda }$
is given by Eq. (19). From Eqs. (23) and
(24), the kinetic energy term is re-written to b
\begin{eqnarray}
\dot{\phi}^{2} &=&-(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln
(m_{p}^{2}L^{2})+\beta L^{-4})  \nonumber \\
&&\times \Big(\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln (m_{p}^{2}L^{2})-4\beta
L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2})}  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right] +\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }}\Big),
\end{eqnarray
while the potential energy term has the for
\begin{eqnarray}
2V(\phi ) &=&(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln (m_{p}^{2}L^{2})+\beta
L^{-4})  \nonumber \\
&&\times \Big(2+\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln
(m_{p}^{2}L^{2})-4\beta L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma
L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2})}  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right] +\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }}\Big).
\nonumber \\
&&
\end{eqnarray
Following the same steps as done for the MVCG, the kinetic term is easily
transformable to the following for
\begin{eqnarray}
\phi (a)-\phi (a_{0}) &=&\frac{1}{H}\int_{0}^{\ln
a}[-(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln (m_{p}^{2}L^{2})+\beta L^{-4})
\nonumber \\
&&\times \frac{2\gamma L^{-2}-4\gamma L^{-2}\ln (m_{p}^{2}L^{2})-4\beta
L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2})}  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right] +\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }
]^{1/2}d\ln a.  \nonumber \\
&&
\end{eqnarray}

\subsection{Viscous generalized Chaplygin gas model and ECHDE}

If we assume that the dark energy as non-viscous as taken in section A and
B, it must results in the occurrence of a cosmic singularity (Big Rip) in
the far future. This singularity can be alleviated by introducing the
quantum corrections due to the conformal anomaly while the other option is
to consider the bulk viscosity $\xi $ of the cosmic fluid \cite{24}. The
theory of bulk viscosity was initially investigated by Eckart and later on
pursued by Landau and Lifshitz \cite{25}. The important feature of dark
energy with bulk viscosity is that it shows the accelerated expansion of
phantom type in the later epoch and softens the coincidence problem, age
problem and phantom crossing \cite{26}. The effective pressure containing
the isotropic pressure and viscous stress is given by the equation of stat
\begin{equation}
p_{\text{eff}}=p_{\Lambda }+\Pi ,
\end{equation
where $p_{\Lambda }=\frac{\chi }{\rho _{\Lambda }^{\alpha }},$ $\chi >0.$
Notice that first term on the right hand side mimics the GCG and the
parameter $\alpha $ varies as $0<\alpha \leq 1.$ If $\alpha =1$ it
represents the Chaplygin gas model. On the other hand if $\alpha <0$, it
corresponds to a polytropic gas. The bulk viscous fluid is represented by
\Pi =-\xi (\rho _{\Lambda })u_{;\mu }^{\mu }$ where $u^{\mu }$ is the
four-velocity vector of the viscous fluid and $\xi >0$ to get the positive
entropy production in conformity with second law of thermodynamics \cite{27
. We choose $\xi (\rho _{\Lambda })=\nu \rho _{\Lambda }^{1/2}$,
with $\nu $ as constant. The energy conservation equation yields the
energy density of
VGCG a
\begin{equation}
\rho _{\Lambda }=[\frac{Da^{-3(\alpha +1)(1-\nu \gamma _{1})}-\chi }{(1-\nu
\gamma _{1})}]^{\frac{1}{\alpha +1}},
\end{equation}
\cite{28}. Here $\gamma _{1}=m_{p}^{-1}\sqrt{1-r_{m}},$ where $r_{m}=\frac
\rho _{m}}{\rho _{\Lambda }}=\frac{\Omega _{m}}{\Omega _{\Lambda }}$ and $D$
some constant of integration. The effective equation of state (45) says that
the universe is expanding in accelerated manner. It has been shown that this
phenomenon of universe can be studied with the help of dynamical evolving
scalar fields usually called inflation. So it was introduced to construct
models dealing with minimally coupled scalar field. Hence we construct the
dynamical scalar field $\phi $ with potential $V(\phi ),$ related to the
energy density and pressure of viscous dark energy model a
\begin{eqnarray}
\rho _{\Lambda } &=&[\frac{Da^{-3(\alpha +1)(1-\nu \gamma _{1})}-\chi }
(1-\nu \gamma _{1})}]^{\frac{1}{\alpha +1}},  \nonumber \\
p_{\Lambda } &=&\chi \lbrack \frac{(1-\nu \gamma _{1})}{Da^{-3(\alpha
+1)(1-\nu \gamma _{1})}-\chi }]^{\frac{\alpha }{\alpha +1}}-3\nu H[\frac
Da^{-3(\alpha +1)(1-\nu \gamma _{1})}-\chi }{(1-\nu \gamma _{1})}]^{1/2}.
\end{eqnarray
To determine the expressions for the unknown $D$ and $\chi $ we take the
following steps. The effective equation of state for the interacting VGCG i
\begin{equation}
w_{\Lambda }^{\text{eff}}=\frac{\chi }{\rho _{\Lambda }^{\alpha +1}
-3\upsilon H\rho _{\Lambda }^{-\frac{1}{2}}+\frac{b^{2}(1+\Omega _{k})}
\Omega _{\Lambda }}.
\end{equation
After substituting the value of $w_{\Lambda }^{\text{eff}}$ in (47) and
making simplification, we obtai
\begin{eqnarray}
\chi  &=&(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln (m_{p}^{2}L^{2})+\beta
L^{-4})^{\alpha +1}  \nonumber \\
&&\times \Big(-1-\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln
(m_{p}^{2}L^{2})-4\beta L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma
L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2})}  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right]   \nonumber \\
&&+3\upsilon H(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln (m_{p}^{2}L^{2})+\beta
L^{-4})^{-1/2}-\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }}\Big).
\nonumber \\
&&
\end{eqnarray
Inserting the value of $\chi $ in (45), we ge
\begin{eqnarray}
D &=&a^{3(\alpha +1)(1-\nu \gamma _{1})}(3n^{2}m_{p}^{2}L^{-2}+\gamma
L^{-4}\ln (m_{p}^{2}L^{2})+\beta L^{-4})^{\alpha +1}  \nonumber \\
&&\times \lbrack -\nu \gamma _{1}-\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln
(m_{p}^{2}L^{2})-4\beta L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma
L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2})}  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right]   \nonumber \\
&&+3\upsilon H(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln (m_{p}^{2}L^{2})+\beta
L^{-4})^{-\frac{1}{2}}-\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }}].
\nonumber \\
&&
\end{eqnarray
Now we can re-write the scalar potential and kinetic energy terms as
followin
\begin{eqnarray}
2V(\phi ) &=&(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln (m_{p}^{2}L^{2})+\beta
L^{-4})  \nonumber \\
&&\times (2+\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln (m_{p}^{2}L^{2})-4\beta
L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2})}  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right] +\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }}).
\nonumber \\
&&
\end{eqnarray
an
\begin{eqnarray}
\dot{\phi}^{2} &=&-(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln
(m_{p}^{2}L^{2})+\beta L^{-4})  \nonumber \\
&&\times \Big(\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln (m_{p}^{2}L^{2})-4\beta
L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2})}  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right] +\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }}\Big).
\end{eqnarray
Again using the equation $\dot{\phi}=\phi ^{\prime }H,$ we can writ
\begin{eqnarray}
\phi (a)-\phi (a_{0}) &=&\frac{1}{H}\int_{0}^{\ln
a}[-(3n^{2}m_{p}^{2}L^{-2}+\gamma L^{-4}\ln (m_{p}^{2}L^{2})+\beta L^{-4})
\nonumber \\
&&\times (\frac{2\gamma L^{-2}-4\gamma L^{-2}\ln (m_{p}^{2}L^{2})-4\beta
L^{-2}-6n^{2}m_{p}^{2}}{3(3n^{2}m_{p}^{2}+\gamma L^{-2}\ln
(m_{p}^{2}L^{2})+\beta L^{-2})}  \nonumber \\
&&\times \left[ 1-\sqrt{\frac{3m_{p}^{2}\Omega _{\Lambda }}
3n^{2}m_{p}^{2}+\gamma L^{-2}\ln (m_{p}^{2}L^{2})+\beta L^{-2}}}\text{cosn}
\sqrt{|k|}y)\right] +\frac{b^{2}(1+\Omega _{k})}{\Omega _{\Lambda }
)]^{1/2}d\ln a.  \nonumber \\
&&
\end{eqnarray
It is interesting to note that the above potential and kinetic energy
expressions for the interacting ECHDE with the viscous generalized Chaplygin
gas coincide with the non-viscous case.

\section{Conclusion}

Enormous literature dealing with the subject of dark energy is available but
the holographic dark energy is considered to be the most promising candidate
of dark energy. In this paper we have constructed a correspondence between
the interacting ECHDE and the Chaplygin gas variants. Several candidates of
dark energy have been suggested to describe cosmic acceleration but
Chaplygin gas has emerged as a unification of dark energy and dark matter.
It's cosmic evolution is similar to initial dust like matter while it
behaves as a cosmological constant at a later epoch. In the present work, we
have investigated a model of dark energy in the presence of entropy
corrections to holographic dark energy. In this context, a link between the
ECHDE and various models of Chaplygin gas has been established. We have
found the kinetic and potential energies corresponding to each model and
also reconstructed the potentials.

redpajama_set_name: RedPajamaArXiv


text:
Q: Ontotext GraphDB SPARQL Query - No acceptable file format found Ontotext GraphDB 9.0.0, Free Edition, Ubuntu Workstation Linux 4.15.0-65-generic x86_64
I have a simple SPARQL query that works fine in the Query & Update page and from the web service:
select * where {
    ?s ?p ?o .
} limit 5

and if I don't provide an Accept: header I get the results back as comma separated values.  However, if I provide a file format like this:
$ curl -G -H "Accept: text/turtle" 'http://localhost:7200/repositories/...'
No acceptable file format found.

Is there list of or a REST query for acceptable media types?

A: A SELECT query does not return an RDF graph (in Turtle or any other synatx)- it returns a SPARQL Result set.
application/sparql-results+json is one format.
If you want an RDF graph, use a CONSTRUCT query and you can ask for text/turtle:
CONSTRUCT { ?s ?p ?o } WHERE { ?s ?p ?o } LIMIT 5

That particular query can be shortened to:
CONSTRUCT WHERE { ?s ?p ?o } LIMIT 5


text:
Q: How to fix annoying Android Emulator Configuration window scroll glitch? Ever since I installed Android Studio, I'm already experiencing this. I can't see the remaining options below. Every time I scroll down, this happens.
enter image description here


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text:
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Studios : Hasbro
The X-Men created by Stan Lee and Jack Kirby
Family Matters 3-Pack with Magneto Action Figure
Magneto #1 Review
Magneto Returns in X-Men Legacy #209
Extended magneto Search
Tag "magneto"
Toys / Comics to Toys / Marvel Legends
June 20, 2021 - 19:53
Magneto is the first villain that the X-Men faced. He was introduced in X-Men #1 in 1963. The original leader of the Brotherhood of Evil Mutants, Magneto recruited his twin daughter and son Scarlet Witch and Quicksilver to help him in his fight against humanity.* He is the master of magnetism, a holocaust survivor and often, switches sides to help the heroes.
This action figure came with the Amazon exclusive Marvel Legends Series Exclusive 6-Inch Family Matters 3-Pack with Magneto, Quicksilver, and Scarlet Witch Action Figures in 2019. It is not the first Magneto action figure as many have been released earlier with Hasbro and Toybiz.
This is the classic Magneto look, not the modernized. The actual sculpt is based off the Jim lee version of Magneto that was released with the X-Men comic #1 from 1991 and not creator Jack Kirby. That means that the multiple threads and parts on his suit have been streamlined over time until just a few were left. For example, instead of having multiple bolts on the from cover of his shoulder armour, he now only has three. The metal gloves and sandals have been simplified too. The crest on his Roman helmet has also taken on a more figurative form, instead of the horn-like shape they had when Kirby designed him.
Jim Lee drew Magneto with a strong chest and huge bolts on his shoulder armour. He also favoured a long cranial structure for the helmet, reducing the face to a smaller area in proportion to the character's head. That's why Magneto appears to have such a small face and big head. The grinning alternative head is a straight representation of the classic X-Men #1 cover from 1991. The only thing missing from the Jim Lee design, are the lace-like cuts to his torso that strip from the top of his shoulder armour to his belt. Clearly, Magneto is meant to look like a Roman figure with his protected face. It is this look, which is so uncommon in superheroes and super villains, that given him his iconic and most recognizable look.
The sculpt is not great. Magneto's legs are too short compared with his thighs. He looks like one of those guys at the gym who only trains his upper torso but avoids the legs. The helmet does not cover his entire cheeks, and so it looks odd. The cape hinders his body shape. It adds weights and gravitas to his shoulders but creates a lack of proportions with the rest of his body. I dislike the cape. The belt is from the Jim Lee design, but it looks like he's wearing adult diapers instead of a belt.
Most of the figure is not shaded and follows the hue of the base plastic. His shoulders and neck, underneath the cape are a darker purple. The application of the purple hue on the straps of his forearms, and his sandals is uneven, with the base plastic easy to spot underneath. Thicker coats that follow the shape of the sculpt would have helped.
Magneto is a tall action figure over six inches. He towers over the Scarlet Witch and Quicksilver. He looks great next to other Marvel Legends action figures but not very good when brought next to Star Wars or G.I. Joe Classified. This is part of a situation that I dislike with Hasbro's Marvel Legends where figures tend to go towards the seven inches instead of anchoring their baseline at six. It makes every character look bigger and oddly out of scale with older Toybiz Marvel Legends, Start Wars, and G.I Joe Classified.
Balance is not easy to obtain with Magneto. His cape which should help hinders him. The added weight on the shoulder and back make the figure top heavy. The shorter legs, even with large feet make it easy to topple. The cape does not allow him to rest, like the Scarlet Witch's. he can be posed and not fall, but you will have to fiddle around a lot to achieve that. Perfect balance also means that he has a tendency to lean forward to compensate for his heavy cape.
The head is on a ball joint giving it a lot of mobility. Also, he has an abdominal crunch and a special peg hole in his back to stabilize the cape. The problem is that when stabilized the cape will still look crooked.
Magneto has shoulder, articulations but no butterfly hinges. These articulations are limited by the cape. Move them too much and the cape will unhook from its peg hole. He has bicep curls, double elbow articulations, and wrist curls. The wrists can also bend up and down.
He has a waist curl, thigh curls, double knee articulations that become loose easily. His hip joints allow the legs to move up, down and sideways but they are stiff and limited. The cape reduces how much they can move. There are also shin curls, and bendable ankles that also pivot sideways.
The plastic appears to be PVC. The cape and helmet have a rubbery feel. The helmet is glued on top of his head in both variants.
Magneto has two sets of hands. One with the open grasping palms, similar to the way Jim Lee drew him in X-Men #1 and a pair of fists. The alternate angry head, as mentioned is also based off the Jim Lee design. Finally, Magneto sports a pair of translucent soft plastic Kirby crackle discs he can use to simulate the use of his magnetic powers. These are the same ones that Hasbro has used for many characters such as Havoc and Polaris.
Magneto came in one huge box containing his kids and himself with a comic back cover. The back of the box featured artwork from the comics which is very nice. There is also a short bio on the characters.
The cost for this is odd. When it came out, the set was $59.99 USD. Amazon runs some sales on this set frequently. But at the same time, the set does increase exponentially a lot too. I bought this set at a steal for $55.99 CAD which is a steal and close to $45.99 USD. Since Amazon has been selling this set for an incredible $249 CAD which I wonder who would be willing to pay for these at this inflated price. Because this is an Amazon exclusive and that the retailer is an expert at variable pricing, your luck is as good as mine.
Because this set is an Amazon exclusive, you will not have many options when trying to buy it except for the secondary market. There is nothing below $100 USD on a popular auction site right now. My recommendation, if you are looking for a good Magneto action figure in the classic style is to wait for Hasbro to redo a new one in a few years. This set was released in 2019. Amazon still has a lot of stock but is not willing to sell them for cheap.
* Following a licensing conflict between Disney and 20th Century Fox, Marvel Comics cancelled Magneto's fatherhood over the twins. They were revealed as not being mutants anymore, for cheap corporate contrivances. Although Magneto being the father of the Scarlet Witch and Quicksilver had been a change made in 1979, it had always rang true for many comic readers. It is odd that Marvel/Disney would let Hasbro release a set called family matters if the characters were not related. Now that Disney owns Fox, perhaps Magneto's fatherhood will be officially reinstated and the twins will be mutants again. it doesn't matter to me. The twins are mutants and Magneto's kids, regardless of Disney lawyers' edicts!
Happy Father's Day!
Rating: 6.5 /10


Forged and Glass External Garden Balustrades.
Our clients have a lovely garden in Newcastle, with "The Devils Burn" running through it. At various points in the garden, bridges made from old railway sleepers provide access over the stream.
We were commissioned to design handrails and balustrades to protect these bridges. the brief was organic, natural and flowing, fitting the feel of the garden and water.
The organic nature of the garden is reflected in the handrail design. Forged steel features flare the bridge entrances, seemingly growing from the earth. We used low iron glass panels over the widths of the stream. Because their vertical curved edges blend into the natural surroundings it gives the effect of stretched canvas.
Profiled Iroko handrails cap the sections of glass cross the water, thus allowing an an opportunity to pause, reflect and enjoy the garden.
For more information on blacksmith forged steel balustrades please speak to our sales team.


Published: Feb 19 at 12:17 a.m.
Updated: Feb 19 at 12:29 a.m.
An SUV was flipped on its side Monday night following a two-vehicle collision in Mount Pearl.
The collision happened at about 11 p.m. at the intersection of Ruth Avenue and Commonwealth Avenue when a car apparently struck the SUV on its side. Firefighters had to cut away the front windshield of the SUV to free the two occupants who had no serious injuries.
The driver of the car was not injured in the incident which left both vehicles with extensive damage.


The Parasound is on Ebay now. And there are a lot of Adcom 555 mkiis for sale.
Ive seen a few Carver TFM-45 and the M4.0T. The6 cost more and would not leave me as much to spend on the caps for the rta12b.
I prefer a dark /warmer sounding amp. I dont get that from the parasound.
Does anyone have experiance with them?
I do 50/50 HT and music in 2.0.
I vote none of the above.
Well my budget for a new apm is $700. While you said non of then, do you have any recomdatio s for that price range?
Any are Polls frowned upon here for some reason?
Well, i leaning towards tb Adcom.
There are some nice amps for sale right here if you can expand your budget.
I own a TFM45. Unless the amp you're looking at has been recapped and completely gone through in the last couple of years you can add 500.00 to what ever price you're paying for it. This is fact and not just "well it should be done" . The icing on the cake is IF someone has been inside and did work it could be more. Many get inside and cause more trouble than its worth.
I like Parasound but I do not like the sound of the Classic line. To me it is to sterile and on the bright side. Never was an Adcom fan so I will leave it @ that. Dogg gave you the best advice on the TFM45.
The HCA series of Parasound are affordable and very good @ what they do. Although these are starting to get long in the tooth age wise, recapping won't break the bank when the time comes. In fact I have a HCA-1500 that still runs as new and is all original.
Or just save up your money and move up the chain. It will be much cheaper in the long run.
The Carver M4.0t is reputed as one of the best sounding amps within the lineup of standard Carver amps and I personally prefer the M4.0t to the TFM-45, even though the TFM-45 was emulated to sound like the famed Silver Seven tube amps. The M4.0t simply sounds better to these ears and presents a well balanced, pleasant to the ears sonic signature. Adcom amps are not what you would consider warm (read bright) and you already stated that you do not prefer the sound of the Parasound amp you have.
Out of the choices you presented? I would choose the Carver M4.0t.
With your price range, I would try to find a Musical Fidelity A3cr and call it a day.
Hard to beat for the money. Sound better than Adcom. No experience with the Parasound, maybe someday.
To continue down the "Carver" road, you'd really need to make sure it has been, or will be recapped given its age.
Personally I'd stick w Parasound over it, which is more of a personal preference as I've owned a fully modded M1.0t MKII, Carver AV-705x, as well as Parasound HCA-1000 and 1200ii.
Tom I'd like to know how they are different? It has always been my understanding they are the same inside. 4.0t was a anthracite gray in color and the TFM as well all know was Black. I might be mistaken but I was sure Roland had told me they were internally the same creature. Were they voiced differently?
If you want dark go B&K.
That's not dark, that's musical.
I can recap and fully calibrate a TFM45/42/M4.0t for about $250 + shipping. I use a bank of smaller capacitors for the main filter caps, as they are virtually extinct now, and any NOS specimens are almost half way through their usable life, before they are ever installed in an amp. The smaller bank of capacitors is superior in performance, with a much lower ESR, and the cost is significantly less.
I would personally go with an M500t, in the mkII configuration - especially if you like a warmer, more musical sound. The 500t is widely considered the most musical of the Carver solid state designs.
That is what Roland at Hi-Tech Audio Ltd. did was a bank of Panasonics IIRC. Also all electrolytic's were replaced and bypassed with good quality film caps. All was approved by the man himself Bob Carver. Once again IIRC Roland stated that with the bank of smaller caps he did the amp had more capacitance that the original HUGE caps. I believe both my TFM45/25 both had superior sound than when new from the factory not once have I regretted spending the money. Roland also did all the output transistors with new heat goop and made sure they were all up to spec and replaced those that were not.
This by no means is a slap at you. That sounds like a great deal.
Between my shipping to and from it was close to the amount I stated. So at about 10yrs ago I felt I wasn't far from reality to cost.
The only problem with the 500T is it is not common ground and cannot be used with SDA's if that is your cup of tea.
The top end rolls off. It would be a good match for the rta12 IMO. Better than the other two options.
Wow, thanks for all the responces. Skip, you hit it on the head. My main focus is the RTA12B. I just like them better than the srs. Plus my room size os a factor for the srs.
Im suprised at the acceptance of the Carver. Also from what i remember as pitdog said, i dont think there is any major diff betweeen the 4.0t and tfm45. Both are function calibrated off the Silver Seven. At least that is what i understood.
Someone stated the Parasound sounded sterile. I agree but did not know what word to descibe it. It just does not effect me like the sound of other amps ive heard. Some make the hair stand up on the back on my neck and some dont. When i first got my NAD 906 hooked up it sounded absolutley phenominal to me. I loved it.
I will keep an eye out on the TFM 45s and the M4.0t. Id rather have the 45. As childish as it soulds i love the VU meters. Lol. If i can find one that needs a repair for the right price i may just go for it and send it to The Carver Site guys for a full upgrade. I think the charge for the 45 is $365 or so.
I have like the sound of B&K in tha past so thats another option. Was also looking at sone Acurus amps.
Thanks again for the info guys.
Fyi my Parasound is on the bay right now. I think 2 days left. Hope it sells.
I honestly don't think you'll like the Carver on them and I know you won't like the Adcom on it. You want something warmer than those.
Might I suggest also looking for a Mitsubishi DA series amplifier if budget is a concern. NAD as you said might do well with the RTA12. I found my RTA12 to need warmth to smooth out the sound.
Both are function calibrated off the Silver Seven.
Biggest joke in audio. None of the Carver SS amps sound anywhere close to the Silver Seven tube amps.
I'd describe the top end as natural as opposed to many amps with a hyper detailed top end that far too many think sounds like real music does.
Here is a link to a NuForce amp that has gotten some pretty good reviews. They are closing it out and the price for new is great. I have no affiliation with this and have no experience with this amp.
My concearn witg the Nuforce is tge 80 watts per rating. While i know 80 watts can be loud but i dont thinknloud enough for me. I do like to play at or near the speakers limit. I like very loud sometimes. Thats the reason i dont use the 90 bridged NAD 906. Plus i cant use it on the sda.
Hi pitdogg2. The TFM 5 series were all emulated to sound like the Silver Seven tube amps (15, 25, 35, 45, 55, 75) and Jesse is 100% correct. They may have been made to emulate the tube amps but the differences between the actual Silver Sevens and the TFM 5 series are vast.
It has always been my understanding that the M4.0t and the TFM-42 with the weird strobe lights in the front were emulated to sound like another amp that escapes me at the moment.
The M1.0 was emulated to sound like Bob wanted and the M1.0t to emulate the sound of the Conrad Johnson Premier 5 after winning the famous Carver challenge against Stereophile magazine and their "Golden Ears" many moons ago in a hotel room over the course of three or 4 days.
FWIW, the M1.0t is the least favorite amp of mine (and many other share this observation) unless you are using it to power a sub or something. The linear frequency curve and sonic signature is.....um, shall we say, bright. Yes, we will call it bright.
With that said, my two favorite sonic signatures and overall sound characteristics within the mainstream Carver amps are the M-500t and the M4.0t. My favorite rare Carver amps are the Silver 7's and the Silver 9 tube amps that still get critical acclaim after all these years.
Yea i have had the pleasure of hearing the tubes back in the day. Their finesse has to be experienced and i agree vast differences in signatures. I was always under the impression that the tfm 22/42 were exactly the same as 25/45 but l.e.d. instead of vu meters. I always wanted a set of the silver 7 or 9 monoblocs those are beasts. With SDA's they would not be a go from my understanding.
Yea it would be nice to experience the world of carverfest i do not ever see it in my future however.


Happy Father's Day from Bud's!
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text:
The most popular languages to learn in Utah
Experts at Writing Tips analyzed the number of average monthly Google searches in each state for learning a language, including terms such as 'how to learn X', 'learn X', 'X classes near me'. The search volume for each term combined with the language were added together to discover the total average monthly searches in each state.
Here in Utah, we wanted to learn these languages the most:
1st Place – Spanish: The language is spoken by approximately 534 million speakers, as well as it being the official language of 21 countries. Almost 13% of the U.S population speak Spanish too – in fact, it is the second most spoken language in the country. Not to mention, it has the highest number of speakers in the family of romance languages.
2nd Place – Korean: Ranked as the 13th most commonly spoken language in the world, Korean has around 77 million speakers. With the Korean pop music gaining millions of U.S fans in recent years, including musicians like famous boy band BTS, it's no surprise that Americans are keen to learn the language.
3rd Place – Japanese: With approximately 128 million speakers, Japanese is the ninth most spoken language across the globe. As well as this, it is one of the most fast-paced languages – however, it has the lowest amount of information density per second.
On a national level, Spanish takes the crown for the most popular language to learn across the U.S with a staggering total of 476,900 average monthly searches, as well as taking the top spot in each and every state. In second place is Korean with 44,090 Google searches, followed closely by Japanese in the third spot with a total monthly search volume of 40,260.
A spokesperson from Writing Tips has commented on the findings: "Learning a new language has an abundance of benefits, from advancing your career to enhancing the connection to other countries and cultures – so it's fascinating to see such different languages make the top of the rankings. Plus, it can even improve communication and vocabulary in your first language. With the sheer amount of searches for learning Spanish across the nation, it will be interesting to see how this impacts the number of speakers in the U.S."
This research was conducted by writingtips.org who create guides to give you the correct approach to writing for nearly every aspect of life, from finding a job to general learning.
2nd Date Update – Return of the Ex
What's Poppin': Weekend of Jan 18th


text:
05 June 1915 – Churchill
Almost three weeks after Prime Minister Henry Asquith shook up his cabinet in the wake of negative press regarding the slow rate of arms and ammunition manufacture, Winston Churchill finds life dull without his former office. No longer the First Lord of the Admiralty thanks to the resignation of Baron John Fisher, the First Sea Lord who objected to his management of the Dardanelles Commission, Churchill is unsatisfied by the narrowly-defined role of Chancellor for the Duchy of Lancaster. Famously, this is the month in which he will take up oil painting to occupy his free time.
Today, he visits Dundee, a town he represents in Parliament, to give his constituents some idea of his feelings on the matter.
(F)or nearly four years, I have borne the heavy burden of being, according to the time-honoured language of my patent, "responsible to Crown and Parliament for all the business of the Admiralty," and when I say responsible, I have been responsible in the real sense, that I have had the blame for everything that has gone wrong. These years have comprised the most important period in our naval history: a period of preparation for war, a period of vigilance and mobilization, and a period of actual war under conditions of which no man has any experience. I have done my best, and the archives of the Admiralty will show in the utmost detail the part I have played in all the great transactions that have taken place. It is to them I look for my defense.
I look also to the general naval situation. The terrible dangers of the beginning of the war are over. The seas have been swept clear: the submarine menace has been fixed within definite limits; the personal ascendency of our men, the superior quality of our ships on the high seas, has been established beyond doubt or question.
Seen from a century's distance, Churchill's remarks seem naive, even delusory. The German U-boat threat has in fact been rising all year, and will only increase with time. Indeed, the chauvinism sounded in statements about "the personal ascendancy of our men" places him far behind the learning-curve of British troops in the Dardanelles — a matter to which he now turns.
I have two things to say to you about the Dardanelles. First, you must expect losses both by land and sea; but the Fleet you are employing there is your surplus Fleet, after all other needs have been provided for. Had it not been used in this great enterprise, it would have been lying idle in your southern ports. A large number of the old vessels of which it is composed have to be laid up, in any case, before the end of the year, because their crews are wanted for the enormous reinforcements of new ships which the industry of your workshops is hurrying into the water. Losses of ships, therefore, as long as the precious lives of the officers and men are saved, as in nearly every case they have been—losses of that kind, I say, may easily be exaggerated in the minds both of friend and foe.
And military operations will also be costly, but those who suppose that Lord Kitchener has embarked upon them without narrowly and carefully considering their requirements in relation to all other needs and in relation to the paramount need of our Army in France and Flanders such people are mistaken and, not only mistaken, they are presumptuous.
In fact, Lord Kitchener's old world, laissez-faire management is a primary reason why the embarrassment of the shell crisis has happened at all, while Kitchener's dithering about the strategic choice to invade the Dardanelles has played an outsize role in creating the disaster. Yet Churchill is undeterred by the continuing failures at Gallipoli, but rather praises the military leaders responsible for the continuing debacle by name — and insists that victory is close at hand:
My second point is this: in looking at your losses squarely and soberly, you must not forget, at the same time, the prize for which you are contending. The Army of Sir Ian Hamilton, the Fleet of Admiral de Robeck, are separated only by a few miles from a victory such as this war has not yet seen. When I speak of victory, I am not referring to those victories which crowd the daily placards of any newspapers. I am speaking of victory in the sense of a brilliant and formidable fact, shaping the destinies of nations and shortening the duration of the war. Beyond those few miles of ridge and scrub on which our soldiers, our French comrades, our gallant Australians, and our New Zealand fellow-subjects are now battling, lie the downfall of a hostile empire, the destruction of an enemy's fleet and army, the fall of a world-famous capital, and probably the accession of powerful Allies. The struggle will be heavy, the risks numerous, the losses cruel; but victory when it comes will make amends for all.
There never was a great subsidiary operation of war in which a more complete harmony of strategic, political, and economic advantages has combined, or which stood in truer relation to the main decision which is in the central theatre. Through the narrows of the Dardanelles and across the ridges of the Gallipoli Peninsula lie some of the shortest paths to a triumphant peace. That is all I say upon that subject this afternoon; but later on, perhaps, when the concluding chapters in this famous story have been written, I may be allowed to return again to the subject.
To be sure, Churchill is correct that the conquest of the Dardanelles would surely bring great material relief to Russia, knock the Turks out of the war, and break the Central Powers. But these are the hopes for breakthrough, not the facts on the ground. A realistic appraisal of the Gallipoli Campaign would take into account Churchill's repeated public statements beforehand in which he telegraphed his intentions to the Ottomans.
But this kind of introspection is too much to ask from Churchill, whose hubris has led him to reject any contrary or cautionary advice while promoting only that information and opinion which would bolster his case for attacking the Dardanelles. Rather than engage in self-examination, Churchill suggests that the real problem in Britain is that anyone would doubt his, or his government's, awesome powers of mentation — especially in the press.
I see some of our newspaper friends are reproaching themselves and reproaching others for having been too optimistic. Let them lay their consciences to rest. It is the general duty of the Press, for the most part faithfully discharged, to sustain the public confidence and spirit in time of war. All the great commanders of the past, the rulers of States in time of crises, have always laboured to discourage pessimism by every means in their power. Our Allies the French have a recent saying that pessimism in the civilian is the counterpart of cowardice in the soldier. That does not mean you must not face facts. You should face facts, but surely from the facts of our situation you will find the means of deriving much encouragement.
[…] It is the duty of all in times like these to give loyalty and confidence to their leaders, be they the soldiers in the active sphere or the statesmen who sit in anxious council here at home, to give them loyalty and confidence, not only when all goes smoothly, for that is easy, but to make them feel that they will not be blamed for necessary losses incurred in valiant enterprise or rounded on in reproach at the first check or twist of fortune. Then you will get from your leaders, be they military or civilian, you will get from them the courage, the energy, the audacity, and readiness to run all risks and shoulder the responsibilities without which no great result in war can ever be achieved.
[…] I do not think that the newspapers ought to be allowed to attack the responsible leaders of the nation, whether in the field or at home, or to write in a manner which is calculated to spread doubts and want of confidence in them or in particular operations, or to write anything which is calculated to make bad blood between them. I apply this not only to the Admirals and Generals, but to the principal Ministers at home, and especially the heads of the great fighting departments. No other nation now at war would allow the newspapers such a license in the present time, and if there is to be criticism, if there must be criticism, first, it should be only the loyal criticism of earnest intention. But if there is to be criticism, let it be in Parliament. If the speeches are such that we cannot allow the enemy to be a party to our discussions, then let Parliament, as is its right, sit for the time being with closed doors. But it seems imperative, in the interests of the country for the future, and for the safety and success of our arms, that irresponsible or malicious carping should not continue.
Churchill suggests that regardless of victory or defeat, the only measure of success for Britain's new coalition government is whether it takes "action."
That is the need, that is the only justification, that there should be a stronger national sentiment, a more powerful driving force, a greater measure of consent in the people, a greater element of leadership and design in the rulers—that is what all parties expect and require in return for the many sacrifices which all parties have after due consideration made from their particular interests and ideals. Action—action, not hesitation; action, not words; action, not agitation.
Churchill does offer one policy view, opposing conscription: "(I)f it were not possible to win this war without taking men by compulsion and sending them into the field, I should support such a measure; but I do not believe that it will be found necessary, and I am sure it is not necessary now." The crowd cheers his words, but they are unduly optimistic, for with the eventual defeat at Gallipoli and the endless meat-grinder of the Western Front, Britain will be forced to adopt military conscription at the beginning of next year. After all, the stakes are so very high:
(W)e are locked in mortal struggle. To fail is to be enslaved, or, at the very best, to be destroyed. Not to win decisively is to have all this misery over again after an uneasy truce, and to fight it over again, probably under less favourable circumstances and, perhaps, alone. Why, after what has happened, there could never be peace in Europe until the German military system has been so shattered and torn and trampled that it is unable to resist by any means the will and decision of the conquering Power. For this purpose our whole nation must be organized —must be socialized, if you like the word, must be organized and mobilized, and I think there must be asserted in some form or other—I do not attempt to prejudge that—but I think there must be asserted in some form or other by the Government, a reserve power to give the necessary control and organizing authority and to make sure that every one of every rank and condition, men and women as well, do, in their own way, their fair share. Democratic principles enjoin it, social justice requires it, national safety demands it, and I shall take back to London, with your authority, the message "Let the Government act according to its faith."
October will see Churchill run out of London over the renewed failures of the Gallipoli Campaign. No one within the government has forgotten about his shameful adventures in Antwerp last September, either, so the public image of an incompetent dilettante will dominate his dismissal. In 1915, the future image of Winston Churchill as a great wartime leader seems like a joke.
17 May 1915 - Coalition Government
In a surprise move today, Prime Minister Herbert Henry Asquith calls for the resignation of his entire cabinet. His timing is not an accident: King George V is aboard the royal train in northern England today, cut off from communication and unable…
14 May 1915 - Whistleblower
The Times creates an uproar today when Charles William Harmsworth, later Alfred Lord Northcliffe, publishes an article by Charles à Court Repington pinning the blame for continued shortfalls in munitions production on the War Office and Lord Kitchener. The burgeoning 'shell crisis' has existed since October, but…
04 October 1914 - Royal Naval Division
'First Lord of the Admiralty' was almost a vestigial office of the English aristocracy when Winston Churchill took the title three years ago. In that time, he has maximized the powers of the office, making decisions that will impact the shape of the…
Britain, Gallipoli Campaign, newspapers, shell crisis, Winston Churchill
12 - June Blast, 1915 - Old World In Ruins
04 June 1915 – The Big Push
06 June 1915 – Air Defense


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Twality Middle School News
Browse past news stories for Twality Middle School in Portland, OR.
Twality Middle School students already planning for 2016 trip to Belize - OregonLive.com
posted on March 21, 2015 at 01:01:58 pm
We're in the middle of spring break and while most of us are still wondering what we'll do with our time, some Twality Middle School students are already planning their 20 ...
Twality Middle School starts school year with new principal, Carol Kinch - OregonLive.com
posted on September 3, 2013 at 06:37:53 pm
TIGARD--The sixth graders who started at Twality Middle School this morning wouldn't know it, but it was Principal Carol Kinch's first day of the school year too. "Come back i ...
Twality Middle School starts school year with new principal, Carol Kinch
Carol Kinch is the new principal at Twality Middle School after spending two years as associate principal. first day of ...
Twality Middle School gets new principal, Byrom Elementary loses one - OregonLive.com
She started in Tigard-Tualatin School District as a learning specialist at Tualatin High School in 1999 and moved to the district office in 2003 as a special education teacher. ...
Twality Middle School students pay tribute to Newtown victims - OregonLive.com
posted on January 23, 2013 at 07:44:29 pm
Tamara Hufford-Wong,a communications consultant in Lake Oswego, pitched the idea to Twality Middle School Principal Rick Patrick after she watched news coverage of December ...
Twality Middle School staff lounge gets donated makeover - OregonLive.com
posted on November 18, 2009 at 01:10:34 am
TIGARD -- Until last week, Twality Middle School's staff lounge was about as pretty as the 1970s yellow-orange laminate on its cabinets. Then Cathy Cooper stepped in. ...
Twality Middle School gets new principal
posted on February 25, 2008 at 09:09:00 pm
Rick Patrick, principal of Byrom Elementary School in Tualatin, will take over in July as principal of Twality Middle School in ...
Indiana Schools Face State Takeover
Learn about the recent vote by the Indiana School Board to allow a state takeover of four Indiana schools beginning next school year.
A Relevant History of Public Education in the United States
10 Major Challenges Facing Public Schools


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Chelsea Manning's Loved Ones Are Crowdsourcing Funds To Help Her After She's Released From Prison
Manning went on hunger strikes, attempted suicide on at least two occasions, and underwent gender reassignment surgery during her incarceration
Penn Collins
Before leaving office in January, President Obama formally commuted most of Chelsea (neé Bradley) Manning's 35-year-sentence for leaking classified information and documents to Wikileaks. The commutation was a divisive one, with many believing that her actions were treasonous, pure and simple, while others believed that she was serving a public good by sharing information with the public.
Her stay in prison was no less contentious as Manning went on hunger strikes, attempted suicide on at least two occasions, and underwent gender reassignment surgery during her incarceration.
Now, on May 17th, she's slated to be released from prison to become a free woman. Her friends and family have launched a GoFundMe effort to ensure that she's able to provide for herself once she's freed.
The project's page explains how the crowdsourced money will help Manning.
"Funds raised will be used to pay for Chelsea's rent, utilities, health care, clothing and other living expenses for the first year after she is released."
The goal of the page is to raise a lofty $100,000, which might cause many to wonder if this is truly being done to fund a year of living expenses or to financially express gratitude for her actions.
The GoFundMe page's language suggests it's both, with the above statement somewhat incongruous with this earlier statement:
For the past seven years, Chelsea has been incarcerated. She survived solitary confinement, systemic denial of health care and years of being separated from her friends and community. Through it all she has remained a steadfast voice for liberty and justice and an inspiration to so many. We now have a chance to show our appreciation for all that she has given us.
Either way, in just two days, Welcome Home Chelsea has raised $48,500 towards its goal, so it's looking likely the target will be met.
Just one day in, Chelsea expressed her gratitude for the outpouring of financial support via Twitter:
Awww <3 Thank you all so very much for pitching in & helping me start my new life ^_^ https://t.co/LGSdkQDdvY #welcomehomefund
— Chelsea E. Manning (@Chelsea E. Manning) 1486510038.0