Whether you are a fashion blogger or a clothing brand, achieving the perfect high-quality fashion fyuse can be a challenge. We've consulted our Fyuse experts to bring you our best tips!
1. Portrait vs Landscape: Portrait fyuses will give you better composition and framing for fitting in half and full-body shots. It is also the best choice when showing off a particular piece of clothing or an entire outfit. Landscape fashion fyuses are ideal if you are doing group shots (with 3 or more subjects) with ample space to move about. We highly suggest wide-angle lens for any landscape fashion fyuses (to fit more in your framing).
2. Indoor vs Outdoor: Lighting will be a key factor in whether you should take a fyuse indoors or outdoors. If you have the proper studio lighting equipment, or ample amount of natural light, taking a Fyuse indoors won't be an issue.
If fyusing outdoors, shoot in the shade, during golden hour (an hour after sunrise and an hour before sunset) or on overcast days for optimal lighting conditions. Avoid shooting in direct sunlight, as direct sunlight will create harsh shadows or overexposed fyuses. We've found outdoor fyuses to be especially good for lifestyle concepts, or to incorporate architecture and landmarks.
3. Standing Still vs Moving: We highly recommend that your subject stays still during a fyuse recording. Your viewers/customers can see the outfit/clothes better since they can see it from multiple angles. Too much movement will create blurs and divert focus from the product. If you decide to incorporate movement, do so using a repeated moving action (such as tilting left and right repeatedly).
4. Spacing: It is very important to give yourself enough space to take a fyuse, whether it is indoors or outdoors. So clear the set or pick an area with lots of room to move about. You don't want to bump into a tree, a pole, or a table as you take a fyuse!
5. Background: For indoor shoots, choose a clean or solid wall/backdrop. For outdoor shoots, choose areas that has minimal background noise. Avoid crowded and busy areas.
Solid walls make for zero background noise—outfits pop even more!
7. Additional Gadgets: If you want to invest in additional equipment that can help with your fashion fyuses, we suggest a 360 rig, an electric board, or a selfie stick.
Stay tuned for the next Trick of the Trade!


Fate brings together an albino and a lawyer, the former who claims to have been unfairly dismissed as a result of discrimination and the latter, Jimi Disu, presented a second chance in life after an accident results in the loss of his family and a once illustrious legal career. It features Damilola Ogunsi, Funsho Adeolu, Ade Laoye, Carol King, Bimbo Manuel, Norbert Young, Omotola Jalade Ekeinde.
Adenike Adebayo reviews The Tribunal on a new episode of The Screening room.
Pulse reports that "Tribunal" is one of the three films commissioned by MultiChoice. The other movies are titled "Omugwo" and"Roti.
What do you think about The Tribunal? Share your thoughts with us in the comments section.


The SH-7 EverTune is the LTD Signature Series model of guitarist Brian "Head" Welch, the seven-string innovator and founding member of nu-metal icons Korn. The design of the SH-7ET was a result of Brian working closely with the ESP product development team, and has a body style with horns that are slightly thinned and streamlined for a sleek, menacing look.
The SH-7ET makes use of innovative Fishman Fluence Modern Humbucker pickups, with the Alnico version in the neck and the Ceramic version in the bridge position. The pickups provide an amazing range of great tones on their own, and the SH-7ET also provides a push-pull tone pot to access two different voicings of the pickups.
The SH-7ET is a neck-thru-body design with a flamed maple top in See Thru Purple finish over its comfortable, contoured basswood body. It employs a three-piece maple neck at 25.5" scale with an ebony fingerboard, and offers glow-in-the-dark side markers so that the fret position can easily be seen even on dark stages.
I was working with Nick Raskulinecz on our latest album. Me and Munky and him were doing guitars and talking... and what I was wanting was the EverTune.
There's all kinds of different possibilities that I had, but they told me that ESP were the forerunners with the EverTune. So I just called them up and I heard great things, they have a great reputation. I talked about everything and this is what we came up with.
Dude, and it just doesn't go out of tune, man. EverTune is amazing. I love it, it's changed my life.


do you have a commercial Property to clear?
At Phoenix we offer a professional commercial clearance, we have many years of experience in the commercial clearance market, we typically clear pubs, schools, offices, nursing homes and storage units to name just a few of the many commercial clearances we undertake.
what commercial clearances do we do?
During our 20 years of experience we have seen and come across just about every type of commercial clearance and domestic clearance you can think of, nothing surprises us, we have seen some of the most appalling sights known to man. Because of this experience you can be sure you can book us with confidence and receive a professional and prompt service.
how do we organise a commercial clearance?
When we start a commercial clearance we will deal with everything on the spot, every aspect of the commercial clearance will be taken into consideration, you will not have to organise or follow up on anything. We always like to make sure is clearance has sufficient man power on them as each commercial clearance is different and can take anywhere from 1 to 7 days to complete depending on the volume and access amongst other thing of the property.
If you would like to discuss a commercial clearance, or any other type of clearance then please phone us on 0800 234 3103 or 0784 537 7429.
can we clear large commercial properties?
As an example we recently cleared a commercial office which required a team of 8 staff from Phoenix, the new office needed to be opened within 2 days so our team had to work flat out over a very long weekend, the office clearance of 24 rooms was completed within 48 hours thereby allowing the business to continue without any loss of productivity or profit. This also allows the business owner to focus on other things essential to the business.
what do we do with confidential documents?
A Commercial clearance needs to be organized properly, on many occasions there is a lot more than you realize in the property! There are also confidential documents that may need to be shredded, we can plan all these different scenarios on site to ensure that the commercial clearance runs as smoothly as possible.
Please phone us on Freephone 0800 234 3103 or 0784 537 7429 to discuss your specific requirements.
Many properties whether a commercial clearance or domestic need clearing for many different reasons, you may have had a relative who has recently died or a company may have gone bankrupt overnight, the reasons are endless. Often not the most welcome of these tasks is having to clear the premises, most property owners find this impossible with their busy lives, that's where we step in!
do you have a surprise for us?
We expect certain items like wardrobes, washing machines, fridges etc to be in the property however it would be really good to know in advance if there is a piano in the lounge, a car in the garage or a motorbike in the attic (yes we have come across these scenarios). After you've told us of these great little treasures you won't have to do anything else, you don't have to pack or spend days sifting through everything. We'll do all the hard work, that's what you're paying us to do.
COMMERCIAL CLEARANCE SPECIAL OFFER! Get a 10% discount, FREE boxes, and a FREE basic property clean when you BOOK ONLINE NOW.


Thanksgiving isn't just something we do once a year – it is an annual reminder that we should be THANKSLIVING!
That is why for Thanksgiving this year, I created this simple game, based off the classic game of "MEMORY," will help kids to think of things they are thankful for – and then focus on them.
Printable Numbers to determine the order of play.
HAVE FUN this Thanksgiving helping your kids to be ThanksLIVING!


text:
David Jiroutek (ur. 2 marca 1973) – czechosłowacki i czeski skoczek narciarski oraz trener skoków narciarskich. Drużynowy mistrz świata juniorów z 1991. W latach 2000–2002, 2009–2014 i 2018–2020 główny trener reprezentacji Czech. W latach 2020–2022 trener reprezentacji Francji. Od 2022 trener reprezentacji Włoch.

Starszy brat Jakuba Jiroutka, również skoczka narciarskiego i trenera.

Kariera zawodnicza
7 marca 1991 reprezentując Czechosłowację zdobył złoty medal w drużynowym konkursie skoków narciarskich na mistrzostwach świata juniorów w Reit im Winkl. W drużynie obok Jiroutka wystąpili Milan Kučera, Tomáš Goder i Roman Lukeš.

23 marca 1991 na mamuciej skoczni w Planicy zadebiutował w zawodach Pucharu Świata, kończąc je na 43. miejscu. Tydzień później w Szczyrbskim Jeziorze zajął 30. miejsce. Wynik ten powtórzył 26 stycznia 1992 w Oberstdorfie. Nigdy nie zajął miejsca wśród najlepszych 15 zawodników, dającego punkty w klasyfikacji generalnej. Jego ostatni występ w Pucharze Świata miał miejsce 15 marca 1992 w Oslo, gdzie zajął 52. miejsce.

Startował w Pucharze Kontynentalnym, punkty do klasyfikacji generalnej cyklu zdobywając od sezonu 1991/1992 do sezonu 1994/1995. Najwyżej – na 33. miejscu – znalazł się w niej w debiutanckim sezonie. Wiosną 1996 zakończył karierę zawodniczą.

Kariera trenerska
W sezonie 2008/2009 pełnił funkcję trenera czeskiej kadry B. W maju 2009 roku został wybrany przez Czeski Związek Narciarski na głównego szkoleniowca reprezentacji Czech w skokach narciarskich. Zastąpił na tym stanowisku Richarda Schallerta.

W sezonie 2009/2010 Pucharu Świata, który dla Jiroutka był pierwszym na stanowisku głównego trenera kadry, w Pucharze Narodów reprezentacja Czech znalazła się na 9. miejscu z 981 punktami. Indywidualnie najwyżej w klasyfikacji generalnej znaleźli się Jakub Janda, który zdobył 256 punktów i sklasyfikowany został na 22. miejscu, a także Antonín Hájek (23. miejsce z 230 punktami). Punkty PŚ zdobyło łącznie 7 Czechów: poza wyżej wymienionymi również Lukáš Hlava, Borek Sedlák, Jan Matura, Martin Cikl i Roman Koudelka, którzy zajęli miejsca pomiędzy piątą a siódmą dziesiątką klasyfikacji generalnej.

Również w sezonie 2010/2011 Czechy znalazły się na 9. miejscu w Pucharze Narodów, tym razem z 1091 punktami. Punkty zdobyło 6 zawodników. Najwyżej, na 16. pozycji, sklasyfikowany został Roman Koudelka. Stanął on na podium indywidualnych zawodów w Harrachovie, co było najlepszym z wyników osiągniętych przez Czechów w sezonie. Poza nim w najlepszej trzydziestce klasyfikacji generalnej (na 27. miejscu) znalazł się Jan Matura. 34. był Jakub Janda, miejsca w piątej dziesiątce zajęli Sedlák i Hlava, a na 82. miejscu z 1 punktem sklasyfikowano Ondřeja Vaculíka.

W sezonie 2011/2012 Czesi zgromadzili 2178 punktów i znaleźli się na 7. miejscu w Pucharze Narodów. Roman Koudelka ukończył sezon na 10. miejscu klasyfikacji generalnej, w trzydziestce znaleźli się również Hlava i Janda (odpowiednio 14. i 25. pozycja). Punkty zdobyli również Matura (52. miejsce) i Cikl (70.). Na podium poszczególnych zawodów stanęli Koudelka, drugi w Willigen, oraz Hlava, trzeci na skoczni normalnej w Lahti.

W sezonie 2012/2013 Czesi ponownie znaleźli się na 7. miejscu klasyfikacji drużynowej Pucharu Świata, tym razem z 1770 punktami. Indywidualnie najlepszym zawodnikiem był Jan Matura. Zakończył sezon na 10. miejscu z 631 punktami. Czterokrotnie stawał na podium: dwukrotnie zwyciężył w Sapporo, a w Harrachovie był drugi i trzeci. Indywidualnie był też dwunasty i piąty na mistrzostwach świata w Val di Fiemme. Z wyjątkiem Matury w Pucharze Świata Czesi zajęli miejsca poza czołową trzydziestką. Dopiero 49. z 40 punktami był, dziesiąty rok wcześniej, Roman Koudelka. Punkty zdobyli też Lukáš Hlava, Antonín Hájek, Čestmír Kožíšek i Jakub Janda.

W 2014 roku na stanowisku trenera kadry Czech zastąpił go Richard Schallert. Jiroutek natomiast, wraz z Matjažem Zupanem, rozpoczął szkolenie reprezentantów Rosji. Schallert to także jego poprzednik na tym stanowisku. W kwietniu 2018 roku został ponownie wybrany przez Czeski Związek Narciarski na głównego szkoleniowca reprezentacji Czech w skokach narciarskich. Zastąpił na tym stanowisku Richarda Schallerta. W styczniu 2020 został zwolniony ze stanowiska.

W czerwcu 2020 roku został głównym trenerem reprezentacji Francji.

W czerwcu 2022 roku został wybrany przez Włoski Związek Sportów Zimowych na głównego szkoleniowca reprezentacji Włoch w skokach narciarskich, zastępując na tym stanowisku Andrea'e Morassiego.

Osiągnięcia indywidualne

Puchar Świata

Miejsca w klasyfikacji generalnej

Miejsca w poszczególnych konkursach Pucharu Świata

Puchar Kontynentalny
Źródło:

Uwagi

Przypisy

Linki zewnętrzne
 David Jiroutek w bazie FIS-u
 David Jiroutek w bazie Skoki.hostigasp.pl
 David Jiroutek w bazie Czeskiego Związku Narciarskiego

Urodzeni w 1973
Czescy skoczkowie narciarscy
Czescy trenerzy skoków narciarskich

redpajama_set_name: RedPajamaWikipedia


Surrender at 20: 1/3 PBE Update: New Skin splash arts, HS Quinn changes, & more!
Welcome to the very first PBE update of 2017! As we continue the 7.1 PBE cycle that started prior to the winter break, tonight's coverage includes new splash art for three upcoming skins, more team summoner icons, tweaks for Heartseeker Quinn, details on XP & Zz'Rot portal chnages, and more!
Splash arts for the upcoming Heartseeker Lucian, Heartseeker Quinn, and Warring Kingdoms Garen skins are now on the PBE.
As previewed before the break, Heartseeker Quinn has received more texture changes in today's update including color tweaks, removal of the design on her thigh left over from old stockings, and more.
Small Raptors - XP increased to 35 from 15.
Adaptive Defenses (Passive) duration lowered to 1.5 seconds from 1.5/2/2.5 seconds.
== KateyKhaos tweeted out a final look at HS Quinn & Valor changes.
== Got a full changelist for the Zz'Rot Portal changes we saw debut earlier in the 7.1 PBE cycle. At the time I had just documented the cooldown/duration change but turns out there was a lot more under the hood.
Active / Void Gate cooldown lowered to 120 seconds from 150 seconds.
Voidling Health per level lowered to 0 from 50.
Voidling Structure Damage per level increased to 20 (360 at 18) from 5 (90 at 18).
Voidlings no longer add to the creep score of enemies who kill them.
12/15 PBE Update: More Esports Icons, WK Vi , & LCU Updates!
12/16 PBE Update: Lunar Revel 2017 Login, Esports Emotes, and more!


James Turrell is a renowned American artist that in the last two decades created a series of fifteen "Autonomous Structures", each intended to challenge the viewer's experience of light.
See also Contemporary art by Beth Cavener HERE!
James Turrell has had over 160 solo exhibitions worldwide since 1967, including the three-venue museum exhibition presented concurrently at the Guggenheim Museum in New York, the Los Angeles County Museum of Art, and the Museum of Fine Arts, Houston in 2013. For over three decades, James Turrell has used light and indeterminate space—not objects or images—to extend and enhance perception. James Turrell's work can been seen in over 70 international collections. Since 1968, when Turrell received a grant from the National Endowment for the Arts, the artist has been receipts numerous awards.
Check more contemporary art HERE!


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Jobs: responsive View All Jobs
JPMorgan Chase Bank, N.A.: Front End Software Engineer at JPMorgan Chase Bank, N.A. (Plano, TX) (Plano, TX)
JPMorgan Chase Bank, N.A.: Digital - Senior User Experience Designer, Associate at JPMorgan Chase Bank, N.A. (New York, NY) (New York, NY)
JPMorgan Chase Bank, N.A.: Software Engineer - Backend Developer Java at JPMorgan Chase Bank, N.A. (Bengaluru, India) (Bengaluru, India)
JPMorgan Chase Bank, N.A.: Software Engineer - UI Lead at JPMorgan Chase Bank, N.A. (Jersey City, NJ) (Jersey City, NJ)
Skyword/TrackMaven: Full Stack Developer at Skyword/TrackMaven (Boston, MA) (allows remote) (Boston, MA)
Graphic Design - eLearning
Full Stack Developer / WooCommerce Wizard
JPMorgan Chase Bank, N.A.: User Experience Designer at JPMorgan Chase Bank, N.A. (Chicago, IL) (Chicago, IL)
Online Partner AB: Full stack developer at Online Partner AB (Hägersten, Sweden) (Hägersten, Sweden)
JPMorgan Chase Bank, N.A.: Software Engineering at JPMorgan Chase Bank, N.A. (Tampa, FL) (Tampa, FL)
Senior Frontend Developer (m/f/d)
Skoobe: Senior Frontend Developer (m/f/d) at Skoobe (München, Deutschland) (München, Deutschland)
Duolingo Inc: Senior Software Engineer, Web at Duolingo Inc (New York, NY) (New York, NY)
Blacksmith Agency: Front-End Wordpress Web Developer at Blacksmith Agency () (allows remote)
Synfioo GmbH: Frontend / Web Software Developer (m,f,d) at Synfioo GmbH (Potsdam, Germany) (Potsdam, Germany)
Shopify Senior Frontend Developer (m/f/x) - Berlin

redpajama_set_name: RedPajamaCommonCrawl


text:
Canada: Fierce storm prompts early Whistler season
Sat, 17 Nov 2007 01:03 UTC
A storm that dumped nearly 80 centimetres of snow on parts of British Columbia has prompted officials to open Whistler for skiing earlier than expected this season.
"We have a great leg up on the season," Doug MacFarlane, Whistler Blackcomb Mountain manager, said in a statement ahead of Saturday's official opening. "Natural snowfall and our snowmaking efforts have allowed for the early opening on Whistler Mountain that skiers and riders have been hoping for."
Australia: Hail storms hit parts of NSW
Sun, 18 Nov 2007 00:55 UTC
Severe rain and hail storms were battering parts of southern NSW on Sunday afternoon. Hail fell at Marulan, in the state's southern tablelands, a caller to Macquarie Radio said.
Climate change: Political outlook murky despite the science
terradaily.com
Science is making headway in predicting how the planet's climate will evolve, but it's anyone's guess what actions policymakers meeting in Bali will take -- or not -- to slow global warming.
With just over two weeks left before the crucial 11-day forum in Indonesia, decision-makers are under intensifying pressure to do something about greenhouse gases -- and do it quickly.
The starkest warning of all came on Saturday from UN's top scientists, gathered under the Nobel-winning Intergovernmental Panel on Climate Change (IPCC).
Feeding the global warming craze: Conference releases summary for action on climate change
Fri, 16 Nov 2007 22:00 UTC
Valencia, Spain: Delegates from more than 140 countries agreed Friday on an environmental "instant guide" for policy makers, stating more forcefully than ever that climate change had begun and that it threatened to alter the planet irreversibly.
Comment: While there is no question that there is global warming in the last few decades, there is much debate in the scientific community about the extent of a human factor. There are plenty of evidences indicating that this is part of a natural cycle that has many causes from geological to cosmic ones. The human factor has been blown up far out of proportion by the governments and media. One has to wonder why it should be that way.
Cyclone Guba: Papua New Guinea flood toll reaches 71
Steve Marshall
Heavy flooding caused by Cyclone Guba has reportedly killed more than 70 people in Papua New Guinea.
More than 70 people are reported to have been killed in Papua New Guinea because of heavy flooding caused by Cyclone Guba.
Seven consecutive days of heavy rain left a trail of destruction in Oro Province, north of Port Moresby.
Seven consecutive days of heavy rain left a trail of destruction in Oro Province.
New Update: Over 2,200 Die in Bangladesh Cyclone
Parveen Ahmed
ABC News/Associated Press
Death Toll Reaches 2,206 in Bangladesh Cyclone As Hundreds of Thousands of Survivors Await Aid
©AP Photo/ Pavel Rahman
Cyclone affected villagers carry corrugated iron sheeting to repair their damaged house in Potuakhali, 152 kilometers (95 miles) south of Bangladesh's capital Saturday, Nov.17, 2007. The official death toll from a savage cyclone in Bangladesh reached 1,723 on Saturday as military helicopters and ships joined rescue efforts in the wake of the deadliest storm to hit the country in a decade.
Chile struck by 6.0 magnitude quake
A 6.0 magnitude earthquake struck northern Chile on Saturday, the latest in a series of aftershocks to hit the mineral-rich Andean country since a powerful temblor on Wednesday.
©REUTERS/Ivan Alvarado
A family walks past a street blocked with debris in the town of Tocopilla, some 1559 km (968 miles) north of Santiago, November 16, 2007.
Bangladesh cyclone toll tops 1600
Anis Ahmed
Military ships and helicopters were trying on Saturday to reach thousands of survivors of a super cyclone that killed more than 1,600 people and pummeled impoverished Bangladesh with mighty winds and waves.
©REUTERS/Rafiqur Rahman
A mother in a veil takes her injured daughter to a hospital in Barisal district town, south west of the Bangladesh capital Dhaka, November 17, 2007.
Satellite instrument helps tackle mysteries of ozone-eating clouds
Polar stratospheric clouds have become the focus of many research projects in recent years due to the discovery of their role in ozone depletion, but essential aspects of these clouds remain a mystery. MIPAS, an instrument onboard ESA's Envisat, is allowing scientists to gain information about these clouds necessary for modelling ozone loss.
"The Michelson Interferometer for Passive Atmospheric Sounding (MIPAS) is unique in its possibilities to detect polar stratospheric clouds (PSCs) since it is the first instrument with the ability to observe these clouds continuously over the polar regions especially during the polar night," Michael Höpfner of Germany's Forschungszentrum Karlsruhe GmbH said.
Using data collected by MIPAS, a German-designed instrument that observes the atmosphere in middle infrared range, Höpfner and other scientists discovered a belt of nitric acid trihydrate (NAT) PSCs developing in the polar night over Antarctica in 2003 about one month after the first PSCs, which were composed of water crystals, were detected.
Whale Found Deep in Brazil Rain Forest
RIO DE JANEIRO, Brazil - An 18-foot minke whale ran aground on a sandbar in the Amazon jungle some 1,000 miles from the ocean, Brazilian media reported Friday. Globo television broadcast images of dozens of people gathered along the Tapajos River splashing water on the animal, whose back and dorsal fin were exposed to the hot Amazon sun. Sea creatures rarely venture so far into fresh water.


text:
\section{Introduction}
\label{sec:intro}

Non-equilibrium dynamics of strongly coupled system is one of the most challenging tasks in theoretical physics. It is not only interesting in cosmology and particle physics, but also interesting within condensed matter physics \cite{henkel,hohenberg,Polkovnikov:2010yn}. In recent years, the central question in understanding the strongly coupled theory was how the critical dynamics across a phase transition react to a time dependent coupling, i.e., a thermal or quantum quench.  We investigate the critical dynamics of a strongly coupled superconducting phase transition within the AdS/CFT correspondence from string theory \cite{Maldacena:1997re}, focusing on the formation and evolution of topological defects after a thermal quench. Spontaneous topological defect formation in such transition is a fundamental component of the celebrated Kibble-Zurek mechanism (KZM) \cite{Kibble:1976sj,Kibble:1980mv,Zurek:1985qw}.

The basic idea of KZM is that: As a continuous symmetry is spontaneously broken during a second order phase transition, the evolution of the system stops being adiabatic and enters the ``freeze-out'' region as a result of the critical slowing down nearby the critical point. Topological defects will form at the interfaces where different symmetry-breaking domains meet and satisfy the ``geodesic rule'' \cite{Bowick:1992rz}. KZM predicts a universal power law between the topological defects number and the quench rate. Such mechanism was first introduced by Kibble \cite{Kibble:1976sj,Kibble:1980mv} into Cosmology that as a result of relativistic causality, topological defects such as cosmic strings, monopoles, and etc., can form in the subsequent evolution of the Universe. It was later introduced by Zurek into condensed matter physics that the vortex lines may occur in a superfluid when the system is quenched, which is accessible in the laboratory \cite{Zurek:1985qw}.
 This scenario was supported by various numerical studies \cite{Laguna:1996pv,Yates:1998kx,Ibaceta:1998yy,Antunes:1998rz,Donaire:2004gp,Das:2011cx,Gillman:2017ycq}, and experiments carried out in a variety of systems \cite{Chuang:1991zz,Bowick:1992rz,Digal:1998ak,Baeuerle:1996zz,Ruutu:1995qz,Carmi:2000zz,Monaco:2002zz,Maniv:2003zz,Golubchik:2010zz,Ado1,Ado2}.

The theory of KZM was proposed in a spatially homogenous background in which the momentum is conserved. However, real materials, which are composed of electrons, atom lattices, impurities and so on, do not possess such kind of momentum conservations (or have conservation only modulo the reciprocal lattice vectors) due to the spatial inhomogeneities \cite{MT}. It will be quite important to investigate the KZM in the strongly coupled systems with momentum dissipation in the framework of holography.  From holography, there have been a number of models built to study momentum dissipation by implementing the effects of translational symmetry breaking. Several approaches among these are to include the lattice effects \cite{Hartnoll:2012rj},  or study the charge transport in the background of a spatially modulated bulk \cite{Horowitz:2012ky,Horowitz:2012gs,Horowitz:2013jaa,Donos:2012js}, or in the presence of impurities  directly \cite{Hartnoll:2008hs,Anantua:2012nj}. However, due to the involved technics in such models, another conceptually distinct approach to holographic momentum dissipation was suggested in \cite{Vegh:2013sk}. This approach does not make use of any conventional mechanism of translational symmetry breaking, but instead provides an effective bulk description of a theory without momentum conservation from massive gravity. Applications of gauge/gravity duality on non-equilibrium dynamics can be found in \cite{Liu:2018crr,Guo:2018mip,Gao:2019baf,Lan:2020kwn,Wittmer:2020mnm,Ewerz:2020wyp,Erdmenger:2020flu,Ecker:2021ukv}.
Previous holographic work on KZM were carried out in \cite{Sonner:2014tca,Chesler:2014gya,Zeng:2019yhi,Li:2019oyz,delCampo:2021rak,Xia:2020cjl,Li:2021dwp}, without any momentum dissipation in the background.

Holographic massive gravity exhibits momentum dissipation \cite{Davison:2013jba} by giving a mass to the graviton. This mass breaks the diffeomorphism invariance of the gravitation theory, via the holographic dictionary, it in turn violates the conservation of energy-momentum in the dual field theory. Many clues have shown that the effect of massive graviton in the bulk gravity can be considered as the effect from the lattice in the dual field theory on the boundary \cite{Blake:2013owa,Hu:2015dnl}. Recently, a nonlinear massive gravity theory has been proposed by de Rham et.al. (dRGT theory) \cite{deRham:2010ik,deRham:2010kj}, and later it is found to be ghost-free \cite{Hassan:2011hr,Hassan:2011tf}. Note that, the dRGT massive gravity is thought to be the only healthy theory in Poincar\'{e} invariant setups, and there have been numerous studies in dRGT massive gravity which we will not list all of them \cite{Blake:2013bqa,Cai:2014znn,Hu:2015xva,Xu:2015rfa,Hendi:2015hoa}.

Our goal in this paper is to explore the effect of the momentum dissipation (equivalently the effect of graviton mass) on the critical dynamics across a second-order phase transition after a linear quench of temperature from the holographic $(3+1)$-dimensional dRGT massive gravity. Quantized superconductor vortices will turn out due to KZM after quench. We will see that the momentum dissipation has little effect on the KZM scaling laws of the vortex number and ``freeze-out'' time to the quench rate. However, it is interesting to see that the coherence length $\hat\xi$ of the order parameter at the ``freeze-out'' time decreases with respect to the graviton mass $m$ from the quasi-normal modes (QNMs) analysis. Physically, it implies that the momentum dissipation will reduce the coherence length. Inspired from Pippard's formula for the coherence length and mean free path \cite{abp}, we propose an analytic expression between the coherence length $\hat\xi$ and the graviton mass $m$. This analytic relation is in good agreement with the results from QNMs analysis. Moreover, we also investigate the relations between the number of vortices $n$ and the graviton mass $m$ from both numerical simulations and analytic approach, and find that they fit very well as $m$ is not too large. The resulting vortex number will increase as graviton mass grows, which in turn indicates that momentum dissipation will enlarge the number of ovrtices.

 The outline of the paper is as follows. In Sec.\ref{KZM}, we briefly review the KZM, and build up the holographic model in the (3+1)-dimensional dRGT massive gravity in in Sec.\ref{sec:setup}; Sec.\ref{numres} contains the main analytical and numerical results of our paper to study the generations of vortices and the relations between graviton mass;  The conclusions are drawn in Sec.\ref{sec:conclusion}; In the Appendix \ref{app} we briefly introduce the dRGT massive gravity.

\section{A brief review of Kibble-Zurek mechanism}
\label{KZM}
KZM is a paradigmatic theory to describe spontaneous generation of topological defects  in non-equilibrium critical dynamics \cite{Kibble:1976sj,Kibble:1980mv,Zurek:1985qw}. In the vicinity of critical point of a second-order phase transition, critical opalescence and critical slowing-down implies that the coherence length $\xi$ and the relaxation time $\tau$ diverge as
\begin{alignat}{1}\label{eq:9}
 \xi(\epsilon)=\xi_0|\epsilon|^{-\nu}, \qquad  \tau(\epsilon)=\tau_0|\epsilon|^{-\nu z},
\end{alignat}
in which $\xi_0$ and $\tau_0$ are constant coefficients depending on the microscopic physics, while $\nu$ and $z$ are the static and dynamic critical exponents in equilibrium states, and $\epsilon$ is the dimensionless distance to the critical temperature, $\epsilon\equiv1-T/T_c$. KZM assumes a linear quench across the critical point as $\epsilon(t)=t/\tau_Q$, in which $\tau_Q$ is the quench rate (or quench time). The ``freeze-out" time occurs at the instant $\hat t$ when the relaxation time of the system $\tau$ equals the time scale of the quench to the critical point, then the dynamics approximately freezes (from nearly adiabatic to approximately impulse behavior within the time interval [$-\hat t$, $\hat t$]).  Therefore, the ``freeze-out'' time can be readily obtained as
\begin{eqnarray}\label{eq:tfreeze}
\hat t=(\tau_0\tau_Q^{\nu z})^{\frac{1}{1+\nu z}}.
\end{eqnarray}
The key insight of the KZM is that the average size $\hat\xi$ of the domains in the broken symmetry phase is set by the the equilibrium coherence length $\xi$ evaluated at the freeze-out time $\hat t$, i.e., $\hat\xi=\xi(\hat t)$. Thus, the size of the symmetry-breaking domain is given by,
\begin{eqnarray}
  \hat\xi=\xi_0\left(\frac{\tau_Q}{\tau_0}\right)^{{\nu}/{(1+\nu z)}}
\end{eqnarray}
Topological defects will occur at the interfaces between various symmetry-breaking domains if they satisfy the ``geodesic rules'' \cite{Bowick:1992rz}.  Therefore, the above estimate of the $\hat\xi$ can be recast as an estimate for the resulting number of topological defects,
\begin{alignat}{1}\label{density}
n\approx \frac{Ap}{\hat\xi^{d}}=\frac{Ap}{\xi_0^{d}}\left(\frac{\tau_0}{\tau_Q}\right)^{\frac{d\nu}{1+\nu z}}.
\end{alignat}
where $A$ is the volume size of the system, $p$ is the average probability for the domains to form defects and $d$ is the spatial dimension of the system. This relation is verified to be universal in various dimensions and for different kinds of topological defects \cite{Laguna:1996pv,Yates:1998kx,Ibaceta:1998yy,Antunes:1998rz,Donaire:2004gp,Das:2011cx,Gillman:2017ycq,Chuang:1991zz,Bowick:1992rz,Digal:1998ak,Baeuerle:1996zz,Ruutu:1995qz,Carmi:2000zz,Monaco:2002zz,Maniv:2003zz,Golubchik:2010zz}.  In particular, the generated topological defects are vortices for superfluids or superconductors in $d=2$ system. We will investigate the KZM for vortices in a strongly coupled superconductor system with background momentum dissipation by virtue of the AdS/CFT technique in the following.

\section{Holographic setup}
\label{sec:setup}
The gravity background we adopt is the dRGT massive gravity in $(3+1)$-dimensional bulk spacetime \cite{deRham:2010ik,deRham:2010kj} (Please consult Appendix \ref{app} for a brief review of dRGT massive gravity). In order to study the dynamics in this background, we work under the Vaidya-AdS solution with flat space $k=0$ and zero charge $q=0$ (We have scaled the AdS radius $L\equiv1$.).
\begin{equation}\label{eq:1}
ds^{2}=\frac{1}{z^{2}}\left[-f(z)dt^2-2dt dz+\left(dx^{2}+dy^{2}\right)\right],
\end{equation}
where
\begin{equation}
f(z)=1-M z^3+\frac{c_1m^2}{2}z+c_2m^2z^2,
\end{equation}
in which $M$ is the mass parameter of the black hole, $c_i~(i=1,2)$ are constants and $m$ stands for the graviton mass.
Location of the AdS boundary is $z=0$ while the horizon is $z=z_+$. Hawking temperature of the black brane thus is
\begin{eqnarray}
T=\frac{1}{4\pi}\left(\frac{3}{z_+}+{c_1m^2}+{c_2m^2}z_+\right).
\end{eqnarray}
We work in the probe limit and adopt the conventional Maxwell-complex scalar action for holographic superconductors \cite{hartnoll}
\begin{eqnarray}\label{eq:3}
  S_{\rm matter} =\int d^4 x\sqrt{-g} \left[-\frac{1}{4}F_{\mu\nu}F^{\mu\nu}-|D_\mu\Psi|^2-m_\psi^2|\Psi|^2\right]
\end{eqnarray}
in which $F_{\mu\nu}=\partial_{\mu}A_\nu-\partial_{\nu}A_\mu$ is the Maxwell field strength, $A_\mu$ is the $U(1)$ gauge field, $D_\mu=\nabla_\mu-iA_\mu$ is the covariant derivative and $m_\psi$ is the mass of the complex scalar field $\Psi$. Thus, the equations of motion can be obtained
\begin{eqnarray}
\label{EoM1}
0&=&(\nabla_\mu-iA_\mu)(\nabla^\mu-iA^\mu)\Psi-m_\Psi^2\Psi,\\
\nabla_\nu F^{\nu\mu}&=&i(\Psi^\ast(\nabla^\mu-iA^\mu)\Psi-\Psi(\nabla^\mu+iA^\mu)\Psi^\ast).\label{EoM2}
\end{eqnarray}
It is convenient to work in axial gauge by setting $A_{z}=0$, and take the ansatz for other fields as $\Psi=\Psi(t,z,x,y),A_{t,x,y}=A_{t,x,y}(t,z,x,y)$.

\subsection{Holographic renormalization and boundary conditions}
In order to solve the above equations, we need to impose suitable boundary conditions at the horizon $(z=z_+)$ and at the AdS boundary $(z=0)$.
Near the boundary $z\to0$, fields can be expanded as,
\begin{eqnarray}
  \Psi = \Psi_{0}z^{\Delta_{-}} + \Psi_{1}z^{\Delta_{+}} +\mathcal{O}(z^{\Delta_{+}+1}) ,~~~
  A_{\mu}= a_\mu +b_\mu z+\mathcal{O}(z^2) ,
\end{eqnarray}
with $\Delta_{\pm}={\left(3\pm\sqrt{9+4m_\psi^2}\right)}/{2}$ are the conformal dimensions of dual scalar operators on boundary. Following the AdS/CFT dictionary, the interpretation of $\Psi_{0}$ is that it sources the symmetry breaking operator $\hat{O}$, while $a_t$ and $a_i$ are the chemical potential and superfluid velocity in the boundary, respectively. The physical meaning of $\Psi_1$ and $b_\mu$ will be clear after the holographic renormalization.

From holographic renormalization \cite{Skenderis:2002wp}, varying the renormalized on-shell action with respect to the source terms one can achieve the corresponding conjugate variables.
In order to obtain finite on-shell action, we should add the counter terms of the scalar fields $S_{\rm ct}=\int d^3x\sqrt{-\gamma}\Psi^*\Psi$ into the divergent on-shell action, where $\gamma$ is determinant of the reduced metric on the boundary. We set Neumann boundary conditions for gauge fields in order to get the dynamical gauge fields in the boundary. In order to have a well-defined variation, the surface term $S_{\rm sf}=\int d^3x\sqrt{-\gamma}n^\mu F_{\mu\nu}A^\nu$  should also be added, where $n^\mu$ is the normal vector perpendicular to the boundary. Hence, we can get the finite renormalized on-shell action $S_{\rm ren}$. The expectation value of the order parameter can be obtained from the holographic renormalization by varying $S_{\rm ren}$ with respect to $\Psi_0$, resulting in $\langle\hat{O}\rangle=\Psi_1$.

We impose $\Psi_0=0$ all time in order to have a spontaneous symmetry breaking of the order parameter. This translates into a homogenous Dirichlet boundary condition for the field $\Psi$ in the AdS boundary, i.e., $\Psi|_{z=0}=0$. Expanding the $z$-component of the Maxwell equations near boundary, we reach $\partial_tb_t+\partial_iJ^i=0$, which is exactly a conservation equation of the charge density $\rho$ and current $J^i$ on the boundary, since from the variation of $S_{\rm ren}$ one can get $b_t=-\rho$ and $J^i=-b_i-(\partial_ia_t-\partial_ta_i)$. At the horizon, we demand the regularity of the fields. Since the metric component $g_{tt}$ is zero at the horizon, the component $A_t$ should be vanishing, while other fields are finite at the horizon.

\subsection{Numerical schemes}
We choose $m_\psi^2=-2$ without loss of generality and set $c_1=1, c_2=-1/2$ in order to make the background thermodynamically stable \cite{Hu:2015dnl,Cai:2014znn}. For convenience of the numerical calculation, we set the black hole mass parameter as $M=1$ and the location of horizon at $z_+=1$. From holographic superconductor \cite{hartnoll}, increasing the chemical potential or the charge density equals decreasing the temperature of the system. We choose to increase the charge density $\rho$ in our paper. In addition, the temperature of the black hole $T$ has the mass dimension one while the charge density $\rho$ has mass dimension two from the dimensional analysis. Therefore, in order to linearize the temperature near the critical point according to KZM, we quench the charge density $\rho$ as $\rho(t)=\rho_c(1-t/\tau_Q)^{-2}$, where $\rho_c$ is the critical charge density for the static and homogeneous holographic superconducting system. We should note that different graviton masses $m$ correspond to different $\rho_c$, which is shown in Fig.\ref{rhom}
\begin{figure}[h]
\centering
\includegraphics[trim=3.5cm 9.5cm 3.5cm 9.5cm, clip=true, scale=0.6,  angle=0] {rhom.pdf}
\caption{Critical charge density versus graviton mass. Red dots are numerical results while the blue line is a fitted critical curve. Upper the critical curve the system is in a superconducting phase while below the curve it is in a normal metal phase (shaded region). }\label{rhom}
\end{figure}

We quench the system from normal state with initial temperature $T_i=1.4T_c$ to superconducting state with the final equilibrium temperature $T_f=0.8T_c$. The size of the boundary system is $(x,y)=(50,50)$. We take advantage of the Chebyshev pseudo-spectral method in the radial direction $z$ and use the Fourier decomposition in the $(x, y)$-directions since the periodic boundary condition is imposed along $(x, y)$-directions. The grids in $z$-direction is 21 while the grids along $(x, y)$-directions are $201\times201$.  We thermalize the system by adding random seeds for the fields at the initial time.  The random seeds are sampled in the bulk by satisfying the white noise distributions $\langle s(t, \vec x)\rangle=0$ and $\langle s(t, \vec x)s(t',\vec x')\rangle=\zeta\delta(t-t')\delta(\vec x-\vec x')$, with the amplitude $\zeta\approx10^{-3}$. The system evolves by using the 4th order Runge-Kutta method with time step $\Delta t=0.01$. Filtering of the high momentum modes are implemented following the ``2/3's rule'' that the uppermost one third Fourier modes are removed \cite{Chesler:2013lia}.

\section{Results}
\label{numres}
\subsection{KZM scalings of vortex number and ``freeze-out" time}
\label{sec:density}
\begin{figure}[h]
\centering
\includegraphics[trim=3.2cm 9.2cm 4.3cm 10cm, clip=true, scale=0.55,  angle=0] {ntq.pdf}~
\includegraphics[trim=3.2cm 9.2cm 4.3cm 10cm, clip=true, scale=0.55,  angle=0] {tftq.pdf
\caption{\label{NT}
 (Left panel) Double logarithmic relation between vortex number $n$ and quench time $\tau_Q$ for graviton mass $m=(0, 1.2,2)$. The circles, triangles and squares are the numerical data while the straight lines are the best fitted lines in the slow quench regime (larger $\tau_Q$). The shaded regions represent the standard deviations away from the mean values.  For the slow quench, the scaling relations satisfy the KZM scaling laws very well; However, for fast quench (smaller $\tau_Q$), vortex number $n$ is almost constant beyond the scope of KZM. (Right panel) Double logarithmic relation between the lag time $t_L$ and quench rate $\tau_Q$. For slow quench the relation between $t_L$ and $\tau_Q$ satisfy the KZM scalings very well, while for fast quench $t_L$ keeps almost constant. This figure was obtained by running $100$ times of simulations for each $\tau_Q$ and $m$. }
\end{figure}

In this subsection, we will examine the KZM scaling laws in Eqs.\eqref{eq:tfreeze} and \eqref{density}, depending on the graviton mass. We count the vortex number $n$ as the order parameter $\langle\hat O\rangle$ saturates to its equilibrium value. Scalings between the number $n$ and quench time $\tau_Q$ under different graviton mass $m$ are exhibited in the left panel of Fig.\ref{NT}. The shaded regions correspond to the standard deviations from the mean values.  In the fast quench regime (small $\tau_Q$) the vortex number approximately saturates due to the finite size effect, which is consistent with previous results in condensed matter or holography \cite{Chesler:2014gya,Sonner:2014tca,Zeng:2019yhi,Li:2019oyz}.  However, in the slow quench regime (large $\tau_Q$), the vortex number will decrease with respect to quench time satisfying the scaling relations as $n_{m=0}\approx 305\times\tau_{Q}^{-0.504}$, $n_{m=1.2}\approx 390\times\tau_{Q}^{-0.5059}$ and $n_{m=2}\approx 805\times\tau_{Q}^{-0.518}$ respectively. From this figure, we can conclude that as $m$ grows, or equivalently momentum dissipation gets stronger, the number of vortices will increase as well. In other words, from the relation $n\propto 1/\hat \xi^2$ we can deduce that the momentum dissipation will reduce the coherence length. We will study this relation between coherence length and the graviton mass in the next subsection in details.

The ``freeze-out'' time $\hat t$ can be reflected by studying the lag time $t_L$ that defined as order parameter begins to grow rapidly \cite{Das:2011cx,Sonner:2014tca,Zeng:2019yhi}. In numerics we operationally set $t_L$ as $\langle \hat O\rangle\sim0.1$ following \cite{Sonner:2014tca,Zeng:2019yhi,Das:2011cx}.
On the right panel of Fig.\ref{NT} we exhibit the relation between $t_L$ and $\tau_Q$. The error bars are not shown since they are very tiny. We see that for fast quench the lag time is almost constant for different $m$'s. However, for slow quench, one can read that $t_{L}\approx6.45\times\tau_{Q}^{0.5102}$ for $m=0$, $t_{L}\approx4.347\times\tau_{Q}^{0.5014}$ for $m=1.2$ and $t_{L}\approx3.98\times\tau_{Q}^{0.4931}$ for $m=2$.
 Therefore, from the two KZM scaling relations in Eqs.\eqref{eq:tfreeze} and \eqref{density}, one can readily evaluate the dynamic critical exponent $z$ and the static critical exponent $\nu$ on the boundary as $(\nu\approx 0.514496, z \approx 2.0246), (\nu \approx 0.50732, z \approx 1.98221)$ and $(\nu \approx 0.510949, z \approx 1.90386)$ for $m=(0, 1.2, 2)$ respectively, in which the exponent matches the mean-field theory values with $z=2$ and $\nu=1/2$. This means graviton mass in dRGT massive gravity does not alter the KZM scaling laws,  which in turn indicates that the existence of graviton mass does not affect critical exponents, $z$ and $\nu$, in the boundary field theory. The boundary field theory remains as a mean-field theory, which is consistent with the assumption of AdS/CFT correspondence that the boundary is a mean-field theory in large $N$ limit \cite{Zaanen:2015oix}.

\subsection{Coherence length and graviton mass}

\subsubsection{Quasi-normal modes analysis}
From previous section \ref{KZM}, we see that the average size of the symmetry-breaking domains $\hat \xi$ is approximately the coherence length of the order parameter at the ``freeze-out'' time $\hat t$ \cite{Zurek:1985qw}.
Fortunately, from holography one can compute the coherence length from QNMs of the scalar field in the bulk by choosing suitable boundary conditions \cite{Kovtun:2005ev,Maeda:2009wv}. The QNMs correspond to the poles of the retarded Green's function of the dual field theory. One can read off the coherence length $\xi$ from the correlation function
\begin{eqnarray}\label{cof}
\langle O(\omega,k)O^\dag(-\omega,-k)\rangle\sim\frac{1}{i\tilde{c}\omega+k^2+1/\xi^2}.
\end{eqnarray}
where $k$ and $\omega$ are the momentum and frequency of perturbation modes respectively, while $\tilde{c}$ is a parameter.  QNMs are computed from small fluctuations of the background fields, such that
$\Psi(t,z,x)=\psi_0(z)+\psi(z)e^{-i\omega t+ikx}$, where $\psi_0(z)$ is the static background of scalar field while $\psi(z)e^{-i\omega t+ikx}$ is small fluctuations with respect to the background. For simplicity, we have assumed the fluctuations as plane waves in the only $x$-direction. We calculate the QNMs in the symmetric phase, i.e., in the normal phase that the background $\psi_0(z)$ is vanishing. This is because from KZM, dynamics ceases to be adiabatic and enters an impulse stage within the time interval [$-\hat t$, $\hat t$] as we learned from previous section \ref{KZM}. The starting of the symmetry breaking will occur at the instant $t\approx-\hat t$, which is in the normal phase before the critical point. This greatly simplifies the complexity of the calculations.

It is convenient to work out the QNMs in the Schwarzschild-AdS metric of the spacetime \cite{Sonner:2014tca,Zeng:2019yhi}.  Substituting the scalar field $\Psi(t,z,x)$ into the EoMs \eqref{EoM1},\eqref{EoM2}, and extracting the first order of the perturbations $\psi(z)$, we arrive at the decoupled linear equation as
\begin{eqnarray}\label{eq:QNM}
\psi''+\frac{f'}{f}\psi'+\left(\frac{(A_t+\omega)^2}{f^2}+\frac{zf'-k^2z^2+2}{z^2f}-\frac{2}{z^2}\right)\psi=0
\end{eqnarray}
 in which $A_t$ is the background gauge field. We impose the ingoing boundary conditions at the horizon $z_+=1$,
\begin{eqnarray}
\psi_{z_+}=(z-1)^{-\frac{iw}{4\pi T}}(1+\mathcal{O}(z-1)),
\end{eqnarray}
where $T$ is the Hawking temperature of black hole. Vanishing boundary conditions are imposed at the boundary $z=0$. We adopt the determinant method \cite{Zeng:2019yhi} to calculate the QNMs and fix the quench rate as $\tau_Q=20$ (other quench rates will have similar results). More specifically, we employ the Chebyshev differential matrix to convert the differentiation with respect to spacetime coordinate into a matrix. Zeros of the determinant of the resulting matrix are the QNMs after imposing the above boundary conditions. The lowest mode in the QNMs makes the most contribution to the perturbations. In practice, the lowest mode is the mode that is closest to the real axis. We can evaluate the coherence length from Eq.\eqref{cof} by setting $\omega=0$, and arrive at $\hat\xi=1/|{\rm Im}(k^*)|$ where $k^*$ is the lowest mode in those QNMs.  After solving the Eq.\eqref{eq:QNM} one can get a series of QNMs in the complex $k$-plane, as is shown in the left panel of Fig.\ref{kk} for $m=2$. The red dots, symmetric and closest to the real axis, stand for the lowest poles $k^*$. Other sub-leading poles  (in blue squares), all locate in the imaginary axis, are also symmetric to the real axis.   Different graviton masses correspond to different series of QNMs, leading to a relation between coherence lengths and $m$, i.e., $\hat\xi=\hat\xi(m)$, which are shown as red dots in the right panel of Fig.\ref{kk}.
\begin{figure}[h]
\centering
\includegraphics[trim=3cm 9cm 4cm 9cm, clip=true, scale=0.55,  angle=0] {QNMskm2.pdf
\includegraphics[trim=3cm 9cm 3cm 9cm, clip=true, scale=0.55,  angle=0] {cm.pdf}
\caption{\label{kk}{(Left panel)} QNMs in the complex $k$-plane for $m=2$ and $\omega=0$.  The leading poles nearest the real axis, marked by red dots, determine the behavior of correlations at large distances. The blue squares are the sub-leading poles which are not important to the correlations. {(Right panel)} Coherence length $\hat\xi$ of the order parameter at the ``freeze-out'' time versus the graviton mass $m$. The red dots represent $\hat\xi=1/|{\rm Im}(k^*)|$, where $k^*$ are the leading QNMs,  and the blue line is the fitting line $\hat\xi\approx0.7466/(1+0.1496m^2)$ from Eq.\eqref{eq:xim}. For both panels, we fix the quench rate as $\tau_Q=20$. }
\end{figure}

\subsubsection{Analytic relation between $\hat\xi$ and $m$}

The analytic relation between the coherence length $\hat\xi$ and the graviton mass $m$ was seldom discussed. In \cite{Hu:2015dnl}, the authors found that the coherence length would decrease with respect to the graviton mass in the system of a holographic Josephson junction. However, they did not propose an analytic relation between $\hat\xi$ and $m$. In this subsection, we will seek this analytic relation between $\hat\xi$ and $m$ and show that this relation matches well with the numerical results from QNMs analysis.

From the discussions in \cite{Vegh:2013sk,Davison:2013jba,Blake:2013owa}, the graviton mass $m$ effectively plays a role of momentum dissipation in the boundary field theory. This momentum dissipation might be from scatterings of electrons to lattices or impurities, which lead to the assumption in Drude model that the relation between the mean free path $l$ and scattering time $\tau_s$ is $\tau_s=l/V_F$, in which $V_F$ is the Fermi velocity \cite{MT}.
In condensed matter physics, the coherence length $\xi$ can be related to the mean free path $l$ from Pippard's formula \cite{abp,MT},
\begin{eqnarray}\label{ppp}
\frac{1}{\xi}=\frac{1}{\xi_p}+\frac{1}{\alpha l},
\end{eqnarray}
where $\xi_p$ is the coherence length of a pure material without any scatterings, and $\alpha$ is a numerical constant.  Then from the relation $\tau_s=l/V_F$ in Drude model, we get
\begin{eqnarray}
\xi=\frac{\xi_p}{1+\frac{\xi_p}{\alpha V_F}\,\tau_s^{-1}}
\end{eqnarray}
Fortunately, from holography \cite{Blake:2013bqa} $\tau_s$ can be related to the graviton mass $m$ as $\tau_s^{-1}=\gamma m^2$ where $\gamma$ is a coefficient independent of $m$. \footnote{From the study of holographic DC conductivity in \cite{Blake:2013bqa}, the authors identified the relation between scattering time $\tau_s$ and position dependent masses $\tilde m(z)$ of perturbations along $t$-$x$ and $z$-$x$ direction at horizon as $\tau_s^{-1}=\frac{\mathcal{S}}{4\pi(\mathcal{E+P})}\tilde m^2(z_+)$. Here, $\mathcal{S}$, $\mathcal{E}$ and $\mathcal{P}$ are the entropy density, energy density and pressure of the black hole respectively. The position dependent mass at horizon is indeed proportional to the graviton mass, i.e., $\tilde m^2(z_+)\propto m^2$. We absorb all of these coefficients into $\gamma$ as $\tau_s^{-1}=\gamma m^2$ where $\gamma$ is a function independent of $m$. } Therefor, we finally reach
\begin{eqnarray}\label{eq:xim}
\xi=\frac{a}{1+b m^2}.
\end{eqnarray}
where $a=\xi_p$ and $b={\xi_p \gamma}/(\alpha V_F)$.  The fitting of this relation \eqref{eq:xim} is exhibited as blue line in the right panel of Fig.\ref{kk}, with fitting parameters as $a\approx0.7466$ and $b\approx0.1496$. From Fig.\ref{kk} we see that the numerical results (red dots) from QNMs analysis are fitted very well with the analytic relation Eq.\eqref{eq:xim}. Therefore, the coherence length $\hat\xi$ at the ``freeze-out'' time will decrease as $m$ increases. This also means stronger momentum dissipation in the boundary field will reduce the average size of the symmetry-breaking domains, which in turn implies that the vortex number $n$ would grow with respect to graviton mass according to $n\varpropto 1/\hat\xi^2$ in Eq.\eqref{density}.

\subsection{Vortex number and graviton mass}

\begin{figure}[h]
\centering
\includegraphics[trim=3.2cm 9.5cm 4.2cm 9.8cm, clip=true, scale=0.6,  angle=0] {nm.pdf
\caption{\label{nm}Vortex number $n$ versus the graviton mass $m$.  Blue solid dots and error bars are from numerical data while blue line is the best fit as $n\approx17.82\times\left(1+0.1585m^2\right)^2$. Error bars denote the standard deviations. From the relation $n\approx Ap\hat\xi^{-2}$ in Eq.\eqref{density}, the numerical data from QNMs analysis in the right panel of Fig.\ref{kk} can be recast into the red dashed line to link the relations between $n$ and $m$. The blue solid line matches very well with the red dashed line as $m\lesssim1.5$. The quench rate in this figure is the same as in Fig.\ref{kk}, i.e., $\tau_Q=20$.}
\end{figure}
We count the vortex number at the final equilibrium state of the system, where the order parameter is well developed. From the above analysis, we expect that the vortex number $n$ would increase with the graviton mass,  and satisfying the following relation via Eq.\eqref{density} and Eq.\eqref{eq:xim}:
\begin{eqnarray}\label{eq:nm}
n\approx\frac{Ap}{\hat\xi^{2}}=\frac{Ap}{a^{2}}\left(1+b m^2\right)^2
\end{eqnarray}
The numerical results of the vortex number $n$ versus the graviton mass $m$ are shown as solid blue dots in Fig.\ref{nm} with error bars presenting the standard deviations. The solid blue line is the fitting relation of the numerical results as $n=17.82\times\left(1+0.1585 m^2\right)^2$ from Eq.\eqref{eq:nm}. Compared to the above $b\approx 0.1496$ in Eq.\eqref{eq:xim} from the right panel of Fig.\ref{kk}, we can see that the values of the coefficient before $m^2$ are close to each other within $5.6151\%$ errors. Estimates of parameter $b$ from these two methods, i.e., one is from the fitting of relation $n\sim m$, the other is from the fitting of $\hat\xi\sim m$, match each other very well! This also indicates that our conjecture of the relation between coherence length and graviton mass, viz. Eq.\eqref{eq:xim} is very trustable.

The overall factor in the front of Eq.\eqref{eq:nm} can even provide us the estimate of the probability $p$, which is the probability for the symmetry-breaking domains to form vortices, in Eq.\eqref{density}. We already knew $a\approx 0.7466$ in Eq.\eqref{eq:xim} from the right panel of Fig.\ref{kk}, and the size of the system is $A=50\times50=2500$, thus we can readily get $p\approx 17.82\times0.7466^2/2500\approx 0.003973$ and $n\approx Ap/\hat\xi^2\approx 9.9331\hat\xi^{-2}$. The later relation is plotted as red dashed line in the Fig.\ref{nm}, where $\hat\xi$ comes from the QNMs analysis in the right panel of Fig.\ref{kk}.  We see that the red dashed line fits very well with the blue fitting line except in the large regime of $m$, such as $m>1.5$.\footnote{In \cite{Blake:2013bqa,Davison:2013jba}, the authors stated that the relation $\tau_s^{-1}=\gamma m^2$ should hold as graviton mass is small, such that the momentum conservation is violated in a minor way. Therefore, if graviton mass is large enough, the above relation $\tau_s^{-1}=\gamma m^2$ may not hold again. Consequently, the analytic relation in Fig.\ref{nm} may not apply as $m$ is large enough.}
This discrepancy originates from the differences between the two fitted values of $b$, i.e, $b\approx 0.1496$ from Eq.\eqref{eq:xim} and $b\approx0.1585$ from Eq.\eqref{eq:nm}. However, the error between these two $b$'s is small, therefore, it is fair to say that our assumption of the relation between the coherence length and the graviton mass, viz. Eq.\eqref{eq:xim} is reliable.

\section{Conclusions and discussions}
\label{sec:conclusion}
In summary, we have investigated the effects of momentum dissipation induced by the graviton mass on the critical dynamics in the background of a $(3+1)$-dimensional dRGT massive gravity by taking advantage of the AdS/CFT correspondence. The KZM scaling laws of the vortex number and the ``freeze-out" time with respect to the quench rate were not affected by the graviton mass. This in turn indicated that the static and dynamic critical exponents were not changed by the existence of graviton mass. It further implied that the boundary field theory was always like a mean-field theory in spite of the graviton mass.

However, the outcome of vortex numbers depended on the graviton mass, since momentum dissipation would shrink the size of the symmetry-breaking domains. Inspired from Pippard's formula on the coherence length and the mean free path, we proposed an analytical relation between the coherence length and the graviton mass. This relation was verified from the QNMs analysis of the perturbations of the scalar field, which was a key result in our paper. We further investigated the relation between the number of vortices and the graviton mass both analytically and numerically, and the results were consistent with each other. Therefore, in conclusion, the momentum dissipation induced by graviton mass would increase the number of vortices, although it would not affect the KZM scaling laws.

\acknowledgments
We are grateful for Adolfo del Campo for helpful discussions and put forward a lot of valuable advices. Besides, we thank Qi-Rong Jiao, Hong-Da Lyu, Han-Qing Shi, Xin-Meng Wu, Chuan-Yin Xia and Jun-Kun Zhao for illuminating discussions. This work was supported by the National Natural Science Foundation of China (Grants No. 11675140, 11705005 and 11875095).

redpajama_set_name: RedPajamaArXiv


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Tag: Hypnotic Eye
Another Posthumous Album Highlights Some of Tom Petty's Most Productive Years
"Angel Dream" is reconfigured and remastered 25th anniversary version of 1996 "She's the One" soundtrack album
While I would call myself a Tom Petty fan and dearly miss him, I'm mostly familiar with his catalog until 1994. Except for his final album with the Heartbreakers, Hypnotic Eye, my knowledge gets spotty when it comes to anything Petty released after his second solo album Wildflowers, alone or together with his longtime band. Among the latter was the August 1996 soundtrack Songs and Music from the Motion Picture "She's the One". That changed over the past few days with Angel Dream, a reconfigured and remastered 25th anniversary edition released on July 2. Listening to the anniversary issue not only led me to check out the original, but also to discover Tom Petty music I really like.
Officially titled Angel Dream (Songs and Music from the Motion Picture "She's the One"), the latest Tom Petty posthumous release is being characterized as a "reimagined reissue." This 25th anniversary edition keeps eight tunes of the original album, eliminates seven and adds four previously unreleased songs. As such, I'm okay with the characterization. But I can also see how some music fans like hotfox63 view the "reimagined reissue" label as a cynical marketing gimmick. Whatever the main motives behind a reissue may be, I think there can be no doubt that money is always part of the equation. Notably, Petty was involved in working on the mixes for Angel Dream with his longtime engineer and co-producer Ryan Ulate prior to his untimely death in October 2017.
I'd like to start this review with Angel Dream (No. 2), the album's beautiful opener, a tune that also appeared on the original edition. During a recent interview on SiriusXM's Tom Petty Radio (channel 31), Heartbreakers co-founder and keyboarder Benmont Tench called it "one of the loveliest songs Tom ever wrote," as transcribed in this Rock Cellar Magazine review. Essentially, Angel Dream (No. 2) bookends the album, with the second bookend being an instrumental reprise titled French Disconnection, one of the previously unreleased tracks.
Among the highlights of the original album and this reissue is Change the Locks, a tune written by Lucinda Williams, which she recorded for her 1988 eponymous third studio album under the slightly different title Changed the Locks. Petty's cover is more straight rock than the more bluesy original. Nice!
One of Life's Little Mysteries is among the previously unreleased tracks. The song's jazzy groove reminds me a bit of Full Grown Body, a tune from the aforementioned Hypnotic Eye. The music certainly fits the lyrics. An excerpt: Go to work in the morning/Try to make a buck/Do everything you're told/And you're still outta luck/It's one of life's little mysteries…
Here's another cool cover and previously unreleased track: Thirteen Days, a J.J. Cale tune included on his fifth studio album 5 that came out in August 1979. "We had a lot of fun playing that song live and it's great to have a recording of it from the studio," said Mike Campbell, ex-Heartbreakers guitarist, during the above SiriusXM interview. I can definitely see why!
The last song I'd like to call out is yet another previously unreleased tune: 105 Degrees, which also is the album's lead single. I realize I already covered this song in my last Best of What's New installment, but since it's an early favorite, I simply couldn't skip it. I just love how this tune is shuffling along!
"'She's The One' was originally a great way to include some of the songs that didn't make it on to Wildflowers, but it has its own thing to it, its own charm, and putting it out now in a restructured form makes for a sweet little treat," Benmont further noted. "At the time in the studio, it was fun working as a band to improvise the scoring cues for the movie rather than playing to preset click tracks and a written score. And it was interesting to try to cut covers of others' songs for a record, instead of learning covers just for live shows."
Here's another tidbit I learned about "She's the One" when doing some research for this post. It's only album by Tom Petty and the Heartbreakers that was recorded without an official drummer. The studio sessions happened following the departure of the band's original drummer Stan Lynch. The album featured contributions from three other drummers: Curt Bisquera, Ringo Starr and Steve Ferrone. Ferrone, who had also played on Wildflowers, became the official drummer of the Heartbreakers shortly after "She's the One" had been recorded.
CD softpak with 12-page booklet.
"These songs are extremely special," added Petty's widow Dana Petty, who together with their two daughters Adria and Annakim manages the Tom Petty estate. "I am grateful this record is getting the recognition it deserves. The remix Ryan Ulyate did sounds amazing, and the unreleased gems are a lovely bonus. Annakim, Adria, and I took a lot of time finding artwork that reflects the mood of the album. I think we finally achieved that with Alia Penner's work. It is surreal and beautiful, just like life during that time."
Angel Dream, which appears on Warner Records and is available in CD and vinyl formats, as well as in digital music platforms, is the fifth posthumous Tom Petty album. It is also the third album with a connection to Wildflowers, widely considered to be one of Petty's best records. October 2020 saw the release of Wildflowers & All the Rest. The super deluxe edition of that reissue, titled Finding Wildflowers, included a disc featuring alternate versions of Wildflowers' 15 tracks, plus You Saw Me Comin', a previously unreleased original song. That CD was released as a standalone under the title Finding Wildflowers (Alternate Versions) in April this year.
I will admit the standalone release does smack a bit like a money grab, since they could have offered it as a separate option when Wildflowers & All the Rest came out. Instead, they waited for six months. In the meantime, if fans wanted to own the alternate versions and that new song, they needed to buy the whole enchilada. I wonder how Tom Petty would have felt about that. After all, he once successfully battled his label MCA when they wanted to sell his then-latest record Damn the Torpedoes at a premium price of $9.98 instead of the usual list price of $8.98.
Sources: Wikipedia; Tom Petty website; Rock Cellar Magazine; YouTube
Author christiansmusicmusingsPosted on July 6, 2021 July 5, 2021 Categories Music ReviewsTags 105 Degrees, 5, Angel Dream (Songs from the Motion Picture "She's the One"), Benmont Tench, Change the Locks, Curt Bisquera, Damn The Torpedoes, Finding Wildflowers, Finding Wildflowers (Alternate Versions), French Disconnection, Full Grown Body, Hypnotic Eye, J.J. Cale, Lucinda Williams, Mike Campbell, Ringo Starr, Rock, Ryan Ulyate, Stan Lynch, Steve Ferrone, Thirteen Days, Tom Petty, Tom Petty and the Heartbreakers, Wildflowers, Wildflowers & All the Rest, You Saw Me Comin'10 Comments on Another Posthumous Album Highlights Some of Tom Petty's Most Productive Years
Second Tom Petty Posthumous Album Out
Career-spanning compilation features hits and two previously unreleased recordings
The title pretty much says it all. The Best Of Everything is a compilation of Tom Petty's amazing music from his 40 years as a recording artist, largely focusing on his better known songs. Released yesterday, it's billed as his first career-spanning collection of hits. Unlike last September's An American Treasure, the 38 tracks for the most part were taken from past albums. There are two exceptions: For Real, a previously unreleased tune, and an alternate version of the title track that restores a lost second verse.
While to a longtime Tom Petty fan like myself it's not exactly news what an outstanding songwriter he was, it's still impressive when you see the track listing. Free Fallin', Mary Jane's Last Dance, Saving Grace, Breakdown, Refugee, American Girl, The Last DJ, Runnin' Down A Dream and Even The Losers, to name some of the gems, surely make for a beautiful collection. While I would say American Treasure is more for die-hard Tom Petty fans, The Best Of Everything is a terrific compilation for folks who know just a few songs and would like to further explore his music beyond the fantastic first Greatest Hits mid-career collection from November 1993.
Released via Geffen Records/UMe, The Best Of Everything is available as a 2-CD or 4-LP set
To make it truly career-spanning, it would have been nice to include a couple of tunes from The Traveling Wilburys. Sure, it's fair to note the supergroup wasn't Petty's band. The Wilburys were primarily initiated by George Harrison and Jeff Lynne, and their songs were credited to all members. Unlike Mudcrutch and Petty's solo albums, Mike Campbell and Benmont Tench, who helped put together The Best Of Everything and last year's compilation, had no involvement with the Wilburys. There may also have been legal reasons for keeping the supergroup's material out. Still, adding two tunes featuring Charlie T. Wilbur Junior on lead vocals would have been cool, in my humble opinion!
Let's get to some music. I deliberately skip the big hits. The track order seems to be a bit random. Perhaps part of the idea here was to spread the bigger hits throughout to keep the more casual Tom Petty fans engaged. The number of YouTube clips from The Best Of Everything is still limited, so I'm borrowing clips from the original albums, as needed. The first tune I'd like to call out is Dreamville from The Last DJ, the 11th studio album by Tom Petty and the Heartbreakers, released in October 2002. I'm glad they included this beautiful ballad, which definitely is not among Petty's big hits.
I Should Have Known It is a nice rocker with a great guitar riff – my kind of song! Perhaps not surprisingly Campbell was a co-writer for this guitar player type of tune, which appeared on the band's 12th studio record Mojo from June 2010. "I was glad that was on there, because I'm really proud of that track and that performance," Campbell noted during an interview with Variety, conducted together with Tench and Petty's eldest daughter Adria Petty, who was also involved in assembling the collection. "It showed a band in their later development still doing quality music." Listen for yourself!
Next up: The alternate version of The Best Of Everything, another great tune! Originally, Tom Petty and the Heartbreakers recorded it for their sixth studio album Southern Accents, which came out in March 1985. Even though I own that record on CD, frankly, I had forgotten about the song.
Scare Easy is a track from the first Mudcrutch album simply titled Mudcrutch, which appeared in April 2008. Initially formed in Gainesville, Fla. in 1970, Mudcrutch was the predecessor to The Heartbreakers. After recording some demos and releasing one single that failed to chart, Mudcrutch broke up in 1975. It's kind of remarkable they lasted for more than four years. Then, in August 2007, Petty reunited the band. In addition to Campbell (guitar, mandolin) and Tench (keyboards), the lineup featured the other two original members Randall Marsh (drums) and Tom Leadon (guitar), with Petty on bass and lead vocals.
The last tune I'd like to call out is For Real. This previously unreleased song also wasn't available on any bootlegs, so until it came out as a single a few weeks ago, it's something even fans hadn't heard before. According to Rolling Stone, the track was recorded in August 2000 and is "a declaration of purpose" by Petty. "That song to me sounds like Tom reporting from his heart — reporting from the front," Tench told Variety during the above interview. "It may sound like it's meant to be a summing up of a career or something, but it's not, really, because it's almost 20 years old. We weren't quite as long-in-tooth and gray then." I think Tench is right, though it's the perfect tune to close out the collection.
"When I went back through all this stuff… I don't want to get heavy with it, but it's very emotional, in being nostalgic, because we were never nostalgic when we were working," Campbell told Variety. "We never looked back. We just always were looking forward. But Ben and I were forced to look back as we went through this stuff, and we both had an epiphany about how we have a legacy that has integrity. We were sad, but also very proud of what we've done." Who can blame them.
Added Adria Petty: "I feel like Ben and Mike haven't had a second to process this, what the next chapter can be, and I think for us, it's kind of the same. Ben had a baby for the first time six or seven weeks after my dad died, and he's been deeply in love and entrenched in that. It's a really horrible thing to have to process both things at the same time, so he probably finally has a little space to just focus on that. Mike's going to be on the road with Fleetwood Mac through April. He had his first grandchild right after Dad died. There's a third generation of Heartbreaker kids coming in that are all amazing."
Benmont Tench (l) and Mike Campbell, August 2018
So after two major compilations, what else might be in store or in the vault I should perhaps better ask. "There a bunch of really great stuff," Tench told Billboard. He noted early Mudcrutch recordings, demos from The Last DJ and music from the period of Hypnotic Eye, the final studio album by Tom Petty and the Heartbreakers from July 2014.
Campbell would like to explore a live album from the band's shows at the Fillmore from 1997 to 1999, he explained to Rolling Stone. "For me, that was almost the pinnacle of the band just being totally spontaneous night to night to night. We might throw in a Grateful Dead song that we just learned that afternoon. We recorded every show and we had guest artists from Bo Diddley to Roger McGuinn to John Lee Hooker. And I know, in my memory of those 20 nights, there's an amazing album in there." That surely sounds like a great idea to me!
However, both Tench and Campbell want to be mindful about further releases to make sure the quality is right and Petty would have wanted to release the material. Adria Petty agrees. "I don't want to inundate the fans with "Hey, here's another record!"," she told Variety. That's a good thing!
Sources: Wikipedia, Tom Petty official website, Variety, Rolling Stone, Billboard, YouTube
Author christiansmusicmusingsPosted on March 2, 2019 Categories Music ReviewsTags An American Treasure, Benmont Tench, Breakdown, Even The Losers, For Real, Free Fallin', George Harrison, Greatest Hits, Hypnotic Eye, I Should Have Known It, Jeff Lynne, Mary Jane's Last Dance, Mike Campbell, Mojo, Randall Marsh, Refugee, Rock, Runnin' Down A Dream, Saving Grace, Scare Easy, Southern Accents, The Best Of Everything, The Last DJ, Tom Leadon, Tom Petty, Tom Petty and the Heartbreakers17 Comments on Second Tom Petty Posthumous Album Out
New Tom Petty Box Set Works Because It's Not A Greatest Hits Or Typical Anthology Compilation
An American Treasure focuses on previously unreleased material, including alternate takes, deep cuts and live versions
When you see a box set being issued one year after the death of a widely beloved music artist like Tom Petty, you can't entirely escape the cynical notion that somebody is trying to make a quick buck here. And while I'm sure Reprise Records wouldn't mind, should An American Treasure turn out to be a hot seller, this box set is neither a greatest hits compilation nor a typical anthology, and that's a good thing! Instead, the career-spanning collection focuses on previously unreleased alternate song versions, live performances and deep cuts. Is it going to gain Tom Petty additional listeners post mortem? Probably not. Are longtime fans going to like it? I certainly do and think others will as well.
An American Treasure, which dropped on September 28, is the first release following Tom Petty's untimely death on October 2, 2017 at age 66 – just one week after the triumphant conclusion of his 40th anniversary tour with the Heartbreakers. I hate to sound like a broken record, but it still hurts and like so many other longtime fans, gosh, I miss him!
According to the official press release that announced the box set in July, Adria Petty and Dana Petty – Tom's daughter and wife, respectively – were the key drivers behind this new collection. They teamed up with former Heartbreakers guitarist and keyboarder Mike Campbell and Benmont Tench, as well as Ryan Ulyate, one of Petty's studio collaborators. Campbell, Tench and Ulyate co-produced the box set, while Adria and Dana Petty served as executive producers.
"Everyone involved in this project chose each track with tremendous care and deep respect for the body of work Tom Petty created over the course of 40 years," Adria and Dana Patty stated. "He also accumulated a wealth of unreleased music in his vaults, and we have collectively uncovered one gem after another that will keep us all listening and discovering new facets of Tom's talent for many years to come. We can't wait to share with Tom's fans this musical portrait of an artist who deeply affected our culture and indelibly touched the lives of fans the world over."
Time for some music. Lost In Your Eyes is a previously unreleased single recorded during sessions in 1974 with Mudcrutch, Tom Petty's band that preceded the Heartbreakers and included future members Mike Campbell (guitar) and Benmont Tench (keyboards). Tom Leadon (guitar and vocals), the brother of former Eagles lead guitarist Bernie Leadon; Jim Lenehan (vocals); and Randall Marsh (drums) rounded out the lineup. Petty was on bass and vocals.
Keep A Little Soul is a previously unreleased tune from the 1982 sessions for Long After Dark, the fifth studio album Tom Petty and the Heartbreakers released in November that year. It also appeared as the collection's first single back in July when the box set was initially announced. Here's a video featuring rare never-before-seen footage of the band.
In 1984, Tom Petty and the Heartbreakers recorded a demo with Stevie Nicks called The Apartment Song. Perhaps it was motivated by the Petty/Campbell co-write Stop Draggin' My Heart Around, which had appeared in July 1981 on Nicks' studio debut Bella Donna, generating a U.S. hit that peaked at no. 3 on the Billboard Hot 100. The tune, which must have been recorded around the same time the band was working on their sixth studio release Southern Accents, did not make that album or any other records, as far as I know.
Another collaboration on the box set is King Of The Hill, a song Roger McGuinn co-wrote with Petty. It became the lead single to McGuinn's sixth studio album Back From Rio released in January 1991. The version on the box set is an early take from November 1987 – great tune!
In April 1999, Tom Petty and the Heartbreakers came out with their 10th studio album Echo. One track that was recorded during the sessions for the record but not included on the album or released separately is Gainesville, an autobiographic song about Petty's home town: Home-grown, in the headphone/Sandy loadin' up the van/Singin' through the speakers/You're alright anywhere you land/Gainesville was a big town/Gainesville was a big town…
The last track I'd like to highlight is another song related to Petty's home state of Florida: Bus To Tampa Bay, yet another previously unreleased tune. It was recorded during the sessions for Hypnotic Eye, the final studio album Tom Petty and the Heartbreakers released in July 2014.
An American Treasure is available in various formats: A Super Deluxe Limited Edition 4-CD set, a 6-LP Vinyl Edition and a 2-CD Standard Edition. All of the recordings have been mixed by Ryan Ulyate from transfers of the original studio multitrack masters. They have been re-mastered by Chris Bellman, a sound engineer at Bernie Grundman Mastering, who has worked with artists like Diana Ross, Neil Young, Carole King, Duran Duran and Van Halen, among others.
Sources: Wikipedia, Tom Petty website, YouTube
Author christiansmusicmusingsPosted on October 5, 2018 Categories Music ReviewsTags Adria Petty, An American Treasure, Back From Rio, Bella Donna, Benmont Tench, Bernie Leadon, Bus To Tampa Bay, Carole King, Chris Bellman, Dana Petty, Diana Ross, Duran Duran, Eagles, Echo, Gainesville, Hypnotic Eye, Jim Lenehan, Keep A Little Soul, King Of The Hill, Long After Dark, Lost In Your Eyes, Mike Campbell, Mudcrutch, Neil Young, Randall Marsh, Rock, Roger McGuinn, Ryan Ulyate, Southern Accents, Stevie Nicks, Stop Draggin' My Heart Around, The Apartment Song, Tom Leadon, Tom Petty, Tom Petty and the Heartbreakers, Van Halen2 Comments on New Tom Petty Box Set Works Because It's Not A Greatest Hits Or Typical Anthology Compilation


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When the human condition is conceived as fragmented and haunted by an unavoidable sense of solitude, the body becomes a site of transformation, a liminal space where the borders between in and out, between subject and object, are blurred.
IN-BE-TWEEN investigates the relationship between absence and presence, between the part and the whole, and takes Elena's research questions on subjectivity and autobiography to create an installation performance where the body is exhibited, either as a still image intersected and fragmented by the structure of the space, or as performing small acts of self-constitution. Traces of the artist's body and personal life stories are exposed within the fragmenting structure of the building.
Performance credits and production: Elena Molinaro.


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The final photo of the "Sundrops" set to end the week. Similar to yesterday's but it has a lot of different qualities so I thought I'd post it.
Beautiful reflections and detail in the millions of droplets. Great background gradient.
gorgeous shot ryan! love the colors and details... also that gradient is very cool.
Best of the series. Much to draw the eye around the frame. Great contrasts throughout - including contrast between upper left and lower right of frame. I like abstracts too, when interesting. And this one is.


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Page 17, 25 January 1896 — The Italian Ambassador (General Ferrero) was present at the banquet,
The Italian Ambassador (General Ferrero) was present at the banquet,
and in responding to the toast of his health. made the happy remark that of two people who were on bad terms with each other, it used to be said that they were " at the Antipodes," but the speeches referring to the attitude of our Colonies to the United Kingdom and to each other, showed that such a phrase had totally lost its meaning, and would express the happiest relations at least as well as the unhappiest. In other speeches of Mr. Chamberlain's, it was noticed by way of illustration of the great area and potential expansion of our Colonies, that even Queensland, where Lord Lamington is to be the Governor, is about three times as great in area as the German Empire,—a hint received with great cheering,—and that in a single generation its popula- tion has increased fifteenfold. It was impossible to overrate the importance of our relations to such mighty dependencies as these, and nothing can be more obvious than that the enthusiastic expressions of loyalty which we received from Australia and Canada alike, will outweigh more and more as time goes on, the supposed significance of our "splendid isolation" on the Continent of Europe. Besides, as the presence of the Italian Ambassador showed, that isolation, even though it is splendid, is not absolutely complete.


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Volunteers spruce up West Side school
Spencer Academy got a makeover during Comcast Cares Day
by Contributing Reporter April 26, 2017 February 10, 2021
During the 16th Annual Comcast Cares Day at Spencer Elementary Technology Academy, 214 N. Lavergne Ave., dozens of volunteers from Comcast and the education organization City Year joined with teachers, students, and community stakeholders to participate in a beautification project on April 22.
Comcast Cares Day represents one of the largest corporate days of service in the nation, with projects occurring simultaneously throughout the country. Comcast held two events in Chicago, one at Spencer and another at CHA Mary Hartwell Catherwood Apartments for Seniors in Lakeview.
Kelly Dean, principal at Spencer Technology Academy, said changing the culture and climate of the school's space is one of the school's major needs. She said her students needed the investment because sometimes they feel no one cares about them. Spencer has 680 students from pre-K through 8th grade.
"I'm like a kid on Christmas," said Kelly. "Comcast Cares Day is really important to us. It's really an investment in making sure the school feels like a school, that it feels like somewhere kids should be, with the idea that if the school starts to look pretty that'll also change the mindset of how students treat the building."
Dean, who is the third principal in four years at Spencer, said she is "not going anywhere" and stressed continuity is key for students to feel that the school is a "safe space".
Dean said volunteers created a Dr. Seuss mural in the primary building, installed accent walls in 10 of the primary classrooms, installed a chalkboard walk in their art room, built cubbies for students to store their personal items, built bookcases, installed interactive whiteboard tables, painted murals on every floor of the building and repainted the cafeteria, among other tasks.
Rebeca Nieves Huffman, vice president and executive director for City Year, said her organization has partnered with Comcast for Comcast Cares Day since 2001.
"The reason why we did this is because Comcast and City Year believe our students deserve beautiful spaces to learn in," said Huffman.
Huffman said she spoke with Dr. Janice Jackson, CPS' chief education officer, about which schools should be under consideration for a clean-up and said it was Jackson who recommended Spencer. Huffman noted a potential project would be optimal for City Year if it could engage at least 200 volunteers.
"This is what Comcast employees do along with City Year corps members and the City Year family," Huffman said. "We pick a school every year with Comcast and we beautify it and that's what our students deserve."
Huffman said she's constantly reminded that people want to get involved and make a difference which makes collecting volunteers easier.
Janet Garrett, a Comcast employee in the sales department, said she selected the Spencer project because she hails from the West Side of Chicago and wanted to help her daughter obtain community service hours for the National Honors Society.
"You just feel better about yourself when you decide to give to others," said Garrett, adding that the event was "awesome."
Cook County Commissioner Richard Boykin (Dist.-1), who spoke at the start of the event, said the volunteer projects would "help raise the level of beautification in the neighborhood".
"This is all about raising the hopes of the kids who actually call this school home," said Boykin. "This gives us all hope that we can put our hands to the plow and we can do some work that's meaningful and that the children will actually benefit from."


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Nettleham
All Saints' Church, Nettleham
Location within Lincolnshire
3,437 (2011 Census)
TF008754
120 mi (190 km) S
Shire county
01522 & 01673
53°15′58″N 0°29′16″W / 53.266167°N 0.487741°W / 53.266167; -0.487741Coordinates: 53°15′58″N 0°29′16″W / 53.266167°N 0.487741°W / 53.266167; -0.487741
Nettleham is a large village and civil parish within the West Lindsey district of Lincolnshire, England, 4 miles (6.4 km) north-east from the city of Lincoln between the A46 and A158.
The population of the civil parish was 3,437 at the 2011 census.[1]
2 Governance
6 Twinning
The now-demolished Bishop's Manor House at Nettleham was the property of Edith of Wessex, wife of Edward the Confessor and later Empress Matilda, daughter of King Henry I, before passing into the possession of the Bishops of Lincoln, who enlarged it to create a Bishop's Palace appropriate to one of the country's most important Sees. On 7 February 1301 King Edward I was staying in the Bishop's Palace when he created his son Edward (later King Edward II) as the first Prince of Wales. The building was damaged during the Lincolnshire Rising of 1536 and completely demolished by 1650, only traces of foundations remaining on the site now called Bishop's Palace Field.[2]
The parish church of All Saints dates from the Saxon period, with medieval and 19th century additions. It is now in the benefice of Nettleham with Riseholme and Grange de Lings.[3]
Thomas Gardiner's grave in Nettleham churchyard
Within the church's graveyard is a headstone in memory of Thomas Gardiner, a post-boy murdered hereabouts by two highway robbers in January 1733. The inscription declares he was 'barbarously murdered' aged 19. The robbers - two brothers by the name of Hallam - committed another murder near Faldingworth before being arrested. They were convicted of murder at Lincoln and executed at the site of their crimes. (Thomas Gardiner's headstone declares he was killed on 3 January 1732 since at the time Britain used the Julian Calendar.)[4][5]
The Royal Society for Nature Conservation (RSNC) had been based in Nettleham but moved to Newark-on-Trent in 1999. The site became the home of the WATCH Trust for Environmental Conservation, but this also moved to Newark a few years ago.[6]
Since April 1974 Nettleham has formed part of the West Lindsey district of Lincolnshire. It forms part of the Gainsborough parliamentary constituency which is represented by Sir Edward Leigh.
The parish boundary meets Greetwell on the A158 Horncastle/Wragby road. It follows the A15 Wragby Road into Lincoln for about 110 yards (100.6 m) where it meets Lincoln, and skirts the edge of the housing estate (Glebe Park) next to the bypass; the Lincoln bypass (A158) from the A46 to the A158 is in the parish. The boundary crosses Nettleham Road (B1182, former A46), south of the bypass roundabout, and follows south of the A46 bypass for about 550 yards (502.9 m) and meets Riseholme (south of the bypass). The bypass passes northwards skirting, the edge of the University of Lincoln's Riseholme College. 550 yards north of Nettleham Hall, it meets Grange de Lings, and borders this parish along a farm track until the A46, where it meets Scothern just north of Nettleham Heath Farm. It crosses Scothern Beck north of Skelton House Farm, passes south, and at Nettleham Beck it meets Sudbrooke, crossing Sudbrooke Lane east of Richmond Farm. North of Manor Farm, it meets Reepham on the A158 Roman road and follows the A158 to North Greetwell, where it meets Greetwell.
Nettleham has won the "Best Kept Village Award" several times,[7] and the centre of the village is a conservation area. Large modern housing estates surround the old village centre. Nettleham is also the location of the Lincolnshire Police headquarters to the west of the village near the A46. It was opened by the Queen in 1980.
Village public houses are the Black Horse on Chapel Lane, the Plough on Church Street, the Brown Cow on Lincoln Road, and the White Hart on High Street.
The parish includes an oil well owned by Star Energy, north of the A158 bypass, which has been producing since 1985.
Nettleham F.C. have been members of the Lincolnshire League since their relegation from the Central Midlands League. They have twice played Aston Villa football club in friendlies.[citation needed] Nettleham Cricket Club play in the Lincolnshire ECB League. Both teams play their home fixtures at Mulsanne Park, Nettleham. The village also has a tennis club.
Mulsanne, Pays de la Loire, north-west France. The sports pitch is called Mulsanne Park.
Henry Holbeach – served as the last Prior and first Dean of Worcester; buried here
HMS Nettleham
^ "Civil Parish population 2011". Neighbourhood Statistics. Office for National Statistics. Retrieved 25 May 2016.
^ Bishops Manor, Pastscape, English Heritage
^ "All Saints Nettleham Parish Church". Retrieved 16 November 2019.
^ Urban, Sylvanus. The Gentleman's Magazine: Or, Monthly Intelligencer. For the Year 1733. Volume III. p.43, 99, 154
^ Codd, Daniel (2013). Tales from the Gibbet Post (The Jeering of Horns in Lincoln). Amazon Media EU S.à r.l. Kindle Edition. ASIN: B00D2B8OWA
^ Wildlife WATCH
^ Nettleham Parish Council. "Nettleham Parish Council". Retrieved 21 October 2011.
Media related to Nettleham at Wikimedia Commons
Nettleham in the Domesday Book
Nettleham medical practice
CE Junior school
Infants school
Nettleham F.C.
Nettleham Parish Church