Quintessence |
In General
> s.a. cosmology; fine-structure constant;
generalized cosmological models.
* Idea: A possibly
time-varying, inhomogenous cosmological scalar field with canonical
kinetic terms and negative pressure (for example, described by a
tachyonic field), rolling down a potential, that may be responsible
for the late accelerated expansion of the universe.
* Issue: How can it be distinguished
from a cosmological constant? Or another field like a Chaplygin gas?
@ Intros, reviews:
Caldwell & Steinhardt pw(00)nov;
Sahni CQG(02)ap;
Martin MPLA(08)-a0803-proc;
Tsujikawa CQG(13)-a1304.
@ General references: Carroll PRL(98)ap;
Huey et al PRD(99)ap/98;
Huterer & Turner PRD(99)ap/98;
Di Pietro & Demaret IJMPD(01)gq/99 [scalar potential];
Brax & Martin PRD(00)ap/99 [and quantum field theory corrections];
Faraoni IJMPD(02)ap/01 [acceleration and non-minimal coupling];
González-Díaz NPB(01);
Mathews et al ap/02-conf;
Gardner NPB(05)ap/04 [model comparison];
Fang et al IJMPD(06) [vs non-linear Born-Infeld scalar];
Linder GRG(08)-a0704 [dynamics];
Gong PLB(14)-a1401 [general dynamical behavior].
> Online resources:
see Wikipedia page.
And Observational Cosmology > s.a. Chameleon Field;
dark matter; FLRW models;
Quintom; Unparticles.
@ General references: Gerke & Efstathiou MNRAS(02)ap [parameters];
Rosati PLB(03) [and dark matter];
Colombo & Gervasi JCAP(06)ap;
La Vacca & Kristiansen JCAP(09);
Sefusatti & Vernizzi JCAP(11) [clustering and structure formation];
Mukherjee & Banerjee EPJP(15)-a1311 [scalar potential reconstruction];
Hussain a1809 [and galaxy power spectrum];
Yang et al PRD(19)-a1810 [constraints];
Landim a1908 [interacting, cosmological perturbations].
@ As dark energy:
Khurshudyan et al IJTP(14)-a1402 [interacting models];
Shahalam et al EPJC(15)-a1503.
@ Solutions: Zlatev et al PRL(99) [tracker field];
Steinhardt et al PRD(99) [tracking];
Chernin et al PLA(02)ap/01;
Harko et al EPJC(14)-a1310;
Roy & Banerjee a1402 [dynamical systems study];
Asenjo & Hojman a1509 [new method].
@ Vs cosmological constant:
Binétruy IJTP(00);
Doran & Wetterich NPPS(03)ap/02;
Melchiorri & Odman ap/02-proc;
Chongchitnan & Efstathiou PRD(07)-a0705.
@ Vs modified gravity: Clemson & Koyama JCAP(13)-a1209.
@ And the cmb: Crooks et al MPLA(01)ap/00;
Grisa & Sorbo PRD(10)-a1002 [preferred directions].
@ And inflation: Faraoni PRD(00)gq;
Gunzig et al PRD(01)gq/00;
Martin & Musso PRD(05)ap/04.
Other Phenomenology
@ General references:
Cooray & Huterer ApJL(99)ap;
Wang et al ApJ(00)ap/99;
Barger & Marfatia PLB(01)ap/00 [vs k-essence];
Yahiro et al PRD(02)ap/01 [constraints];
Wetterich PLB(04) [parametrization of equation of state].
@ Black holes: Fernando GRG(12)-a1202 [surrounded by quintessence];
> s.a. schwarzschild-de sitter spacetime [Nariai black holes].
@ Galactic dynamics:
Matos & Guzman AdP(00)ap;
Arbey et al PRD(01)ap,
PRD(02)ap/01 [galaxy halos];
Schrempp & Brown JCAP(10)-a0912 [and clustered matter].
@ Particle physics: Amendola PRD(00)ap/99,
Chiba PRD(99)gq [matter coupling];
Rosati hp/00-proc [inflaton];
Chung et al PLB(03).
Models and Variations > s.a. duality.
@ Brans-Dicke theory: Banerjee & Pavón CQG(01)gq/00;
Sen & Seshadri IJMPD(03)gq/00;
Chakraborty et al MPLA(03).
@ Other scalar-tensor gravity: Bartolo & Pietroni PRD(00)hp/99;
Esposito-Farèse in(02)gq/00.
@ Supergravity: Brax & Martin PLB(99)ap,
ap/00-proc;
Copeland et al PRD(00).
@ Brane cosmology: González-Díaz PLB(00);
Maeda PRD(01)ap/00;
Mizuno & Maeda PRD(01)hp.
@ Other models: de la Macorra & Piccinelli PRD(00)hp/99;
Perrotta et al PRD(00)ap/99 [extended];
Sahni & Wang PRD(00)ap/99;
Chimento et al gq/99-proc [inhomogeneous];
Riazuelo & Uzan PRD(00)ap [with scalar and gravitational radiation];
Signore NCB(01) [negative curvature];
Zimdahl et al PLB(01)ap [with cold dark matter];
Bento et al PRD(02)ap/01 [2 fields];
Cardenas et al PRD(03)ap/02 [both quintessence and cosmological constant];
Wetterich PRL(03)ht/02 [conformal fixed point, cosmological constant];
Svrček ht/06 [axions from string theory];
Guarnizo et al a1910-MG15 [p-form].
@ Variations:
Boyle et al PLB(02),
Banerjee & Das ApSS(06)gq/05 [spintessence];
Chugreev et al TMP(07)gq/06 [in relativistic theory of gravity];
Mehrabi et al ApSS(17)-a1510 [from non-Abelian gauge fields];
> s.a. k-Essence.
main page
– abbreviations
– journals – comments
– other sites – acknowledgements
send feedback and suggestions to bombelli at olemiss.edu – modified 24 oct 2019