In General > s.a. cosmology; dark
energy; fine-structure constant; relativistic
cosmological models.
* Idea: A possibly time-varying, inhomogenous cosmological scalar
field with canonical kinetic terms and negative pressure, rolling down a potential,
that may be responsible for the acceleration of the universe.
* Issue: How can it be
distinguished from a cosmological constant? Or another field like
a Chaplygin gas?
And Cosmology > s.a. dark
matter; FRW models; Quintom;
Unparticles.
@ General references: Crooks et al MPLA(01)ap/00 [cmb];
Chernin et al PLA(02)ap/01 [solutions];
Yahiro et al PRD(02)ap/01 [constraints];
Faraoni IJMPD(02)ap/01 [acceleration
and
non-minimal
coupling]; González-Díaz NPB(01);
Mathews et al ap/02-in;
Gardner
NPB(05)ap/04 [model
comparison]; Fang et al IJMPD(06)
[vs non-linear Born-Infeld scalar]; Martin MPLA(08)-a0803-in
[rev].
@ Vs cosmological constant:
Binétruy IJTP(00);
Doran & Wetterich ap/02-in;
Melchiorri & Odman ap/02-in;
Chongchitnan & Efstathiou PRD(07)-a0705.
@ And observational cosmology: Gerke & Efstathiou MNRAS(02)ap [parameters];
Rosati PLB(03)
[and dark matter]; Colombo & Gervasi JCAP(06)ap;
La Vacca & Kristiansen JCAP(09).
@ Inflation: Faraoni PRD(00)gq;
Gunzig et al PRD(01)gq/00;
Martin & Musso PRD(05)ap/04.
@ And supergravity: Brax & Martin PLB(99)ap,
ap/00-in;
Copeland et al PRD(00).
@ From brane cosmology: González-Díaz PLB(00);
Maeda PRD(01)ap/00;
Mizuno & Maeda PRD(01)hp.
@ From Brans-Dicke: Banerjee & Pavón CQG(01)gq/00; Sen & Seshadri
IJMPD(03)gq/00;
Chakraborty et al MPLA(03).
References and Related Topics > s.a. duality.
@ II: Caldwell & Steinhardt
pw(00)nov.
@ General: Carroll PRL(98)ap;
Huey et al PRD(99)ap/98;
Huterer & Turner PRD(99)ap/98;
Amendola PRD(00)ap/99,
Chiba PRD(99)gq [matter
coupling]; Di Pietro & Demaret
IJMPD(01)gq/99 [scalar
pot]; Brax & Martin PRD(00)ap/99 [and
quantum field theory corrections]; Zlatev et al PRL(99)
[tracker field]; Steinhardt et al PRD(99)
[tracker solutions]; Sahni CQG(02)ap [rev];
Linder GRG(08)-a0704
[dynamics].
@ Scalar-tensor gravity:
Bartolo & Pietroni PRD(00)hp/99;
Esposito-Farèse in(02)gq/00.
@ 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-in
[inhomogeneous]; Riazuelo & Uzan
PRD(00)ap [with
scalar and grav rad]; 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]; Svrcek ht/06 [axions
from string theory].
@ Phenomenology: Cooray & Huterer ApJL(99)ap;
Wang et al ApJ(00)ap/99;
Barger & Marfatia PLB(01)ap/00 [vs
k-essence]; Wetterich PLB(04)
[parametrization of equation of state].
@ And galactic dynamics: Matos & Guzman AdP(00)ap;
Arbey et al PRD(01)ap,
PRD(02)ap/01 [galaxy
halos].
@ And particle physics: Rosati hp/00-in
[inflaton]; Chung et al PLB(03).
@ Variations: Boyle et al PLB(02),
Banerjee & Das ASS(06)gq/05 [spintessence];
Chugreev
et al TMP(07)gq/06 [in
relativistic theory of gravity]; > s.a. K-Essence.
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sep 2009