Dark Energy| Dark Energy |
In General
> s.a. cosmological constant [including history] and models;
cosmology [future]; varying constants.
* Idea: A component of the content of the
universe with negative pressure, which accelerates its expansion; May be a cosmological
contant or may be dynamical; The name seems to have been introduced by M Turner.
* Status: 2003, Various methods
give −1.22 < w < −0.78 at 95% c.l.; 2004–2005,
Analysis still favors a cosmological constant – other models give as good a fit,
but are not as simple (1-parameter) or physically motivated – with quintessence a
second possibility; 2006, Evidence from Brad Schaefer's analysis of distant GRBs that it
may be changing; 2006, Evidence from supernovas at z = 1 consistent with constant
dark energy; 2007, Supernova survey gives w = −1.07 (+0.09−0.09 stat,
1 σ) (± 0.12 sys); 2009, Observations are still consistent with a cosmological
constant; 2015, First data from the Dark Energy Survey.
* Plans: 2006, Two satellites
planned, DES (possible launch 2008–2009) and SNAP (launch after 2010).
@ I: Turner ThSc(00)nov;
Kirshner 02;
Caldwell pw(04)may;
Conselice SA(07)feb;
Linder & Perlmutter pw(07)dec [future];
Perlmutter SA(08)apr;
news PhysOrg(12)nov [hints that dark energy is dynamic];
Lincoln & Nord TPT(14)sep;
news Cosmos(17)sep [timescape, Wiltshire's alternative].
@ General references: Finelli et al PRD(07)ap/06 [light bending];
Heavens et al MNRAS(06)ap [3D cosmic shear];
White RPP(07)-a0704,
response Kolb RPP(07)-a0708 [and astronomy];
Dobado & Maroto ASS(09)-a0802-proc [intro];
Ellis conf(09)-a0811;
Daly AIP(09)-a0901;
Greenhill et al a0902-rp;
Sami CS(09)-a0904 [primer];
Ruiz-Lapuente ed-10 [theory and observations];
news ns(12)dec [Einstein-Schrödinger correspondence];
Heymans Phy(15) [Dark Energy Survey];
Ziaeepour a1411-Hab [and phenomenology];
> s.a. gas; topological defects.
@ Reviews: Carroll ap/01-ch;
Peebles & Ratra RMP(03);
Lima BJP(04)-ap/04;
Sahni LNP(05)ap/04 [and dark matter];
Frampton ap/04-talk;
Padmanabhan CS(05)ap/04;
Linder NAR(05)ap/04-conf,
ap/05-conf;
Bean et al ap/05-rp;
Weinberg NAR(05)ap-proc;
Padmanabhan ap/05-proc,
AIP(06)ap;
Barnes et al PASA(05)ap;
Copeland et al IJMPD(06)ht;
Straumann MPLA(06)hp;
Polarski AIP(06)ap;
Carroll NJP(06);
Padmanabhan GRG(08)-a0705;
Linder AJP(08)mar-a0705 [RL];
Turner & Huterer JPSJ(07)-a0706;
Capozziello IJGMP(07)-a0706;
Stubbs IJMPD(07)-a0712 [and fundamental physics];
issue GRG(08)feb;
Zhao MPLA(08) [and modified gravity];
Padmanabhan ASL(09)-a0807-in;
Wanas a0809-conf;
Frieman AIP(08)-a0904-ln;
Harvey EJP(09);
Kesavan MSc(09)-a0908;
issue NPPS(09)194 [proc];
Linder a1009-ch;
Amendola & Tsujikawa 10;
Wang 10 [r PT(11)jun];
Matarrese et al ed-11;
Durrer PTRS(11)-a1103-talk [what we really know];
Li et al CTP(11)-a1103,
FoP-a1209;
Capozziello & Lambiase NAP-a1304;
Polarski IJMPD(13);
Mortonson et al PDG-a1401;
Gleyzes et al IJMPD(14)-a1411 [unifying description];
Novosyadlyj et al a1502-book;
Huterer & Shafer RPP(18)-a1709.
Phenomenology and Evidence
> s.a. Chameleon Field; dark-energy models
and equations of state; dark energy and dark matter.
* 2008: Evidence that dark energy
slowed down the growth of structure (galaxy clusters) significantly.
@ Evidence:
Scranton et al ap/03/PRL [SDSS and WMAP analysis];
Straumann gq/03-talk [rev];
Alam et al JCAP(04)ap [dynamical];
Ishak FP(07)ap/05 [general discussion];
Trotta & Bower A&G(06)ap [surveys, rev];
news pw(06)nov,
pw(06)nov [distant supernovas];
Bambi PRD(07) [Mpc-scale];
Sarkar GRG(08)-a0710 [critical view];
Bothun et al PLB(08) [precision observations without supernovas];
Chernin et al G&C(10) [evidence near the Milky Way];
Frieman PT(14)apr
[upcoming Dark Energy Survey of 200 million galaxies];
Ho & Hsu APP(16)-a1501 [astrophysical force];
> s.a. acceleration.
@ Lab evidence and tests: Beck & Mackey PLB(05)ap/04 [proposal],
refutation Jetzer & Straumann PLB(05);
Frampton MPLA(06)ht/05 [re possible Josephson junction cutoff];
Corasaniti et al MNRAS(06)ap/05 [with ALPACA];
Fassbender et al SPIE(06)ap [VADER mission proposal];
Phillips et al SPIE(06)ap [JEDI proposal];
de Matos & Beck AiA(09)-a0707 [rotating superconductors];
Brax et al JHEP(09)-a0904 [collider constraints on interactions];
Fujii & Homma a0912,
PTP(11)-a1006 [proposed lab searches];
Perl IJMPA(09)-a0809 [questioning the detection possibility];
Perl a1007 [proposal using atom interferometry];
> s.a. neutrons.
@ Other observations: Mersini-Houghton & Kelleher a0808 [radiation from black-hole binaries];
Honscheid & DuPoy a0810-conf [Dark Energy Camera];
Gould a0902-rp [wide-field imager in space];
Mortonson et al PRD(10),
PRD(10)-a1004 [probes, figures of merit];
Joudaki & Kaplinghat PRD(12)-a1106.
@ Density:
Wang & Mukherjee PRD(07) [and cosmic curvature];
Reichardt et al ApJL(12)-a1110 [bound on early dark energy density].
@ Distribution, and large-scale structure: Solevi et al MNRAS(06)ap/05 [from galaxy distribution];
Wang & Freese PLB(06) [density];
Takada PRD(06)ap [and redshift surveys];
Martín-Moruno et al GRG(09)-a0803 [accretion onto black holes];
Bhattacharya & Kosowsky PRD(08) [galaxy cluster peculiar velocities];
Blomqvist et al JCAP(08)-a0806,
Cooray et al JCAP(10)-a0812 [inhomogeneities, from supernova observations];
Chapline a1004 [clumped into dark-energy stars];
Prescod-Weinstein & Afshordi a1010/ApJ [dark-matter haloes];
Grande & Perivolaropoulos PRD(11)-a1103 [constraints on inhomogeneities];
Bernal et al JCAP(16)-a1511 [homogeneous?];
Średzińska et al a1606-proc [tracing with quasars];
Ntelis & Ealet for Euclid a1805-conf [homogeneity scale].
@ Anisotropy: Appleby et al PRD(10)-a0912 [bounds];
Campanelli et al IJMPD(11)-a1103 [anisotropic model and observations].
@ And perturbations: Gordon NPPS(05)ap;
Gordon & Wands PRD(05)ap;
Polarski & Gannouji PLB(08)-a0710;
Ballesteros & Riotto PLB(08);
news an(08)dec [effect on galaxy clusters];
Dent et al PRD(09)-a0903 [scale dependence of the growth function];
Li et al PLB(11)-a1008;
Anselmi et al JCAP(11)-a1106 [dark-energy clustering].
@ Structure formation: Linder & Jenkins MNRAS(03)ap;
Speliotopoulos a0711;
Alimi et al MNRAS(10)-a0903;
Courtin et al MNRAS(11)-a1001;
Lee MPLA(10);
Novosyadlyj et al KPCB(14)-a1311 [stability, galaxies and galaxy clusters].
Related Topics > s.a. acceleration [including alternatives];
black holes [dark energy stars]; galaxies;
neutrinos; spherical solutions.
@ And entropy, holography: Hsu PLB(04) [and entropy bounds];
Linder ht/04 ["dark entropy"];
Pavón & Zimdahl AIP(06)ht/05;
Beltrán Almeida & Pereira PLB(06),
Guberina et al PLB(06),
Simpson JCAP(07)ap/06,
Pavón JPA(07)gq/06-proc,
Zimdahl IJMPD(08)-a0705 [holographic];
Medved GRG(09)-a0802;
Setare IJMPD(09)-a0901 [from f(R) gravity];
Zhang et al IJMPD(11)-a1001;
Durán et al JCAP(10) [observational constraints];
Viaggiu a1312;
Wang et al PRP(17)-a1612 [rev];
Rodriguez-Benites et al a1905-conf;
> s.a. entropy
bounds; holography.
@ Interactions, particles:
Amendola et al ApJL(03)ap/02;
Böhmer & Harko FP(08)gq/06 [quanta];
DeDeo PRD(06);
Ichiki & Keum a0803 [neutrinos];
Jiménez & Martín-Moruno a1004 [accretion onto black holes and wormholes];
del Campo et al IJMPD(11)-a1103;
Clemson et al PRD(12)-a1109;
Vagnozzi et al a1911 [dark energy-baryon scattering];
> s.a. gravitational waves.
@ Analysis, interpretation:
Choudhury & Padmanabhan A&A(05)ap/03;
Gong CQG(05)ap/04;
Linder PRD(04)ap,
PRD(04)ap;
Linder PRD(07)-ap/06 [limits to z-resolution];
Clarkson et al JCAP(07) [need to include curvature as parameter];
Wang a0712-talk [observational approaches];
Clarkson AIP(10)-a0911;
Bolejko A&A(11)-a1006 [determining its evolution from measurements];
Jiménez et al JCAP(12)-a1201 [effective Lagrangian].
@ Thermodynamics: Gong et al PRD(07)gq/06;
Bilić FdP(08)-a0812-conf.
@ Other theory: Garriga & Vilenkin PRD(03)ap/02 [and anthropic principle];
Padmanabhan & Choudhury MNRAS(03)ap/02 [and supernova data];
Krauss & Chaboyer Sci(03)jan [and globular clusters];
Huey ap/04 [data-driven approach];
Brevik & Gorbunova GRG(05)gq [and viscosity];
Baccigalupi & Acquaviva PoS-ap/06 [and cmb lensing];
Neupane & Carter PLB(06) [relaxation and cosmological constant];
Durrer & Maartens GRG(08) [overview];
Antoniadis et al NJP(07) [dynamical screening of cosmological constant];
Pereira a0806 [negative chemical potential];
Frampton a1004 [universe as black hole];
Ahn et al PLB(11)-a1106 [and renormalization group flow];
Barboza et al PRD(15)-a1501 [constraints].
@ Modified Friedmann equation:
Dvali & Turner ap/03;
> s.a. cosmological models in general relativity
and in modified theories [including Cardassian].
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