|  Cosmological Parameters | 
In General
  > s.a. cosmological models; modern
  cosmology [theory]; observational cosmology [including age].
  * Idea: The standard ΛCDM
    cosmological model depends on 6 parameters, extensions include additional parameters;
    The main tools to obtain estimates of their values are measurements of the microwave
    background, supernovae, and galaxy clusters (distribution, lensing, X-rays,
    Sunyaev-Zel'dovich effect).
  @ Reviews: Lahav & Liddle ap/04-PDG,
    JPG(06)ap;
    Sánchez et al ap/06-ASP;
    Lahav & Liddle PLB(04)-a1002;
    Croft & Dailey QPR-a1112
      [analysis of parameter determinations 1990-2010];
    Lahav & Liddle a1401-PDG.
  @ General references: Freedman PNAS(98)ap/97;
    Carlberg ap/98-conf;
    Tegmark et al ap/98/ApJL;
    Noyes gq/99;
    Roos & Harun-or-Rashid ap/99-proc;
    Turner AIP(99)ap;
    Freedman PS(00)ap/99-in,
    PRP(00)ap/99-in;
    Primack ASP-ap/99,
    NPPS(00)ap;
    Novosyadlyj et al A&A-ap/99,
    ap/00-proc;
    Fukugita ap/00-in;
    Durrer & Novosyadlyj MNRAS(01)ap/00;
    Peebles ap/00-IAU;
    Krauss ap/01-proc;
    Leach et al PRD(02)ap [and inflation];
    Freedman IJMPA(02)ap-proc;
    Deustua et al ap/02-conf;
    Roos & Harun-or-Rashid ap/02;
    Shemi-Zadeh gq/02 [??];
    Krauss ESO(03)ap-proc;
    Blanchard ap/03-conf;
    Bridle et al Nat(03)ap [open issues];
    Douspis CRP(03)ap/04 [method];
    Roos ap/05 [consensus];
    Wilczek hp/05-conf [reasoning];
    Balbi PoS-ap/06;
    Apunevych et al a0802 [WMAP2006];
    Wraith et al PRD(09) [adaptive importance sampling];
    Sato et al PRL(10)-a1011 [using a copula likelihood function];
    Gong et  MNRAS(13)-a1110 [effect of different observational data];
    Paoletti et al MNRAS(12)-a1112 [multifrequency approach];
    Axelsson et al ApJL(13)-a1303 [directional dependence];
    Crandall & Ratra PLB(14)-a1311 [median statistics values].
  @ Models and parameter sets:
    Liddle MNRAS(04)ap;
    Godłowski & Szydłowski PLB(05) [with dark energy];
    Hajian PRD(07) [Hamiltonian Monte Carlo technique];
    Eifler et al A&A(09)-a0810 [and cosmic shear];
    Liddle ARNPS(09)-a0903 [statistical methods];
    Dinculescu ASS(09)-a0907 [tentative derivation];
    Shafieloo & Linder PRD(11)-a1107 [data used and degeneracy in parameter values];
    Dossett & Ishak PRD(12)-a1205 [effect of spatial curvature];
    Sharov & Vorontsova JCAP(14)-a1407 [ΛCDM, generalized Chaplygin gas and multidimensional model];
    > s.a. standard model [including extensions].
  @ Errors: Dodelson & Schneider PRD(13)-a1304 [effect of covariance estimator error];
    Joachimi & Taylor IAU-a1412 [cosmological parameter covariance].
  > Related topics: see acceleration;
    expansion rate; geometry; matter content
    [including density values] and distribution; relativistic
    cosmology [averaging].
From the Cosmic Microwave Background > s.a. cmb.
  @ General references: Jungman et al PRD(96);
    Hancock et al MNRAS(98)ap/97;
    Bartlett et al ap/98-proc;
    Efstathiou ap/00;
    Tegmark & Zaldarriaga ApJ(00)ap;
    de Bernardis et al Nat(00)apr-ap;
    Lange et al PRD(01)ap/00 [Boomerang];
    Christensen et al CQG(01) [Bayesian];
    Cornish PRD(01) [acoustic peak];
    Douspis et al A&A(01)ap;
    Sakellariadou ap/01-conf;
    Melchiorri ap/02-conf;
    Kosowsky et al PRD(02)ap;
    Wang et al PRD(02)ap [consistency];
    Rubiño-Martin et al MNRAS(03)ap/02 [from VSA];
    Contaldi & CBI ap/02-proc;
    Melchiorri & Ödman PRD(03)ap [pre-WMAP];
    Lineweaver ap/03-ln [and inflation];
    Bouchet ap/04-proc;
    Rebolo et al MNRAS(04)ap [VSA data];
    Das et al JCAP(15)-a1406 [after BICEP 2 and BOSS].
  @ And large-scale structure:
    Percival et al MNRAS(02)ap [+2dF survey];
    Doux et al MNRAS(18)-a1706.
  @ And lensing: Contaldi et al PRL(03)ap;
    Chantavat et al PRD(16)-a1409 [with cosmic voids].
  @ And polarization:
    Jiménez et al PRD(04);
    QUaD collaboration ApJ(09)-a0901;
    Cheng & Huang EPJC(14)-a1403 [from BICEP2, Planck and WMAP].
  @ From WMAP data: Lewis ap/03-conf [questioning models for WMAP];
    Hansen et al MNRAS(04)ap;
    Komatsu et al ApJS(09)-a0803,
    Dunkley et al ApJS(09)-a0803,
    Lewis PRD(08) [5-year results];
    Jarosik et al ApJS(11)-a1001 [7-year results];
    Finelli et al MNRAS(13)-a1207 [WMAP-7 reanalysis];
    Hinshaw et al ApJS(13)-a1212 [9-year results].
  @ From Planck data: Planck Collaboration A&A(16)-a1502.
  @ Theory: Komatsu & Seljak MNRAS(02)ap [Sunyaev-Zel'dovich effect];
    Perotto et al JCAP(06)ap/06 [Monte Carlo simulations];
    Smidt et al PRD(10) [impact of secondary non-Gaussianities];
    Catena & Notari JCAP(13)-a1210 [impact of cmb aberration].
From Other Observations > s.a. early-universe
  cosmology [nucleosynthesis]; observational cosmology [chemistry].
  @ HI clouds / 21-cm background: Mao et al PRD(08)-a0802;
    Bharadwaj et al PRD(09)-a0809;
    Visbal et al JCAP(09)-a0812;
    > s.a. astronomy.
  @ Galaxy surveys: Tegmark PRL(97);
    Peel & Knox NPPS(03)ap/02 [peculiar neutrinos];
    Tegmark et al PRD(04)ap/03 [SDSS];
    Pope et al ApJ(04)ap [SDSS];
    Del Popolo & Ercan IAU(04)ap [theory];
    Gaztañaga et al MNRAS(06)ap/04 [and cmb];
    Seljak et al PRD(05)ap/04 [and SN, WMAP, Ly-α];
    Reboul & Cordoni A&A(06)ap [interacting galaxies];
    Tozzi LNP(07)ap/06;
    Xanthopoulos et al AIP(06)ap [VLA];
    Blake et al MNRAS(07)ap/06 [SDSS];
    Sánchez & Cole MNRAS(08)-a0708 [power spectrum difference between 2dFGRS and SDSS];
    Betancort-Rijo et al MNRAS(09)-a0901 [statistics of voids];
    Sánchez et al MNRAS(09)-a0901;
    Hamann et al JCAP(10)-a1003;
    Allen et al ARAA(11)-a1103 [galaxy clusters];
    Burenin & Vikhlinin AL(12)-a1202 [galaxy-cluster mass functions];
    Di Dio et al JCAP(14)-a1308 [large-scale structure];
    Penna-Lima et al JCAP(14) [biases on estimators].
  @ Supernovae: Nesseris & Perivolaropoulos PRD(04)ap [models];
    Odman et al IJMPD(04)ap;
    Wang & Dai MNRAS(06)ap/05 [and GRBs];
    Neill et al ApJL(07)-a0704,
    Gordon et al PRL(07) [using supernova peculiar velocities];
    Kowalski et al ApJ(08)-a0804;
    Kessler et al ApJS(09)-a0908 [SDSS-II];
    Kirshner a0910-ch;
    March et al MNRAS(11)-a1102;
    Baumgärtel a1106
      [k = 1 in Friedmann equation, and constraints on other parameters];
    Gao & Gong CQG(14)-a1308 [tension with cmb results];
    Benítez-Herrera et al MNRAS(13)-a1308 [model-independent approach];
    Li et al ApJL(14)-a1409 [associated with GRBs].
  @ Gravitational waves: Cutler & Holz PRD(09)-a0906 [BBO];
    Del Pozzo PRD(12) [second-generation interferometers];
    Zhang et al a1907 [simulated ET standard siren data].
  @ Other observations:
    Bagla et al CA(96)ap/95 [matter];
    Coe & Moustakas ApJ(09)-a0906 [lensing delays];
    Behera & Wagner a0908-in [EBL attenuation of VHE spectra];
    Jullo et al Sci(10)-a1008 [strong lensing];
    Pavlov et al ApJ(12)-a1206 [space-based galaxy surveys];
    van den Bosch et al MNRAS(13)-a1206 [galaxy clustering and  lensing];
    Moresco et al JCAP(12) [expansion rate of the universe];
    Prasad & Souradeep PRD(12),
    Prasad a1412 [using particle swarm optimization];
    Wei et al ApJ(13)-a1301,
    Amati et al IJMPD(13) [GRBs];
    Khadka & Ratra MNRAS-a2007.
  @ Effects of inhomogeneities: Buchert & Carfora CQG(02)gq,
    PRL(03)gq/02 [smoothing and dressed parameters];
    Valkenburg & Bjaelde MNRAS(12)-a1203 [living near the Great Attractor];
    Fleury et al PRD(13)-a1302;
    Fleury a1511-PhD;
    > s.a. cosmological principle.
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