Cosmological constraints from gas mass fractions of massive, relaxed galaxy clusters

被引:43
作者
Mantz, Adam B. [1 ]
Morris, R. Glenn [1 ,2 ]
Allen, Steven W. [1 ,2 ,3 ]
Canning, Rebecca E. A. [1 ,4 ]
Baumont, Lucie [5 ]
Benson, Bradford [6 ,7 ,8 ]
Bleem, Lindsey E. [8 ,9 ]
Ehlert, Steven R. [10 ]
Floyd, Benjamin [11 ]
Herbonnet, Ricardo [5 ]
Kelly, Patrick L. [12 ]
Liang, Shuang [5 ]
von Der Linden, Anja [5 ]
McDonald, Michael [13 ]
Rapetti, David A. [14 ,15 ,16 ]
Schmidt, Robert W. [17 ]
Werner, Norbert [18 ]
Wright, Adam [19 ]
机构
[1] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, 452 Lomita Mall, Stanford, CA 94305 USA
[2] SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA
[3] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA
[4] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England
[5] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA
[6] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[7] Univ Chicago, Dept Astron & Astrophys, 5640 S Ellis Ave, Chicago, IL 60637 USA
[8] Univ Chicago, Kavli Inst Cosmol Phys, 5640 S Ellis Ave, Chicago, IL 60637 USA
[9] Argonne Natl Lab, HEP Div, Argonne, IL 60439 USA
[10] Marshall Space Flight Ctr, Huntsville, AL 35812 USA
[11] Univ Missouri, Dept Phys & Astron, 5110 Rockhill Rd, Kansas City, MO 64110 USA
[12] Univ Minnesota, Sch Phys & Astron, 116 Church St SE, Minneapolis, MN 55455 USA
[13] MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[14] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[15] Univ Space Res Assoc, Res Inst Adv Comp Sci, Mountain View, CA 94043 USA
[16] Univ Colorado, Ctr Astrophys & Space Astron, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USA
[17] Heidelberg Univ, Astron Rech Inst, Zentrum Astron, Monchhofstr 12-14, D-69120 Heidelberg, Germany
[18] Masaryk Univ, Fac Sci, Dept Theoret Phys & Astrophys, Kotlaeska 2, CZ-61137 Brno, Czech Republic
[19] Milwaukee Sch Engn, Dept Phys & Chem, 432 E Kilbourn Ave, Milwaukee, WI 53202 USA
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
cosmological parameters; cosmology: observations; dark matter; distance scale; galaxies: clusters: general; X-rays: galaxies: clusters; X-RAY-CLUSTERS; DARK ENERGY; INTRACLUSTER MEDIUM; BARYON FRACTION; HOT GAS; ASTROPHYSICS; SIMULATIONS; I; PARAMETERS; TELESCOPE;
D O I
10.1093/mnras/stab3390
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present updated cosmological constraints from measurements of the gas mass fractions (f(gas)) of massive, dynamically relaxed galaxy clusters. Our new data set has greater leverage on models of dark energy, thanks to the addition of the Perseus cluster at low redshifts, two new clusters at redshifts z greater than or similar to 1, and significantly longer observations of four clusters at 0.6 < z < 0.9. Our low-redshift (z < 0.16) f(gas) data, combined with the cosmic baryon fraction measured from the cosmic microwave background (CMB), imply a Hubble constant of h = 0.722 +/- 0.067. Combining the full f(gas) data set with priors on the cosmic baryon density and the Hubble constant, we constrain the dark energy density to be Omega(Lambda) = 0.865 +/- 0.119 in non-flat Lambda cold dark matter (cosmological constant) models, and its equation of state to be in flat, constant-w models, respectively 41percent and 29percent tighter than our previous work, and comparable to the best constraints available from other probes. Combining f(gas), CMB, supernova, and baryon acoustic oscillation data, we also constrain models with global curvature and evolving dark energy. For the massive, relaxed clusters employed here, we find the scaling of f(gas) with mass to be consistent with a constant, with an intrinsic scatter that corresponds to just similar to 3percent in distance.
引用
收藏
页码:131 / 145
页数:15
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