The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae

被引:124
作者
Blake, Chris [1 ]
Glazebrook, Karl [1 ]
Davis, Tamara M. [2 ,3 ]
Brough, Sarah [4 ]
Colless, Matthew [4 ]
Contreras, Carlos [1 ]
Couch, Warrick [1 ]
Croom, Scott [5 ]
Drinkwater, Michael J. [2 ]
Forster, Karl [6 ]
Gilbank, David [7 ]
Gladders, Mike [8 ]
Jelliffe, Ben [5 ]
Jurek, Russell J. [9 ]
Li, I-hui [1 ]
Madore, Barry [10 ]
Martin, D. Christopher [6 ]
Pimbblet, Kevin [11 ]
Poole, Gregory B. [1 ]
Pracy, Michael [1 ,12 ]
Sharp, Rob [2 ,12 ]
Wisnioski, Emily [1 ]
Woods, David [13 ]
Wyder, Ted K. [6 ]
Yee, H. K. C. [14 ]
机构
[1] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
[2] Univ Queensland, Sch Math & Phys, Brisbane, Qld 4072, Australia
[3] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, DK-2100 Copenhagen O, Denmark
[4] Australian Astron Observ, Epping, NSW 1710, Australia
[5] Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW 2006, Australia
[6] CALTECH, Pasadena, CA 91125 USA
[7] Univ Waterloo, Dept Phys & Astron, Astrophys & Gravitat Grp, Waterloo, ON N2L 3G1, Canada
[8] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[9] CSIRO, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
[10] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA
[11] Monash Univ, Sch Phys, Clayton, Vic 3800, Australia
[12] Australian Natl Univ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia
[13] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[14] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 3H4, Canada
基金
澳大利亚研究理事会;
关键词
surveys; dark energy; distance scale; DIGITAL SKY SURVEY; BARYON ACOUSTIC-OSCILLATIONS; BVRI LIGHT CURVES; REDSHIFT-SPACE; COSMOLOGICAL MODEL; POWER-SPECTRUM; IA SUPERNOVAE; UNIVERSE; CONSTRAINTS; EVOLUTION;
D O I
10.1111/j.1365-2966.2011.19606.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Astronomical observations suggest that todays Universe is dominated by a dark energy of unknown physical origin. One of the most notable results obtained from many models is that dark energy should cause the expansion of the Universe to accelerate: but the expansion rate as a function of time has proved very difficult to measure directly. We present a new determination of the cosmic expansion history by combining distant supernovae observations with a geometrical analysis of large-scale galaxy clustering within the WiggleZ Dark Energy Survey, using the AlcockPaczynski test to measure the distortion of standard spheres. Our result constitutes a robust and non-parametric measurement of the Hubble expansion rate as a function of time, which we measure with 1015 per cent precision in four bins within the redshift range 0.1 < z < 0.9. We demonstrate, in a manner insensitive to the assumed cosmological model, that the cosmic expansion is accelerating. Furthermore, we find that this expansion history is consistent with a cosmological-constant dark energy.
引用
收藏
页码:1725 / 1735
页数:11
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