WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies

被引：54

作者：

Riemer-Sorensen, Signe ^{[1
]}

Blake, Chris ^{[2
]}

Parkinson, David ^{[1
]}

Davis, Tamara M. ^{[1
]}

Brough, Sarah ^{[3
]}

Colless, Matthew ^{[3
]}

Contreras, Carlos ^{[2
]}

Couch, Warrick ^{[2
]}

Croom, Scott ^{[4
]}

Croton, Darren ^{[2
]}

Drinkwater, Michael J. ^{[1
]}

Forster, Karl ^{[5
]}

Gilbank, David ^{[6
]}

Gladders, Mike ^{[7
]}

Glazebrook, Karl ^{[2
]}

Jelliffe, Ben ^{[4
]}

Jurek, Russell J. ^{[8
]}

Li, I-Hui ^{[2
]}

Madore, Barry ^{[9
]}

Martin, D. Christopher ^{[5
]}

Pimbblet, Kevin ^{[10
]}

Poole, Gregory B. ^{[2
]}

Pracy, Michael ^{[4
]}

Sharp, Rob ^{[3
,11
]}

Wisnioski, Emily ^{[2
]}

Woods, David ^{[12
]}

Wyder, Ted K. ^{[5
]}

Yee, H. K. C. ^{[13
]}

机构：

[1] Univ Queensland, Sch Math & Phys, Brisbane, Qld 4072, Australia

[2] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia

[3] Australian Astron Observ, Epping, NSW 1710, Australia

[4] Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW 2006, Australia

[5] CALTECH, Pasadena, CA 91125 USA

[6] S African Astron Observ, ZA-7935 Observatory, South Africa

[7] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA

[8] CSIRO Astron & Space Sci, Australia Telescope Natl Facil, Epping, NSW 1710, Australia

[9] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA

[10] Monash Univ, Sch Phys, Clayton, Vic 3800, Australia

[11] Australian Natl Univ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia

[12] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada

[13] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 3H4, Canada

来源：

PHYSICAL REVIEW D | 2012年 / 85卷 / 08期

基金：

澳大利亚研究理事会;

关键词：

POWER-SPECTRUM; SPACE; RED;

D O I：

10.1103/PhysRevD.85.081101

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The absolute neutrino mass scale is currently unknown, but can be constrained by cosmology. The WiggleZ high redshift, star-forming, and blue galaxy sample offers a complementary data set to previous surveys for performing these measurements, with potentially different systematics from nonlinear structure formation, redshift-space distortions, and galaxy bias. We obtain a limit of Sigma m(v) < 0.60 eV (95% confidence) for WiggleZ+Wilkinson Microwave Anisotropy Probe. Combining with priors on the Hubble parameter and the baryon acoustic oscillation scale gives Sigma m(v) < 0: 29 eV, which is the strongest neutrino mass constraint derived from spectroscopic galaxy redshift surveys.

引用

页数：7

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