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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity

文献类型：期刊论文

作者Mueller, Eva-Maria3; Percival, Will3; Linder, Eric4,5,6; Alam, Shadab7,8,9; Zhao, Gong-Bo3,10; Sanchez, Ariel G.11; Beutler, Florian3; Brinkmann, Jon1,2
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2018-04-01
卷号475期号:2页码:2122-2131
ISSN号0035-8711
关键词gravitation cosmological parameters dark energy large-scale structure of Universe cosmology: observations cosmology: theory
DOI10.1093/mnras/stx3232
英文摘要We use baryon acoustic oscillation and redshift space distortion from the completed Baryon Oscillation Spectroscopic Survey, corresponding to Data Release 12 of the Sloan Digital Sky Survey, combined sample analysis in combination with cosmic microwave background, supernova, and redshift space distortion measurements from additional spectroscopic surveys to test deviations from general relativity. We present constraints on several phenomenological models of modified gravity: First, we parametrize the growth of structure using the growth index gamma, finding gamma = 0.566 +/- 0.058 (68 per cent C. L.). Secondly, we modify the relation of the two Newtonian potentials by introducing two additional parameters, GM and G(L). In this approach, G(M) refers to modifications of the growth of structure whereas G(L) to modification of the lensing potential. We consider a power law to model the redshift dependence of G(M) and G(L) as well as binning in redshift space, introducing four additional degrees of freedom, G(M)(z < 0.5), G(M)(z > 0.5), G(L)(z < 0.5), and G(L)(z > 0.5). At 68 per cent C. L., we measure G(M) = 0.980 +/- 0.096 and G(L) = 1.082 +/- 0.060 for a linear model, G(M) = 1.01 +/- 0.36 and G(L) = 1.31 +/- 0.19 for a cubic model as well as G(M)(z < 0.5) = 1.26 +/- 0.32, G(M)(z > 0.5) = 0.986 +/- 0.022, G(L)(z < 0.5) = 1.067 +/- 0.058, and G(L)(z > 0.5) = 1.037 +/- 0.029. Thirdly, we investigate general scalar tensor theories of gravity, finding the model to be mostly unconstrained by current data. Assuming a one-parameter f(R) model, we can constrain B-0 < 7.7 x 10(-5) (per cent C. L). For all models we considered, we find good agreement with general relativity.
WOS关键词DIGITAL SKY SURVEY ; REDSHIFT-SPACE DISTORTIONS ; SURVEY COSMOLOGICAL IMPLICATIONS ; LARGE-SCALE STRUCTURE ; GROWTH-RATE ; POWER SPECTRUM ; DARK ENERGY ; COSMIC STRUCTURE ; FOURIER SPACE ; SAMPLE
资助项目European Research Council[614030] ; UK Science and Technology Facilities Council[ST/N000668/1] ; UK Space Agency[ST/N00180X/1] ; NSF[PHY-1066293] ; Energetic Cosmos Laboratory ; US Department of Energy, Office of Science, Office of High Energy Physics[DE-SC-0007867] ; US Department of Energy, Office of Science, Office of High Energy Physics[DE-AC02-05CH11231] ; Trans-regional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; NSFC[11673025] ; Chinese Academy of Sciences[XDB09000000] ; University of Portsmouth ; European Research Council through the COSFORM Research Grant[670193] ; Alfred P. Sloan Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; University of Arizona ; Brazilian Participation Group ; Brookhaven National Laboratory ; Carnegie Mellon University ; University of Florida ; French Participation Group ; German Participation Group ; Harvard University ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; NewMexico State University ; New York University ; Ohio State University ; Pennsylvania State University ; Princeton University ; Spanish Participation Group ; University of Tokyo ; University of Utah ; Vanderbilt University ; University of Virginia ; University of Washington ; Yale University
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:000427345900046
资助机构European Research Council ; European Research Council ; UK Science and Technology Facilities Council ; UK Science and Technology Facilities Council ; UK Space Agency ; UK Space Agency ; NSF ; NSF ; Energetic Cosmos Laboratory ; Energetic Cosmos Laboratory ; US Department of Energy, Office of Science, Office of High Energy Physics ; US Department of Energy, Office of Science, Office of High Energy Physics ; Trans-regional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; Trans-regional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; NSFC ; NSFC ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; University of Portsmouth ; University of Portsmouth ; European Research Council through the COSFORM Research Grant ; European Research Council through the COSFORM Research Grant ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; Carnegie Mellon University ; Carnegie Mellon University ; University of Florida ; University of Florida ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; Max Planck Institute for Extraterrestrial Physics ; NewMexico State University ; NewMexico State University ; New York University ; New York University ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; Yale University ; Yale University ; European Research Council ; European Research Council ; UK Science and Technology Facilities Council ; UK Science and Technology Facilities Council ; UK Space Agency ; UK Space Agency ; NSF ; NSF ; Energetic Cosmos Laboratory ; Energetic Cosmos Laboratory ; US Department of Energy, Office of Science, Office of High Energy Physics ; US Department of Energy, Office of Science, Office of High Energy Physics ; Trans-regional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; Trans-regional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; NSFC ; NSFC ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; University of Portsmouth ; University of Portsmouth ; European Research Council through the COSFORM Research Grant ; European Research Council through the COSFORM Research Grant ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; Carnegie Mellon University ; Carnegie Mellon University ; University of Florida ; University of Florida ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; Max Planck Institute for Extraterrestrial Physics ; NewMexico State University ; NewMexico State University ; New York University ; New York University ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; Yale University ; Yale University ; European Research Council ; European Research Council ; UK Science and Technology Facilities Council ; UK Science and Technology Facilities Council ; UK Space Agency ; UK Space Agency ; NSF ; NSF ; Energetic Cosmos Laboratory ; Energetic Cosmos Laboratory ; US Department of Energy, Office of Science, Office of High Energy Physics ; US Department of Energy, Office of Science, Office of High Energy Physics ; Trans-regional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; Trans-regional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; NSFC ; NSFC ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; University of Portsmouth ; University of Portsmouth ; European Research Council through the COSFORM Research Grant ; European Research Council through the COSFORM Research Grant ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; Carnegie Mellon University ; Carnegie Mellon University ; University of Florida ; University of Florida ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; Max Planck Institute for Extraterrestrial Physics ; NewMexico State University ; NewMexico State University ; New York University ; New York University ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; Yale University ; Yale University ; European Research Council ; European Research Council ; UK Science and Technology Facilities Council ; UK Science and Technology Facilities Council ; UK Space Agency ; UK Space Agency ; NSF ; NSF ; Energetic Cosmos Laboratory ; Energetic Cosmos Laboratory ; US Department of Energy, Office of Science, Office of High Energy Physics ; US Department of Energy, Office of Science, Office of High Energy Physics ; Trans-regional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; Trans-regional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; NSFC ; NSFC ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; University of Portsmouth ; University of Portsmouth ; European Research Council through the COSFORM Research Grant ; European Research Council through the COSFORM Research Grant ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; Carnegie Mellon University ; Carnegie Mellon University ; University of Florida ; University of Florida ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; Max Planck Institute for Extraterrestrial Physics ; NewMexico State University ; NewMexico State University ; New York University ; New York University ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; Yale University ; Yale University
源URL[http://ir.bao.ac.cn/handle/114a11/37272]  
专题中国科学院国家天文台
通讯作者Mueller, Eva-Maria
作者单位1.Apache Point Observ, Sunspot, NM 88349 USA
2.New Mexico State Univ, Sunspot, NM 88349 USA
3.Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England
4.Univ Calif Berkeley, Berkeley Ctr Cosmol Phys, Berkeley, CA 94720 USA
5.Univ Calif Berkeley, Berkeley Lab, Berkeley, CA 94720 USA
6.Nazarbayev Univ, Energet Cosmos Lab, Astana 010000, Kazakhstan
7.Carnegie Mellon Univ, Dept Phys, 5000 Forbes Ave, Pittsburgh, PA 15213 USA
8.Carnegie Mellon Univ, McWilliams Ctr Cosmol, 5000 Forbes Ave, Pittsburgh, PA 15213 USA
9.Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
10.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714		 Mueller, Eva-Maria,Percival, Will,Linder, Eric,et al. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,475(2):2122-2131.
APA Mueller, Eva-Maria.,Percival, Will.,Linder, Eric.,Alam, Shadab.,Zhao, Gong-Bo.,...&Brinkmann, Jon.(2018).The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,475(2),2122-2131.
MLA Mueller, Eva-Maria,et al."The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 475.2(2018):2122-2131.

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来源：国家天文台

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