Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing
Autor(a) principal: | |
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Data de Publicação: | 2019 |
Outros Autores: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.99.123505 http://hdl.handle.net/11449/228700 |
Resumo: | We present constraints on extensions of the minimal cosmological models dominated by dark matter and dark energy, ΛCDM and wCDM, by using a combined analysis of galaxy clustering and weak gravitational lensing from the first-year data of the Dark Energy Survey (DES Y1) in combination with external data. We consider four extensions of the minimal dark energy-dominated scenarios: (1) nonzero curvature ωk, (2) number of relativistic species Neff different from the standard value of 3.046, (3) time-varying equation-of-state of dark energy described by the parameters w0 and wa (alternatively quoted by the values at the pivot redshift, wp, and wa), and (4) modified gravity described by the parameters μ0 and ς0 that modify the metric potentials. We also consider external information from Planck cosmic microwave background measurements; baryon acoustic oscillation measurements from SDSS, 6dF, and BOSS; redshift-space distortion measurements from BOSS; and type Ia supernova information from the Pantheon compilation of datasets. Constraints on curvature and the number of relativistic species are dominated by the external data; when these are combined with DES Y1, we find ωk=0.0020-0.0032+0.0037 at the 68% confidence level, and the upper limit Neff<3.28(3.55) at 68% (95%) confidence, assuming a hard prior Neff>3.0. For the time-varying equation-of-state, we find the pivot value (wp,wa)=(-0.91-0.23+0.19,-0.57-1.11+0.93) at pivot redshift zp=0.27 from DES alone, and (wp,wa)=(-1.01-0.04+0.04,-0.28-0.48+0.37) at zp=0.20 from DES Y1 combined with external data; in either case we find no evidence for the temporal variation of the equation of state. For modified gravity, we find the present-day value of the relevant parameters to be ς0=0.43-0.29+0.28 from DES Y1 alone, and (ς0,μ0)=(0.06-0.07+0.08,-0.11-0.46+0.42) from DES Y1 combined with external data. These modified-gravity constraints are consistent with predictions from general relativity. |
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Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensingWe present constraints on extensions of the minimal cosmological models dominated by dark matter and dark energy, ΛCDM and wCDM, by using a combined analysis of galaxy clustering and weak gravitational lensing from the first-year data of the Dark Energy Survey (DES Y1) in combination with external data. We consider four extensions of the minimal dark energy-dominated scenarios: (1) nonzero curvature ωk, (2) number of relativistic species Neff different from the standard value of 3.046, (3) time-varying equation-of-state of dark energy described by the parameters w0 and wa (alternatively quoted by the values at the pivot redshift, wp, and wa), and (4) modified gravity described by the parameters μ0 and ς0 that modify the metric potentials. We also consider external information from Planck cosmic microwave background measurements; baryon acoustic oscillation measurements from SDSS, 6dF, and BOSS; redshift-space distortion measurements from BOSS; and type Ia supernova information from the Pantheon compilation of datasets. Constraints on curvature and the number of relativistic species are dominated by the external data; when these are combined with DES Y1, we find ωk=0.0020-0.0032+0.0037 at the 68% confidence level, and the upper limit Neff<3.28(3.55) at 68% (95%) confidence, assuming a hard prior Neff>3.0. For the time-varying equation-of-state, we find the pivot value (wp,wa)=(-0.91-0.23+0.19,-0.57-1.11+0.93) at pivot redshift zp=0.27 from DES alone, and (wp,wa)=(-1.01-0.04+0.04,-0.28-0.48+0.37) at zp=0.20 from DES Y1 combined with external data; in either case we find no evidence for the temporal variation of the equation of state. For modified gravity, we find the present-day value of the relevant parameters to be ς0=0.43-0.29+0.28 from DES Y1 alone, and (ς0,μ0)=(0.06-0.07+0.08,-0.11-0.46+0.42) from DES Y1 combined with external data. These modified-gravity constraints are consistent with predictions from general relativity.Cerro Tololo Inter-American Observatory National Optical Astronomy Observatory, Casilla 603Department of Physics and Astronomy University College London, Gower StreetDepartment of Physics and Electronics Rhodes University, P.O. Box 94Institute of Cosmology and Gravitation University of PortsmouthKavli Institute for Cosmology University of Cambridge, Madingley RoadInstitute of Astronomy University of Cambridge, Madingley RoadDepartment of Physics and Astronomy University of PennsylvaniaLSST, 933 North Cherry AvenueArgonne National Laboratory, 9700 South Cass AvenueCNRS UMR 7095 Institut d'Astrophysique de ParisSorbonne Universités UPMC Univ Paris 06 UMR 7095 Institut d'Astrophysique de ParisCenter for Cosmology and Astro-Particle Physics Ohio State UniversityInstitute of Physics Laboratory of Astrophysics École Polytechnique Fédérale de Lausanne (EPFL) Observatoire de SauvernyJodrell Bank Center for Astrophysics School of Physics and Astronomy University of Manchester, Oxford RoadKavli Institute for Particle Astrophysics and Cosmology Stanford University, P.O. Box 2450SLAC National Accelerator LaboratoryInstituto de Física Teórica Universidade Estadual PaulistaDepartment of Physics Carnegie Mellon UniversityLaboratório Interinstitucional de E-Astronomia - LIneA, Rua Gal. José Cristino 77Observatório Nacional, Rua Gal. José Cristino 77Department of Astronomy University of Illinois at Urbana-Champaign, 1002 W. Green StreetNational Center for Supercomputing Applications, 1205 West Clark StreetInstitut de Física d'Altes Energies (IFAE) Barcelona Institute of Science and Technology Campus UABInstitute of Space Sciences (ICE-CSIC) Campus UAB, Carrer de Can Magrans, s/nInstitut d'Estudis Espacials de Catalunya (IEEC)Kavli Institute for Cosmological Physics University of ChicagoDepartment of Physics University of MichiganCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)Department of Physics Stanford University 382 Via Pueblo MallDepartment of Physics IIT HyderabadFermi National Accelerator Laboratory, P. O. Box 500Excellence Cluster Universe, Boltzmannstrasse 2Faculty of Physics Ludwig-Maximilians-Universität, Scheinerstrasse 1Jet Propulsion Laboratory California Institute of Technology, 4800 Oak Grove DriveDepartment of Astronomy/Steward Observatory, 933 North Cherry AvenueDepartment of Astronomy University of MichiganInstitute for Astronomy University of EdinburghJet Propulsion Laboratory California Institute of TechnologyComputer Science and Mathematics Division Oak Ridge National LaboratoryInstituto de Fisica Teorica UAM/CSIC Universidad Autonoma de MadridUniversitäts-Sternwarte Fakultät für Physik Ludwig-Maximilians Universität München, Scheinerstr. 1Department of Physics ETH Zurich, Wolfgang-Pauli-Strasse 16Santa Cruz Institute for Particle PhysicsDepartment of Physics Ohio State UniversityMax Planck Institute for Extraterrestrial Physics, GiessenbachstrasseLawrence Berkeley National Laboratory, 1 Cyclotron RoadAustralian Astronomical ObservatoryDepartamento de Física Matemática Instituto de Física Universidade de São Paulo, CP 66318George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy Department of Physics and Astronomy Texas AandM UniversityDepartment of Astronomy Ohio State UniversityInstitució Catalana de Recerca i Estudis AvançatsFaculty of Physics Ludwig-Maximilians-Universität, Scheinerstr. 1Excellence Cluster Universe, Boltzmannstr. 2Department of Physics and Astronomy Pevensey Building University of SussexInstituto de Física Gleb Wataghin Universidade Estadual de CampinasICTP South American Institute Fundamental Research Instituto de Física Teórica Universidade Estadual PaulistaSchool of Physics and Astronomy University of SouthamptonBrandeis University Physics Department, 415 South StreetInstituto de Física Teórica Universidade Estadual PaulistaICTP South American Institute Fundamental Research Instituto de Física Teórica Universidade Estadual PaulistaNational Optical Astronomy ObservatoryUniversity College LondonRhodes UniversityUniversity of PortsmouthUniversity of CambridgeUniversity of PennsylvaniaLSSTArgonne National LaboratoryInstitut d'Astrophysique de ParisOhio State UniversityObservatoire de SauvernyUniversity of ManchesterStanford UniversitySLAC National Accelerator LaboratoryUniversidade Estadual Paulista (UNESP)Carnegie Mellon UniversityLaboratório Interinstitucional de E-Astronomia - LIneAObservatório NacionalUniversity of Illinois at Urbana-ChampaignNational Center for Supercomputing ApplicationsBarcelona Institute of Science and TechnologyInstitute of Space Sciences (ICE-CSIC)Institut d'Estudis Espacials de Catalunya (IEEC)University of ChicagoUniversity of MichiganMedioambientales y Tecnológicas (CIEMAT)382 Via Pueblo MallIIT HyderabadFermi National Accelerator LaboratoryExcellence Cluster UniverseLudwig-Maximilians-UniversitätCalifornia Institute of TechnologyUniversity of EdinburghOak Ridge National LaboratoryUniversidad Autonoma de MadridLudwig-Maximilians Universität MünchenETH ZurichSanta Cruz Institute for Particle PhysicsMax Planck Institute for Extraterrestrial PhysicsLawrence Berkeley National LaboratoryAustralian Astronomical ObservatoryUniversidade de São Paulo (USP)Texas AandM UniversityInstitució Catalana de Recerca i Estudis AvançatsUniversity of SussexUniversidade Estadual de Campinas (UNICAMP)University of SouthamptonPhysics DepartmentAbbott, T. M.C.Abdalla, F. B.Avila, S.Banerji, M.Baxter, E.Bechtol, K.Becker, M. R.Bertin, E.Blazek, J.Bridle, S. L.Brooks, D.Brout, D.Burke, D. L.Campos, A. [UNESP]Carnero Rosell, A.Carrasco Kind, M.Carretero, J.Castander, F. J.Cawthon, R.Chang, C.Chen, A.Crocce, M.Cunha, C. E.Da Costa, L. N.Davis, C.De Vicente, J.Derose, J.Desai, S.Di Valentino, E.Diehl, H. T.Dietrich, J. P.Dodelson, S.Doel, P.Drlica-Wagner, A.Eifler, T. F.Elvin-Poole, J.Evrard, A. E.Fernandez, E.Ferté, A.Flaugher, B.Fosalba, P.Frieman, J.García-Bellido, J.Gaztanaga, E.Gerdes, D. W.Giannantonio, T.Gruen, D.Gruendl, R. A.Gschwend, J.Gutierrez, G.Hartley, W. G.Hollowood, D. L.Honscheid, K.Hoyle, B.Huterer, D.Jain, B.Jeltema, T.Johnson, M. W.G.Johnson, M. D.Kim, A. G.Krause, E.Kuehn, K.Kuropatkin, N.Lahav, O.Lee, S.Lemos, P.Leonard, C. D.Li, T. S.Liddle, A. R.Lima, M.Lin, H.Maia, M. A.G.Marshall, J. L.Martini, P.Menanteau, F.Miller, C. J.Miquel, R.Miranda, V.Mohr, J. J.Muir, J.Nichol, R. C.Nord, B.Ogando, R. L.C.Plazas, A. A.Raveri, M.Rollins, R. P.Romer, A. K.Roodman, A.Rosenfeld, R. [UNESP]Samuroff, S.Sanchez, E.Scarpine, V.Schindler, R.Schubnell, M.Scolnic, D.Secco, L. F.Serrano, S.Sevilla-Noarbe, I.Smith, M.Soares-Santos, M.Sobreira, F.Suchyta, E.Swanson, M. E.C.Tarle, G.Thomas, D.Troxel, M. A.Vikram, V.Walker, A. R.Weaverdyck, N.Wechsler, R. H.Weller, J.Yanny, B.Zhang, Y.Zuntz, J.2022-04-29T08:28:07Z2022-04-29T08:28:07Z2019-06-07info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.99.123505Physical Review D, v. 99, n. 12, 2019.2470-00292470-0010http://hdl.handle.net/11449/22870010.1103/PhysRevD.99.1235052-s2.0-85068989756Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2022-04-29T08:28:09Zoai:repositorio.unesp.br:11449/228700Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462022-04-29T08:28:09Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing |
title |
Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing |
spellingShingle |
Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing Abbott, T. M.C. |
title_short |
Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing |
title_full |
Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing |
title_fullStr |
Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing |
title_full_unstemmed |
Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing |
title_sort |
Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing |
author |
Abbott, T. M.C. |
author_facet |
Abbott, T. M.C. Abdalla, F. B. Avila, S. Banerji, M. Baxter, E. Bechtol, K. Becker, M. R. Bertin, E. Blazek, J. Bridle, S. L. Brooks, D. Brout, D. Burke, D. L. Campos, A. [UNESP] Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Castander, F. J. Cawthon, R. Chang, C. Chen, A. Crocce, M. Cunha, C. E. Da Costa, L. N. Davis, C. De Vicente, J. Derose, J. Desai, S. Di Valentino, E. Diehl, H. T. Dietrich, J. P. Dodelson, S. Doel, P. Drlica-Wagner, A. Eifler, T. F. Elvin-Poole, J. Evrard, A. E. Fernandez, E. Ferté, A. Flaugher, B. Fosalba, P. Frieman, J. García-Bellido, J. Gaztanaga, E. Gerdes, D. W. Giannantonio, T. Gruen, D. Gruendl, R. A. Gschwend, J. Gutierrez, G. Hartley, W. G. Hollowood, D. L. Honscheid, K. Hoyle, B. Huterer, D. Jain, B. Jeltema, T. Johnson, M. W.G. Johnson, M. D. Kim, A. G. Krause, E. Kuehn, K. Kuropatkin, N. Lahav, O. Lee, S. Lemos, P. Leonard, C. D. Li, T. S. Liddle, A. R. Lima, M. Lin, H. Maia, M. A.G. Marshall, J. L. Martini, P. Menanteau, F. Miller, C. J. Miquel, R. Miranda, V. Mohr, J. J. Muir, J. Nichol, R. C. Nord, B. Ogando, R. L.C. Plazas, A. A. Raveri, M. Rollins, R. P. Romer, A. K. Roodman, A. Rosenfeld, R. [UNESP] Samuroff, S. Sanchez, E. Scarpine, V. Schindler, R. Schubnell, M. Scolnic, D. Secco, L. F. Serrano, S. Sevilla-Noarbe, I. Smith, M. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M. E.C. Tarle, G. Thomas, D. Troxel, M. A. Vikram, V. Walker, A. R. Weaverdyck, N. Wechsler, R. H. Weller, J. Yanny, B. Zhang, Y. Zuntz, J. |
author_role |
author |
author2 |
Abdalla, F. B. Avila, S. Banerji, M. Baxter, E. Bechtol, K. Becker, M. R. Bertin, E. Blazek, J. Bridle, S. L. Brooks, D. Brout, D. Burke, D. L. Campos, A. [UNESP] Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Castander, F. J. Cawthon, R. Chang, C. Chen, A. Crocce, M. Cunha, C. E. Da Costa, L. N. Davis, C. De Vicente, J. Derose, J. Desai, S. Di Valentino, E. Diehl, H. T. Dietrich, J. P. Dodelson, S. Doel, P. Drlica-Wagner, A. Eifler, T. F. Elvin-Poole, J. Evrard, A. E. Fernandez, E. Ferté, A. Flaugher, B. Fosalba, P. Frieman, J. García-Bellido, J. Gaztanaga, E. Gerdes, D. W. Giannantonio, T. Gruen, D. Gruendl, R. A. Gschwend, J. Gutierrez, G. Hartley, W. G. Hollowood, D. L. Honscheid, K. Hoyle, B. Huterer, D. Jain, B. Jeltema, T. Johnson, M. W.G. Johnson, M. D. Kim, A. G. Krause, E. Kuehn, K. Kuropatkin, N. Lahav, O. Lee, S. Lemos, P. Leonard, C. D. Li, T. S. Liddle, A. R. Lima, M. Lin, H. Maia, M. A.G. Marshall, J. L. Martini, P. Menanteau, F. Miller, C. J. Miquel, R. Miranda, V. Mohr, J. J. Muir, J. Nichol, R. C. Nord, B. Ogando, R. L.C. Plazas, A. A. Raveri, M. Rollins, R. P. Romer, A. K. Roodman, A. Rosenfeld, R. [UNESP] Samuroff, S. Sanchez, E. Scarpine, V. Schindler, R. Schubnell, M. Scolnic, D. Secco, L. F. Serrano, S. Sevilla-Noarbe, I. Smith, M. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M. E.C. Tarle, G. Thomas, D. Troxel, M. A. Vikram, V. Walker, A. R. Weaverdyck, N. Wechsler, R. H. Weller, J. Yanny, B. Zhang, Y. Zuntz, J. |
author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
dc.contributor.none.fl_str_mv |
National Optical Astronomy Observatory University College London Rhodes University University of Portsmouth University of Cambridge University of Pennsylvania LSST Argonne National Laboratory Institut d'Astrophysique de Paris Ohio State University Observatoire de Sauverny University of Manchester Stanford University SLAC National Accelerator Laboratory Universidade Estadual Paulista (UNESP) Carnegie Mellon University Laboratório Interinstitucional de E-Astronomia - LIneA Observatório Nacional University of Illinois at Urbana-Champaign National Center for Supercomputing Applications Barcelona Institute of Science and Technology Institute of Space Sciences (ICE-CSIC) Institut d'Estudis Espacials de Catalunya (IEEC) University of Chicago University of Michigan Medioambientales y Tecnológicas (CIEMAT) 382 Via Pueblo Mall IIT Hyderabad Fermi National Accelerator Laboratory Excellence Cluster Universe Ludwig-Maximilians-Universität California Institute of Technology University of Edinburgh Oak Ridge National Laboratory Universidad Autonoma de Madrid Ludwig-Maximilians Universität München ETH Zurich Santa Cruz Institute for Particle Physics Max Planck Institute for Extraterrestrial Physics Lawrence Berkeley National Laboratory Australian Astronomical Observatory Universidade de São Paulo (USP) Texas AandM University Institució Catalana de Recerca i Estudis Avançats University of Sussex Universidade Estadual de Campinas (UNICAMP) University of Southampton Physics Department |
dc.contributor.author.fl_str_mv |
Abbott, T. M.C. Abdalla, F. B. Avila, S. Banerji, M. Baxter, E. Bechtol, K. Becker, M. R. Bertin, E. Blazek, J. Bridle, S. L. Brooks, D. Brout, D. Burke, D. L. Campos, A. [UNESP] Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Castander, F. J. Cawthon, R. Chang, C. Chen, A. Crocce, M. Cunha, C. E. Da Costa, L. N. Davis, C. De Vicente, J. Derose, J. Desai, S. Di Valentino, E. Diehl, H. T. Dietrich, J. P. Dodelson, S. Doel, P. Drlica-Wagner, A. Eifler, T. F. Elvin-Poole, J. Evrard, A. E. Fernandez, E. Ferté, A. Flaugher, B. Fosalba, P. Frieman, J. García-Bellido, J. Gaztanaga, E. Gerdes, D. W. Giannantonio, T. Gruen, D. Gruendl, R. A. Gschwend, J. Gutierrez, G. Hartley, W. G. Hollowood, D. L. Honscheid, K. Hoyle, B. Huterer, D. Jain, B. Jeltema, T. Johnson, M. W.G. Johnson, M. D. Kim, A. G. Krause, E. Kuehn, K. Kuropatkin, N. Lahav, O. Lee, S. Lemos, P. Leonard, C. D. Li, T. S. Liddle, A. R. Lima, M. Lin, H. Maia, M. A.G. Marshall, J. L. Martini, P. Menanteau, F. Miller, C. J. Miquel, R. Miranda, V. Mohr, J. J. Muir, J. Nichol, R. C. Nord, B. Ogando, R. L.C. Plazas, A. A. Raveri, M. Rollins, R. P. Romer, A. K. Roodman, A. Rosenfeld, R. [UNESP] Samuroff, S. Sanchez, E. Scarpine, V. Schindler, R. Schubnell, M. Scolnic, D. Secco, L. F. Serrano, S. Sevilla-Noarbe, I. Smith, M. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M. E.C. Tarle, G. Thomas, D. Troxel, M. A. Vikram, V. Walker, A. R. Weaverdyck, N. Wechsler, R. H. Weller, J. Yanny, B. Zhang, Y. Zuntz, J. |
description |
We present constraints on extensions of the minimal cosmological models dominated by dark matter and dark energy, ΛCDM and wCDM, by using a combined analysis of galaxy clustering and weak gravitational lensing from the first-year data of the Dark Energy Survey (DES Y1) in combination with external data. We consider four extensions of the minimal dark energy-dominated scenarios: (1) nonzero curvature ωk, (2) number of relativistic species Neff different from the standard value of 3.046, (3) time-varying equation-of-state of dark energy described by the parameters w0 and wa (alternatively quoted by the values at the pivot redshift, wp, and wa), and (4) modified gravity described by the parameters μ0 and ς0 that modify the metric potentials. We also consider external information from Planck cosmic microwave background measurements; baryon acoustic oscillation measurements from SDSS, 6dF, and BOSS; redshift-space distortion measurements from BOSS; and type Ia supernova information from the Pantheon compilation of datasets. Constraints on curvature and the number of relativistic species are dominated by the external data; when these are combined with DES Y1, we find ωk=0.0020-0.0032+0.0037 at the 68% confidence level, and the upper limit Neff<3.28(3.55) at 68% (95%) confidence, assuming a hard prior Neff>3.0. For the time-varying equation-of-state, we find the pivot value (wp,wa)=(-0.91-0.23+0.19,-0.57-1.11+0.93) at pivot redshift zp=0.27 from DES alone, and (wp,wa)=(-1.01-0.04+0.04,-0.28-0.48+0.37) at zp=0.20 from DES Y1 combined with external data; in either case we find no evidence for the temporal variation of the equation of state. For modified gravity, we find the present-day value of the relevant parameters to be ς0=0.43-0.29+0.28 from DES Y1 alone, and (ς0,μ0)=(0.06-0.07+0.08,-0.11-0.46+0.42) from DES Y1 combined with external data. These modified-gravity constraints are consistent with predictions from general relativity. |
publishDate |
2019 |
dc.date.none.fl_str_mv |
2019-06-07 2022-04-29T08:28:07Z 2022-04-29T08:28:07Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1103/PhysRevD.99.123505 Physical Review D, v. 99, n. 12, 2019. 2470-0029 2470-0010 http://hdl.handle.net/11449/228700 10.1103/PhysRevD.99.123505 2-s2.0-85068989756 |
url |
http://dx.doi.org/10.1103/PhysRevD.99.123505 http://hdl.handle.net/11449/228700 |
identifier_str_mv |
Physical Review D, v. 99, n. 12, 2019. 2470-0029 2470-0010 10.1103/PhysRevD.99.123505 2-s2.0-85068989756 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review D |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1799965597006561280 |