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Cosmic shear, galaxy clustering, and the abundance of massive halos each probe the large-scale structure of the Universe in complementary ways. We present cosmological constraints from the joint analysis of the three probes, building on the…

宇宙学与河外天体物理 · 物理学 2025-03-14 S. Bocquet , S. Grandis , E. Krause , C. To , L. E. Bleem , M. Klein , J. J. Mohr , T. Schrabback , A. Alarcon , O. Alves , A. Amon , F. Andrade-Oliveira , E. J. Baxter , K. Bechtol , M. R. Becker , G. M. Bernstein , J. Blazek , H. Camacho , A. Campos , A. Carnero Rosell , M. Carrasco Kind , R. Cawthon , C. Chang , R. Chen , A. Choi , J. Cordero , M. Crocce , C. Davis , J. DeRose , H. T. Diehl , S. Dodelson , C. Doux , A. Drlica-Wagner , K. Eckert , T. F. Eifler , F. Elsner , J. Elvin-Poole , S. Everett , X. Fang , A. Ferté , P. Fosalba , O. Friedrich , J. Frieman , M. Gatti , G. Giannini , D. Gruen , R. A. Gruendl , I. Harrison , W. G. Hartley , K. Herner , H. Huang , E. M. Huff , D. Huterer , M. Jarvis , N. Kuropatkin , P. -F. Leget , P. Lemos , A. R. Liddle , N. MacCrann , J. McCullough , J. Muir , J. Myles , A. Navarro-Alsina , S. Pandey , Y. Park , A. Porredon , J. Prat , M. Raveri , R. P. Rollins , A. Roodman , R. Rosenfeld , E. S. Rykoff , C. Sánchez , J. Sanchez , L. F. Secco , I. Sevilla-Noarbe , E. Sheldon , T. Shin , M. A. Troxel , I. Tutusaus , T. N. Varga , N. Weaverdyck , R. H. Wechsler , H. -Y. Wu , B. Yanny , B. Yin , Y. Zhang , J. Zuntz , T. M. C. Abbott , P. A. R. Ade , M. Aguena , S. Allam , S. W. Allen , A. J. Anderson , B. Ansarinejad , J. E. Austermann , M. Bayliss , J. A. Beall , A. N. Bender , B. A. Benson , F. Bianchini , M. Brodwin , D. Brooks , L. Bryant , D. L. Burke , R. E. A. Canning , J. E. Carlstrom , J. Carretero , F. J. Castander , C. L. Chang , P. Chaubal , H. C. Chiang , T-L. Chou , R. Citron , C. Corbett Moran , M. Costanzi , T. M. Crawford , A. T. Crites , L. N. da Costa , M. E. S. Pereira , T. M. Davis , T. de Haan , M. A. Dobbs , P. Doel , W. Everett , A. Farahi , B. Flaugher , A. M. Flores , B. Floyd , J. Gallicchio , E. Gaztanaga , E. M. George , M. D. Gladders , N. Gupta , G. Gutierrez , N. W. Halverson , S. R. Hinton , J. Hlavacek-Larrondo , G. P. Holder , D. L. Hollowood , W. L. Holzapfel , J. D. Hrubes , N. Huang , J. Hubmayr , K. D. Irwin , D. J. James , F. Kéruzoré , G. Khullar , K. Kim , L. Knox , R. Kraft , K. Kuehn , O. Lahav , A. T. Lee , S. Lee , D. Li , C. Lidman , M. Lima , A. Lowitz , G. Mahler , A. Mantz , J. L. Marshall , M. McDonald , J. J. McMahon , J. Mena-Fernández , S. S. Meyer , R. Miquel , J. Montgomery , T. Natoli , J. P. Nibarger , G. I. Noble , V. Novosad , R. L. C. Ogando , S. Padin , P. Paschos , S. Patil , A. A. Plazas Malagón , C. Pryke , C. L. Reichardt , J. Roberson , A. K. Romer , C. Romero , J. E. Ruhl , B. R. Saliwanchik , L. Salvati , S. Samuroff , E. Sanchez , B. Santiago , A. Sarkar , A. Saro , K. K. Schaffer , K. Sharon , C. Sievers , G. Smecher , M. Smith , T. Somboonpanyakul , M. Sommer , B. Stalder , A. A. Stark , J. Stephen , V. Strazzullo , E. Suchyta , M. E. C. Swanson , G. Tarle , D. Thomas , C. Tucker , D. L. Tucker , T. Veach , J. D. Vieira , A. von der Linden , G. Wang , N. Whitehorn , W. L. K. Wu , V. Yefremenko , M. Young , J. A. Zebrowski , H. Zohren , DES Collaboration , SPT Collaboration

We derive new constraints on the neutron lifetime based on the recent Planck 2015 observations of temperature and polarization anisotropies of the CMB. Under the assumption of standard Big Bang Nucleosynthesis, we show that Planck data…

宇宙学与河外天体物理 · 物理学 2016-04-05 Laura Salvati , Luca Pagano , Rosa Consiglio , Alessandro Melchiorri

We present the CMB anisotropy induced by the non-linear perturbations in the massive neutrino density associated to the non-linear gravitational clustering. We show that the non-linear time varying potential induced by the gravitational…

天体物理学 · 物理学 2007-05-23 L. A. Popa , C. Burigana , N. Mandolesi

Distortions of CMB temperature and polarization anisotropy maps caused by gravitational lensing, observable with high angular resolution and sensitivity, can be used to constrain the sterile neutrino mass, offering several advantages…

天体物理学 · 物理学 2009-06-23 L. A. Popa , A. Vasile

The recent measurements of the Cosmic Microwave Background Anisotropies provided by the Planck satellite experiment have significantly improved the constraints on several cosmological parameters. In this brief paper we point out a small but…

宇宙学与河外天体物理 · 物理学 2015-06-23 Laura Salvati , Najla Said , Alessandro Melchiorri

We present the results of analysis of constraints on cosmological parameters from cosmic microwave background (CMB) alone and in combination with galaxy cluster baryon fraction assuming inflation--generated adiabatic scalar fluctuations.…

天体物理学 · 物理学 2009-11-06 M. Douspis , A. Blanchard , R. Sadat , J. G. Bartlett , M. Le Dour

We investigate the potential of observations of anisotropies in the cosmic microwave background (CMB) and large-scale structure in the Universe to detect possible modifications of standard inflationary models by physics beyond the Planck…

天体物理学 · 物理学 2009-11-10 Oystein Elgaroy , Steen Hannestad

In the past years 'quintessence' models have been considered which can produce the accelerated expansion in the universe suggested by recent astronomical observations. One of the key differences between quintessence and a cosmological…

天体物理学 · 物理学 2014-10-13 Rachel Bean , Steen H. Hansen , Alessandro Melchiorri

We consider the distribution of the non-Gaussian signal induced by weak lensing on the primary total intensity cosmic microwave background (CMB) anisotropies. Our study focuses on the three point statistics exploiting an harmonic analysis…

天体物理学 · 物理学 2009-11-10 Fabio Giovi , Carlo Baccigalupi , Francesca Perrotta

We studied a constraint on the primordial helium abundance Y_p from current and future observations of CMB. Using the currently available data from WMAP, ACBAR, CBI and BOOMERANG, we obtained the constraint as Y_p = 0.25^{+0.10}_{-0.07} at…

天体物理学 · 物理学 2008-11-26 Kazuhide Ichikawa , Toyokazu Sekiguchi , Tomo Takahashi

Primordial gravitational waves (GWs) with frequencies > 10^{-15} Hz contribute to the radiation density of the Universe at the time of decoupling of the cosmic microwave background (CMB). The effects of this GW background on the CMB and…

天体物理学 · 物理学 2009-11-11 Tristan L. Smith , Elena Pierpaoli , Marc Kamionkowski

A critical review is given of the current status of cosmological nucleosynthesis. In the framework of the Standard Model with 3 types of relativistic neutrinos, the baryon-to-photon ratio, $\eta$, corresponding to the inferred primordial…

天体物理学 · 物理学 2011-02-09 Brian Fields , Subir Sarkar

We study constraints on time variation of the fine structure constant alpha from cosmic microwave background (CMB) taking into account simultaneous change in alpha and the electron mass m_e which might be implied in unification theories. We…

天体物理学 · 物理学 2008-11-26 Kazuhide Ichikawa , Toru Kanzaki , Masahiro Kawasaki

We consider the case of a coupling in the dark cosmological sector, where a dark energy scalar field modifies the gravitational attraction between dark matter particles. We find that the strength of the coupling {\beta} is constrained using…

宇宙学与河外天体物理 · 物理学 2013-05-30 Valeria Pettorino , Luca Amendola , Carlo Baccigalupi , Claudia Quercellini

Primordial nucleosynthesis provides a probe of the universal abundance of baryons when the universe was only a few minutes old. Recent observations of anisotropy in the cosmic microwave background (CMB) probe the baryon abundance when the…

天体物理学 · 物理学 2007-05-23 G. Steigman , J. P. Kneller , A. Zentner

We present constraints on the cosmic growth history with recent cosmological data, allowing for deviations from Lambda CDM as might arise if cosmic acceleration is due to modifications to GR or inhomogeneous dark energy. We combine measures…

宇宙学与河外天体物理 · 物理学 2010-05-12 Rachel Bean , Matipon Tangmatitham

The standard $\Lambda$CDM cosmological model informed by cosmic microwave background (CMB) anisotropies makes a precise prediction for the growth of matter density fluctuations over cosmic time on linear scales. A variety of cosmological…

宇宙学与河外天体物理 · 物理学 2024-11-14 Mathew S. Madhavacheril

We extend our recent work on the effects of a time-varying fine-structure constant $\alpha$ in the cosmic microwave background, by providing a thorough analysis of the degeneracies between $\alpha$ and the other cosmological parameters, and…

天体物理学 · 物理学 2008-11-26 C. J. A. P. Martins , A. Melchiorri , R. Trotta , R. Bean , G. Rocha , P. P. Avelino , P. T. P. Viana

We study Planck 2015 cosmic microwave background (CMB) anisotropy data using the energy density inhomogeneity power spectrum generated by quantum fluctuations during an early epoch of inflation in the non-flat XCDM model. Here dark energy…

宇宙学与河外天体物理 · 物理学 2018-12-19 Junpei Ooba , Bharat Ratra , Naoshi Sugiyama

A critical review is given of the current status of cosmological nucleosynthesis. In the framework of the Standard Model with 3 types of relativistic neutrinos, the baryon-to-photon ratio, $\eta$, corresponding to the inferred primordial…

宇宙学与河外天体物理 · 物理学 2015-06-23 Brian D. Fields , Paolo Molaro , Subir Sarkar