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Exploring cosmic origins with CORE: Cosmological parameters

机译:探索宇宙起源与核心:宇宙学参数

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We forecast the main cosmological parameter constraints achievable with the CORE space mission which is dedicated to mapping the polarisation of the Cosmic Mi-crowave Background (CMB). CORE was recently submitted in response to ESA's ?fth call for medium-sized mission proposals (M5). Here we report the results from our pre-submission study of the impact of various instrumental options, in particular the telescope size and sensitivity level, and review the great, transformative potential of the mission as proposed. Speci?cally, we assess the impact on a broad range of fundamental parameters of our Universe as a function of the expected CMB characteristics, with other papers in the series focusing on controlling astrophysical and instrumental residual systematics. In this paper, we assume that only a few central CORE frequency channels are usable for our purpose, all others being devoted to the cleaning of astrophysical contaminants. On the theoretical side, we assume ΛCDM as our general framework and quantify the improvement provided by CORE over the current constraints from the Planck 2015 release. We also study the joint sensitivity of CORE and of future Baryon Acoustic Oscillation and Large Scale Structure experiments like DESI and Euclid. Speci?c constraints on the physics of in?ation are presented in another paper of the series. In addition to the six parameters of the base ΛCDM, which describe the matter content of a spatially ?at universe with adiabatic and scalar primordial ?uctua-tions from in?ation, we derive the precision achievable on parameters like those describing curvature, neutrino physics, extra light relics, primordial helium abundance, dark matter an-nihilation, recombination physics, variation of fundamental constants, dark energy, modi?ed gravity, reionization and cosmic birefringence. In addition to assessing the improvement on the precision of individual parameters, we also forecast the post-CORE overall reduction of the allowed parameter sp
机译:我们预测具有核心空间特派团可实现的主要宇宙学参数约束,该特性专用于映射宇宙MI-荷图背景(CMB)的极化。核心最近是回应ESA的?FTH呼吁中型特派团提案(M5)。在这里,我们从提交预先提交研究结果报告了各种乐器选择的影响,特别是望远镜尺寸和敏感水平,并审查了所提出的使命的伟大变革潜力。具体而言,我们根据预期的CMB特性,评估对我们宇宙广泛的基本参数的影响,其中卷中的其他纸张专注于控制天体物理和仪器残留的系统。在本文中,我们假设只有少数核心核心频率频率可以用于我们的目的,所有其他人都致力于清洁天体物理污染物。在理论方面,我们假设λcdm作为我们的总体框架,并通过普朗克2015释放的当前约束来量化核心提供的改进。我们还研究了核心和未来的Baryon声学振荡和大规模结构实验的联合敏感性,如Desi和Euclid。对In的物理学的限制在该系列的另一种纸上呈现。除了基础λcdm的六个参数之外,它还描述了空间的物质含量?在宇宙中的绝热和标量原始的?uctua-tions from in?aion,我们从描述曲率,中微子物理学的参数上获得的精确度,额外的韵律,原始氦气丰富,暗物质,重组物理,基本常数的变异,黑能量,modi?Ed重力,标准化和宇宙双折射。除了评估各个参数精度的改进外,我们还预测允许参数SP的后核整体减少

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  • 作者单位

    Institut d'Astrophysique de Paris (UMR7095: CNRS &

    UPMC-Sorbonne Universités) F-75014 Paris France;

    Institut d'Astrophysique de Paris (UMR7095: CNRS &

    UPMC-Sorbonne Universités) F-75014 Paris France;

    The Oskar Klein Centre for Cosmoparticle Physics Department of Physics Stockholm University AlbaNova SE-106 91 Stockholm Sweden;

    Institute for Theoretical Particle Physics and Cosmology (TTK) RWTH Aachen University D-52056 Aachen Germany;

    Institut d'Astrophysique de Paris (UMR7095: CNRS &

    UPMC-Sorbonne Universités) F-75014 Paris France;

    Institute for Theoretical Particle Physics and Cosmology (TTK) RWTH Aachen University D-52056 Aachen Germany;

    Physics Department and Sezione INFN Università di Roma "La Sapienza" Piazzale Aldo Moro 2 00185 Rome Italy;

    Jodrell Bank Centre for Astrophysics School of Physics and Astronomy The University of Manchester Oxford Road Manchester M13 9PL U.K.;

    Institute for Theoretical Particle Physics and Cosmology (TTK) RWTH Aachen University D-52056 Aachen Germany;

    APC AstroParticule et Cosmologie Université Paris Diderot CNRS/IN2P3 CEA/Irfu Observatoire de Paris Sorbonne Paris Cité 10 rue Alice Domon et Leonie Duquet 75205 Paris Cedex 13 France;

    Department of Physics Harvard University Cambridge MA 02138 U.S.A.;

    Dipartimento di Fisica e Scienze della Terra Università degli Studi di Ferrara Via Giuseppe Saragat 1 44122 Ferrara Italy;

    Institut d'Astrophysique de Paris (UMR7095: CNRS &

    UPMC-Sorbonne Universités) F-75014 Paris France;

    Institute for Theoretical Particle Physics and Cosmology (TTK) RWTH Aachen University D-52056 Aachen Germany;

    Dipartimento di Fisica e Scienze della Terra Università degli Studi di Ferrara Via Giuseppe Saragat 1 44122 Ferrara Italy;

    Centro de Astrofísica da Universidade do Porto and IA-Porto Rua das Estrelas 4150-762 Porto Portugal;

    Physics Department and Sezione INFN Università di Roma "La Sapienza" Piazzale Aldo Moro 2 00185 Rome Italy;

    Physics Department and Sezione INFN Università di Roma "La Sapienza" Piazzale Aldo Moro 2 00185 Rome Italy;

    Physics Department and Sezione INFN Università di Roma "La Sapienza" Piazzale Aldo Moro 2 00185 Rome Italy;

    McWilliams Center for Cosmology Department of Physics Carnegie Mellon University Pittsburgh PA 15213 U.S.A.;

    Institut d'Astrophysique de Paris (UMR7095: CNRS &

    UPMC-Sorbonne Universités) F-75014 Paris France;

    Dipartimento di Fisica e Scienze della Terra Università degli Studi di Ferrara Via Giuseppe Saragat 1 44122 Ferrara Italy;

    Institut d'Astrophysique Spatiale CNRS Univ. Paris-Sud University Paris-Saclay. 121 91405 Orsay cedex France;

    McWilliams Center for Cosmology Department of Physics Carnegie Mellon University Pittsburgh PA 15213 U.S.A.;

    Instituto de Astrofísica de Canarias C/Vía Láctea s/n La Laguna Tenerife Spain;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 宇宙学;天体物理学;
  • 关键词

    cosmological parameters from CMBR; CMBR experiments; neutrino masses from cosmology;

    机译:来自CMBR的宇宙学参数;CMBR实验;来自宇宙学的中微子群众;

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