Hyper Suprime-Cam Year 3 results: Cosmology from cosmic shear two-point correlation functions
Xiangchong LiKavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study (UTIAS), The University of Tokyo, Chiba 277-8583, JapanTianqing ZhangMcWilliams Center for Cosmology, Department of Physics, Carnegie Mellon University, 5000 Forbes Avenue, Pittsburgh, Pennsylvania 15213, USASunao SugiyamaDepartment of Physics, The University of Tokyo, Bunkyo, Tokyo 113-0031, JapanRoohi DalalDepartment of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USARyo TerasawaDepartment of Physics, The University of Tokyo, Bunkyo, Tokyo 113-0031, JapanMarkus Michael RauHigh Energy Physics Division, Argonne National Laboratory, Lemont, Illinois 60439, USARachel MandelbaumMcWilliams Center for Cosmology, Department of Physics, Carnegie Mellon University, 5000 Forbes Avenue, Pittsburgh, Pennsylvania 15213, USAMasahiro TakadaKavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study (UTIAS), The University of Tokyo, Chiba 277-8583, JapanSurhud MoreKavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study (UTIAS), The University of Tokyo, Chiba 277-8583, JapanMichael A. StraussDepartment of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USAHironao MiyatakeInstitute for Advanced Research, Nagoya University, Nagoya 464-8601, JapanMasato ShirasakiNational Astronomical Observatory of Japan, National Institutes of Natural Sciences, Mitaka, Tokyo 181-8588, JapanTakashi HamanaNational Astronomical Observatory of Japan, National Institutes of Natural Sciences, Mitaka, Tokyo 181-8588, JapanMasamune OguriCenter for Frontier Science, Chiba University, 1-33 Yayoi-cho, Inage-ku, Chiba 263-8522, JapanWentao LuoCAS Key Laboratory for Researches in Galaxies and Cosmology/Department of Astronomy, School of Astronomy and Space Science, University of Science and Technology of China, Hefei, Anhui 230026, ChinaAtsushi J. NishizawaGifu Shotoku Gakuen University, Gifu 501-6194, JapanRyuichi TakahashiFaculty of Science and Technology, Hirosaki University, 3 Bunkyo-cho, Hirosaki, Aomori 036-8561, JapanAndrina NicolaArgelander Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, GermanyKen OsatoCenter for Frontier Science, Chiba University, 1-33 Yayoi-cho, Inage-ku, Chiba 263-8522, JapanArun KannawadiDepartment of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USATomomi SunayamaDepartment of Astronomy and Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85719, USAR. ArmstrongLawrence Livermore National Laboratory, Livermore, California 94551, USAJames BoschDepartment of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USAYutaka KomiyamaDepartment of Advanced Sciences, Faculty of Science and Engineering, Hosei University, 3-7-2 Kajino-cho, Koganei-shi, Tokyo 184-8584, JapanRobert H. LuptonDepartment of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USANate B. LustDepartment of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USALauren A. MacArthurDepartment of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USASatoshi MiyazakiSubaru Telescope, National Astronomical Observatory of Japan, 650 North Aohoku Place Hilo, Hawaii 96720, USAHitoshi MurayamaBerkeley Center for Theoretical Physics, University of California, Berkeley, California 94720, USATakahiro NishimichiCenter for Gravitational Physics and Quantum Information, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, JapanYuki OkuraNational Astronomical Observatory of Japan, National Institutes of Natural Sciences, Mitaka, Tokyo 181-8588, JapanP. A. PriceDepartment of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USAPhilip J. TaitSubaru Telescope, National Astronomical Observatory of Japan, 650 North Aohoku Place Hilo, Hawaii 96720, USAMasayuki TanakaNational Astronomical Observatory of Japan, National Institutes of Natural Sciences, Mitaka, Tokyo 181-8588, JapanShiang‐Yu WangInstitute of Astronomy and Astrophysics, Academia Sinica, Taipei 10617, Taiwan
2023en
ABI
Abstract
A new analysis of the distribution of matter in the Universe continues to find a discrepancy in the clumpiness of dark matter in the late and early Universe, suggesting a fundamental error in the standard cosmological model.
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