Revealing the effects of curvature on the cosmological models

被引:21
作者
Yang, Weiqiang [1 ]
Giare, William [2 ,3 ]
Pan, Supriya [4 ,5 ]
Di Valentino, Eleonora [6 ]
Melchiorri, Alessandro [7 ,8 ]
Silk, Joseph [9 ,10 ,11 ,12 ]
机构
[1] Liaoning Normal Univ, Dept Phys, Dalian 116029, Peoples R China
[2] Ctr Nazl INFN Studi Avanzati, Galileo Galilei Inst Theoret Phys, Largo Enrico Fermi 2, I-50125 Florence, Italy
[3] Ist Nazl Fis Nucl, Sez Roma, Ple A Moro 2, I-00185 Rome, Italy
[4] Presidency Univ, Dept Math, 86-1 Coll St, Kolkata 700073, India
[5] Durban Univ Technol, Inst Syst Sci, POB 1334, ZA-4000 Durban, South Africa
[6] Univ Sheffield, Sch Math & Stat, Hounsfield Rd, Sheffield S3 7RH, England
[7] Univ Roma La Sapienza, Phys Dept, Ple Aldo Moro 2, I-00185 Rome, Italy
[8] Univ Roma La Sapienza, INFN, Ple Aldo Moro 2, I-00185 Rome, Italy
[9] CNRS, Inst Astrophys Paris, UMR7095, F-75014 Paris, France
[10] UPMC, Sorbonne Univ, F-75014 Paris, France
[11] Johns Hopkins Univ, Dept Phys & Astron, Homewood Campus, Baltimore, MD 21218 USA
[12] Univ Oxford, Dept Phys, BIPAC, Keble Rd, Oxford OX1 3RH, England
基金
中国国家自然科学基金;
关键词
DYNAMICAL DARK ENERGY; HUBBLE CONSTANT; CONSTRAINTS; GALAXY; H-0; OSCILLATION; TENSIONS; RELEASE;
D O I
10.1103/PhysRevD.107.063509
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we consider the effects of adding curvature in extended cosmologies involving a free-tovary neutrino sector and different parametrizations of dark energy (DE). We make use of the Planck 2018 cosmic microwave background temperature and polarization data, baryon acoustic oscillations and Pantheon type Ia supernovae data. Our main result is that a nonflat Universe cannot be discarded in light of the current astronomical data, because we find an indication for a closed Universe in most of the DE cosmologies explored in this work. On the other hand, forcing the Universe to be flat can significantly bias the constraints on the equation of state of the DE component and its dynamical nature.
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页数:40
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共 138 条
  • [1] Abbott DTMC, 2023, Arxiv, DOI [arXiv:2207.05766, DOI 10.30919/ESMM5-766, 10.48550/arXiv.2207.05766]
  • [2] Abdalla Elcio, 2022, JOURNAL OF HIGH ENERGY ASTROPHYSICS, V34, P49, DOI DOI 10.1016/J.JHEAP.2022.04.002
  • [3] Abell P. A., arXiv
  • [4] Implications of the S8 tension for decaying dark matter with warm decay products
    Abellan, Guillermo F.
    Murgia, Riccardo
    Poulin, Vivian
    Lavalle, Julien
    [J]. PHYSICAL REVIEW D, 2022, 105 (06)
  • [5] Abitbol Maximilian H., 2019, Bull. Am. Astron. Soc., V51, P147
  • [6] Simple-graduated dark energy and spatial curvature
    Acquaviva, Giovanni
    Akarsu, Ozgur
    Katirci, Nihan
    Vazquez, J. Alberto
    [J]. PHYSICAL REVIEW D, 2021, 104 (02)
  • [7] The Simons Observatory: science goals and forecasts
    Ade, Peter
    Aguirre, James
    Ahmed, Zeeshan
    Aiola, Simone
    Ali, Aamir
    Alonso, David
    Alvarez, Marcelo A.
    Arnold, Kam
    Ashton, Peter
    Austermann, Jason
    Awan, Humna
    Baccigalupi, Carlo
    Baildon, Taylor
    Barron, Darcy
    Battaglia, Nick
    Battye, Richard
    Baxter, Eric
    Bazarko, Andrew
    Beall, James A.
    Bean, Rachel
    Beck, Dominic
    Beckman, Shawn
    Beringue, Benjamin
    Bianchini, Federico
    Boada, Steven
    Boettger, David
    Bond, J. Richard
    Borrill, Julian
    Brown, Michael L.
    Bruno, Sarah Marie
    Bryan, Sean
    Calabrese, Erminia
    Calafut, Victoria
    Calisse, Paolo
    Carron, Julien
    Challinor, Anthony
    Chesmore, Grace
    Chinone, Yuji
    Chluba, Jens
    Cho, Hsiao-Mei Sherry
    Choi, Steve
    Coppi, Gabriele
    Cothard, Nicholas F.
    Coughlin, Kevin
    Crichton, Devin
    Crowley, Kevin D.
    Crowley, Kevin T.
    Cukierman, Ari
    D'Ewart, John M.
    Dunner, Rolando
    [J]. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2019, (02):
  • [8] Planck 2018 results: VI. Cosmological parameters
    Aghanim, N.
    Akrami, Y.
    Ashdown, M.
    Aumont, J.
    Baccigalupi, C.
    Ballardini, M.
    Banday, A. J.
    Barreiro, R. B.
    Bartolo, N.
    Basak, S.
    Battye, R.
    Benabed, K.
    Bernard, J. -P.
    Bersanelli, M.
    Bielewicz, P.
    Bock, J. J.
    Bond, J. R.
    Borrill, J.
    Bouchet, F. R.
    Boulanger, F.
    Bucher, M.
    Burigana, C.
    Butler, R. C.
    Calabrese, E.
    Cardoso, J. -F.
    Carron, J.
    Challinor, A.
    Chiang, H. C.
    Chluba, J.
    Colombo, L. P. L.
    Combet, C.
    Contreras, D.
    Crill, B. P.
    Cuttaia, F.
    de Bernardis, P.
    de Zotti, G.
    Delabrouille, J.
    Delouis, J. -M.
    Di Valentino, E.
    Diego, J. M.
    Dore, O.
    Douspis, M.
    Ducout, A.
    Dupac, X.
    Dusini, S.
    Efstathiou, G.
    Elsner, F.
    Ensslin, T. A.
    Eriksen, H. K.
    Fantaye, Y.
    [J]. ASTRONOMY & ASTROPHYSICS, 2020, 641
  • [9] Planck 2018 results: V. CMB power spectra and likelihoods
    Aghanim, N.
    Akrami, Y.
    Ashdown, M.
    Aumont, J.
    Baccigalupi, C.
    Ballardini, M.
    Banday, A. J.
    Barreiro, R. B.
    Bartolo, N.
    Basak, S.
    Benabed, K.
    Bernard, J. -P.
    Bersanelli, M.
    Bielewicz, P.
    Bock, J. J.
    Bond, J. R.
    Borrill, J.
    Bouchet, F. R.
    Boulanger, F.
    Bucher, M.
    Burigana, C.
    Butler, R. C.
    Calabrese, E.
    Cardoso, J. -F.
    Carron, J.
    Casaponsa, B.
    Challinor, A.
    Chiang, H. C.
    Colombo, L. P. L.
    Combet, C.
    Crill, B. P.
    Cuttaia, F.
    de Bernardis, P.
    de Rosa, A.
    de Zotti, G.
    Delabrouille, J.
    Delouis, J. -M.
    Di Valentino, E.
    Diego, J. M.
    Dore, O.
    Douspis, M.
    Ducout, A.
    Dupac, X.
    Dusini, S.
    Efstathiou, G.
    Elsner, F.
    Ensslin, T. A.
    Eriksen, H. K.
    Fantaye, Y.
    Fernandez-Cobos, R.
    [J]. ASTRONOMY & ASTROPHYSICS, 2020, 641
  • [10] A precision calculation of relic neutrino decoupling
    Akita, Kensuke
    Yamaguchi, Masahide
    [J]. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2020, (08):