Light dark matter: A common solution to the lithium and H0 problems
Currently, the standard cosmological model faces some tensions and discrepancies between observations at early and late cosmological time. One of them concerns the well-known H0-tension problem, i.e., a ∼4.4σ-difference between the early-time estimate and late-time measurements of the Hubble constan...
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| Published in | Physics letters. B Vol. 812; p. 136008 |
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| Main Authors | , , , |
| Format | Journal Article |
| Language | English |
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Elsevier B.V
10.01.2021
Elsevier |
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| Abstract | Currently, the standard cosmological model faces some tensions and discrepancies between observations at early and late cosmological time. One of them concerns the well-known H0-tension problem, i.e., a ∼4.4σ-difference between the early-time estimate and late-time measurements of the Hubble constant, H0. Another puzzling question rests in the cosmological lithium abundance, where again local measurements differ from the one predicted by Big Bang Nucleosynthesis (BBN). In this work, we show that a mechanism of light dark matter production might hold the answer for these questions. If dark matter particles are sufficiently light and a fraction of them were produced non-thermally in association with photons, this mechanism has precisely what is needed to destroy Lithium without spoiling other BBN predictions. Besides, it produces enough radiation that leads to a larger H0 value, reconciling early and late-time measurements of the Hubble expansion rate without leaving sizable spectral distortions in the Cosmic Microwave Background spectrum. |
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| AbstractList | Currently, the standard cosmological model faces some tensions and discrepancies between observations at early and late cosmological time. One of them concerns the well-known H0-tension problem, i.e., a ∼4.4σ-difference between the early-time estimate and late-time measurements of the Hubble constant, H0. Another puzzling question rests in the cosmological lithium abundance, where again local measurements differ from the one predicted by Big Bang Nucleosynthesis (BBN). In this work, we show that a mechanism of light dark matter production might hold the answer for these questions. If dark matter particles are sufficiently light and a fraction of them were produced non-thermally in association with photons, this mechanism has precisely what is needed to destroy Lithium without spoiling other BBN predictions. Besides, it produces enough radiation that leads to a larger H0 value, reconciling early and late-time measurements of the Hubble expansion rate without leaving sizable spectral distortions in the Cosmic Microwave Background spectrum. |
| ArticleNumber | 136008 |
| Author | Masiero, Antonio Alcaniz, Jailson Bernal, Nicolás Queiroz, Farinaldo S. |
| Author_xml | – sequence: 1 givenname: Jailson surname: Alcaniz fullname: Alcaniz, Jailson email: alcaniz@on.br organization: Observatório Nacional, 20921-400, Rio de Janeiro, RJ, Brazil – sequence: 2 givenname: Nicolás surname: Bernal fullname: Bernal, Nicolás email: nicolas.bernal@uan.edu.co organization: Centro de Investigaciones, Universidad Antonio Nariño, Bogotá, Colombia – sequence: 3 givenname: Antonio surname: Masiero fullname: Masiero, Antonio email: antonio.masiero@pd.infn.it organization: Dipartimento di Fisica e Astronomia “G. Galilei”, Universita di Padova, Italy – sequence: 4 givenname: Farinaldo S. orcidid: 0000-0002-7141-5532 surname: Queiroz fullname: Queiroz, Farinaldo S. email: farinaldo.queiroz@iip.ufrn.br organization: International Institute of Physics, Universidade Federal do Rio Grande do Norte, Campus Universitário, Lagoa Nova, Natal-RN 59078-970, Brazil |
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| Title | Light dark matter: A common solution to the lithium and H0 problems |
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