The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe

It is commonly assumed that the energy density of the Universe was dominated by radiation between reheating after inflation and the onset of matter domination 54,000 years later. While the abundance of light elements indicates that the Universe was radiation dominated during Big Bang Nucleosynthesis...

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Published inThe open journal of astrophysics Vol. 4; no. 1
Main Authors Allahverdi, Rouzbeh, Amin, Mustafa A., Berlin, Asher, Bernal, Nicholas, Byrnes, Christian T., Delos, M. Sten, Erickcek, Adrienne L., Escudero, Miguel, Figueroa, Daniel G., Freese, Katherine, Harada, Tomohiro, Hooper, Dan, Kaiser, David I., Karwal, Tanvi, Kohri, Kazunori, Krnjaci, Gordan, Lewicki, Marek, Lozanov, Kaloian D., Poulin, Vivian, Sinha, Kuver, Smith, Tristan L., Takahashi, Tomo, Tenkanen, Tommi, Unwin, James, Watson, Scottname>
Format Journal Article
LanguageEnglish
Published United States Maynooth Academic Publishing 2021
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Summary:It is commonly assumed that the energy density of the Universe was dominated by radiation between reheating after inflation and the onset of matter domination 54,000 years later. While the abundance of light elements indicates that the Universe was radiation dominated during Big Bang Nucleosynthesis (BBN), there is scant evidence that the Universe was radiation dominated prior to BBN. It is therefore possible that the cosmological history was more complicated, with deviations from the standard radiation domination during the earliest epochs. Indeed, several interesting proposals regarding various topics such as the generation of dark matter, matter-antimatter asymmetry, gravitational waves, primordial black holes, or microhalos during a nonstandard expansion phase have been recently made. In this paper, we review various possible causes and consequences of deviations from radiation domination in the early Universe - taking place either before or after BBN - and the constraints on them, as they have been discussed in the literature during the recent years.
Bibliography:National Aeronautics and Space Administration (NASA)
Science and Technology Facilities Council (STFC)
Simons Foundation
Fondo Nacional de Financiamiento para la Ciencia, la Tecnologia y la Innovacion (MinCiencias)
Estonian Research Council
Ministry of Economic Affairs and Digital Transformation of Spain (MINECO)
Research Corporation
Swedish Research Council (VR)
National Science Foundation (NSF)
Royal Society
Japan Society for the Promotion of Science (JSPS)
AC02-07CH11359; PHY-1720174; 80NSSC20K0518; 2018204; 2019101; 2019248; FPA2017-84543-P; 80740-465-2020; 860881-HIDDeN; PHY-1752752; 648680 DARKHORIZONS; RYC-2017-23493; SC007859; 638-2013-8993; JP19K03876; JP19H01895; ST/P000258/1; 2018/31/D/ST2/02048; SC0009956; 80NSSC18K0728; 17H01131; 19K03874; 15H05888; 19H05110; DMS-1440140; PRG803; FG02-85ER40237; AST-1813834; PHY-1748958; SC0012567; JP17H01131; JP15H05889; JP18H04594; JP19H05114; JP20H04750; SC0007859
USDOE Office of Science (SC), High Energy Physics (HEP)
National Science Centre of Poland (NCN)
European Research Council (ERC)
Ministry of Education, Culture, Sports, Science and Technology (MEXT)
European Union's Horizon 2020
FERMILAB-PUB-20-242-A; KCL-PH-TH/2020-33; KEK-Cosmo-257, KEK-TH-2231; IPMU20-0070; PI/UAN-2020-674FT; RUP-20-22; arXiv:2006.16182
ISSN:2565-6120
2565-6120
DOI:10.21105/astro.2006.16182