Investigating cosmic histories with a stiff era through gravitational waves

We investigate the potential of gravitational-wave background searches to constrain cosmic histories characterized by a stiff equation of state, preceded by a period of matter domination. Such a scenario leads to a characteristic peak in the primordial gravitational-wave spectrum originating from cosmological inflation. Assuming instant transitions between distinct epochs, which allows for an analytical treatment of the gravitational-wave spectrum, we perform a Bayesian inference analysis to derive constraints from the first three observing runs of the LIGO-Virgo-KAGRA Collaboration. Additionally, we consider a smooth transition, employing an axionlike particle physics model, and highlight the differences compared to the instant transition approximation. Finally, we forecast detection prospects for such a cosmic history through future gravitational-wave experiments.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2024-11-07
DOI
https://doi.org/10.1103/physrevd.110.103503
Citations
8
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
2.65

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article

Investigating cosmic histories with a stiff era through gravitational waves

Mairi Sakellariadou, Sachiko Kuroyanagi, A. Romero, Alberto Mariotti et al.
8 citations
Physical review. D/Physical review. D.
Cosmology and Gravitation Theories
2.65
article

Investigating cosmic histories with a stiff era through gravitational waves

Mairi Sakellariadou, Sachiko Kuroyanagi, A. Romero, Alberto Mariotti, H. Duval
article en
8 citations

Abstract

We investigate the potential of gravitational-wave background searches to constrain cosmic histories characterized by a stiff equation of state, preceded by a period of matter domination. Such a scenario leads to a characteristic peak in the primordial gravitational-wave spectrum originating from cosmological inflation. Assuming instant transitions between distinct epochs, which allows for an analytical treatment of the gravitational-wave spectrum, we perform a Bayesian inference analysis to derive constraints from the first three observing runs of the LIGO-Virgo-KAGRA Collaboration. Additionally, we consider a smooth transition, employing an axionlike particle physics model, and highlight the differences compared to the instant transition approximation. Finally, we forecast detection prospects for such a cosmic history through future gravitational-wave experiments.

Physical review. D/Physical review. D.Vol. 110(10)
Vrije Universiteit Brussel (BE), Consejo Superior de Investigaciones Científicas (ES), King's College London (GB), Nagoya University (JP)
National Science Foundation, Comunidad de Madrid, Ministry of Education, Culture, Sports, Science and Technology, Academia Sinica, Fonds Wetenschappelijk Onderzoek, National Research Foundation of Korea, Max-Planck-Gesellschaft, Vrije Universiteit Brussel, Centre National de la Recherche Scientifique, Ministerio de Ciencia e Innovación, Vlaamse Interuniversitaire Raad, Ministry of Science and ICT, South Korea, Science and Technology Facilities Council, Australian Research Council, Japan Society for the Promotion of Science, Consejo Superior de Investigaciones Científicas, Instituto Nazionale di Fisica Nucleare, Agencia Estatal de Investigación, Centro de Excelencia en Geotermia de Los Andes
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Openalex Percentile: Top 10%
Cosmology and Gravitation Theories
2.65
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