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Early Universe Tomography with CMB and Gravitational Waves

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Kuroyanagi, Sachiko [University of Tokyo] Ringeval, Christophe [UCL] Takahashi, Tomo [Saga University]

We discuss how one can reconstruct the thermal history of the Universe by combining cosmic microwave background (CMB) measurements and gravitational wave (GW) direct detection experiments. Assuming various expansion eras to take place after the inflationary reheating and before Big-Bang Nucleosynthesis (BBN), we show how measurements of the GW spectrum can be used to break the degeneracies associated with CMB data, the latter being sensitive to the total amount of cosmic expansion only. In this context, we argue that the expected constraints from future CMB and GW experiments can probe a scenario in which there exists late-time entropy production in addition to the standard reheating. We show that, for some cases, combining data from future CMB and GW direct detection experiments allows the determination of the reheating temperature, the amount of entropy produced and the temperature at which the standard radiation era started.

Document type Article de périodique (Journal article) – Article de recherche
Access type Accès libre
Publication date 2013
Language Anglais
Journal information "Physical Review. D, Particles, Fields, Gravitation and Cosmology" - Vol. 87, no.8, p. 083502 [14 pages] (2013)
Peer reviewed yes
Publisher American Physical Society
issn 1550-7998
e-issn 1550-2368
Publication status Publié
Affiliation UCL - SST/IRMP - Institut de recherche en mathématique et physique
Links
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Bibliographic reference Kuroyanagi, Sachiko ; Ringeval, Christophe ; Takahashi, Tomo . Early Universe Tomography with CMB and Gravitational Waves. In: Physical Review. D, Particles, Fields, Gravitation and Cosmology, Vol. 87, no.8, p. 083502 [14 pages] (2013)
Permanent URL http://hdl.handle.net/2078.1/139895