26-30 July 2021
Europe/Berlin timezone

Gravitational Waves as a Big Bang Thermometer

26 Jul 2021, 15:35


Parallel session talk Astroparticle and Gravitational Waves T01: Astroparticle and Gravitational Waves


Carlos Tamarit (Technische Universität München)


There is a guaranteed background of stochastic gravitational waves produced in the thermal plasma in the early universe. Its energy density per logarithmic frequency interval scales with the maximum temperature Tmax which the primordial plasma attained at the beginning of the standard hot big bang era. It peaks in the microwave range, at around 80 GHz [106.75/gs(Tmax)]^(1/3), where gs(Tmax) is the effective number of entropy degrees of freedom in the primordial plasma at Tmax. We present a state-of-the-art prediction of this Cosmic Gravitational Microwave Background (CGMB) for general models, and carry out calculations for the case of the Standard Model (SM) as well as for several of its extensions. On the side of minimal extensions we consider the Neutrino Minimal SM (νMSM) and the SM-Axion-Seesaw-Higgs portal inflation model (SMASH), which provide a complete and consistent cosmological history including inflation. As an example of a non-minimal extension of the SM we consider the Minimal Supersymmetric Standard Model (MSSM). Furthermore, we discuss the current upper limits and the prospects to detect the CGMB in laboratory experiments and thus measure the maximum temperature and the effective number of degrees of freedom at the beginning of the hot big bang.

First author Carlos Tamarit
Collaboration / Activity Technical University of Munich
Email carlos.tamarit@tum.de

Primary authors

Carlos Tamarit (Technische Universität München) Andreas Ringwald (ALPS (Any Light Particle Search)) Jan Schütte-Engel (Uni Hamburg)

Presentation Materials