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13–17 May 2024
University of Pittsburgh / Carnegie Mellon University
US/Eastern timezone

Probing flavor violation and baryogenesis via primordial gravitational waves

15 May 2024, 14:30
15m
David Lawrence Hall 105 (University of Pittsburgh)

David Lawrence Hall 105

University of Pittsburgh

Gravity & Gravitational Waves Gravity & Gravitational Waves

Speaker

Zafri Ahmed Borboruah (IIT Bombay)

Description

We show that observations of primordial gravitational waves of inflationary origin can shed light into the scale of flavor violation in a flavon model. The mass hierarchy of fermions can be explained by a flavon field. If it exists, the energy density stored in oscillations of the flavon field around the minimum of its potential redshifts as matter and is expected to dominate over radiation in the early universe. The evolution of primoridial gravitational waves acts as a bookkeeping method to understand the expansion history of the universe. Importantly, the gravitational wave spectrum is different if there is an early matter dominated era, compared to radiation domination expected from standard cosmological model and gets damped by the entropy released in the flavon decays, determined by the mass of the flavon field mS and new scale of flavor violation ΛFV. Furthermore, the flavon decays can source the baryon asymmetry of the universe. We show that the mSΛFV parameter space in which the correct baryon asymmetry is produced can also be probed by gravitational wave observatories like BBO, DECIGO, U-DECIGO, ARES, LISA, ET, CE etc. for a blue-tilted gravitational wave spectrum. Our results are compatible with primordial origin of NANO-GRAV observations.

Author

Co-authors

Anish Ghoshal (University of Warsaw, Poland) Seyda Ipek

Presentation materials