Leptogenesis via Bubble Collisions

26 Sept 2024, 14:48
16m
Main Auditorium (DESY Hamburg)

Main Auditorium

DESY Hamburg

Notkestr. 85 D-22607 Hamburg, Germany
Cosmology & Astroparticle Physics Parallel Thursday Cosmo 1

Speaker

Martina Cataldi (UNI/TH (Uni Hamburg, Institut fuer Theoretische Physik))

Description

We present a novel realization of leptogenesis from the decays of sterile (right-handed) neutrinos (RHNs) produced from runaway bubble collisions at a first order phase transition. Such configurations can produce heavy RHNs with mass many orders of magnitude above the scale of symmetry breaking, thereby enabling (non-resonant) leptogenesis without the need for high reheat temperatures while also naturally suppressing washout effects. This mechanism also extends the window of viability to RHN masses $\gtrsim 10^{14}$ GeV, the natural scale for type-I seesaw with $\mathcal{O}(1)$ couplings, where standard thermal leptogenesis cannot produce the observed baryon asymmetry. The corresponding phase transitions are at scales $\gtrsim\!10^8$ GeV and can produce gravitational wave signals within reach of future experiments.

Primary authors

Bibhushan Shakya (T (Cosmology)) Martina Cataldi (UNI/TH (Uni Hamburg, Institut fuer Theoretische Physik))

Presentation materials