Abstract: In a curved spacetime, the definition of particles depends on the observer's frame of reference. Consequently, in non-stationary spacetimes, such as those present in the Early Universe during and after inflation or during the gravitational collapse leading to black hole formation, a substantial production of particles may occur. This talk explores the impact of gravitational particle production (GPP) on scenarios generating the observed matter-antimatter asymmetry, particularly in the context of leptogenesis. We first examine the effects of cosmological GPP, showing that the observed asymmetry could be produced without requiring the Universe to be reheated to temperatures matching the right-handed neutrino masses. Additionally, we investigate the interplay between leptogenesis and primordial black holes, demonstrating that Hawking evaporation can either enhance or suppress the generated asymmetry, depending on the specific black hole parameter space.

Speaker Bio: Dr. Perez-Gonzalez received his PhD in 2017 at the University of Sao Paulo, Brazil, under the supervision of Prof. Dr. Renata Zukanovich Funchal. He was a research associate at Fermilab and Northwestern University (2018–2021), and later at the Institute for Particle Physics Phenomenology, Durham University (2021–2024). He is now a postdoctoral researcher at the DFT and IFT of UAM. His research focuses on neutrinos, black hole evaporation, baryon asymmetry and dark matter generation in the Early Universe.