Speaker
Paola Simone
Description
Hawking radiation from primordial black holes provides a unique link between particle physics and black hole physics. In this work, we investigate the phenomenology of black hole evaporation, focusing on photon and neutrino signals produced through secondary emission processes. Particular attention is given to potential signatures arising in Beyond Standard Model scenarios, such as supersymmetric extensions. Using Monte Carlo simulations, we assess whether these effects lead to observable features, providing an astrophysical probe of new physics complementary to current collider searches.
Author
Co-authors
Prof.
Francesco Sannino
(University of Southern Denmark)
Prof.
Giacomo Cacciapaglia
(LPTHE)
Dr
Vania Vellucci
(University of Southern Denmark)