7–12 Jul 2024
Aurum, the ‘Gabriele d’Annunzio’ University and ICRANet
Europe/Rome timezone

Neutrino counterpart of kHz GW sources

11 Jul 2024, 17:22
22m
M2 (Palazzo Micara of the ‘Gabriele d’Annunzio’ University)

M2

Palazzo Micara of the ‘Gabriele d’Annunzio’ University

Viale Pindaro, 42, Pescara
Invited talk in a parallel session Gravitational kHz waves - LIGO-Virgo-KAGRA Gravitational kHz waves - LIGO-Virgo-KAGRA

Speaker

IRENE DI PALMA (INFN AND SAPIENZA UNIVERSITY OF ROME)

Description

Multimessenger astrophysics provides unique and valuable insights into the properties and processes of the physical universe. The recent discovery of gravitational waves and high energy cosmic neutrinos, marked the beginning of a new era of the multimessenger astronomy. These new messengers, along with electromagnetic radiation and cosmic rays, give new insights into the most extreme energetic cosmic events. Among them supernovae explosion is one of the challenging targets of this new astronomical approach. We developed a machine learning algorithm to further improve the detectability of such type of source. Prospects for a third generation gravitational wave detector will be presented.

Primary authors

Mr Alessandro Veutro (Universita' di Roma La Sapienza, I-00185 Roma, Italy) Prof. Fulvio Ricci (Universita' di Roma La Sapienza, I-00185 Roma, Italy) IRENE DI PALMA (INFN AND SAPIENZA UNIVERSITY OF ROME) Prof. Marco Drago (Universita' di Roma La Sapienza, I-00185 Roma, Italy) Ms Melissa Lopez (Institute for Gravitational and Subatomic Physics (GRASP), Department of Physics) Prof. Pablo Cerda-Duran (Departamento de Astronomia y Astrofisica, Universitat de Valencia,)

Presentation materials