28 August 2023 to 1 September 2023
University of Vienna
Europe/Vienna timezone

Exploiting the standing accretion shock instability for multi-messenger analysis of core-collapse supernovae

30 Aug 2023, 17:45
15m
Hörsaal 1 lecture hall (University of Vienna)

Hörsaal 1 lecture hall

University of Vienna

Universitätsring 1 A-1010 Vienna, Austria
Parallel talk Gravitational waves Gravitational waves

Speaker

Marco Drago (Sapienza University and INFN Roma 1)

Description

Core Collapse supernovae are among the most interesting source of possible multimessenger detections, given the joint production of electromagnetic, neutrino and gravitational waves (GW). In this work we investigate the correlation of SASI structure of neutrino and GW to enhance the GW detection. We compare different search analyses for the case of a benchmark three-dimensional CCSN simulation with zero-age main sequence mass of 24 solar masses. In particular, we build a matched filter analysis which increase detection efficiency of 30% with respect to a standard excess power algorithm for nearby CCSN (less than 1.5 kpc). At further distance we expect that additional work is needed to outline the best strategy for GW detection from CCSN.

Submitted on behalf of a Collaboration? No

Author

Marco Drago (Sapienza University and INFN Roma 1)

Co-authors

Alejandro Torres Fornè (Universitat de Valencia) Haakon Andresen (Oskar Klein Centre) Irene Di Palma Irene Tamborra (Niels Bohr Institute)

Presentation materials