EPJ Web Conf.
Volume 280, 2023RICAP-22, 8th Roma International Conference on Astroparticle Physics
|Number of page(s)||4|
|Published online||20 March 2023|
Exploiting synergies between neutrino telescopes for the next galactic core-collapse supernova
Laboratoire Astroparticules et Cosmologie, Université Paris Cité, Paris
2 CEA Saclay, Department of Astrophysics
3 Faculty of Sciences, Mohammed V University, Rabat
* e-mail: firstname.lastname@example.org
Published online: 20 March 2023
Observing and characterizing the next galactic core-collapse supernova will be a critical step for neutrino experiments. Extracting information about the supernova progenitors and neutrino properties within minutes after an observation will in particular be crucial in order to optimize analysis strategies at other observatories. Moreover, certain classes of progenitors, with strong magnetic ﬁelds, could give rise to gamma-ray bursts but have been underinvestigated to date. In this contribution we propose a strategy to combine results from next-generation neutrino experiments, focusing notably on the determination of the progenitor mass and the neutrino mass ordering. Additionally, we investigate the impact of strong magnetic ﬁelds on neutrino observations, and demonstrate the detectability of the associated eﬀects in upcoming experiments.
© The Authors, published by EDP Sciences, 2023
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.