Exploiting synergies between neutrino telescopes for the next galactic core-collapse supernova

被引：0

作者：

Bendahman, Meriem ^{[1
,3
]}

Buellet, Anne-Cecile ^{[2
]}

Bugli, Matteo ^{[2
]}

Coelhol, Joao ^{[1
]}

Coleirol, Alexis ^{[1
]}

de Wasseigel, Gwenhael ^{[1
]}

El Iledril, Sonia ^{[1
]}

Foglizzo, Thierry ^{[2
]}

Francol, Davide ^{[1
]}

Goosl, Isabel ^{[1
]}

Guilet, Jerome

Kouchnerl, Antoine ^{[1
]}

Tayalati, Yahya ^{[3
]}

Tonazzol, Alessandra ^{[1
]}

Volpe, Cristina ^{[1
]}

机构：

[1] Univ Paris Cite, Lab Astroparticules & Cosmol, Paris, France

[2] CEA Saclay, Dept Astrophys, Paris, France

[3] Mohammed V Univ, Fac Sci, Rabat, Morocco

来源：

RICAP-22, 8TH ROMA INTERNATIONAL CONFERENCE ON ASTROPARTICLE PHYSICS | 2023年 / 280卷

关键词：

D O I：

10.1051/epjconf/202328005002

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：4

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