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Communication Dans Un Congrès Année : 2021

Exploring the Potential of Multi-Detector Analyses for Core-Collapse Supernova Neutrino Detection

Résumé

The core-collapse supernova (CCSN) SN1987A has been the first extragalactic transient source observed in neutrinos, and the 25 events detected by the neutrino telescopes running at the time marked the beginning of neutrino astronomy. Despite the very large number of CCSNs detected in the electromagnetic spectrum since 1987, neutrino telescopes could not perform another observation due to the far distances of the sources. It is thus of primary importance to optimize the detection channel of sensitive detectors in anticipation of a forthcoming Galactic CCSN. Beyond being used as an early warning of a close-by CCSN, neutrinos can provide unique information on the explosion mechanisms, and can be used to probe neutrino flavor evolution in dense environments. In this contribution, we will present the potential of multi-detector analyses to enhance the scientific outputs from the next close-by CCSN. Combining the expected light curves in neutrino detectors sensitive to different flavors, we will study the constraints that could be set on the properties of the progenitor itself, such as its mass, as well as on the neutrino oscillation parameters. We will also present the results of a triangulation algorithm using a prior source map in the definition of the region of interest.

Dates et versions

hal-03373051 , version 1 (11-10-2021)

Identifiants

Citer

Meriem Bendahman, Matteo Bugli, Alexis Coleiro, Marta Colomer Molla, Gwenhaël de Wasseige, et al.. Exploring the Potential of Multi-Detector Analyses for Core-Collapse Supernova Neutrino Detection. 37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.1090, ⟨10.22323/1.395.1090⟩. ⟨hal-03373051⟩
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