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Detecting Low Energy Astrophysical Neutrinos with KM3NeT ORCA the Transient Neu...

Detecting Low Energy Astrophysical Neutrinos with KM3NeT ORCA the Transient Neutrino Sky at the GeV Scale "The era of Multi-Messenger (MM) astronomy has started with the joint observations of gravitational and electromagnetic waves in August 2017, and the announcement of a common source of high-energy neutrinos and gamma rays in July... ver más

07/10/2021

UPCité

185K€

Presupuesto del proyecto: 185K€

Líder del proyecto

UNIVERSITE PARIS CITE No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Fecha límite participación Sin fecha límite de participación.

Financiación concedida El organismo H2020 notifico la concesión del proyecto el día 2021-10-07

MSCA-IF-2018: Individual Fellowships Objective:The goal of the Individual Fellowships is to enhance the creative and innovative potential...

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1 Participantes

UPCité

184.71K€ | Lider

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Duración del proyecto: 29 meses Fecha Inicio: 2019-04-16
Fecha Fin: 2021-10-07

Líder del proyecto

UNIVERSITE PARIS CITE No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Presupuesto del proyecto 185K€

Fecha límite de participación Sin fecha límite de participación.

Descripción del proyecto "The era of Multi-Messenger (MM) astronomy has started with the joint observations of gravitational and electromagnetic waves in August 2017, and the announcement of a common source of high-energy neutrinos and gamma rays in July 2018. The ""Low-Energy Astrophysical Neutrinos in ORca"" (LEANOR) project aspires to be the next MM observation, coupling low-energy (GeV) neutrinos with electromagnetic and gravitational waves emitted during short gamma-ray bursts (SGRBs). While the signal/background differentiation is more challenging for low energy neutrinos, they have the advantage to be more abundant than their high-energy counterpart. Produced as a consequence of the accelerated proton flux colliding with the matter surrounding the source, they stand as promising messengers to constrain the local environment and would furthermore be of great help to identify new cosmic sources. To reach this goal, we propose to convert the KM3NeT-ORCA detector, initially designed for neutrino oscillation studies, into a telescope able to study astrophysical GeV neutrinos. A detailed study of the environmental noise will be coupled to a specific selection of ORCA data targeting GeV neutrino interactions. The data sample acquired will then be used to search for statistically significant excess of neutrinos during SGRBs. Three different analyses, based on electromagnetic or gravitational wave observations, will be developed. These analyses will allow to constrain the source environment as well as the hadronic acceleration process taking place in SGRBs. The project will lead to either the first joint observation of GeV neutrinos, electromagnetic and gravitational waves, or the first observational limits set in this energy range for the studied source population. Opening a new line of research in ORCA, LEANOR will also provide the KM3NeT collaboration with new tools to develop a variety of searches for low energy neutrinos emitted during transient events, such as Novae or Fast radio bursts."

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