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NEUCOS SIGNED

Neutrinos and the origin of the cosmic rays

Total Cost €

0

EC-Contrib. €

0

Partnership

0

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 NEUCOS project word cloud

Explore the words cloud of the NEUCOS project. It provides you a very rough idea of what is the project "NEUCOS" about.

neutrinos    physics    origin    rays    cosmic    solve    gamma    sources    ray    astrophysics    fluxes    neutrino    particle    nuclei   

Project "NEUCOS" data sheet

The following table provides information about the project.

Coordinator
STIFTUNG DEUTSCHES ELEKTRONEN-SYNCHROTRON DESY 

Organization address
address: NOTKESTRASSE 85
city: HAMBURG
postcode: 22607
website: www.desy.de

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Germany [DE]
 Total cost 1˙746˙000 €
 EC max contribution 1˙746˙000 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2014-CoG
 Funding Scheme /ERC-COG
 Starting year 2015
 Duration (year-month-day) from 2015-09-01   to  2020-08-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    STIFTUNG DEUTSCHES ELEKTRONEN-SYNCHROTRON DESY DE (HAMBURG) coordinator 1˙746˙000.00

Mappa

 Project objective

The discovery of cosmic neutrinos is one of the major breakthroughs in science in the year 2013. These neutrinos are expected to point back to the origin of the cosmic rays, which are produced in the most powerful accelerators in the universe. In order to solve the puzzle where the highest energetic neutrinos and cosmic rays come from, the key information could be the composition of the observed cosmic ray flux. The question critical for the future development of high-energy astrophysics is especially how heavier nuclei can be accelerated and escape from the sources, such as gamma-ray bursts or active galactic nuclei, without disintegration, or what the consequences for the neutrino fluxes and cosmic ray compositions at the sources are. Neutrinos, on the other hand, may be good for surprises, such as new physics only detectable at extreme energies, distances, or densities. In addition, the possibility to measure neutrino properties in neutrino telescopes has been emerging, either using astrophysical or atmospheric neutrino fluxes, which means that the border line between neutrino physics and astrophysics applications in these experiments fades. The key idea of this proposal is therefore to combine the expertise from astrophysics and particle physics in a multi-disciplinary working group 1) to study the effect of heavy nuclei on the source fluxes from multiple messengers, such as a neutrinos, cosmic rays, and gamma-rays, using efficient descriptions for the radiation processes and particle interactions, and 2) to optimize future experiment infrastructure in ice and sea water for both astro- and particle physics applications. The key goals are to eventually identify the origin of the cosmic rays and cosmic neutrinos, and to solve the open questions in particle physics, such as neutrino mass hierarchy and leptonic CP violation.

 Work performed, outcomes and results:  advancements report(s) 

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The information about "NEUCOS" are provided by the European Opendata Portal: CORDIS opendata.

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