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PeV-Radio SIGNED

Digital Radio Detectors for Galactic PeV Particles

Total Cost €

0

EC-Contrib. €

0

Partnership

0

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 PeV-Radio project word cloud

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

expertise    setting    unknown    leadership    elevations    human    aperture    charged    detected    pev    astroparticle    accelerated    mass    sources    twenty    eev    pole    digital    parallel    purpose    lower    detectors    galaxy    first    photon    fundamental    technique    neutrinos    discovery    sensitive    extrapolation    observations    view    energy    accelerator    proven    lowered    anisotropies    lhc    ray    dramatically    made    dependent    radio    discovered    separation    center    exposure    candidates    showers    air    directions    accuracy    particle    breakthrough    presently    unprecedented    natural    energetic    cern    origin    significantly    threshold    chance    array    sky    tev    simultaneously    successfully    antenna    accelerators    siberia    create    scientific    frequencies    24    detection    particles    cosmic    provides    south    highest    correlation    search    outside    predicts    rays    photons    building    energies    physics    galactic   

Project "PeV-Radio" data sheet

The following table provides information about the project.

Coordinator
KARLSRUHER INSTITUT FUER TECHNOLOGIE 

Organization address
address: KAISERSTRASSE 12
city: KARLSRUHE
postcode: 76131
website: www.kit.edu

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˙629˙541 €
 EC max contribution 1˙629˙541 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2018-STG
 Funding Scheme ERC-STG
 Starting year 2019
 Duration (year-month-day) from 2019-02-01   to  2024-01-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    KARLSRUHER INSTITUT FUER TECHNOLOGIE DE (KARLSRUHE) coordinator 1˙629˙541.00

Map

 Project objective

The most energetic particles in our Galaxy are accelerated by yet unknown sources to energies much beyond the reach of human-made accelerators such as LHC at CERN. The detection of PeV photons from such a natural Galactic accelerator will be a fundamental breakthrough. For this purpose I propose a digital radio array for air showers at South Pole building on my proven expertise in successfully setting up and managing an antenna array in Siberia. Recently, we have discovered that by using higher radio frequencies than before the energy threshold can be lowered dramatically from 100 PeV to about 1 PeV. The new radio array will significantly enhance the present PeV particle detectors at South Pole in both, accuracy and aperture towards lower elevations. One of the most promising candidates for the origin of cosmic rays, the Galactic Center presently outside of the field of view, will be observable 24/7 with the radio array. The extrapolation of classical TeV observations predicts more than twenty PeV photons to be detected by the radio array within three years. Since the radio array is sensitive simultaneously to cosmic photons and charged particles from all directions of the sky, the search for any photon sources can be done in parallel to cosmic-ray physics with unprecedented accuracy and exposure in the energy range of 1 PeV to 1 EeV. Thus, this radio array will create highest impact in astroparticle physics by the following scientific objectives all targeting the most energetic particles in our Galaxy: PeV photons and their correlation with sources of neutrinos and charged cosmic rays, mass separation of cosmic rays, search for mass-dependent anisotropies, particle physics beyond the reach of LHC. This timely proposal is a unique chance for European leadership in this novel technique. It provides the chance for scientific breakthrough by detection of the first PeV photons ever, and by the discovery of natural accelerators of multi-PeV particles.

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The information about "PEV-RADIO" are provided by the European Opendata Portal: CORDIS opendata.

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