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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.

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

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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