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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.

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

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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