Opendata, web and dolomites

PeV-Radio SIGNED

Digital Radio Detectors for Galactic PeV Particles

Total Cost €

0

EC-Contrib. €

0

Partnership

0

Views

0

 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.

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

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.

Are you the coordinator (or a participant) of this project? Plaese send me more information about the "PEV-RADIO" project.

For instance: the website url (it has not provided by EU-opendata yet), the logo, a more detailed description of the project (in plain text as a rtf file or a word file), some pictures (as picture files, not embedded into any word file), twitter account, linkedin page, etc.

Send me an  email (fabio@fabiodisconzi.com) and I put them in your project's page as son as possible.

Thanks. And then put a link of this page into your project's website.

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

More projects from the same programme (H2020-EU.1.1.)

ERC VP CSA (2018)

Support to the Vice-Presidents of the ERC Scientific Council 2018

Read More  

CELPRED (2020)

Circuit elements of the cortical circuit for predictive processing

Read More  

AST (2019)

Automatic System Testing

Read More