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.

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

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.)

HEIST (2020)

High-temperature Electrochemical Impedance Spectroscopy Transmission electron microscopy on energy materials

Read More  

HyperBio (2019)

Vis-NIR Hyperspectral imaging for biomaterial quality control

Read More  

AncientAdhesives (2019)

Ancient Adhesives - A window on prehistoric technological complexity

Read More