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DMIDAS SIGNED

Astrophysical constraints on the identity of the dark matter

Total Cost €

0

EC-Contrib. €

0

Partnership

0

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 DMIDAS project word cloud

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

compelling    dark    forms    spectra    microwave    superbit    sources    clustering    small    equally    power    fundamental    interacting    imaging    disprovable    types    photometric    implications    elementary    identity    models    staggering    borne    candidate    back    cosmology    bang    standard    big    durham    structure    cdm    hundreds    innovative    simulations    diagnostics    lcdm    asymmetric    clusters    times    candidates    theoretical    cosmic    differ    joint    smaller    inconclusive    particle    surveys    basis    observations    epochs    larger    investigation    physics    stellar    lensing    scales    particles    searches    shortly    astrophysical    agree    pattern    hydrodynamics    laboratory    survey    cosmological    individual    code    desi    created    halos    warm    acquire    balloon    consists    spectro    temperature    gravitational    turned    data    collect    stars    swift    dwarf    solution    rule    remarkably    predictive    background    model    astronomy    observational    predictions    1980s    telescope    dating    cold    bright    galaxies    milky    galaxy    exclusive    magnitude    radiation    self    proved    favoured   

Project "DMIDAS" data sheet

The following table provides information about the project.

Coordinator
UNIVERSITY OF DURHAM 

Organization address
address: STOCKTON ROAD THE PALATINE CENTRE
city: DURHAM
postcode: DH1 3LE
website: www.dur.ac.uk

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 United Kingdom [UK]
 Total cost 2˙493˙439 €
 EC max contribution 2˙493˙439 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2017-ADG
 Funding Scheme ERC-ADG
 Starting year 2018
 Duration (year-month-day) from 2018-10-01   to  2023-09-30

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    UNIVERSITY OF DURHAM UK (DURHAM) coordinator 2˙493˙439.00

Map

 Project objective

The identity of the dark matter is a fundamental problem in Physics whose solution will have major implications for cosmology, astronomy and particle physics. There is compelling evidence that the dark matter consists of elementary particles created shortly after the Big Bang, but searches for them in the laboratory and from astrophysical sources have proved inconclusive. The currently favoured candidate is cold dark matter or CDM. This forms the basis of the standard model of cosmology, LCDM, whose predictions, dating back to the 1980s, turned out to agree remarkably well with observations covering a staggering range of epochs and scales, from the temperature structure of the cosmic microwave background radiation to the large-scale pattern of galaxy clustering. Yet, this agreement is not exclusive to CDM: models based on other types of particles -- warm, self-interacting or asymmetric, for example -- agree equally well with these data but differ on scales smaller than individual bright galaxies. These are the scales targeted in this application in which we propose a comprehensive investigation of small-scale structure, with the aim of testing dark matter candidates, by focusing on three key astrophysical diagnostics: strong gravitational lensing, dwarf galaxies and stellar halos. We propose a joint theoretical and observational programme exploiting three major developments: SWIFT, a new code developed at Durham that will enable cosmological hydrodynamics simulations an order of magnitude larger than is possible today; SuperBIT, an innovative balloon-borne wide-field imaging telescope that will collect gravitational lensing data for hundreds of galaxy clusters; and DESI, a spectro-photometric survey that will acquire 10 times more spectra of stars in the Milky Way than previous surveys. The particle models that we will consider have predictive power and are disprovable. Our programme has the potential to rule out many dark matter particle candidates, including CDM.

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The information about "DMIDAS" are provided by the European Opendata Portal: CORDIS opendata.

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