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DustOrigin SIGNED

The origin of cosmic dust in galaxies

Total Cost €

0

EC-Contrib. €

0

Partnership

0

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 DustOrigin project word cloud

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

stars    source    size    models    galaxy    technique    hydrogen    infrared    molecular    infer    composition    observations    laboratory    sn    simultaneously    experimental    shocks    polarimetric    observational    first    rates    simulations    efficiencies    pillars    found    responsible    snrs    opportune    mechanism    dominant    legacy    radiative    energies    herschel    model    galactic    structures    light    driving    inferring    starlight    50    structure    building    modelled    collapsing    grain    3d    lerma    erc    myself    galaxies    cosmological    metals    clouds    ism    alma    diffusion    massive    dust    adsorption    net    form    grains    route    expanded    sources    detect    physics    me    unknown    neglect    outcome    universe    overestimated    destruction    data    efficient    remnants    exploited    realistic    feedback    supernova    inhomogeneous    obscuration    origin    evolution    deus    outflows    redshift    collaborators    nearby    assumed    cloud    cooling    delivered    time    expertise    lack    re    statistical    condensation    experiments    pervades    chemical   

Project "DustOrigin" data sheet

The following table provides information about the project.

Coordinator
UNIVERSITEIT GENT 

Organization address
address: SINT PIETERSNIEUWSTRAAT 25
city: GENT
postcode: 9000
website: http://www.ugent.be

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 Belgium [BE]
 Total cost 1˙500˙000 €
 EC max contribution 1˙500˙000 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2019-STG
 Funding Scheme ERC-STG
 Starting year 2020
 Duration (year-month-day) from 2020-09-01   to  2025-08-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    UNIVERSITEIT GENT BE (GENT) coordinator 1˙500˙000.00

Map

 Project objective

Dust pervades the Universe; it is responsible for the obscuration of 50% of starlight, for the formation of molecular hydrogen, for the cooling of clouds collapsing to form stars, and for radiative feedback processes capable of driving massive galactic outflows. Due to the unknown origin of dust, cosmological simulations lack detailed dust physics, which will affect the outcome of galaxy evolution models. Current work by myself and collaborators have delivered observational evidence for the efficient condensation of dust in supernova remnants (SNRs). Up to now, grain growth is assumed to be the dominant dust source, but a viable chemical route for growing grains in the ISM has yet to be found. Current dust destruction efficiencies have been overestimated due to the neglect of inhomogeneous cloud structures. With Herschel's legacy of dust in the nearby Universe and ALMA's capabilities to detect the first infrared light of galaxies, this is an opportune time to re-evaluate the origin of dust. Building upon my expertise in dust in both SNRs and nearby galaxies, I will re-evaluate net SN dust production rates by inferring the composition and grain size of SN dust based on my own dust polarimetric data of Galactic SNRs. With my collaborators from LERMA, I will exploit a new experimental technique to simultaneously infer adsorption and diffusion energies; these laboratory measurements will allow me to assess whether grain growth can provide a viable mechanism for dust formation. My Dust and Element evolUtion modelS (DEUS) will be expanded to include a 3D inhomogeneous ISM structure, and will be exploited to model the destruction of dust by shocks in a realistic multi-phase ISM. Finally, the evolution of dust and metals will be modelled in a statistical sample of low- and high-redshift galaxies to infer the dominant dust sources. The three pillars (observations, modelling and laboratory experiments) of my ERC project are essential to solve the origin of dust problem.

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

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

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