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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.

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

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.

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

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