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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.

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

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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