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TackTDEs SIGNED

Tackling the complexity of Tidal Disruption Events

Total Cost €

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EC-Contrib. €

0

Partnership

0

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 TackTDEs project word cloud

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

power    origin    few    debris    uv    viscous    too    researcher    drive    evolution    lightcurve    thirring    galaxies    forces    optical    lense    powered    date    influence    play    combination    full    when    close    falls    missions    gets    diffusion    tidal    back    contains    radiation    spin    investigations    discovered    urgently    observational    self    energy    otherwise    star    onto    output    bands    cross    pericentre    accretion    geometry    angular    torques    object    physical    disc    disrupted    supermassive    settled    ray    stream    rotation    compact    events    dynamics    stellar    signal    delay    phases    disruption    near    tdes    mechanisms    data    producing    quiescent    analytical    photon    emission    gas    hole    larger    magnetic    elongated    shock    transport    tools    missing    dozen    precession    ultimate    black    holes    he    momentum    collision    initiates    numerical    relativistic    participate    huge    predictive    considering   

Project "TackTDEs" data sheet

The following table provides information about the project.

Coordinator
KOBENHAVNS UNIVERSITET 

Organization address
address: NORREGADE 10
city: KOBENHAVN
postcode: 1165
website: www.ku.dk

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 Denmark [DK]
 Total cost 207˙312 €
 EC max contribution 207˙312 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2018
 Funding Scheme MSCA-IF-EF-ST
 Starting year 2020
 Duration (year-month-day) from 2020-09-01   to  2022-08-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    KOBENHAVNS UNIVERSITET DK (KOBENHAVN) coordinator 207˙312.00

Map

 Project objective

When a star gets too close to a supermassive black hole, it gets disrupted by the strong tidal forces of the compact object. A few dozen of these tidal disruption events (TDEs) have been discovered to date and a much larger number is expected from current and near-future missions. The observed signal contains rich information about the mechanisms and conditions at play around black holes in otherwise quiescent galaxies. A full exploitation of the huge predictive power of TDEs urgently requires to improve our understanding of their dynamics and the associated emission. Through a combination of analytical and numerical tools, the proposed research aims at studying the different phases of these events considering crucial physical processes missing from previous investigations. After the star has been disrupted, the debris evolves into an elongated gas stream that partially falls back towards the black hole. The researcher will determine how the geometry of this matter evolves under the influence of stellar magnetic field and rotation. As this stream comes back to pericentre, general-relativistic effects cause it to self-cross, which initiates the formation of an accretion disc and could participate to the emission of TDEs in the optical and UV bands. The researcher will determine the influence of the black hole spin on this process, focusing on the delay of stream-stream collision induced by Lense-Thirring precession. He will also investigate photon diffusion during disc formation to determine the evolution of the emerging shock-powered lightcurve. After the gas has settled, viscous torques drive the accretion of the stellar matter onto the black hole, producing X-ray radiation. The researcher will study this ultimate phase to evaluate the energy output and the origin of angular momentum transport in TDEs. This work will result in great advances in this research field on the theoretical side that will be used to better exploit observational data.

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

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