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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.

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

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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