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BlackHoleMergers SIGNED

Formation of Black Hole Mergers in Dense Stellar Systems

Total Cost €

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EC-Contrib. €

0

Partnership

0

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 BlackHoleMergers project word cloud

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

learned    unsolved    interdisciplinary    framework    tidal    community    origins    ramirez    bhs    accurate    fundamental    bh    ensures    atmosphere    gr    black    scientists    binary    scatterings    models    encounters    incoming    gw    ideal    weak    carlo    dense    merge    gws    ring    waves    compact    interactions    leader    true    relativity    eccentric    infer    exotic    mergers    holes    ligo    virgo    astrophysical    vibrant    fellowship    near    body    evolution    seems    observations    exist    orbital    led    well    curie    analytical    form    corrections    remarkable    intellectual    supervisions    questions    bohr    numerical    time    bbh    enrico    describe    gravitational    environment    monte    martin    dynamical    nature    pair    helps    events    diffusion    data    merger    distributions    pioneering    secular    bbhs    carry    populations    timescale    einstein    origin    massive    prof    emitted    central    stellar    few    ruiz    host    mature    exceptional    pessah    marie    niels    signal    first    close   

Project "BlackHoleMergers" 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 219˙312 €
 EC max contribution 219˙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 2019
 Duration (year-month-day) from 2019-12-01   to  2021-11-30

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    KOBENHAVNS UNIVERSITET DK (KOBENHAVN) coordinator 219˙312.00

Map

Leaflet | Map data © OpenStreetMap contributors, CC-BY-SA, Imagery © Mapbox

 Project objective

The recent pioneering observations of gravitational waves (GWs) from merging black holes (BHs) by LIGO/Virgo have already led to new remarkable insight: From the first few events we have learned that BHs do indeed exist, that Einstein's General Relativity (GR) seems to very well describe their merger and ring-down evolution, and that nature is able to pair BHs in compact binary systems. However, many astrophysical key questions still remain unsolved, including, how and where BHs form and what helps them to get close enough to merge on an observable timescale. The project I propose will provide new state-of-the-art insight into such fundamental questions by addressing how BBHs form and merge in dense stellar systems, as well as how well one can infer their origin from their emitted GW signal. In order to achieve this goal, I will develop a new numerical Monte-Carlo framework for evolving dense stellar systems, which for the first time will include: stellar tidal interactions and GR corrections during strong few-body scatterings, orbital diffusion from weak encounters, and secular effects near a possible central massive BH. From my recent analytical models, these effects are expected to lead to the formation of eccentric BBH mergers, as well as other exotic populations, all of which can be used to constrain the dynamical origins of BBHs. The goal is to provide the community with accurate BBH merger distributions that can be used to constrain the origin of BBH mergers using incoming data from LIGO/Virgo. I will carry out the project at the Niels Bohr Institute under the supervisions of Prof. Martin Pessah and Niels Bohr Prof. Enrico Ramirez-Ruiz. The interdisciplinary environment, vibrant atmosphere, and exceptional scientists make the Niels Bohr Institute not only the ideal host for this project, but further ensures that I will mature into a true intellectual leader in my field during the time of the Marie Curie Fellowship.

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