Opendata, web and dolomites

BHstabNL TERMINATED

The fate of black holes in high-energy physics -- exploring their dynamical instabilities

Total Cost €

0

EC-Contrib. €

0

Partnership

0

Views

0

 BHstabNL project word cloud

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

anti    describe    tool    guides    viewed    entirely    universe    sr    gr    energy    ultra    gravity    intend    concerning    sitter    point    turbulence    latest    always    cosmology    relativity    fundamental    predicted    gravitational    methodological    theories    theoretical    stability    scenarios    spacetimes    nr    humankind    conceptual    goals    discovered    successful    course    astrophysics    vastly    nature    latter    linear    physics    asymptotically    appear    push    date    tackle    game    offers    bhs    opening    combining    gauge    phenomena    bar    einstein    mode    play    mysteries    dynamical    gain    quest    dimensional    restricted    progress    numerical    superradiant    detect    attempting    de    spinning    models    duality    black    time    window    limits    former    standard    uncover    ads    quantum    secrets    establishing    enters    mechanics    force    binds    world    objects    mechanisms    ripe    regime    instabilities    explore    context    despite    employing    tick    perturbative    inmost    profound    techniques    ranging    hard    particle    expansion    marry    holes    wish   

Project "BHstabNL" data sheet

The following table provides information about the project.

Coordinator
UNIVERSITAT DE BARCELONA 

Organization address
address: GRAN VIA DE LES CORTS CATALANES 585
city: BARCELONA
postcode: 8007
website: http://www.ub.es

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 Spain [ES]
 Project website https://kclpure.kcl.ac.uk/portal/helvi.witek.html
 Total cost 158˙121 €
 EC max contribution 158˙121 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2014
 Funding Scheme MSCA-IF-EF-ST
 Starting year 2016
 Duration (year-month-day) from 2016-09-29   to  2018-09-28

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    UNIVERSITAT DE BARCELONA ES (BARCELONA) coordinator 158˙121.00

Map

 Project objective

Humankind has always been on a quest to uncover the secrets of our universe and ``detect the inmost force that binds the world and guides its course'. We intend to take important steps towards a more profound understanding of nature's mysteries by employing black holes (BHs). These exciting objects have been predicted by Einstein's general relativity (GR), one of the most successful models to-date to describe our universe, and they also appear in more fundamental theories attempting to marry GR with quantum physics. BHs can be viewed as the point-particle analogue of classical mechanics and play a key role in vastly different fields ranging from astrophysics and cosmology to high-energy physics. The latter enters the game in the context of higher dimensional gravity and the gauge/gravity duality which offers a unique tool to explore hard-to-tackle phenomena in field theories by investigating gravity in asymptotically anti-de Sitter (AdS) spacetimes.

Despite recent progress concerning the properties of BHs in these scenarios, most studies have been restricted to the linear regime. We wish to push these limits beyond the state-of-the-art and investigate the non-linear, dynamical behaviour and stability of BHs in asymptotically AdS and higher dimensional spacetimes, thus opening up an entirely new window to gain insight into the mechanisms that make our world tick. Specifically, we wish to explore the superradiant (SR) instabilities and the recently discovered gravitational turbulence in the former case and the non-linear response of BHs towards both the bar-mode and ultra-spinning instabilities in the latter. With the latest progress on the conceptual, theoretical and methodological level the time is ripe to accomplish these challenging goals by establishing novel techniques combining numerical relativity (NR), ``standard' perturbative methods and the large-D expansion recently developed by leading European researchers.

 Publications

year authors and title journal last update
List of publications.
2017 Robert Benkel, Thomas P Sotiriou, Helvi Witek
Black hole hair formation in shift-symmetric generalised scalar-tensor gravity
published pages: 64001, ISSN: 0264-9381, DOI: 10.1088/1361-6382/aa5ce7
Classical and Quantum Gravity 34/6 2019-06-13
2016 Robert Benkel, Thomas P. Sotiriou, Helvi Witek
Dynamical scalar hair formation around a Schwarzschild black hole
published pages: , ISSN: 2470-0010, DOI: 10.1103/PhysRevD.94.121503
Physical Review D 94/12 2019-06-13

Are you the coordinator (or a participant) of this project? Plaese send me more information about the "BHSTABNL" project.

For instance: the website url (it has not provided by EU-opendata yet), the logo, a more detailed description of the project (in plain text as a rtf file or a word file), some pictures (as picture files, not embedded into any word file), twitter account, linkedin page, etc.

Send me an  email (fabio@fabiodisconzi.com) and I put them in your project's page as son as possible.

Thanks. And then put a link of this page into your project's website.

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

More projects from the same programme (H2020-EU.1.3.2.)

MY MITOCOMPLEX (2021)

Functional relevance of mitochondrial supercomplex assembly in myeloid cells

Read More  

POLINGO (2018)

The Politics of Legitimacy: Non-partisan global governance and networked INGO power in the global governance of post-war states

Read More  

RipGEESE (2020)

Identifying the ripples of gene regulation evolution in the evolution of gene sequences to determine when animal nervous systems evolved

Read More