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REGMat SIGNED

Rotational effects on strongly gravitating systems with matter

Total Cost €

0

EC-Contrib. €

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Partnership

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Project "REGMat" 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://sites.google.com/site/regmat656882/
 Total cost 170˙121 €
 EC max contribution 170˙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 2015
 Duration (year-month-day) from 2015-10-01   to  2017-09-30

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    UNIVERSITAT DE BARCELONA ES (BARCELONA) coordinator 170˙121.00

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 Project objective

Black holes (BHs), where gravity is strongest in the universe, are the objects where we must confront the most extreme phenomena predicted by general relativity (GR) and extensions thereof. As for the majority of astrophysical bodies, BHs are typically spinning. However, addressing rotation in GR is notoriously difficult. Moreover, BHs are ‘dirty’: they are accompanied by clouds of gas or accretion disks, which introduce deviations from the known vacuum solutions. The complexity of the Einstein equations, taking into account the presence of matter and the rotation of spacetime, hampers attempts to model realistic BHs.

The prime goal of this research proposal is to deepen our understanding of BH dynamics in the presence of matter, and in particular the interplay between matter and the rotation of spacetime. This line of research will significantly advance our knowledge regarding the stability of more realistic (non-vacuum, non-spherically symmetric) BHs, as well as on outstanding issues, such as cosmic censorship.

Moreover, BHs nowadays are central to many areas of physics through the application of GR to fields other than the traditional ones of astrophysics and cosmology, namely to the more modern ones such as quantum gravity, high-energy physics (HEP) and strongly coupled quantum systems. Higher-dimensional gravity and the gauge/gravity duality provide a strong motivation to investigate BHs in contexts formerly regarded as removed from physical applications, in particular asymptotically anti-de Sitter (AdS) spacetimes of more than four dimensions. This proposal investigates, as a natural extension of the above-mentioned problems, the dynamics of rotating AdS BHs with implications for our understanding of thermalization in strongly coupled quantum theories.

 Publications

year authors and title journal last update
List of publications.
2016 Vitor Cardoso, Jorge V. Rocha
Collapsing shells, critical phenomena, and black hole formation
published pages: , ISSN: 1550-7998, DOI: 10.1103/PhysRevD.93.084034
Physical Review D 93/8 2019-06-13
2017 Pedro Aniceto, Jorge V. Rocha
Dynamical black holes in low-energy string theory
published pages: , ISSN: 1029-8479, DOI: 10.1007/JHEP05(2017)035
Journal of High Energy Physics 2017/5 2019-06-13
2016 Pedro Aniceto, Paolo Pani, Jorge V. Rocha
Radiating black holes in Einstein-Maxwell-dilaton theory and cosmic censorship violation
published pages: , ISSN: 1029-8479, DOI: 10.1007/JHEP05(2016)115
Journal of High Energy Physics 2016/5 2019-06-13
2016 Bidisha Chakrabarty, Jorge V. Rocha, Amitabh Virmani
Smooth non-extremal D1-D5-P solutions as charged gravitational instantons
published pages: , ISSN: 1029-8479, DOI: 10.1007/JHEP08(2016)027
Journal of High Energy Physics 2016/8 2019-06-13
2016 Richard Brito, Vitor Cardoso, Jorge V. Rocha
Interacting shells in AdS spacetime and chaos
published pages: , ISSN: 1550-7998, DOI: 10.1103/PhysRevD.94.024003
Physical Review D 94/2 2019-06-13

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