Explore the words cloud of the REGMat project. It provides you a very rough idea of what is the project "REGMat" about.
The following table provides information about the project.
UNIVERSITAT DE BARCELONA
|Coordinator Country||Spain [ES]|
|Total cost||170˙121 €|
|EC max contribution||170˙121 € (100%)|
1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
|Duration (year-month-day)||from 2015-10-01 to 2017-09-30|
Take a look of project's partnership.
|1||UNIVERSITAT DE BARCELONA||ES (BARCELONA)||coordinator||170˙121.00|
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.
|year||authors and title||journal||last update|
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|
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|
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|
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|
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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