HIDGR

Higher dimensional general relativity: explicit solutions and the classification and stability of black holes

 Coordinatore THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF CAMBRIDGE 

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 Nazionalità Coordinatore United Kingdom [UK]
 Totale costo 1˙337˙044 €
 EC contributo 1˙337˙044 €
 Programma FP7-IDEAS-ERC
Specific programme: "Ideas" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
 Code Call ERC-2011-StG_20101014
 Funding Scheme ERC-SG
 Anno di inizio 2011
 Periodo (anno-mese-giorno) 2011-11-01   -   2016-10-31

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF CAMBRIDGE

 Organization address address: The Old Schools, Trinity Lane
city: CAMBRIDGE
postcode: CB2 1TN

contact info
Titolo: Dr.
Nome: Harvey Stephen
Cognome: Reall
Email: send email
Telefono: 441224000000

UK (CAMBRIDGE) hostInstitution 1˙337˙044.00
2    THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF CAMBRIDGE

 Organization address address: The Old Schools, Trinity Lane
city: CAMBRIDGE
postcode: CB2 1TN

contact info
Titolo: Ms.
Nome: Renata
Cognome: Schaeffer
Email: send email
Telefono: +44 1223 333543
Fax: +44 1223 332988

UK (CAMBRIDGE) hostInstitution 1˙337˙044.00

Mappa


 Word cloud

Esplora la "nuvola delle parole (Word Cloud) per avere un'idea di massima del progetto.

holes    hole    black    solutions    classification    dimensional    gr   

 Obiettivo del progetto (Objective)

'Higher-dimensional General Relativity (GR) is well-motivated by string theory e.g. via the gauge/gravity correspondence or scenarios that predict black hole production at the Large Hadron Collider. In this proposal it is regarded as a self-contained mathematical subject that extends conventional 4d GR. It is known that higher-dimensional GR exhibits qualitative differences from 4d GR, especially for black holes, e.g. there exist 'black ring' solutions describing rotating, donut-shaped black holes. It is likely that there are many other interesting solutions. This project will investigate the following topics in higher-dimensional GR: 1. Methods for obtaining explicit solutions of the Einstein equation, especially those based on algebraic classification of the Weyl tensor; 2. Classical stability of black holes; 3. Classification of black hole solutions: What data is required to specify uniquely black hole solutions? What are the allowed topologies and symmetries of black holes?'

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