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
Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie. |
| 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
| # | ||||
|---|---|---|---|---|
| 1 |
THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF CAMBRIDGE
Organization address
address: The Old Schools, Trinity Lane contact info |
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 contact info |
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.
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?'