STRING-QCD-BH

"String Theory, QCD and Black Holes"

Coordinatore	COMMISSARIAT A L ENERGIE ATOMIQUE ET AUX ENERGIES ALTERNATIVES    more Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie.
Nazionalità Coordinatore	France [FR]
Totale costo	652˙500 €
EC contributo	652˙500 €
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-2009-StG
Funding Scheme	ERC-SG
Anno di inizio	2010
Periodo (anno-mese-giorno)	2010-01-01   -   2014-12-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	COMMISSARIAT A L ENERGIE ATOMIQUE ET AUX ENERGIES ALTERNATIVES  Organization address address: RUE LEBLANC 25 city: PARIS 15 postcode: 75015 contact info Titolo: Dr. Nome: Iosif Lucian Razvan Cognome: Bena Email: send email Telefono: -69087436 Fax: -69088088	FR (PARIS 15)	hostInstitution	652˙500.00
2	COMMISSARIAT A L ENERGIE ATOMIQUE ET AUX ENERGIES ALTERNATIVES  Organization address address: RUE LEBLANC 25 city: PARIS 15 postcode: 75015 contact info Titolo: Mr. Nome: Jean-Christophe Cognome: Coste Email: send email Telefono: +33 1 69089097 Fax: +33 1 69082199	FR (PARIS 15)	hostInstitution	652˙500.00

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 Obiettivo del progetto (Objective)

'I intend to use string theory to understand gauge theories in four dimensions, both at strong and weak coupling. This includes describing strongly interacting gauge theories and their metastable vacua using their supergravity and string duals, as well as understanding gauge theories at intermediate coupling via integrability. It also includes using and developing new string-inspired twistor-space techniques to analyze QCD and N=1 amplitudes at one loop level. I also plan to thoroughly investigate the implications of string theory for the physics of black holes. In particular I want to construct and analyze black hole microstates -- smooth horizon-less solutions that are very similar to the black hole asymptotically, but differ from the black hole at the location of the horizon. Counting and understanding these microstates via the AdS-CFT correspondence will establish whether black holes should be thought of as ensembles of such microstate geometries.'