QM-SING

Quantum Resolution of Gravitational Singularities

Coordinatore	UNIVERSITEIT VAN AMSTERDAM    more  Organization address address: SPUI 21 city: AMSTERDAM postcode: 1012WX contact info Titolo: Ms. Nome: Jo Cognome: Lansbergen Email: send email Telefono: +31 20 525 6915 Fax: +31 20 525 7675
Nazionalità Coordinatore	Netherlands [NL]
Totale costo	183˙469 €
EC contributo	183˙469 €
Programma	FP7-PEOPLE Specific programme "People" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
Code Call	FP7-PEOPLE-2012-IEF
Funding Scheme	MC-IEF
Anno di inizio	2013
Periodo (anno-mese-giorno)	2013-10-01   -   2016-03-02

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	UNIVERSITEIT VAN AMSTERDAM  Organization address address: SPUI 21 city: AMSTERDAM postcode: 1012WX contact info Titolo: Ms. Nome: Jo Cognome: Lansbergen Email: send email Telefono: +31 20 525 6915 Fax: +31 20 525 7675	NL (AMSTERDAM)	coordinator	183˙469.80

Mappa

 Word cloud

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

 Obiettivo del progetto (Objective)

'String Theory is a promising theory of quantum gravity, unifying all known forces. However, it is notoriously hard to extract testable predictions from it. Black holes are ubiquitous in string theory (and any theory of General Relativity (GR) for that matter). Their study offers a shortcut for successfully testing the validity of string theory. This projects pursues a theoretical test of string theory, through the study of black holes. In classical GR, black holes are solutions with enigmatic properties, such as a spacetime singularity. When coupling them to quantum fields, there appear questions that GR cannot explain: the information paradox, black hole entropy.

In this project, we will answer these issues by studying black hole microstates. Their existence would resolve the black hole singularity, solve the information paradox and explain black hole entropy. For supersymmetric black holes, which are rather unrealistic, there has been quite some success in constructing these microstates, but not nearly enough to solve all black hole problems. We plan as a first step in the string theory test to systematically construct (1) new supersymmetric black hole microstates, and (2) take the story further to more realistic, non-supersymmetric radiating black holes. A later stage of this research will be to determine their properties. Additionally, the implications on cosmological singularities will be intitiated, with the expertise of the GRAPPA Institute (Gravitational AstroParticle Physics Amsterdam), affiliated with the ITFA, training the researcher in a new field (cosmology).

In addition, the researcher will supervise master students, coach graduate students and lecture graduate courses in an international school. Furthermore, he will present his work in leading international conferences, and develop research management skills. This complete and intensive training will greatly enhance the researcher's abilities to lead a research group in the future.'