FDP-MBH

Fundamental dynamical processes near massive black holes in galactic nuclei

Coordinatore	WEIZMANN INSTITUTE OF SCIENCE    more Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie.
Nazionalità Coordinatore	Israel [IL]
Totale costo	879˙999 €
EC contributo	879˙999 €
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-2007-StG
Funding Scheme	ERC-SG
Anno di inizio	2008
Periodo (anno-mese-giorno)	2008-09-01   -   2013-08-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	WEIZMANN INSTITUTE OF SCIENCE  Organization address address: HERZL STREET 234 city: REHOVOT postcode: 7610001 contact info Titolo: Dr. Nome: Tal Cognome: Alexander Email: send email Telefono: -9343519 Fax: -9343513	IL (REHOVOT)	hostInstitution	0.00
2	WEIZMANN INSTITUTE OF SCIENCE  Organization address address: HERZL STREET 234 city: REHOVOT postcode: 7610001 contact info Titolo: Ms. Nome: Talia Cognome: Tzahor Email: send email Telefono: +972 8 934 4026 Fax: -9343201	IL (REHOVOT)	hostInstitution	0.00

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 Obiettivo del progetto (Objective)

'I propose to combine analytical studies and simulations to explore fundamental open questions in the dynamics and statistical mechanics of stars near massive black holes. These directly affect key issues such as the rate of supply of single and binary stars to the black hole, the growth and evolution of single and binary massive black holes and the connections to the evolution of the host galaxy, capture of stars around the black hole, the rate and modes of gravitational wave emission from captured compact objects, stellar tidal heating and destruction, and the emergence of 'exotic' stellar populations around massive black holes. These processes have immediate observational implications and relevance in view of the huge amounts of data on massive black holes and galactic nuclei coming from earth-bound and space-borne telescopes, from across the electromagnetic spectrum, from cosmic rays, and in the near future also from neutrinos and gravitational waves.'