FDP-MBH

Fundamental dynamical processes near massive black holes in galactic nuclei

 Coordinatore WEIZMANN INSTITUTE OF SCIENCE 

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 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

Mappa


 Word cloud

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

massive    stellar    holes    black    hole    binary    gravitational    stars    rate    evolution    single    near   

 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.'

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