NEPAL

Non-Equilibrium Processes in Galaxy Clusters

 Coordinatore BEN-GURION UNIVERSITY OF THE NEGEV 

 Organization address address: Office of the President - Main Campus
city: BEER SHEVA
postcode: 84105

contact info
Titolo: Ms.
Nome: Daphna
Cognome: Tripto
Email: send email
Telefono: +972 8 6472435
Fax: +972 8 6472930

 Nazionalità Coordinatore Israel [IL]
 Totale costo 100˙000 €
 EC contributo 100˙000 €
 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-2011-CIG
 Funding Scheme MC-CIG
 Anno di inizio 2011
 Periodo (anno-mese-giorno) 2011-11-01   -   2015-10-31

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    BEN-GURION UNIVERSITY OF THE NEGEV

 Organization address address: Office of the President - Main Campus
city: BEER SHEVA
postcode: 84105

contact info
Titolo: Ms.
Nome: Daphna
Cognome: Tripto
Email: send email
Telefono: +972 8 6472435
Fax: +972 8 6472930

IL (BEER SHEVA) coordinator 100˙000.00

Mappa


 Word cloud

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

theoretical    observational    clusters    cores    observations    simulations    recent    icm    theory    numerical   

 Obiettivo del progetto (Objective)

'I propose to study the dynamical and nonthermal processes in the intracluster medium (ICM) by combining a phenomenological analysis of observational data, a theoretical study, and dedicated numerical simulations. The proposed research is designed to address the central open questions in the theory of clusters, resolve the present tension between observations and simulations, distinguish between different theoretical models, and prepare for future observations. One main goal of the research is to disentangle the distributions of cosmic-rays, magnetic fields, and turbulence in the ICM, and identify their origins, evolution, and implications. A second goal is to facilitate a self-consistent model for the cool cores observed in the centers of most clusters, by identifying the mechanism that stabilizes the core against cooling, the feedback processes that render it robust, and the role played by active galactic nuclei and global flows. The research is motivated in part by the apparent lag of ICM theory behind the recent observational progress and the present numerical capabilities. In particular, it would utilize the recent observations of cold fronts, spiral patterns, and radio minihalos, that appear to exist in most cores.'

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