MULTIFAST

Variability in Relativistic Jets: the Fastest Time Scales at all Wavelengths

 Coordinatore ISTITUTO NAZIONALE DI ASTROFISICA 

 Organization address address: Viale del Parco Mellini 84
city: ROMA
postcode: 136

contact info
Titolo: Prof.
Nome: Fabrizio
Cognome: Fiore
Email: send email
Telefono: +39 06 94286433
Fax: +39 06 9447243

 Nazionalità Coordinatore Italy [IT]
 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-2012-CIG
 Funding Scheme MC-CIG
 Anno di inizio 2012
 Periodo (anno-mese-giorno) 2012-09-01   -   2016-08-31

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    ISTITUTO NAZIONALE DI ASTROFISICA

 Organization address address: Viale del Parco Mellini 84
city: ROMA
postcode: 136

contact info
Titolo: Prof.
Nome: Fabrizio
Cognome: Fiore
Email: send email
Telefono: +39 06 94286433
Fax: +39 06 9447243

IT (ROMA) coordinator 100˙000.00

Mappa


 Word cloud

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

mass    data    numerical    recently    compact    scientific    jet    lambda    relativistic    host    jets    amount    stellar    am   

 Obiettivo del progetto (Objective)

'I propose to fully harness a new exciting window recently opened in Astrophysics, which I am pioneering: the study of multi-lambda fast variability from relativistic jets from stellar-mass compact objects. I will (a) identify and apply strategies to maximize the scientific output of a large amount of data, and formally define and publish new standard methods for multi-lambda statistical and timing analysis, to serve as points of reference for future works; (b) initiate an ambitious numerical code for the variable emission from a relativistic jet from a stellar-mass compact object; (c) apply the above techniques and codes to a large amount of data, placing unprecedented constraints to the physics of jets, and comparing the jet properties in black holes and neutron stars, ultimately answering the fundamental question about how the jet properties are influenced by the presence of a hard surface or an event horizon (and/or ergosphere), as well as by the presence of large-scale bipolar magnetic fields. I am one of the precursors in this field, which has already shown its large potential. I have built and am currently a leading member of a large international collaboration, which has acquired a large amount of data with the most diverse sets of observational facilities and data structure. The complexity of the field, together with its clear potential, demands a focussed and continuous effort, which I am planning to take. I will tackle the objective with a multi-disciplinary approach, working on observations, theory and numerical simulations, maximizing the scientific exploitation of the method. I have been hired recently by the host institution with a researcher permanent position, which guarantees my stability during the project and the feasibility of the project itself. As the topics of the proposed project nicely complement the present expertise at the host institution, the CIG funding will help me enourmously in integrating myself in the host institution.'

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