DISCSIM

Hydrodynamical simulations of protoplanetary discs in the era of ALMA imaging

Coordinatore	THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF CAMBRIDGE    more Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie.
Nazionalità Coordinatore	United Kingdom [UK]
Totale costo	1˙892˙844 €
EC contributo	1˙892˙844 €
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-2013-ADG
Funding Scheme	ERC-AG
Anno di inizio	2014
Periodo (anno-mese-giorno)	2014-02-01   -   2019-01-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF CAMBRIDGE  Organization address address: The Old Schools, Trinity Lane city: CAMBRIDGE postcode: CB2 1TN contact info Titolo: Ms. Nome: Renata Cognome: Schaeffer Email: send email Telefono: 441223000000 Fax: 441223000000	UK (CAMBRIDGE)	hostInstitution	1˙892˙844.00
2	THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF CAMBRIDGE  Organization address address: The Old Schools, Trinity Lane city: CAMBRIDGE postcode: CB2 1TN contact info Titolo: Prof. Nome: Catherine Cognome: Clarke Email: send email Telefono: -340266 Fax: -338702	UK (CAMBRIDGE)	hostInstitution	1˙892˙844.00

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 Obiettivo del progetto (Objective)

'This is a proposal for an ambitious programme of state of the art hydrodynamical simulations, designed to answer some key questions about the role of disc self-gravity in planet formation. The programme is also designed so as to maximize the synergy with the new observational constraints from high resolution imaging data from the Atacama Large Millimetre Array that will become available over the timescale of the grant. The five year programme should provide definitive answers about whether planet formation is able to get going during the early, self-gravitating phase of disc evolution and how, if so, it would affect the further evolution of the disc. The topic of gravitational disc fragmentation as a route to planet formation is currently in a state of crisis, with recent simulations undermining what had become a consensus view on the subject. A dedicated and carefully constructed approach, as detailed here, is required to solve this problem.'