DARKSURVEY

Using Galaxy Surveys to Understand the Dark Universe

Coordinatore	UNIVERSITY OF PORTSMOUTH HIGHER EDUCATION CORPORATION    more Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie.
Nazionalità Coordinatore	United Kingdom [UK]
Totale costo	2˙151˙192 €
EC contributo	2˙151˙192 €
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-CoG
Funding Scheme	ERC-CG
Anno di inizio	2014
Periodo (anno-mese-giorno)	2014-06-01   -   2019-05-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	UNIVERSITY OF PORTSMOUTH HIGHER EDUCATION CORPORATION  Organization address address: "University House, Winston Churchill Avenue" city: PORTSMOUTH postcode: PO1 2UP contact info Titolo: Dr. Nome: Elizabeth Cognome: Bartle Email: send email Telefono: +44 2392843309 Fax: +44 2392843449	UK (PORTSMOUTH)	hostInstitution	2˙151˙192.00
2	UNIVERSITY OF PORTSMOUTH HIGHER EDUCATION CORPORATION  Organization address address: "University House, Winston Churchill Avenue" city: PORTSMOUTH postcode: PO1 2UP contact info Titolo: Prof. Nome: William Cognome: Percival Email: send email Telefono: +44 2392843107 Fax: +44 2392845626	UK (PORTSMOUTH)	hostInstitution	2˙151˙192.00

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 Obiettivo del progetto (Objective)

'Galaxy Surveys are a key resource for observational cosmology, with the potential to provide the answers to many fundamental questions in modern physics. The Darksurvey project will use the Dark Energy Survey (DES) and extended-Baryon Oscillation Spectroscopic Survey (eBOSS) within which Will Percival has key leadership positions, and future projects including MS-DESI to measure the cosmological expansion rate between redshifts 0.5 and 2, testing Dark Energy. Complimentary structure growth measurements will test Einstein's theory of Gravity on the largest scales possible. The large-scale clustering of galaxies will be used to constrain primordial non-Gaussianity, testing and constraining models of inflation. The scale-dependence of the clustering signal will be used to measure the masses of neutrinos through their early Universe effects, and to set constraints on the evolution of galaxies and structure over cosmological time-scales. Parallel development of innovative tests and measurement methods will be undertaken to enable and enhance these results, while joint analysis with CMB and weak-lensing data will be used to perform additional tests, and to break degeneracies present when cosmological models are tested. This grant will consolidate the world-leading position of the group initiated by Will Percival at the University of Portsmouth, and developed over the last 4 years. Furthermore, it will train and develop a group of scientists within Europe with the key experimental skills required for the ESA Euclid mission.'