DARKSURVEY

Using Galaxy Surveys to Understand the Dark Universe

 Coordinatore UNIVERSITY OF PORTSMOUTH HIGHER EDUCATION CORPORATION 

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 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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 Word cloud

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percival    survey    cosmological    energy    group    galaxies    models    scales    structure    clustering    tests    dark   

 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.'

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