GW ASAP

Gravitational Wave Astrophysics and Analysis with Pulsars

Coordinatore	MAX PLANCK GESELLSCHAFT ZUR FOERDERUNG DER WISSENSCHAFTEN E.V.    more  Organization address address: Hofgartenstrasse 8 city: MUENCHEN postcode: 80539 contact info Titolo: Mr. Nome: Karl-Heinz Cognome: Böckelmann Email: send email Telefono: +49 228 525 242 Fax: +49 228 525 409
Nazionalità Coordinatore	Germany [DE]
Totale costo	262˙975 €
EC contributo	262˙975 €
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-2013-IOF
Funding Scheme	MC-IOF
Anno di inizio	2014
Periodo (anno-mese-giorno)	2014-06-01   -   2017-05-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	MAX PLANCK GESELLSCHAFT ZUR FOERDERUNG DER WISSENSCHAFTEN E.V.  Organization address address: Hofgartenstrasse 8 city: MUENCHEN postcode: 80539 contact info Titolo: Mr. Nome: Karl-Heinz Cognome: Böckelmann Email: send email Telefono: +49 228 525 242 Fax: +49 228 525 409	DE (MUENCHEN)	coordinator	262˙975.20

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 Obiettivo del progetto (Objective)

'Gravitational waves, ripples of space-time from accelerating masses, are the most elusive prediction of Einstein’s theory of General Relativity; So elusive in fact, that they have yet to be directly detected, although indirect evidence from binary pulsars (e.g. Taylor and Weisberg, 1982) supports their existence. This project implements new and novel techniques to search for direct evidence of gravitational waves from supermassive black holes using Pulsar Timing Arrays by means of a new interdisciplinary collaboration in radio and infrared astronomy, data analysis and astrophysics. I will lead an international team of experts to simulate an astrophysically motivated gravitational wave background using candidate supermassive black hole binaries from galaxy catalogues. We will then assess the expected level of anisotropy in the gravitational wave background and use this information as a prior in a new and novel data analysis project which implements anisotropy in GW search algorithms. Finally, we extend the anisotropic search method to gravitational waves from single sources using a new 'hybridized' technique which may prove to be an invaluable tool in the search for, and first detection of, gravitational waves.'