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4 projets européens trouvés

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 TERMINÉ 

Gravitational Wave Initial Training Network (GRAWITON)

Date du début: 1 févr. 2014, Date de fin: 31 janv. 2018,

...e enlarging of the world wide scientific community, with new actors coming from emerging countries and thanks to the boosting action due to the Einstein Telescope project, previously supported by the European Commission with the FP7-Design Study tool. The ESRs will be embedded in this exciting research environment and will be trained in the cutting edge technologies adopted in the Gravitational Wa ...
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 10

 TERMINÉ 

SHAring Researchers’ Passion for Engagement and Responsibility (SHARPER)

Date du début: 1 mai 2016, Date de fin: 30 nov. 2017,

..., combined with new knowledge and innovative discoveries. All these elements are summarized in the acronym SHARPER - Sharing Researchers’ Passion for Engagement and Responsibility the name of the European Researchers’ Night in the Centre and South of Italy that will take place on the 30th of September 2016 and on the 29th of September 2017 simultaneously in five cities: Perugia, L’Aquila, Ancona a ...
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 7

 TERMINÉ 

ET-LCGT Telescopes: Exchange of Scientists (ELiTES)

Date du début: 1 mars 2012, Date de fin: 28 févr. 2017,

A new way to investigate the Universe will be possible when the new generation of gravitational wave telescopes becomes operative. First, the advanced detectors, then the 3rd generation observatories will allow to detect the gravitational wave signal emitted in catastrophic event in the Universe. The Large-scale Cryogenic Gravitational wave Telescope (LCGT, now named KAGRA) in Japan and the Einste ...
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 9

 TERMINÉ 

Einstein gravitational-wave Telescope (ET)

Date du début: 5 mai 2008, Date de fin: 4 juil. 2011,

...new development in our quest to understand the history and future of the Universe, the emergence of the field of Gravitational Wave Astronomy. We are proposing to study the conceptual design of a new European infrastructure, a GW observatory that could cover the complete frequency range from about 1 Hz to 10 kHz that is potentially observable from ground. We are aiming at the identification of the ...
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