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Ground based gravitational-wave astronomy in the next decades
mardi 08 février 2022

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Descriptif

After the first gravitational wave detection in 2015 and the GW170817 multi-messenger observation, the gravitational-wave astronomy has evolved rapidly. LIGO and Virgo detectors have performed their 3rd observing run between April 2019 and March 2020 and the third catalog of gravitational-waves sources (GWTC-3) has just been released, with a total of 90 sources detected so far. Upgrades of LIGO and Virgo are planned in the decade 2020-2030, increasing the scientific potential of the gravitational-wave detector network, which will include two more instruments in the next years: KAGRA in Japan and a third LIGO in India. In the decade 2030, the Einstein Telescope project, an European underground gravitational-wave observatory, aims to increase the sensitivity of current detector by one order of magnitude. In this seminar, after an summary about the current gravitational-wave observations, I will be describe in detail the LIGO-Virgo plans for the 2020 decade and then the scientific objectives and plans for Einstein Telescope.

Conférence donnée par Matteo Barsuglia,directeur du « Paris Centre for Cosmological Physics », lors du colloquium 2021/2022 du département de physique de l'ENS.

 

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Auteur(s)
Matteo Barsuglia
CNRS / Université de Paris
Astrophysicien / Directeur de recherches

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Matteo Barsuglia est directeur de recherche au CNRS.

Ses recherches portent sur la détection des ondes gravitationnelles et en particulier sur le développement des détecteurs interférométriques. De 2005 au 2007 il a dirigé l’équipe en charge de la mise au point du détecteur Virgo. De 2008 a 2018 il était responsable de l’équipe Virgo au laboratoire APC et membre du comité de pilotage du projet. Il est actuellement membre du comité de pilotage du projet Einstein Telescope. Depuis 2018 il est directeur du PCCP (Paris Centre for Cosmological Physics).

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Dernière mise à jour : 15/03/2022