'Advanced virgo' diaporamas de présentation

Status of the Advanced Virgo detector

Status of the Advanced Virgo detector. F. Piergiovanni on behalf of The Virgo Collaboration. GWPAW, Osaka, 06/17/2015. Talk outline. The Advanced Virgo challenges Where we stand and what we are going to do Construction and integration highlights Perspectives and conclusions.

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Substrates, Polishing, Coatings and Metrology for the 2 nd generation of GW detector

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Status of Virgo

Piero Rapagnani Department of Physics, La Sapienza & INFN, Sez. Roma On behalf of the Virgo Collaboration LIGO-G060281-00-Z. Status of Virgo. EGO. LAPP - Annecy INFN - Firenze/Urbino INFN - Frascati IPN - Lyon INFN - Napoli OCA - Nice. ESPCI - Paris LAL - Orsay INFN - Perugia

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Preliminary Thoughts on the optimal Arm Cavity Finesse of Advanced Virgo

Preliminary Thoughts on the optimal Arm Cavity Finesse of Advanced Virgo. Stefan Hild and A.Freise Advanced Virgo meeting, December 2008. Overview. Advanced Virgo design: Many decissions have to been taken in near future.

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TCS update

TCS update. INFN Roma Tor Vergata. Thermal Lensing Effects in Advanced Virgo. The cavity becomes less concentric, and the spot sizes at the mirrors will shrink (increase of thermal noise and reduction of arm cavity coupling to the input beam)

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Gravitational waves Jo van den Brand

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Stefan Hild ASR Group meting, November 2008

Squeezing the best astrophysics out of Advanced Virgo. Stefan Hild ASR Group meting, November 2008. Advanced Virgo. Virgo is currently the second largest gravitational wave detector in the world (3km).

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R&D on thermal noise in Europe: the STREGA Project

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Stefan Hild ASR Group meting, November 2008

Squeezing the best astrophysics out of Advanced Virgo. Stefan Hild ASR Group meting, November 2008. Advanced Virgo. Virgo is currently the second largest gravitational wave detector in the world (3km).

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Virgo Computing

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Towards Advanced Virgo

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Faraday thermal lensing numerical simulations

Faraday thermal lensing numerical simulations. Slim Hamdani EGO LIGO-G070358-00-Z. Faraday Thermal Lensing. Virgo: 10W + 3W mismaching:~0.5%. Virgo +: 40W + 10W mismaching:~5%. Advanced Virgo: 150W + 50W mismaching:~37%. When heated, the Faraday isolator:

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Why use FinesseTools for Advanced Virgo simulations, a simple example .

Why use FinesseTools for Advanced Virgo simulations, a simple example. Stefan Hild (University of Birmingham) + A.Freise, M.Mantovani, A.Perreca Advanced Virgo telecon, June 2008. Outline. Motivation: Why to use FinesseTools for OSD-work? Infrastructure for OSD-Simulations

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Composizione del Gruppo Virgo di Padova-Trento: FTE = 5.9

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1 st Feedback from the Gravitational-waves working group

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VESB NEWS Viviana Fafone and Roberto Passaquieti for the VESB VIR-0288A-17

VESB NEWS Viviana Fafone and Roberto Passaquieti for the VESB VIR-0288A-17. NEXT CONFERENCES. GWADW ( Hamilton Island- AU, May 07-12 ) Event moderator : F. Fidecaro et al Presentations Alessio Rocchi: Advanced Virgo: Where do we stand (for the Virgo Coll.)

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Beam sizes and mirror curvatures for Advanced Virgo

Beam sizes and mirror curvatures for Advanced Virgo. Stefan Hild and Andreas Freise University of Birmingham Advanced Virgo telecon, June 2008. Introduction. Advanced Virgo conceptual shows an inconsisten-cy regarding the beam size: The optics section uses 3.5cm radius

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