Zobrazeno 1 - 10
of 77
pro vyhledávání: '"Barsuglia, Matteo"'
Autor:
Zhao, Yuhang, Capocasa, Eleonora, Eisenmann, Marc, Aritomi, Naoki, Page, Michael, Guo, Yuefan, Polini, Eleonora, Arai, Koji, Aso, Yoichi, van Beuzekom, Martin, Huang, Yao-Chin, Lee, Ray-Kuang, Lück, Harald, Miyakawa, Osamu, Prat, Pierre, Shoda, Ayaka, Tacca, Matteo, Takahashi, Ryutaro, Vahlbruch, Henning, Vardaro, Marco, Wu, Chien-Ming, Leonardi, Matteo, Barsuglia, Matteo, Flaminio, Raffaele
Frequency dependent squeezing is the main upgrade for achieving broadband quantum noise reduction in upcoming observation runs of gravitational wave detectors. The proper frequency dependence of the squeezed quadrature is obtained by reflecting squee
Externí odkaz:
http://arxiv.org/abs/2203.10815
Autor:
Shoemaker, D. H., Ballmer, Stefan, Barsuglia, Matteo, Berger, E., Berti, Emanuele, Brown, Duncan A., Chandra, Poonam, Evans, Matthew, Fang, Ke, Fong, Wen-fai, Freise, Andreas, Fritschel, Peter, Greene, Jenny, Horowitz, C. J., Kissel, Jeff, Lantz, Brian, Lasky, Paul D., Lueck, Harald, Miller, M. Coleman, Nitz, Alexander H., Ottaway, David, Peiris, Hiranya V., Punturo, Michele, Reitze, D. H., Sanders, Gary H., Sathyaprakash, B. S., Sigg, Daniel, Slagmolen, Bram, Smartt, S. J., Smith, Joshua R., Steiner, Andrew W., Troja, Eleonora, Villar, V. Ashley, Weiss, Rainer, Wolff, Sidney C., Yeck, Jim
The workshop Dawn VI: Next Generation Observatories took place online over three days, 5-7 October, 2021. More than 200 physicists and astronomers attended to contribute to, and learn from, a discussion of next-generation ground-based gravitational-w
Externí odkaz:
http://arxiv.org/abs/2112.12718
Autor:
Capocasa, Eleonora, Barsuglia, Matteo, Degallaix, Jérôme, Pinard, Laurent, Straniero, Nicolas, Schnabel, Roman, Somiya, Kentaro, Aso, Yoichi, Tatsumi, Daisuke, Flaminio, Raffaele
Publikováno v:
Phys. Rev. D 93, 082004 (2016)
The sensitivity of the gravitational-wave detector KAGRA, presently under construction, will be limited by quantum noise in a large fraction of its spectrum. The most promising technique to increase the detector sensitivity is the injection of squeez
Externí odkaz:
http://arxiv.org/abs/2004.00210
Autor:
Zhao, Yuhang, Aritomi, Naoki, Capocasa, Eleonora, Leonardi, Matteo, Eisenmann, Marc, Guo, Yuefan, Polini, Eleonora, Tomura, Akihiro, Arai, Koji, Aso, Yoichi, Huang, Yao-Chin, Lee, Ray-Kuang, Lück, Harald, Miyakawa, Osamu, Prat, Pierre, Shoda, Ayaka, Tacca, Matteo, Takahashi, Ryutaro, Vahlbruch, Henning, Vardaro, Marco, Wu, Chien-Ming, Barsuglia, Matteo, Flaminio, Raffaele
Publikováno v:
Phys. Rev. Lett. 124, 171101 (2020)
The astrophysical reach of current and future ground-based gravitational-wave detectors is mostly limited by quantum noise, induced by vacuum fluctuations entering the detector output port. The replacement of this ordinary vacuum field with a squeeze
Externí odkaz:
http://arxiv.org/abs/2003.10672
Autor:
Capocasa, Eleonora, Guo, Yuefan, Eisenmann, Marc, Zhao, Yuhang, Tomura, Akihiro, Arai, Koji, Aso, Yoichi, Marchiò, Manuel, Pinard, Laurent, Prat, Pierre, Somiya, Kentaro, Schnabel, Roman, Tacca, Matteo, Takahashi, Ryutaro, Tatsumi, Daisuke, Leonardi, Matteo, Barsuglia, Matteo, Flaminio, Raffaele
Earth-based gravitational-wave detectors will be limited by quantum noise in a large part of their spectrum. The most promising technique to achieve a broadband reduction of such noise is the injection of a frequency dependent squeezed vacuum state f
Externí odkaz:
http://arxiv.org/abs/1806.10506
Publikováno v:
Phys. Rev. D 97, 062003 (2018)
Density changes in the atmosphere produce a fluctuating gravity field that affect gravity strainmeters or gravity gradiometers used for the detection of gravitational-waves and for geophysical applications. This work addresses the impact of the atmos
Externí odkaz:
http://arxiv.org/abs/1801.04564
Publikováno v:
Phys.Rev.Lett.105:231102,2010
We report on the first experimental demonstration of higher-order Laguerre-Gauss (LGpl) mode generation and interferometry using a method scalable to the requirements of gravitational wave (GW) detection. GW detectors which use higher-order LGpl mode
Externí odkaz:
http://arxiv.org/abs/1008.0795
Autor:
Vallée, Martin, Ampuero, Jean Paul, Juhel, Kévin, Bernard, Pascal, Montagner, Jean-Paul, Barsuglia, Matteo
Publikováno v:
Science, 2017 Dec 01. 358(6367), 1164-1168.
Externí odkaz:
https://www.jstor.org/stable/26400975
Autor:
Arnaud, Nicolas, Barsuglia, Matteo, Bizouard, Marie-Anne, Brisson, Violette, Cavalier, Fabien, Davier, Michel, Hello, Patrice, Kreckelbergh, Stephane, Porter, Edward K.
Publikováno v:
Astropart.Phys. 21 (2004) 201-221
Trying to detect the gravitational wave (GW) signal emitted by a type II supernova is a main challenge for the GW community. Indeed, the corresponding waveform is not accurately modeled as the supernova physics is very complex; in addition, all the e
Externí odkaz:
http://arxiv.org/abs/gr-qc/0307101