Zobrazeno 1 - 10
of 88
pro vyhledávání: '"Rosa, Rosário"'
Autor:
Koley, Soumen, Harms, Jan, Allocca, Annalisa, Calloni, Enrico, De Rosa, Rosario, Errico, Luciano, Esposito, Marina, Badaracco, Francesca, Rei, Luca, Bertolini, Alessandro, Bulik, Tomasz, Cieslar, Marek, Pietrzak, Mateusz, Suchenek, Mariusz, Fiori, Irene, Paoli, Andrea, Tringali, Maria Concetta, Ruggi, Paolo, Hild, Stefan, Singha, Ayatri, Idzkowski, Bartosz, Suchinski, Maciej, Masserot, Alain, Rolland, Loic, Mours, Benoit, Paoletti, Federico
A system was recently implemented in the Virgo detector to cancel noise in its data produced by seismic waves directly coupling with the suspended test masses through gravitational interaction. The data from seismometers are being filtered to produce
Externí odkaz:
http://arxiv.org/abs/2404.13170
Autor:
Janssens, Kamiel, Boileau, Guillaume, Christensen, Nelson, van Remortel, Nick, Badaracco, Francesca, Canuel, Benjamin, Cardini, Alessandro, Contu, Andrea, Coughlin, Michael W., Decitre, Jean-Baptiste, De Rosa, Rosario, Di Giovanni, Matteo, D'Urso, Domenico, Gaffet, Stéphane, Giunchi, Carlo, Harms, Jan, Koley, Soumen, Mangano, Valentina, Naticchioni, Luca, Olivieri, Marco, Paoletti, Federico, Rozza, Davide, Sabulsky, Dylan O., Shani-Kadmiel, Shahar, Trozzo, Lucia
We report correlations in underground seismic measurements with horizontal separations of several hundreds of meters to a few kilometers in the frequency range 0.01Hz to 40Hz. These seismic correlations could threaten science goals of planned interfe
Externí odkaz:
http://arxiv.org/abs/2402.17320
The 5-vector method is one of the main pipeline used by the LIGO-Virgo-KAGRA Collaboration for the analysis of continuous gravitational waves (CWs). This method is a matched filter in the frequency domain based on the splitting in five frequencies of
Externí odkaz:
http://arxiv.org/abs/2311.14071
Pulsars are promising targets for the first detection of continuous gravitational waves (CWs) by the LIGO-Virgo-KAGRA (LVK) Collaboration. Targeted searches leverage critical information derived from continued monitoring of pulsars related to the spi
Externí odkaz:
http://arxiv.org/abs/2311.14052
Autor:
D'Onofrio, Luca, De Rosa, Rosario, Palomba, Cristiano, Leaci, Paola, Piccinni, Ornella J., Sequino, Valeria, Errico, Luciano, Trozzo, Lucia, Palfreyman, Jim, McKee, James W., Meyers, Bradley W., Stairs, Ingrid, Guillemot, Lucas, Cognard, Ismael, Theureau, Gilles, Keith, Michael J., Lyne, Andrew, Flynn, Chris, Stappers, Ben
Publikováno v:
Phys. Rev. D 108, 122002 , Published 4 December 2023
The 5n-vector ensemble method is a multiple test for the targeted search of continuous gravitational waves from an ensemble of known pulsars. This method can improve the detection probability combining the results from individually undetectable pulsa
Externí odkaz:
http://arxiv.org/abs/2311.08229
Autor:
Koley, Soumen, Harms, Jan, Allocca, Annalisa, Calloni, Enrico, De Rosa, Rosario, Errico, Luciano, Esposito, Marina, Badaracco, Francesca, Rei, Luca, Bertolini, Alessandro, Bulik, Tomasz, Cieslar, Marek, Pietrzak, Mateusz, Suchenek, Mariusz, Fiori, Irene, Paoli, Andrea, Tringali, Maria Concetta, Ruggi, Paolo, Hild, Stefan, Singha, Ayatri, Idzkowski, Bartosz, Suchinski, Maciej, Masserot, Alain, Rolland, Loic, Mours, Benoit, Paoletti, Federico
Terrestrial gravity perturbations caused by seismic fields produce the so-called Newtonian noise in gravitational-wave detectors, which is predicted to limit their sensitivity in the upcoming observing runs. In the past, this noise was seen as an inf
Externí odkaz:
http://arxiv.org/abs/2310.17781
Autor:
Allocca, Annalisa, Avino, Saverio, Balestrieri, Sergio, Calloni, Enrico, Caprara, Sergio, Carpinelli, Massimo, D'Onofrio, Luca, D'Urso, Domenico, De Rosa, Rosario, Errico, Luciano, Gagliardi, Gianluca, Grilli, Marco, Mangano, Valentina, Marsella, Maria, Naticchioni, Luca, Pasqualetti, Antonio, Pepe, Giovanni Piero, Perciballi, Maurizio, Pesenti, Luca, Puppo, Paola, Rapagnani, Piero, Ricci, Fulvio, Rosa, Luigi, Rovelli, Carlo, Rozza, Davide, Ruggi, Paolo, Saini, Naurang, Sequino, Valeria, Sipala, Valeria, Stornaiuolo, Daniela, Tafuri, Francesco, Tagliacozzo, Arturo, Melo, Iara Tosta e, Trozzo, Lucia
We provide a novel methodological approach to the estimate of the change of the Quantum Vacuum electromagnetic energy density in a High critical Temperature superconducting metal bulk sample, when it undergoes the transition in temperature, from the
Externí odkaz:
http://arxiv.org/abs/2209.10593
Autor:
Arnaud, Nicolas, De Rosa, Rosario, Di Renzo, Francesco, Fiori, Irene, Giunchi, Carlo, Janssens, Kamiel, Longo, Alessandro, Olivieri, Marco, Paoletti, Federico, Ruggi, Paolo, Tringali, Maria Concetta
Sources of geophysical noise, such as wind, sea waves and earthquakes, can have an impact on gravitational wave interferometers causing sensitivity worsening and gaps in data taking. During the 1-year long O3 run (April 1st 2019 to March 27th 2020),
Externí odkaz:
http://arxiv.org/abs/2204.03993
Autor:
Harms, Jan, Naticchioni, Luca, Calloni, Enrico, De Rosa, Rosario, Ricci, Fulvio, D'Urso, Domenico
The Einstein Telescope (ET) is a proposed third-generation gravitational-wave (GW) underground observatory. It will have greatly increased sensitivity compared to current GW detectors, and it is designed to extend the observation band down to a few H
Externí odkaz:
http://arxiv.org/abs/2202.12841
Autor:
Garaventa, Barbara, Sequino, Valeria, Ali, Wajid, Sorrentino, Fiodor, Zendri, Jean-Pierre, Chincarini, Andrea, Fiori, Irene, Armato, Federico, De Rosa, Rosario, Graziaplena, Mario, Paoletti, Federico, Quéméner, Gilles, Tringali, Maria Concetta
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A September 2024 1066
