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  1. Article: Earthquake Early Warning Using Future Generation Gravity Strainmeters

    Juhel, K. / Ampuero, J. P. / Barsuglia, M. / Bernard, P. / Chassande‐Mottin, E. / Fiorucci, D. / Harms, J. / Montagner, J.‐P. / Vallée, M. / Whiting, B. F.

    Journal of geophysical research. 2018 Dec., v. 123, no. 12

    2018  

    Abstract: Recent studies reported the observation of prompt elastogravity signals during the 2011 M9.1 Tohoku earthquake, recorded with broadband seismometers and gravimeter between the rupture onset and the arrival of the seismic waves. Here we show that to ... ...

    Abstract Recent studies reported the observation of prompt elastogravity signals during the 2011 M9.1 Tohoku earthquake, recorded with broadband seismometers and gravimeter between the rupture onset and the arrival of the seismic waves. Here we show that to extend the range of magnitudes over which the gravity perturbations can be observed and reduce the time needed for their detection, high‐precision gravity strainmeters under development could be used, such as torsion bars, superconducting gradiometers, or strainmeters based on atom interferometers. These instruments measure the differential gravitational acceleration between two seismically isolated test masses and are initially designed to observe gravitational waves around 0.1 Hz. Our analysis involves simulations of the expected gravity strain signals generated by fault rupture, based on an analytical model of gravity perturbations in a homogeneous half‐space. We show that future gravity strainmeters should be able to detect prompt gravity perturbations induced by earthquakes larger than M7, up to 1,000 km from the earthquake centroid within P waves travel time and up to 120 km within the first 10 s of rupture onset, provided a sensitivity in gravity strain of 10⁻¹⁵ Hz⁻¹/² at 0.1 Hz can be achieved. Our results further suggest that, in comparison to conventional P wave‐based earthquake‐early warning systems, gravity‐based earthquake‐early warning systems could perform faster detections of large offshore subduction earthquakes (at least larger than M7.3). Gravity strainmeters could also perform earlier magnitude estimates, within the duration of the fault rupture, and therefore complement current tsunami warning systems.
    Keywords earthquakes ; geophysics ; gravity ; models ; research ; subduction ; tsunamis
    Language English
    Dates of publication 2018-12
    Size p. 10,889-10,902.
    Publishing place John Wiley & Sons, Ltd
    Document type Article
    Note JOURNAL ARTICLE
    ISSN 2169-9313
    DOI 10.1029/2018JB016698
    Database NAL-Catalogue (AGRICOLA)

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  2. Article ; Online: Compact radio emission indicates a structured jet was produced by a binary neutron star merger.

    Ghirlanda, G / Salafia, O S / Paragi, Z / Giroletti, M / Yang, J / Marcote, B / Blanchard, J / Agudo, I / An, T / Bernardini, M G / Beswick, R / Branchesi, M / Campana, S / Casadio, C / Chassande-Mottin, E / Colpi, M / Covino, S / D'Avanzo, P / D'Elia, V /
    Frey, S / Gawronski, M / Ghisellini, G / Gurvits, L I / Jonker, P G / van Langevelde, H J / Melandri, A / Moldon, J / Nava, L / Perego, A / Perez-Torres, M A / Reynolds, C / Salvaterra, R / Tagliaferri, G / Venturi, T / Vergani, S D / Zhang, M

    Science (New York, N.Y.)

    2019  Volume 363, Issue 6430, Page(s) 968–971

    Abstract: The binary neutron star merger event GW170817 was detected through both electromagnetic radiation and gravitational waves. Its afterglow emission may have been produced by either a narrow relativistic jet or an isotropic outflow. High-spatial-resolution ... ...

    Abstract The binary neutron star merger event GW170817 was detected through both electromagnetic radiation and gravitational waves. Its afterglow emission may have been produced by either a narrow relativistic jet or an isotropic outflow. High-spatial-resolution measurements of the source size and displacement can discriminate between these scenarios. We present very-long-baseline interferometry observations, performed 207.4 days after the merger by using a global network of 32 radio telescopes. The apparent source size is constrained to be smaller than 2.5 milli-arc seconds at the 90% confidence level. This excludes the isotropic outflow scenario, which would have produced a larger apparent size, indicating that GW170817 produced a structured relativistic jet. Our rate calculations show that at least 10% of neutron star mergers produce such a jet.
    Language English
    Publishing date 2019-02-21
    Publishing country United States
    Document type Journal Article
    ZDB-ID 128410-1
    ISSN 1095-9203 ; 0036-8075
    ISSN (online) 1095-9203
    ISSN 0036-8075
    DOI 10.1126/science.aau8815
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  3. Article ; Online: Prompt gravity signal induced by the 2011 Tohoku-Oki earthquake.

    Montagner, Jean-Paul / Juhel, Kévin / Barsuglia, Matteo / Ampuero, Jean Paul / Chassande-Mottin, Eric / Harms, Jan / Whiting, Bernard / Bernard, Pascal / Clévédé, Eric / Lognonné, Philippe

    Nature communications

    2016  Volume 7, Page(s) 13349

    Abstract: Transient gravity changes are expected to occur at all distances during an earthquake rupture, even before the arrival of seismic waves. Here we report on the search of such a prompt gravity signal in data recorded by a superconducting gravimeter and ... ...

    Abstract Transient gravity changes are expected to occur at all distances during an earthquake rupture, even before the arrival of seismic waves. Here we report on the search of such a prompt gravity signal in data recorded by a superconducting gravimeter and broadband seismometers during the 2011 Mw 9.0 Tohoku-Oki earthquake. During the earthquake rupture, a signal exceeding the background noise is observed with a statistical significance higher than 99% and an amplitude of a fraction of μGal, consistent in sign and order of magnitude with theoretical predictions from a first-order model. While prompt gravity signal detection with state-of-the-art gravimeters and seismometers is challenged by background seismic noise, its robust detection with gravity gradiometers under development could open new directions in earthquake seismology, and overcome fundamental limitations of current earthquake early-warning systems imposed by the propagation speed of seismic waves.
    Language English
    Publishing date 2016-11-22
    Publishing country England
    Document type Journal Article ; Research Support, U.S. Gov't, Non-P.H.S.
    ISSN 2041-1723
    ISSN (online) 2041-1723
    DOI 10.1038/ncomms13349
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  4. Article ; Online: Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger.

    Pian, E / D'Avanzo, P / Benetti, S / Branchesi, M / Brocato, E / Campana, S / Cappellaro, E / Covino, S / D'Elia, V / Fynbo, J P U / Getman, F / Ghirlanda, G / Ghisellini, G / Grado, A / Greco, G / Hjorth, J / Kouveliotou, C / Levan, A / Limatola, L /
    Malesani, D / Mazzali, P A / Melandri, A / Møller, P / Nicastro, L / Palazzi, E / Piranomonte, S / Rossi, A / Salafia, O S / Selsing, J / Stratta, G / Tanaka, M / Tanvir, N R / Tomasella, L / Watson, D / Yang, S / Amati, L / Antonelli, L A / Ascenzi, S / Bernardini, M G / Boër, M / Bufano, F / Bulgarelli, A / Capaccioli, M / Casella, P / Castro-Tirado, A J / Chassande-Mottin, E / Ciolfi, R / Copperwheat, C M / Dadina, M / De Cesare, G / Di Paola, A / Fan, Y Z / Gendre, B / Giuffrida, G / Giunta, A / Hunt, L K / Israel, G L / Jin, Z-P / Kasliwal, M M / Klose, S / Lisi, M / Longo, F / Maiorano, E / Mapelli, M / Masetti, N / Nava, L / Patricelli, B / Perley, D / Pescalli, A / Piran, T / Possenti, A / Pulone, L / Razzano, M / Salvaterra, R / Schipani, P / Spera, M / Stamerra, A / Stella, L / Tagliaferri, G / Testa, V / Troja, E / Turatto, M / Vergani, S D / Vergani, D

    Nature

    2017  Volume 551, Issue 7678, Page(s) 67–70

    Abstract: The merger of two neutron stars is predicted to give rise to three major detectable phenomena: a short burst of γ-rays, a gravitational-wave signal, and a transient optical-near-infrared source powered by the synthesis of large amounts of very heavy ... ...

    Abstract The merger of two neutron stars is predicted to give rise to three major detectable phenomena: a short burst of γ-rays, a gravitational-wave signal, and a transient optical-near-infrared source powered by the synthesis of large amounts of very heavy elements via rapid neutron capture (the r-process). Such transients, named 'macronovae' or 'kilonovae', are believed to be centres of production of rare elements such as gold and platinum. The most compelling evidence so far for a kilonova was a very faint near-infrared rebrightening in the afterglow of a short γ-ray burst at redshift z = 0.356, although findings indicating bluer events have been reported. Here we report the spectral identification and describe the physical properties of a bright kilonova associated with the gravitational-wave source GW170817 and γ-ray burst GRB 170817A associated with a galaxy at a distance of 40 megaparsecs from Earth. Using a series of spectra from ground-based observatories covering the wavelength range from the ultraviolet to the near-infrared, we find that the kilonova is characterized by rapidly expanding ejecta with spectral features similar to those predicted by current models. The ejecta is optically thick early on, with a velocity of about 0.2 times light speed, and reaches a radius of about 50 astronomical units in only 1.5 days. As the ejecta expands, broad absorption-like lines appear on the spectral continuum, indicating atomic species produced by nucleosynthesis that occurs in the post-merger fast-moving dynamical ejecta and in two slower (0.05 times light speed) wind regions. Comparison with spectral models suggests that the merger ejected 0.03 to 0.05 solar masses of material, including high-opacity lanthanides.
    Language English
    Publishing date 2017-11-02
    Publishing country England
    Document type Journal Article
    ZDB-ID 120714-3
    ISSN 1476-4687 ; 0028-0836
    ISSN (online) 1476-4687
    ISSN 0028-0836
    DOI 10.1038/nature24298
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  5. Article ; Online: Frequency-Dependent Squeezed Vacuum Source for the Advanced Virgo Gravitational-Wave Detector.

    Acernese, F / Agathos, M / Ain, A / Albanesi, S / Alléné, C / Allocca, A / Amato, A / Amra, C / Andia, M / Andrade, T / Andres, N / Andrés-Carcasona, M / Andrić, T / Ansoldi, S / Antier, S / Apostolatos, T / Appavuravther, E Z / Arène, M / Arnaud, N /
    Assiduo, M / Melo, S Assis de Souza / Astone, P / Aubin, F / Babak, S / Badaracco, F / Bagnasco, S / Baird, J / Baka, T / Ballardin, G / Baltus, G / Banerjee, B / Barneo, P / Barone, F / Barsuglia, M / Barta, D / Basti, A / Bawaj, M / Bazzan, M / Beirnaert, F / Bejger, M / Benedetto, V / Berbel, M / Bernuzzi, S / Bersanetti, D / Bertolini, A / Bhardwaj, U / Bianchi, A / Bilicki, M / Bini, S / Bischi, M / Bitossi, M / Bizouard, M-A / Bobba, F / Boër, M / Bogaert, G / Boileau, G / Boldrini, M / Bonavena, L D / Bondarescu, R / Bondu, F / Bonnand, R / Boschi, V / Boudart, V / Bouffanais, Y / Bozzi, A / Bradaschia, C / Braglia, M / Branchesi, M / Breschi, M / Briant, T / Brillet, A / Brooks, J / Bruno, G / Bucci, F / Bulashenko, O / Bulik, T / Bulten, H J / Buscicchio, R / Buskulic, D / Buy, C / Cabras, G / Cabrita, R / Cagnoli, G / Calloni, E / Canepa, M / Santoro, G Caneva / Cannavacciuolo, M / Capocasa, E / Carapella, G / Carbognani, F / Carpinelli, M / Carullo, G / Diaz, J Casanueva / Casentini, C / Caudill, S / Cavalieri, R / Cella, G / Cerdá-Durán, P / Cesarini, E / Chaibi, W / Chanial, P / Chassande-Mottin, E / Chaty, S / Chessa, P / Chiadini, F / Chiarini, G / Chierici, R / Chincarini, A / Chiofalo, M L / Chiummo, A / Christensen, N / Chua, S / Ciani, G / Ciecielag, P / Cieślar, M / Cifaldi, M / Ciolfi, R / Clesse, S / Cleva, F / Coccia, E / Codazzo, E / Cohadon, P-F / Colombo, A / Colpi, M / Conti, L / Cordero-Carrión, I / Corezzi, S / Cortese, S / Coulon, J-P / Coupechoux, J-F / Croquette, M / Cudell, J R / Cuoco, E / Curyło, M / Dabadie, P / Canton, T Dal / Dall'Osso, S / Dálya, G / D'Angelo, B / Dangoisse, G / Danilishin, S / D'Antonio, S / Dattilo, V / Davier, M / Degallaix, J / De Laurentis, M / Deléglise, S / De Lillo, F / Dell'Aquila, D / Del Pozzo, W / De Matteis, F / Depasse, A / De Pietri, R / De Rosa, R / De Rossi, C / De Simone, R / Di Fiore, L / Di Giorgio, C / Di Giovanni, F / Di Giovanni, M / Di Girolamo, T / Diksha, D / Di Lieto, A / Di Michele, A / Ding, J / Di Pace, S / Di Palma, I / Di Renzo, F / D'Onofrio, L / Dooney, T / Dorosh, O / Drago, M / Ducoin, J-G / Dupletsa, U / Durante, O / D'Urso, D / Duverne, P-A / Eisenmann, M / Errico, L / Estevez, D / Fabrizi, F / Faedi, F / Fafone, V / Favaro, G / Fays, M / Fenyvesi, E / Ferrante, I / Fidecaro, F / Figura, P / Fiori, A / Fiori, I / Fittipaldi, R / Fiumara, V / Flaminio, R / Font, J A / Frasca, S / Frasconi, F / Freise, A / Freitas, O / Fronzé, G G / Gadre, B / Gamba, R / Garaventa, B / Garcia-Bellido, J / Gargiulo, J / Garufi, F / Gasbarra, C / Gemme, G / Gennai, A / Ghosh, Archisman / Giacoppo, L / Giri, P / Gissi, F / Gkaitatzis, S / Glotin, F / Goncharov, B / Gosselin, M / Gouaty, R / Grado, A / Granata, M / Granata, V / Greco, G / Grignani, G / Grimaldi, A / Guerra, D / Guetta, D / Guidi, G M / Gulminelli, F / Guo, Y / Gupta, P / Gutierrez, N / Haegel, L / Halim, O / Hannuksela, O / Harder, T / Haris, K / Harmark, T / Harms, J / Haskell, B / Heidmann, A / Heitmann, H / Hello, P / Hemming, G / Hennes, E / Hennig, J-S / Hennig, M / Hild, S / Hofman, D / Holland, N A / Hui, V / Iandolo, G A / Idzkowski, B / Iess, A / Iorio, G / Iosif, P / Jacqmin, T / Jacquet, P-E / Janquart, J / Janssens, K / Jaraba, S / Jaranowski, P / Jasal, P / Juste, V / Kalaghatgi, C / Karathanasis, C / Katsanevas, S / Kéfélian, F / Koekoek, G / Koley, S / Kolstein, M / Kranzhoff, S L / Królak, A / Kuijer, P / Kuroyanagi, S / Lagabbe, P / Laghi, D / Lalleman, M / Lamberts, A / La Rana, A / La Rosa, I / Lartaux-Vollard, A / Lazzaro, C / Leaci, P / Lemaître, A / Lenti, M / Leonova, E / Lequime, M / Leroy, N / Letendre, N / Lethuillier, M / Leyde, K / Linde, F / London, L / Longo, A / Portilla, M Lopez / Lorenzini, M / Loriette, V / Losurdo, G / Lumaca, D / Macquet, A / Magazzù, C / Maggiore, R / Magnozzi, M / Majorana, E / Man, N / Mangano, V / Mantovani, M / Mapelli, M / Marchesoni, F / Pina, D Marín / Marion, F / Marquina, A / Marsat, S / Martelli, F / Martinez, M / Martinez, V / Masserot, A / Mastrodicasa, M / Mastrogiovanni, S / Meijer, Q / Menendez-Vazquez, A / Mereni, L / Merzougui, M / Miani, A / Michel, C / Miller, A / Miller, B / Milotti, E / Minenkov, Y / Mir, Ll M / Miravet-Tenés, M / Mitchell, A L / Mondal, C / Montani, M / Morawski, F / Morras, G / Moscatello, A / Mours, B / Mow-Lowry, C M / Msihid, E / Muciaccia, F / Mukherjee, Suvodip / Nagar, A / Napolano, V / Nardecchia, I / Narola, H / Naticchioni, L / Neilson, J / Nesseris, S / Nguyen, C / Nieradka, G / Nissanke, S / Nitoglia, E / Nocera, F / Novak, J / No Siles, J F Nu / Oertel, M / Oganesyan, G / Oliveri, R / Orselli, M / Palomba, C / Pang, P T H / Pannarale, F / Paoletti, F / Paoli, A / Paolone, A / Pappas, G / Parisi, A / Pascucci, D / Pasqualetti, A / Passaquieti, R / Passuello, D / Patricelli, B / Pedurand, R / Pegna, R / Pegoraro, M / Perego, A / Pereira, A / Périgois, C / Perreca, A / Perriès, S / Perry, J W / Pesios, D / Petrillo, C / Phukon, K S / Piccinni, O J / Pichot, M / Piendibene, M / Piergiovanni, F / Pierini, L / Pierra, G / Pierro, V / Pillant, G / Pillas, M / Pilo, F / Pinard, L / Pinto, I M / Pinto, M / Piotrzkowski, K / Placidi, A / Placidi, E / Plastino, W / Poggiani, R / Polini, E / Porcelli, E / Portell, J / Porter, E K / Poulton, R / Pracchia, M / Pradier, T / Principe, M / Prodi, G A / Prosposito, P / Puecher, A / Punturo, M / Puosi, F / Puppo, P / Raaijmakers, G / Radulesco, N / Rapagnani, P / Razzano, M / Regimbau, T / Rei, L / Rettegno, P / Revenu, B / Reza, A / Rezaei, A S / Ricci, F / Rinaldi, S / Robinet, F / Rocchi, A / Rolland, L / Romanelli, M / Romano, R / Romero, A / Ronchini, S / Rosa, L / Rosińska, D / Roy, S / Rozza, D / Ruggi, P / Morales, E Ruiz / Saffarieh, P / Salafia, O S / Salconi, L / Salemi, F / Sallé, M / Samajdar, A / Sanchis-Gual, N / Sanuy, A / Sasli, A / Sassi, P / Sassolas, B / Sayah, S / Schmidt, S / Seglar-Arroyo, M / Sentenac, D / Sequino, V / Servignat, G / Setyawati, Y / Shcheblanov, N S / Sieniawska, M / Silenzi, L / Singh, N / Singha, A / Sipala, V / Soldateschi, J / Sordini, V / Sorrentino, F / Sorrentino, N / Soulard, R / Spagnuolo, V / Spera, M / Spinicelli, P / Stachie, C / Steer, D A / Steinlechner, J / Steinlechner, S / Stergioulas, N / Stratta, G / Suchenek, M / Sur, A / Suresh, J / Swinkels, B L / Syx, A / Szewczyk, P / Tacca, M / Tamanini, N / Tanasijczuk, A J / Martín, E N Tapia San / Taranto, C / Tonelli, M / Torres-Forné, A / E Melo, I Tosta / Tournefier, E / Trapananti, A / Travasso, F / Trenado, J / Tringali, M C / Troiano, L / Trovato, A / Trozzo, L / Tsang, K W / Turbang, K / Turconi, M / Turski, C / Ubach, H / Utina, A / Valentini, M / Vallero, S / van Bakel, N / van Beuzekom, M / van Dael, M / van den Brand, J F J / Van Den Broeck, C / van der Sluys, M / Van de Walle, A / van Dongen, J / van Haevermaet, H / van Heijningen, J V / van Ranst, Z / van Remortel, N / Vardaro, M / Vasúth, M / Vedovato, G / Verdier, P / Verkindt, D / Verma, P / Vetrano, F / Viceré, A / Vinet, J-Y / Viret, S / Virtuoso, A / Vocca, H / Walet, R C / Was, M / Yadav, N / Zadrożny, A / Zelenova, T / Zendri, J-P / Zhao, Y / Zerrad, M / Vahlbruch, H / Mehmet, M / Lück, H / Danzmann, K

    Physical review letters

    2023  Volume 131, Issue 4, Page(s) 41403

    Abstract: In this Letter, we present the design and performance of the frequency-dependent squeezed vacuum source that will be used for the broadband quantum noise reduction of the Advanced Virgo Plus gravitational-wave detector in the upcoming observation run. ... ...

    Abstract In this Letter, we present the design and performance of the frequency-dependent squeezed vacuum source that will be used for the broadband quantum noise reduction of the Advanced Virgo Plus gravitational-wave detector in the upcoming observation run. The frequency-dependent squeezed field is generated by a phase rotation of a frequency-independent squeezed state through a 285 m long, high-finesse, near-detuned optical resonator. With about 8.5 dB of generated squeezing, up to 5.6 dB of quantum noise suppression has been measured at high frequency while close to the filter cavity resonance frequency, the intracavity losses limit this value to about 2 dB. Frequency-dependent squeezing is produced with a rotation frequency stability of about 6 Hz rms, which is maintained over the long term. The achieved results fulfill the frequency dependent squeezed vacuum source requirements for Advanced Virgo Plus. With the current squeezing source, considering also the estimated squeezing degradation induced by the interferometer, we expect a reduction of the quantum shot noise and radiation pressure noise of up to 4.5 dB and 2 dB, respectively.
    Language English
    Publishing date 2023-07-05
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.131.041403
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  6. Article ; Online: Quantum Backaction on kg-Scale Mirrors: Observation of Radiation Pressure Noise in the Advanced Virgo Detector.

    Acernese, F / Agathos, M / Aiello, L / Ain, A / Allocca, A / Amato, A / Ansoldi, S / Antier, S / Arène, M / Arnaud, N / Ascenzi, S / Astone, P / Aubin, F / Babak, S / Badaracco, F / Bader, M K M / Bagnasco, S / Baird, J / Ballardin, G /
    Baltus, G / Barbieri, C / Barneo, P / Barone, F / Barsuglia, M / Barta, D / Basti, A / Bawaj, M / Bazzan, M / Bejger, M / Belahcene, I / Bernuzzi, S / Bersanetti, D / Bertolini, A / Bischi, M / Bitossi, M / Bizouard, M-A / Blanch, O / Bobba, F / Boer, M / Bogaert, G / Boldrini, M / Bondu, F / Bonnand, R / Boom, B A / Boschi, V / Boudart, V / Bouffanais, Y / Bozzi, A / Bradaschia, C / Branchesi, M / Breschi, M / Briant, T / Brighenti, F / Brillet, A / Brooks, J / Bruno, G / Bulik, T / Bulten, H J / Buskulic, D / Cagnoli, G / Calloni, E / Canepa, M / Carapella, G / Carbognani, F / Carpinelli, M / Carullo, G / Diaz, J Casanueva / Casentini, C / Caudill, S / Cavalier, F / Cavalieri, R / Cella, G / Cerdá-Durán, P / Cesarini, E / Chaibi, W / Chanial, P / Chassande-Mottin, E / Chiadini, F / Chierici, R / Chincarini, A / Chiummo, A / Christensen, N / Chua, S / Ciani, G / Ciecielag, P / Cieślar, M / Cifaldi, M / Ciolfi, R / Cipriano, F / Cirone, A / Clesse, S / Cleva, F / Coccia, E / Cohadon, P-F / Cohen, D E / Colpi, M / Conti, L / Cordero-Carrión, I / Corezzi, S / Corre, D / Cortese, S / Coulon, J-P / Croquette, M / Cudell, J R / Cuoco, E / Curylo, M / D'Angelo, B / D'Antonio, S / D'Onofrio, L / D'Urso, D / Canton, T Dal / Dattilo, V / Davier, M / De Laurentis, M / De Matteis, F / De Pietri, R / De Rosa, R / De Rossi, C / Degallaix, J / Del Pozzo, W / Deléglise, S / Depasse, A / Di Fiore, L / Di Giorgio, C / Di Giovanni, F / Di Giovanni, M / Di Girolamo, T / Di Lieto, A / Di Pace, S / Di Palma, I / Di Renzo, F / Dietrich, T / Drago, M / Ducoin, J-G / Durante, O / Duverne, P-A / Eisenmann, M / Errico, L / Estevez, D / Fafone, V / Farinon, S / Fays, M / Feng, F / Fenyvesi, E / Ferrante, I / Fidecaro, F / Figura, P / Fiori, I / Fiorucci, D / Fittipaldi, R / Fiumara, V / Flaminio, R / Font, J A / Fournier, J-D / Frasca, S / Frasconi, F / Frey, V / Fronzé, G G / Gamba, R / Garaventa, B / Garufi, F / Gemme, G / Gennai, A / Ghosh, Archisman / Giacomazzo, B / Giacoppo, L / Giri, P / Gosselin, M / Gouaty, R / Grado, A / Granata, M / Granata, V / Greco, G / Grignani, G / Grimaldi, A / Grimm, S J / Gruning, P / Guidi, G M / Guixé, G / Guo, Y / Gupta, P / Haegel, L / Halim, O / Hannuksela, O / Harder, T / Haris, K / Harms, J / Heidmann, A / Heitmann, H / Hello, P / Hemming, G / Hennes, E / Hofman, D / Hui, V / Idzkowski, B / Iess, A / Intini, G / Jacqmin, T / Janssens, K / Jaranowski, P / Jonker, R J G / Karathanasis, C / Katsanevas, S / Kéfélian, F / Khan, I / Khetan, N / Koekoek, G / Koley, S / Kolstein, M / Królak, A / La Rosa, I / Laghi, D / Lamberts, A / Lartaux-Vollard, A / Lazzaro, C / Leaci, P / Leroy, N / Letendre, N / Linde, F / Llorens-Monteagudo, M / Longo, A / Lorenzini, M / Loriette, V / Losurdo, G / Lumaca, D / Macquet, A / Magazzù, C / Majorana, E / Maksimovic, I / Man, N / Mangano, V / Mantovani, M / Mapelli, M / Marchesoni, F / Marion, F / Marquina, A / Marsat, S / Martelli, F / Martinez, M / Martinez, V / Masserot, A / Mastrogiovanni, S / Menendez-Vazquez, A / Mereni, L / Merzougui, M / Metzdorff, R / Miani, A / Michel, C / Milano, L / Miller, A / Milotti, E / Minazzoli, O / Minenkov, Y / Mir, Ll M / Montani, M / Morawski, F / Mours, B / Muciaccia, F / Nagar, A / Nardecchia, I / Naticchioni, L / Neilson, J / Nelemans, G / Nguyen, C / Nissanke, S / Nocera, F / Oganesyan, G / Olivetto, C / Pagano, G / Pagliaroli, G / Palomba, C / Pang, T H / Pannarale, F / Paoletti, F / Paoli, A / Paolone, A / Pascucci, D / Pasqualetti, A / Passaquieti, R / Passuello, D / Patricelli, B / Pegoraro, M / Perego, A / Périgois, C / Perreca, A / Perriès, S / Phukon, K S / Piccinni, O J / Pichot, M / Piendibene, M / Piergiovanni, F / Pierini, L / Pierro, V / Pillant, G / Pilo, F / Pinard, L / Pinto, I M / Piotrzkowski, K / Placidi, E / Plastino, W / Poggiani, R / Polini, E / Popolizio, P / Porter, E K / Pracchia, M / Principe, M / Prodi, G A / Prosposito, P / Puecher, A / Punturo, M / Puosi, F / Puppo, P / Raaijmakers, G / Radulesco, N / Rapagnani, P / Razzano, M / Regimbau, T / Rei, L / Rettegno, P / Ricci, F / Riemenschneider, G / Robinet, F / Rocchi, A / Rolland, L / Romanelli, M / Romano, R / Romero, A / Ronchini, S / Rosińska, D / Ruggi, P / Salafia, O S / Salconi, L / Samajdar, A / Sanchis-Gual, N / Santos, E / Sassolas, B / Sauter, O / Sayah, S / Seglar-Arroyo, M / Sentenac, D / Sequino, V / Sharma, A / Sieniawska, M / Singh, N / Singhal, A / Sipala, V / Sordini, V / Sorrentino, F / Sorrentino, N / Soulard, R / Spera, M / Stachie, C / Steer, D A / Stratta, G / Sur, A / Swinkels, B L / Tacca, M / Tanasijczuk, A J / Martin, E N Tapia San / Tonelli, M / Torres-Forné, A / Tosta E Melo, I / Trapananti, A / Travasso, F / Tringali, M C / Trovato, A / Tsang, K W / Turconi, M / Valentini, M / van Bakel, N / van Beuzekom, M / van den Brand, J F J / Van Den Broeck, C / van der Schaaf, L / Vardaro, M / Vasúth, M / Vedovato, G / Verkindt, D / Vetrano, F / Viceré, A / Vinet, J-Y / Vocca, H / Walet, R C / Was, M / Zadrożny, A / Zelenova, T / Zendri, J-P / Mehmet, M / Vahlbruch, H / Lück, H / Danzmann, K

    Physical review letters

    2020  Volume 125, Issue 13, Page(s) 131101

    Abstract: The quantum radiation pressure and the quantum shot noise in laser-interferometric gravitational wave detectors constitute a macroscopic manifestation of the Heisenberg inequality. If quantum shot noise can be easily observed, the observation of quantum ... ...

    Abstract The quantum radiation pressure and the quantum shot noise in laser-interferometric gravitational wave detectors constitute a macroscopic manifestation of the Heisenberg inequality. If quantum shot noise can be easily observed, the observation of quantum radiation pressure noise has been elusive, so far, due to the technical noise competing with quantum effects. Here, we discuss the evidence of quantum radiation pressure noise in the Advanced Virgo gravitational wave detector. In our experiment, we inject squeezed vacuum states of light into the interferometer in order to manipulate the quantum backaction on the 42 kg mirrors and observe the corresponding quantum noise driven displacement at frequencies between 30 and 70 Hz. The experimental data, obtained in various interferometer configurations, is tested against the Advanced Virgo detector quantum noise model which confirmed the measured magnitude of quantum radiation pressure noise.
    Language English
    Publishing date 2020-10-09
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.125.131101
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  7. Article ; Online: Increasing the Astrophysical Reach of the Advanced Virgo Detector via the Application of Squeezed Vacuum States of Light.

    Acernese, F / Agathos, M / Aiello, L / Allocca, A / Amato, A / Ansoldi, S / Antier, S / Arène, M / Arnaud, N / Ascenzi, S / Astone, P / Aubin, F / Babak, S / Bacon, P / Badaracco, F / Bader, M K M / Baird, J / Baldaccini, F / Ballardin, G /
    Baltus, G / Barbieri, C / Barneo, P / Barone, F / Barsuglia, M / Barta, D / Basti, A / Bawaj, M / Bazzan, M / Bejger, M / Belahcene, I / Bernuzzi, S / Bersanetti, D / Bertolini, A / Bischi, M / Bitossi, M / Bizouard, M A / Bobba, F / Boer, M / Bogaert, G / Bondu, F / Bonnand, R / Boom, B A / Boschi, V / Bouffanais, Y / Bozzi, A / Bradaschia, C / Branchesi, M / Breschi, M / Briant, T / Brighenti, F / Brillet, A / Brooks, J / Bruno, G / Bulik, T / Bulten, H J / Buskulic, D / Cagnoli, G / Calloni, E / Canepa, M / Carapella, G / Carbognani, F / Carullo, G / Casanueva Diaz, J / Casentini, C / Castañeda, J / Caudill, S / Cavalier, F / Cavalieri, R / Cella, G / Cerdá-Durán, P / Cesarini, E / Chaibi, O / Chassande-Mottin, E / Chiadini, F / Chierici, R / Chincarini, A / Chiummo, A / Christensen, N / Chua, S / Ciani, G / Ciecielag, P / Cieślar, M / Ciolfi, R / Cipriano, F / Cirone, A / Clesse, S / Cleva, F / Coccia, E / Cohadon, P-F / Cohen, D / Colpi, M / Conti, L / Cordero-Carrión, I / Corezzi, S / Corre, D / Cortese, S / Coulon, J-P / Croquette, M / Cudell, J-R / Cuoco, E / Curylo, M / D'Angelo, B / D'Antonio, S / Dattilo, V / Davier, M / Degallaix, J / De Laurentis, M / Deléglise, S / Del Pozzo, W / De Pietri, R / De Rosa, R / De Rossi, C / Dietrich, T / Di Fiore, L / Di Giorgio, C / Di Giovanni, F / Di Giovanni, M / Di Girolamo, T / Di Lieto, A / Di Pace, S / Di Palma, I / Di Renzo, F / Drago, M / Ducoin, J-G / Durante, O / D'Urso, D / Eisenmann, M / Errico, L / Estevez, D / Fafone, V / Farinon, S / Feng, F / Fenyvesi, E / Ferrante, I / Fidecaro, F / Fiori, I / Fiorucci, D / Fittipaldi, R / Fiumara, V / Flaminio, R / Font, J A / Fournier, J-D / Frasca, S / Frasconi, F / Frey, V / Fronzè, G / Garufi, F / Gemme, G / Genin, E / Gennai, A / Ghosh, Archisman / Giacomazzo, B / Gosselin, M / Gouaty, R / Grado, A / Granata, M / Greco, G / Grignani, G / Grimaldi, A / Grimm, S J / Gruning, P / Guidi, G M / Guixé, G / Guo, Y / Gupta, P / Halim, O / Harder, T / Harms, J / Heidmann, A / Heitmann, H / Hello, P / Hemming, G / Hennes, E / Hinderer, T / Hofman, D / Huet, D / Hui, V / Idzkowski, B / Iess, A / Intini, G / Isac, J-M / Jacqmin, T / Jaranowski, P / Jonker, R J G / Katsanevas, S / Kéfélian, F / Khan, I / Khetan, N / Koekoek, G / Koley, S / Królak, A / Kutynia, A / Laghi, D / Lamberts, A / La Rosa, I / Lartaux-Vollard, A / Lazzaro, C / Leaci, P / Leroy, N / Letendre, N / Linde, F / Llorens-Monteagudo, M / Longo, A / Lorenzini, M / Loriette, V / Losurdo, G / Lumaca, D / Macquet, A / Majorana, E / Maksimovic, I / Man, N / Mangano, V / Mantovani, M / Mapelli, M / Marchesoni, F / Marion, F / Marquina, A / Marsat, S / Martelli, F / Martinez, V / Masserot, A / Mastrogiovanni, S / Mejuto Villa, E / Mereni, L / Merzougui, M / Metzdorff, R / Miani, A / Michel, C / Milano, L / Miller, A / Milotti, E / Minazzoli, O / Minenkov, Y / Montani, M / Morawski, F / Mours, B / Muciaccia, F / Nagar, A / Nardecchia, I / Naticchioni, L / Neilson, J / Nelemans, G / Nguyen, C / Nichols, D / Nissanke, S / Nocera, F / Oganesyan, G / Olivetto, C / Pagano, G / Pagliaroli, G / Palomba, C / Pang, P T H / Pannarale, F / Paoletti, F / Paoli, A / Pascucci, D / Pasqualetti, A / Passaquieti, R / Passuello, D / Patricelli, B / Perego, A / Pegoraro, M / Périgois, C / Perreca, A / Perriès, S / Phukon, K S / Piccinni, O J / Pichot, M / Piendibene, M / Piergiovanni, F / Pierro, V / Pillant, G / Pinard, L / Pinto, I M / Piotrzkowski, K / Plastino, W / Poggiani, R / Popolizio, P / Porter, E K / Prevedelli, M / Principe, M / Prodi, G A / Punturo, M / Puppo, P / Raaijmakers, G / Radulesco, N / Rapagnani, P / Razzano, M / Regimbau, T / Rei, L / Rettegno, P / Ricci, F / Riemenschneider, G / Robinet, F / Rocchi, A / Rolland, L / Romanelli, M / Romano, R / Rosińska, D / Ruggi, P / Salafia, O S / Salconi, L / Samajdar, A / Sanchis-Gual, N / Santos, E / Sassolas, B / Sauter, O / Sayah, S / Sentenac, D / Sequino, V / Sharma, A / Sieniawska, M / Singh, N / Singhal, A / Sipala, V / Sordini, V / Sorrentino, F / Spera, M / Stachie, C / Steer, D A / Stratta, G / Sur, A / Swinkels, B L / Tacca, M / Tanasijczuk, A J / Tapia San Martin, E N / Tiwari, S / Tonelli, M / Torres-Forné, A / Tosta E Melo, I / Travasso, F / Tringali, M C / Trovato, A / Tsang, K W / Turconi, M / Valentini, M / van Bakel, N / van Beuzekom, M / van den Brand, J F J / Van Den Broeck, C / van der Schaaf, L / Vardaro, M / Vasúth, M / Vedovato, G / Verkindt, D / Vetrano, F / Viceré, A / Vinet, J-Y / Vocca, H / Walet, R / Was, M / Zadrożny, A / Zelenova, T / Zendri, J-P / Vahlbruch, Henning / Mehmet, Moritz / Lück, Harald / Danzmann, Karsten

    Physical review letters

    2019  Volume 123, Issue 23, Page(s) 231108

    Abstract: Current interferometric gravitational-wave detectors are limited by quantum noise over a wide range of their measurement bandwidth. One method to overcome the quantum limit is the injection of squeezed vacuum states of light into the interferometer's ... ...

    Abstract Current interferometric gravitational-wave detectors are limited by quantum noise over a wide range of their measurement bandwidth. One method to overcome the quantum limit is the injection of squeezed vacuum states of light into the interferometer's dark port. Here, we report on the successful application of this quantum technology to improve the shot noise limited sensitivity of the Advanced Virgo gravitational-wave detector. A sensitivity enhancement of up to 3.2±0.1  dB beyond the shot noise limit is achieved. This nonclassical improvement corresponds to a 5%-8% increase of the binary neutron star horizon. The squeezing injection was fully automated and over the first 5 months of the third joint LIGO-Virgo observation run O3 squeezing was applied for more than 99% of the science time. During this period several gravitational-wave candidates have been recorded.
    Language English
    Publishing date 2019-12-23
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.123.231108
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  8. Article ; Online: In-vacuum optical isolation changes by heating in a Faraday isolator.

    Acernese, Fausto / Alshourbagy, Mohamed / Amico, Paolo / Antonucci, Federica / Aoudia, S / Astone, P / Avino, Saverio / Ballardin, G / Baggio, L / Barone, Fabrizio / Barsotti, Lisa / Barsuglia, Matteo / Bauer, Th S / Bigotta, Stefano / Birindelli, Simona / Bizouard, Marie-Anne / Boccara, Albert-Claude / Bondu, François / Bosi, Leone /
    Braccini, Stefano / Bradaschia, Carlo / Brillet, Alain / Brisson, Violette / Buskulic, Damir / Cagnoli, G / Calloni, Enrico / Campagna, Enrico / Carbognani, Franco / Carbone, L / Cavalier, Fabien / Cavalieri, R / Cella, G / Cesarini, E / Chassande-Mottin, E / Chatterji, S / Cleva, F / Coccia, E / Corda, C / Corsi, A / Cottone, F / Coulon, J-P / Cuoco, E / D'Antonio, S / Dari, A / Dattilo, V / Davier, M / De Rosa, R / Del Prete, M / Di Fiore, L / Di Lieto, A / Di Paolo Emilio, M / Di Virgilio, A / Evans, M / Fafone, V / Ferrante, I / Fidecaro, F / Fiori, I / Flaminio, R / Fournier, J-D / Frasca, S / Frasconi, F / Gammaitoni, L / Garufi, F / Genin, E / Gennai, A / Giazotto, A / Giordano, L / Granata, V / Greverie, C / Grosjean, D / Guidi, G / Hamdani, S / Hebri, S / Heitmann, H / Hello, P / Huet, D / La Penna, P / Laval, M / Leroy, N / Letendre, N / Lopez, B / Lorenzini, M / Loriette, V / Losurdo, G / Mackowski, J-M / Majorana, E / Man, N / Mantovani, M / Marchesoni, F / Marion, F / Marque, J / Martelli, F / Masserot, A / Menzinger, F / Milano, L / Minenkov, Y / Moins, C / Morgado, N / Mosca, S / Mours, B / Neri, I / Nocera, F / Pagliaroli, G / Palomba, C / Paoletti, F / Pardi, S / Pasqualetti, A / Passaquieti, R / Passuello, D / Persichetti, G / Piergiovanni, F / Pinard, L / Poggiani, R / Punturo, M / Puppo, P / Rabaste, O / Rapagnani, P / Regimbau, T / Remillieux, A / Ricci, F / Ricciardi, I / Rocchi, A / Rolland, L / Romano, R / Ruggi, P / Russo, G / Sentenac, D / Solimeno, S / Swinkels, B L / Tarallo, M / Terenzi, R / Toncelli, A / Tonelli, M / Tournefier, E / Travasso, F / Vajente, G / van den Brand, J F J / van der Putten, S / Verkindt, D / Vetrano, F / Viceré, A / Vinet, J-Y / Vocca, H / Yvert, M

    Applied optics

    2008  Volume 47, Issue 31, Page(s) 5853–5861

    Abstract: We describe a model evaluating changes in the optical isolation of a Faraday isolator when passing from air to vacuum in terms of different thermal effects in the crystal. The changes are particularly significant in the crystal thermal lensing ( ... ...

    Abstract We describe a model evaluating changes in the optical isolation of a Faraday isolator when passing from air to vacuum in terms of different thermal effects in the crystal. The changes are particularly significant in the crystal thermal lensing (refraction index and thermal expansion) and in its Verdet constant and can be ascribed to the less efficient convection cooling of the magneto-optic crystal of the Faraday isolator. An isolation decrease by a factor of 10 is experimentally observed in a Faraday isolator that is used in a gravitational wave experiment (Virgo) with a 10 W input laser when going from air to vacuum. A finite element model simulation reproduces with a great accuracy the experimental data measured on Virgo and on a test bench. A first set of measurements of the thermal lensing has been used to characterize the losses of the crystal, which depend on the sample. The isolation factor measured on Virgo confirms the simulation model and the absorption losses of 0.0016 +/- 0.0002/cm for the TGG magneto-optic crystal used in the Faraday isolator.
    Language English
    Publishing date 2008-09-25
    Publishing country United States
    Document type Journal Article
    ISSN 1539-4522
    ISSN (online) 1539-4522
    DOI 10.1364/ao.47.005853
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  9. Article ; Online: A state observer for the Virgo inverted pendulum.

    Accadia, T / Acernese, F / Astone, P / Ballardin, G / Barone, F / Barsuglia, M / Basti, A / Bauer, Th S / Bebronne, M / Beker, M G / Belletoile, A / Bitossi, M / Bizouard, M A / Blom, M / Bondu, F / Bonelli, L / Bonnand, R / Boschi, V / Bosi, L /
    Bouhou, B / Braccini, S / Bradaschia, C / Branchesi, M / Briant, T / Brillet, A / Brisson, V / Bulik, T / Bulten, H J / Buskulic, D / Buy, C / Cagnoli, G / Calloni, E / Canuel, B / Carbognani, F / Cavalier, F / Cavalieri, R / Cella, G / Cesarini, E / Chaibi, O / Chassande-Mottin, E / Chincarini, A / Chiummo, A / Cleva, F / Coccia, E / Cohadon, P-F / Colacino, C N / Colas, J / Colla, A / Colombini, M / Conte, A / Corsi, A / Coulon, J-P / Cuoco, E / D' Antonio, S / Dattilo, V / Davier, M / Day, R / De Rosa, R / Debreczeni, G / Del Pozzo, W / del Prete, M / Di Fiore, L / Di Lieto, A / Di Paolo Emilio, M / Di Virgilio, A / Dietz, A / Drago, M / Endroczi, G / Fafone, V / Ferrante, I / Fidecaro, F / Fiori, I / Flaminio, R / Forte, L A / Fournier, J-D / Franc, J / Frasca, S / Frasconi, F / Galimberti, M / Gammaitoni, L / Garufi, F / Gáspár, M E / Gemme, G / Genin, E / Gennai, A / Giazotto, A / Gouaty, R / Granata, M / Greverie, C / Guidi, G M / Hayau, J-F / Heidmann, A / Heitmann, H / Hello, P / Jaranowski, P / Kowalska, I / Królak, A / Leroy, N / Letendre, N / Li, T G F / Liguori, N / Lorenzini, M / Loriette, V / Losurdo, G / Majorana, E / Maksimovic, I / Man, N / Mantovani, M / Marchesoni, F / Marion, F / Marque, J / Martelli, F / Masserot, A / Michel, C / Milano, L / Minenkov, Y / Mohan, M / Morgado, N / Morgia, A / Mours, B / Naticchioni, L / Nocera, F / Pagliaroli, G / Palladino, L / Palomba, C / Paoletti, F / Parisi, M / Pasqualetti, A / Passaquieti, R / Passuello, D / Persichetti, G / Piergiovanni, F / Pietka, M / Pinard, L / Poggiani, R / Prato, M / Prodi, G A / Punturo, M / Puppo, P / Rabeling, D S / Rácz, I / Rapagnani, P / Re, V / Regimbau, T / Ricci, F / Robinet, F / Rocchi, A / Rolland, L / Romano, R / Rosińska, D / Ruggi, P / Sassolas, B / Sentenac, D / Sperandio, L / Sturani, R / Swinkels, B / Tacca, M / Taffarello, L / Toncelli, A / Tonelli, M / Torre, O / Tournefier, E / Travasso, F / Vajente, G / van den Brand, J F J / Van den Broeck, C / van der Putten, S / Vasuth, M / Vavoulidis, M / Vedovato, G / Verkindt, D / Vetrano, F / Viceré, A / Vinet, J-Y / Vitale, S / Vocca, H / Ward, R L / Was, M / Yvert, M / Zadroźny, A / Zendri, J-P

    The Review of scientific instruments

    2011  Volume 82, Issue 9, Page(s) 94502

    Abstract: We report an application of Kalman filtering to the inverted pendulum (IP) of the Virgo gravitational wave interferometer. Using subspace method system identification techniques, we calculated a linear mechanical model of Virgo IP from experimental ... ...

    Abstract We report an application of Kalman filtering to the inverted pendulum (IP) of the Virgo gravitational wave interferometer. Using subspace method system identification techniques, we calculated a linear mechanical model of Virgo IP from experimental transfer functions. We then developed a Kalman filter, based on the obtained state space representation, that estimates from open loop time domain data, the state variables of the system. This allows the observation (and eventually control) of every resonance mode of the IP mechanical structure independently.
    Language English
    Publishing date 2011-09
    Publishing country United States
    Document type Journal Article
    ZDB-ID 209865-9
    ISSN 1089-7623 ; 0034-6748
    ISSN (online) 1089-7623
    ISSN 0034-6748
    DOI 10.1063/1.3637466
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  10. Article ; Online: Search for Subsolar-Mass Binaries in the First Half of Advanced LIGO's and Advanced Virgo's Third Observing Run.

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    Physical review letters

    2022  Volume 129, Issue 6, Page(s) 61104

    Abstract: We report on a search for compact binary coalescences where at least one binary component has a mass between 0.2  M_{⊙} and 1.0  M_{⊙} in Advanced LIGO and Advanced Virgo data collected between 1 April 2019 1500 UTC and 1 October 2019 1500 UTC. We extend ...

    Abstract We report on a search for compact binary coalescences where at least one binary component has a mass between 0.2  M_{⊙} and 1.0  M_{⊙} in Advanced LIGO and Advanced Virgo data collected between 1 April 2019 1500 UTC and 1 October 2019 1500 UTC. We extend our previous analyses in two main ways: we include data from the Virgo detector and we allow for more unequal mass systems, with mass ratio q≥0.1. We do not report any gravitational-wave candidates. The most significant trigger has a false alarm rate of 0.14  yr^{-1}. This implies an upper limit on the merger rate of subsolar binaries in the range [220-24200]  Gpc^{-3} yr^{-1}, depending on the chirp mass of the binary. We use this upper limit to derive astrophysical constraints on two phenomenological models that could produce subsolar-mass compact objects. One is an isotropic distribution of equal-mass primordial black holes. Using this model, we find that the fraction of dark matter in primordial black holes in the mass range 0.2  M_{⊙}<m_{PBH}<1.0  M_{⊙} is f_{PBH}≡Ω_{PBH}/Ω_{DM}≲6%. This improves existing constraints on primordial black hole abundance by a factor of ∼3. The other is a dissipative dark matter model, in which fermionic dark matter can collapse and form black holes. The upper limit on the fraction of dark matter black holes depends on the minimum mass of the black holes that can be formed: the most constraining result is obtained at M_{min}=1  M_{⊙}, where f_{DBH}≡Ω_{DBH}/Ω_{DM}≲0.003%. These are the first constraints placed on dissipative dark models by subsolar-mass analyses.<br />
    Language English
    Publishing date 2022-08-28
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.129.061104
    Database MEDical Literature Analysis and Retrieval System OnLINE

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