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  1. Book ; Online: Lightning-Fast Gravitational Wave Parameter Inference through Neural Amortization

    Delaunoy, Arnaud / Wehenkel, Antoine / Hinderer, Tanja / Nissanke, Samaya / Weniger, Christoph / Williamson, Andrew R. / Louppe, Gilles

    2020  

    Abstract: Gravitational waves from compact binaries measured by the LIGO and Virgo detectors are routinely analyzed using Markov Chain Monte Carlo sampling algorithms. Because the evaluation of the likelihood function requires evaluating millions of waveform ... ...

    Abstract Gravitational waves from compact binaries measured by the LIGO and Virgo detectors are routinely analyzed using Markov Chain Monte Carlo sampling algorithms. Because the evaluation of the likelihood function requires evaluating millions of waveform models that link between signal shapes and the source parameters, running Markov chains until convergence is typically expensive and requires days of computation. In this extended abstract, we provide a proof of concept that demonstrates how the latest advances in neural simulation-based inference can speed up the inference time by up to three orders of magnitude -- from days to minutes -- without impairing the performance. Our approach is based on a convolutional neural network modeling the likelihood-to-evidence ratio and entirely amortizes the computation of the posterior. We find that our model correctly estimates credible intervals for the parameters of simulated gravitational waves.

    Comment: V1: First version; V2: Updated references; V3: Update references and camera-ready version; V4: Correct figure labels
    Keywords Astrophysics - Instrumentation and Methods for Astrophysics ; Computer Science - Machine Learning ; General Relativity and Quantum Cosmology
    Subject code 310
    Publishing date 2020-10-24
    Publishing country us
    Document type Book ; Online
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  2. Article ; Online: A mildly relativistic wide-angle outflow in the neutron-star merger event GW170817.

    Mooley, K P / Nakar, E / Hotokezaka, K / Hallinan, G / Corsi, A / Frail, D A / Horesh, A / Murphy, T / Lenc, E / Kaplan, D L / De, K / Dobie, D / Chandra, P / Deller, A / Gottlieb, O / Kasliwal, M M / Kulkarni, S R / Myers, S T / Nissanke, S /
    Piran, T / Lynch, C / Bhalerao, V / Bourke, S / Bannister, K W / Singer, L P

    Nature

    2018  Volume 554, Issue 7691, Page(s) 207–210

    Abstract: GW170817 was the first gravitational-wave detection of a binary neutron-star merger. It was accompanied by radiation across the electromagnetic spectrum and localized to the galaxy NGC 4993 at a distance of 40 megaparsecs. It has been proposed that the ... ...

    Abstract GW170817 was the first gravitational-wave detection of a binary neutron-star merger. It was accompanied by radiation across the electromagnetic spectrum and localized to the galaxy NGC 4993 at a distance of 40 megaparsecs. It has been proposed that the observed γ-ray, X-ray and radio emission is due to an ultra-relativistic jet being launched during the merger (and successfully breaking out of the surrounding material), directed away from our line of sight (off-axis). The presence of such a jet is predicted from models that posit neutron-star mergers as the drivers of short hard-γ-ray bursts. Here we report that the radio light curve of GW170817 has no direct signature of the afterglow of an off-axis jet. Although we cannot completely rule out the existence of a jet directed away from the line of sight, the observed γ-ray emission could not have originated from such a jet. Instead, the radio data require the existence of a mildly relativistic wide-angle outflow moving towards us. This outflow could be the high-velocity tail of the neutron-rich material that was ejected dynamically during the merger, or a cocoon of material that breaks out when a jet launched during the merger transfers its energy to the dynamical ejecta. Because the cocoon model explains the radio light curve of GW170817, as well as the γ-ray and X-ray emission (and possibly also the ultraviolet and optical emission), it is the model that is most consistent with the observational data. Cocoons may be a ubiquitous phenomenon produced in neutron-star mergers, giving rise to a hitherto unidentified population of radio, ultraviolet, X-ray and γ-ray transients in the local Universe.
    Language English
    Publishing date 2018--08
    Publishing country England
    Document type Journal Article ; Research Support, Non-U.S. Gov't ; Research Support, U.S. Gov't, Non-P.H.S.
    ZDB-ID 120714-3
    ISSN 1476-4687 ; 0028-0836
    ISSN (online) 1476-4687
    ISSN 0028-0836
    DOI 10.1038/nature25452
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  3. Article: Binary-black-hole merger: symmetry and the spin expansion.

    Boyle, Latham / Kesden, Michael / Nissanke, Samaya

    Physical review letters

    2008  Volume 100, Issue 15, Page(s) 151101

    Abstract: We regard binary-black-hole (BBH) merger as a map from a simple initial state (two Kerr black holes, with dimensionless spins a and b) to a simple final state (a Kerr black hole with mass m, dimensionless spin s, and kick velocity k). By expanding this ... ...

    Abstract We regard binary-black-hole (BBH) merger as a map from a simple initial state (two Kerr black holes, with dimensionless spins a and b) to a simple final state (a Kerr black hole with mass m, dimensionless spin s, and kick velocity k). By expanding this map around a=b=0 and applying symmetry constraints, we obtain a simple formalism that is remarkably successful at explaining existing BBH simulations. It also makes detailed predictions and suggests a more efficient way of mapping the parameter space of binary black-hole merger. Since we rely on symmetry rather than dynamics, our expansion complements previous analytical techniques.
    Language English
    Publishing date 2008-04-18
    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.100.151101
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  4. Article ; Online: A radio counterpart to a neutron star merger.

    Hallinan, G / Corsi, A / Mooley, K P / Hotokezaka, K / Nakar, E / Kasliwal, M M / Kaplan, D L / Frail, D A / Myers, S T / Murphy, T / De, K / Dobie, D / Allison, J R / Bannister, K W / Bhalerao, V / Chandra, P / Clarke, T E / Giacintucci, S / Ho, A Y Q /
    Horesh, A / Kassim, N E / Kulkarni, S R / Lenc, E / Lockman, F J / Lynch, C / Nichols, D / Nissanke, S / Palliyaguru, N / Peters, W M / Piran, T / Rana, J / Sadler, E M / Singer, L P

    Science (New York, N.Y.)

    2017  

    Abstract: Gravitational waves have been detected from a binary neutron star merger event, GW170817. The detection of electromagnetic radiation from the same source has shown that the merger occurred in the outskirts of the galaxy NGC 4993, at a distance of 40 ... ...

    Abstract Gravitational waves have been detected from a binary neutron star merger event, GW170817. The detection of electromagnetic radiation from the same source has shown that the merger occurred in the outskirts of the galaxy NGC 4993, at a distance of 40 megaparsecs from Earth. We report the detection of a counterpart radio source that appears 16 days after the event, allowing us to diagnose the energetics and environment of the merger. The observed radio emission can be explained by either a collimated ultra-relativistic jet viewed off-axis, or a cocoon of mildly relativistic ejecta. Within 100 days of the merger, the radio light curves will distinguish between these models and very long baseline interferometry will have the capability to directly measure the angular velocity and geometry of the debris.
    Language English
    Publishing date 2017-10-16
    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.aap9855
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  5. Article ; Online: LOFAR 144-MHz follow-up observations of GW170817

    Broderick, J. / Shimwell, T. / Gourdji, K. / Rowlinson, A. / Nissanke, S. / Hotokezaka, K. / Jonker, P. / Tasse, C. / Hardcastle, M. / Oonk, J. / Fender, R. / Wijers, R. / Shulevski, A. / Stewart, A. / ter Veen, S. / Moss, V. / van der Wiel, M. / Nichols, D. / Piette, A. /
    Bell, M. / Carbone, D. / Corbel, S. / Eisloeffel, J. / Griessmeier, J. / Keane, E. / Law, C. / Munoz-Darias, T. / Pietka, M. / Serylak, M. / van der Horst, A. / van Leeuwen, J. / Wijnands, R. / Zarka, P. / Anderson, J. / Bentum, M. / Blaauw, R. / Brouw, W. / Bruggen, M. / Ciardi, B. / de Vos, M. / Duscha, S. / Fallows, R. / Franzen, T. / Garrett, M. / Gunst, A. / Hoeft, M. / Horandel, J. / Iacobelli, M. / Jutte, E. / Koopmans, L. / Krankowski, A. / Maat, P. / Mann, G. / Mulder, H. / Nelles, A. / Paas, H. / Pandey-Pommier, M. / Pekal, R. / Reich, W. / Rottgering, H. / Schwarz, D. / Smirnov, O. / Soida, M. / Toribio, M. / van Haarlem, M. / van Weeren, R. / Vocks, C. / Wucknitz, O. / Zucca, P.

    Monthly Notices of the Royal Astronomical Society

    2020  

    Publishing country de
    Document type Article ; Online
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  6. Article ; Online: Illuminating gravitational waves: A concordant picture of photons from a neutron star merger.

    Kasliwal, M M / Nakar, E / Singer, L P / Kaplan, D L / Cook, D O / Van Sistine, A / Lau, R M / Fremling, C / Gottlieb, O / Jencson, J E / Adams, S M / Feindt, U / Hotokezaka, K / Ghosh, S / Perley, D A / Yu, P-C / Piran, T / Allison, J R / Anupama, G C /
    Balasubramanian, A / Bannister, K W / Bally, J / Barnes, J / Barway, S / Bellm, E / Bhalerao, V / Bhattacharya, D / Blagorodnova, N / Bloom, J S / Brady, P R / Cannella, C / Chatterjee, D / Cenko, S B / Cobb, B E / Copperwheat, C / Corsi, A / De, K / Dobie, D / Emery, S W K / Evans, P A / Fox, O D / Frail, D A / Frohmaier, C / Goobar, A / Hallinan, G / Harrison, F / Helou, G / Hinderer, T / Ho, A Y Q / Horesh, A / Ip, W-H / Itoh, R / Kasen, D / Kim, H / Kuin, N P M / Kupfer, T / Lynch, C / Madsen, K / Mazzali, P A / Miller, A A / Mooley, K / Murphy, T / Ngeow, C-C / Nichols, D / Nissanke, S / Nugent, P / Ofek, E O / Qi, H / Quimby, R M / Rosswog, S / Rusu, F / Sadler, E M / Schmidt, P / Sollerman, J / Steele, I / Williamson, A R / Xu, Y / Yan, L / Yatsu, Y / Zhang, C / Zhao, W

    Science (New York, N.Y.)

    2017  

    Abstract: Merging neutron stars offer an exquisite laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart (EM170817) to gravitational waves (GW170817) ... ...

    Abstract Merging neutron stars offer an exquisite laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart (EM170817) to gravitational waves (GW170817) detected from merging neutron stars. By synthesizing a panchromatic dataset, we demonstrate that merging neutron stars are a long-sought production site forging heavy elements by r-process nucleosynthesis. The weak gamma-rays seen in EM170817 are dissimilar to classical short gamma-ray bursts with ultra-relativistic jets. Instead, we suggest that breakout of a wide-angle, mildly-relativistic cocoon engulfing the jet elegantly explains the low-luminosity gamma-rays, the high-luminosity ultraviolet-optical-infrared and the delayed radio/x-ray emission. We posit that all merging neutron stars may lead to a wide-angle cocoon breakout; sometimes accompanied by a successful jet and sometimes a choked jet.
    Language English
    Publishing date 2017-10-16
    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.aap9455
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  7. 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 / 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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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  8. 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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  9. 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
    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.

    Abbott, R / Abbott, T D / Acernese, F / Ackley, K / Adams, C / Adhikari, N / Adhikari, R X / Adya, V B / Affeldt, C / Agarwal, D / Agathos, M / Agatsuma, K / Aggarwal, N / Aguiar, O D / Aiello, L / Ain, A / Ajith, P / Albanesi, S / Allocca, A /
    Altin, P A / Amato, A / Anand, C / Anand, S / Ananyeva, A / Anderson, S B / Anderson, W G / Andrade, T / Andres, N / Andrić, T / Angelova, S V / Ansoldi, S / Antelis, J M / Antier, S / Appert, S / Arai, K / Araya, M C / Areeda, J S / Arène, M / Arnaud, N / Aronson, S M / Arun, K G / Asali, Y / Ashton, G / Assiduo, M / Aston, S M / Astone, P / Aubin, F / Austin, C / Babak, S / Badaracco, F / Bader, M K M / Badger, C / Bae, S / Baer, A M / Bagnasco, S / Bai, Y / Baird, J / Ball, M / Ballardin, G / Ballmer, S W / Balsamo, A / Baltus, G / Banagiri, S / Bankar, D / Barayoga, J C / Barbieri, C / Barish, B C / Barker, D / Barneo, P / Barone, F / Barr, B / Barsotti, L / Barsuglia, M / Barta, D / Bartlett, J / Barton, M A / Bartos, I / Bassiri, R / Basti, A / Bawaj, M / Bayley, J C / Baylor, A C / Bazzan, M / Bécsy, B / Bedakihale, V M / Bejger, M / Belahcene, I / Benedetto, V / Beniwal, D / Bennett, T F / Bentley, J D / BenYaala, M / Bergamin, F / Berger, B K / Bernuzzi, S / Berry, C P L / Bersanetti, D / Bertolini, A / Betzwieser, J / Beveridge, D / Bhandare, R / Bhardwaj, U / Bhattacharjee, D / Bhaumik, S / Bilenko, I A / Billingsley, G / Bini, S / Birney, R / Birnholtz, O / Biscans, S / Bischi, M / Biscoveanu, S / Bisht, A / Biswas, B / Bitossi, M / Bizouard, M-A / Blackburn, J K / Blair, C D / Blair, D G / Blair, R M / Bobba, F / Bode, N / Boer, M / Bogaert, G / Boldrini, M / Bonavena, L D / Bondu, F / Bonilla, E / Bonnand, R / Booker, P / Boom, B A / Bork, R / Boschi, V / Bose, N / Bose, S / Bossilkov, V / Boudart, V / Bouffanais, Y / Bozzi, A / Bradaschia, C / Brady, P R / Bramley, A / Branch, A / Branchesi, M / Brau, J E / Breschi, M / Briant, T / Briggs, J H / Brillet, A / Brinkmann, M / Brockill, P / Brooks, A F / Brooks, J / Brown, D D / Brunett, S / Bruno, G / Bruntz, R / Bryant, J / Bulik, T / Bulten, H J / Buonanno, A / Buscicchio, R / Buskulic, D / Buy, C / Byer, R L / Cadonati, L / Cagnoli, G / Cahillane, C / Bustillo, J Calderón / Callaghan, J D / Callister, T A / Calloni, E / Cameron, J / Camp, J B / Canepa, M / Canevarolo, S / Cannavacciuolo, M / Cannon, K C / Cao, H / Capote, E / Carapella, G / Carbognani, F / Carlin, J B / Carney, M F / Carpinelli, M / Carrillo, G / Carullo, G / Carver, T L / Diaz, J Casanueva / Casentini, C / Castaldi, G / Caudill, S / Cavaglià, M / Cavalier, F / Cavalieri, R / Ceasar, M / Cella, G / Cerdá-Durán, P / Cesarini, E / Chaibi, W / Chakravarti, K / Subrahmanya, S Chalathadka / Champion, E / Chan, C-H / Chan, C / Chan, C L / Chan, K / Chandra, K / Chanial, P / Chao, S / Charlton, P / Chase, E A / Chassande-Mottin, E / Chatterjee, C / Chatterjee, Debarati / Chatterjee, Deep / Chaturvedi, M / Chaty, S / Chatziioannou, K / Chen, H Y / Chen, J / Chen, X / Chen, Y / Chen, Z / Cheng, H / Cheong, C K / Cheung, H Y / Chia, H Y / Chiadini, F / Chiarini, G / Chierici, R / Chincarini, A / Chiofalo, M L / Chiummo, A / Cho, G / Cho, H S / Choudhary, R K / Choudhary, S / Christensen, N / Chu, Q / Chua, S / Chung, K W / Ciani, G / Ciecielag, P / Cieślar, M / Cifaldi, M / Ciobanu, A A / Ciolfi, R / Cipriano, F / Cirone, A / Clara, F / Clark, E N / Clark, J A / Clarke, L / Clearwater, P / Clesse, S / Cleva, F / Coccia, E / Codazzo, E / Cohadon, P-F / Cohen, D E / Cohen, L / Colleoni, M / Collette, C G / Colombo, A / Colpi, M / Compton, C M / Constancio, M / Conti, L / Cooper, S J / Corban, P / Corbitt, T R / Cordero-Carrión, I / Corezzi, S / Corley, K R / Cornish, N / Corre, D / Corsi, A / Cortese, S / Costa, C A / Cotesta, R / Coughlin, M W / Coulon, J-P / Countryman, S T / Cousins, B / Couvares, P / Coward, D M / Cowart, M J / Coyne, D C / Coyne, R / Creighton, J D E / Creighton, T D / Criswell, A W / Croquette, M / Crowder, S G / Cudell, J R / Cullen, T J / Cumming, A / Cummings, R / Cunningham, L / Cuoco, E / Curyło, M / Dabadie, P / Canton, T Dal / Dall'Osso, S / Dálya, G / Dana, A / DaneshgaranBajastani, L M / D'Angelo, B / Danilishin, S / D'Antonio, S / Danzmann, K / Darsow-Fromm, C / Dasgupta, A / Datrier, L E H / Datta, S / Dattilo, V / Dave, I / Davier, M / Davies, G S / Davis, D / Davis, M C / Daw, E J / Dean, R / DeBra, D / Deenadayalan, M / Degallaix, J / De Laurentis, M / Deléglise, S / Del Favero, V / De Lillo, F / De Lillo, N / Del Pozzo, W / DeMarchi, L M / De Matteis, F / D'Emilio, V / Demos, N / Dent, T / Depasse, A / De Pietri, R / De Rosa, R / De Rossi, C / DeSalvo, R / De Simone, R / Dhurandhar, S / Díaz, M C / Diaz-Ortiz, M / Didio, N A / Dietrich, T / Di Fiore, L / Di Fronzo, C / Di Giorgio, C / Di Giovanni, F / Di Giovanni, M / Di Girolamo, T / Di Lieto, A / Ding, B / Di Pace, S / Di Palma, I / Di Renzo, F / Divakarla, A K / Dmitriev, A / Doctor, Z / D'Onofrio, L / Donovan, F / Dooley, K L / Doravari, S / Dorrington, I / Drago, M / Driggers, J C / Drori, Y / Ducoin, J-G / Dupej, P / Durante, O / D'Urso, D / Duverne, P-A / Dwyer, S E / Eassa, C / Easter, P J / Ebersold, M / Eckhardt, T / Eddolls, G / Edelman, B / Edo, T B / Edy, O / Effler, A / 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/ Ward, R L / Warner, J / Was, M / Washington, N Y / Watchi, J / Weaver, B / Webster, S A / Weinert, M / Weinstein, A J / Weiss, R / Weller, C M / Wellmann, F / Wen, L / Weßels, P / Wette, K / Whelan, J T / White, D D / Whiting, B F / Whittle, C / Wilken, D / Williams, D / Williams, M J / Williamson, A R / Willis, J L / Willke, B / Wilson, D J / Winkler, W / Wipf, C C / Wlodarczyk, T / Woan, G / Woehler, J / Wofford, J K / Wong, I C F / Wu, D S / Wysocki, D M / Xiao, L / Yamamoto, H / Yang, F W / Yang, L / Yang, Yang / Yang, Z / Yap, M J / Yeeles, D W / Yelikar, A B / Ying, M / Yoo, J / Yu, Hang / Yu, Haocun / Zadrożny, A / Zanolin, M / Zelenova, T / Zendri, J-P / Zevin, M / Zhang, J / Zhang, L / Zhang, T / Zhang, Y / Zhao, C / Zhao, G / Zhao, Yue / Zhou, R / Zhou, Z / Zhu, X J / Zimmerman, A B / Zucker, M E / Zweizig, J / Jeong, Donghui / Shandera, Sarah

    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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