Search for Gravitational Waves Associated with Fast Radio Bursts Detected by CHIME/FRB during the LIGO–Virgo Observing Run O3a
Search for Gravitational Waves Associated with Fast Radio Bursts Detected by CHIME/FRB during the LIGO–Virgo Observing Run O3a
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DOI：
10.3847/1538-4357/acd770
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发表时间：
2023-09
期刊：
影响因子：
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通讯作者：
B. Lane;R. Lang;J. Lange;B. Lantz;I. L. Rosa;A. Lartaux-Vollard;P. Lasky;M. Laxen;A. Lazzarini;C. Lazzaro;P. Leaci;S. Leavey;Y. Lecoeuche;H. Lee;H. Lee;H. W. Lee;J. Lee;K. Lee;Ray-Kuang Lee;J. Lehmann;A. Lemaitre;M. Leonardi;N. Leroy;N. Letendre;C. Lévesque;Y. Levin;J. Leviton;K. Leyde;A. Li;B. Li;J. Li;K. Li;T. G. F. Li;X. Li;C.Y. Lin;F. Lin;F. Lin;H. Lin;L. Lin;F. Linde;S. Linker;J. Linley;T. Littenberg;G. Liu;J. Liu;K. Liu;X. Liu;F. Llamas;M. Llorens-Monteagudo;R. K. Lo;A. Lockwood;L. London;A. Longo;D. Lopez;M. Portilla;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo;T. Lott;J. Lough;C. Lousto;G. Lovelace;J. F. Lucaccioni;H. Lück;D. Lumaca;A. Lundgren;L. Luo;J. Lynam;R. Macas;M. Macinnis;D. Macleod;I. MacMillan;A. Macquet;I. M. Hernandez;C. Magazzù;R. Magee;R. Maggiore;M. Magnozzi;S. Mahesh;E. Majorana;C. Makarem;I. Maksimovic;S. Maliakal;A. Malik;N. Man;V. Mandic;V. Mangano;J. Mango;G. Mansell;M. Manske;M. Mantovani;M. Mapelli;F. Marchesoni;M. Marchiò;F. Marion;Z. Mark;S. Márka;Z. Márka;C. Markakis;A. Markosyan;A. Markowitz;E. Maros;A. Marquina;S. Marsat;F. Martelli;I. Martin;R. Martin;M. Martínez;V. Martínez;V. Martínez;K. Martinovic;D. Martynov;E. J. Marx;H. Masalehdan;K. Mason;E. Massera;A. Masserot;T. Massinger;M. Masso-Reid;S. Mastrogiovanni;A. Matas;M. Mateu-Lucena;F. Matichard;M. Matiushechkina;N. Mavalvala;J. McCann;R. Mccarthy;D. McClelland;P. McClincy;S. Mccormick;L. McCuller;G. McGhee;S. Mcguire;C. McIsaac;J. McIver;T. McRae;S. McWilliams;D. Meacher;M. Mehmet;A. Mehta;Q. Meijer;A. Melatos;D. Melchor;G. Mendell;A. Menéndez-Vázquez;C. Menoni;R. Mercer;L. Mereni;K. Merfeld;E. Merilh;J. D. Merritt;M. Merzougui;S. Meshkov;C. Messenger;C. Messick;P. Meyers;F. Meylahn;A. Mhaske;A. Miani;H. Miao;I. Michaloliakos;C. Michel;Y. Michimura;H. Middleton;L. Milano;A. Miller;A. Miller;B. Miller;M. Millhouse;J. Mills;E. Milotti;O. Minazzoli;Y. Minenkov;N. Mio;L. Mir;M. Miravet-Tenés;C. Mishra;T. Mishra;T. Mistry;S. Mitra;V. Mitrofanov;G. Mitselmakher;R. Mittleman;O. Miyakawa;A. Miyamoto;Y. Miyazaki;K. Miyo;S. Miyoki;G. Mo;E. Moguel;K. Mogushi;S. Mohapatra;S. Mohite;I. Molina;M. Molina-Ruiz;M. Mondin;M. Montani;C. Moore;D. Moraru;F. Morawski;C. Moreno;G. Moreno;Y. Mori;S. Morisaki;Y. Moriwaki;B. Mours;C. Mow-Lowry;S. Mozzon;F. Muciaccia;A. Mukherjee;D. Mukherjee;S. Mukherjee;S. Mukherjee;S. Mukherjee;N. Mukund;A. Mullavey;J. Munch;E. Muniz;P. Murray;R. Musenich;S. Muusse;S. Nadji;K. Nagano;S. Nagano;A. Nagar;K. Nakamura;H. Nakano;M. Nakano;R. Nakashima;Y. Nakayama;V. Napolano;I. Nardecchia;T. Narikawa;L. Naticchioni;B. Nayak;R. Nayak;R. Negishi;B. Neil;J. Neilson;G. Nelemans;T. Nelson;M. Nery;P. Neubauer;A. Neunzert;K. Ng;S. Ng;C. Nguyen;P. Nguyen;T. Nguyen;L. Quynh;S. Nichols;A. Nishizawa;S. Nissanke;E. Nitoglia;F. Nocera;Manuel Norman;S. Nozaki;L. Nuttall;J. Oberling;B. O'Brien;Y. Obuchi;J. O'Dell;E. Oelker;W. Ogaki;G. Oganesyan;J. Oh;K. Oh;S. -. Oh;M. Ohashi;N. Ohishi;M. Ohkawa;F. Ohme;H. Ohta;M. A. Okada;Y. Okutani;K. Okutomi;C. Olivetto;K. Oohara;C. Ooi;R. Oram;B. O'reilly;R. Ormiston;N. Ormsby;L. F. Ortega;R. O’Shaughnessy;É. O’Shea;S. Oshino;S. Ossokine;C. Osthelder;S. Otabe;D. Ottaway;H. Overmier;A. Pace;G. Pagano;M. Page;G. Pagliaroli;A. Pai;O. Palashov;C. Palomba;H. Pan;K. Pan;P. Panda;H. Pang;C. Pankow;F. Pannarale;F. Panther;F. Paoletti;A. Paoli;A. Paolone;A. Parisi;H. Park;J. Park;W. Parker;D. Pascucci;A. Pasqualetti;R. Passaquieti;D. Passuello;M. Patel;M. Pathak;B. Patricelli;A. S. Patron;S. Patrone;S. Paul;E. Payne;M. Pedraza;M. Pegoraro;A. Pele;F. Arellano;S. Penn;A. Perego;A. Pereira;T. Pereira;C. Perez;C. Périgois;C. Perkins;A. Perreca;S. Perriès;J. Petermann;D. Petterson;H. Pfeiffer;K. A. Pham;K. S. Phukon;O. Piccinni;M. Piendibene;F. Piergiovanni;L. Pierini;V. Pierro;G. Pillant;M. Pillas;F. Pilo;L. Pinard;M. Pinto;B. Piotrzkowski;K. Piotrzkowski;M. Pirello;E. Placidi;L. Planas;W. Plastino;C. Pluchar;R. Poggiani;E. Polini;R. Poulton;J. Powell;M. Pracchia;T. Pradier;A. K. Prajapati;K. Prasai;R. Prasanna;G. Pratten;L. Prokhorov;P. Prosposito;L. Prudenzi;A. Puecher;M. Punturo;F. Puosi;V. Quetschke;F. Raab;G. Raaijmakers;N. Radulesco;P. Raffai;S. Raja;C. Rajan;K. Ramirez;J. Rana;P. Rapagnani;U. Rapol;A. Ray;V. Raymond;M. Razzano;L. A. Rees;T. Regimbau;L. Rei;S. Reid;S. Reid;D. Reitze;P. Relton;A. Renzini;P. Rettegno;M. Rezac;F. Ricci
中科院分区：
文献类型：
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作者：
B. Lane;R. Lang;J. Lange;B. Lantz;I. L. Rosa;A. Lartaux-Vollard;P. Lasky;M. Laxen;A. Lazzarini;C. Lazzaro;P. Leaci;S. Leavey;Y. Lecoeuche;H. Lee;H. Lee;H. W. Lee;J. Lee;K. Lee;Ray-Kuang Lee;J. Lehmann;A. Lemaitre;M. Leonardi;N. Leroy;N. Letendre;C. Lévesque;Y. Levin;J. Leviton;K. Leyde;A. Li;B. Li;J. Li;K. Li;T. G. F. Li;X. Li;C.Y. Lin;F. Lin;F. Lin;H. Lin;L. Lin;F. Linde;S. Linker;J. Linley;T. Littenberg;G. Liu;J. Liu;K. Liu;X. Liu;F. Llamas;M. Llorens-Monteagudo;R. K. Lo;A. Lockwood;L. London;A. Longo;D. Lopez;M. Portilla;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo;T. Lott;J. Lough;C. Lousto;G. Lovelace;J. F. Lucaccioni;H. Lück;D. Lumaca;A. Lundgren;L. Luo;J. Lynam;R. Macas;M. Macinnis;D. Macleod;I. MacMillan;A. Macquet;I. M. Hernandez;C. Magazzù;R. Magee;R. Maggiore;M. Magnozzi;S. Mahesh;E. Majorana;C. Makarem;I. Maksimovic;S. Maliakal;A. Malik;N. Man;V. Mandic;V. Mangano;J. Mango;G. Mansell;M. Manske;M. Mantovani;M. Mapelli;F. Marchesoni;M. Marchiò;F. Marion;Z. Mark;S. Márka;Z. Márka;C. Markakis;A. Markosyan;A. Markowitz;E. Maros;A. Marquina;S. Marsat;F. Martelli;I. Martin;R. Martin;M. Martínez;V. Martínez;V. Martínez;K. Martinovic;D. Martynov;E. J. Marx;H. Masalehdan;K. Mason;E. Massera;A. Masserot;T. Massinger;M. Masso-Reid;S. Mastrogiovanni;A. Matas;M. Mateu-Lucena;F. Matichard;M. Matiushechkina;N. Mavalvala;J. McCann;R. Mccarthy;D. McClelland;P. McClincy;S. Mccormick;L. McCuller;G. McGhee;S. Mcguire;C. McIsaac;J. McIver;T. McRae;S. McWilliams;D. Meacher;M. Mehmet;A. Mehta;Q. Meijer;A. Melatos;D. Melchor;G. Mendell;A. Menéndez-Vázquez;C. Menoni;R. Mercer;L. Mereni;K. Merfeld;E. Merilh;J. D. Merritt;M. Merzougui;S. Meshkov;C. Messenger;C. Messick;P. Meyers;F. Meylahn;A. Mhaske;A. Miani;H. Miao;I. Michaloliakos;C. Michel;Y. Michimura;H. Middleton;L. Milano;A. Miller;A. Miller;B. Miller;M. Millhouse;J. Mills;E. Milotti;O. Minazzoli;Y. Minenkov;N. Mio;L. Mir;M. Miravet-Tenés;C. Mishra;T. Mishra;T. Mistry;S. Mitra;V. Mitrofanov;G. Mitselmakher;R. Mittleman;O. Miyakawa;A. Miyamoto;Y. Miyazaki;K. Miyo;S. Miyoki;G. Mo;E. Moguel;K. Mogushi;S. Mohapatra;S. Mohite;I. Molina;M. Molina-Ruiz;M. Mondin;M. Montani;C. Moore;D. Moraru;F. Morawski;C. Moreno;G. Moreno;Y. Mori;S. Morisaki;Y. Moriwaki;B. Mours;C. Mow-Lowry;S. Mozzon;F. Muciaccia;A. Mukherjee;D. Mukherjee;S. Mukherjee;S. Mukherjee;S. Mukherjee;N. Mukund;A. Mullavey;J. Munch;E. Muniz;P. Murray;R. Musenich;S. Muusse;S. Nadji;K. Nagano;S. Nagano;A. Nagar;K. Nakamura;H. Nakano;M. Nakano;R. Nakashima;Y. Nakayama;V. Napolano;I. Nardecchia;T. Narikawa;L. Naticchioni;B. Nayak;R. Nayak;R. Negishi;B. Neil;J. Neilson;G. Nelemans;T. Nelson;M. Nery;P. Neubauer;A. Neunzert;K. Ng;S. Ng;C. Nguyen;P. Nguyen;T. Nguyen;L. Quynh;S. Nichols;A. Nishizawa;S. Nissanke;E. Nitoglia;F. Nocera;Manuel Norman;S. Nozaki;L. Nuttall;J. Oberling;B. O'Brien;Y. Obuchi;J. O'Dell;E. Oelker;W. Ogaki;G. Oganesyan;J. Oh;K. Oh;S. -. Oh;M. Ohashi;N. Ohishi;M. Ohkawa;F. Ohme;H. Ohta;M. A. Okada;Y. Okutani;K. Okutomi;C. Olivetto;K. Oohara;C. Ooi;R. Oram;B. O'reilly;R. Ormiston;N. Ormsby;L. F. Ortega;R. O’Shaughnessy;É. O’Shea;S. Oshino;S. Ossokine;C. Osthelder;S. Otabe;D. Ottaway;H. Overmier;A. Pace;G. Pagano;M. Page;G. Pagliaroli;A. Pai;O. Palashov;C. Palomba;H. Pan;K. Pan;P. Panda;H. Pang;C. Pankow;F. Pannarale;F. Panther;F. Paoletti;A. Paoli;A. Paolone;A. Parisi;H. Park;J. Park;W. Parker;D. Pascucci;A. Pasqualetti;R. Passaquieti;D. Passuello;M. Patel;M. Pathak;B. Patricelli;A. S. Patron;S. Patrone;S. Paul;E. Payne;M. Pedraza;M. Pegoraro;A. Pele;F. Arellano;S. Penn;A. Perego;A. Pereira;T. Pereira;C. Perez;C. Périgois;C. Perkins;A. Perreca;S. Perriès;J. Petermann;D. Petterson;H. Pfeiffer;K. A. Pham;K. S. Phukon;O. Piccinni;M. Piendibene;F. Piergiovanni;L. Pierini;V. Pierro;G. Pillant;M. Pillas;F. Pilo;L. Pinard;M. Pinto;B. Piotrzkowski;K. Piotrzkowski;M. Pirello;E. Placidi;L. Planas;W. Plastino;C. Pluchar;R. Poggiani;E. Polini;R. Poulton;J. Powell;M. Pracchia;T. Pradier;A. K. Prajapati;K. Prasai;R. Prasanna;G. Pratten;L. Prokhorov;P. Prosposito;L. Prudenzi;A. Puecher;M. Punturo;F. Puosi;V. Quetschke;F. Raab;G. Raaijmakers;N. Radulesco;P. Raffai;S. Raja;C. Rajan;K. Ramirez;J. Rana;P. Rapagnani;U. Rapol;A. Ray;V. Raymond;M. Razzano;L. A. Rees;T. Regimbau;L. Rei;S. Reid;S. Reid;D. Reitze;P. Relton;A. Renzini;P. Rettegno;M. Rezac;F. Ricci
在高级LIGO和高级处女座第三次观测运行的第一部分(2019年4月1日15：00 UTC-2019年10月1日15：00 UTC)，我们搜索与加拿大氢强度测绘实验快速射电爆发项目探测到的快速射电爆发(FRB)相关的引力波(GW)瞬变。通过搜索双星中子星(BNS)和中子星-黑洞(NSBH)的合并，分析了22个FRB的触发因素。对40个FRB进行了有针对性的通用GW瞬变搜索。在这两种搜索中，我们都没有发现与GW相关的重要证据。鉴于我们的FRB样本的距离存在很大的不确定性，我们无法排除GW关联的可能性。评估FRB和二元合并的体积事故率，对于BNS合并，关联被限制在FRB总体的15%，对于NSBH合并，关联被限制在1%。我们报告了一系列GW前体模型到每个FRB距离的90%置信度下限，并为一系列排放场景设置了通过GW发射的能量上限。对于中心GW频率在70-3560赫兹范围内的模型，我们找到了1051-1057erg数量级的值。在这种搜索的敏感性下，我们发现这些限制高于所考虑的模型的预测GW排放量。我们也没有发现GWS与已知最接近的河外FRB中继器FRB 20200120E有显著的一致性。
We search for gravitational-wave (GW) transients associated with fast radio bursts (FRBs) detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst Project, during the first part of the third observing run of Advanced LIGO and Advanced Virgo (2019 April 1 15:00 UTC–2019 October 1 15:00 UTC). Triggers from 22 FRBs were analyzed with a search that targets both binary neutron star (BNS) and neutron star–black hole (NSBH) mergers. A targeted search for generic GW transients was conducted on 40 FRBs. We find no significant evidence for a GW association in either search. Given the large uncertainties in the distances of our FRB sample, we are unable to exclude the possibility of a GW association. Assessing the volumetric event rates of both FRB and binary mergers, an association is limited to 15% of the FRB population for BNS mergers or 1% for NSBH mergers. We report 90% confidence lower bounds on the distance to each FRB for a range of GW progenitor models and set upper limits on the energy emitted through GWs for a range of emission scenarios. We find values of order 1051–1057 erg for models with central GW frequencies in the range 70–3560 Hz. At the sensitivity of this search, we find these limits to be above the predicted GW emissions for the models considered. We also find no significant coincident detection of GWs with the repeater, FRB 20200120E, which is the closest known extragalactic FRB.