Model comparison from LIGO–Virgo data on GW170817’s binary components and consequences for the merger remnant

Abbott, B. P.; Abbott, R.; Abbott, T. D.; Abraham, S.; Acernese, F.; Ackley, K.; Adams, C.; Adya, V. B.; Affeldt, C.; Agathos, M.; Agatsuma, K.; Aggarwal, N.; Aguiar, O. D.; Aiello, L.; Ain, A.; Ajith, P.; Allen, G.; Allocca, A.; Aloy, M. A.; Altin, P. A.; Amato, A.; Anand, S.; Ananyeva, A.; Anderson, S. B.; Anderson, W. G.; Angelova, S. V.; Antier, S.; Appert, S.; Arai, K.; Araya, M. C.; Areeda, J. S.; Arène, M.; Arnaud, N.; Aronson, S. M.; Arun, K. G.; Ascenzi, S.; Ashton, G.; Aston, S. M.; Astone, P.; Aubin, F.; Aufmuth, P.; AultONeal, K.; Austin, C.; Avendano, V.; Avila-Alvarez, A.; Babak, S.; Bacon, P.; Badaracco, F.; Bader, M. K. M.; Bae, S.; Baird, J.; Baker, P. T.; Baldaccini, F.; Ballardin, G.; Ballmer, S. W.; Bals, A.; Banagiri, S.; Barayoga, J. C.; Barbieri, C.; Barclay, S. E.; Barish, B. C.; Barker, D.; Barkett, K.; Barnum, S.; Barone, F.; Barr, B.; Barsotti, L.; Barsuglia, M.; Barta, D.; Bartlett, J.; Bartos, I.; Bassiri, R.; Basti, A.; Bawaj, M.; Bayley, J. C.; Bazzan, M.; Bécsy, B.; Bejger, M.; Belahcene, I.; Bell, A. S.; Beniwal, D.; Benjamin, M. G.; Berger, B. K.; Bergmann, G.; Bernuzzi, S.; Berry, C. P. L.; Bersanetti, D.; Bertolini, A.; Betzwieser, J.; Bhandare, R.; Bidler, J.; Biggs, E.; Bilenko, I. A.; Bilgili, S. A.; Billingsley, G.; Birney, R.; Birnholtz, O.; Biscans, S.; Bischi, M.; Biscoveanu, S.; Bisht, A.; Bitossi, M.; Bizouard, M. A.; Blackburn, J. K.; Blackman, J.; Blair, C. D.; Blair, D. G.; Blair, R. M.; Bloemen, S.; Bobba, F.; Bode, N.; Boer, M.; Boetzel, Y.; Bogaert, G.; Bondu, F.; Bonnand, R.; Booker, P.; Boom, B. A.; Bork, R.; Boschi, V.; Bose, S.; Bossilkov, V.; Bosveld, J.; Bouffanais, Y.; Bozzi, A.; Bradaschia, C.; Brady, P. R.; Bramley, A.; Branchesi, M.; Brau, J. E.; Breschi, M.; Briant, T.; Briggs, J. H.; Brighenti, F.; Brillet, A.; Brinkmann, M.; Brockill, P.; Brooks, A. F.; Brooks, J.; Brown, D. D.; Brunett, S.; Buikema, A.; Bulik, T.; Bulten, H. J.; Buonanno, A.; Buskulic, D.; Buy, C.; Byer, R. L.; Cabero, M.; Cadonati, L.; Cagnoli, G.; Cahillane, C.; Calderón Bustillo, J.; Callister, T. A.; Calloni, E.; Camp, J. B.; Campbell, W. A.; Canepa, M.; Cannon, K. C.; Cao, H.; Cao, J.; Carapella, G.; Carbognani, F.; Caride, S.; Carney, M. F.; Carullo, G.; Casanueva Diaz, J.; Casentini, C.; Caudill, S.; Cavaglià, M.; Cavalier, F.; Cavalieri, R.; Cella, G.; Cerdá-Durán, P.; Cesarini, E.; Chaibi, O.; Chakravarti, K.; Chamberlin, S. J.; Chan, M.; Chao, S.; Charlton, P.; Chase, E. A.; Chassande-Mottin, E.; Chatterjee, D.; Chaturvedi, M.; Chatziioannou, K.; Cheeseboro, B. D.; Chen, H. Y.; Chen, X.; Chen, Y.; Cheng, H-P; Cheong, C. K.; Chia, H. Y.; Chiadini, F.; Chincarini, A.; Chiummo, A.; Cho, G.; Cho, H. S.; Cho, M.; Christensen, N.; Chu, Q.; Chua, S.; Chung, K. W.; Chung, S.; Ciani, G.; Cieślar, M.; Ciobanu, A. A.; Ciolfi, R.; Cipriano, F.; Cirone, A.; Clara, F.; Clark, J. A.; Clearwater, P.; Cleva, F.; Coccia, E.; Cohadon, P-F; Cohen, D.; Colleoni, M.; Collette, C. 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doi:10.1088/1361-6382/ab5f7c

Title: Model comparison from LIGO–Virgo data on GW170817’s binary components and consequences for the merger remnant

Abstract

GW170817 is the very first observation of gravitational waves originating from the coalescence of two compact objects in the mass range of neutron stars, accompanied by electromagnetic counterparts, and offers an opportunity to directly probe the internal structure of neutron stars. We perform Bayesian model selection on a wide range of theoretical predictions for the neutron star equation of state. For the binary neutron star hypothesis, we find that we cannot rule out the majority of theoretical models considered. In addition, the gravitational-wave data alone does not rule out the possibility that one or both objects were low-mass black holes. We discuss the possible outcomes in the case of a binary neutron star merger, finding that all scenarios from prompt collapse to long-lived or even stable remnants are possible. For long-lived remnants, we place an upper limit of 1.9 kHz on the rotation rate. If a black hole was formed any time after merger and the coalescing stars were slowly rotating, then the maximum baryonic mass of non-rotating neutron stars is at most 3.05 $$M_\odot$$, and three equations of state considered here can be ruled out. We obtain a tighter limit of 2.67 $$M_\odot$$ for the case that the merger results in a hypermassive neutron star.

Authors:: Abbott, B. P.; Abbott, R.; Abbott, T. D.; Abraham, S.; Acernese, F.; Ackley, K.; Adams, C.; Adya, V. B.; Affeldt, C.; Agathos, M.; Agatsuma, K.; Aggarwal, N.; Aguiar, O. D.; Aiello, L.; Ain, A.; Ajith, P.; Allen, G.; Allocca, A.; Aloy, M. A.; Altin, P. A. more »« less

Publication Date:: Thu Jan 16 00:00:00 EST 2020

Research Org.:: Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)

Sponsoring Org.:: USDOE Office of Science (SC); National Science Foundation (NSF)

Contributing Org.:: The LIGO Scientific Collaboration and The Virgo Collaboration

OSTI Identifier:: 1603630

Grant/Contract Number:: AC02-05CH11231

Resource Type:: Accepted Manuscript

Journal Name:: Classical and Quantum Gravity

Additional Journal Information:: Journal Volume: 37; Journal Issue: 4; Journal ID: ISSN 0264-9381

Publisher:: IOP Publishing

Country of Publication:: United States

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; neutron stars; neutron star equation of state; gravitational wave astronomy; compact object mergers

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                    Abbott, B. P., Abbott, R., Abbott, T. D., Abraham, S., Acernese, F., Ackley, K., Adams, C., Adya, V. B., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Allen, G., Allocca, A., Aloy, M. A., Altin, P. A., Amato, A., Anand, S., Ananyeva, A., Anderson, S. B., Anderson, W. G., Angelova, S. V., Antier, S., Appert, S., Arai, K., Araya, M. C., Areeda, J. S., Arène, M., Arnaud, N., Aronson, S. M., Arun, K. G., Ascenzi, S., Ashton, G., Aston, S. M., Astone, P., Aubin, F., Aufmuth, P., AultONeal, K., Austin, C., Avendano, V., Avila-Alvarez, A., Babak, S., Bacon, P., Badaracco, F., Bader, M. K. M., Bae, S., Baird, J., Baker, P. T., Baldaccini, F., Ballardin, G., Ballmer, S. W., Bals, A., Banagiri, S., Barayoga, J. C., Barbieri, C., Barclay, S. E., Barish, B. C., Barker, D., Barkett, K., Barnum, S., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Bawaj, M., Bayley, J. C., Bazzan, M., Bécsy, B., Bejger, M., Belahcene, I., Bell, A. S., Beniwal, D., Benjamin, M. G., Berger, B. K., Bergmann, G., Bernuzzi, S., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhandare, R., Bidler, J., Biggs, E., Bilenko, I. A., Bilgili, S. A., Billingsley, G., Birney, R., Birnholtz, O., Biscans, S., Bischi, M., Biscoveanu, S., Bisht, A., Bitossi, M., Bizouard, M. A., Blackburn, J. K., Blackman, J., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bobba, F., Bode, N., Boer, M., Boetzel, Y., Bogaert, G., Bondu, F., Bonnand, R., Booker, P., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bossilkov, V., Bosveld, J., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Bramley, A., Branchesi, M., Brau, J. E., Breschi, M., Briant, T., Briggs, J. H., Brighenti, F., Brillet, A., Brinkmann, M., Brockill, P., Brooks, A. F., Brooks, J., Brown, D. D., Brunett, S., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Calderón Bustillo, J., Callister, T. A., Calloni, E., Camp, J. B., Campbell, W. A., Canepa, M., Cannon, K. C., Cao, H., Cao, J., Carapella, G., Carbognani, F., Caride, S., Carney, M. F., Carullo, G., Casanueva Diaz, J., Casentini, C., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cerdá-Durán, P., Cesarini, E., Chaibi, O., Chakravarti, K., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chase, E. A., Chassande-Mottin, E., Chatterjee, D., Chaturvedi, M., Chatziioannou, K., Cheeseboro, B. D., Chen, H. Y., Chen, X., Chen, Y., Cheng, H-P, Cheong, C. K., Chia, H. Y., Chiadini, F., Chincarini, A., Chiummo, A., Cho, G., Cho, H. S., Cho, M., Christensen, N., Chu, Q., Chua, S., Chung, K. W., Chung, S., Ciani, G., Cieślar, M., Ciobanu, A. A., Ciolfi, R., Cipriano, F., Cirone, A., Clara, F., Clark, J. A., Clearwater, P., Cleva, F., Coccia, E., Cohadon, P-F, Cohen, D., Colleoni, M., Collette, C. G., Collins, C., Colpi, M., Cominsky, L. R., 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., Coughlin, S. B., Coulon, J-P, Countryman, S. T., Couvares, P., Covas, P. B., Cowan, E. E., Coward, D. M., Cowart, M. J., Coyne, D. C., Coyne, R., Creighton, J. D. E., Creighton, T. D., Cripe, J., Croquette, M., Crowder, S. G., Cullen, T. J., Cumming, A., Cunningham, L., Cuoco, E., Dal Canton, T., Dálya, G., D’Angelo, B., Danilishin, S. L., D’Antonio, S., Danzmann, K., Dasgupta, A., Da Silva Costa, C. F., Datrier, L. E. H., Dattilo, V., Dave, I., Davier, M., Davis, D., Daw, E. J., DeBra, D., Deenadayalan, M., Degallaix, J., De Laurentis, M., Deléglise, S., Del Pozzo, W., DeMarchi, L. M., Demos, N., Dent, T., De Pietri, R., De Rosa, R., De Rossi, C., DeSalvo, R., de Varona, O., Dhurandhar, S., Díaz, M. C., Dietrich, T., Di Fiore, L., DiFronzo, 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., Donovan, F., Dooley, K. L., Doravari, S., Dorrington, I., Downes, T. P., Drago, M., Driggers, J. C., Du, Z., Ducoin, J-G, Dupej, P., Durante, O., Dwyer, S. E., Easter, P. J., Eddolls, G., Edo, T. B., Effler, A., Ehrens, P., Eichholz, J., Eikenberry, S. S., Eisenmann, M., Eisenstein, R. A., Errico, L., Essick, R. C., Estelles, H., Estevez, D., Etienne, Z. B., Etzel, T., Evans, M., Evans, T. M., Fafone, V., Fairhurst, S., Fan, X., Farinon, S., Farr, B., Farr, W. M., Fauchon-Jones, E. J., Favata, M., Fays, M., Fazio, M., Fee, C., Feicht, J., Fejer, M. M., Feng, F., Fernandez-Galiana, A., Ferrante, I., Ferreira, E. C., Ferreira, T. A., Fidecaro, F., Fiori, I., Fiorucci, D., Fishbach, M., Fisher, R. P., Fishner, J. M., Fittipaldi, R., Fitz-Axen, M., Fiumara, V., Flaminio, R., Fletcher, M., Floden, E., Flynn, E., Fong, H., Font, J. A., Forsyth, P. W. F., Fournier, J-D, Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fritschel, P., Frolov, V. V., Fronzè, G., Fulda, P., Fyffe, M., Gabbard, H. A., Gadre, B. U., Gaebel, S. M., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., García-Quirós, C., Garufi, F., Gateley, B., Gaudio, S., Gaur, G., Gayathri, V., Gemme, G., Genin, E., Gennai, A., George, D., George, J., Gergely, L., Ghonge, S., Ghosh, Abhirup, Ghosh, Archisman, Ghosh, S., Giacomazzo, B., Giaime, J. A., Giardina, K. D., Gibson, D. R., Gill, K., Glover, L., Gniesmer, J., Godwin, P., Goetz, E., Goetz, R., Goncharov, B., González, G., Gonzalez Castro, J. M., Gopakumar, A., Gossan, S. E., Gosselin, M., Gouaty, R., Grace, B., Grado, A., Granata, M., Grant, A., Gras, S., Grassia, P., Gray, C., Gray, R., Greco, G., Green, A. C., Green, R., Gretarsson, E. M., Grimaldi, A., Grimm, S. J., Groot, P., Grote, H., Grunewald, S., Gruning, P., Guidi, G. M., Gulati, H. K., Guo, Y., Gupta, A., Gupta, Anchal, Gupta, P., Gustafson, E. K., Gustafson, R., Haegel, L., Halim, O., Hall, B. R., Hall, E. D., Hamilton, E. Z., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Hanna, C., Hannam, M. D., Hannuksela, O. A., Hansen, T. J., Hanson, J., Harder, T., Hardwick, T., Haris, K., Harms, J., Harry, G. M., Harry, I. W., Hasskew, R. K., Haster, C. J., Haughian, K., Hayes, F. J., Healy, J., Heidmann, A., Heintze, M. C., Heitmann, H., Hellman, F., Hello, P., Hemming, G., Hendry, M., Heng, I. S., Hennig, J., Hernandez Vivanco, Francisco, Heurs, M., Hild, S., Hinderer, T., Ho, W. C. G., Hochheim, S., Hofman, D., Holgado, A. M., Holland, N. A., Holt, K., Holz, D. E., Hopkins, P., Horst, C., Hough, J., Howell, E. J., Hoy, C. G., Huang, Y., Hübner, M. T., Huerta, E. A., Huet, D., Hughey, B., Hui, V., Husa, S., Huttner, S. H., Huynh-Dinh, T., Idzkowski, B., Iess, A., Inchauspe, H., Ingram, C., Inta, R., Intini, G., Irwin, B., Isa, H. N., Isac, J-M, Isi, M., Iyer, B. R., Jacqmin, T., Jadhav, S. J., Jani, K., Janthalur, N. N., Jaranowski, P., Jariwala, D., Jenkins, A. C., Jiang, J., Johnson, D. S., Jones, A. W., Jones, D. I., Jones, J. D., Jones, R., Jonker, R. J. G., Ju, L., Junker, J., Kalaghatgi, C. V., Kalogera, V., Kamai, B., Kandhasamy, S., Kang, G., Kanner, J. B., Kapadia, S. J., Karki, S., Kashyap, R., Kasprzack, M., Kastaun, W., Katsanevas, S., Katsavounidis, E., Katzman, W., Kaufer, S., Kawabe, K., Keerthana, N. V., Kéfélian, F., Keitel, D., Kennedy, R., Key, J. S., Khalili, F. Y., Khan, I., Khan, S., Khazanov, E. A., Khetan, N., Khursheed, M., Kijbunchoo, N., Kim, Chunglee, Kim, J. C., Kim, K., Kim, W., Kim, W. S., Kim, Y-M, Kimball, C., King, P. J., Kinley-Hanlon, M., Kirchhoff, R., Kissel, J. S., Kleybolte, L., Klika, J. H., Klimenko, S., Knowles, T. D., Koch, P., Koehlenbeck, S. M., Koekoek, G., Koley, S., Kondrashov, V., Kontos, A., Koper, N., Korobko, M., Korth, W. Z., Kovalam, M., Kozak, D. B., Krämer, C., Kringel, V., Krishnendu, N., Królak, A., Krupinski, N., Kuehn, G., Kumar, A., Kumar, P., Kumar, Rahul, Kumar, Rakesh, Kuo, L., Kutynia, A., Kwang, S., Lackey, B. D., Laghi, D., Lai, K. H., Lam, T. L., Landry, M., Landry, P., Lane, B. B., Lang, R. N., Lange, J., Lantz, B., Lanza, R. K., Lartaux-Vollard, A., Lasky, P. D., Laxen, M., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lecoeuche, Y. K., Lee, C. H., Lee, H. K., Lee, H. M., Lee, H. W., Lee, J., Lee, K., Lehmann, J., Lenon, A. K., Leroy, N., Letendre, N., Levin, Y., Li, A., Li, J., Li, K. J. L., Li, T. G. F., Li, X., Lin, F., Linde, F., Linker, S. D., Littenberg, T. B., Liu, J., Liu, X., Llorens-Monteagudo, M., Lo, R. K. L., London, L. T., Longo, A., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lousto, C. O., Lovelace, G., Lower, M. E., Lück, H., Lumaca, D., Lundgren, A. P., Lynch, R., Ma, Y., Macas, R., Macfoy, S., MacInnis, M., Macleod, D. M., Macquet, A., Magaña Hernandez, I., Magaña-Sandoval, F., Magee, R. M., Majorana, E., Maksimovic, I., Malik, A., Man, N., Mandic, V., Mangano, V., Mansell, G. L., Manske, M., Mantovani, M., Mapelli, M., Marchesoni, F., Marion, F., Márka, S., Márka, Z., Markakis, C., Markosyan, A. S., Markowitz, A., Maros, E., Marquina, A., Marsat, S., Martelli, F., Martin, I. W., Martin, R. M., Martinez, V., Martynov, D. V., Masalehdan, H., Mason, K., Massera, E., Masserot, A., Massinger, T. J., Masso-Reid, M., Mastrogiovanni, S., Matas, A., Matichard, F., Matone, L., Mavalvala, N., McCann, J. J., McCarthy, R., McClelland, D. E., McCormick, S., McCuller, L., McGuire, S. C., McIsaac, C., McIver, J., McManus, D. J., McRae, T., McWilliams, S. T., Meacher, D., Meadors, G. D., Mehmet, M., Mehta, A. K., Meidam, J., Mejuto Villa, E., Melatos, A., Mendell, G., Mercer, R. A., Mereni, L., Merfeld, K., Merilh, E. L., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Messina, F., Metzdorff, R., Meyers, P. M., Meylahn, F., Miani, A., Miao, H., Michel, C., Middleton, H., Milano, L., Miller, A. L., Millhouse, M., Mills, J. C., Milovich-Goff, M. C., Minazzoli, O., Minenkov, Y., Mishkin, A., Mishra, C., Mistry, T., Mitra, S., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Mo, G., Moffa, D., Mogushi, K., Mohapatra, S. R. P., Molina-Ruiz, M., Mondin, M., Montani, M., Moore, C. J., Moraru, D., Morawski, F., Moreno, G., Morisaki, S., Mours, B., Mow-Lowry, C. M., Muciaccia, F., Mukherjee, Arunava, Mukherjee, D., Mukherjee, S., Mukherjee, Subroto, Mukund, N., Mullavey, A., Munch, J., Muñiz, E. A., Muratore, M., Murray, P. G., Nagar, A., Nardecchia, I., Naticchioni, L., Nayak, R. K., Neil, B. F., Neilson, J., Nelemans, G., Nelson, T. J. N., Nery, M., Neunzert, A., Nevin, L., Ng, K. Y., Ng, S., Nguyen, C., Nguyen, P., Nichols, D., Nichols, S. A., Nissanke, S., Nocera, F., North, C., Nuttall, L. K., Obergaulinger, M., Oberling, J., O’Brien, B. D., Oganesyan, G., Ogin, G. H., Oh, J. J., Oh, S. H., Ohme, F., Ohta, H., Okada, M. A., Oliver, M., Oppermann, P., Oram, Richard J., O’Reilly, B., Ormiston, R. G., Ortega, L. F., O’Shaughnessy, R., Ossokine, S., Ottaway, D. J., Overmier, H., Owen, B. J., Pace, A. E., Pagano, G., Page, M. A., Pagliaroli, G., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Palomba, C., Pan, H., Panda, P. K., Pang, P. T. H., Pankow, C., Pannarale, F., Pant, B. C., Paoletti, F., Paoli, A., Parida, A., Parker, W., Pascucci, D., Pasqualetti, A., Passaquieti, R., Passuello, D., Patil, M., Patricelli, B., Payne, E., Pearlstone, B. L., Pechsiri, T. C., Pedersen, A. J., Pedraza, M., Pedurand, R., Pele, A., Penn, S., Perego, A., Perez, C. J., Périgois, C., Perreca, A., Petermann, J., Pfeiffer, H. P., Phelps, M., Phukon, K. S., Piccinni, O. J., Pichot, M., Piergiovanni, F., Pierro, V., Pillant, G., Pinard, L., Pinto, I. M., Pirello, M., Pitkin, M., Plastino, W., Poggiani, R., Pong, D. Y. T., Ponrathnam, S., Popolizio, P., Porter, E. K., Powell, J., Prajapati, A. K., Prasad, J., Prasai, K., Prasanna, R., Pratten, G., Prestegard, T., Principe, M., Prodi, G. A., Prokhorov, L., Punturo, M., Puppo, P., Pürrer, M., Qi, H., Quetschke, V., Quinonez, P. J., Raab, F. J., Raaijmakers, G., Radkins, H., Radulesco, N., Raffai, P., Raja, S., Rajan, C., Rajbhandari, B., Rakhmanov, M., Ramirez, K. E., Ramos-Buades, A., Rana, Javed, Rao, K., Rapagnani, P., Raymond, V., Razzano, M., Read, J., Regimbau, T., Rei, L., Reid, S., Reitze, D. H., Rettegno, P., Ricci, F., Richardson, C. J., Richardson, J. W., Ricker, P. M., Riemenschneider, G., Riles, K., Rizzo, M., Robertson, N. A., Robinet, F., Rocchi, A., Rolland, L., Rollins, J. G., Roma, V. J., Romanelli, M., Romano, R., Romel, C. L., Romie, J. H., Rose, C. A., Rose, D., Rose, K., Rosińska, D., Rosofsky, S. G., Ross, M. P., Rowan, S., Rüdiger, A., Ruggi, P., Rutins, G., Ryan, K., Sachdev, S., Sadecki, T., Sakellariadou, M., Salafia, O. S., Salconi, L., Saleem, M., Samajdar, A., Sammut, L., Sanchez, E. J., Sanchez, L. E., Sanchis-Gual, N., Sanders, J. R., Santiago, K. A., Santos, E., Sarin, N., Sassolas, B., Sathyaprakash, B. S., Sauter, O., Savage, R. L., Schale, P., Scheel, M., Scheuer, J., Schmidt, P., Schnabel, R., Schofield, R. M. S., Schönbeck, A., Schreiber, E., Schulte, B. W., Schutz, B. F., Scott, J., Scott, S. M., Seidel, E., Sellers, D., Sengupta, A. S., Sennett, N., Sentenac, D., Sequino, V., Sergeev, A., Setyawati, Y., Shaddock, D. A., Shaffer, T., Shahriar, M. S., Shaner, M. B., Sharma, A., Sharma, P., Shawhan, P., Shen, H., Shink, R., Shoemaker, D. H., Shoemaker, D. M., Shukla, K., ShyamSundar, S., Siellez, K., Sieniawska, M., Sigg, D., Singer, L. P., Singh, D., Singh, N., Singhal, A., Sintes, A. M., Sitmukhambetov, S., Skliris, V., Slagmolen, B. J. J., Slaven-Blair, T. J., Smith, J. R., Smith, R. J. E., Somala, S., Son, E. J., Soni, S., Sorazu, B., Sorrentino, F., Souradeep, T., Sowell, E., Spencer, A. P., Spera, M., Srivastava, A. K., Srivastava, V., Staats, K., Stachie, C., Standke, M., Steer, D. A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stevenson, S. P., Stocks, D., Stone, R., Stops, D. J., Strain, K. A., Stratta, G., Strigin, S. E., Strunk, A., Sturani, R., Stuver, A. L., Sudhir, V., Summerscales, T. Z., Sun, L., Sunil, S., Sur, A., Suresh, J., Sutton, P. J., Swinkels, B. L., Szczepańczyk, M. J., Tacca, M., Tait, S. C., Talbot, C., Tanner, D. B., Tao, D., Tápai, M., Tapia, A., Tasson, J. D., Taylor, R., Tenorio, R., Terkowski, L., Thomas, M., Thomas, P., Thondapu, S. R., Thorne, K. A., Thrane, E., Tiwari, Shubhanshu, Tiwari, Srishti, Tiwari, V., Toland, K., Tonelli, M., Tornasi, Z., Torres-Forné, A., Torrie, C. I., Töyrä, D., Travasso, F., Traylor, G., Tringali, M. C., Tripathee, A., Trovato, A., Trozzo, L., Tsang, K. W., Tse, M., Tso, R., Tsukada, L., Tsuna, D., Tsutsui, T., Tuyenbayev, D., Ueno, K., Ugolini, D., Unnikrishnan, C. S., Urban, A. L., Usman, S. A., Vahlbruch, H., Vajente, G., Valdes, G., Valentini, M., van Bakel, N., van Beuzekom, M., van den Brand, J. F. J., Van Den Broeck, C., Van der-Hyde, D. C., van der Schaaf, L., Van Heijningen, J. V., van Veggel, A. A., Vardaro, M., Varma, V., Vass, S., Vasúth, M., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Venkateswara, K., Venugopalan, G., Verkindt, D., Vetrano, F., Viceré, A., Viets, A. D., Vinciguerra, S., Vine, D. J., Vinet, J-Y, Vitale, S., Vo, T., Vocca, H., Vorvick, C., Vyatchanin, S. P., Wade, A. R., Wade, L. E., Wade, M., Walet, R., Walker, M., Wallace, L., Walsh, S., Wang, H., Wang, J. Z., Wang, S., Wang, W. H., Wang, Y. F., Ward, R. L., Warden, Z. A., Warner, J., Was, M., Watchi, J., Weaver, B., Wei, L-W, Weinert, M., Weinstein, A. J., Weiss, R., Wellmann, F., Wen, L., Wessel, E. K., Weßels, P., Westhouse, J. W., Wette, K., Whelan, J. T., Whiting, B. F., Whittle, C., Wilken, D. M., Williams, D., Williamson, A. R., Willis, J. L., Willke, B., Winkler, W., Wipf, C. C., Wittel, H., Woan, G., Woehler, J., Wofford, J. K., Wright, J. L., Wu, D. S., Wysocki, D. M., Xiao, S., Xu, R., Yamamoto, H., Yancey, C. C., Yang, L., Yang, Y., Yang, Z., Yap, M. J., Yazback, M., Yeeles, D. W., Yu, Hang, Yu, Haocun, Yuen, S. H. R., Zadrożny, A. K., Zadrożny, A., Zanolin, M., Zappa, F., Zelenova, T., Zendri, J-P, Zevin, M., Zhang, J., Zhang, L., Zhang, T., Zhao, C., Zhao, G., Zhou, M., Zhou, Z., Zhu, X. J., Zimmerman, A. B., Zlochower, Y., Zucker, M. E., and Zweizig, J. Model comparison from LIGO–Virgo data on GW170817’s binary components and consequences for the merger remnant.  United States: N. p., 2020. 
Web.  doi:10.1088/1361-6382/ab5f7c.

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                    Abbott, B. P., Abbott, R., Abbott, T. D., Abraham, S., Acernese, F., Ackley, K., Adams, C., Adya, V. B., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Allen, G., Allocca, A., Aloy, M. A., Altin, P. A., Amato, A., Anand, S., Ananyeva, A., Anderson, S. B., Anderson, W. G., Angelova, S. V., Antier, S., Appert, S., Arai, K., Araya, M. C., Areeda, J. S., Arène, M., Arnaud, N., Aronson, S. M., Arun, K. G., Ascenzi, S., Ashton, G., Aston, S. M., Astone, P., Aubin, F., Aufmuth, P., AultONeal, K., Austin, C., Avendano, V., Avila-Alvarez, A., Babak, S., Bacon, P., Badaracco, F., Bader, M. K. M., Bae, S., Baird, J., Baker, P. T., Baldaccini, F., Ballardin, G., Ballmer, S. W., Bals, A., Banagiri, S., Barayoga, J. C., Barbieri, C., Barclay, S. E., Barish, B. C., Barker, D., Barkett, K., Barnum, S., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Bawaj, M., Bayley, J. C., Bazzan, M., Bécsy, B., Bejger, M., Belahcene, I., Bell, A. S., Beniwal, D., Benjamin, M. G., Berger, B. K., Bergmann, G., Bernuzzi, S., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhandare, R., Bidler, J., Biggs, E., Bilenko, I. A., Bilgili, S. A., Billingsley, G., Birney, R., Birnholtz, O., Biscans, S., Bischi, M., Biscoveanu, S., Bisht, A., Bitossi, M., Bizouard, M. A., Blackburn, J. K., Blackman, J., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bobba, F., Bode, N., Boer, M., Boetzel, Y., Bogaert, G., Bondu, F., Bonnand, R., Booker, P., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bossilkov, V., Bosveld, J., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Bramley, A., Branchesi, M., Brau, J. E., Breschi, M., Briant, T., Briggs, J. H., Brighenti, F., Brillet, A., Brinkmann, M., Brockill, P., Brooks, A. F., Brooks, J., Brown, D. D., Brunett, S., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Calderón Bustillo, J., Callister, T. A., Calloni, E., Camp, J. B., Campbell, W. A., Canepa, M., Cannon, K. C., Cao, H., Cao, J., Carapella, G., Carbognani, F., Caride, S., Carney, M. F., Carullo, G., Casanueva Diaz, J., Casentini, C., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cerdá-Durán, P., Cesarini, E., Chaibi, O., Chakravarti, K., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chase, E. A., Chassande-Mottin, E., Chatterjee, D., Chaturvedi, M., Chatziioannou, K., Cheeseboro, B. D., Chen, H. Y., Chen, X., Chen, Y., Cheng, H-P, Cheong, C. K., Chia, H. Y., Chiadini, F., Chincarini, A., Chiummo, A., Cho, G., Cho, H. S., Cho, M., Christensen, N., Chu, Q., Chua, S., Chung, K. 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S., Hennig, J., Hernandez Vivanco, Francisco, Heurs, M., Hild, S., Hinderer, T., Ho, W. C. G., Hochheim, S., Hofman, D., Holgado, A. M., Holland, N. A., Holt, K., Holz, D. E., Hopkins, P., Horst, C., Hough, J., Howell, E. J., Hoy, C. G., Huang, Y., Hübner, M. T., Huerta, E. A., Huet, D., Hughey, B., Hui, V., Husa, S., Huttner, S. H., Huynh-Dinh, T., Idzkowski, B., Iess, A., Inchauspe, H., Ingram, C., Inta, R., Intini, G., Irwin, B., Isa, H. N., Isac, J-M, Isi, M., Iyer, B. R., Jacqmin, T., Jadhav, S. J., Jani, K., Janthalur, N. N., Jaranowski, P., Jariwala, D., Jenkins, A. C., Jiang, J., Johnson, D. S., Jones, A. W., Jones, D. I., Jones, J. D., Jones, R., Jonker, R. J. G., Ju, L., Junker, J., Kalaghatgi, C. V., Kalogera, V., Kamai, B., Kandhasamy, S., Kang, G., Kanner, J. B., Kapadia, S. J., Karki, S., Kashyap, R., Kasprzack, M., Kastaun, W., Katsanevas, S., Katsavounidis, E., Katzman, W., Kaufer, S., Kawabe, K., Keerthana, N. V., Kéfélian, F., Keitel, D., Kennedy, R., Key, J. 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K., Zadrożny, A., Zanolin, M., Zappa, F., Zelenova, T., Zendri, J-P, Zevin, M., Zhang, J., Zhang, L., Zhang, T., Zhao, C., Zhao, G., Zhou, M., Zhou, Z., Zhu, X. J., Zimmerman, A. B., Zlochower, Y., Zucker, M. E., & Zweizig, J. Model comparison from LIGO–Virgo data on GW170817’s binary components and consequences for the merger remnant.  United States.  https://doi.org/10.1088/1361-6382/ab5f7c

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                    Abbott, B. P., Abbott, R., Abbott, T. D., Abraham, S., Acernese, F., Ackley, K., Adams, C., Adya, V. B., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Allen, G., Allocca, A., Aloy, M. A., Altin, P. A., Amato, A., Anand, S., Ananyeva, A., Anderson, S. B., Anderson, W. G., Angelova, S. V., Antier, S., Appert, S., Arai, K., Araya, M. C., Areeda, J. S., Arène, M., Arnaud, N., Aronson, S. M., Arun, K. G., Ascenzi, S., Ashton, G., Aston, S. M., Astone, P., Aubin, F., Aufmuth, P., AultONeal, K., Austin, C., Avendano, V., Avila-Alvarez, A., Babak, S., Bacon, P., Badaracco, F., Bader, M. K. M., Bae, S., Baird, J., Baker, P. T., Baldaccini, F., Ballardin, G., Ballmer, S. W., Bals, A., Banagiri, S., Barayoga, J. C., Barbieri, C., Barclay, S. E., Barish, B. C., Barker, D., Barkett, K., Barnum, S., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Bawaj, M., Bayley, J. C., Bazzan, M., Bécsy, B., Bejger, M., Belahcene, I., Bell, A. S., Beniwal, D., Benjamin, M. G., Berger, B. K., Bergmann, G., Bernuzzi, S., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhandare, R., Bidler, J., Biggs, E., Bilenko, I. A., Bilgili, S. A., Billingsley, G., Birney, R., Birnholtz, O., Biscans, S., Bischi, M., Biscoveanu, S., Bisht, A., Bitossi, M., Bizouard, M. A., Blackburn, J. K., Blackman, J., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bobba, F., Bode, N., Boer, M., Boetzel, Y., Bogaert, G., Bondu, F., Bonnand, R., Booker, P., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bossilkov, V., Bosveld, J., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Bramley, A., Branchesi, M., Brau, J. E., Breschi, M., Briant, T., Briggs, J. 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"Model comparison from LIGO–Virgo data on GW170817’s binary components and consequences for the merger remnant".  United States.  https://doi.org/10.1088/1361-6382/ab5f7c.  https://www.osti.gov/servlets/purl/1603630.

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@article{osti_1603630,

  title        = {Model comparison from LIGO–Virgo data on GW170817’s binary components and consequences for the merger remnant},

  author       = {Abbott, B. P. and Abbott, R. and Abbott, T. D. and Abraham, S. and Acernese, F. and Ackley, K. and Adams, C. and Adya, V. B. and Affeldt, C. and Agathos, M. and Agatsuma, K. and Aggarwal, N. and Aguiar, O. D. and Aiello, L. and Ain, A. and Ajith, P. and Allen, G. and Allocca, A. and Aloy, M. A. and Altin, P. A. and Amato, A. and Anand, S. and Ananyeva, A. and Anderson, S. B. and Anderson, W. G. and Angelova, S. V. and Antier, S. and Appert, S. and Arai, K. and Araya, M. C. and Areeda, J. S. and Arène, M. and Arnaud, N. and Aronson, S. M. and Arun, K. G. and Ascenzi, S. and Ashton, G. and Aston, S. M. and Astone, P. and Aubin, F. and Aufmuth, P. and AultONeal, K. and Austin, C. and Avendano, V. and Avila-Alvarez, A. and Babak, S. and Bacon, P. and Badaracco, F. and Bader, M. K. M. and Bae, S. and Baird, J. and Baker, P. T. and Baldaccini, F. and Ballardin, G. and Ballmer, S. W. and Bals, A. and Banagiri, S. and Barayoga, J. C. and Barbieri, C. and Barclay, S. E. and Barish, B. C. and Barker, D. and Barkett, K. and Barnum, S. and Barone, F. and Barr, B. and Barsotti, L. and Barsuglia, M. and Barta, D. and Bartlett, J. and Bartos, I. and Bassiri, R. and Basti, A. and Bawaj, M. and Bayley, J. C. and Bazzan, M. and Bécsy, B. and Bejger, M. and Belahcene, I. and Bell, A. S. and Beniwal, D. and Benjamin, M. G. and Berger, B. K. and Bergmann, G. and Bernuzzi, S. and Berry, C. P. L. and Bersanetti, D. and Bertolini, A. and Betzwieser, J. and Bhandare, R. and Bidler, J. and Biggs, E. and Bilenko, I. A. and Bilgili, S. A. and Billingsley, G. and Birney, R. and Birnholtz, O. and Biscans, S. and Bischi, M. and Biscoveanu, S. and Bisht, A. and Bitossi, M. and Bizouard, M. A. and Blackburn, J. K. and Blackman, J. and Blair, C. D. and Blair, D. G. and Blair, R. M. and Bloemen, S. and Bobba, F. and Bode, N. and Boer, M. and Boetzel, Y. and Bogaert, G. and Bondu, F. and Bonnand, R. and Booker, P. and Boom, B. A. and Bork, R. and Boschi, V. and Bose, S. and Bossilkov, V. and Bosveld, J. and Bouffanais, Y. and Bozzi, A. and Bradaschia, C. and Brady, P. R. and Bramley, A. and Branchesi, M. and Brau, J. E. and Breschi, M. and Briant, T. and Briggs, J. H. and Brighenti, F. and Brillet, A. and Brinkmann, M. and Brockill, P. and Brooks, A. F. and Brooks, J. and Brown, D. D. and Brunett, S. and Buikema, A. and Bulik, T. and Bulten, H. J. and Buonanno, A. and Buskulic, D. and Buy, C. and Byer, R. L. and Cabero, M. and Cadonati, L. and Cagnoli, G. and Cahillane, C. and Calderón Bustillo, J. and Callister, T. A. and Calloni, E. and Camp, J. B. and Campbell, W. A. and Canepa, M. and Cannon, K. C. and Cao, H. and Cao, J. and Carapella, G. and Carbognani, F. and Caride, S. and Carney, M. F. and Carullo, G. and Casanueva Diaz, J. and Casentini, C. and Caudill, S. and Cavaglià, M. and Cavalier, F. and Cavalieri, R. and Cella, G. and Cerdá-Durán, P. and Cesarini, E. and Chaibi, O. and Chakravarti, K. and Chamberlin, S. J. and Chan, M. and Chao, S. and Charlton, P. and Chase, E. A. and Chassande-Mottin, E. and Chatterjee, D. and Chaturvedi, M. and Chatziioannou, K. and Cheeseboro, B. D. and Chen, H. Y. and Chen, X. and Chen, Y. and Cheng, H-P and Cheong, C. K. and Chia, H. Y. and Chiadini, F. and Chincarini, A. and Chiummo, A. and Cho, G. and Cho, H. S. and Cho, M. and Christensen, N. and Chu, Q. and Chua, S. and Chung, K. W. and Chung, S. and Ciani, G. and Cieślar, M. and Ciobanu, A. A. and Ciolfi, R. and Cipriano, F. and Cirone, A. and Clara, F. and Clark, J. A. and Clearwater, P. and Cleva, F. and Coccia, E. and Cohadon, P-F and Cohen, D. and Colleoni, M. and Collette, C. G. and Collins, C. and Colpi, M. and Cominsky, L. R. and Constancio, M. and Conti, L. and Cooper, S. J. and Corban, P. and Corbitt, T. R. and Cordero-Carrión, I. and Corezzi, S. and Corley, K. R. and Cornish, N. and Corre, D. and Corsi, A. and Cortese, S. and Costa, C. A. and Cotesta, R. and Coughlin, M. W. and Coughlin, S. B. and Coulon, J-P and Countryman, S. T. and Couvares, P. and Covas, P. B. and Cowan, E. E. and Coward, D. M. and Cowart, M. J. and Coyne, D. C. and Coyne, R. and Creighton, J. D. E. and Creighton, T. D. and Cripe, J. and Croquette, M. and Crowder, S. G. and Cullen, T. J. and Cumming, A. and Cunningham, L. and Cuoco, E. and Dal Canton, T. and Dálya, G. and D’Angelo, B. and Danilishin, S. L. and D’Antonio, S. and Danzmann, K. and Dasgupta, A. and Da Silva Costa, C. F. and Datrier, L. E. H. and Dattilo, V. and Dave, I. and Davier, M. and Davis, D. and Daw, E. J. and DeBra, D. and Deenadayalan, M. and Degallaix, J. and De Laurentis, M. and Deléglise, S. and Del Pozzo, W. and DeMarchi, L. M. and Demos, N. and Dent, T. and De Pietri, R. and De Rosa, R. and De Rossi, C. and DeSalvo, R. and de Varona, O. and Dhurandhar, S. and Díaz, M. C. and Dietrich, T. and Di Fiore, L. and DiFronzo, C. and Di Giorgio, C. and Di Giovanni, F. and Di Giovanni, M. and Di Girolamo, T. and Di Lieto, A. and Ding, B. and Di Pace, S. and Di Palma, I. and Di Renzo, F. and Divakarla, A. K. and Dmitriev, A. and Doctor, Z. and Donovan, F. and Dooley, K. L. and Doravari, S. and Dorrington, I. and Downes, T. P. and Drago, M. and Driggers, J. C. and Du, Z. and Ducoin, J-G and Dupej, P. and Durante, O. and Dwyer, S. E. and Easter, P. J. and Eddolls, G. and Edo, T. B. and Effler, A. and Ehrens, P. and Eichholz, J. and Eikenberry, S. S. and Eisenmann, M. and Eisenstein, R. A. and Errico, L. and Essick, R. C. and Estelles, H. and Estevez, D. and Etienne, Z. B. and Etzel, T. and Evans, M. and Evans, T. M. and Fafone, V. and Fairhurst, S. and Fan, X. and Farinon, S. and Farr, B. and Farr, W. M. and Fauchon-Jones, E. J. and Favata, M. and Fays, M. and Fazio, M. and Fee, C. and Feicht, J. and Fejer, M. M. and Feng, F. and Fernandez-Galiana, A. and Ferrante, I. and Ferreira, E. C. and Ferreira, T. A. and Fidecaro, F. and Fiori, I. and Fiorucci, D. and Fishbach, M. and Fisher, R. P. and Fishner, J. M. and Fittipaldi, R. and Fitz-Axen, M. and Fiumara, V. and Flaminio, R. and Fletcher, M. and Floden, E. and Flynn, E. and Fong, H. and Font, J. A. and Forsyth, P. W. F. and Fournier, J-D and Frasca, S. and Frasconi, F. and Frei, Z. and Freise, A. and Frey, R. and Frey, V. and Fritschel, P. and Frolov, V. V. and Fronzè, G. and Fulda, P. and Fyffe, M. and Gabbard, H. A. and Gadre, B. U. and Gaebel, S. M. and Gair, J. R. and Gammaitoni, L. and Gaonkar, S. G. and García-Quirós, C. and Garufi, F. and Gateley, B. and Gaudio, S. and Gaur, G. and Gayathri, V. and Gemme, G. and Genin, E. and Gennai, A. and George, D. and George, J. and Gergely, L. and Ghonge, S. and Ghosh, Abhirup and Ghosh, Archisman and Ghosh, S. and Giacomazzo, B. and Giaime, J. A. and Giardina, K. D. and Gibson, D. R. and Gill, K. and Glover, L. and Gniesmer, J. and Godwin, P. and Goetz, E. and Goetz, R. and Goncharov, B. and González, G. and Gonzalez Castro, J. M. and Gopakumar, A. and Gossan, S. E. and Gosselin, M. and Gouaty, R. and Grace, B. and Grado, A. and Granata, M. and Grant, A. and Gras, S. and Grassia, P. and Gray, C. and Gray, R. and Greco, G. and Green, A. C. and Green, R. and Gretarsson, E. M. and Grimaldi, A. and Grimm, S. J. and Groot, P. and Grote, H. and Grunewald, S. and Gruning, P. and Guidi, G. M. and Gulati, H. K. and Guo, Y. and Gupta, A. and Gupta, Anchal and Gupta, P. and Gustafson, E. K. and Gustafson, R. and Haegel, L. and Halim, O. and Hall, B. R. and Hall, E. D. and Hamilton, E. Z. and Hammond, G. and Haney, M. and Hanke, M. M. and Hanks, J. and Hanna, C. and Hannam, M. D. and Hannuksela, O. A. and Hansen, T. J. and Hanson, J. and Harder, T. and Hardwick, T. and Haris, K. and Harms, J. and Harry, G. M. and Harry, I. W. and Hasskew, R. K. and Haster, C. J. and Haughian, K. and Hayes, F. J. and Healy, J. and Heidmann, A. and Heintze, M. C. and Heitmann, H. and Hellman, F. and Hello, P. and Hemming, G. and Hendry, M. and Heng, I. S. and Hennig, J. and Hernandez Vivanco, Francisco and Heurs, M. and Hild, S. and Hinderer, T. and Ho, W. C. G. and Hochheim, S. and Hofman, D. and Holgado, A. M. and Holland, N. A. and Holt, K. and Holz, D. E. and Hopkins, P. and Horst, C. and Hough, J. and Howell, E. J. and Hoy, C. G. and Huang, Y. and Hübner, M. T. and Huerta, E. A. and Huet, D. and Hughey, B. and Hui, V. and Husa, S. and Huttner, S. H. and Huynh-Dinh, T. and Idzkowski, B. and Iess, A. and Inchauspe, H. and Ingram, C. and Inta, R. and Intini, G. and Irwin, B. and Isa, H. N. and Isac, J-M and Isi, M. and Iyer, B. R. and Jacqmin, T. and Jadhav, S. J. and Jani, K. and Janthalur, N. N. and Jaranowski, P. and Jariwala, D. and Jenkins, A. C. and Jiang, J. and Johnson, D. S. and Jones, A. W. and Jones, D. I. and Jones, J. D. and Jones, R. and Jonker, R. J. G. and Ju, L. and Junker, J. and Kalaghatgi, C. V. and Kalogera, V. and Kamai, B. and Kandhasamy, S. and Kang, G. and Kanner, J. B. and Kapadia, S. J. and Karki, S. and Kashyap, R. and Kasprzack, M. and Kastaun, W. and Katsanevas, S. and Katsavounidis, E. and Katzman, W. and Kaufer, S. and Kawabe, K. and Keerthana, N. V. and Kéfélian, F. and Keitel, D. and Kennedy, R. and Key, J. S. and Khalili, F. Y. and Khan, I. and Khan, S. and Khazanov, E. A. and Khetan, N. and Khursheed, M. and Kijbunchoo, N. and Kim, Chunglee and Kim, J. C. and Kim, K. and Kim, W. and Kim, W. S. and Kim, Y-M and Kimball, C. and King, P. J. and Kinley-Hanlon, M. and Kirchhoff, R. and Kissel, J. S. and Kleybolte, L. and Klika, J. H. and Klimenko, S. and Knowles, T. D. and Koch, P. and Koehlenbeck, S. M. and Koekoek, G. and Koley, S. and Kondrashov, V. and Kontos, A. and Koper, N. and Korobko, M. and Korth, W. Z. and Kovalam, M. and Kozak, D. B. and Krämer, C. and Kringel, V. and Krishnendu, N. and Królak, A. and Krupinski, N. and Kuehn, G. and Kumar, A. and Kumar, P. and Kumar, Rahul and Kumar, Rakesh and Kuo, L. and Kutynia, A. and Kwang, S. and Lackey, B. D. and Laghi, D. and Lai, K. H. and Lam, T. L. and Landry, M. and Landry, P. and Lane, B. B. and Lang, R. N. and Lange, J. and Lantz, B. and Lanza, R. K. and Lartaux-Vollard, A. and Lasky, P. D. and Laxen, M. and Lazzarini, A. and Lazzaro, C. and Leaci, P. and Leavey, S. and Lecoeuche, Y. K. and Lee, C. H. and Lee, H. K. and Lee, H. M. and Lee, H. W. and Lee, J. and Lee, K. and Lehmann, J. and Lenon, A. K. and Leroy, N. and Letendre, N. and Levin, Y. and Li, A. and Li, J. and Li, K. J. L. and Li, T. G. F. and Li, X. and Lin, F. and Linde, F. and Linker, S. D. and Littenberg, T. B. and Liu, J. and Liu, X. and Llorens-Monteagudo, M. and Lo, R. K. L. and London, L. T. and Longo, A. and Lorenzini, M. and Loriette, V. and Lormand, M. and Losurdo, G. and Lough, J. D. and Lousto, C. O. and Lovelace, G. and Lower, M. E. and Lück, H. and Lumaca, D. and Lundgren, A. P. and Lynch, R. and Ma, Y. and Macas, R. and Macfoy, S. and MacInnis, M. and Macleod, D. M. and Macquet, A. and Magaña Hernandez, I. and Magaña-Sandoval, F. and Magee, R. M. and Majorana, E. and Maksimovic, I. and Malik, A. and Man, N. and Mandic, V. and Mangano, V. and Mansell, G. L. and Manske, M. and Mantovani, M. and Mapelli, M. and Marchesoni, F. and Marion, F. and Márka, S. and Márka, Z. and Markakis, C. and Markosyan, A. S. and Markowitz, A. and Maros, E. and Marquina, A. and Marsat, S. and Martelli, F. and Martin, I. W. and Martin, R. M. and Martinez, V. and Martynov, D. V. and Masalehdan, H. and Mason, K. and Massera, E. and Masserot, A. and Massinger, T. J. and Masso-Reid, M. and Mastrogiovanni, S. and Matas, A. and Matichard, F. and Matone, L. and Mavalvala, N. and McCann, J. J. and McCarthy, R. and McClelland, D. E. and McCormick, S. and McCuller, L. and McGuire, S. C. and McIsaac, C. and McIver, J. and McManus, D. J. and McRae, T. and McWilliams, S. T. and Meacher, D. and Meadors, G. D. and Mehmet, M. and Mehta, A. K. and Meidam, J. and Mejuto Villa, E. and Melatos, A. and Mendell, G. and Mercer, R. A. and Mereni, L. and Merfeld, K. and Merilh, E. L. and Merzougui, M. and Meshkov, S. and Messenger, C. and Messick, C. and Messina, F. and Metzdorff, R. and Meyers, P. M. and Meylahn, F. and Miani, A. and Miao, H. and Michel, C. and Middleton, H. and Milano, L. and Miller, A. L. and Millhouse, M. and Mills, J. C. and Milovich-Goff, M. C. and Minazzoli, O. and Minenkov, Y. and Mishkin, A. and Mishra, C. and Mistry, T. and Mitra, S. and Mitrofanov, V. P. and Mitselmakher, G. and Mittleman, R. and Mo, G. and Moffa, D. and Mogushi, K. and Mohapatra, S. R. P. and Molina-Ruiz, M. and Mondin, M. and Montani, M. and Moore, C. J. and Moraru, D. and Morawski, F. and Moreno, G. and Morisaki, S. and Mours, B. and Mow-Lowry, C. M. and Muciaccia, F. and Mukherjee, Arunava and Mukherjee, D. and Mukherjee, S. and Mukherjee, Subroto and Mukund, N. and Mullavey, A. and Munch, J. and Muñiz, E. A. and Muratore, M. and Murray, P. G. and Nagar, A. and Nardecchia, I. and Naticchioni, L. and Nayak, R. K. and Neil, B. F. and Neilson, J. and Nelemans, G. and Nelson, T. J. N. and Nery, M. and Neunzert, A. and Nevin, L. and Ng, K. Y. and Ng, S. and Nguyen, C. and Nguyen, P. and Nichols, D. and Nichols, S. A. and Nissanke, S. and Nocera, F. and North, C. and Nuttall, L. K. and Obergaulinger, M. and Oberling, J. and O’Brien, B. D. and Oganesyan, G. and Ogin, G. H. and Oh, J. J. and Oh, S. H. and Ohme, F. and Ohta, H. and Okada, M. A. and Oliver, M. and Oppermann, P. and Oram, Richard J. and O’Reilly, B. and Ormiston, R. G. and Ortega, L. F. and O’Shaughnessy, R. and Ossokine, S. and Ottaway, D. J. and Overmier, H. and Owen, B. J. and Pace, A. E. and Pagano, G. and Page, M. A. and Pagliaroli, G. and Pai, A. and Pai, S. A. and Palamos, J. R. and Palashov, O. and Palomba, C. and Pan, H. and Panda, P. K. and Pang, P. T. H. and Pankow, C. and Pannarale, F. and Pant, B. C. and Paoletti, F. and Paoli, A. and Parida, A. and Parker, W. and Pascucci, D. and Pasqualetti, A. and Passaquieti, R. and Passuello, D. and Patil, M. and Patricelli, B. and Payne, E. and Pearlstone, B. L. and Pechsiri, T. C. and Pedersen, A. J. and Pedraza, M. and Pedurand, R. and Pele, A. and Penn, S. and Perego, A. and Perez, C. J. and Périgois, C. and Perreca, A. and Petermann, J. and Pfeiffer, H. P. and Phelps, M. and Phukon, K. S. and Piccinni, O. J. and Pichot, M. and Piergiovanni, F. and Pierro, V. and Pillant, G. and Pinard, L. and Pinto, I. M. and Pirello, M. and Pitkin, M. and Plastino, W. and Poggiani, R. and Pong, D. Y. T. and Ponrathnam, S. and Popolizio, P. and Porter, E. K. and Powell, J. and Prajapati, A. K. and Prasad, J. and Prasai, K. and Prasanna, R. and Pratten, G. and Prestegard, T. and Principe, M. and Prodi, G. A. and Prokhorov, L. and Punturo, M. and Puppo, P. and Pürrer, M. and Qi, H. and Quetschke, V. and Quinonez, P. J. and Raab, F. J. and Raaijmakers, G. and Radkins, H. and Radulesco, N. and Raffai, P. and Raja, S. and Rajan, C. and Rajbhandari, B. and Rakhmanov, M. and Ramirez, K. E. and Ramos-Buades, A. and Rana, Javed and Rao, K. and Rapagnani, P. and Raymond, V. and Razzano, M. and Read, J. and Regimbau, T. and Rei, L. and Reid, S. and Reitze, D. H. and Rettegno, P. and Ricci, F. and Richardson, C. J. and Richardson, J. W. and Ricker, P. M. and Riemenschneider, G. and Riles, K. and Rizzo, M. and Robertson, N. A. and Robinet, F. and Rocchi, A. and Rolland, L. and Rollins, J. G. and Roma, V. J. and Romanelli, M. and Romano, R. and Romel, C. L. and Romie, J. H. and Rose, C. A. and Rose, D. and Rose, K. and Rosińska, D. and Rosofsky, S. G. and Ross, M. P. and Rowan, S. and Rüdiger, A. and Ruggi, P. and Rutins, G. and Ryan, K. and Sachdev, S. and Sadecki, T. and Sakellariadou, M. and Salafia, O. S. and Salconi, L. and Saleem, M. and Samajdar, A. and Sammut, L. and Sanchez, E. J. and Sanchez, L. E. and Sanchis-Gual, N. and Sanders, J. R. and Santiago, K. A. and Santos, E. and Sarin, N. and Sassolas, B. and Sathyaprakash, B. S. and Sauter, O. and Savage, R. L. and Schale, P. and Scheel, M. and Scheuer, J. and Schmidt, P. and Schnabel, R. and Schofield, R. M. S. and Schönbeck, A. and Schreiber, E. and Schulte, B. W. and Schutz, B. F. and Scott, J. and Scott, S. M. and Seidel, E. and Sellers, D. and Sengupta, A. 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  abstractNote = {GW170817 is the very first observation of gravitational waves originating from the coalescence of two compact objects in the mass range of neutron stars, accompanied by electromagnetic counterparts, and offers an opportunity to directly probe the internal structure of neutron stars. We perform Bayesian model selection on a wide range of theoretical predictions for the neutron star equation of state. For the binary neutron star hypothesis, we find that we cannot rule out the majority of theoretical models considered. In addition, the gravitational-wave data alone does not rule out the possibility that one or both objects were low-mass black holes. We discuss the possible outcomes in the case of a binary neutron star merger, finding that all scenarios from prompt collapse to long-lived or even stable remnants are possible. For long-lived remnants, we place an upper limit of 1.9 kHz on the rotation rate. If a black hole was formed any time after merger and the coalescing stars were slowly rotating, then the maximum baryonic mass of non-rotating neutron stars is at most 3.05 $M_\odot$, and three equations of state considered here can be ruled out. We obtain a tighter limit of 2.67 $M_\odot$ for the case that the merger results in a hypermassive neutron star.},

  doi          = {10.1088/1361-6382/ab5f7c},

  journal      = {Classical and Quantum Gravity},

  number       = 4,

  volume       = 37,

  place        = {United States},

  year         = {Thu Jan 16 00:00:00 EST 2020},

  month        = {Thu Jan 16 00:00:00 EST 2020}

}

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Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817
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Collaboration, The LIGO Scientific; Collaboration, The Virgo; Abbott, B. P.
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Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817
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Collaboration, The LIGO Scientific; Collaboration, The Virgo; Abbott, B. P.
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Search for Post-merger Gravitational Waves from the Remnant of the Binary Neutron Star Merger GW170817

Journal Article Abbott, B. P. ; Abbott, R. ; Abbott, T. D. ; ... - The Astrophysical Journal. Letters (Online)

The first observation of a binary neutron star (NS) coalescence by the Advanced LIGO and Advanced Virgo gravitational-wave (GW) detectors offers an unprecedented opportunity to study matter under the most extreme conditions. After such a merger, a compact remnant is left over whose nature depends primarily on the masses of the inspiraling objects and on the equation of state of nuclear matter. This could be either a black hole (BH) or an NS, with the latter being either long-lived or too massive for stability implying delayed collapse to a BH. In this work, we introduce a search for GWs from the remnant of the binary NS merger GW170817 using data from Advanced LIGO and Advanced Virgo. We search for short- (lesssim1 s) and intermediate-duration (lesssim500 s) signals, which include GW emission from a hypermassive NS or supramassive NS, respectively. We find no signal from the post-merger remnant. Our derived strain upper limits are more than an order of magnitude larger than those predicted by most models. For short signals, our best upper limit on the root sum square of the GW strain emitted from 1–4 kHz ismore »« less
Cited by 146
https://doi.org/10.3847/2041-8213/aa9a35

Full Text Available
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. VII. Properties of the Host Galaxy and Constraints on the Merger Timescale

Journal Article Blanchard, P. K. ; Berger, E. ; Fong, W. ; ... - The Astrophysical Journal. Letters (Online)

We present the properties of NGC 4993, the host galaxy of GW170817, the first gravitational wave (GW) event from the merger of a binary neutron star (BNS) system and the first with an electromagnetic (EM) counterpart. We use both archival photometry and new optical/near-IR imaging and spectroscopy, together with stellar population synthesis models to infer the global properties of the host galaxy. We infer a star formation history peaked atmore »« less
Cited by 70
https://doi.org/10.3847/2041-8213/aa9055

Full Text Available
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. III. Optical and UV Spectra of a Blue Kilonova from Fast Polar Ejecta

Journal Article Nicholl, Matt ; Berger, E. ; Kasen, D. ; ... - The Astrophysical Journal. Letters (Online)

Here, we present optical and ultraviolet spectra of the first electromagnetic counterpart to a gravitational wave (GW) source, the binary neutron star merger GW170817. Spectra were obtained nightly between 1.5 and 9.5 days post-merger, using the SOAR and Magellan telescopes; the UV spectrum was obtained with the Hubble Space Telescope at 5.5 days. Our data reveal a rapidly-fading blue component (more »« less
Cited by 266
https://doi.org/10.3847/2041-8213/aa9029

Full Text Available
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. III. Optical and UV Spectra of a Blue Kilonova from Fast Polar Ejecta

Journal Article Nicholl, M. ; Berger, E. ; Alexander, K. D. ; ... - Astrophysical Journal Letters

We present optical and ultraviolet spectra of the first electromagnetic counterpart to a gravitational-wave (GW) source, the binary neutron star merger GW170817. Spectra were obtained nightly between 1.5 and 9.5 days post-merger, using the Southern Astrophysical Research and Magellan telescopes; the UV spectrum was obtained with the Hubble Space Telescope at 5.5 days. Our data reveal a rapidly fading blue component (T≈5500 K at 1.5 days) that quickly reddens; spectra later than ≳4.5 days peak beyond the optical regime. The spectra are mostly featureless, although we identify a possible weak emission line at ∼7900 Å at t≲4.5 days. The colors,more »« less
https://doi.org/10.3847/2041-8213/AA9029
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. VII. Properties of the Host Galaxy and Constraints on the Merger Timescale

Journal Article Blanchard, P. K. ; Berger, E. ; Nicholl, M. ; ... - Astrophysical Journal Letters

We present the properties of NGC 4993, the host galaxy of GW170817, the first gravitational-wave (GW) event from the merger of a binary neutron star (BNS) system and the first with an electromagnetic (EM) counterpart. We use both archival photometry and new optical/near-IR imaging and spectroscopy, together with stellar population synthesis models to infer the global properties of the host galaxy. We infer a star formation history peaked at ≳10 Gyr ago, with subsequent exponential decline leading to a low current star formation rate of 0.01 M{sub ⊙} yr{sup −1}, which we convert into a binary merger timescale probability distribution.more »« less
https://doi.org/10.3847/2041-8213/AA9055

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Title: Model comparison from LIGO–Virgo data on GW170817’s binary components and consequences for the merger remnant

Abstract

Citation Formats

Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817 journal, August 2018

Gamma-Ray Burst Afterglow with Continuous Energy Injection: Signature of a Highly Magnetized Millisecond Pulsar journal, May 2001

GW170817: Observation of gravitational waves from a binary neutron star inspiral text, January 2017

Advanced Virgo: a second-generation interferometric gravitational wave detector journal, December 2014

Masses, Radii, and the Equation of State of Neutron Stars journal, September 2016

Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of GW170817 journal, November 2017

Symmetry energy I: Semi-infinite matter journal, February 2009

Neutron Skins and Neutron Stars in the Multimessenger Era journal, April 2018

Gravitational-Wave Constraints on the Neutron-Star-Matter Equation of State journal, April 2018

Observing the post-merger signal of GW170817-like events with improved gravitational-wave detectors journal, February 2019

Revisiting the Lower Bound on Tidal Deformability Derived by AT 2017gfo journal, May 2019

Binary neutron star mergers: a review of Einstein’s richest laboratory journal, July 2017

Origin of the heavy elements in binary neutron-star mergers from a gravitational-wave event journal, October 2017

Probing the internal composition of neutron stars with gravitational waves journal, November 2015

Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral journal, June 2010

Parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library journal, February 2015

Reconstructing the calibrated strain signal in the Advanced LIGO detectors journal, April 2018

Waveform systematics for binary neutron star gravitational wave signals: Effects of the point-particle baseline and tidal descriptions journal, December 2018

Matter imprints in waveform models for neutron star binaries: Tidal and self-spin effects journal, January 2019

GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs journal, September 2019

Improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors journal, February 2017

Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors journal, February 2016

Improving astrophysical parameter estimation via offline noise subtraction for Advanced LIGO journal, February 2019

On the mass Distribution and Birth Masses of Neutron Stars journal, September 2012

Comprehensive comparison of numerical relativity and effective-one-body results to inform improvements in waveform models for binary neutron star systems journal, June 2017

Equation of state for dense nucleon matter journal, August 1988

Nonparametric inference of the neutron star equation of state from gravitational wave observations journal, April 2019

Using Gravitational-wave Observations and Quasi-universal Relations to Constrain the Maximum Mass of Neutron Stars journal, January 2018

GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations journal, January 2018

Measurability of the tidal polarizability of neutron stars in late-inspiral gravitational-wave signals journal, June 2012

Quadratic-in-spin effects in the orbital dynamics and gravitational-wave energy flux of compact binaries at the 3PN order journal, September 2015

γ -Ray Bursts and Afterglows from Rotating Strange Stars and Neutron Stars journal, November 1998

Modeling the Complete Gravitational Wave Spectrum of Neutron Star Mergers journal, August 2015

Short-duration gamma-ray bursts with extended emission from protomagnetar spin-down journal, April 2008

Radiative Transfer Simulation for the Optical and Near-infrared Electromagnetic Counterparts to GW170817 journal, September 2018

Constraining the neutron star equation of state with gravitational wave signals from coalescing binary neutron stars journal, July 2015

Inferring the post-merger gravitational wave emission from binary neutron star coalescences journal, December 2017

Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries journal, February 2014

Tidal Deformability from GW170817 as a Direct Probe of the Neutron Star Radius journal, April 2018

Approximate universal relations for neutron stars and quark stars journal, April 2017

Relativistic tidal properties of neutron stars journal, October 2009

Skyrme-force parametrization: Least-squares fit to nuclear ground-state properties journal, January 1986

Properties of the Binary Neutron Star Merger GW170817 journal, January 2019

Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817 journal, October 2018

Dynamical tides in general relativity: Effective action and effective-one-body Hamiltonian journal, November 2016

Structure of proton drip-line nuclei around doubly magic Ni 48 journal, February 1996

Bayeswave: Bayesian inference for gravitational wave bursts and instrument glitches journal, June 2015

Effective-one-body multipolar waveform for tidally interacting binary neutron stars up to merger journal, February 2019

Binary neutron star mergers: Dependence on the nuclear equation of state journal, June 2011

Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817 journal, December 2017

Equation of state of nucleon matter and neutron star structure journal, September 1998

Frequency-domain gravitational waves from nonprecessing black-hole binaries. II. A phenomenological model for the advanced detector era journal, February 2016

Neutron-star Radius Constraints from GW170817 and Future Detections journal, November 2017

The Nuclear Equation of State and Neutron Star Masses journal, November 2012

Systematic and statistical errors in a Bayesian approach to the estimation of the neutron-star equation of state using advanced gravitational wave detectors journal, May 2014

Charge distributions of Pb 208 , Pb 206 , and Tl 205 and the mean-field approximation journal, December 1989

Formation of Double Neutron Star Systems journal, September 2017

Multi-messenger Observations of a Binary Neutron Star Merger journal, October 2017

Modeling dynamical ejecta from binary neutron star mergers and implications for electromagnetic counterparts journal, April 2017

Shape coexistence and the effective nucleon-nucleon interaction journal, June 1999

Frequency-domain gravitational waves from nonprecessing black-hole binaries. I. New numerical waveforms and anatomy of the signal journal, February 2016

Constraints on interquark interaction parameters with GW170817 in a binary strange star scenario journal, April 2018

The Neutron star mass Distribution journal, November 2013

Constraining neutron-star tidal Love numbers with gravitational-wave detectors journal, January 2008

Causal representations of neutron-star equations of state journal, June 2018

The double pulsar system: a unique laboratory for gravity journal, February 2009

Bayes Factors journal, June 1995

Static Solutions of Einstein's Field Equations for Spheres of Fluid journal, February 1939

The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models journal, October 2017

Post-1-Newtonian tidal effects in the gravitational waveform from binary inspirals journal, April 2011

Merger of binary neutron stars to a black hole: Disk mass, short gamma-ray bursts, and quasinormal mode ringing journal, March 2006

New Constraints on Radii and Tidal Deformabilities of Neutron Stars from GW170817 journal, June 2018

Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides, and self-spin effects journal, November 2018

From hadrons to quarks in neutron stars: a review journal, March 2018

Unified picture of the post-merger dynamics and gravitational wave emission in neutron star mergers journal, June 2015

Search for Gravitational Waves from a Long-lived Remnant of the Binary Neutron Star Merger GW170817 journal, April 2019

The Timing of nine Globular Cluster Pulsars journal, January 2012

Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817
journal, August 2018

Gamma-Ray Burst Afterglow with Continuous Energy Injection: Signature of a Highly Magnetized Millisecond Pulsar
journal, May 2001

GW170817: Observation of gravitational waves from a binary neutron star inspiral
text, January 2017

Advanced Virgo: a second-generation interferometric gravitational wave detector
journal, December 2014

Masses, Radii, and the Equation of State of Neutron Stars
journal, September 2016

Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of GW170817
journal, November 2017

Symmetry energy I: Semi-infinite matter
journal, February 2009

Neutron Skins and Neutron Stars in the Multimessenger Era
journal, April 2018

Gravitational-Wave Constraints on the Neutron-Star-Matter Equation of State
journal, April 2018

Observing the post-merger signal of GW170817-like events with improved gravitational-wave detectors
journal, February 2019

Revisiting the Lower Bound on Tidal Deformability Derived by AT 2017gfo
journal, May 2019

Binary neutron star mergers: a review of Einstein’s richest laboratory
journal, July 2017

Origin of the heavy elements in binary neutron-star mergers from a gravitational-wave event
journal, October 2017

Probing the internal composition of neutron stars with gravitational waves
journal, November 2015

Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral
journal, June 2010

Parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
journal, February 2015

Reconstructing the calibrated strain signal in the Advanced LIGO detectors
journal, April 2018

Waveform systematics for binary neutron star gravitational wave signals: Effects of the point-particle baseline and tidal descriptions
journal, December 2018

Matter imprints in waveform models for neutron star binaries: Tidal and self-spin effects
journal, January 2019

GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
journal, September 2019

Improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
journal, February 2017

Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors
journal, February 2016

Improving astrophysical parameter estimation via offline noise subtraction for Advanced LIGO
journal, February 2019

On the mass Distribution and Birth Masses of Neutron Stars
journal, September 2012

Comprehensive comparison of numerical relativity and effective-one-body results to inform improvements in waveform models for binary neutron star systems
journal, June 2017

Equation of state for dense nucleon matter
journal, August 1988

Nonparametric inference of the neutron star equation of state from gravitational wave observations
journal, April 2019

Using Gravitational-wave Observations and Quasi-universal Relations to Constrain the Maximum Mass of Neutron Stars
journal, January 2018

GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations
journal, January 2018

Measurability of the tidal polarizability of neutron stars in late-inspiral gravitational-wave signals
journal, June 2012

Quadratic-in-spin effects in the orbital dynamics and gravitational-wave energy flux of compact binaries at the 3PN order
journal, September 2015

$γ$ -Ray Bursts and Afterglows from Rotating Strange Stars and Neutron Stars
journal, November 1998

Modeling the Complete Gravitational Wave Spectrum of Neutron Star Mergers
journal, August 2015

Short-duration gamma-ray bursts with extended emission from protomagnetar spin-down
journal, April 2008

Radiative Transfer Simulation for the Optical and Near-infrared Electromagnetic Counterparts to GW170817
journal, September 2018

Constraining the neutron star equation of state with gravitational wave signals from coalescing binary neutron stars
journal, July 2015

Inferring the post-merger gravitational wave emission from binary neutron star coalescences
journal, December 2017

Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries
journal, February 2014

Tidal Deformability from GW170817 as a Direct Probe of the Neutron Star Radius
journal, April 2018

Approximate universal relations for neutron stars and quark stars
journal, April 2017

Relativistic tidal properties of neutron stars
journal, October 2009

Skyrme-force parametrization: Least-squares fit to nuclear ground-state properties
journal, January 1986

Properties of the Binary Neutron Star Merger GW170817
journal, January 2019

Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817
journal, October 2018

Dynamical tides in general relativity: Effective action and effective-one-body Hamiltonian
journal, November 2016

Structure of proton drip-line nuclei around doubly magic ${}^{48}{Ni}$
journal, February 1996

Bayeswave: Bayesian inference for gravitational wave bursts and instrument glitches
journal, June 2015

Effective-one-body multipolar waveform for tidally interacting binary neutron stars up to merger
journal, February 2019

Binary neutron star mergers: Dependence on the nuclear equation of state
journal, June 2011

Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817
journal, December 2017

Equation of state of nucleon matter and neutron star structure
journal, September 1998

Frequency-domain gravitational waves from nonprecessing black-hole binaries. II. A phenomenological model for the advanced detector era
journal, February 2016

Neutron-star Radius Constraints from GW170817 and Future Detections
journal, November 2017

The Nuclear Equation of State and Neutron Star Masses
journal, November 2012

Systematic and statistical errors in a Bayesian approach to the estimation of the neutron-star equation of state using advanced gravitational wave detectors
journal, May 2014

Charge distributions of ${}^{208}{Pb}$ , ${}^{206}{Pb}$ , and ${}^{205}{Tl}$ and the mean-field approximation
journal, December 1989

Formation of Double Neutron Star Systems
journal, September 2017

Multi-messenger Observations of a Binary Neutron Star Merger
journal, October 2017

Modeling dynamical ejecta from binary neutron star mergers and implications for electromagnetic counterparts
journal, April 2017

Shape coexistence and the effective nucleon-nucleon interaction
journal, June 1999

Frequency-domain gravitational waves from nonprecessing black-hole binaries. I. New numerical waveforms and anatomy of the signal
journal, February 2016

Constraints on interquark interaction parameters with GW170817 in a binary strange star scenario
journal, April 2018

The Neutron star mass Distribution
journal, November 2013

Constraining neutron-star tidal Love numbers with gravitational-wave detectors
journal, January 2008

Causal representations of neutron-star equations of state
journal, June 2018

The double pulsar system: a unique laboratory for gravity
journal, February 2009

Bayes Factors
journal, June 1995

Static Solutions of Einstein's Field Equations for Spheres of Fluid
journal, February 1939

The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models
journal, October 2017

Post-1-Newtonian tidal effects in the gravitational waveform from binary inspirals
journal, April 2011

Merger of binary neutron stars to a black hole: Disk mass, short gamma-ray bursts, and quasinormal mode ringing
journal, March 2006

New Constraints on Radii and Tidal Deformabilities of Neutron Stars from GW170817
journal, June 2018

Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides, and self-spin effects
journal, November 2018

From hadrons to quarks in neutron stars: a review
journal, March 2018

Unified picture of the post-merger dynamics and gravitational wave emission in neutron star mergers
journal, June 2015

Search for Gravitational Waves from a Long-lived Remnant of the Binary Neutron Star Merger GW170817
journal, April 2019

The Timing of nine Globular Cluster Pulsars
journal, January 2012

Effective action approach to higher-order relativistic tidal interactions in binary systems and their effective one body description
journal, June 2012

Accurate evolutions of inspiralling neutron-star binaries: Prompt and delayed collapse to a black hole
journal, October 2008

A Massive Pulsar in a Compact Relativistic Binary
journal, April 2013