@Article{AbbottAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAABBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBCCCCBCCCCCCCCCCCCCDCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCDDDDDDCDDDDDDDDDLDLPDDDPRRDVDDDFDGGGGLDPPRDDDDDDDDDDDDDDDDEEEEEEEEEEEEEEEEEFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFVFFFFFFFFFFFGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGCGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHIIIIIIIIIIIJJJJJJJJJJJJJJJJJKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLMMMMMMHMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMVMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMNNNNNNNNNNNNNNNNNNNNNOOOOOOOOOOOOOOOOOOOOOPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPQQQRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSTTTTTTTTTTTTTTTTTTTTTTTTTTTTTTTTTTTTTTUUUUUVVVVBBBBVSVVVVVVVVVVVVVVVVVVVVVVVVWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWXXYYYYYYYYYYYZZZZZZZZZZZZZZZZZ:2020:ObCoBi,
author = "Abbott, B. P. and Abbott, R. and Abbott, T. D. and Abraham, S. and
Acernese, F. and Ackley, K. and Adams, C. and Adhikari, R. X. and
Adya, V. B. and Affeldt, C. and Agathos, M. and Agatsuma, K. and
Aggarwal, N. and Aguiar, Odylio Denys de 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 Ar{\`e}ne, 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 Baylor, A. C. and Bazzan, M. and B{\'e}csy, 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,
David 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 Bustillo, J. Calder{\'o}n 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 Diaz, J. Casanueva and Casentini, C. and Caudill, S. and
Cavagli{\`a}, M. and Cavalier, F. and Cavalieri, R. and Cella, G.
and Cerd{\'a}-Dur{\'a}n, 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 Cie'Lar, 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{\'a}rcio and Conti, L. and Cooper, S. J. and Corban, P. and
Corbitt, T. R. and Cordero-Carri{\'o}n, 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.
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Crowder, S. G. and Cullen, T. J. and Cumming, A. and Cunningham,
L. and Cuoco, E. and Canton, T. Dal and D{\'a}lya, G. and
D?angelo, B. and Danilishin, S. L. and D?antonio, S. and Danzmann,
K. and Dasgupta, A. and Costa, C. F. da Silva 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 Laurentis, M. de and Del{\'e}glise, S. and Lillo, N. de and
Pozzo, W. Del and Demarchi, L. M. and Demos, N. and Dent, T. and
Pietri, R. de and Rosa, R. de and Rossi, C. de and Desalvo, R. and
Varona, O. de and Dhurandhar, S. and D{\'{\i}}az, M. C. and
Dietrich, T. and Fiore, L. Di and Difronzo, C. and Giorgio, C. Di
and Giovanni, F. Di and Giovanni, M. Di and Girolamo, T. Di and
Lieto, A. Di and Ding, B. and Pace, S. Di and Palma, I. Di and
Renzo, F. Di and Divakarla, A. K. and Dmitriev, A. and Doctor, Z.
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and Ducoin, J. -G. and Dudi, R. 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, Elvis
Camilo and Ferreira, Tabata Aira 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 Vivanco, Francisco Hernandez and Frasca, S. and Frasconi,
F. and Frei, Z. and Freise, A. and Frey, R. and Frey, V. and
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and Fyffe, M. and Gabbard, H. A. and Gadre, B. U. and Gaebel, S.
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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
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G. and Haney, M. and Hanke, M. M. and Hanks, J. and Hanna, C. and
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J. and Harder, T. and Hardwick, T. and Haris, K. and Harms, J. and
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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
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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
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and Hui, V. and Husa, S. and Huttner, S. H. and Huynh-Dinh, T. and
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and Kovalam, M. and Kozak, D. B. and Kr{\"a}mer, C. and Kringel,
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affiliation = "{} and {} and {} and {} and {} and {} and {} and {} and {} and {}
and {} and {} and {} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {} and {} and {} and {} and {} and {} and {}
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and {} and {} and {} and {} and {} and {} and {} and {} and {} and
{} and {} and {} and {} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {} and {} and {} and {} and {} and {} and {}
and {} and {} and {} and {} and {} and {} and {} and {} and {} and
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and {} and {} and {} and {} and {} and {} and {} and {} and {} and
{} and {} and {} and {} and {} and {} and {} and {} and {} and {}
and {} and {} and {} and {} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)}",
title = "GW190425: observation of a compact binary coalescence with total
mass ~3.4M",
journal = "The Astrophysical Journal",
year = "2020",
volume = "892",
number = "1",
pages = "L3",
keywords = "GW190425, Compact binary coalescences, neutron stars.",
abstract = "On 2019 April 25, the LIGO Livingston detector observed a compact
binary coalescence with signal-to-noise ratio 12.9. The Virgo
detector was also taking data that did not contribute to detection
due to a low signal-to-noise ratio, but were used for subsequent
parameter estimation. The 90% credible intervals for the component
masses range from1.12 to 2.52 M\ (1.461.87 M\ if
we restrict the dimensionless component spin magnitudes to be
smaller than 0.05). These mass parameters are consistent with the
individual binary components being neutron stars. However, both
the source-frame chirp mass - 1.44+ 0.02 0.02 M\ and the
total mass - 3.4+ 0.1 0.3M\ of this system are
significantly larger than those of any other known binary neutron
star (BNS) system. The possibility that one or both binary
components of the system are black holes cannot be ruled out from
gravitational-wave data. We discuss possible origins of the system
based on its inconsistency with the known Galactic BNS population.
Under the assumption that the signal was produced by a BNS
coalescence, the local rate of neutron star mergers is updated to
2502810 Gpc yr - - 3 1.",
doi = "10.3847/2041-8213/ab75f5",
url = "http://dx.doi.org/10.3847/2041-8213/ab75f5",
issn = "0004-637X",
label = "lattes: 3325984959083987 14
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language = "pt",
targetfile = "abbot_190425.pdf",
urlaccessdate = "27 abr. 2024"
}