Notice
This is not the latest version of this item. The latest version can be found at:https://dspace.mit.edu/handle/1721.1/133564.2
Optically targeted search for gravitational waves emitted by core-collapse supernovae during the first and second observing runs of advanced LIGO and advanced Virgo
| dc.date.accessioned | 2021-10-27T19:53:33Z | |
| dc.date.available | 2021-10-27T19:53:33Z | |
| dc.date.issued | 2020 | |
| dc.identifier.uri | https://hdl.handle.net/1721.1/133564 | |
| dc.description.abstract | © 2020 American Physical Society. We present the results from a search for gravitational-wave transients associated with core-collapse supernovae observed within a source distance of approximately 20 Mpc during the first and second observing runs of Advanced LIGO and Advanced Virgo. No significant gravitational-wave candidate was detected. We report the detection efficiencies as a function of the distance for waveforms derived from multidimensional numerical simulations and phenomenological extreme emission models. The sources with neutrino-driven explosions are detectable at the distances approaching 5 kpc, and for magnetorotationally driven explosions the distances are up to 54 kpc. However, waveforms for extreme emission models are detectable up to 28 Mpc. For the first time, the gravitational-wave data enabled us to exclude part of the parameter spaces of two extreme emission models with confidence up to 83%, limited by coincident data coverage. Besides, using ad hoc harmonic signals windowed with Gaussian envelopes, we constrained the gravitational-wave energy emitted during core collapse at the levels of 4.27×10-4 M·c2 and 1.28×10-1 M·c2 for emissions at 235 and 1304 Hz, respectively. These constraints are 2 orders of magnitude more stringent than previously derived in the corresponding analysis using initial LIGO, initial Virgo, and GEO 600 data. | |
| dc.language.iso | en | |
| dc.publisher | American Physical Society (APS) | |
| dc.relation.isversionof | 10.1103/PHYSREVD.101.084002 | |
| dc.rights | Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. | |
| dc.source | APS | |
| dc.title | Optically targeted search for gravitational waves emitted by core-collapse supernovae during the first and second observing runs of advanced LIGO and advanced Virgo | |
| dc.type | Article | |
| dc.relation.journal | Physical Review D | |
| dc.eprint.version | Final published version | |
| dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
| eprint.status | http://purl.org/eprint/status/PeerReviewed | |
| dc.date.updated | 2021-07-09T14:42:14Z | |
| dspace.orderedauthors | Abbott, BP; Abbott, R; Abbott, TD; Abraham, S; Acernese, F; Ackley, K; Adams, C; Adya, VB; Affeldt, C; Agathos, M; Agatsuma, K; Aggarwal, N; Aguiar, OD; Aiello, L; Ain, A; Ajith, P; Allen, G; Allocca, A; Aloy, MA; Altin, PA; Amato, A; Anand, S; Ananyeva, A; Anderson, SB; Anderson, WG; Angelova, SV; Antier, S; Appert, S; Arai, K; Araya, MC; Areeda, JS; Arène, M; Arnaud, N; Aronson, SM; Ascenzi, S; Ashton, G; Aston, SM; Astone, P; Aubin, F; Aufmuth, P; AultONeal, K; Austin, C; Avendano, V; Avila-Alvarez, A; Babak, S; Bacon, P; Badaracco, F; Bader, MKM; Bae, S; Baird, J; Baker, PT; Baldaccini, F; Ballardin, G; Ballmer, SW; Bals, A; Banagiri, S; Barayoga, JC; Barbieri, C; Barclay, SE; Barish, BC; 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, JC; Bazzan, M; Bécsy, B; Bejger, M; Belahcene, I; Bell, AS; Beniwal, D; Benjamin, MG; Bergmann, G; Bernuzzi, S; Berry, CPL; Bersanetti, D; Bertolini, A; Betzwieser, J; Bhandare, R; Bidler, J; Biggs, E; Bilenko, IA; Bilgili, SA; Billingsley, G; Birney, R; Birnholtz, O; Biscans, S; Bischi, M; Biscoveanu, S; Bisht, A; Bitossi, M; Bizouard, MA; Blackburn, JK; Blackman, J; Blair, CD; Blair, DG; Blair, RM; Bloemen, S; Bobba, F; Bode, N; Boer, M; Boetzel, Y; Bogaert, G; Bondu, F; Bonnand, R; Booker, P; Boom, BA; Bork, R; Boschi, V; Bose, S; Bossilkov, V; Bosveld, J; Bouffanais, Y; Bozzi, A; Bradaschia, C; Brady, PR; Bramley, A; Branchesi, M; Brau, JE; Breschi, M; Briant, T; Briggs, JH; Brighenti, F; Brillet, A; Brinkmann, M; Brockill, P; Brooks, AF; Brooks, J; Brown, DD; Brunett, S; Buikema, A; Bulik, T; Bulten, HJ; Buonanno, A; Buskulic, D; Buy, C; Byer, RL; Cabero, M; Cadonati, L; Cagnoli, G; Cahillane, C; Bustillo, JC; Callister, TA; Calloni, E; Camp, JB; Campbell, WA; Canepa, M; Cannon, KC; Cao, H; Cao, J; Carapella, G; Carbognani, F; Caride, S; Carney, MF; Carullo, G; Diaz, JC; Casentini, C; Caudill, S; Cavaglià, M; 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| dspace.date.submission | 2021-07-09T14:42:15Z | |
| mit.journal.volume | 101 | |
| mit.journal.issue | 8 | |
| mit.license | PUBLISHER_POLICY | |
| mit.metadata.status | Authority Work and Publication Information Needed |
