[논문]Effects of waveform model systematics on the interpretation of GW150914

Abbott, B P; Abbott, R; Abbott, T D; Abernathy, M R; Acernese, F; Ackley, K; Adams, C; Adams, T; Addesso, P; Adhikari, R X; Adya, V B; Affeldt, C; Agathos, M; Agatsuma, K; Aggarwal, N; Aguiar, O D; Aiello, L; Ain, A; Ajith, P; Allen, B; Allocca, A; Altin, P A; Ananyeva, A; Anderson, S B; Anderson, W G; Appert, S; Arai, K; Araya, M C; Areeda, J S; Arnaud, N; Arun, K G; Ascenzi, S; Ashton, G; Ast, M; Aston, S M; Astone, P; Aufmuth, P; Aulbert, C; Avila-Alvarez, A; Babak, S; Bacon, P; Bader, M K M; Baker, P T; Baldaccini, F; Ballardin, G; Ballmer, S W; Barayoga, J C; Barclay, S E; Barish, B C; Barker, D; Barone, F; Barr, B; Barsotti, L; Barsuglia, M; Barta, D; Bartlett, J; Bartos, I; Bassiri, R; Basti, A; Batch, J C; Baune, C; Bavigadda, V; Bazzan, M; Beer, C; Bejger, M; Belahcene, I; Belgin, M; Bell, A S; Berger, B K; Bergmann, G; Berry, C P L; Bersanetti, D; Bertolini, A; Betzwieser, J; Bhagwat, S; Bhandare, R

doi:10.1088/1361-6382/aa6854

Effects of waveform model systematics on the interpretation of GW150914 원문보기

Classical and quantum gravity, v.34 no.10, 2017년, pp.104002 -

Abbott, B P (LIGO, California Institute of Technology, Pasadena, CA 91125, United States of America) , Abbott, R (LIGO, California Institute of Technology, Pasadena, CA 91125, United States of America) , Abbott, T D (Louisiana State University, Baton Rouge, LA 70803, United States of America) , Abernathy, M R (American University, Washington, DC 20016, United States of America) , Acernese, F (Università) , Ackley, K (di Salerno, Fisciano, I-84084 Salerno, Italy) , Adams, C (University of Florida, Gainesville, FL 32611, United States of America) , Adams, T (LIGO Livingston Observatory, Livingston, LA 70754, United States of America) , Addesso, P (Laboratoire d’Annecy-le-Vieux de Physique des Particules (LAPP), Université) , Adhikari, R X (Savoie Mont Blanc, CNRS) , Adya, V B (University of Sannio at Benevento, I-82100 Benevento, Italy) , Affeldt, C (LIGO, California Institute of Technology, Pasadena, CA 91125, United States of America) , Agathos, M (Albert-Einstein-Institut, Max-Planck-Institut fü) , Agatsuma, K (r Gravitationsphysik, D-30167 Hannover, Germany) , Aggarwal, N (Albert-Einstein-Institut, Max-Planck-Institut fü) , Aguiar, O D (r) , Aiello, L , Ain, A , Ajith, P , Allen, B , Allocca, A , Altin, P A , Ananyeva, A , Anderson, S B , Anderson, W G , Appert, S , Arai, K , Araya, M C , Areeda, J S , Arnaud, N , Arun, K G , Ascenzi, S , Ashton, G , Ast, M , Aston, S M , Astone, P , Aufmuth, P , Aulbert, C , Avila-Alvarez, A , Babak, S , Bacon, P , Bader, M K M , Baker, P T , Baldaccini, F , Ballardin, G , Ballmer, S W , Barayoga, J C , Barclay, S E , Barish, B C , Barker, D , Barone, F , Barr, B , Barsotti, L , Barsuglia, M , Barta, D , Bartlett, J , Bartos, I , Bassiri, R , Basti, A , Batch, J C , Baune, C , Bavigadda, V , Bazzan, M , Beer, C , Bejger, M , Belahcene, I , Belgin, M , Bell, A S , Berger, B K , Bergmann, G , Berry, C P L , Bersanetti, D , Bertolini, A , Betzwieser, J , Bhagwat, S , Bhandare, R

Abstract ▼ AI-Helper

Parameter estimates of GW150914 were obtained using Bayesian inference, based on three semi-analytic waveform models for binary black hole coalescences. These waveform models differ from each other in their treatment of black hole spins, and all three models make some simplifying assumptions, notably to neglect sub-dominant waveform harmonic modes and orbital eccentricity. Furthermore, while the models are calibrated to agree with waveforms obtained by full numerical solutions of Einstein’s equations, any such calibration is accurate only to some non-zero tolerance and is limited by the accuracy of the underlying phenomenology, availability, quality, and parameter-space coverage of numerical simulations. This paper complements the original analyses of GW150914 with an investigation of the effects of possible systematic errors in the waveform models on estimates of its source parameters. To test for systematic errors we repeat the original Bayesian analysis on mock signals from numerical simulations of a series of binary configurations with parameters similar to those found for GW150914. Overall, we find no evidence for a systematic bias relative to the statistical error of the original parameter recovery of GW150914 due to modeling approximations or modeling inaccuracies. However, parameter biases are found to occur for some configurations disfavored by the data of GW150914: for binaries inclined edge-on to the detector over a small range of choices of polarization angles, and also for eccentricities greater than ∼0.05. For signals with higher signal-to-noise ratio than GW150914, or in other regions of the binary parameter space (lower masses, larger mass ratios, or higher spins), we expect that systematic errors in current waveform models may impact gravitational-wave measurements, making more accurate models desirable for future observations.

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용어 설명: PCR은 세균 특이성이 있는 primer를 이용하여 적은 수의 세균이 있을지라도 쉽게 검출할 수 있는 유용한 방법이며, 이를 이용하여 구강 내 치면세균막이나 타액에서 직접 세균을 검출할 수 있게 되었다[8].

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Effects of waveform model systematics on the interpretation of GW150914 원문보기

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