作者
B Abbott, R Abbott, R Adhikari, A Ageev, B Allen, R Amin, SB Anderson, WG Anderson, M Araya, H Armandula, M Ashley, F Asiri, Peter Aufmuth, C Aulbert, Stanislav Babak, Ramachandran Balasubramanian, S Ballmer, BC Barish, C Barker, D Barker, M Barnes, B Barr, MA Barton, K Bayer, R Beausoleil, K Belczynski, R Bennett, Steven J Berukoff, J Betzwieser, B Bhawal, IA Bilenko, G Billingsley, E Black, K Blackburn, L Blackburn, B Bland, B Bochner, L Bogue, Rolf Bork, Sukanta Bose, Patrick R Brady, VB Braginsky, JE Brau, Duncan A Brown, A Bullington, Alexander Bunkowski, A Buonanno, R Burgess, D Busby, WE Butler, RL Byer, L Cadonati, G Cagnoli, JB Camp, CA Cantley, L Cardenas, K Carter, Morag M Casey, J Castiglione, A Chandler, J Chapsky, P Charlton, S Chatterji, Simon Chelkowski, Y Chen, V Chickarmane, D Chin, Nelson Christensen, D Churches, Thomas Cokelaer, C Colacino, R Coldwell, M Coles, D Cook, Thomas Corbitt, D Coyne, Jolien DE Creighton, Teviet D Creighton, DRM Crooks, P Csatorday, BJ Cusack, Curt Cutler, Erika D’Ambrosio, K Danzmann, E Daw, D DeBra, T Delker, V Dergachev, R DeSalvo, Sanjeev Dhurandhar, A Di Credico, M Díaz, H Ding, RWP Drever, RJ Dupuis, JA Edlund, P Ehrens, EJ Elliffe, T Etzel, M Evans, T Evans, Stephen Fairhurst, Carsten Fallnich, D Farnham, MM Fejer, T Findley, M Fine, Lee S Finn, KY Franzen, Andreas Freise, R Frey, P Fritschel, VV Frolov, M Fyffe, KS Ganezer, J Garofoli, JA Giaime, A Gillespie, Keisuke Goda, Gabriela Gonzalez, S Goßler, P Grandclément, A Grant, C Gray, AM Gretarsson, D Grimmett, H Grote, S Grunewald, Mathias Guenther, E Gustafson, R Gustafson, WO Hamilton, M Hammond, J Hanson, C Hardham, Jan Harms, G Harry, A Hartunian, J Heefner, Y Hefetz, G Heinzel, Ik Siong Heng, M Hennessy, N Hepler, A Heptonstall, Michèle Heurs, M Hewitson, S Hild, N Hindman, P Hoang
发表日期
2005/10/25
期刊
Physical Review D
卷号
72
期号
8
页码范围
082002
出版商
American Physical Society
简介
We use data from the second science run of the LIGO gravitational-wave detectors to search for the gravitational waves from primordial black hole binary coalescence with component masses in the range 0.2–1.0 M⊙. The analysis requires a signal to be found in the data from both LIGO observatories, according to a set of coincidence criteria. No inspiral signals were found. Assuming a spherical halo with core radius 5 kpc extending to 50 kpc containing nonspinning black holes with masses in the range 0.2–1.0 M⊙, we place an observational upper limit on the rate of primordial black hole coalescence of 63 per year per Milky Way halo (MWH) with 90% confidence.
引用总数
20052006200720082009201020112012201320142015201620172018201920202021202220232024816181716465724437616942
学术搜索中的文章