您的位置:首页>分类数据>详情
Observational limit on gravitational waves from binary neutron stars in the Galaxy
所属领域: 空间引力波探测领域
资源类型: 引力波探测 / 双星绕转
文献作者: Allen, B; Blackburn, JK; Brady, PR; Creighton, JDE; Creighton, T; Droz, S; Gillespie, AD; Hughes, SA; Kawamura, S; Lyons, TT; Mason, JE; Owen, BJ; Raab, FJ; Regehr, MW; Sathyaprakash, BS; Savage, RL; Whitcomb, S; Wiseman, AG
文献发表年份: 1999
文献期刊: PHYSICAL REVIEW LETTERS
文献摘要:Using optimal matched filtering, we search 25 hours of data from the LIGO 40-m prototype laser interferometric gravitational-wave detector for gravitational-wave chirps emitted by coalescing binary systems within our Galaxy. This is the first test of this filtering technique on real interferometric data. An upper limit on the rate R of neutron star binary inspirals in our Galaxy is obtained: with 90% confidence, R < 0.5 h(-1). Similar experiments with LIGO interferometers will provide constraints on the population of tight binary neutron star systems in the Universe.
文献类型: Article
文献语种: English
关键词: COMPACT BINARIES; INTERFEROMETER; PARAMETERS; DETECTORS; SEARCH; LIGO
文献作者地址: Univ Wisconsin, Dept Phys, Milwaukee, WI 53201 USA; CALTECH, LIGO Project, Pasadena, CA 91125 USA; Univ Calif Santa Barbara, Inst Theoret Phys, Santa Barbara, CA 93106 USA; Univ Guelph, Dept Phys, Guelph, ON N1G 2W1, Canada; UWCC, Dept Phys & Astron, Cardiff CF2 3YB, S Glam, Wales

版权所有@2017中国科学院文献情报中心

制作维护:中国科学院文献情报中心信息系统部地址:北京中关村北四环西路33号邮政编号:100190