|
學年
|
111 |
|
學期
|
1 |
|
出版(發表)日期
|
2022-11-28 |
|
作品名稱
|
All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data |
|
作品名稱(其他語言)
|
使用先進 LIGO 與先進 Virgo O3 數據對孤立中子星進行全天候連續重力波搜尋 |
|
著者
|
LIGO Scientific Collaboration, Virgo Collaboration, and KAGRA Collaboration |
|
單位
|
|
|
出版者
|
|
|
著錄名稱、卷期、頁數
|
Physical Review D 106(10), 102008 |
|
摘要
|
We present results of an all-sky search for continuous gravitational waves which can be produced by spinning neutron stars with an asymmetry around their rotation axis, using data from the third observing run of the Advanced LIGO and Advanced Virgo detectors. Four different analysis methods are used to search in a gravitational-wave frequency band from 10 to 2048 Hz and a first frequency derivative from −10−8 to 10−9 Hz/s. No statistically significant periodic gravitational-wave signal is observed by any of the four searches. As a result, upper limits on the gravitational-wave strain amplitude ℎ0 are calculated. The best upper limits are obtained in the frequency range of 100 to 200 Hz and they are ∼1.1 ×10−25 at 95% confidence level. The minimum upper limit of 1.10 ×10−25 is achieved at a frequency 111.5 Hz. We also place constraints on the rates and abundances of nearby planetary- and asteroid-mass primordial black holes that could give rise to continuous gravitational-wave signals. |
|
關鍵字
|
|
|
語言
|
en |
|
ISSN
|
2470-0029; 2470-0010 |
|
期刊性質
|
國外 |
|
收錄於
|
SCI
|
|
產學合作
|
|
|
通訊作者
|
|
|
審稿制度
|
否 |
|
國別
|
USA |
|
公開徵稿
|
|
|
出版型式
|
,電子版,紙本 |