A note on gravitational wave lensing

被引:16
作者
De Paolis, F
Ingrosso, G
Nucita, AA
Qadir, A
机构
[1] Univ Lecce, Dipartimento Fis, I-73100 Lecce, Italy
[2] Ist Nazl Fis Nucl, Sez Leece, I-73100 Lecce, Italy
[3] King Fahd Univ Petr & Minerals, Dept Math Sci, Dhahran 31261, Saudi Arabia
[4] Quaid I Azam Univ, Dept Math, Islamabad, Pakistan
关键词
gravitation; gravitational waves; gravitational lensing;
D O I
10.1051/0004-6361:20021258
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In a recent paper (Ruffa 1999) it was proposed that the massive black hole at the Galactic center may act as a gravitational lens focusing gravitational wave energy to the Earth. Considering the gravitational wave signal emitted by galactic spinning pulsars, an enhancement in the gravitational wave intensity by a factor of a few thousand is found. For galactic and extra-galactic sources the intensity enhancement can be as high as 4000 and 17 000, respectively. In this note we consider the probability of significant signal enhancement from galactic and extra-galactic pulsars by the proposed mechanism and find that it is actually negligible. The lensing effect due to a possible companion object (a star or the galactic center black hole) of the gravitational wave source is also investigated in the framework of the classical microlensing theory.
引用
收藏
页码:749 / 752
页数:4
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