Gravitational wave bursts induced by r-mode spin-down of hybrid stars

被引:3
作者
Drago, A [1 ]
Pagliara, G
Berezhiani, Z
机构
[1] Univ Ferrara, Dipartimento Fis, I-44100 Ferrara, Italy
[2] Ist Nazl Fis Nucl, Sez Ferrara, I-44100 Ferrara, Italy
[3] Univ Aquila, Dipartimento Fis, I-67010 Laquila, Italy
[4] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67010 Laquila, Italy
来源
ASTRONOMY & ASTROPHYSICS | 2006年 / 445卷 / 03期
关键词
gravitational waves; equation of state; stars : neutron; stars : evolution; stars : rotation; stars : interiors;
D O I
10.1051/0004-6361:20053276
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that sudden variations in the composition and structure of a hybrid star can be triggered by its rapid spin-down, induced by r-mode instabilities. The discontinuity of this process is due to the surface tension between hadronic and quark matter and in particular to the over-pressure needed to nucleate new structures of quark matter in the mixed phase. The consequent mini-collapses in the star can produce highly energetic gravitational wave bursts. The possible connection between the predictions of this model and the burst signal found by EXPLORER and NAUTILUS detectors during 2001 is also investigated.
引用
收藏
页码:1053 / 1060
页数:8
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