Superfluid dark stars

被引：0
|
作者：
Cipriani, Lorenzo [1 ,2 ]
Mannarelli, Massimo [2 ]
Nesti, Fabrizio [1 ,2 ]
Trabucco, Silvia [2 ,3 ]
机构：
[1] Univ Aquila, Dipartimento Sci Fis & Chim, Via Vetoio, I-67100 Laquila, Italy
[2] INFN Lab Nazl Gran Sasso, Via G Acitelli 22, I-67100 Assergi, AQ, Italy
[3] Gran Sasso Sci Inst, Viale Francesco Crispi 7, I-67100 Laquila, Italy
来源：
PHYSICAL REVIEW D | 2024年 / 110卷 / 02期
关键词：
EQUATION-OF-STATE; DENSE MATTER; NEUTRON-STARS; HYDRODYNAMICS; PARTICLES; SKYRME;
D O I：
10.1103/PhysRevD.110.L021301
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present a superfluid dark star model consisting of relativistic dark bosons with two-body selfinteraction. The obtained masses, radii, and tidal deformability depend in a simple way on the boson mass and interaction strength. We report first results on binary mergers: the distinctive amplitude and frequency of the emitted gravitational waves are well within reach of terrestrial interferometers.
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页数：8
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