Prospects for the observation of continuous gravitational waves from deformed fast-spinning white dwarfs

被引：2

作者：

Sousa, Manoel F. ^{[1
,2
]}

Otoniel, Edson ^{[3
]}

Coelho, Jaziel G. ^{[2
,4
,5
]}

de Araujo, Jose C. N. ^{[2
]}

机构：

[1] Univ Tecnol Fed Parana, Programa Posgrad Fis & Astron, Ave Sete Setembro 3165, BR-80230901 Curitiba, PR, Brazil

[2] Inst Nacl Pesquisas Espaciais, Div Astrofis, Av Astronautas 1758, BR-12227010 Sao Jose Dos Campos, SP, Brazil

[3] Univ Fed Cariri, Inst Formacao Educadores, R Olegario Emidio Araujo S-N Aldeota, BR-63260000 Brejo Santo, CE, Brazil

[4] Univ Fed Espirito Santo, Nucleo Astrofis & Cosmol Cosmo Ufes, BR-29075910 Vitoria, ES, Brazil

[5] Univ Fed Espirito Santo, Dept Fis, BR-29075910 Vitoria, ES, Brazil

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2024年 / 531卷 / 01期

基金：

巴西圣保罗研究基金会;

关键词：

gravitational waves; stars: magnetic field; white dwarfs; ROTATING RELATIVISTIC STARS; X-RAY PULSATIONS; NEUTRON-STARS; PULSARS; DISCOVERY; MERGER; MASS; INSTABILITY; MAGNETARS; EVOLUTION;

D O I：

10.1093/mnras/stae1232

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

There has been a growing interest within the astrophysics community in highly magnetized and fast-spinning white dwarfs (WDs), commonly referred to as HMWDs. WDs with these characteristics are quite uncommon and possess magnetic fields >= 10(6) G, along with short rotation periods ranging from seconds to just a few minutes. Based on our previous work, we analyse the emission of Gravitational Waves (GWs) in HMWDs through two mechanisms: matter accretion and magnetic deformation, which arise due to the asymmetry surrounding the star's rotational axis. Here, we perform a thorough self-consistent analysis, accounting for rotation and employing a realistic equation of state to investigate the stability of stars. Our investigation focuses on the emission of gravitational radiation from six rapidly spinning WDs: five of them are situated within binary systems, while one is an AXP, proposed as a magnetic accreting WD. Furthermore, we apply the matter accretion mechanism alongside the magnetic deformation mechanism to assess the influence of one process on the other. Our discoveries indicate that these WDs could potentially act as GW sources for BBO and DECIGO, depending on specific parameters, such as their mass, the angle (alpha) between the magnetic and rotational axes, and the accumulated mass (delta m) at their magnetic poles, which is influenced by the effect of matter accretion. However, detecting this particular class of stars using the LISA and TianQin space detectors seems unlikely due to the challenging combination of parameters such as a large delta m, a large alpha angle and a small WD mass value.

引用

页码：1496 / 1505

页数：10

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