scholarly journals Bosonic dark matter in neutron stars and its effect on gravitational wave signal

2022 ◽  
Vol 105 (2) ◽  
Author(s):  
Davood Rafiei Karkevandi ◽  
Soroush Shakeri ◽  
Violetta Sagun ◽  
Oleksii Ivanytskyi
Author(s):  
Rabinarayan Swain ◽  
Priyasmita Panda ◽  
Hena Priti Lima ◽  
Bijayalaxmi Kuanar ◽  
Biswajit Dalai

Detection of Gravitational waves opened a new path for cosmological study in a new approach. From the detection of gravitational waves signal by advanced LIGO, its research climbed the peak. After the collaboration of LIGO and Virgo, several observations get collected from different sources of binary systems like black holes, binary neutron stars even both binary black hole and neutron star. The rigorous detection of gravitational signals may provide an additional thrust in the study of complex binary systems, dark matter, dark energy, Hubble constant, etc. In this review paper, we went through multiple research manuscripts to analyze gravitational wave signals. Here we have reviewed the history and current situation of gravitational waves detection, and we explained the concept and process of detection. Also, we go through different parts of a detector and their working. Then multiple gravitational wave signals are focused, originated from various sources and then found correlation between them. From this, the contribution of gravitational waves in different fields like complex binary systems (black holes, neutron stars), dark matter, dark energy and Hubble Constant have been discussed in this manuscript.


2012 ◽  
Vol 8 (S290) ◽  
pp. 265-266
Author(s):  
Jinzhong Liu ◽  
Yu Zhang

AbstractAccording to the theoretical study, a deformation object (e.g., a spinning non-axisymmetric pulsar star) will radiate a gravitational wave (GW) signal during an accelaration motion process by LIGO science project. These types of disturbance sources with a large bump or dimple on the equator would survive and be identifiable as GW sources. In this work, we aim to provide a method for exploring GW radiation from isolated neutron stars (NSs) with deformation state using some observational results, which can be confirmed by the next LIGO project. Combination with the properties in observation results (e.g., PSR J1748-2446, PSR 1828-11 and Cygnus X-1), based on a binary population synthesis (BPS) approach we give a numerical GW radiation under the assumption that NS should have non-axisymmetric and give the results of energy spectrum. We find that the GW luminosity of LGW can be changed from about 1040 erg/s – 1055 erg/s.


2021 ◽  
Vol 32 ◽  
pp. 100796
Author(s):  
Raul Ciancarella ◽  
Francesco Pannarale ◽  
Andrea Addazi ◽  
Antonino Marcianò
Keyword(s):  

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