2018/12/27 by A. B. Wahidin, A. Rahmansyah, A. Sulaksono
Physics and Astronomy · #Boson #Dark Matter and Cosmic Phenomena #Dark fluid #Dark matter #High-Energy Particle Collisions Research #Neutron star #Pulsars and Gravitational Waves Research #Scalar (mathematics) #Scalar boson #Scalar field dark matter #Stars #astro-ph.SR #gr-qc #hep-ph #nucl-th
paper · pdf · doi:10.1142/s0218271819500718
27 pages,11 figures, accepted for publication in IJMPD
openalex publication_date 2018/12/27 · arxiv created 2019/01/03 · openalex created_date 2019/01/11 · arxiv updated 2019/03/27 · openalex updated_date 2026/08/05
The role of scalar boson exchange as a mediator of the fermionic dark particle interaction and the mass of dark particle on the bulk properties of fermionic dark stars including their moment of inertia and tidal deformability are studied. We have found that the role of the attractive nature of the scalar boson exchange and the fermionic dark particle mass can control the stiffness of the fermionic dark star equation-of-state. By increasing the strength of scalar boson coupling, the fermionic dark star becomes more compact. As a consequence, if scalar boson exchange contribution is included the compactness of a dark star can exceed [Formula: see text] = 0.22. We also compare the fermionic dark stars moment of inertia and tidal deformability to those of neutron stars (with and without hyperons in neutron star core) predicted by relativistic mean field model. It is evident that the properties of both types of stars are quite different. We also have found that the universal I-Love relation in fermionic dark stars is not affected by scalar boson exchange contribution and the fermionic dark particle mass. Possible observations of fermionic dark stars are also discussed.