2014/12/02 by S. Latifah, Siti Latifah, A. Sulaksono +1 · 1 citation
Physics and Astronomy · #Astrophysics #Boson #Cosmology and Gravitation Theories #Particle physics #Physics #Pulsars and Gravitational Waves Research #Quantum Chromodynamics and Particle Interactions #Star (game theory) #astro-ph.SR #hep-ph #nucl-th
paper · pdf · doi:10.1103/physrevd.90.127501
published as Phys. Rev. D 90, 127501 (2014) · 5 pages, 5 figures
openalex publication_date 2014/12/02 · arxiv created 2014/12/04 · arxiv updated 2014/12/24 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
By using a simple thermodynamical method, we confirm the finding of Chavanis and Harko that stable Bose-Einstein condensate stars can form. However, by using a thermodynamically consistent boson equation of state, we obtain a less massive Bose-Einstein condensate star compared to the one predicted by Chavanis and Harko. We also obtain that the maximum mass of a boson star is insensitive to the change of matter temperature. However, the mass of a boson star with relatively large radius depends significantly on the temperature of the boson matter.