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Boson star (BS) rotation is studied under Newtonian approximation. A Coulombian potential term is added as perturbation to the radial potential of the system without disturbing the angular momentum. The… Click to show full abstract
Boson star (BS) rotation is studied under Newtonian approximation. A Coulombian potential term is added as perturbation to the radial potential of the system without disturbing the angular momentum. The results of the stationary states of these ground state, first and second excited state are analyzed with the correction of Coulombian potential. It is found that the results with correction increased in the amplitude of oscillation of BS in comparison to potential without perturbation correction.
Keywords:
oscillation boson;
newtonian approximation;
boson star
Journal Title: Modern Physics Letters A
Year Published: 2017
Link to full text (if available)
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Journal Title: Modern Physics Letters A
Year Published: 2017
Link to full text (if available)
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recommendations!