Stability of mini-boson stars

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Abstract

A mini-boson star refers to a bound system of a complex scalar boson field with an astronomically large particle number N, but only a very small stellar radius ≅ Compton wavelength of a free boson, m-1. The star is held together by gravity. We prove that the lowest mass 1s solutions are stable against small oscillations, whereas other ns solutions (n ≥ 2) are not. Thus, the critical mass of mini-boson stars is the Kaup-Ruffini-Bonazzola limit M ≅ 0.633(Gm)-1where G is Newton's constant. © 1989.

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APA

Lee, T. D., & Pang, Y. (1989). Stability of mini-boson stars. Nuclear Physics, Section B, 315(2), 477–516. https://doi.org/10.1016/0550-3213(89)90365-9

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