Acoustic modes of pulsating axion stars: Non-radial oscillations
arXiv:1904.07195 · doi:10.1142/S0218271819501116
Abstract
We compute the lowest frequency non-radial oscillation modes of dilute axion stars. The effective potential that enters into the Schr{ö}dinger-like equation, several associated eigenfunctions, and the large as well as the small frequency separations are shown as well.
arXiv comment15 pages, 5 figures, 1 table, accepted for publication in IJMPD. arXiv admin note: text overlap with arXiv:1904.07191
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