Bosonic and Fermionic love number of static acoustic black hole
arXiv:2512.23305 · doi:10.1103/35lw-pvfz
Abstract
We compute static () tilde Love numbers for scalar () and Dirac () perturbations of static acoustic black holes (ABHs) in (3+1) and (2+1) dimensions respectively. By imposing horizon regularity condition and matching to the large-radius expansion, we extract the ratio between decaying and growing modes. It turns out that in (3+1) dimensions the scalar Love number is generically nonzero for ABHs, while the Fermionic Love numbers follow a universal power-law form . In (2+1) dimensions the scalar field exhibits a strange logarithmic structure, causing the Bosonic Love number to vanish for even but remain nontrivial for odd ; In contrast, the Fermionic Love number in this case retains a simple power-law form and is generically nonzero. These results provide insights into tidal response in analogue gravity systems and highlight qualitative differences between integer- and half-integer-spin fields.
12 pages
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