| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8186221 | Physics Letters B | 2018 | 5 Pages |
Abstract
We calculate the gravitational radiation background generated from boson star binaries formed in locally dense clusters with formation rate tracked by the regular star formation rate. We compute how the frequency window in gravitational waves is affected by the boson field mass and repulsive self-coupling, anticipating constraints from EPTA and LISA. We also comment on the possible detectability of these binaries.
Related Topics
Physical Sciences and Engineering
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Nuclear and High Energy Physics
Authors
Djuna Croon, Marcelo Gleiser, Sonali Mohapatra, Chen Sun,