Vector gauge boson radiation from compact binary systems in a gauged $L_\mu-L_\tau$ scenario
Tanmay Kumar Poddar, Subhendra Mohanty, Soumya Jana

TL;DR
This paper investigates how massive vector gauge boson radiation, specifically in a gauged $L__$ scenario, affects the orbital decay of compact binary systems, providing new constraints on the gauge coupling and boson mass.
Contribution
It derives the energy loss due to $L__$ gauge boson radiation from binary systems and constrains the gauge coupling for ultra-light vector bosons based on orbital decay data.
Findings
Constraints on gauge coupling: $g<10^{-20}$ for $M_{Z'}<10^{-19}$ eV.
Derived energy loss formulas for massive vector boson radiation.
Excluded parameter space for massive vector Proca fields coupling to muons.
Abstract
The orbital period of a compact binary system decays mainly due to quadrupole gravitational radiation, which agrees with the observation to within one percent. Other types of radiation such as ultralight scalar or pseudoscalar radiation, massive vector boson radiation also contribute to the decay of orbital period as long as the mass of the emitted particle is less than the orbital frequency of the compact binary system. We obtain an expression of the energy loss due to the radiation of massive vector field from the neutron star-neutron star and neutron star-white dwarf binaries. Due to large chemical potential of the degenerate electrons, neutron stars have large muon charge. We derive the energy loss due to gauge boson radiation from the binaries. For the radiation of vector boson, the mass is restricted by are the orbital…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
