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Title: Diluted axion star collisions with neutron stars

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1];  [2];  [3]
  1. University of Wisconsin, Madison, WI (United States); Univ. of Wisconsin, Madison, WI (United States)
  2. Carnegie Observatories, Pasadena, CA (United States)
  3. Harvard University, Cambridge, MA (United States)

Diluted axion star, a self-gravitating object with the quantum pressure balancing gravity, has been predicted in many models with a QCD axion or axion-like particle. It can be formed in the early universe and composes a sizable fraction of dark matter. One could detect the transient radio signals when it passes by a magnetar with the axion particle converted into photon in the magnetic field. Using both numerical and semi-analytic approaches, we simulate the axion star's dynamic evolution and estimate the fraction of axion particles that can have a resonance conversion during such a collision event. We have found that both self-gravity and quantum pressure are not important after the diluted axion star enters the Roche radius. A free-fall approximate can capture individual particle trajectories very well. Finally, with some optimistic cosmological and astrophysical assumptions, the QCD axion parameter space can be probed from detecting such a collision event by radio telescopes.

Research Organization:
University of Wisconsin, Madison, WI (United States)
Sponsoring Organization:
USDOE Office of Science (SC); National Aeronautics and Space Administration (NASA); Japan Society for the Promotion of Science (JSPS)
Grant/Contract Number:
SC0017647
OSTI ID:
1979352
Journal Information:
Journal of Cosmology and Astroparticle Physics, Journal Name: Journal of Cosmology and Astroparticle Physics Journal Issue: 01 Vol. 2022; ISSN 1475-7516
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English

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