6533b86efe1ef96bd12ccaf9
RESEARCH PRODUCT
Radio signatures from encounters between Neutron Stars and QCD-Axion Minihalos around Primordial Black Holes
Tsutomu T. YanagidaSami NurmiSami NurmiEnrico D. SchiappacasseEnrico D. Schiappacassesubject
Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and DetectorsMilky WayAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesPrimordial black holeAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyRadio telescopeHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsAxionPhysicsQuantum chromodynamicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxyHigh Energy Physics - PhenomenologyNeutron star13. Climate actionAstrophysics of Galaxies (astro-ph.GA)Astrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysicsdescription
Probing the QCD axion dark matter (DM) hypothesis is extremely challenging as the axion interacts very weakly with Standard Model particles. We propose a new avenue to test the QCD axion DM via transient radio signatures coming from encounters between neutron stars (NSs) and axion minihalos around primordial black holes (PBHs). We consider a general QCD axion scenario in which the PQ symmetry breaking occurs before (or during) inflation coexisting with a small fraction of DM in the form of PBHs. The PBHs will unavoidably acquire around them axion minihalos with the typical length scale of parsecs. The axion density in the minihalos may be much higher than the local DM density, and the presence of these compact objects in the Milky Way today provides a novel chance for testing the axion DM hypothesis. We study the evolution of the minihalo mass distribution in the Galaxy accounting for tidal forces and estimate the encounter rate between NSs and the dressed PBHs. We find that the encounters give rise to transient line-like emission of radio frequency photons produced by the resonant axion-photon conversion in the NS magnetosphere and the characteristic signal could be detectable with the sensitivity of current and prospective radio telescopes. It would be important to investigate in detail search strategies for such signals which would provide a novel pathway for QCD axion detection.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2021-02-10 |