Axion sourcing in dense stellar matter via CP-violating couplings

Fuente: arXiv
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Auteurs principaux: Anzuini, Filippo, Gómez-Bañón, Antonio, Pons, José A., Melatos, Andrew, Lasky, Paul D.
Format: Preprint
Publié: 2023
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author Anzuini, Filippo
Gómez-Bañón, Antonio
Pons, José A.
Melatos, Andrew
Lasky, Paul D.
author_facet Anzuini, Filippo
Gómez-Bañón, Antonio
Pons, José A.
Melatos, Andrew
Lasky, Paul D.
contents Compact objects such as neutron stars and white dwarfs can source axion-like particles and QCD axions due to CP-violating axion-fermion couplings. The magnitude of the axion field depends on the stellar density and on the strength of the axion-fermion couplings. We show that even CP-violating couplings one order of magnitude smaller than existing constraints source extended axion field configurations. For axion-like particles, the axion energy is comparable to the magnetic energy in neutron stars with inferred magnetic fields of the order of $10^{13}$ G, and exceeds by more than one order of magnitude the magnetic energy content of white dwarfs with inferred fields of the order of $10^{4}$ G. On the other hand, the energy stored in the QCD axion field is orders of magnitude lower due to the smallness of the predicted CP-violating couplings. It is shown that the sourced axion field can polarize the photons emitted from the stellar surface, and stimulate the production of photons with energies in the radio band.
format Preprint
id arxiv_https___arxiv_org_abs_2311_13776
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Axion sourcing in dense stellar matter via CP-violating couplings
Anzuini, Filippo
Gómez-Bañón, Antonio
Pons, José A.
Melatos, Andrew
Lasky, Paul D.
High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
Compact objects such as neutron stars and white dwarfs can source axion-like particles and QCD axions due to CP-violating axion-fermion couplings. The magnitude of the axion field depends on the stellar density and on the strength of the axion-fermion couplings. We show that even CP-violating couplings one order of magnitude smaller than existing constraints source extended axion field configurations. For axion-like particles, the axion energy is comparable to the magnetic energy in neutron stars with inferred magnetic fields of the order of $10^{13}$ G, and exceeds by more than one order of magnitude the magnetic energy content of white dwarfs with inferred fields of the order of $10^{4}$ G. On the other hand, the energy stored in the QCD axion field is orders of magnitude lower due to the smallness of the predicted CP-violating couplings. It is shown that the sourced axion field can polarize the photons emitted from the stellar surface, and stimulate the production of photons with energies in the radio band.
title Axion sourcing in dense stellar matter via CP-violating couplings
topic High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2311.13776