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Main Authors: Song, Ningqiang, Su, Liangliang, Wu, Lei
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2402.15144
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author Song, Ningqiang
Su, Liangliang
Wu, Lei
author_facet Song, Ningqiang
Su, Liangliang
Wu, Lei
contents Neutron stars provide ideal astrophysical laboratories for probing new physics beyond the Standard Model. If axions exist, photons can develop linear polarization during photon-axion conversion in the magnetic field of a neutron star. We find that the plasma in the neutron star magnetosphere could dramatically enhance the polarization through the resonant conversion effect. With the polarization measurements from PSR B0656+14, 4U 0142+61, and the benchmark polarization measurement in the mid-infrared band, we demonstrate that optical and infrared polarization from neutron stars can provide strong constraints on the axion-photon coupling over a broad axion mass range $10^{-11}\lesssim m_a \lesssim 10^{-3}$ eV.
format Preprint
id arxiv_https___arxiv_org_abs_2402_15144
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Polarization Signals from Axion-Photon Resonant Conversion in Neutron Star Magnetosphere
Song, Ningqiang
Su, Liangliang
Wu, Lei
High Energy Physics - Phenomenology
Neutron stars provide ideal astrophysical laboratories for probing new physics beyond the Standard Model. If axions exist, photons can develop linear polarization during photon-axion conversion in the magnetic field of a neutron star. We find that the plasma in the neutron star magnetosphere could dramatically enhance the polarization through the resonant conversion effect. With the polarization measurements from PSR B0656+14, 4U 0142+61, and the benchmark polarization measurement in the mid-infrared band, we demonstrate that optical and infrared polarization from neutron stars can provide strong constraints on the axion-photon coupling over a broad axion mass range $10^{-11}\lesssim m_a \lesssim 10^{-3}$ eV.
title Polarization Signals from Axion-Photon Resonant Conversion in Neutron Star Magnetosphere
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2402.15144