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Autores principales: Li, Hai-Jun, Chao, Wei, Zhou, Yu-Feng
Formato: Preprint
Publicado: 2023
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Acceso en línea:https://arxiv.org/abs/2312.05555
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author Li, Hai-Jun
Chao, Wei
Zhou, Yu-Feng
author_facet Li, Hai-Jun
Chao, Wei
Zhou, Yu-Feng
contents We present the limits on photon to axionlike particle (ALP) coupling from the 10-year period observations of the TeV BL Lacertae blazar 1ES 1215+303 (with redshift $z=0.130$). The contemporaneous gamma-ray spectra are measured by the collaborations Fermi-LAT and VERITAS with five flux phases from 2008 to 2017, including four low states and one flare. Using these flux phases, we show the spectral energy distributions (SEDs) under the null/ALP hypotheses and set the combined limit on ALP. The 95% $\rm C.L.$ combined limit set by 1ES 1215+303 with the 10-year gamma-ray data is roughly at the photon-ALP coupling constant $g_{aγ} \gtrsim 1.5\times 10^{-11} \rm \, GeV^{-1}$ for the ALP mass $5.0\times10^{-10} \, {\rm eV} \lesssim m_a \lesssim 1.0\times10^{-7} \, {\rm eV}$.
format Preprint
id arxiv_https___arxiv_org_abs_2312_05555
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Axion limits from the 10-year gamma-ray emission 1ES 1215+303
Li, Hai-Jun
Chao, Wei
Zhou, Yu-Feng
High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
We present the limits on photon to axionlike particle (ALP) coupling from the 10-year period observations of the TeV BL Lacertae blazar 1ES 1215+303 (with redshift $z=0.130$). The contemporaneous gamma-ray spectra are measured by the collaborations Fermi-LAT and VERITAS with five flux phases from 2008 to 2017, including four low states and one flare. Using these flux phases, we show the spectral energy distributions (SEDs) under the null/ALP hypotheses and set the combined limit on ALP. The 95% $\rm C.L.$ combined limit set by 1ES 1215+303 with the 10-year gamma-ray data is roughly at the photon-ALP coupling constant $g_{aγ} \gtrsim 1.5\times 10^{-11} \rm \, GeV^{-1}$ for the ALP mass $5.0\times10^{-10} \, {\rm eV} \lesssim m_a \lesssim 1.0\times10^{-7} \, {\rm eV}$.
title Axion limits from the 10-year gamma-ray emission 1ES 1215+303
topic High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2312.05555