Axion limits from the 10-year gamma-ray emission 1ES 1215+303

Li, Hai-Jun; Chao, Wei; Zhou, Yu-Feng

doi:10.1016/j.physletb.2024.138531

Physics Letters B

2024

DOI: 10.1016/j.physletb.2024.138531

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Axion limits from the 10-year gamma-ray emission 1ES 1215+303

Hai-Jun Li,

Wei Chao,

Yu-Feng Zhou

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Cited by 2 publications

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Upper limit on the axion-photon coupling from Markarian 421

Li,

Chao,

Zhou

2024

Physics Letters B

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Upper limit on the axion-photon coupling from Markarian 421

Li,

Chao,

Zhou

2024

Physics Letters B

View full text Add to dashboard Cite

Detecting ultralight dark matter gravitationally with laser interferometers in space

Yu,

Cao,

Tang

et al. 2024

Phys. Rev. D

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Ultralight dark matter (ULDM) is one of the leading well-motivated dark matter candidates, predicted in many theories beyond the standard model of particle physics and cosmology. There has been increasing interest in searching for ULDM in physical and astronomical experiments, mostly assuming there are additional interactions other than gravity between ULDM and normal matter. Here we demonstrate that even if ULDM has only gravitational interaction, it shall induce gravitational perturbations in solar system that may be large enough to cause detectable signals in future gravitational-wave (GW) laser interferometers in space. We investigate the sensitivities of Michelson time-delay interferometer to ULDM of various spins, and show vector ULDM with mass m≲10−18 eV can be probed by space-based GW detectors aiming at μHz frequencies. Our findings exhibit that GW detectors may directly probe ULDM in some mass ranges that otherwise are challenging to examine. Published by the American Physical Society 2024

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Axion limits from the 10-year gamma-ray emission 1ES 1215+303

Cited by 2 publications

References 55 publications

Upper limit on the axion-photon coupling from Markarian 421

Upper limit on the axion-photon coupling from Markarian 421

Detecting ultralight dark matter gravitationally with laser interferometers in space

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