2022
DOI: 10.1103/physrevd.105.035022
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Muonic boson limits: Supernova redux

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Cited by 107 publications
(119 citation statements)
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“…A precise evaluation in a SN core is difficult because electrons are relativistic and degenerate, however implying that their contribution both as scattering targets and for screening is small. We follow our earlier discussion [7] and neglect electrons, so for screening we use the Debye-Hückel scale of the quasi-static ions…”
Section: A Primakoff Processmentioning
confidence: 99%
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“…A precise evaluation in a SN core is difficult because electrons are relativistic and degenerate, however implying that their contribution both as scattering targets and for screening is small. We follow our earlier discussion [7] and neglect electrons, so for screening we use the Debye-Hückel scale of the quasi-static ions…”
Section: A Primakoff Processmentioning
confidence: 99%
“…While in a SN core, the charged particles are typically protons, in some regions small nuclear clusters dominate instead. Following our earlier discussion [7], we use Ŷ = 1 − Y n for estimating the Primakoff production and absorption rate in a given SN model. Photons in the medium suffer nontrivial dispersion that is dominated by the relativistic electron plasma frequency ω 2 p = (4α/3π)(µ 2 e + π 2 T 2 /3), where µ e is the electron chemical potential.…”
Section: A Primakoff Processmentioning
confidence: 99%
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