File:Strumia2022 Article DarkMatterInterpretationOfTheN.pdf

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Original file(1,239 × 1,752 pixels, file size: 449 KB, MIME type: application/pdf, 16 pages)

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Dark Matter interpretation of the neutron decay anomaly

Summary[edit]

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English: We add to the Standard Model a new fermion χ with minimal baryon number 1/3. Neutron decay n → χχχ into non-relativistic χ can account for the neutron decay anomaly, compatibly with bounds from neutron stars. χ can be Dark Matter, and its cosmological abundance can be generated by freeze-in dominated at T ∼ mn. The associated processes n → χχχγ, hydrogen decay H → χχχν(γ) and DM-induced neutron disappearance χ¯¯¯n → χχ(γ) have rates below experimental bounds and can be of interest for future experiments.
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https://link.springer.com/article/10.1007/JHEP02(2022)067

https://doi.org/10.1007/JHEP02(2022)067
Author Alessandro Strumia

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current10:40, 19 April 2022Thumbnail for version as of 10:40, 19 April 20221,239 × 1,752, 16 pages (449 KB)Pamputt (talk | contribs)Uploaded a work by Alessandro Strumia from https://link.springer.com/article/10.1007/JHEP02(2022)067 https://doi.org/10.1007/JHEP02(2022)067 with UploadWizard

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