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Millicharge or Decay: A Critical Take on Minimal Dark Matter

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arxiv 1512.05353 v3 pith:TKFYTJHD submitted 2015-12-16 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords candidatesdarkmatterdecayframeworkminimalviableabandon
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Minimal Dark Matter (MDM) is a theoretical framework highly appreciated for its minimality and yet its predictivity. Of the two only viable candidates singled out in the original analysis, the scalar eptaplet has been found to decay too quickly to be around today, while the fermionic quintuplet is now being probed by indirect Dark Matter (DM) searches. It is therefore timely to critically review the MDM paradigm, possibly pointing out generalizations of this framework. We propose and explore two distinct directions. One is to abandon the assumption of DM electric neutrality in favor of absolutely stable, millicharged DM candidates which are part of $SU(2)_{\text{L}}$ multiplets with integer isospin. Another possibility is to lower the cutoff of the model, which was originally fixed at the Planck scale, to allow for DM decays. We find new viable MDM candidates and study their phenomenology in detail.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

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    Fermi-LAT data exclude the lower end of the Minimal Dark Matter 5-plet thermal mass window, while about 600 hours of CTAO observations of Ursa Major II could probe the central mass.

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    Consistency of minimally coupled Rarita-Schwinger fields in Einstein-Maxwell backgrounds requires a mass lower bound set by charge and cosmological constant, forcing Planck-scale masses for charged gravitinos.

  4. Planck mass gravitinos in Einstein-Maxwell backgrounds

    hep-th 2026-06 conditional novelty 4.0 of 10

    A charged massive spin-3/2 field in an Einstein-Maxwell background propagates consistently only when m^2 > 2q^2/3κ^2 − Λ/3, a bound rederived here and used to argue for Planck-scale charged gravitino dark matter.

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