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Planck Mass Charged Gravitino Dark Matter

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arxiv 1809.01441 v3 pith:HOT3UD6A submitted 2018-09-05 hep-ph astro-ph.CO

Planck Mass Charged Gravitino Dark Matter

classification hep-ph astro-ph.CO
keywords chargeddarkmattercandidatesdetectdiscussearlierexplain
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Following up on our earlier work predicting fractionally charged supermassive gravitinos, we explain their potential relevance as novel candidates for Dark Matter and discuss possible signatures and ways to detect them.

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Cited by 3 Pith papers

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

  1. Solving Cosmological Puzzles using Finite Temperature $\nu$SMEFT

    hep-ph 2026-04 unverdicted novelty 5.0

    A minimal extension of the Standard Model with three heavy Majorana neutrinos simultaneously realizes fermionic dark matter, a strong first-order electroweak phase transition, and low-scale resonant leptogenesis consi...

  2. Planck mass gravitinos in Einstein-Maxwell backgrounds

    hep-th 2026-06 unverdicted novelty 4.0

    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.

  3. Planck mass gravitinos in Einstein-Maxwell backgrounds

    hep-th 2026-06 conditional novelty 4.0

    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.