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Planck Mass Charged Gravitino Dark Matter
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Planck Mass Charged Gravitino Dark Matter
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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.
Forward citations
Cited by 3 Pith papers
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Solving Cosmological Puzzles using Finite Temperature $\nu$SMEFT
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...
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Planck mass gravitinos in Einstein-Maxwell backgrounds
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.
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Planck mass gravitinos in Einstein-Maxwell backgrounds
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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