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Two Component Feebly Interacting Massive Particle (FIMP) Dark Matter

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arxiv 1709.05955 v2 pith:6FLF46ZI submitted 2017-09-18 hep-ph

Two Component Feebly Interacting Massive Particle (FIMP) Dark Matter

classification hep-ph
keywords darkmatterfimpparticlemodelscalarcandidatecomponent
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We explore the idea of an alternative candidate for particle dark matter namely Feebly Interacting Massive Particle (FIMP) in the framework of a two component singlet scalar model. Singlet scalar dark matter has already been demonstrated to be a viable candidate for WIMP (Weakly Interacting Massive Particle) dark matter in literature. In the FIMP scenario, dark matter particles are slowly produced via "thermal frreze-in" mechanism in the early Universe and are never abundant enough to reach thermal equilibrium or to undergo pair annihilation inside the Universe's plasma due to their extremely small couplings. We demonstrate that for smaller couplings too, required for freeze-in process, a two component scalar dark matter model considered here could well be a viable candidate for FIMP. In this scenario, the Standard Model of particle physics is extended by two gauge singlet real scalars whose stability is protected by an unbroken $Z_{2}\times {Z'}_{2}$ symmetry and they are assumed to acquire no VEV after Spontaneous Symmetry Breaking. We explore the viable mass regions in the present two scalar DM model that is in accordance with the FIMP scenario. We also explore the upper limits of masses of the two components from the consideration of their self interactions.

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Cited by 1 Pith paper

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

  1. FIMPs in a two-component dark matter model with $Z_2 \times Z_4$ symmetry

    hep-ph 2026-02 conditional novelty 5.0

    In a Z2×Z4 two-component FIMP model, the scalar coupling λds can be as small as ~10^-20 to 10^-24 while h2-mediated processes still control scalar dark matter production.