Lightish but clumpy: scalar dark matter from inflationary fluctuations
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Publication:5023659
DOI10.1088/1475-7516/2018/10/022OpenAlexW3103994803MaRDI QIDQ5023659
Gonzalo Alonso-Álvarez, Joerg Jaeckel
Publication date: 24 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1807.09785
Related Items (13)
Dark photon dark matter from a rolling inflaton ⋮ Misalignment & Co.: (pseudo-)scalar and vector dark matter with curvature couplings ⋮ Impact of Higgs portal on gravity-mediated production of superheavy dark matter ⋮ Primordial dark matter from curvature induced symmetry breaking ⋮ Gravitational misalignment mechanism of Dark Matter production ⋮ Implications of time-dependent inflaton decay on reheating and dark matter production ⋮ Production of purely gravitational dark matter: the case of fermion and vector boson ⋮ Gravitational production of superheavy dark matter and associated cosmological signatures ⋮ Very light asymmetric dark matter ⋮ Gravitational waves from global cosmic strings in quintessential inflation ⋮ Despicable dark relics: generated by gravity with unconstrained masses ⋮ Vector dark matter production at the end of inflation ⋮ Hidden photon dark matter interacting via axion-like particles
Uses Software
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- Cosmological perturbations in coherent oscillating scalar field models
- Scale-invariant scalar field dark matter through the Higgs portal
- Production of purely gravitational dark matter
- Abelian discrete symmetries \(\mathbf{Z}_N\) and \(\mathbf{Z}_{n R}\) from string orbifolds
- Pure gravitational dark matter, its mass and signatures
- Indirect Detection of Dark Matter
- Dark matter from gravitational particle production at reheating
- Quantum Fields in Curved Space
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