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An Introduction to Particle Dark Matter

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arxiv 1910.05610 v1 pith:PL2H3MEV submitted 2019-10-12 hep-ph astro-ph.GAhep-th

Stefano Profumo , Leonardo Giani , Oliver F. Piattella This is my paper · ORCID
classification hep-phastro-ph.GAhep-th
keywords darkmatterparticlecandidatesearlyfeaturesformationimplications
verification ladder T0 review T1 audit T2 compute T3 formal
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We review the features of Dark Matter as a particle, presenting some old and new instructive models, and looking for their physical implications in the early universe and in the process of structure formation. We also present a schematic of Dark Matter searches and introduce the most promising candidates to the role of Dark Matter particle.

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Cited by 5 Pith papers

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

  1. Detecting the Coupling of Axion Dark Matter to Neutron Spins at Spallation Sources via Rabi Oscillation

    hep-ph 2024-12 conditional novelty 6.0 of 10

    A neutron-beam Rabi oscillation setup with double Stern-Gerlach spin selection could reach fa/Cn around 1.3e7 GeV and probe axion dark matter masses from 3e-13 to 1e-10 eV.

  2. Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology

    astro-ph.CO 2026-08 reject novelty 5.0 of 10

    Using BBN and WIMP relic density, the authors constrain the Yukawa gravity coupling α to about -0.017 to 0.018, with the lithium discrepancy still unexplained.

  3. Learning from galactic rotation curves: a neural network approach

    astro-ph.CO 2024-12 conditional novelty 5.0 of 10

    Neural networks trained on simulated rotation curves can infer ultra-light dark matter and baryonic parameters from SPARC dwarf galaxies, with uncertainties comparable to MCMC.

  4. Revisiting the limits on dark matter annihilation cross-section and decay lifetime in light of electron and positron fluxes

    hep-ph 2025-10 conditional novelty 4.0 of 10

    Using CALET, AMS-02, DAMPE, HESS, HAWC, GRAPES-3 and CASA-MIA data, this paper derives 95% C.L. constraints on dark matter annihilation and decay up to 10^16 GeV.

  5. Dark matter from axion and small neutrino mass

    hep-ph 2024-12 conditional novelty 4.0 of 10

    A KSVZ-like model with a fermion dark matter candidate produced by UV freeze-in through the axion portal is shown to have viable parameter space at TeV mass and axion decay constant near 10^10 to 10^11 GeV.

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