pith. machine review for the scientific record. sign in

arxiv: hep-ph/0612275 · v2 · submitted 2006-12-21 · ✦ hep-ph · astro-ph

Recognition: unknown

The Inert Doublet Model: an Archetype for Dark Matter

Authors on Pith no claims yet
classification ✦ hep-ph astro-ph
keywords modeldarkmatterarchetypedoubletinertabundanceanalysis
0
0 comments X
read the original abstract

The Inert Doublet Model (IDM), a two Higgs extension of the Standard Model with an unbroken $Z_2$ symmetry, is a simple and yet rich model of dark matter. We present a systematic analysis of the dark matter abundance and investigate the potentialities for direct and gamma indirect detection. We show that the model should be within the range of future experiments, like GLAST and ZEPLIN. The lightest stable scalar in the IDM is a perfect example, or archetype of a weakly interacting massive particle.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 3 Pith papers

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

  1. Search for pair production of additional neutral scalars within the Inert Doublet Model in a final state with two electrons or two muons in proton-proton collisions at $\sqrt{s}$ = 13 TeV and 13.6 TeV

    hep-ex 2026-05 accept novelty 5.0

    No significant excess found; new exclusion limits reach m_H = 108 GeV for m_H - m_A = 78 GeV in the Inert Doublet Model.

  2. Probing the Inert Doublet Dark Matter with Stellar-Mass Black Hole Mini-Spikes

    hep-ph 2026-05 unverdicted novelty 5.0

    Fermi LAT data on mini-spikes around stellar-mass black holes rules out substantial regions of Inert Doublet Model dark matter parameter space, especially at multi-TeV masses.

  3. LHC Mono-$W/Z$ Signatures as a Probe for Dark Matter Explanations of Astrophysical Excesses

    hep-ph 2026-05 unverdicted novelty 5.0

    LHC mono-W/Z searches with a new channel-separation method can exclude large ranges of neutral and charged mass splittings in the 70-75 GeV IDM dark matter scenario that fits astrophysical excesses.