REVIEW 4 cited by
micrOMEGAs : a tool for dark matter studies
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
micrOMEGAs is a tool for cold dark matter (DM) studies in generic extensions of the standard model with a R-parity like discrete symmetry that guarantees the stability of the lightest odd particle. The code computes the DM relic density, the elastic scattering cross sections of DM on nuclei relevant for direct detection, and the spectra of positrons, anti-protons and photons originating from DM annihilation including porpagation of charged cosmic rays. The cross sections and decay properties of new particles relevant for collider studies are included as well as constraints from the flavour sector on the parameter space of supersymmetric models.
Forward citations
Cited by 4 Pith papers
-
Deciphering compressed electroweakino excesses with MadAnalysis 5
MadAnalysis 5 v1.11 adds validated recasting of two ATLAS compressed-electroweakino searches and shows that a proposed NMSSM scenario fits the soft-lepton and monojet excesses less well than simpler models.
-
A joint explanation for the soft lepton and monojet LHC excesses in the wino-bino model
A combined fit to four LHC Run 2 searches prefers a wino-bino supersymmetric spectrum with m(wino) ~ 320 GeV and mass splitting ~ 20 GeV, compatible with bino dark matter.
-
Symmetry-Protected Momentum Exchange between Dark Matter and Dark Energy
Symmetry-protected pure momentum exchange between inert-doublet dark matter and pNGB dark energy saturates σ8 suppression at ~3.6%, short of resolving the S8 tension.
-
Dark Matter signals in solar neutrinos fluxes as probe of non-linear symmetry breaking
Solar neutrino fluxes from dark matter annihilation differ by up to five to six orders of magnitude between the non-linear and linear Higgs portal models at high DM mass, which could discriminate the two frameworks.
Discussion (0). Continue with ORCID to comment.