0000000000275092

AUTHOR

ÓScar Zapata

showing 3 related works from this author

Gravitino dark matter and neutrino masses with bilinear R-parity violation

2011

Bilinear R-parity violation provides an attractive origin for neutrino masses and mixings. In such schemes the gravitino is a viable decaying dark matter particle whose R-parity violating decays lead to monochromatic photons with rates accessible to astrophysical observations. We determine the parameter region allowed by gamma-ray line searches, dark matter relic abundance and neutrino oscillation data, obtaining a limit on the gravitino mass $m_{\tilde G} \lsim$ 1-10 GeV corresponding to a relatively low reheat temperature $T_R \lsim$ few $\times 10^7-10^8$ GeV. Neutrino mass and mixing parameters may be reconstructed at accelerator experiments like the Large Hadron Collider.

Nuclear and High Energy PhysicsParticle physicsPhotonAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesMasas de neutrinos01 natural sciencesNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)R-paridad bilinealR-parity0103 physical sciences010306 general physicsNeutrino oscillationLine (formation)PhysicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologyGravitinoHigh Energy Physics::ExperimentNeutrinoGravitino
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Bound-state dark matter and Dirac neutrino mass

2018

We propose a simple theory for the idea that cosmological dark matter (DM) may be present today mainly in the form of stable neutral hadronic thermal relics. In our model neutrino masses arise radiatively from the exchange of colored DM constituents, giving a common origin for both dark matter and neutrino mass. The exact conservation of $B-L$ symmetry ensures dark matter stability and the Dirac nature of neutrinos. The theory can be falsified by dark matter nuclear recoil direct detection experiments, leading also to possible signals at a next generation hadron collider.

PhysicsConservation lawParticle physicsSIMPLE (dark matter experiment)010308 nuclear & particles physicsDirac (video compression format)Dark matterHadronHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Recoil0103 physical sciencesBound stateHigh Energy Physics::ExperimentNeutrino010306 general physics
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Bound-state dark matter with Majorana neutrinos

2019

We propose a simple scenario in which dark matter (DM) emerges as a stable neutral hadronic thermal relics, its stability following from an exact $\operatorname{U}(1)_D$ symmetry. Neutrinos pick up radiatively induced Majorana masses from the exchange of colored DM constituents. There is a common origin for both dark matter and neutrino mass, with a lower bound for neutrinoless double beta decay. Direct DM searches at nuclear recoil experiments will test the proposal, which may also lead to other phenomenological signals at future hadron collider and lepton flavour violation experiments.

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderHadronDark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesComputer Science::Digital Librarieslcsh:QC1-999High Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Phenomenology (hep-ph)Double beta decayBound stateHigh Energy Physics::ExperimentNeutrinoNuclear Experimentlcsh:PhysicsLepton
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