0000000000644048

AUTHOR

Takashi Toma

showing 2 related works from this author

Effective Majorana mass matrix from tau and pseudoscalar meson lepton number violating decays

2018

An observation of any lepton number violating process will undoubtedly point towards the existence of new physics and indirectly to the clear Majorana nature of the exchanged fermion. In this work, we explore the potential of a minimal extension of the Standard Model via heavy sterile fermions with masses in the $[ 0.1 - 10]$ GeV range concerning an extensive array of "neutrinoless" meson and tau decay processes. We assume that the Majorana neutrinos are produced on-shell, and focus on three-body decays. We conduct an update on the bounds on the active-sterile mixing elements, $|U_{\ell_\alpha 4} U_{\ell_\beta 4}|$, taking into account the most recent experimental bounds (and constraints) a…

Particle physicsNuclear and High Energy PhysicsMesonPhysics beyond the Standard ModelFOS: Physical sciences7. Clean energy01 natural sciencesPseudoscalar mesonHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)double-beta decay: (0neutrino)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino Physics010306 general physicsnumerical calculationslepton number: violationPhysicsneutrino: heavy: decay010308 nuclear & particles physicsnew physicsHigh Energy Physics::Phenomenologyneutrino: Majorana: massFermionneutrino: sterileMass matrixsensitivityLepton numberMAJORANAHigh Energy Physics - Phenomenologypseudoscalar meson: decay[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Beyond Standard Modellcsh:QC770-798neutrino: Majorana[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimenttau: decayNeutrinoneutrino: mixing
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Observing Higgs boson production through its decay into gamma-rays: A messenger for Dark Matter candidates

2012

In this Letter, we study the gamma-ray signatures subsequent to the production of a Higgs boson in space by dark matter annihilations. We investigate the cases where the Higgs boson is produced at rest or slightly boosted and show that such configurations can produce characteristic bumps in the gamma-ray data. These results are relevant in the case of the Standard Model-like Higgs boson provided that the dark matter mass is about 63 GeV, 109 GeV or 126 GeV, but can be generalized to any other Higgs boson masses. Here, we point out that it may be worth looking for a 63 GeV line since it could be the signature of the decay of a Standard Model-like Higgs boson produced in space, as in the case…

Particle physicsNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesNeutralino annihilationElementary particle7. Clean energy01 natural sciencesNuclear physicssymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsLight dark matterBosonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologyScalar bosonHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Higgs bosonsymbolsHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaHiggs mechanismRoot-s=7 tev
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