<p>Popular extensions of the standard model of particle physics feature new fields and symmetries which could, for example, dynamically generate neutrino masses from <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(B-L\)</EquationSource> </InlineEquation> spontaneous symmetry breaking. If a new light scalar that decays into dark radiation appears in the spectrum of the theory, it could significantly modify the cosmological observables. In this case, cold dark matter could have a stable and a decaying component and limits on its decay rate <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(\Gamma _\textrm{dcdm}\)</EquationSource> </InlineEquation> can be used to put constraints on the new energy scales of a given model. We illustrate this idea using a gauged <InlineEquation ID="IEq5"> <EquationSource Format="TEX">\(B-L\)</EquationSource> </InlineEquation> model where the dark radiation is in the form of light neutrinos.</p>

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Constraints on Energy Scales from Dark Matter Decay in a Gauged \(B-L\) Model

  • Guillermo Gambini,
  • Pedro C. de Holanda,
  • Saulo Carneiro

摘要

Popular extensions of the standard model of particle physics feature new fields and symmetries which could, for example, dynamically generate neutrino masses from \(B-L\) spontaneous symmetry breaking. If a new light scalar that decays into dark radiation appears in the spectrum of the theory, it could significantly modify the cosmological observables. In this case, cold dark matter could have a stable and a decaying component and limits on its decay rate \(\Gamma _\textrm{dcdm}\) can be used to put constraints on the new energy scales of a given model. We illustrate this idea using a gauged \(B-L\) model where the dark radiation is in the form of light neutrinos.