Mostrando 3,601 - 3,620 Resultados de 8,091 Para Buscar '"neutrinos"', tiempo de consulta: 0.19s Limitar resultados
  1. 3601
    “…Using a no-scale supergravity framework, we construct an SO(10) model that makes predictions for cosmic microwave background observables similar to those of the Starobinsky model of inflation, and incorporates a double-seesaw model for neutrino masses consistent with oscillation experiments and late-time cosmology. …”
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    Enlace del recurso
  2. 3602
  3. 3603
    “…We also discuss the model's predictions for neutrino masses, and pay particular attention to the behaviours of scalar fields during and after inflation, reheating and the GUT phase transition. …”
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    Enlace del recurso
  4. 3604
  5. 3605
    por Ghiglieri, J., Laine, M.
    Publicado 2017
    “…The scenario of baryogenesis through GeV-scale sterile neutrino oscillations is governed by non-linear differential equations for the time evolution of a sterile neutrino density matrix and Standard Model lepton and baryon asymmetries. …”
    Enlace del recurso
    Enlace del recurso
  6. 3606
    por Ereditato, Antonio
    Publicado 2018
    “…Many fundamental discoveries in particle physics had the neutrino involved in one way or another. To date, neutrino physics is still one of the hottest topics of modern particle physics. …”
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  7. 3607
    por Wang, Wenxiao
    Publicado 2018
    “…​This talk focuses on the search for exotic heavy Majorana or Dirac neutrinos and heavy gauge bosons in events with two same- or opposite-sign charged leptons and jets. …”
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  8. 3608
  9. 3609
  10. 3610
  11. 3611
  12. 3612
  13. 3613
  14. 3614
  15. 3615
  16. 3616
    “…The observation by the IceCube Collaboration of a high-energy ($E \gtrsim 200$ TeV) neutrino from the direction of the blazar TXS 0506+056 and the coincident observations of enhanced $\gamma$-ray emissions from the same object by MAGIC and other experiments can be used to set stringent constraints on Lorentz violation in the propagation of neutrinos that is linear in the neutrino energy: $\Delta v = - E/M_1$, where $\Delta v$ is the deviation from the velocity of light, and $M_1$ is an unknown high energy scale to be constrained by experiment. …”
    Enlace del recurso
    Enlace del recurso
  17. 3617
  18. 3618
    “…Background: The reconstruction of the neutrino energy is crucial in oscillation experiments that use interactions with nuclei to detect the neutrino. …”
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    Enlace del recurso
  19. 3619
  20. 3620
    por Nagai, Yoshikazu
    Publicado 2018
    “…A precise prediction of the neutrino flux is a key ingredient for achieving the physics goals of long-baseline neutrino experiments. …”
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