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Space-time localization diagrams ``unlock" subtle aspects of $\nu$ oscillations such as coherence and entanglement. Observability of propagation decoherence in oscillating neutrino state is discussed. The sizes of WPs of reactor and source…

High Energy Physics - Phenomenology · Physics 2022-12-21 Alexei Y Smirnov

In the simplistic quantum mechanical picture of flavor mixing, conditions on the maximum size and minimum coherence time of the source and detector regions for the observation of interference---as well as the very viability of the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Christian Y. Cardall

We study the complementarity between accelerator and reactor coherent elastic neutrino-nucleus elastic scattering (CE$\nu$NS) experiments for constraining new physics in the form of non-standard neutrino interactions (NSI). Firstly,…

High Energy Physics - Phenomenology · Physics 2018-02-14 James B. Dent , Bhaskar Dutta , Shu Liao , Jayden L. Newstead , Louis E. Strigari , Joel W. Walker

We study spin and flavor oscillations of astrophysical neutrinos under the influence of external fields in curved spacetime. First, we consider spin oscillations in case of neutrinos gravitationally scattered off a rotating supermassive…

High Energy Physics - Phenomenology · Physics 2023-06-01 Maxim Dvornikov

Deviations from unitarity in the three-neutrino mixing canonical picture are expected in many physics scenarios beyond the Standard Model. The mixing of new heavy neutral leptons with the three light neutrinos would in principle modify the…

High Energy Physics - Phenomenology · Physics 2023-03-24 Stefano Gariazzo , Pablo Martínez-Miravé , Olga Mena , Sergio Pastor , Mariam Tórtola

Providing an accurate modeling of neutrino physics in dense astrophysical environments such as binary neutron star mergers presents a challenge for hydrodynamic simulations. Nevertheless, understanding how flavor transformation can occur…

High Energy Astrophysical Phenomena · Physics 2025-01-15 Julien Froustey , Sherwood Richers , Evan Grohs , Samuel Flynn , Francois Foucart , James P. Kneller , Gail C. McLaughlin

We present an expression for the transition probability between Dirac or Majorana neutrino flavors obtained from first principles within quantum field theory. Our derivation is based on a standard quantum mechanical setup and includes the…

High Energy Physics - Phenomenology · Physics 2008-10-23 Luca Visinelli , Paolo Gondolo

In the framework of quantum field theory, we analyze the neutrino oscillations in the presence of a torsion background. We consider the Einstein-Cartan theory and we study the cases of constant torsion and of linearly time dependent…

High Energy Physics - Phenomenology · Physics 2024-02-13 Antonio Capolupo , Giuseppe De Maria , Simone Monda , Aniello Quaranta , Raoul Serao

We study neutrino oscillations in a rotating spacetime under the weak gravity limit for the trajectories of neutrinos which are constrained in the equatorial plane. Using the asymptotic form of the Kerr metric, we show that the rotation of…

High Energy Physics - Phenomenology · Physics 2022-11-01 Himanshu Swami

The quantum field theoretical description of coherence in the oscillations of particles, especially neutrinos, is a standing problem in particle physics. In this talk, several inconsistencies of the standard approach to particle…

High Energy Physics - Phenomenology · Physics 2021-01-01 Anca Tureanu

To describe neutrino oscillations in the sense of quantum mechanics and quantum field theory, we propose to use an off-diagonal neutrino-Higgs (mass) interaction, as discussed originally in a family gauge theory and in the extended Standard…

High Energy Physics - Phenomenology · Physics 2013-08-16 W. -Y. Pauchy Hwang

The neutrino oscillations in vacuum are derived in a manifestly coherent scheme. The mechanism is operative in a quantum field theoretical framework, justifying nevertheless a formal analogy with quantum mechanical two- (or more) level…

High Energy Physics - Phenomenology · Physics 2023-08-09 Anca Tureanu

IceCube have observed neutrinos which are presumably of extra-galactic origin. Since specific sources have not yet been identified, we discuss what could be learned from the conceptual point of view. We use a simple model for neutrino…

High Energy Astrophysical Phenomena · Physics 2014-11-19 Walter Winter

The neutrino oscillation patterns can be modified by neutrino interactions with external environments including electromagnetic fields that can influence on neutrinos in the case neutrinos have nonzero electromagnetic properties [1]. The…

High Energy Physics - Phenomenology · Physics 2020-01-01 Konstantin Stankevich , Alexander Studenikin

The connection between cosmological observations and neutrino physics is discussed in detail. Neutrinos decouple from thermal contact in the early Universe at a temperature of order 1 MeV which coincides with the temperature where light…

High Energy Physics - Phenomenology · Physics 2008-11-26 Steen Hannestad

We study three-flavor neutrino oscillations in the early universe in the presence of neutrino chemical potentials. We take into account all effects from the background medium, i.e. collisional damping, the refractive effects from charged…

High Energy Physics - Phenomenology · Physics 2009-11-07 A. D. Dolgov , S. H. Hansen , S. Pastor , S. T. Petcov , G. G. Raffelt , D. V. Semikoz

In this chapter we present basic concepts of neutrino physics. We start with a brief introduction to the standard model electroweak sector, followed by calculations of some relevant neutrino interaction cross sections. We obtain the…

High Energy Physics - Phenomenology · Physics 2022-06-28 Pedro A. N. Machado

In this work we propose an extended formulation for the interaction between neutrinos and gravitational fields. It is based on the parametrized post-Newtonian aproach, and includes a violation of the universality of the gravitational…

High Energy Physics - Phenomenology · Physics 2009-12-30 H. Casini , J. C. D'Olivo , R. Montemayor , L. F. Urrutia

We study the mixing of different kind of fields (scalar in 0+1D, scalar in 3+1D, fermion in 3+1D) treating the mixing term as an interaction. To this aim, we employ the usual perturbative series in the interaction picture. We find that…

High Energy Physics - Phenomenology · Physics 2023-07-31 Massimo Blasone , Francesco Giacosa , Luca Smaldone , Giorgio Torrieri

In dense astrophysical environments, notably core-collapse supernovae and neutron star mergers, neutrino-neutrino forward scattering can spawn flavor conversion on very short scales. Scattering with the background medium can impact…

High Energy Physics - Phenomenology · Physics 2024-07-31 Damiano F. G. Fiorillo , Ian Padilla-Gay , Georg G. Raffelt
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