Results 71 to 80 of about 3,039,927 (219)

Supernova ν flavour conversions in DUNE: the slow, the fast and the standard

open access: yesJournal of High Energy Physics
The flavour composition of a future supernova neutrino signal is expected to carry measurable imprints of flavour conversion processes in the dense stellar medium.
A. Giarnetti, J. T. Penedo
doaj   +1 more source

Nonstandard interactions in solar neutrino oscillations with Hyper-Kamiokande and JUNO

open access: yesPhysics Letters B, 2017
Measurements of the solar neutrino mass-squared difference from KamLAND and solar neutrino data are somewhat discrepant, perhaps due to nonstandard neutrino interactions in matter.
Jiajun Liao   +2 more
doaj   +1 more source

Microscopic and macroscopic effects in the decoherence of neutrino oscillations

open access: yesJournal of High Energy Physics, 2022
We present a generic structure (the layer structure) for decoherence effects in neutrino oscillations, which includes decoherence from quantum mechanical and classical uncertainties. The calculation is done by combining the concept of open quantum system
Ting Cheng   +2 more
doaj   +1 more source

Work Versus Force: Simultaneous Processes for Describing Interactions

open access: yesAdvanced Physics Research, Volume 5, Issue 6, June 2026.
ABSTRACT Achieving a unified description of interactions remains an open challenge in theoretical physics, which currently describes four fundamental forces. This situation may be viewed differently when interactions are formulated in terms of processes (work as actio) rather than forces (force as actio), not only at the macroscopic level but also at ...
Grit Kalies   +2 more
wiley   +1 more source

Phenomenology of a Low-Energy Neutrino Factory and Related Experiments [PDF]

open access: yes, 2010
The discovery of neutrino oscillations is one of the most important in the recent history of particle physics, being the first evidence of physics beyond the Standard Model.
LI, TRACEY,CHUIYEE, Li, Tracey Chuiyee
core  

Dispersion relation of the neutrino plasma: unifying fast, slow, and collisional instabilities

open access: yesJournal of High Energy Physics
In neutrino-dense astrophysical environments, these particles exchange flavor through a coherent weak field, forming a collisionless neutrino plasma with collective flavor dynamics.
Damiano F. G. Fiorillo, Georg G. Raffelt
doaj   +1 more source

Constraining general U(1) interactions from neutrino-electron scattering measurements at DUNE near detector

open access: yesJournal of High Energy Physics, 2022
The neutrino-electron scattering process is a powerful tool to explore new physics beyond the standard model. Recently the possibility of DUNE Near Detector (ND) to constrain various new physics scenarios using this process have been highlighted in the ...
Kaustav Chakraborty   +3 more
doaj   +1 more source

Hidden No More: Spotlight on Tidal Disruption Events in Active Galactic Nuclei

open access: yesAstronomische Nachrichten, Volume 347, Issue 5, June 2026.
ABSTRACT Tidal disruption events (TDEs) are typically discovered in previously quiescent galaxies. However, earlier studies have revealed a handful of TDEs occurring in pre‐existing active galactic nuclei (AGN). We discuss AT2019aalc, a promising TDE candidate in an AGN, and compare it to similar sources.
Patrik Milán Veres
wiley   +1 more source

Quasielastic neutrino-nucleus interactions [PDF]

open access: yesNuclear Physics B, 1971
Abstract Calculations of the Pauli exclusion effect are made in a simple shell model. Shell structure effects, associated with spin-orbit splitting, appear, but are not large and decrease rapidly with increasing momentum transfer. The shell model remains less exclusive on the whole than the standard Fermi gas, but not sufficiently so to explain the ...
BELL, J. S., SMITH, C. H. LLEWELLYN
openaire   +2 more sources

Neutrino-Nucleus Interactions and Long-Baseline Experiments

open access: yes, 2018
In long-baseline experiments the extraction of neutrino mixing parameters and the CP-violating phase requires an event-by-event reconstruction of the neutrino energy from the final state of a neutrino-nucleus reaction.
Mosel, Ulrich (5384957), Mosel, Ulrich
core   +1 more source

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