Results 81 to 90 of about 579,711 (182)

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

Journal 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

Signature of supernova neutrino flavor mixing in water Čerenkov detectors [PDF]

, 1994
We study supernova neutrino burst signals in large water erenkov detectors, examining the effects of mixing between νe and either νμ or ντ and taking account of charged current νe capture on oxygen in the detector.
Qian, Yong-Zhong, Fuller, George M
core   +1 more source

Vertex reconstruction in the TAO experiment

Journal of High Energy Physics
The Taishan Antineutrino Observatory (TAO) is a tonne-scale gadolinium-doped liquid scintillator satellite experiment of the Jiangmen Underground Neutrino Observatory (JUNO).
Hangyu Shi, Jun Wang, Guofu Cao, Wei Wang, Yuehuan Wei   +4 more
doaj   +1 more source

Neutrino oscillation prospects with a dual-baseline beam from BNL to SNOLAB and SURF

Journal of High Energy Physics
The Electron-Ion Collider (EIC) is a next-generation accelerator primarily designed to study the internal structure of nucleons through high-precision electron-hadron collisions.
Nishat Fiza, Mehedi Masud, Kim Siyeon, Guang Yang   +3 more
doaj   +1 more source

Neutrino Physics : Majorana Neutrino Masses and Mixing (2/4)

, 2009
The general theory of neutrino masses and mixing is introduced. The theory of neutrino oscillations in vacuum and in matter is reviewed, with discussion of the most important general phenomenological aspects.
Carlo GIUNTI
core  

Single-wave solutions of the neutrino fast flavor system. Part I. Mechanical properties

Journal of High Energy Physics
A dense neutrino plasma can exhibit collective flavor evolution caused by neutrino-neutrino refraction. Recently, a new class of exact nonlinear inhomogeneous solutions was discovered: single-wave (SW) solutions of the fast flavor system.
Damiano F. G. Fiorillo, Georg G. Raffelt
doaj   +1 more source

88th Annual Meeting of the Meteoritical Society 2026: Abstracts

Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley   +1 more source

Neutrino Physics : Phenomenology of Three-Neutrino Mixing (4/4)

, 2009
The general theory of neutrino masses and mixing is introduced. The theory of neutrino oscillations in vacuum and in matter is reviewed, with discussion of the most important general phenomenological aspects.
Carlo GIUNTI
core  

Neutrino Physics : Dirac Neutrino Masses and Mixing (1/4)

, 2009
The general theory of neutrino masses and mixing is introduced. The theory of neutrino oscillations in vacuum and in matter is reviewed, with discussion of the most important general phenomenological aspects.
Carlo GIUNTI
core  

Theory of neutrino slow flavor evolution. Part II. Space-time evolution of linear instabilities

Journal of High Energy Physics
Slow flavor evolution (defined as driven by neutrino masses and not necessarily “slow”) is receiving fresh attention in the context of compact astrophysical environments.
Damiano F. G. Fiorillo, Georg G. Raffelt
doaj   +1 more source