Results 111 to 120 of about 457,852 (205)

Distinguishing Dirac and Majorana neutrinos with astrophysical fluxes [PDF]

open access: yesarXiv, 2017
Massive neutrinos can have helicity $s_{\parallel}\neq -1$. Neutrino helicity changes when the neutrino interacts with an external magnetic field and it is possible that the left-handed neutrinos born inside the Sun or a supernova could leave their sources with a different helicity.
arxiv  

Relativistic quantum theories and neutrino oscillations

open access: yes, 2010
Neutrino oscillations are examined under the broad requirements of Poincar\'e-invariant scattering theory in an S-matrix formulation. This approach can be consistently applied to theories with either field or particle degrees of freedom.
Akhmedov E K Smirnov A Y   +8 more
core   +1 more source

Aspects of Neutrino Cosmology [PDF]

open access: yesarXiv, 1993
Primordial nucleosynthesis constrains the properties of light, stable neutrinos. Apart from the well--known limit on the number of neutrino species, there are also bounds on neutrino masses and magnetic moments. I discuss also sterile neutrinos and neutrino propagation in a primordial magnetic field, such as could be the origin of the observed galactic
arxiv  

Neutrino Physics: Fundamentals of Neutrino Oscillations [PDF]

open access: yesarXiv, 1996
In this lecture we review some of the basic properties of neutrinos, in particular their mass and the oscillation behavior. First we discuss how to describe the neutrino mass. Then, under the assumption that neutrinos are massive and mixed, the fundamentals of the neutrino oscillations are discussed with emphasis on subtle aspects which have been ...
arxiv  

New bounds on neutrino electric millicharge from limits on neutrino magnetic moment

open access: yes, 2014
Using the new limit on the neutrino anomalous magnetic moment recently obtained by the GEMMA experiment on measurements of the cross section for the reactor antineutrino scattering on free electrons, we get a new direct upper bound on the neutrino ...
Studenikin, Alexander
core   +1 more source

Neutrino Astrophysics [PDF]

open access: yesarXiv, 2012
A review of neutrino astrophysics is presented, including solar and atmospheric neutrinos; neutrino mass and oscillations; the supernova mechanism, supernova neutrino production, and associated nucleosynthesis; cosmological neutrinos and Big Bang nucleosynthesis; neutrino cooling and associated limits on neutrino properties; and high-energy ...
arxiv  

DUNE potential as a new physics probe

open access: yesJournal of High Energy Physics
Neutrino experiments, in the next years, aim to determine with precision all the six parameters of the three-neutrino standard paradigm. The complete success of the experimental program is, nevertheless, attached to the non-existence (or at least ...
Adriano Cherchiglia, José Santiago
doaj   +1 more source

Neutrino Mass and New Physics

open access: yes, 2006
We review the present state of and future outlook for our understanding of neutrino masses and mixings. We discuss what we think are the most important perspectives on the plausible and natural scenarios for neutrinos and what may have the most promise ...
A.Y. Smirnov   +4 more
core   +1 more source

Theoretical Results on Neutrinos [PDF]

open access: yesarXiv, 2015
In this talk, I first summarize our current knowledge about the fundamental properties of neutrinos and emphasize the remaining unsolved problems in neutrino physics. Then, recent theoretical results on neutrino mass models are introduced. Different approaches to understanding tiny neutrino masses, lepton flavor mixing and CP violation are presented ...
arxiv  

Unleashing the power of EFT in neutrino-nucleus scattering

open access: yesJournal of High Energy Physics
Neutrino physics is advancing into a precision era with the construction of new experiments, particularly in the few GeV energy range. Within this energy range, neutrinos exhibit diverse interactions with nucleons and nuclei.
Joachim Kopp, Noemi Rocco, Zahra Tabrizi
doaj   +1 more source

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