Results 31 to 40 of about 457,852 (205)

Neutrino Properties, Cosmology [PDF]

open access: yesMod.Phys.Lett.A22:1841-1848,2007, 2007
Review of neutrino properties; double beta decay; very high energy neutrinos ...
arxiv   +1 more source

$ν- K^0$ Analogy, Dirac-Majorana Neutrino Duality and the Neutrino Oscillations [PDF]

open access: yesInt.J.Mod.Phys.A16:4911-4924,2001, 2001
The intent of this paper is to convey a new primary physical idea of a Dirac-Majorana neutrino duality in relation to the topical problem of neutrino oscillations. In view of the new atmospheric, solar and the LSND neutrino oscillation data, the Pontecorvo $\nu - K^0$ oscillation analogy is generalized to the notion of neutrino duality with ...
arxiv   +1 more source

Is there evidence for additional neutrino species from cosmology? [PDF]

open access: yes, 2017
It has been suggested that recent cosmological and flavor-oscillation data favor the existence of additional neutrino species beyond the three predicted by the Standard Model of particle physics.
Feeney, Stephen M.   +2 more
core   +1 more source

Dark Matter, Baryogenesis and Neutrino Oscillations from Right Handed Neutrinos [PDF]

open access: yes, 2012
We show that, leaving aside accelerated cosmic expansion, all experimental data in high energy physics that are commonly agreed to require physics beyond the Standard Model can be explained when completing it by three right handed neutrinos that can be ...
Canetti, Laurent   +3 more
core   +1 more source

Neutrino electromagnetic properties [PDF]

open access: yesPhys.Atom.Nucl.72:2089-2125,2009, 2008
The main goal of the paper is to give a short review on neutrino electromagnetic properties. In the introductory part of the paper a summary on what we really know about neutrinos is given: we discuss the basics of neutrino mass and mixing as well as the phenomenology of neutrino oscillations.
arxiv   +1 more source

Lectures on neutrino phenomenology [PDF]

open access: yesNucl.Phys.Proc.Suppl.203-204:45-81,2010, 2010
The fundamental properties of the lepton sector include the neutrino masses and flavor mixings. Both are difficult to observe because of the extremely small neutrino masses and neutrino-matter cross sections. In these lectures, we focus on the basic concepts for the determination of neutrino properties.
arxiv   +1 more source

Compressibility Function and Speed of Sound in the Non‐Commutative Quantum Hadrodynamics Type‐I Model for Neutron Stars

open access: yesAstronomische Nachrichten, EarlyView.
ABSTRACT We investigate the effects of a minimal measurable length on neutron stars, within the quantum hadrodynamics (QHD‐I) model modified by the Generalized Uncertainty Principle (GUP). Working in a deformed Poisson algebra framework, we incorporate GUP effects via a time‐invariant transformation of the phase space volume, effectively reducing the ...
João Gabriel Galli Gimenez   +2 more
wiley   +1 more source

The effect of electromagnetic properties of neutrinos on the photon-neutrino decoupling temperature [PDF]

open access: yesInternational Journal of Modern Physics A, Vol. 27, No. 32 (2012) 1250187, 2012
We examine the impact of electromagnetic properties of neutrinos on the annihilation of relic neutrinos with ultra high energy cosmic neutrinos for the $\nu \bar{\nu}\to \gamma\gamma$ process. For this process, photon-neutrino decoupling temperature is calculated via effective lagrangian model beyond the standard model.
arxiv   +1 more source

Imprints of scalar NSI on the CP-violation sensitivity using synergy among DUNE, T2HK and T2HKK

open access: yesJournal of High Energy Physics, 2023
The Non-Standard Interactions (NSIs) are subdominant effects, often appearing in various extensions of SM, which may impact the neutrino oscillations through matter.
Abinash Medhi   +2 more
doaj   +1 more source

Invisible Labor and the “Ghost Particle”: Underground Physics at the Kolar Gold Fields**

open access: yesBerichte zur Wissenschaftsgeschichte, EarlyView.
Abstract When cosmic rays—high‐energy particles from outer space—encounter the Earth's atmosphere, they produce particles called neutrinos. To detect them, physicists go underground inside deep mines where the overlying rock can filter out the cosmic‐ray background radiation.
Nithyanand Rao
wiley   +1 more source

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