scholarly journals Seesaw, coherence and neutrino oscillations

2021 ◽  
Vol 81 (12) ◽  
Author(s):  
Tomi Kupiainen ◽  
Anca Tureanu

AbstractWe present a prescription for consistently constructing non-Fock coherent flavour neutrino states within the framework of the seesaw mechanism, and establish that the physical vacuum of massive neutrinos is a condensate of Standard Model massless neutrino states. The coherent states, involving a finite number of massive states, are derived by constructing their creation operator. This construction fulfills automatically the key requirement of coherence for the oscillations of particles to occur. We comment on the inherent non-unitarity of the oscillation probability induced by the requirement of coherence.

1997 ◽  
Vol 52 (1-2) ◽  
pp. 167-178
Author(s):  
P. Ramond

Abstract We catalog models with massive neutrinos, emphasizing their uses as probes of physics beyond the standard model. We discuss their experimental implications, in terms of neutrino oscillations and the MSW effect.


2003 ◽  
Vol 18 (22) ◽  
pp. 4085-4096 ◽  
Author(s):  
SHARADA IYER DUTTA ◽  
MARY HALL RENO ◽  
INA SARCEVIC

The ultrahigh energy neutrino cross section is well understood in the standard model for neutrino energies up to 1012 GeV, Tests of neutrino oscillations (νμ ↔ ντ) from extragalactic sources of neutrinos are possible with large underground detectors. Measurements of horizontal air shower event rates at neutrino energies above 1010 GeV will be able to constrain nonstandard model contributions to the neutrino-nucleon cross section, e.g., from mini-black hole production.


1989 ◽  
Vol 61 (1) ◽  
pp. 169-169 ◽  
Author(s):  
S. M. Bilenky ◽  
S. T. Petcov

1987 ◽  
Vol 02 (08) ◽  
pp. 565-571
Author(s):  
G. V. DASS ◽  
K. V. L. SARMA

Proceeding in analogy to the Mikheyev-Smirnov enhancement of matter effects on neutrino oscillations we consider the limit wherein the effects of the medium on [Formula: see text] oscillations are maximized. In this limit it is found that the ratio of the strangeness-oscillation probability in matter to that in vacuum cannot exceed unity.


2009 ◽  
Vol 24 (18n19) ◽  
pp. 3286-3296 ◽  
Author(s):  
ZHI-ZHONG XING

I argue that TeV neutrino physics might become an exciting frontier of particle physics in the era of the Large Hadron Collider (LHC). The origin of non-zero but tiny masses of three known neutrinos is probably related to the existence of some heavy degrees of freedom, such as heavy Majorana neutrinos or heavy Higgs bosons, via a TeV-scale seesaw mechanism. I take a few examples to illustrate how to get a balance between theoretical naturalness and experimental testability of TeV seesaws. Besides possible collider signatures at the LHC, new and non-unitary CP-violating effects are also expected to show up in neutrino oscillations for type-I, type-(I+II) and type-III seesaws at the TeV scale.


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