Frontiers in Science
p-ISSN: 2166-6083 e-ISSN: 2166-6113
2016; 6(2): 36-39
doi:10.5923/j.fs.20160602.02

Mário Everaldo de Souza
Departamento de Física, Universidade Federal de Sergipe, Brazil
Correspondence to: Mário Everaldo de Souza, Departamento de Física, Universidade Federal de Sergipe, Brazil.
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Taking into account the weaknesses of the neutrino oscillation proposal with respect to the experimental data, either the lack of tau neutrino fluxes or the latest results of the Daya Bay Collaboration, it is proposed that the electron neutrino production at the Sun’s core in the pp and CNO cycles should be much larger than what is predicted by the Standard Solar Model, due to the action of a new interaction of matter which has recently been reported. This conclusion is achieved because it is shown that the interaction of electron neutrinos in the Sun’s core medium due to the new interaction cannot account for the observed electron neutrino deficits on Earth. It is implied, therefore, that, in their quest for proving neutrino oscillations, many experiments on neutrinos have found important features of this new interaction of matter.
Keywords: Neutrino, Neutrino Oscillations, New Fundamental Interaction
Cite this paper: Mário Everaldo de Souza, Neutrino Oscillations Hint at a New Fundamental Interaction, Frontiers in Science, Vol. 6 No. 2, 2016, pp. 36-39. doi: 10.5923/j.fs.20160602.02.
pairs, and the OPERA collaboration [16] found one tau neutrino in its quest for neutrino oscillations. The lack of
fluxes invalidates the claim for the neutrino oscillations
and 



but such decays have not been observed at all.
and
prefer to change to
which, according to the neutrino oscillation proposal, would be the most massive neutrino? Why not the opposite, that is, the oscillation of
and
to
? In such a case we would observe higher fluxes of 
and
. Therefore, it is expected that neutrinos should interact with matter by means of this interaction. It is also expected that there should be interplays between this new interaction and the weak interaction because both interactions involve leptons. It is important at this point to comment Daya Bay Collaboration results. This collaboration had reported in 2012 [10] a disappearance of about 6% in the electron antineutrino flux along a distance of 1648 m with respect to the produced flux according to the current models of nuclear theory, but in a paper that has just been published [23] the collaboration corrects the previous results because they report now that the actual production is 6% larger than that one expected from the theoretical nuclear models, and thus, this invalidates their previous disappearance claims.
CC interaction. Its significance, based on our best conservative knowledge of the background, exceeds two
. This does not allow yet claiming the observation of
oscillation. Given its sensitivity, the OPERA experiment will require the detection of a few more candidate events in order to firmly establish neutrino oscillations in direct appearance mode through the identification of the final charged lepton.”We make use below of the concept of particle transparency in a medium and use it for the electron neutrinos in the Sun’s core. Extending the concept of transparency developed by Shapiro and Teukolsky [25] in their analysis of neutrino transparency in stars with core temperatures smaller than
we can say that the effective mean free path of a neutrino in the Sun’s core is given by
in which
and
are the neutrino mean free paths due to elastic scattering off neutrons and the
weak inelastic scattering, respectively, and
is the neutrino mean free path due to the new interaction. Let us try to find an estimate for the new interaction cross section by making the following considerations. In order to significantly diminish the electron neutrino flux to about 45% along the Sun’s core we should have
m where
is the core radius of the Sun and
is the Sun’s radius, assuming that the neutrino flux diminishes exponentially along the travelled distance. The product
is given by the following relation [25]
where
is the neutrino energy in electron-volt,
is the nuclear density and
is the Sun’s core density. For 8B neutrinos the energy spectrum [26] goes from zero up to 14 MeV, and the neutrino flux peaks around 7 MeV [27]. Thus, making
we obtain
and from the relation
we have then
The mean free path
is related to the inelastic cross section
due to the new interaction by the equation
where
is the number of nucleons per unit volume. For the Sun’s core the density of 100 g/cm3 means
nucleons/cm3 and, hence, we obtain
cm2.As
and
depend on the electron and neutron densities, we should take the above calculation with caution because the electron and neutron densities depend strongly on the distance from the core center [28], and thus,
is an average number. Another very important fact raised by Lopes and Turck-Chièze [28] is that different electron neutrinos are generated in different shells in the Sun’s core, and thus, we cannot compare the different values for
and
from the neutrino data of different collaborations when they refer to different neutrinos, but because of the conclusion below we do not need to make such comparisons.The problem with the above calculation is that
cm2 is too large to be true. And as we saw above, although the new interaction is produced through hadronic couplings, its boson only decays to
and
. This means that not only the neutrino, but also the electron would interact strongly by means of this new interaction, but this has not been observed for the electron. All this means that
has to be much smaller than the above number. Reinforcing this reasoning it is worth recalling that the strong interaction between two protons has a cross section of about 40 mbarn, and thus,
would be about 10000 times larger than the strong interaction cross section. Therefore, the solar neutrino problem may only have the other solution presented below.