# LOG#136. Flavor ν mixtures.

Neutrino oscillations are one of the most surprising “sounds” in the whole Universe. Since neutrinos do oscillate/mix, they are massive. And due to mass, they can experiment “mixing” or “changes” of flavor (mass and flavor basis are different!). Even more, if some neutrino species were provided to experiment “decay”, we would have a very striking analogy with classical mechanics and sound waves: sound waves experiment frequency (mass) oscillations and damping or attenuation when “air” vibrates. Of course, the analogy is not full or complete since we do not know what is the vibrating medium (of course, in field theory, we assume that is the neutrino field what oscillates) and the decay of neutrino, if it exists, is either impossible or a very uncommon phenomenon. Anyway, we can study these effects and this analogy (with the pictures above) should be helpful for eager readers.

We can implement the celebrated density matrix approach in the description of the flavor mixture for neutrinos. It provides a very convenient tool for further extensions, such as the inclusion of neutrino decay. Neutrino decay is important because it is a possibility we have when we consider BSM (Beyond Standard Model) theories and/or some interesting cosmological applications.

Let us define some weights , with , so

In the initial time the system is described by a pure diagonal density matrix (pure state):

and it is normalized under the condition

Using the common PMNS (Pontecorvo-Maki-Nakagawa-Sakata) matrix for the neutrino mixing matrix,

Then, we also have

The time evolution of the density matrix is determined by the following equation

Equivalently, we can write it as follows

and where

In general, this density matrix will not be diagonal, and here there

is the annihilation rate (or decay width). Note that , using the damping term

accounts for the absorption, decay or instability of some particular neutrino species! The probability for some flavor state to detect the state is giving by the next quantum result (remember that with no neutrino masses and complete stability of all neutrino species we get some uninteresting result):

We can also rewrite this deep result separating the diagonal and non diagonal part (due to quantum interference!). The final formula reads

with

Averaging with this formula, we get that for detected neutrinos in the flavor state (remember that due to mass, mass eigenstates are different to flavor eigenstates):

Cosmic neutrino detectors (neutrino telescopes) are unlikely to be capable of neutrino flavor tagging. Therefore, summing over all neutrino species

and where we have supposed the common assumption that under “a long journey”, and with 3 active neutrino species, we would expect equiprobability, i.e., equal weights

so

for all and .

This density matrix formalism is very useful when one tries to include the redshift effect on neutrino oscillations and it makes us to wonder if quantum entanglement with neutrino beams could be observed in the near future. Indeed, the potential applications of neutrino entanglement are yet to be unveiled. Perhaps, neutrino entanglement could be useful for medicine, security, encryption and decode of information, and fascinating new technologies…

See you in my next TSOR post!!!!!

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