scholarly journals Chiral oscillations in the non-relativistic regime

2021 ◽  
Vol 81 (5) ◽  
Author(s):  
Victor A. S. V. Bittencourt ◽  
Alex E. Bernardini ◽  
Massimo Blasone

AbstractMassive Dirac particles are a superposition of left and right chiral components. Since chirality is not a conserved quantity, the free Dirac Hamiltonian evolution induces chiral quantum oscillations, a phenomenon related to the Zitterbewegung, the trembling motion of free propagating particles. While not observable for particles in relativistic dynamical regimes, chiral oscillations become relevant when the particle’s rest energy is comparable to its momentum. In this paper, we quantify the effect of chiral oscillations on the non-relativistic evolution of a particle state described as a Dirac bispinor and specialize our results to describe the interplay between chiral and flavor oscillations of non-relativistic neutrinos: we compute the time-averaged survival probability and observe an energy-dependent depletion of the quantity when compared to the standard oscillation formula. In the non-relativistic regime, this depletion due to chiral oscillations can be as large as 40$$\%$$ % . Finally, we discuss the relevance of chiral oscillations in upcoming experiments which will probe the cosmic neutrino background.

Author(s):  
W-Y. PAUCHY HWANG

We attempt to answer whether neutrinos and antineutrinos, such as those in the cosmic neutrino background, would clusterize among themselves or even with other dark-matter particles, under certain time span, say 1 Gyr. With neutrino masses in place, the similarity with the ordinary matter increases and so is our confidence for neutrino clustering if time is long enough. In particular, the clusterings could happen with some seeds (cf. see the text for definition), the chance in the dark-matter world to form dark-matter galaxies increases. If the dark-matter galaxies would exist in a time span of 1 Gyr, then they might even dictate the formation of the ordinary galaxies (i.e. the dark-matter galaxies get formed first); thus, the implications for the structure of our Universe would be tremendous.


2014 ◽  
Vol 90 (7) ◽  
Author(s):  
Mariangela Lisanti ◽  
Benjamin R. Safdi ◽  
Christopher G. Tully

1982 ◽  
Vol 67 (2) ◽  
pp. 213-222
Author(s):  
V. Alonso ◽  
J. Chela-Flores ◽  
R. Paredes

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