scholarly journals Unveiling dipolar spectral regimes of large dielectric Mie spheres from helicity conservation

2020 ◽  
Vol 2 (4) ◽  
Author(s):  
Jorge Olmos-Trigo ◽  
Diego R. Abujetas ◽  
Cristina Sanz-Fernández ◽  
Xavier Zambrana-Puyalto ◽  
Nuno de Sousa ◽  
...  
2021 ◽  
Vol 87 (1) ◽  
Author(s):  
Valery V. Pipin

We study the helicity density patterns which can result from the emerging bipolar regions. Using the relevant dynamo model and the magnetic helicity conservation law we find that the helicity density patterns around the bipolar regions depend on the configuration of the ambient large-scale magnetic field, and in general they show a quadrupole distribution. The position of this pattern relative to the equator can depend on the tilt of the bipolar region. We compute the time–latitude diagrams of the helicity density evolution. The longitudinally averaged effect of the bipolar regions shows two bands of sign for the density distributions in each hemisphere. Similar helicity density patterns are provided by the helicity density flux from the emerging bipolar regions subjected to surface differential rotation.


1972 ◽  
Vol 49 ◽  
pp. 441-457 ◽  
Author(s):  
J.V. Beaupré ◽  
M. Deutschmann ◽  
P. Finkler ◽  
H. Grässler ◽  
K.F. Albrecht ◽  
...  

1972 ◽  
Vol 5 (11) ◽  
pp. 2864-2868
Author(s):  
Paul Langacker

1971 ◽  
Vol 1 (22) ◽  
pp. 927-930 ◽  
Author(s):  
H. J. W. Müller

1998 ◽  
Vol 13 (29) ◽  
pp. 5023-5036 ◽  
Author(s):  
SALVATORE ESPOSITO

We analyze both chirality-changing and chirality-preserving transitions of Dirac–Majorana neutrinos. In vacuum, the first ones are suppressed with respect to the others due to helicity conservation and the interactions with a ("normal") medium practically does not affect the expressions of the probabilities for these transitions, even if the amplitudes of oscillations change slightly. For usual situations involving relativistic neutrinos we find no resonant enhancement for all flavor-conserving transitions. However, for very light neutrinos propagating in superdense media, the pattern of oscillations [Formula: see text] is dramatically altered with respect to the vacuum case, the transition probability practically vanishing. An application of this result is envisaged.


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