scholarly journals Nonperturbative quasiclassical theory of the nonlinear electrodynamic response of graphene

2017 ◽  
Vol 95 (8) ◽  
Author(s):  
S. A. Mikhailov
2005 ◽  
Vol 14 (02) ◽  
pp. 309-321 ◽  
Author(s):  
MAXIM DVORNIKOV ◽  
ALEXANDER GRIGORIEV ◽  
ALEXANDER STUDENIKIN

We develop the quasiclassical theory of a massive neutrino spin evolution in the presence of gravitational fields, and the corresponding probability of the neutrino spin oscillations in gravitational fields is derived for the first time. On this basis we also predict a new mechanism for electromagnetic radiation by a neutrino moving in the vicinity of gravitating objects (the "spin light of neutrino," SLν, in gravitational fields). It is shown that the total power of this radiation is proportional to the neutrino gamma factor to the fourth power, and the emitted photon energy, for the case of an ultra relativistic neutrino, spans up to gamma-rays. We investigate the SLν caused by both gravitational and electromagnetic fields, also accounting for effects of arbitrary moving and polarized matter, in various astrophysical environments. In particular, we discuss the SLν emitted by a neutrino moving in the vicinity of a rotating neutron star, black hole surrounded by dense matter, as well as by a neutrino propagating in the relativistic jet from a quasar.


2002 ◽  
Vol 318 (2-3) ◽  
pp. 162-179 ◽  
Author(s):  
M.H.S. Amin ◽  
A.N. Omelyanchouk ◽  
S.N. Rashkeev ◽  
M. Coury ◽  
A.M. Zagoskin

Author(s):  
Oleksandr Kostiantynovych Reity ◽  
Volodymyr Yuriiovych Lazur ◽  
Vladyslav Kostiantynovych Reity

2020 ◽  
Vol 29 (05) ◽  
pp. 2050032
Author(s):  
Shuang Yu ◽  
Changjun Gao

We construct exact black hole solutions to Einstein gravity with nonlinear electrodynamic field. In these solutions, there are, in general, four parameters. They are physical mass, electric charge, cosmological constant and the coupling constant. These solutions differ significantly from the Reissner–Nordström–de Sitter solution in Einstein–Maxwell gravity with a cosmological constant, due to the presence of coupling constant. For example, some of them are endowed with a topological defect on angle [Formula: see text] and the electric charge of some can be much larger or smaller than their mass by varying the coupling constant. On the other hand, these spacetimes are all asymptotically de Sitter (or anti-de Sitter). As a result, their causal structure is similar to the Reissner–Nordström–de Sitter spacetime. Finally, the investigations on the thermodynamics reveal that the coupling constant except for solution-4 has the opposite effect as temperature on the phase, structure of black holes. Concretely, the phase-space changes from single phase to three phases with the decrease of temperature. On the contrary, it changes from three phases to a single phase with the decrease of coupling constant.


2003 ◽  
Vol 13 (2) ◽  
pp. 3734-3737 ◽  
Author(s):  
Zhi Qi ◽  
Hengyi Xu ◽  
Wei Wang ◽  
Daole Yin ◽  
Furen Wang ◽  
...  

2007 ◽  
Vol 105 (11-12) ◽  
pp. 1471-1485 ◽  
Author(s):  
Leonid V. Poluyanov ◽  
Sabyashachi Mishra ◽  
Wolfgang Domcke

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