The role of photon polarization modes in the magnetization and instability of the vacuum in a supercritical field

被引:4
作者
Villalba-Chavez, Selym [1 ]
机构
[1] Graz Univ, Inst Phys, A-8010 Graz, Austria
基金
奥地利科学基金会;
关键词
Vacuum polarization; Vacuum magnetization; Photon emission; STRANGE STARS; GAMMA-QUANTA; DISPERSION; PULSAR; PROPAGATION; RADIATION; COLLAPSE;
D O I
10.1016/j.physletb.2010.08.002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
response of the QED vacuum in an asymptotically large electromagnetic field is studied. In this regime the vacuum energy is strongly influenced by the vacuum polarization effect. The possible interaction between the virtual electromagnetic radiation and a superstrong magnetic field suggests that a background of virtual photons is a source of magnetization to the whole vacuum. The corresponding contribution to the vacuum magnetization density is determined by considering the individual contribution of each vacuum polarization eigenmode in the Euler-Heisenberg Lagrangian. Additional issues concerning the transverse pressures are analyzed. We also study the case in which the vacuum is occupied by a superstrong electric field. It is discussed that, in addition to the electron-positron pairs, the vacuum could create photons with different propagation modes. The possible relation between the emission of photons and the birefringent character of the vacuum is shown as well. (C) 2010 Elsevier B.V. All rights reserved.
引用
收藏
页码:317 / 322
页数:6
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