Vacuum instability due to the creation of neutral fermion with anomalous magnetic moment by magnetic-field inhomogeneities

被引:6
作者
Adorno, T. C. [1 ,2 ,3 ]
He, Zi-Wang [1 ,2 ]
Gavrilov, S. P. [3 ,4 ]
Gitman, D. M. [3 ,5 ,6 ]
机构
[1] Hebei Univ, Coll Phys Sci & Technol, Dept Phys, Wusidong Rd 180, Baoding 071002, Peoples R China
[2] Hebei Univ, Key Lab High Precis Computat & Applicat Quantum, Wusidong Rd 180, Baoding 071002, Peoples R China
[3] Tomsk State Univ, Dept Phys, Lenin Prospekt 36, Tomsk 634050, Russia
[4] Herzen State Pedag Univ Russia, Dept Gen & Expt Phys, Moyka Embankment 48, St Petersburg 191186, Russia
[5] PN Lebedev Phys Inst, 53 Leninskiy Prospekt, Moscow 119991, Russia
[6] Univ Sao Paulo, Inst Fis, Caixa Postal 66318, BR-05508090 Sao Paulo, SP, Brazil
基金
俄罗斯科学基金会;
关键词
Nonperturbative Effects; Neutrino Physics; PAIR CREATION; HELIUM FLASH; CORE MASS; ELECTRON; SCATTERING; EVOLUTION; MATTER;
D O I
10.1007/JHEP12(2021)046
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We study neutral fermions pair creation with anomalous magnetic moment from the vacuum by time-independent magnetic-field inhomogeneity as an external background. We show that the problem is technically reduced to the problem of charged-particle creation by an electric step, for which the nonperturbative formulation of strong-field QED is used. We consider a magnetic step given by an analytic function and whose inhomogeneity may vary from a "gradual" to a "sharp" field configuration. We obtain corresponding exact solutions of the Dirac-Pauli equation with this field and calculate pertinent quantities characterizing vacuum instability, such as the differential mean number and flux density of pairs created from the vacuum, vacuum fluxes of energy and magnetic moment. We show that the vacuum flux in one direction is formed from fluxes of particles and antiparticles of equal intensity and with the same magnetic moments parallel to the external field. Backreaction to the vacuum fluxes leads to a smoothing of the magnetic-field inhomogeneity. We also estimate critical magnetic field intensities, near which the phenomenon could be observed.
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页数:31
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