The representation of microscopic charge and current densities in terms of polarization and magnetization fields

The microscopic charge and current densities due to an aggregate of charged point particles are shown to be derivable from polarization and magnetization fields defined as sums of line integrals of delta functions along curves joining an arbitrary reference point, which may be moving, to the positions of the particles. The analysis given generalizes previous treatm ents th at deal with a fixed reference point and includes the description of ionic, free electronic and Rontgen currents. The class of ‘admissible’ polarization and magnetization fields, which give rise to a specified charge and current distribution, is shown to be generated by two arbitrary differentiable fields, one scalar and one vector. The class of these latter fields that effect the transformation connecting two given pairs of admissible polarization and magnetization fields is shown in turn to be generated by two arbitrary scalar fields, one a function of position and time and the other a function of time only. The transformation rules are verified for polarization and magnetization fields that are representable as sums of line integrals of delta functions, and the scalar and vector fields that appear in the transformations are identified with integrals over certain moving surfaces and volumes. By means of these identifications it is demonstrated that the class of polarization and magnetization fields that are representable as sums of line integrals of delta functions forms a proper subset of the total class of admissible fields, so that not every admissible polarization or magnetization field is so representable.

1995 ◽  
Vol 10 (16) ◽  
pp. 2333-2347
Author(s):  
N.N. SHTYKOV

We compute the one-loop potential (the Casimir energy) for scalar fields with coupling ξR and massive spinor and vector fields on the spaces Rm+1×Y with Y=SN, CP2. We find that in most of the models a divergent part of the Casimir energy on even-dimensional spaces is canceled by means of the appropriate values of ξ, msp, mv. As a physical model we consider spinor electrodynamics on four-dimensional product manifolds and show that the Casimir energy is finite on R1×S3, R3×S1 and R2×S2 for msp=0, msp=0 and [Formula: see text] respectively.


1994 ◽  
Vol 09 (10) ◽  
pp. 875-883 ◽  
Author(s):  
NOUREDDINE MOHAMMEDI

We consider gravity using the formalism of a differential Z2-graded algebra of 2 × 2 matrices whose elements are differential forms on space-time. The connection and the orthonormal frame are extended to incorporate additional scalar and vector fields. The extended torsion-free constraints are solved for a simple case. The resulting action describes a set of scalar fields minimally coupled to Einstein-Hilbert gravity.


Author(s):  
Jian Ge ◽  
Rui Wang ◽  
Haobin Dong ◽  
Huan Liu ◽  
Qianwei Zheng ◽  
...  

2001 ◽  
Vol 16 (23) ◽  
pp. 1479-1486 ◽  
Author(s):  
A. A. BYTSENKO ◽  
A. E. GONÇALVES ◽  
S. ZERBINI

The non-planar contribution to the effective potentials for massless scalar and vector quantum field theories on D-dimensional manifold with p compact noncommutative extra dimensions is evaluated by means of dimensional regularization implemented by zeta function techniques. It is found that, the zeta function associated with the one-loop operator may not be regular at the origin. Thus, the related heat kernel trace has a logarithmic term in the short t asymptotic expansion. Consequences of this fact are briefly discussed.


Author(s):  
Iosif L. Buchbinder ◽  
Ilya L. Shapiro

This chapter discusses classical fields in an arbitrary Riemann spacetime. General considerations are followed by the formulation of scalar fields with non-minimal coupling. Spontaneous symmetry breaking in curved space is shown to provide the induced gravity action with a cosmological constant. The construction of spinor fields in curved spacetime is based on the notions of group theory from Part I and on the local Lorentz invariance. Massless vector fields (massless vector gauge fields) are described and the interactions between scalar, fermion and gauge fields formulated. A detailed discussion of classical conformal transformations and conformal symmetry for both matter fields and vacuum action is also provided.


1991 ◽  
Vol 130 ◽  
pp. 71-74
Author(s):  
A.Z. Dolginov ◽  
N.A. Silant’ev

AbstractA new method for the calculation of kinetic coefficients is presented. This method allows us to obtain the distribution of scalar and vector fields (such as the temperature, the admixture particle number density and the magnetic field) in turbulent cosmic media with any value of S = u0т0/R0. The explicit expression for the “turbulent” diffusivity DT is obtained. In some cases DT becomes negative, implying the clustering of the admixture particles in patches (a local increase of the temperature and magnetic fields). The magnetic α-effect is considered for the case S ~ 1.


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