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This is the divergence theorem. [2] The divergence theorem is employed in any conservation law which states that the total volume of all sinks and sources, that is the volume integral of the divergence, is equal to the net flow across the volume's boundary. [3]
However, many such phenomena may be explained using a halfway theory of quantum matter coupled to a classical electromagnetic field, either as external field or with the expected value of the charge current and density on the right hand side of Maxwell's equations.
The electromagnetic tensor is the combination of the electric and magnetic fields into a covariant antisymmetric tensor whose entries are B-field quantities. [1] = (/ / / / / /) and the result of raising its indices is = = (/ / / / / /), where E is the electric field, B the magnetic field, and c the speed of light.
In physics (specifically electromagnetism), Gauss's law, also known as Gauss's flux theorem (or sometimes Gauss's theorem), is one of Maxwell's equations. It is an application of the divergence theorem , and it relates the distribution of electric charge to the resulting electric field .
These forms are equivalent due to the divergence theorem. The name "Gauss's law for magnetism" [1] is not universally used. The law is also called "Absence of free magnetic poles". [2] It is also referred to as the "transversality requirement" [3] because for plane waves it requires that the polarization be transverse to the direction of ...
By the divergence theorem, Gauss's law for the field P can be stated in differential form as: =, where ∇ · P is the divergence of the field P through a given surface containing the bound charge density .
As a component of the 4D Gauss' Theorem / Stokes' Theorem / Divergence Theorem [ edit ] In vector calculus , the divergence theorem , also known as Gauss's theorem or Ostrogradsky's theorem, is a result that relates the flow (that is, flux ) of a vector field through a surface to the behavior of the vector field inside the surface.
The divergence theorem gives an equivalent integral definition of a solenoidal field; namely that for any closed surface, the net total flux through the surface must be zero: v ⋅ d S = 0 , {\displaystyle \;\;\mathbf {v} \cdot \,d\mathbf {S} =0,}