Mathematical descriptions of the electromagnetic field

From Wikipedia, the free encyclopedia
Jump to: navigation, search

There are various mathematical descriptions of the electromagnetic field that are used in the study of electromagnetism, one of the four fundamental forces of nature. In this article three approaches are discussed, generally the equations are in terms of electric and magnetic fields, potentials, and charges with currents.

Vector field approach[edit]

The most common description of the electromagnetic field uses two three-dimensional vector fields called the electric field and the magnetic field. These vector fields each have a value defined at every point of space and time and are thus often regarded as functions of the space and time coordinates. As such, they are often written as E(x, y, z, t) (electric field) and B(x, y, z, t) (magnetic field).

If only the electric field (E) is non-zero, and is constant in time, the field is said to be an electrostatic field. Similarly, if only the magnetic field (B) is non-zero and is constant in time, the field is said to be a magnetostatic field. However, if either the electric or magnetic field has a time-dependence, then both fields must be considered together as a coupled electromagnetic field using Maxwell's equations.

Maxwell's equations in the vector field approach[edit]

Main article: Maxwell's equations

The behaviour of electric and magnetic fields, whether in cases of electrostatics, magnetostatics, or electrodynamics (electromagnetic fields), is governed in a vacuum by Maxwell's equations:

Maxwell's equations (vector fields)
\nabla \cdot \mathbf{E} = \frac{\rho}{\varepsilon_0}    Gauss' law
\nabla \cdot \mathbf{B} = 0    Gauss's law for magnetism
\nabla \times \mathbf{E} = -\frac {\partial \mathbf{B}}{\partial t}    Faraday's law
\nabla \times \mathbf{B} = \mu_0 \mathbf{J} + \mu_0\varepsilon_0  \frac{\partial \mathbf{E}}{\partial t}    Ampère–Maxwell law

where ρ is the charge density, which can (and often does) depend on time and position, ε0 is the electric constant, μ0 is the magnetic constant, and J is the current per unit area, also a function of time and position. The units used above are the standard SI units.

Inside a linear material, Maxwell's equations change by switching the permeability and permittivity of free space with the permeability and permittivity of the linear material in question. Inside other materials which possess more complex responses to electromagnetic fields, these properties can be represented by tensors, with time-dependence related to the material's ability to respond to fast field changes (dispersion (optics), Green–Kubo relations), and possibly also field dependencies representing nonlinear and/or nonlocal material responses to large amplitude fields (nonlinear optics).

Potential field approach[edit]

Many times in the use and calculation of electric and magnetic fields, the approach used first computes an associated potential: the electric potential, \varphi, for the electric field, and the magnetic potential, A, for the magnetic field. The electric potential is a scalar field, while the magnetic potential is a vector field. This is why sometimes the electric potential is called the scalar potential and the magnetic potential is called the vector potential. These potentials can be used to find their associated fields as follows:

\mathbf E = - \mathbf \nabla \varphi - \frac{\partial \mathbf A}{\partial t}
\mathbf B = \mathbf \nabla \times \mathbf A

Maxwell's equations in potential formulation[edit]

These relations can be substituted into Maxwell's equations to express the latter in terms of the potentials. Faraday's law and Gauss's law for magnetism reduce to identities (e.g. in the case of Gauss's Law for magnetism, 0 = 0). The other two of Maxwell's equations turn out less simply.

Maxwell's equations (Potential formulation)

\nabla^2 \varphi + \frac{\partial}{\partial t} \left ( \mathbf \nabla \cdot \mathbf A \right ) = - \frac{\rho}{\varepsilon_0}

\left ( \nabla^2 \mathbf A - \frac{1}{c^2} \frac{\partial^2 \mathbf A}{\partial t^2} \right ) - \mathbf \nabla \left ( \mathbf \nabla \cdot \mathbf A + \frac{1}{c^2} \frac{\partial \varphi}{\partial t} \right ) = - \mu_0 \mathbf J

These equations taken together are as powerful and complete as Maxwell's equations. Moreover, the problem has been reduced somewhat, as between the electric and magnetic fields, each had three components which needed to be solved for, meaning it was necessary to solve for six quantities.[1] In the potential formulation, there are only four quantities, the electric potential and the three components of the vector potential. However, this improvement is contrasted with the equations being much messier than Maxwell's equations using just the electric and magnetic fields.

Gauge freedom[edit]

Fortunately, there is a way to simplify these equations that takes advantage of the fact that the potential fields are not what is observed, the electric and magnetic fields are. Thus there is a freedom to impose conditions on the potentials so long as whatever condition is chosen to impose does not affect the resultant electric and magnetic fields. This freedom is called gauge freedom. Specifically for these equations, for any choice of a scalar function of position and time λ, the potentials can be changed as follows:

\mathbf A' = \mathbf A + \mathbf \nabla \lambda
\varphi' = \varphi - \frac{\partial \lambda}{\partial t}

This freedom can be used to greatly simplify the potential formulation. Generally, two such scalar functions are chosen.

Coulomb gauge[edit]

The Coulomb gauge is chosen in such a way that \mathbf \nabla \cdot \mathbf A' = 0, which corresponds to the case of magnetostatics. In terms of λ, this means that it must satisfy the equation

\nabla^2 \lambda = - \mathbf \nabla \cdot \mathbf A.

This choice of function results in the following formulation of Maxwell's equations:

\nabla^2 \varphi' = -\frac{\rho}{\varepsilon_0}
\nabla^2 \mathbf A' - \mu_0 \varepsilon_0 \frac{\partial^2 \mathbf A'}{\partial t^2} = - \mu_0 \mathbf J + \mu_0 \varepsilon_0 \nabla \left ( \frac{\partial \varphi'}{\partial t} \right )

Several features about Maxwell's equations in the Coulomb gauge are as follows. Firstly, solving for the electric potential is very easy, as the equation is a version of Poisson's equation. Secondly, solving for the magnetic vector potential is particularly difficult. This is the big disadvantage of this gauge. The third thing to note, and something which is not immediately obvious, is that the electric potential changes instantly everywhere in response to a change in conditions in one locality.

For instance, if a charge is moved in New York at 1 pm local time, then a hypothetical observer in Australia who could measure the electric potential directly would measure a change in the potential at 1 pm New York time. This seemingly goes against the prohibition in special relativity of sending information, signals, or anything faster than the speed of light. The solution to this apparent problem lies in the fact that, as previously stated, no observers measure the potentials, they measure the electric and magnetic fields. So, the combination of φ and ∂A/∂t used in determining the electric field restores the speed limit imposed by special relativity for the electric field, making all observable quantities consistent with relativity.

Lorenz gauge[edit]

Another gauge (used very often) is the Lorenz gauge. This scalar function λ is chosen such that

\mathbf \nabla \cdot \mathbf A' = - \mu_0 \varepsilon_0 \frac{\partial \varphi'}{\partial t}.

meaning λ must satisfy the equation

\nabla^2 \lambda - \mu_0 \varepsilon_0 \frac{\partial^2 \lambda }{\partial t^2}= - \mathbf \nabla \cdot \mathbf A - \mu_0 \varepsilon_0 \frac{\partial \varphi}{\partial t}.

The Lorenz gauge results in the following form of Maxwell's equations:

\nabla^2 \mathbf A' - \mu_0 \varepsilon_0 \frac{\partial^2 \mathbf A'}{\partial t^2} = \Box^2 \mathbf A' = - \mu_0 \mathbf J
\nabla^2 \varphi' - \mu_0 \varepsilon_0 \frac{\partial^2 \varphi'}{\partial t^2} = \Box^2 \varphi' = - \frac{\rho}{\varepsilon_0}

The operator \Box^2 is called the d'Alembertian (some authors denote by just one square \Box). These equations are inhomogeneous versions of the wave equation, with the terms on the right side of the equation serving as the source functions for the wave. These equations lead to two solutions: advanced potentials (which depend on the configuration of the sources at future points in time), and retarded potentials (which depend on the past configurations of the sources); the former are usually (and sensibly) dismissed as 'non-physical' in favor of the latter, which preserve causality.

As pointed out above, the Lorenz gauge is no more valid than any other gauge, as the potentials themselves are unobservable (with only a few loopholes[clarification needed], such as the Aharonov–Bohm effect, that still leave gauge invariance intact); any violations of causality exhibited by the potentials will vanish for the observable fields, which are the physically meaningful quantities.

Extension to quantum electrodynamics[edit]

Canonical quantization of the electromagnetic fields proceeds by elevating the scalar and vector potentials; φ(x), A(x), from fields to field operators. Substituting 1/c2 = ε0μ0 into the previous Lorenz gauge equations gives:

\nabla^2 \mathbf A - \frac 1 {c^2} \frac{\partial^2 \mathbf A}{\partial t^2} = - \mu_0 \mathbf J
\nabla^2 \varphi - \frac 1 {c^2} \frac{\partial^2 \varphi}{\partial t^2} = - \frac{\rho}{\varepsilon_0}

Here, J and ρ are the current and charge density of the matter field. If the matter field is taken so as to describe the interaction of electromagnetic fields with the Dirac electron given by the four-component Dirac spinor field ψ, the current and charge densities have form:[2]

\mathbf{J}=-e\psi^{\dagger}\boldsymbol{\alpha}\psi\,\quad \rho=-e\psi^{\dagger}\psi \,,

where α are the first three Dirac matrices. Using this, we can re-write Maxwell's equations as:

Maxwell's equations (QED)

\nabla^2 \mathbf A - \frac 1 {c^2} \frac{\partial^2 \mathbf A}{\partial t^2} = \mu_0 e \psi^{\dagger} \boldsymbol{\alpha} \psi

\nabla^2 \varphi - \frac 1 {c^2} \frac{\partial^2 \varphi}{\partial t^2} = \frac{1}{\varepsilon_0} e \psi^{\dagger} \psi

which is the form used in quantum electrodynamics.

Geometric algebra formulations[edit]

Analogous to the tensor formulation, two objects, one for the field and one for the current, are introduced. In geometric algebra (GA) these are multivectors. The field multivector, known as the Riemann–Silberstein vector, is

 \bold{F} = \bold{E} + Ic\bold{B} = E^k\sigma_k + IcB^k\sigma_k

and the current multivector is

 c \rho - \bold{J} = c \rho - J^k\sigma_k

where, in the algebra of physical space (APS) C\ell_{3,0}(\mathbb{R}) with the vector basis \{\sigma_k\}. The unit pseudoscalar is I=\sigma_1\sigma_2\sigma_3 (assuming an orthonormal basis). Orthonormal basis vectors share the algebra of the Pauli matrices, but are usually not equated with them. After defining the derivative

 \boldsymbol{\nabla} = \sigma^k \partial_k

Maxwell's equations are reduced to a single equation,[3]

Maxwell's equations (APS formulation)

 \left(\frac{1}{c}\dfrac{\partial }{\partial t} + \boldsymbol{\nabla}\right)\bold{F} = \mu_0 c (c \rho - \bold{J})

In three dimensions, the derivative has a special structure allowing the introduction of a cross product:

 \boldsymbol{\nabla}\bold{F} = \boldsymbol{\nabla} \cdot \bold{F} + \boldsymbol{\nabla} \wedge \bold{F} = \boldsymbol{\nabla} \cdot \bold{F} + I \boldsymbol{\nabla} \times \bold{F}

from which it is easily seen that Gauss's law is the scalar part, the Ampère–Maxwell law is the vector part, Faraday's law is the pseudovector part, and Gauss's law for magnetism is the pseudoscalar part of the equation. After expanding and rearranging, this can be written as


\left( \boldsymbol{\nabla} \cdot \mathbf{E} - \frac{\rho}{\epsilon_0} \right)- c \left( \boldsymbol{\nabla} \times \mathbf{B} - \mu_0 \epsilon_0 \frac{\partial {\mathbf{E}}}{\partial {t}} - \mu_0 \mathbf{J} \right)+ I \left( \boldsymbol{\nabla} \times \mathbf{E} + \frac{\partial {\mathbf{B}}}{\partial {t}} \right)+ I c \left( \boldsymbol{\nabla} \cdot \mathbf{B} \right)= 0

We can upgrade from APS to spacetime algebra (STA) C\ell_{1,3}(\mathbb{R}) by reassigning \sigma_k=\gamma_k\gamma_0 with unit pseudoscalar I=\gamma_0\gamma_1\gamma_2\gamma_3. The new basis vectors share the algebra of the gamma matrices but like above are usually not equated with them. The derivative is now

\nabla = \gamma^\mu \partial_\mu.

It is customary to leave the Riemann–Silberstein vector as a bivector

F = \bold{E} + Ic\bold{B} = E^k\gamma_k\gamma_0 -c(B^1\gamma_2\gamma_3 + B^2\gamma_3\gamma_1 + B^3\gamma_1\gamma_2),

but to reduce the current to a vector

J = J^\mu \gamma_\mu = c \rho \gamma_0 + J^k \gamma_k = \gamma_0(c \rho - J^k \sigma_k).

Owing to the very simple identity

\gamma_0 \nabla = \gamma_0\gamma^0 \partial_0 + \gamma_0\gamma^k\partial_k = \partial_0 + \sigma^k\partial_k = \frac{1}{c}\dfrac{\partial }{\partial t} + \boldsymbol{\nabla},

all of Maxwell's equations reduce to an even terser single equation:

Maxwell's equations (STA formulation)

 \nabla F = \mu_0 c J

Differential forms approach[edit]

Field 2-form[edit]

In free space, where ε = ε0 and μ = μ0 are constant everywhere, Maxwell's equations simplify considerably once the language of differential geometry and differential forms is used. In what follows, cgs-Gaussian units, not SI units are used. (To convert to SI, see here.) The electric and magnetic fields are now jointly described by a 2-form F in a 4-dimensional spacetime manifold, The Maxwell tensor F_{\mu\nu} can be written as a 2-form in Minkowski space as

 \begin{align}
\bold{F} \equiv & \frac{1}{2}F_{\mu\nu} dx^{\mu} \wedge dx^{\nu} \\
= & B_x dy \wedge dz + B_y dz \wedge dx + B_z dx \wedge dy + E_x dx \wedge dt + E_y dy \wedge dt + E_z dz \wedge dt
\end{align}

which, as the curvature form, is the exterior derivative of the electromagnetic four-potential,

 \bold{F} = \mathrm{d} \bold{A} = ( \partial_{\mu}  A_{\nu} ) dx^{\mu} \wedge dx^{\nu}

The source free equations can be written by the action of the exterior derivative on this 2-form. But for the equations with source terms (Gauss's law and the Ampère-Maxwell equation), the Hodge dual of this 2-form is needed. The Hodge 'star' dual takes a p-form to a dp form, where d is the number of dimensions. Here, it takes the 2-form (F) and gives another 2-form (in four dimensions, dp = 4 − 2 = 2). For the basis cotangent vectors, the Hodge dual is given as (see here)

 {\star dx} \wedge dy = - dz \wedge dt ,\quad {\star dx} \wedge dt = dy \wedge dz,

and so on. Using these relations, the dual of Maxwell 2-form is


{\star \bold{F}} = - B_x dx \wedge dt - B_y dy \wedge dt - B_z dz \wedge dt + E_x dy \wedge dz + E_y dz \wedge dx + E_z dx \wedge dy

Current 3-form, dual current 1-form[edit]

Here, the 3-form J is called the electric current form or current 3-form:

 
\bold{J} = \rho dx \wedge dy \wedge dz - j_x dt \wedge dy \wedge dz - j_y dt \wedge dz \wedge dx - j_z dt \wedge dx \wedge dy

with the corresponding dual 1-form:

 
{\star \bold{J}} = -\rho dt + j_x dx + j_y dy + j_z dz

Maxwell's equations then reduce to the Bianchi identity and the source equation, respectively:

Maxwell's equations (current 3-form)

\mathrm{d}\bold{F}=0

\mathrm{d}\,{\star\bold{F}}=\bold{J}

where d denotes the exterior derivative — a natural coordinate and metric independent differential operator acting on forms, and the (dual) Hodge star operator \star is a linear transformation from the space of 2-forms to the space of (4−2)-forms defined by the metric in Minkowski space (in four dimensions even by any metric conformal to this metric). The fields are in natural units where 1/4πε0 = 1.

Since d2 = 0, the 3-form J satisfies the continuity equation:

\mathrm{d}{\bold{J}}=0.

The current 3-form can be integrated over a 3-dimensional space-time region. The physical interpretation of this integral is the charge in that region if it is spacelike, or the amount of charge that flows through a surface in a certain amount of time if that region is a spacelike surface cross a timelike interval. As the exterior derivative is defined on any manifold, the differential form version of the Bianchi identity makes sense for any 4-dimensional manifold, whereas the source equation is defined if the manifold is oriented and has a Lorentz metric. In particular the differential form version of the Maxwell equations are a convenient and intuitive formulation of the Maxwell equations in general relativity.

Linear macroscopic influence of matter[edit]

In a linear, macroscopic theory, the influence of matter on the electromagnetic field is described through more general linear transformation in the space of 2-forms. We call

 C:\Lambda^2\ni\bold{F}\mapsto \bold{G}\in\Lambda^{(4-2)}

the constitutive transformation. The role of this transformation is comparable to the Hodge duality transformation. The Maxwell equations in the presence of matter then become:

 \mathrm{d}\bold{F} = 0
 \mathrm{d}\bold{G} = \bold{J}

where the current 3-form J still satisfies the continuity equation dJ = 0.

When the fields are expressed as linear combinations (of exterior products) of basis forms θp,

 \bold{F} = \frac{1}{2}F_{pq}\bold{\theta}^p\wedge\bold{\theta}^q.

the constitutive relation takes the form

 G_{pq} = C_{pq}^{mn}F_{mn}

where the field coefficient functions are antisymmetric in the indices and the constitutive coefficients are antisymmetric in the corresponding pairs. In particular, the Hodge duality transformation leading to the vacuum equations discussed above are obtained by taking

 C_{pq}^{mn} = \frac{1}{2}g^{ma}g^{nb} \epsilon_{abpq} \sqrt{-g}

which up to scaling is the only invariant tensor of this type that can be defined with the metric.

In this formulation, electromagnetism generalises immediately to any 4-dimensional oriented manifold or with small adaptations any manifold, requiring not even a metric.

Current 1-form, dual current 3-form[edit]

In the literature, the current is usually defined as a 1-form (i.e. the hodge dual of the 3-form J above):

 
\bold{J} = -\rho dt + j_x dx + j_y dy + j_z dz

with the corresponding dual 3-form:


{\star \bold{J}} = \rho dx \wedge dy \wedge dz - j_x dt \wedge dy \wedge dz - j_y dt \wedge dz \wedge dx - j_z dt \wedge dx \wedge dy

In terms of these forms, the Maxwell equations are:[4]

Maxwell's equations (current 1-form)

\mathrm{d}\bold{F}=0

\mathrm{d}\,{\star \bold{F}} = {\star \bold{J}}

The conservation of current (continuity equation) simply follows from the property of exterior derivative that d2 = 0 (exterior derivative).

 \mathrm{d}\,{\star \bold{J}} = \mathrm{d}^2\,{\star \bold{F}} = 0

which is the conservation of current.

Curved spacetime[edit]

Traditional formulation[edit]

Matter and energy generate curvature of spacetime. This is the subject of general relativity. Curvature of spacetime affects electrodynamics. An electromagnetic field having energy and momentum also generates curvature in spacetime. Maxwell's equations in curved spacetime can be obtained by replacing the derivatives in the equations in flat spacetime with covariant derivatives. (Whether this is the appropriate generalization requires separate investigation.) The sourced and source-free equations become (cgs-Gaussian units):

 { 4 \pi \over c   }j^{\beta} = \partial_{\alpha} F^{\alpha\beta} + {\Gamma^{\alpha}}_{\mu\alpha} F^{\mu\beta} + {\Gamma^{\beta}}_{\mu\alpha} F^{\alpha \mu} \ \stackrel{\mathrm{def}}{=}\  \nabla_{\alpha} F^{\alpha\beta} \ \stackrel{\mathrm{def}}{=}\  {F^{\alpha\beta}}_{;\alpha} \, \!

and

0 = \partial_{\gamma} F_{\alpha\beta} + \partial_{\beta} F_{\gamma\alpha} + \partial_{\alpha} F_{\beta\gamma} = \nabla_{\gamma} F_{\alpha\beta} + \nabla_{\beta} F_{\gamma\alpha} + \nabla_{\alpha} F_{\beta\gamma}.\,

Here,

{\Gamma^{\alpha}}_{\mu\beta} \!

is a Christoffel symbol that characterizes the curvature of spacetime and ∇α is the covariant derivative.

Formulation in terms of differential forms[edit]

The formulation of the Maxwell equations in terms of differential forms can be used without change in general relativity. The equivalence of the more traditional general relativistic formulation using the covariant derivative with the differential form formulation can be seen as follows. Choose local coordinates xα which gives a basis of 1-forms dxα in every point of the open set where the coordinates are defined. Using this basis and cgs-Gaussian units we define

  • The antisymmetric infinitesimal field tensor Fαβ, corresponding to the field 2-form F
 \bold{F} = \frac{1}{2}F_{\alpha\beta} \,\mathrm{d}\,x^{\alpha} \wedge \mathrm{d}\,x^{\beta}.
  • The current-vector infinitesimal 3-form J
 \bold{J} = {4 \pi \over c } \left ( \frac{1}{6} j^{\alpha} \sqrt{-g} \, \epsilon_{\alpha\beta\gamma\delta} \mathrm{d}\,x^{\beta} \wedge \mathrm{d}\,x^{\gamma} \wedge \mathrm{d}\,x^{\delta}. \right)

The epsilon tensor contracted with the differential 3-form produces 6 times the number of terms required.

Here g is as usual the determinant of the metric tensor gαβ. A small computation that uses the symmetry of the Christoffel symbols (i.e., the torsion-freeness of the Levi-Civita connection) and the covariant constantness of the Hodge star operator then shows that in this coordinate neighborhood we have:

  • the Bianchi identity
 \mathrm{d}\bold{F} = 2(\partial_{\gamma} F_{\alpha\beta} + \partial_{\beta} F_{\gamma\alpha} + \partial_{\alpha} F_{\beta\gamma})\mathrm{d}\,x^{\alpha}\wedge \mathrm{d}\,x^{\beta} \wedge \mathrm{d}\,x^{\gamma} = 0,
  • the source equation
 \mathrm{d}\,{\star \bold{F}} = \frac{1}{6}{F^{\alpha\beta}}_{;\alpha}\sqrt{-g} \, \epsilon_{\beta\gamma\delta\eta}\mathrm{d}\,x^{\gamma} \wedge \mathrm{d}\,x^{\delta} \wedge \mathrm{d}\,x^{\eta} = \bold{J},
  • the continuity equation
 \mathrm{d}\bold{J} = { 4 \pi \over c } {j^{\alpha}}_{;\alpha} \sqrt{-g} \, \epsilon_{\alpha\beta\gamma\delta}\mathrm{d}\,x^{\alpha}\wedge \mathrm{d}\,x^{\beta} \wedge \mathrm{d}\,x^{\gamma} \wedge \mathrm{d}\,x^{\delta} = 0.

Classical electrodynamics as the curvature of a line bundle[edit]

An elegant and intuitive way to formulate Maxwell's equations is to use complex line bundles or principal bundles with fibre U(1). The connection ∇ on the line bundle has a curvature F = ∇2 which is a two-form that automatically satisfies dF = 0 and can be interpreted as a field-strength. If the line bundle is trivial with flat reference connection d we can write ∇ = d + A and F = dA with A the 1-form composed of the electric potential and the magnetic vector potential.

In quantum mechanics, the connection itself is used to define the dynamics of the system. This formulation allows a natural description of the Aharonov–Bohm effect. In this experiment, a static magnetic field runs through a long magnetic wire (e.g., an iron wire magnetized longitudinally). Outside of this wire the magnetic induction is zero, in contrast to the vector potential, which essentially depends on the magnetic flux through the cross-section of the wire and does not vanish outside. Since there is no electric field either, the Maxwell tensor F = 0 throughout the space-time region outside the tube, during the experiment. This means by definition that the connection ∇ is flat there.

However, as mentioned, the connection depends on the magnetic field through the tube since the holonomy along a non-contractible curve encircling the tube is the magnetic flux through the tube in the proper units. This can be detected quantum-mechanically with a double-slit electron diffraction experiment on an electron wave traveling around the tube. The holonomy corresponds to an extra phase shift, which leads to a shift in the diffraction pattern.[5][6]

Discussion[edit]

Following are the reasons for using each of such formulations.

Potential formulation[edit]

In advanced classical mechanics it is often useful, and in quantum mechanics frequently essential, to express Maxwell's equations in a potential formulation involving the electric potential (also called scalar potential) φ, and the magnetic potential (also called vector potential) A. For example, the analysis of radio antennas makes full use of Maxwell's vector and scalar potentials to separate the variables, a common technique used in formulating the solutions of differential equations. The potentials can be introduced by using the Poincaré lemma on the homogeneous equations to solve them in a universal way (this assumes that we consider a topologically simple, e.g. contractible space). The potentials are defined as in the table above. Alternatively, these equations define E and B in terms of the electric and magnetic potentials which then satisfy the homogeneous equations for E and B as identities. Substitution gives the non-homogeneous Maxwell equations in potential form.

Many different choices of A and φ are consistent with given observable electric and magnetic fields E and B, so the potentials seem to contain more, (classically) unobservable information. The non uniqueness of the potentials is well understood, however. For every scalar function of position and time λ(x, t), the potentials can be changed by a gauge transformation as

\varphi' = \varphi - \frac{\partial \lambda}{\partial t}, \quad \mathbf A' = \mathbf A + \mathbf \nabla \lambda

without changing the electric and magnetic field. Two pairs of gauge transformed potentials (φ, A) and (φ′, A′) are called gauge equivalent, and the freedom to select any pair of potentials in its gauge equivalence class is called gauge freedom. Again by the Poincaré lemma (and under its assumptions), gauge freedom is the only source of indeterminacy, so the field formulation is equivalent to the potential formulation if we consider the potential equations as equations for gauge equivalence classes.

The potential equations can be simplified using a procedure called gauge fixing. Since the potentials are only defined up to gauge equivalence, we are free to impose additional equations on the potentials, as long as for every pair of potentials there is a gauge equivalent pair that satisfies the additional equations (i.e. if the gauge fixing equations define a slice to the gauge action). The gauge-fixed potentials still have a gauge freedom under all gauge transformations that leave the gauge fixing equations invariant. Inspection of the potential equations suggests two natural choices. In the Coulomb gauge, we impose \mathbf \nabla \cdot \mathbf A = 0 which is mostly used in the case of magneto statics when we can neglect the c−22A/∂t2 term. In the Lorenz gauge (named after the Dane Ludvig Lorenz), we impose

\mathbf \nabla \cdot \mathbf A + \frac{1}{c^2} \frac{\partial \varphi}{\partial t} = 0\,.

The Lorenz gauge condition has the advantage of being Lorentz invariant and leading to Lorentz-invariant equations for the potentials.

Manifestly covariant (tensor) approach[edit]

Maxwell's equations are exactly consistent with special relativity—i.e., if they are valid in one inertial reference frame, then they are automatically valid in every other inertial reference frame. In fact, Maxwell's equations were crucial in the historical development of special relativity. However, in the usual formulation of Maxwell's equations, their consistency with special relativity is not obvious; it can only be proven by a laborious calculation.

For example, consider a conductor moving in the field of a magnet.[7] In the frame of the magnet, that conductor experiences a magnetic force. But in the frame of a conductor moving relative to the magnet, the conductor experiences a force due to an electric field. The motion is exactly consistent in these two different reference frames, but it mathematically arises in quite different ways.

For this reason and others, it is often useful to rewrite Maxwell's equations in a way that is "manifestly covariant"—i.e. obviously consistent with special relativity, even with just a glance at the equations—using covariant and contravariant four-vectors and tensors. This can be done using the EM tensor F, or the 4-potential A, with the 4-current J – see covariant formulation of classical electromagnetism.

Differential forms approach[edit]

Gauss's law for magnetism and the Faraday–Maxwell law can be grouped together since the equations are homogeneous, and be seen as geometric identities expressing the field F (a 2-form), which can be derived from the 4-potential A. Gauss's law for electricity and the Ampere–Maxwell law could be seen as the dynamical equations of motion of the fields, obtained via the Lagrangian principle of least action, from the "interaction term" A J (introduced through gauge covariant derivatives), coupling the field to matter. For the field formulation of Maxwell's equations in terms of a principle of extremal action, see electromagnetic tensor.

Often, the time derivative in the Faraday–Maxwell equation motivates calling this equation "dynamical", which is somewhat misleading in the sense of the preceding analysis. This is rather an artifact of breaking relativistic covariance by choosing a preferred time direction. To have physical degrees of freedom propagated by these field equations, one must include a kinetic term F *F for A, and take into account the non-physical degrees of freedom which can be removed by gauge transformation AA' = A − dα. See also gauge fixing and Faddeev–Popov ghosts.

Geometric calculus approach[edit]

This formulation is structured on the algebra that spacetime generates through the introduction of a distributive, associative (but not commutative) product called the geometric product. Every element and every operation within the algebra has geometric meaning. The members of the algebra carry a grade (as in the formalism of differential forms) and the (geometric) product of a vector with a k-vector can always be decomposed into a (k-1)-vector and a (k+1)-vector. The grade-lowering product can be identified with the inner product and the grade-raising product as the outer product. Of great importance is the fact that the geometric product is invertible while the inner and outer products are not. The derivatives that appear in Maxwell's equations are vectors and Electromagnetic fields are represented by the Faraday bivector F. This formulation is more general than that of differential forms as one can construct a unique r-vector which yields a quantity which has al the properties of a differential form. The description is more general in many senses and all results of differential forms can be reproduced. In the light of this formulation one can identify that the dynamics of electromagnetic fields is given by one equation, Maxwell's equation. This equation can be separated into parts as is done above for comparative reasons.

References and notes[edit]

  1. ^ Introduction to Electrodynamics by Griffiths
  2. ^ Quantum Electrodynamics, Mathworld
  3. ^ Oersted Medal Lecture David Hestenes "Reforming the Mathematical Language of Physics" (Am. J. Phys. 71 (2), February 2003, pp. 104–121) Online:http://geocalc.clas.asu.edu/html/Oersted-ReformingTheLanguage.html p26
  4. ^ Misner, Charles W.; Thorne, Kip; Wheeler, John Archibald (1973). Gravitation. W. H. Freeman. p. 81. ISBN 0-7167-0344-0. 
  5. ^ M. Murray (5 September 2008). "Line Bundles. Honours 1996". University of Adelaide. Retrieved 2010-11-19. 
  6. ^ R. Bott (1985). "On some recent interactions between mathematics and physics". Canadian Mathematical Bulletin 28 (2): 129–164. doi:10.4153/CMB-1985-016-3. 
  7. ^ Albert Einstein (1905) On the electrodynamics of moving bodies

See also[edit]