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Riemann–Silberstein vector

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Riemann–Silberstein vector

In mathematical physics, in particular electromagnetism, the Riemann–Silberstein vector, named after Bernhard Riemann and Ludwik Silberstein, (or sometimes ambiguously called the "electromagnetic field") is a complex vector that combines the electric field E and the magnetic field B.[1][2]

Definition

Given an electric field E and a magnetic field B defined on a common region of spacetime, the Riemann–Silberstein vector is

\mathbf{F} = \mathbf{E} + ic \mathbf{B}

where c is the speed of light, with some authors preferring to multiply the right hand side by an overall constant \sqrt{\epsilon_0 / 2} where ε0 is the permittivity of free space. It is analogous to the electromagnetic tensor F, a 2-vector used in the covariant formulation of classical electromagnetism.

In Silberstein's formulation, i was defined as the imaginary unit, and F was defined as a complexified 3-dimensional vector field. The value of F at an event was a bivector.[3]

Application

Bernhard Riemann used \mathfrak{E} + i\ \mathfrak{M} to illustrate consolidation of Maxwell’s equations. According to lectures published by Heinrich Martin Weber in 1901, the real and imaginary components of the equation

\operatorname{curl}(\mathfrak{E} + i\ \mathfrak{M}) = \frac{i}{c}\ \frac {\partial (\mathfrak{E} + i\ \mathfrak{M})} {\partial t}

are an interpretation of Maxwell’s equations without charges or currents. Riemann’s lectures are available on-line from University of Michigan Historical Math Collection in Weber’s book, §138, S. 348, under the title Zusammenziehung der Maxwell’schen Gleichungen (Consolidation of Maxwell’s Equations).

The Riemann–Silberstein vector is used as a point of reference in the geometric algebra formulation of electromagnetism. Maxwell's four equations in vector calculus reduce to one equation in the algebra of physical space:

\left(\frac{1}{c}\dfrac{\partial }{\partial t} + \boldsymbol{\nabla}\right)\mathbf{F} = \frac{1}{\epsilon_0}\left( \rho - \frac{1}{c}\mathbf{J} \right).

Expressions for the fundamental invariants and the energy density and momentum density also take on simple forms:

\mathbf{F}^2 = \mathbf{E}^2 - c^2\mathbf{B}^2 + 2 i c\mathbf{E} \cdot \mathbf{B}
\frac{\epsilon_0}{2}\mathbf{F}^{\dagger}\mathbf{F} = \frac{\epsilon_0}{2}\left( \mathbf{E}^2 + c^2\mathbf{B}^2 \right) + \frac{1}{c} \mathbf{S},

where S is the Poynting vector.

The Riemann–Silberstein vector is used for an exact matrix representations of Maxwell's equations in an inhohogeneous medium with sources.[4][5]

Photon wave function

In 1996 contribution to quantum electrodynamics, Iwo Bialynicki-Birula used the Riemann–Silberstein vector as the basis for an approach to the photon, noting that it is a "complex vector-function of space coordinates r and time t that adequately describes the quantum state of a single photon". To put the Riemann–Silberstein vector in contemporary parlance, a transition is made:

With the advent of spinor calculus that superseded the quaternionic calculus, the transformation properties of the Riemann-Silberstein vector have become even more transparent ... a symmetric second-rank spinor.

Bialynicki-Birula acknowledges that the photon wave function is a controversial concept and that it cannot have all the properties of Schrödinger wave functions of non-relativistic wave mechanics. Yet defense is mounted on the basis of practicality: describing quantum states of excitation of a free field, electromagnetic fields acting on a medium, vacuum excitation of virtual positron-electron pairs, and to present the photon among quantum particles that do have wave functions.

Schrödinger equation for the photon and the Heisenberg uncertainty relations

Mulitplying the two time dependent Maxwell equations by \hbar the Schrödinger equation for photon in the vacuum is given by

i \hbar \partial_{t} {\mathbf F}=c (\mathbf S \cdot {\hbar \over i} \nabla) \mathbf F = c (\mathbf S \cdot \mathbf p ) \mathbf F

where {\mathbf S} is the vector built from the spin of the length 1 matrices generating full infinitesimal rotations of 3-spinor particle. One may therefore notice that the Hamiltonian in the Schrödinger equation of the photon is the projection of its spin 1 onto its momentum since the normal momentum operator appears there from combining parts of rotations.

In contrast to the electron wave function the modulus square of the wave function of the photon (Riemann-Silbertein vector) is not dimensionless and must be multiplied by the "local photon wavelength" with the proper power to give dimensionless expression to normalize i.e. it is normalized in the exotic way with the integral kernel

\|\mathbf F\|={1 \over \hbar c}\int {\mathbf F^*(x) \cdot \mathbf F(x') \over |x-x'|^2}dx^3 dx'^3=1

The two residual Maxwell equations are only constraints i.e.

\nabla \cdot \mathbf F=0

and the are automatically fullfiled all time if only fulfilled at the initial time t=0, i.e.

\mathbf F(0)= \nabla \times \mathbf G

where \mathbf G is any complex vector field with the non-vanishing rotation, or it is a vector potential for the Riemann–Silberstein vector.

While having the wave function of the photon one can estimate the uncertainty relations for the photon.[6] It shows up that photons are "more quantum" than the electron while their uncertainties of position and the momentum are higher. The natural candidates to estimate the uncertainty are the natural momentum like simply the projection E/c or H/c from Einstein formula for the photoelectric effect and the simplest theory of quanta and the r, the uncertainty of the position length vector.

We will use the general relation for the uncertainty for the operators A, B

\sigma_{A}\sigma_{B} \geq \frac{1}{2}\left|\langle[\hat{A},\hat{B}]\rangle \right|.

We want the uncertainty relation for \sigma_{r}\sigma_{p} i.e. for the operators

r^2=x^2+y^2+z^2
p^2=(\mathbf S \cdot \mathbf p )^2

The first step is to find the auxiliary operator \tilde r such that this relation can be used directly. First we make the same trick for r that Dirac made to calculate the square root of the Klein-Gordon operator to get the Dirac equation:

\tilde r = \alpha_1 x + \alpha_2 y + \alpha_3 z

where \alpha_i are matrices from the Dirac equation:

\alpha_i^2=1
\alpha_i \alpha_k + \alpha_k \alpha_i= 2 \delta_{ik}

Therefore we have

\tilde r^2 = r^2

Because the spin matrices 1 are only 3 \times 3 to calculate the commutator in the same space we approximate the spin matrices by angular momentum matrices of the particle with the length 3/2 \approx 1 while dropping the multiplying 1/2 since the resulting Maxwell equations in 4 dimensions would look too artificial to the original (alternatively we can keep the original 1/2 factors but normalize the new 4-spinor to 2 as 4 scalar particles normalized to 1/2):

\tilde p^2 = (\mathbf \tilde L \cdot \mathbf p)^2

We can now readily calculate the commutator while calculating commutators of \alpha_i matrixes and scaled \tilde L_i and noticing that the symmetric Gaussian state e^{-a r^2} is annihilating in average the terms containing mixed variable like x p_y Calculating 9 commutators (mixed may be zero by Gaussian example and the L_z \alpha_z=\alpha_z L_z=0 since those matrices are counter-diagonal) and estimating terms from the norm of the resulting 4 \times 4 matrix containing four 2\sqrt 3 factors giving square of the most natural L2, 1 norm of this matrix as 48 \approx 49=7^2 \approx 8^2 and using the norm inequality for the estimate

||\mathbf A \mathbf x|| \leq ||\mathbf A|| ||\mathbf x|| \approx ||\mathbf A|| ||\mathbf x||

we obtain

\left|\langle[\tilde r,\tilde p]\rangle \right|\geq 8 \hbar .

or

\sigma_{r}\sigma_{p}\geq 4 \hbar

which is much more then for the mass particle in 3 dimensions that is

\sigma_{r}\sigma_{p}\geq \frac{3}{2}\hbar

and therefore photons turn out to be particles 8/3 times or almost 3 times "more quantum" than particles with the mass like electrons.

References

  1. ^ Silberstein, Ludwik (1907). "Elektromagnetische Grundgleichungen in bivectorieller Behandlung".  
  2. ^ Silberstein, Ludwik (1907). "'"Nachtrag zur Abhandlung über 'Elektromagnetische Grundgleichungen in bivectorieller Behandlung.  
  3. ^ Aste, Andreas (2012). "Complex representation theory of the electromagnetic field".  
  4. ^ Bialynicki-Birula, Iwo (1996). "Photon wave function".  
  5. ^ Khan, Sameen Ahmed (2005). "An Exact Matrix Representation of Maxwell's Equations".  
  6. ^ Bialynicki-Birula, Iwo (2012). "Uncertainty Relation for Photon". Phys. Rev. Lett. 108: 140401–1–5. - This publication is using slightly different definitions of position and momentum uncertainties resigning from the position operator and normalizing uncertainty of r^2 to uncertainty of r

Further reading

  • Heinrich Martin Weber (1901) Die partiellen Differential-Gleichungen der mathematischen Physik nach Riemann's Vorlesungen, S. 348, Braunscheweig: Friedrich Vieweg und Sohn, available from University of Michigan Historical Math Collection.
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