Justin Dressel
Schmid College of Science and Technology
Institute for Quantum Studies
Chapman University
Advances in Operator Theory
with Applications to Mathematical Physics
November 12-16, 2018, Chapman U, Orange CA
Minkowski Space \(\mathcal{M}_{1,3}(\mathbb{R})\) :
Minkowski metric
(symmetric bilinear form)
Algebraic Axioms: \(a,b,c\in\mathcal{M}_{1,3}(\mathbb{R})\)
Axioms constructively define Clifford algebra \( \text{Cl}_{1,3}(\mathbb{R}) \)
Symmetric part of product encodes metric:
Anti-symmetric part is Grassman wedge product:
(others zero)
Grade
0
1
2
3
4
Bivector Planes (of rotation):
3 hyperbolic | 3 elliptic
Vector Lines (of translation):
1 timelike | 3 spacelike
Scalar Points
Pseudovector Volumes:
1 spacelike | 3 timelike
Pseudoscalar 4-Volumes
Multivector: \( M = \langle M \rangle_0 + \langle M \rangle_1 + \langle M \rangle_2 + \langle M \rangle_3 + \langle M \rangle_4 \)
0
1
2
3
(Spacetime-aware "imaginary unit" is the unit pseudoscalar: \(I^2 = -1\))
(commutes with even grade, anti-commutes with odd grade)
4
Relative 3D space embedded as even-graded subspace:
\( \text{Cl}_{3,0}(\mathbb{R}) \)
Complexified 3-vector algebra is equivalent to this relative 3D Clifford algebra since \(I\) commutes with even grades
(Observed spatial directions in reference frame)
(Space axis dragged along temporal worldline)
Note duality transformation of left multiplication by \(-I\) : Hodge star operation
Multivector: \( M = [\alpha + (v_0 + \vec{v})\gamma_0 + \vec{A}] + I[\vec{B} + (w_0 + \vec{w})\gamma_0 + \beta] \)
Proper Form of Multivector:
\( M = \alpha + v + \mathbf{F} + Iw + I\beta = (\alpha + I\beta) + (v + Iw) + \mathbf{F} \)
Relative Frame Form of Multivector:
\( M = \alpha + (v_0 + \vec{v})\gamma_0 + (\vec{A} + I\vec{B}) + I(w_0 + \vec{w})\gamma_0 + I\beta \)
Components:
complex scalar
complex vector
bivector
scalar
polar paravector
polar vector
axial vector
axial paravector
pseudoscalar
4-vector
scalar
bivector
pseudovector
pseudoscalar
4-vector components, or a scalar and a relative 3-vector
rank-2 antisymmetric tensor components, or a pair of 3-vectors (one polar, one axial)
Multivector field: (in tangent algebra at point \(x\) of manifold)
\( M(x) = \alpha(x) + v(x) + \mathbf{F}(x) + Iw(x) + I\beta(x) \)
Vector derivative (Dirac operator):
\( \displaystyle \vec{\nabla} \equiv \sum_k \vec{\sigma}^k \frac{\partial}{\partial x^k} \) ; \( \vec{\nabla}\vec{v} = \vec{\nabla}\cdot\vec{v} + \vec{\nabla} \wedge \vec{v} = \vec{\nabla}\cdot\vec{v} + (\vec{\nabla}\times \vec{v})I \) (contains divergence and curl)
\(\nabla^2 = \nabla\gamma_0^2\nabla = (\partial_{ct} - \vec{\nabla})(\partial_{ct} + \vec{\nabla}) = \partial^2_{ct} - \vec{\nabla}\cdot\vec{\nabla} = \Box \) (d'Alembertian)
EM is naturally a bivector field
electric charge
density and current
This is Maxwell's Equation
Electromagnetic field bivector:
Same form as complex (Riemann-Silberstein) 3-vector
Electromagnetic source complex vector:
magnetic charge
density and current
Contains all of the usual 3D Maxwell's Equations, permitting both electric and magnetic charges
Usual Lagrangian density for field
"axion" contribution to Lagrangian
Only possible Lorentz-invariant scalars
Note that a global phase degeneracy appears for a "null field" with zero magnitude
Even though null fields have global phase degeneracy, their local phases must be connected in order to satisfy Maxwell's equation, which breaks the phase symmetry
Consider field with constant amplitude:
For phase and amplitude to both be nonzero, they must be noninvertible and therefore null
Since \(\mathbf{f}\) is constant, \(\nabla \phi\) must also be constant, which forces the linear solution :
\(\phi(x) = \phi_0 \pm k\cdot x \) with null wavevector \( k = \nabla \phi \),
as well as the decomposition \(\mathbf{f} = s\wedge k = -k\wedge s \) for some constant spacelike vector \(s\) s.t. \(s\cdot k = 0\)
Since the global phase is arbitrary, we choose \(\phi_0 = 0\) to find the plane-wave solutions:
\( \mathbf{F}(x) = sk\,e^{\pm I k\cdot x} \)
Writing out the directional null factor \(k = (\omega/c)\gamma_0(1 - \vec{k}/|\vec{k}|)\) and \(s = \vec{E}\gamma_0 \), this solution expands to:
\( \mathbf{F}(t,\vec{x}) = [\vec{E} \cos(\vec{k}\cdot\vec{x} - \omega t) \mp \hat{k}\times\vec{E} \sin(\vec{k}\cdot\vec{x} - \omega t)] + [\vec{E} \sin(\vec{k}\cdot\vec{x}-\omega t) \pm \hat{k}\times\vec{E} \cos(\vec{k}\cdot{x} - \omega t)]I \)
These are circularly polarized (constant helicity) electromagnetic plane wave modes.
Complete EM dynamics:
A hidden gauge symmetry is now evident:
The pseudoscalar \(I\) generates phase rotations in the usual way:
this has the effect of swapping the electromagnetic fields and source charges
Physics is the same provided that both source and field definitions are changed in tandem
Can always choose \(\phi\) to make all charges electric (\(j'_m = 0\))
Vacuum fields (\(j = 0\)) always have this field-exchange symmetry
Postulate vector potential:
Must be complex field to satisfy dual symmetry
Lorenz-Fitzgerald conditions assumed
Relative EM fields regain apparent symmetry in definitions
Obvious wave equation
Proper force law:
Charge must be complex to admit dual symmetry
Relative force law:
Rate of work performed (c=1)
Relative Lorentz force, including magnetic charge
A new gauge symmetry leads to an independently conserved quantity : certainly conserved in vacuum
Helicity Pseudocurrent (tensor) is newly conserved
Spin-density vector is the helicity flux density
Scalar helicity density
These definitions only make sense when full dual-symmetric fields are used
They match postulated definitions of these quantities in the constrained case with \( \mathbf{F} = \mathbf{F}I \)
Thank you!
JD, et al. Physics Reports 589 1-71 (2015)