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First-Order Maxwell Operator Formalism

Updated 18 July 2026
  • First-order Maxwell operator formalism redefines Maxwell’s equations as a first-order system using varied field multiplets to enhance analysis of gauge invariance and spectral properties.
  • Different representations—including Palatini-like, Newman–Penrose, and DKP-type—enable precise treatment of boundary conditions, energy conservation, and asymptotic behavior.
  • Applications range from macroscopic QED and cylindrical waveguides to curved spacetime, offering tractable evolution equations and explicit spectral decompositions.

First-order Maxwell operator formalism denotes a family of representations in which Maxwell theory is written as a first-order system on an enlarged field space rather than exclusively as a second-order wave equation. In these representations the fundamental variable may be a complex electromagnetic six-vector, a pair (A,F)(A,F) of potential and field strength, a null-frame multiplet (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T, or a Duffin–Kemmer–Petiau-type wavefunction, and the operator may be realized as a self-adjoint generator, a covariant constraint map, or a resolvent-based propagator (Nittis et al., 2017, Pietrzyk et al., 2022, Xiao et al., 16 Feb 2026, Kruglov, 2010, Agarwal et al., 29 Mar 2026). The common objective is to retain the first-order differential structure of Maxwell’s equations while making gauge invariance, spectral theory, asymptotics, conserved quantities, boundary data, or quantization more transparent.

1. Core operator reformulations

A central pattern is the replacement of the real-field Maxwell system by a complex first-order evolution equation. In linear, dispersionless media with

W(x)=(εχ χμ)(x),W(x)=\begin{pmatrix}\varepsilon&\chi\ \chi^*&\mu\end{pmatrix}(x),

the dynamical equations can be written as

$W \partial_t\Psi_{\mathrm{phys}}=\mathrm{Rot}\,\Psi_{\mathrm{phys}}-J_{\mathrm{phys}}, \qquad \mathrm{Rot}:=\begin{pmatrix}0&i\nabla\times\-i\nabla\times&0\end{pmatrix},$

and, after complexification and restriction to nonnegative frequencies,

itΨ(t)=MΨ(t)iJ(t),M=W1Rotω0,i\,\partial_t\Psi(t)=M\Psi(t)-i\,J(t),\qquad M=W^{-1}\,\mathrm{Rot}\big|_{\omega\ge 0},

with (E,H)=2ReΨ(\mathbf E,\mathbf H)=2\,\mathrm{Re}\,\Psi (Nittis et al., 2017). In the covariant Palatini-like formulation, the first-order operator is instead the map

M:(A,F)(dAF,δF),\mathcal M:(A,F)\longmapsto (dA-F,\delta F),

so that dAF=0dA-F=0 encodes the definition of FF and δF=0\delta F=0 encodes Maxwell’s equations (Pietrzyk et al., 2022). In frequency-domain macroscopic QED, the dual field

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T0

obeys

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T1

with (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T2 and (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T3 (Agarwal et al., 29 Mar 2026).

Setting Field multiplet First-order equation
Linear media (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T4 (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T5
Covariant Palatini-like form (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T6 (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T7
Null-tetrad form (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T8 (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T9
Macroscopic QED W(x)=(εχ χμ)(x),W(x)=\begin{pmatrix}\varepsilon&\chi\ \chi^*&\mu\end{pmatrix}(x),0 W(x)=(εχ χμ)(x),W(x)=\begin{pmatrix}\varepsilon&\chi\ \chi^*&\mu\end{pmatrix}(x),1

These constructions differ in state space, boundary conditions, and interpretation, but they all preserve the first-order character of the field equations. This suggests that the phrase “first-order Maxwell operator” refers not to a unique canonical matrix but to a structural class of formulations adapted to different analytical tasks.

2. Newman–Penrose null-tetrad operator

A differential-form and Newman–Penrose (NP) formulation expresses Maxwell theory in terms of the gauge potential W(x)=(εχ χμ)(x),W(x)=\begin{pmatrix}\varepsilon&\chi\ \chi^*&\mu\end{pmatrix}(x),2, the Faraday 2-form

W(x)=(εχ χμ)(x),W(x)=\begin{pmatrix}\varepsilon&\chi\ \chi^*&\mu\end{pmatrix}(x),3

and its Hodge dual

W(x)=(εχ χμ)(x),W(x)=\begin{pmatrix}\varepsilon&\chi\ \chi^*&\mu\end{pmatrix}(x),4

with W(x)=(εχ χμ)(x),W(x)=\begin{pmatrix}\varepsilon&\chi\ \chi^*&\mu\end{pmatrix}(x),5 and W(x)=(εχ χμ)(x),W(x)=\begin{pmatrix}\varepsilon&\chi\ \chi^*&\mu\end{pmatrix}(x),6. Gauge invariance is immediate from W(x)=(εχ χμ)(x),W(x)=\begin{pmatrix}\varepsilon&\chi\ \chi^*&\mu\end{pmatrix}(x),7 (Xiao et al., 16 Feb 2026).

The NP decomposition introduces a null tetrad W(x)=(εχ χμ)(x),W(x)=\begin{pmatrix}\varepsilon&\chi\ \chi^*&\mu\end{pmatrix}(x),8 satisfying

W(x)=(εχ χμ)(x),W(x)=\begin{pmatrix}\varepsilon&\chi\ \chi^*&\mu\end{pmatrix}(x),9

$W \partial_t\Psi_{\mathrm{phys}}=\mathrm{Rot}\,\Psi_{\mathrm{phys}}-J_{\mathrm{phys}}, \qquad \mathrm{Rot}:=\begin{pmatrix}0&i\nabla\times\-i\nabla\times&0\end{pmatrix},$0

and

$W \partial_t\Psi_{\mathrm{phys}}=\mathrm{Rot}\,\Psi_{\mathrm{phys}}-J_{\mathrm{phys}}, \qquad \mathrm{Rot}:=\begin{pmatrix}0&i\nabla\times\-i\nabla\times&0\end{pmatrix},$1

The associated directional derivatives are

$W \partial_t\Psi_{\mathrm{phys}}=\mathrm{Rot}\,\Psi_{\mathrm{phys}}-J_{\mathrm{phys}}, \qquad \mathrm{Rot}:=\begin{pmatrix}0&i\nabla\times\-i\nabla\times&0\end{pmatrix},$2

and the electromagnetic field is encoded in the NP scalars

$W \partial_t\Psi_{\mathrm{phys}}=\mathrm{Rot}\,\Psi_{\mathrm{phys}}-J_{\mathrm{phys}}, \qquad \mathrm{Rot}:=\begin{pmatrix}0&i\nabla\times\-i\nabla\times&0\end{pmatrix},$3

In vacuum, $W \partial_t\Psi_{\mathrm{phys}}=\mathrm{Rot}\,\Psi_{\mathrm{phys}}-J_{\mathrm{phys}}, \qquad \mathrm{Rot}:=\begin{pmatrix}0&i\nabla\times\-i\nabla\times&0\end{pmatrix},$4 and $W \partial_t\Psi_{\mathrm{phys}}=\mathrm{Rot}\,\Psi_{\mathrm{phys}}-J_{\mathrm{phys}}, \qquad \mathrm{Rot}:=\begin{pmatrix}0&i\nabla\times\-i\nabla\times&0\end{pmatrix},$5 yield four first-order PDEs: $W \partial_t\Psi_{\mathrm{phys}}=\mathrm{Rot}\,\Psi_{\mathrm{phys}}-J_{\mathrm{phys}}, \qquad \mathrm{Rot}:=\begin{pmatrix}0&i\nabla\times\-i\nabla\times&0\end{pmatrix},$6

$W \partial_t\Psi_{\mathrm{phys}}=\mathrm{Rot}\,\Psi_{\mathrm{phys}}-J_{\mathrm{phys}}, \qquad \mathrm{Rot}:=\begin{pmatrix}0&i\nabla\times\-i\nabla\times&0\end{pmatrix},$7

$W \partial_t\Psi_{\mathrm{phys}}=\mathrm{Rot}\,\Psi_{\mathrm{phys}}-J_{\mathrm{phys}}, \qquad \mathrm{Rot}:=\begin{pmatrix}0&i\nabla\times\-i\nabla\times&0\end{pmatrix},$8

$W \partial_t\Psi_{\mathrm{phys}}=\mathrm{Rot}\,\Psi_{\mathrm{phys}}-J_{\mathrm{phys}}, \qquad \mathrm{Rot}:=\begin{pmatrix}0&i\nabla\times\-i\nabla\times&0\end{pmatrix},$9

With itΨ(t)=MΨ(t)iJ(t),M=W1Rotω0,i\,\partial_t\Psi(t)=M\Psi(t)-i\,J(t),\qquad M=W^{-1}\,\mathrm{Rot}\big|_{\omega\ge 0},0, these may be organized as a itΨ(t)=MΨ(t)iJ(t),M=W1Rotω0,i\,\partial_t\Psi(t)=M\Psi(t)-i\,J(t),\qquad M=W^{-1}\,\mathrm{Rot}\big|_{\omega\ge 0},1 differential operator itΨ(t)=MΨ(t)iJ(t),M=W1Rotω0,i\,\partial_t\Psi(t)=M\Psi(t)-i\,J(t),\qquad M=W^{-1}\,\mathrm{Rot}\big|_{\omega\ge 0},2, or, after isolating a dynamical subsystem, as a square itΨ(t)=MΨ(t)iJ(t),M=W1Rotω0,i\,\partial_t\Psi(t)=M\Psi(t)-i\,J(t),\qquad M=W^{-1}\,\mathrm{Rot}\big|_{\omega\ge 0},3 operator (Xiao et al., 16 Feb 2026).

The same formalism accommodates Lorentz-violating extensions while preserving gauge invariance because the actions are built from itΨ(t)=MΨ(t)iJ(t),M=W1Rotω0,i\,\partial_t\Psi(t)=M\Psi(t)-i\,J(t),\qquad M=W^{-1}\,\mathrm{Rot}\big|_{\omega\ge 0},4 and itΨ(t)=MΨ(t)iJ(t),M=W1Rotω0,i\,\partial_t\Psi(t)=M\Psi(t)-i\,J(t),\qquad M=W^{-1}\,\mathrm{Rot}\big|_{\omega\ge 0},5. For the CPT-odd dimension-3 CFJ/MCS term, the field equation becomes

itΨ(t)=MΨ(t)iJ(t),M=W1Rotω0,i\,\partial_t\Psi(t)=M\Psi(t)-i\,J(t),\qquad M=W^{-1}\,\mathrm{Rot}\big|_{\omega\ge 0},6

producing source-like NP terms linear in itΨ(t)=MΨ(t)iJ(t),M=W1Rotω0,i\,\partial_t\Psi(t)=M\Psi(t)-i\,J(t),\qquad M=W^{-1}\,\mathrm{Rot}\big|_{\omega\ge 0},7. For the CPT-even dimension-4 itΨ(t)=MΨ(t)iJ(t),M=W1Rotω0,i\,\partial_t\Psi(t)=M\Psi(t)-i\,J(t),\qquad M=W^{-1}\,\mathrm{Rot}\big|_{\omega\ge 0},8 term,

itΨ(t)=MΨ(t)iJ(t),M=W1Rotω0,i\,\partial_t\Psi(t)=M\Psi(t)-i\,J(t),\qquad M=W^{-1}\,\mathrm{Rot}\big|_{\omega\ge 0},9

and the NP equations acquire additional linear couplings to directional derivatives of (E,H)=2ReΨ(\mathbf E,\mathbf H)=2\,\mathrm{Re}\,\Psi0 and to (E,H)=2ReΨ(\mathbf E,\mathbf H)=2\,\mathrm{Re}\,\Psi1 itself. Myers–Pospelov dimension-5 terms generate second derivatives along (E,H)=2ReΨ(\mathbf E,\mathbf H)=2\,\mathrm{Re}\,\Psi2, while dimension-6 Podolsky/Lee–Wick operators produce up to third-order derivatives in the NP scalars (Xiao et al., 16 Feb 2026).

The formal closure of the system relies on the NP commutators, Ricci identities, and decoupling identities such as

(E,H)=2ReΨ(\mathbf E,\mathbf H)=2\,\mathrm{Re}\,\Psi3

In this setting the first-order Maxwell operator is simultaneously a compact encoding of the field equations and an asymptotic tool for radiation and polarization analysis.

3. Self-adjoint generators in media and cylindrical waveguides

In the Schrödinger formalism for electromagnetism, the Maxwell operator acts on a weighted Hilbert space

(E,H)=2ReΨ(\mathbf E,\mathbf H)=2\,\mathrm{Re}\,\Psi4

with scalar product

(E,H)=2ReΨ(\mathbf E,\mathbf H)=2\,\mathrm{Re}\,\Psi5

Under the assumptions (E,H)=2ReΨ(\mathbf E,\mathbf H)=2\,\mathrm{Re}\,\Psi6 and (E,H)=2ReΨ(\mathbf E,\mathbf H)=2\,\mathrm{Re}\,\Psi7, one takes

(E,H)=2ReΨ(\mathbf E,\mathbf H)=2\,\mathrm{Re}\,\Psi8

and (E,H)=2ReΨ(\mathbf E,\mathbf H)=2\,\mathrm{Re}\,\Psi9 is self-adjoint. The corresponding unitary group M:(A,F)(dAF,δF),\mathcal M:(A,F)\longmapsto (dA-F,\delta F),0 yields

M:(A,F)(dAF,δF),\mathcal M:(A,F)\longmapsto (dA-F,\delta F),1

and preserves the electromagnetic energy

M:(A,F)(dAF,δF),\mathcal M:(A,F)\longmapsto (dA-F,\delta F),2

Because M:(A,F)(dAF,δF),\mathcal M:(A,F)\longmapsto (dA-F,\delta F),3, the spectrum is symmetric, with positive and negative branches and a zero eigenspace of longitudinal modes. The projector

M:(A,F)(dAF,δF),\mathcal M:(A,F)\longmapsto (dA-F,\delta F),4

selects the unique complex nonnegative-frequency representative of a real field (Nittis et al., 2017).

In an infinite cylinder M:(A,F)(dAF,δF),\mathcal M:(A,F)\longmapsto (dA-F,\delta F),5 with scalar coefficients M:(A,F)(dAF,δF),\mathcal M:(A,F)\longmapsto (dA-F,\delta F),6 and M:(A,F)(dAF,δF),\mathcal M:(A,F)\longmapsto (dA-F,\delta F),7, the Maxwell operator is the self-adjoint first-order block matrix

M:(A,F)(dAF,δF),\mathcal M:(A,F)\longmapsto (dA-F,\delta F),8

in M:(A,F)(dAF,δF),\mathcal M:(A,F)\longmapsto (dA-F,\delta F),9, with domain

dAF=0dA-F=00

subject to perfect-conductivity conditions

dAF=0dA-F=01

and divergence-free constraints dAF=0dA-F=02, dAF=0dA-F=03 (Filonov, 2020).

Because dAF=0dA-F=04 and dAF=0dA-F=05 depend only on the longitudinal variable, separation of variables reduces the three-dimensional operator to a countable family of one-dimensional first-order matrix systems. The invariant subspaces dAF=0dA-F=06, dAF=0dA-F=07, and dAF=0dA-F=08 carry dAF=0dA-F=09, FF0, and FF1 blocks, respectively. Under stabilization at infinity, each block square is unitarily equivalent to a direct sum of scalar Schrödinger operators with short-range potential; under periodicity, the squares become Hill operators. The resulting spectral description is explicit: for stabilizing coefficients, FF2, and the absolutely continuous spectrum is either FF3 or has a single gap around zero depending on the topology of the cross-section; for periodic coefficients, FF4, FF5, and FF6 has a finite number of gaps (Filonov, 2020).

Together these results place the first-order Maxwell operator within functional analysis and spectral theory: self-adjointness is not merely formal, but the basis for well-posed evolution, conserved quadratic observables, and reduction to tractable one-dimensional blocks.

4. Duffin–Kemmer–Petiau-type formulation of Maxwell–Chern–Simons theory

In FF7 dimensions, the Maxwell–Chern–Simons system

FF8

admits a first-order matrix reformulation in terms of the six-component wavefunction

FF9

The field equations become

δF=0\delta F=00

or, equivalently,

δF=0\delta F=01

with δF=0\delta F=02 a projector onto the tensor subspace (Kruglov, 2010).

In the ordered basis δF=0\delta F=03, the δF=0\delta F=04 matrices δF=0\delta F=05 obey the Duffin–Kemmer–Petiau algebra

δF=0\delta F=06

A Hermitianizing matrix exists,

δF=0\delta F=07

satisfying δF=0\delta F=08, so that the bilinear form δF=0\delta F=09 is Lorentz invariant.

The formalism also supplies covariant projection operators. In momentum space, with (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T00 and (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T01, one constructs

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T02

and then spin projectors from the covariant Pauli–Lubanski scalar

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T03

namely

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T04

with (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T05.

After eliminating non-dynamical components by the Lorentz gauge, the theory reduces to a (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T06 Schrödinger Hamiltonian (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T07. Its minimal polynomial implies the eigenvalues

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T08

for the physical sector and

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T09

for the pure-gauge sector (Kruglov, 2010). In this case the first-order Maxwell operator is not a self-adjoint curl generator but a relativistic wave operator of DKP type, adapted to topologically massive spin-1 dynamics.

5. Covariant Hamiltonian and perturbative curved-spacetime operators

A covariant Hamiltonian treatment begins from the Palatini-like Lagrangian

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T10

with independent (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T11 and antisymmetric auxiliary field (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T12. The De Donder–Weyl polymomenta are

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T13

and the generalized Dirac–Bergmann analysis yields the reduced Hamiltonian

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T14

and reduced polysymplectic form

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T15

The De Donder–Weyl equations then reproduce the first-order Maxwell system

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T16

which is equivalently encoded by

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T17

or, in differential-form notation,

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T18

(Pietrzyk et al., 2022). The same framework supports a covariant Hamilton–Jacobi equation

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T19

with the embedding condition (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T20.

In curved spacetime, the source-free Maxwell equations

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T21

together with the Lorenz gauge (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T22 imply

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T23

For a vacuum gravitational wave in TT gauge, (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T24, so (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T25. Expanding

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T26

one obtains the first-order perturbation equation

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T27

with

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T28

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T29

The paper also shows that the (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T30-tensor and (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T31-potential formulations are mathematically equivalent at first order, and that the perturbative equation is gauge-invariant under residual gauge transformations compatible with the first-order Lorenz-gauge constraint (Lou et al., 27 May 2026).

Explicit first-order fields and stress tensor are available: (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T32 and

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T33

For a plane EM wave interacting with a TT gravitational wave, the maximum modulus of the coupling coefficient is on the order of (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T34, and a typical astrophysical strain (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T35 generates a first-order EM response on the order of (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T36 relative to the incident field amplitude (Lou et al., 27 May 2026). Here the first-order Maxwell operator functions as a perturbative transport operator on electromagnetic degrees of freedom in a weakly curved background.

6. First-order Green operators and macroscopic quantum electrodynamics

In macroscopic QED, the first-order operator formalism is formulated directly in the frequency domain and retains both (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T37 and (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T38 as components of a dual field,

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T39

The operator equation is

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T40

with

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T41

The retarded Green operator

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T42

has kernel (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T43 satisfying

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T44

and the interior field obeys the Stratton–Chu representation

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T45

The boundary term is intrinsic rather than discarded, and (ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T46 propagates both volume sources and tangential surface data (Agarwal et al., 29 Mar 2026).

Two bilinear structures organize the formalism. Under the energy inner product,

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T47

one derives the generalized optical theorem,

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T48

Under the reciprocal inner product

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T49

one obtains Lorentz reciprocity,

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T50

for reciprocal media.

Quantization proceeds through a Heisenberg–Langevin treatment. The constitutive relation is

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T51

with bulk noise commutator

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T52

The operator-valued field solution is

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T53

and the total field satisfies the exact closed commutation relation

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T54

The same framework yields an exact quantum transfer relation between input and output surfaces,

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T55

with

(ϕ0,ϕ1,ϕ2)T(\phi_0,\phi_1,\phi_2)^T56

This formalism extends first-order Maxwell operators from classical propagation to open-system quantization in absorptive and dispersive photonic structures (Agarwal et al., 29 Mar 2026).

Taken together, these developments suggest that first-order Maxwell operator formalisms are best understood as a broad operator-theoretic framework in which Maxwell’s equations are embedded into enlarged state spaces so that gauge structure, spectral decomposition, asymptotic propagation, reciprocity, and quantization become directly accessible within a single first-order language.

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