Matter and Radiation at Extremes, Volume. 10, Issue 3, 037201(2025)

3+1 formulation of light modes in nonlinear electrodynamics

Chul Min Kim1,2,3 and Sang Pyo Kim4,5
Author Affiliations
  • 1Advanced Photonics Research Institute, Gwangju Institute of Science and Technology, Gwangju 61005, South Korea
  • 2Center for Relativistic Laser Science, Institute for Basic Science, Gwangju 61005, South Korea
  • 3Department of Physics and Photon Science, Gwangju Institute of Science and Technology, Gwangju 61005, South Korea
  • 4Department of Physics, Kunsan National University, Gunsan 54150, South Korea
  • 5Asia Pacific Center for Theoretical Physics, Pohang 37673, South Korea
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    Figures & Tables(5)
    Configuration of the background magnetic field B=B0ẑ, the light propagation direction n̂, and the two polarization vectors δE⊥ and δE‖. The vector δE⊥ is perpendicular to the plane formed by B and n̂, while δE‖ is in the plane. The light modes in Table III refer to this configuration.
    Departures of the refractive indices n and the parallel polarization vector’s angle ϕ from their free-space values as functions of the magnetic field strength for PM and HES Lagrangians: (a) n⊥ − 1 and n‖ − 1; (b) (ϕ − π/4)/π. Here, the parameters η1 and η2 of the PM Lagrangian are chosen to match the HES Lagrangian in the weak-field limit: η1/4 = η2/7 = e4/(360π2m4). Bc = m2c2/eℏ = 4.4 × 1013 G. The propagation vector’s angle (θ in Fig. 1) is π/4.
    • Table 1. Determination of polarization vectors for a given refractive index. The symbol ∼ between two quantities indicates that the two vectors are equivalent, i.e., differ only by a factor. In this table, the case n = 1 is excluded. In the nondegenerate case, n = 1 leads to the FPC. In the degenerate case, n = 1 can hold when δEZ × X for general configurations as well as the FPC.

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      Table 1. Determination of polarization vectors for a given refractive index. The symbol ∼ between two quantities indicates that the two vectors are equivalent, i.e., differ only by a factor. In this table, the case n = 1 is excluded. In the nondegenerate case, n = 1 leads to the FPC. In the degenerate case, n = 1 can hold when δEZ × X for general configurations as well as the FPC.

      Nondegenerate case (c ≠ 0)δE = pX′ + qY′ + rZ
      n (≠ 1) from MNH2 = 0 (33)X′, Y′, Z′ from (26)
      Cases(p, q, r)
      H ≠ 0, M ≠ 0, N ≠ 0H,M,(ZX)H/d2+(ZY)M/d2
      ∼ (−N, H, (ZX)N/d2 − (ZY)H/d2)
      H = 0, M ≠ 0, N = 0(0, − M, (ZY)M/d2) ∼ (0, 1, − (ZY)/d2)
      H = 0, M = 0, N ≠ 0(−N, 0, (ZX)N/d2) ∼ (1, 0, − (ZX)/d2)
      H = 0, M = 0, N = 0p,q,(ZX)p/d2(ZY)q/d2;
      p and q are arbitrary.
      Degenerate case (c = 0)δE = pX′ + rZ
      n (≠ 1) from M̃ÑH̃2=0(38)X′, Z′ from (36)
      Cases(p, r)
      H̃0, M̃0, Ñ0(H̃,M̃)(Ñ,H̃)
      H̃=0, M̃0, Ñ=0(0,M̃)(0,1)
      H̃=0, M̃=0, Ñ0(Ñ,0)(1,0)
      H̃=0, M̃=0, Ñ=0(p, r); p and r are arbitrary.
    • Table 2. Procedure to find light modes in a nonlinear nondegenerate vacuum. The steps from 7 to 9 should be implemented for each value of n found in step 6. In Sec. IV C, we present the essential formulas used in the procedure in order. A similar procedure can be set up in the degenerate case.

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      Table 2. Procedure to find light modes in a nonlinear nondegenerate vacuum. The steps from 7 to 9 should be implemented for each value of n found in step 6. In Sec. IV C, we present the essential formulas used in the procedure in order. A similar procedure can be set up in the degenerate case.

      StepTaskEquations
      1Specify Lagrangian(16)
      2Calculate a2, ab, b2, c2, and d2 without specifying E and B(24)
      3Specify E, B, and n̂ and rule out the FPC
      4Calculate a2, ab, b2, c2, and d2 for E and B, and confirm c ≠ 0(24)
      5Calculate α, β, and γ in terms of a2, ab, b2, c2, and d2(32)
      6Calculate λ(±) and n > 0(31) and (34)
      7Calculate X, Y, Z, V, X′, Y′, and Z(23) and (26)
      8Calculate H, M, and N(28)
      9Determine (p, q, r) and calculate δETable I, (25)
    • Table 3. Refractive indices and polarization vectors for various Lagrangians in a purely magnetic background field: B=B0ẑ and n̂=(sinθ,0,cosθ), as shown in Fig. 1. For HES, a2, c2, and d2 are from (55). The FPC is not included here.

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      Table 3. Refractive indices and polarization vectors for various Lagrangians in a purely magnetic background field: B=B0ẑ and n̂=(sinθ,0,cosθ), as shown in Fig. 1. For HES, a2, c2, and d2 are from (55). The FPC is not included here.

      LagrangianDegeneracy (c = 0)(Refractive index)2Polarization vectorParameters
      Post-Maxwellian (PM)Non211μsin2θδE ≡ (0, 1, 0)μ=2η1B021η1B02
      n21+ϵ1+ϵcos2θδEcosθ,0,11+ϵsinθϵ=2η2B021η1B02
      Born–Infeld (BI)Non2E + Eϵ=B02/T
      p, q arbitrary
      ModMax (MM)Yesn2(=1)δEμ = 0
      n2δEϵ = e2g − 1
      Heisenberg–Euler–Schwinger (HES)Non2δEμ=B02a2/d2
      n2δEϵ=B02c2/d2
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    Chul Min Kim, Sang Pyo Kim. 3+1 formulation of light modes in nonlinear electrodynamics[J]. Matter and Radiation at Extremes, 2025, 10(3): 037201

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    Paper Information

    Received: Sep. 27, 2024

    Accepted: Mar. 3, 2025

    Published Online: Jul. 16, 2025

    The Author Email:

    DOI:10.1063/5.0240870

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