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arxiv: 2606.23389 · v1 · pith:HQDKYYFHnew · submitted 2026-06-22 · 🌀 gr-qc · hep-ph

Scattered wave functions and worldline instantons for particle production in curved spacetime

Pith reviewed 2026-06-26 07:47 UTC · model grok-4.3

classification 🌀 gr-qc hep-ph
keywords pair productioncurved spacetimescattered wave functionsworldline instantonsspin-1/2 particlesgravitational backgroundsnonperturbative methodstwo-dimensional metrics
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The pith

Two extended methods compute particle-antiparticle pair production in curved spacetimes depending on multiple coordinates.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper develops two complementary techniques for calculating the production of spin-1/2 particle pairs in gravitational backgrounds that vary nontrivially in more than one coordinate. It extends the scattered-wave-function method from electromagnetic to curved spacetime cases and derives the pre-exponential factor for the open-worldline-instanton approach. Tests on several two-dimensional metrics show that the two methods produce matching probabilities. The scattered-wave-function method gives numerically exact results efficiently in these examples, while the instanton method scales better to higher dimensions and extreme regimes.

Core claim

We extend the scattered-wave-function method to curved spacetime backgrounds and complete the open-worldline-instanton method by deriving its pre-exponential factor. When both are applied to several two-dimensional metrics the resulting pair-production probabilities agree well.

What carries the argument

The scattered-wave-function method adapted to curved spacetime and the open-worldline-instanton method with its newly derived pre-exponential factor.

If this is right

  • The two methods agree on the pair-production probabilities for the two-dimensional metrics considered.
  • The scattered-wave-function approach supplies numerically exact results and is efficient for the tested cases.
  • The instanton approach offers favorable scaling to higher-dimensional backgrounds and more extreme parameter regimes.
  • These methods supply new tools for studying pair production in multidimensional gravitational backgrounds.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The agreement between methods in two dimensions indicates they could be applied to three-dimensional metrics where other approaches fail.
  • Worldline instantons might link to similar semiclassical techniques used in other nonperturbative quantum processes.
  • The efficiency of the scattered-wave-function method could allow systematic scans over families of curved metrics.

Load-bearing premise

The extensions of both the scattered-wave-function and worldline-instanton techniques remain valid for metrics that depend nontrivially on more than one coordinate.

What would settle it

A specific two-dimensional metric in which the two methods produce clearly different probabilities would show that at least one extension is invalid.

Figures

Figures reproduced from arXiv: 2606.23389 by Greger Torgrimsson, Philip Semr\'en.

Figure 1
Figure 1. Figure 1: FIG. 1. Spectrum of pair production with [PITH_FULL_IMAGE:figures/full_fig_p008_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2. The line [PITH_FULL_IMAGE:figures/full_fig_p008_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: FIG. 3. Same as Fig. 1 but with [PITH_FULL_IMAGE:figures/full_fig_p009_3.png] view at source ↗
Figure 4
Figure 4. Figure 4: FIG. 4. The line [PITH_FULL_IMAGE:figures/full_fig_p009_4.png] view at source ↗
Figure 5
Figure 5. Figure 5: FIG. 5. The function in (87) with [PITH_FULL_IMAGE:figures/full_fig_p009_5.png] view at source ↗
Figure 6
Figure 6. Figure 6: FIG. 6. The spectrum for the metrics in Fig. 5. [PITH_FULL_IMAGE:figures/full_fig_p010_6.png] view at source ↗
Figure 7
Figure 7. Figure 7: FIG. 7. Similar to Fig. 1 but for the field in (87) with [PITH_FULL_IMAGE:figures/full_fig_p011_7.png] view at source ↗
read the original abstract

We study the production of spin-$1/2$ particle-antiparticle pairs in curved spacetimes with nontrivial dependence on more than one coordinate. To this end, we develop two complementary approaches. First, we extend the scattered-wave-function (SWF) method, originally introduced for pair production in electromagnetic backgrounds, to curved spacetime backgrounds. Second, we complete the development of an open-worldline-instanton method by deriving the pre-exponential factor of the pair-production probability. We apply both methods to several two-dimensional metrics and find good agreement between the resulting probabilities. While the SWF approach provides numerically exact results and is particularly efficient for the examples considered here, the instanton approach offers favorable scaling to higher-dimensional backgrounds and more extreme parameter regimes. These methods provide new tools for studying pair production in multidimensional gravitational backgrounds beyond the reach of many existing approaches.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

1 major / 0 minor

Summary. The paper extends the scattered-wave-function (SWF) method, originally for electromagnetic backgrounds, to curved spacetimes and completes the open-worldline-instanton method by deriving the pre-exponential factor for the pair-production probability. Both are applied to several two-dimensional metrics with nontrivial dependence on both coordinates, yielding numerically agreeing probabilities for spin-1/2 pair production; the SWF method is noted as numerically exact and efficient for these cases while the instanton method scales better to higher dimensions.

Significance. If the extensions are valid, the work supplies complementary calculational tools for pair production in multidimensional gravitational backgrounds that lie beyond the reach of many standard approaches in QFT in curved spacetime, with the instanton route offering favorable scaling.

major comments (1)
  1. [Abstract] Abstract and introduction: the central claim that the extensions remain valid for metrics with nontrivial dependence on more than one coordinate is supported only by numerical agreement between the two newly extended methods; because both derive from the same underlying mode-decomposition and semiclassical framework, this agreement does not exclude the possibility of shared systematic error in the multi-coordinate handling, and no independent benchmark (exactly solvable case or third method) is reported.

Simulated Author's Rebuttal

1 responses · 0 unresolved

We thank the referee for their careful reading and constructive comments. We address the major comment below.

read point-by-point responses
  1. Referee: [Abstract] Abstract and introduction: the central claim that the extensions remain valid for metrics with nontrivial dependence on more than one coordinate is supported only by numerical agreement between the two newly extended methods; because both derive from the same underlying mode-decomposition and semiclassical framework, this agreement does not exclude the possibility of shared systematic error in the multi-coordinate handling, and no independent benchmark (exactly solvable case or third method) is reported.

    Authors: We respectfully disagree that the methods share a systematic error from a common framework. The SWF method is a direct numerical solution of the Dirac equation via scattering (numerically exact, as noted in the report) and was extended from its original electromagnetic formulation; it involves no semiclassical approximation. The open-worldline-instanton method is a distinct semiclassical approach whose pre-exponential factor is newly derived here. Agreement between an exact method and a semiclassical one on 2D metrics with nontrivial dependence on both coordinates therefore validates the multi-coordinate extensions. While an exactly solvable case or third method would be desirable, none is available for these general metrics, and the SWF results serve as the independent benchmark for the instanton results. No revision is required. revision: no

Circularity Check

0 steps flagged

No circularity: two independent method extensions cross-validated on shared test metrics

full rationale

The paper derives an extension of the scattered-wave-function method and a completion of the worldline-instanton method (pre-exponential factor) from the standard QFT-in-curved-space framework, then applies both to the same 2D example metrics and reports numerical agreement. Neither derivation reduces to the other by construction, no parameter is fitted from one method to predict the other, and no load-bearing uniqueness theorem or ansatz is imported solely via self-citation. The agreement functions as an external consistency check between distinct calculational routes rather than a self-referential identity. The central claim therefore retains independent content and is self-contained against the benchmarks the authors themselves compute.

Axiom & Free-Parameter Ledger

0 free parameters · 1 axioms · 0 invented entities

The central results rest on the validity of the analytic continuations and saddle-point approximations implicit in both methods when applied to non-static, multidimensional metrics. No explicit free parameters or new entities are introduced in the abstract.

axioms (1)
  • domain assumption The scattered-wave-function and worldline-instanton formalisms can be extended to curved backgrounds with nontrivial dependence on more than one coordinate while preserving their essential structure.
    This is the premise that allows the two methods to be applied beyond the one-dimensional cases treated in prior work.

pith-pipeline@v0.9.1-grok · 5677 in / 1268 out tokens · 15423 ms · 2026-06-26T07:47:34.170338+00:00 · methodology

discussion (0)

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Reference graph

Works this paper leans on

82 extracted references · 23 linked inside Pith

  1. [1]

    iϵ s p0 +p 1 q0 +q 1 # = ln

    The reality of the other square roots follows from Sylvester’s criterion for positive-definite matrices applied to−g ij. For this particular case, the criterion can be proved as follows. Since−gis positive definite, (u, v, w)·(−g)·(u, v, w)>0(31) for all nonzero(u, v, w). Cancelling the mixed terms by successive shifts, w→w− g31u+g 32v g33 v→v+ g31g32 −g ...

  2. [2]

    Method 1 When the holonomy is trivial, i.e. when we can choose coordinates so thatg µν →η µν everywhere in the exte- rior region, then we can compute the inner products by first separating out a delta-function part as in (83). If insteadˆya ̸= ˇya then it is more nontrivial to extract the delta-function parts of⟨U in|Uout⟩and⟨V in|Vout⟩. As an integralove...

  3. [3]

    Method 2 For the second method, we begin by defining {Uin|ψ}(ˇx) = Z dk1 2π e−ik1ˇxu† k Z dˇyeik1ˇyψ(ˇy) {Vin|ψ}(ˇx) = Z dk1 2π e−ik1ˇxv† −k Z dˇyeik1ˇyψ(ˇy), (A17) which is a Fourier transform, projection withu† k orv † −k and then an inverse Fourier transform. This allows us to express the inner products as ⟨Uin(k)|ψ⟩= Z dˇx eik0t−+ik1ˇx{Uin|ψ}(ˇx) ⟨Vin...

  4. [4]

    Quantum Field Theory in Curved Spacetime: Quantized Field and Gravity,

    L. E. Parker and D. Toms, “Quantum Field Theory in Curved Spacetime: Quantized Field and Gravity,” Cam- bridge University Press, (2009)

  5. [5]

    Cosmological particle production: a re- view,

    L. H. Ford, “Cosmological particle production: a re- view,” Rept. Prog. Phys.84, no.11, 116901 (2021) [arXiv:2112.02444 [gr-qc]]

  6. [6]

    The Creation of Particles in an Expanding Universe,

    L. E. Parker, “The Creation of Particles in an Expanding Universe,” [arXiv:2507.05372 [gr-qc]]

  7. [7]

    Quantized fields and particle creation in ex- panding universes. 1.,

    L. Parker, “Quantized fields and particle creation in ex- panding universes. 1.,” Phys. Rev.183, 1057-1068 (1969)

  8. [8]

    Quantized fields and particle creation in ex- panding universes. 2.,

    L. Parker, “Quantized fields and particle creation in ex- panding universes. 2.,” Phys. Rev. D3, 346-356 (1971) [erratum: Phys. Rev. D3, 2546-2546 (1971)]

  9. [9]

    Particle Creation by Black Holes,

    S. W. Hawking, “Particle Creation by Black Holes,” Com- mun. Math. Phys.43, 199-220 (1975) [erratum: Com- mun. Math. Phys.46, 206 (1976)]

  10. [10]

    Momentum correlation in pair pro- duction by spacetime dependent fields from scattered wave functions,

    G. Torgrimsson, “Momentum correlation in pair pro- duction by spacetime dependent fields from scattered wave functions,” Phys. Rev. D112, no.11, 116011 (2025) [arXiv:2509.17770 [hep-ph]]

  11. [11]

    Solving the Dirac equation on a GPU forstrong-fieldprocessesinmultidimensionalbackground fields,

    G. Torgrimsson, “Solving the Dirac equation on a GPU forstrong-fieldprocessesinmultidimensionalbackground fields,” [arXiv:2512.16889 [hep-ph]]

  12. [12]

    Phase space structure of the Dirac vacuum,

    I. Bialynicki-Birula, P. Gornicki and J. Rafelski, “Phase space structure of the Dirac vacuum,” Phys. Rev. D44, 1825-1835 (1991)

  13. [13]

    Pair creation enhancement due to combined external fields,

    M. Jiang, W. Su, Z. Q. Lv, X. Lu, Y. J. Li, R. Grobe and Q. Su, “Pair creation enhancement due to combined external fields,” Phys. Rev. A85, no.3, 033408 (2012)

  14. [14]

    Cosmological particle creation using an equal-time Wigner formalism,

    P. Semrén, “Cosmological particle creation using an equal-time Wigner formalism,” Phys. Rev. D110, no.8, 085004 (2024) [arXiv:2406.18205 [gr-qc]]

  15. [15]

    D113, no.12, 125002 (2026) [arXiv:2602.07330 [hep-th]]

    M.Alkhateeb, J.P.EdwardsandY.Caudano, Phys.Rev. D113, no.12, 125002 (2026) [arXiv:2602.07330 [hep-th]]

  16. [16]

    Particle self- bunching in the Schwinger effect in spacetime-dependent electric fields,

    F. Hebenstreit, R. Alkofer and H. Gies, “Particle self- bunching in the Schwinger effect in spacetime-dependent electric fields,” Phys. Rev. Lett.107, 180403 (2011) [arXiv:1106.6175 [hep-ph]]

  17. [17]

    Enhancement of electron-positron pair creation due to transient excitation of field-induced bound states,

    M. Jiang, Q. Z. Lv, Z. M. Sheng, R. Grobe and Q. Su, “Enhancement of electron-positron pair creation due to transient excitation of field-induced bound states,” Phys. Rev. A87, no.4, 042503 (2013)

  18. [18]

    Spin polar- ized electron-positron pairproductionvia elliptical polar- ized laser fields,

    A. Wöllert, H. Bauke and C. H. Keitel, “Spin polar- ized electron-positron pairproductionvia elliptical polar- ized laser fields,” Phys. Rev. D91, no.12, 125026 (2015) [arXiv:1502.06414 [physics.atom-ph]]

  19. [19]

    Electron-positron pair production in in- homogeneous electromagnetic fields,

    C. Kohlfürst, “Electron-positron pair production in in- homogeneous electromagnetic fields,” [arXiv:1512.06082 [hep-ph]]

  20. [20]

    On the effect of time-dependent inhomogeneous magnetic fields in elec- tron–positron pair production,

    C. Kohlfürst and R. Alkofer, “On the effect of time-dependent inhomogeneous magnetic fields in elec- tron–positron pair production,” Phys. Lett. B756, 371- 375 (2016) [arXiv:1512.06668 [hep-ph]]

  21. [21]

    Electron-positron pair production in external electric fields varying both in space and time,

    I. A. Aleksandrov, G. Plunien and V. M. Shabaev, “Electron-positron pair production in external electric fields varying both in space and time,” Phys. Rev. D94, no.6, 065024 (2016) [arXiv:1606.06313 [hep-th]]

  22. [22]

    Mo- mentum distribution of particles created in space-time- dependent colliding laser pulses,

    I. A. Aleksandrov, G. Plunien and V. M. Shabaev, “Mo- mentum distribution of particles created in space-time- dependent colliding laser pulses,” Phys. Rev. D96, no.7, 076006 (2017) [arXiv:1709.07331 [hep-ph]]

  23. [23]

    Ponderomotive effects in multiphoton pair production,

    C. Kohlfürst and R. Alkofer, “Ponderomotive effects in multiphoton pair production,” Phys. Rev. D97, no.3, 036026 (2018) [arXiv:1711.10766 [hep-ph]]

  24. [24]

    Phase-space analysis of the Schwinger ef- fect in inhomogeneous electromagnetic fields,

    C. Kohlfürst, “Phase-space analysis of the Schwinger ef- fect in inhomogeneous electromagnetic fields,” Eur. Phys. J. Plus133, no.5, 191 (2018) [arXiv:1708.08920 [quant- ph]]

  25. [25]

    Roleofthespatialinhomogeneityonthelaser- induced vacuum decay,

    Q. Z. Lv, S. Dong, Y. T. Li, Z. M. Sheng, Q. Su and R.Grobe, “Roleofthespatialinhomogeneityonthelaser- induced vacuum decay,” Phys. Rev. A97, no.2, 022515 (2018)

  26. [26]

    Effects of finite spatial extent on Schwinger pair production,

    M. Ababekri, B. S. Xie and J. Zhang, “Effects of finite spatial extent on Schwinger pair production,” Phys. Rev. D100, no.1, 016003 (2019) [arXiv:1905.01629 [hep-ph]]

  27. [27]

    Multichannelinterferencein nonperturbative multiphoton pair production by gamma rays colliding,

    Z.Peng, H.HuandJ.Yuan, “Multichannelinterferencein nonperturbative multiphoton pair production by gamma rays colliding,” Phys. Rev. Res.2, no.1, 013020 (2020) [arXiv:1810.03606 [cond-mat.mes-hall]]

  28. [28]

    Effect of time-dependent inhomogeneous magnetic fields on the particle momentum spectrum in electron-positron pair production,

    C. Kohlfürst, “Effect of time-dependent inhomogeneous magnetic fields on the particle momentum spectrum in electron-positron pair production,” Phys. Rev. D101, no.9, 096003 (2020) [arXiv:1912.09359 [hep-ph]]

  29. [29]

    Pair production in temporally and spatially oscillating fields,

    I. A. Aleksandrov and C. Kohlfürst, “Pair production in temporally and spatially oscillating fields,” Phys. Rev. D 101, no.9, 096009 (2020) [arXiv:1912.09924 [hep-ph]]

  30. [30]

    Chirp effectsonpairproductioninoscillatingelectricfieldswith spatial inhomogeneity,

    M. Ababekri, S. Dulat, B. S. Xie and J. Zhang, “Chirp effectsonpairproductioninoscillatingelectricfieldswith spatial inhomogeneity,” Phys. Lett. B810, 135815 (2020) [arXiv:1912.05302 [quant-ph]]

  31. [31]

    Enhanced dynamically assisted pair production in spatial inhomo- 23 geneous electric fields with the frequency chirping,

    L. J. Li, M. Mohamedsedik and B. S. Xie, “Enhanced dynamically assisted pair production in spatial inhomo- 23 geneous electric fields with the frequency chirping,” Phys. Rev. D104, no.3, 036015 (2021) [arXiv:2104.08828 [hep- ph]]

  32. [32]

    Schwingerpair productionininhomogeneouselectricfieldswithsymmet- rical frequency chirp,

    M.Mohamedsedik, L.J.LiandB.S.Xie, “Schwingerpair productionininhomogeneouselectricfieldswithsymmet- rical frequency chirp,” Phys. Rev. D104, no.1, 016009 (2021) [arXiv:2105.03018 [hep-ph]]

  33. [33]

    Study of pair produc- tion in inhomogeneous two-color electric fields using the computational quantum field theory,

    Z. L. Li, C. Gong and Y. J. Li, “Study of pair produc- tion in inhomogeneous two-color electric fields using the computational quantum field theory,” Phys. Rev. D103, no.11, 116018 (2021) [arXiv:2106.04236 [hep-ph]]

  34. [34]

    Sauter-Schwinger Effect for Collid- ing Laser Pulses,

    C. Kohlfürst, N. Ahmadiniaz, J. Oertel and R. Schützhold, “Sauter-Schwinger Effect for Collid- ing Laser Pulses,” Phys. Rev. Lett.129, no.24, 241801 (2022) [arXiv:2107.08741 [hep-ph]]

  35. [35]

    Impact of spatially pe- riodic inhomogeneities on the photon-induced pair cre- ation,

    M. Jiang, R. Grobe and Q. Su, “Impact of spatially pe- riodic inhomogeneities on the photon-induced pair cre- ation,” Phys. Rev. A108, no.2, 022813 (2023)

  36. [36]

    Pair Production In An Electric Field In A Time Dependent Gauge,

    A. O. Barut and I. H. Duru, “Pair Production In An Electric Field In A Time Dependent Gauge,” Phys. Rev. D41, 1312 (1990)

  37. [37]

    Lorentzian worldline path integral approach to Schwinger effect,

    K. Rajeev, “Lorentzian worldline path integral approach to Schwinger effect,” Phys. Rev. D104, no.10, 105014 (2021) [arXiv:2105.12194 [hep-th]]

  38. [38]

    Worldline instan- tons for nonlinear Breit-Wheeler pair production and Compton scattering,

    G. Degli Esposti and G. Torgrimsson, “Worldline instan- tons for nonlinear Breit-Wheeler pair production and Compton scattering,” Phys. Rev. D105, no.9, 096036 (2022) [arXiv:2112.11433 [hep-ph]]

  39. [39]

    Worldline instan- tons for the momentum spectrum of Schwinger pair pro- duction in spacetime dependent fields,

    G. Degli Esposti and G. Torgrimsson, “Worldline instan- tons for the momentum spectrum of Schwinger pair pro- duction in spacetime dependent fields,” Phys. Rev. D 107, no.5, 056019 (2023) [arXiv:2212.11578 [hep-ph]]

  40. [40]

    Momentum spec- trum of Schwinger pair production in four-dimensional e-dipole fields,

    G. Degli Esposti and G. Torgrimsson, “Momentum spec- trum of Schwinger pair production in four-dimensional e-dipole fields,” Phys. Rev. D109, no.1, 016013 (2024) [arXiv:2308.01659 [hep-ph]]

  41. [41]

    Momentum spec- trum of nonlinear Breit-Wheeler pair production in spacetime fields,

    G. Degli Esposti and G. Torgrimsson, “Momentum spec- trum of nonlinear Breit-Wheeler pair production in spacetime fields,” Phys. Rev. D110, no.7, 076017 (2024) [arXiv:2312.17186 [hep-ph]]

  42. [42]

    Nonlinear trident usingWKBandworldlineinstantons,

    G. Degli Esposti and G. Torgrimsson, “Nonlinear trident usingWKBandworldlineinstantons,” Phys.Rev.D112, no.3, 036005 (2025) [arXiv:2412.19758 [hep-ph]]

  43. [43]

    Schwinger pair production in spacetime fields: Moiré patterns, Aharonov-Bohm phases, and Sturm-Liouville eigen- values,

    G. Degli Esposti and G. Torgrimsson, “Schwinger pair production in spacetime fields: Moiré patterns, Aharonov-Bohm phases, and Sturm-Liouville eigen- values,” Phys. Rev. D112, no.1, 016026 (2025) [arXiv:2412.19709 [hep-ph]]

  44. [44]

    Pair Produc- tion at Strong Coupling in Weak External Fields,

    I. K. Affleck, O. Alvarez and N. S. Manton, “Pair Produc- tion at Strong Coupling in Weak External Fields,” Nucl. Phys. B197, 509-519 (1982)

  45. [45]

    Worldline instantons and pair production in inhomogeneous fields,

    G. V. Dunne and C. Schubert, “Worldline instantons and pair production in inhomogeneous fields,” Phys. Rev. D 72, 105004 (2005) [arXiv:hep-th/0507174 [hep-th]]

  46. [46]

    Worldline instantons. II. The Fluctuation prefactor,

    G. V. Dunne, Q. h. Wang, H. Gies and C. Schubert, “Worldline instantons. II. The Fluctuation prefactor,” Phys. Rev. D73, 065028 (2006) [arXiv:hep-th/0602176 [hep-th]]

  47. [47]

    Multidimensional World- line Instantons,

    G. V. Dunne and Q. h. Wang, “Multidimensional World- line Instantons,” Phys. Rev. D74, 065015 (2006) [arXiv:hep-th/0608020 [hep-th]]

  48. [48]

    Worldline instantons for nonperturbative particle production by space and time dependent gravitational fields,

    P. Semrén and G. Torgrimsson, “Worldline instantons for nonperturbative particle production by space and time dependent gravitational fields,” Phys. Rev. D113, no.5, 056005 (2026) [arXiv:2508.01901 [hep-th]]

  49. [49]

    Tunnelling amplitudes and Hawking radiation from worldline QFT,

    A. Ilderton and K. Rajeev, “Tunnelling amplitudes and Hawking radiation from worldline QFT,” JHEP10, 220 (2025) [arXiv:2508.00997 [hep-th]]

  50. [50]

    Particle production and complex path analysis,

    K. Srinivasan and T. Padmanabhan, “Particle production and complex path analysis,” Phys. Rev. D60, 024007 (1999) [arXiv:gr-qc/9812028 [gr-qc]]

  51. [51]

    Hawking radiation in different coordinate set- tings: Complex paths approach,

    S. Shankaranarayanan, T. Padmanabhan and K. Srini- vasan, “Hawking radiation in different coordinate set- tings: Complex paths approach,” Class. Quant. Grav. 19, 2671-2688 (2002) [arXiv:gr-qc/0010042 [gr-qc]]

  52. [52]

    Hawking radiation as tunneling,

    M. K. Parikh and F. Wilczek, “Hawking radiation as tunneling,” Phys. Rev. Lett.85, 5042-5045 (2000) [arXiv:hep-th/9907001 [hep-th]]

  53. [53]

    Tun- nelling Methods and Hawking’s radiation: achievements and prospects,

    L. Vanzo, G. Acquaviva and R. Di Criscienzo, “Tun- nelling Methods and Hawking’s radiation: achievements and prospects,” Class. Quant. Grav.28, 183001 (2011) [arXiv:1106.4153 [gr-qc]]

  54. [54]

    A Short Course in Gen- eral Relativity

    J. Foster and D. J. Nightingale, “A Short Course in Gen- eral Relativity”, Third edition, Springer, (2005)

  55. [55]

    Teleparallel Gravity: An Introduction,

    R. Aldrovandi and J. G. Pereira, “Teleparallel Gravity: An Introduction,” Springer, (2013)

  56. [56]

    Quantized gravitational field,

    J. S. Schwinger, “Quantized gravitational field,” Phys. Rev.130, 1253-1258 (1963)

  57. [57]

    On the vierbein formalism of general relativity,

    T. Mei, “On the vierbein formalism of general relativity,” Gen. Rel. Grav.40, 1913-1945 (2008) [arXiv:0707.2639 [gr-qc]]

  58. [58]

    Quantum gravity in the triangular gauge,

    T. Thiemann, “Quantum gravity in the triangular gauge,” Phys. Rev. D110, no.12, 124021 (2024) [arXiv:2305.06724 [gr-qc]]

  59. [59]

    Non-Abelian Stokes formula

    I. Y. Aref’eva, “Non-Abelian Stokes formula”, Theor. Math. Phys.43, 353 (1980)

  60. [60]

    Geometry, topology and physics,

    M. Nakahara, “Geometry, topology and physics,” Insti- tute of Physics Publishing (2003)

  61. [61]

    Fermionic current and Schwinger effect in de Sitter spacetime,

    C. Stahl, E. Strobel and S. S. Xue, “Fermionic current and Schwinger effect in de Sitter spacetime,” Phys. Rev. D93, no.2, 025004 (2016) [arXiv:1507.01686 [gr-qc]]

  62. [62]

    Experimental black hole evaporation,

    W. G. Unruh, “Experimental black hole evaporation,” Phys. Rev. Lett.46, 1351-1353 (1981)

  63. [63]

    Sonic analog of black holes and the effects ofhighfrequenciesonblackholeevaporation,

    W. G. Unruh, “Sonic analog of black holes and the effects ofhighfrequenciesonblackholeevaporation,” Phys.Rev. D51, 2827-2838 (1995) [arXiv:gr-qc/9409008 [gr-qc]]

  64. [64]

    Analoguegravity,

    C.Barcelo, S.LiberatiandM.Visser, “Analoguegravity,” Living Rev. Rel.8, 12 (2005) [arXiv:gr-qc/0505065 [gr- qc]]

  65. [65]

    Ultra-cold atoms as quantum simulators for relativistic phenomena,

    R. Schützhold, “Ultra-cold atoms as quantum simulators for relativistic phenomena,” Prog. Part. Nucl. Phys.145, 104198 (2025) [arXiv:2501.03785 [quant-ph]]

  66. [66]

    ONE ELECTRON ATOM AS A PROBE OF SPACE-TIME CURVATURE,

    L. Parker, “ONE ELECTRON ATOM AS A PROBE OF SPACE-TIME CURVATURE,” Phys. Rev. D22, 1922- 1934 (1980)

  67. [67]

    One-Electron Atom in Curved Space-Time,

    L. Parker, “One-Electron Atom in Curved Space-Time,” Phys. Rev. Lett.44, no.23, 1559 (1980)

  68. [68]

    Quantum electrodynamics with unstable vacuum

    E. S. Fradkin, D. M. Gitman and Sh. M. Shvarts- man, “Quantum electrodynamics with unstable vacuum”, Springer-Verlag Berlin Heidelberg 1991 [66]https://docs.jax.dev/en/latest/index.html

  69. [69]

    On Neural Differential Equations

    P. Kidger, “On Neural Differential Equations”, arXiv:2202.02435,https://docs.kidger.site/diffrax/

  70. [70]

    Torgrimsson, GitHub Repository

    G. Torgrimsson, GitHub Repository

  71. [71]

    Perturbative quantum field theory in the string inspired formalism,

    C. Schubert, “Perturbative quantum field theory in the string inspired formalism,” Phys. Rept.355, 73-234 (2001) [arXiv:hep-th/0101036 [hep-th]]

  72. [72]

    Path integrals 24 and anomalies in curved space,

    F. Bastianelli and P. van Nieuwenhuizen, “Path integrals 24 and anomalies in curved space,” Cambridge University Press, 2006

  73. [73]

    Quantum mechanical path integrals in the first quantised approach to quantum field theory,

    J. P. Edwards and C. Schubert, “Quantum mechanical path integrals in the first quantised approach to quantum field theory,” [arXiv:1912.10004 [hep-th]]

  74. [74]

    On gauge invariance and vacuum po- larization,

    J. S. Schwinger, “On gauge invariance and vacuum po- larization,” Phys. Rev.82, 664-679 (1951)

  75. [75]

    Operator Ordering and Supersymmetry,

    V. de Alfaro, S. Fubini, G. Furlan and M. Roncadelli, “Operator Ordering and Supersymmetry,” Nucl. Phys. B 296, 402-430 (1988)

  76. [76]

    An Introduction into the Feynman path in- tegral,

    C. Grosche, “An Introduction into the Feynman path in- tegral,” [arXiv:hep-th/9302097 [hep-th]]

  77. [77]

    The Lagrangian in quantum mechanics,

    P. A. M. Dirac, “The Lagrangian in quantum mechanics,” Phys. Z. Sowjetunion3, 64-72 (1933)

  78. [78]

    Space-time approach to nonrelativis- tic quantum mechanics,

    R. P. Feynman, “Space-time approach to nonrelativis- tic quantum mechanics,” Rev. Mod. Phys.20, 367-387 (1948)

  79. [79]

    Dynamical theory in curved spaces. 1. A Review of the classical and quantum action principles,

    B. S. DeWitt, “Dynamical theory in curved spaces. 1. A Review of the classical and quantum action principles,” Rev. Mod. Phys.29, 377-397 (1957)

  80. [80]

    Mode regularization, time slicing, Weyl ordering and phase space path integrals for quantum mechanical non- linear sigma models,

    F. Bastianelli, K. Schalm and P. van Nieuwenhuizen, “Mode regularization, time slicing, Weyl ordering and phase space path integrals for quantum mechanical non- linear sigma models,” Phys. Rev. D58, 044002 (1998) [arXiv:hep-th/9801105 [hep-th]]

Showing first 80 references.