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Particles, Detectors, and Nonadiabatic Production

Particle number, detector excitation, and energy flux are different observables in curved or accelerated settings. This chapter connects them through mode evolution and localized measurements while making their operational assumptions explicit.

Begin with Particles, Local Observables, and Detector Dependence to choose between mode occupation, detector response, and stress-energy observables.

Helpful background. Vacuum Ambiguity, Time Flow, and Observer Dependence and Green Operators, Causal Propagators, and State-Dependent Two-Point Functions develop the definitions used by the chapter’s opening pages.

  1. Particles, Local Observables, and Detector Dependence — Separates number, clicks, correlators, and stress flux.
  2. Mode Bases, In/Out States, and Number Operators — States when asymptotic particle counting is controlled.
  3. Detector Response Along Curved and Accelerated Worldlines — Derives the response from the pulled-back two-point function.
  4. Switching, Smearing, Finite-Time Response, and Transients — Controls finite duration and ultraviolet sensitivity.
  5. Particle Creation in Time-Dependent Backgrounds — Computes in/out Bogoliubov production and its energy.
  6. Adiabaticity, Stokes Phenomena, and Production Rates — Treats complex turning points, interference, and error domains.
  7. Parametric-Oscillator and Solvable Production Benchmarks — Supplies exact quench fixtures.
  8. Unruh Effect and Uniformly Accelerated Detectors — Derives acceleration-temperature detailed balance.
  9. Tolman Redshift, KMS Structure, and Local Temperature — Distinguishes global KMS data from calibrated local temperature.
  10. Acceleration, Gravity, and the Limits of Equivalence-Principle Arguments — Isolates local kinematics from curvature, state, and horizon data.
  11. Moving Mirrors and the Dynamical Casimir Effect — Compares Bogoliubov particles, boundary work, and outgoing flux.
  12. Schwinger and Gravitational Production: A Controlled Comparison — Identifies shared turning-point mathematics and different physics.

A time-dependent background can mix positive- and negative-frequency modes, producing an in/out occupation number when the asymptotic bases are defined. A detector instead samples the field’s two-point function along its trajectory with a specified switching and spatial profile. Acceleration can therefore change detector response without changing the global Minkowski vacuum Unruh 1976, pp. 870–892.

Thermal detailed balance requires a suitable stationary or long-time limit. Finite switching introduces transients, and an instantaneous basis occupation depends on how the basis was chosen. These differences should be resolved before assigning a temperature or production rate.

The comparison below separates the assumptions and tests needed for these different conclusions.

ConstructionState, geometry, and trajectoryBasis or interactionSwitching, asymptotics, and regulatorReported observableEnergy accountingLicensed claim and decisive failure
In/out numberIn-state; asymptotically stationary past and futureComplete normalized in/out basesWavepackets or volume normalization; controlled asymptotic regions⟨Nfout⟩\langle N_f^{\mathrm{out}}\rangleOut energy from ωfNf\omega_fN_f plus vacuum and interference terms as applicableAsymptotic occupation; fails without an out splitting
Instantaneous basisState on one slice; chosen canonical variablesTime-local diagonalization or WKB basisAdiabatic order and phase conventionnk(t)n_{\mathbf k}(t)Basis Hamiltonian, not automatically local stress energyDiagnostic occupation; fails as an invariant under time-dependent basis changes
Localized detectorHadamard state; declared worldlineProbe gap and field couplingSmooth switching, spatial profile, perturbative orderExcitation probability or transition rateWork supplied by detector control and trajectoryResponse of that apparatus; fails as pre-existing density when protocol changes it
KMS or detailed balanceStationary state and normalized flowStationary detector or algebra automorphismLong-time or exact KMS domainSpectral ratio e−βΩe^{-\beta\Omega}Equilibrium exchange with respect to the same generatorThermality for that flow; fails for finite transients or a rescaled generator
Stress fluxRenormalizable state; local geometryLocal TμνT_{\mu\nu} and observer or null directionLocally covariant subtraction and boundary data⟨Tμν⟩renuμnν\langle T_{\mu\nu}\rangle_{\mathrm{ren}}u^\mu n^\nuDirect transported energy with source or boundary workLocal flux; fails if subtraction or conservation is uncontrolled
WKB or Stokes productionSpecified in-state and analytic frequency profileComplex turning points and connection matricesSaddle set, Stokes graph, prefactor, uniform errorSemiclassical ∣βk∣2\lvert\beta_{\mathbf k}\rvert^2Compare integrated energy with background workAsymptotic production estimate; fails outside its saddle and asymptotic regime

Continue to Curved Channels, Communication, and Entanglement Harvesting to specify the local couplings and accessible algebras of a communication task.

  • William G. Unruh, “Notes on Black-Hole Evaporation,” Physical Review D 14 (1976), 870–892, DOI.