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Euclidean Preparation and Lorentzian State Dictionaries

A Euclidean path integral that ends on a spatial slice already defines a state wavefunctional on that slice. Gluing embeds this state in a complete complex-time contour and, at saddle level, converts it into Lorentzian classical field and momentum data; the placement of later insertions then selects time-ordered, Wightman, or retarded observables. This page derives that dictionary for a scalar in asymptotically AdSd+1_{d+1}, using standard quantization, a cap source supported away from the join, and source-free linearized Lorentzian evolution.

Required background. Timelike Boundary, Causality, and Boundary-Value Problems supplies the admissible AdS boundary data and symplectic-flux condition. The GKPW Generating-Functional Relation supplies the source convention and Euclidean saddle prescription. States, Geometries, and Radial Quantization supplies the state–operator and energy dictionaries.

Helpful background. Initial Density Matrices and Contour Boundary Conditions explains how a general initial density matrix is encoded on a Schwinger–Keldysh contour.

Here a cap is the oriented Euclidean segment τ∈(−∞,0]\tau\in(-\infty,0] of the complex-time contour, and its join Σ\Sigma is the terminal codimension-one spatial slice at τ=0\tau=0. A corner, when mentioned in the cited real-time construction, is the lower-dimensional intersection of this join with the radial conformal boundary.

Take Euclidean global AdS with boundary-cylinder time τ\tau,

dsE2=L2(cosh⁡2ρ dτ2+dρ2+sinh⁡2ρ dΩd−12),τ≤0,\mathrm ds_E^2=L^2\left( \cosh^2\rho\,\mathrm d\tau^2+\mathrm d\rho^2 +\sinh^2\rho\,\mathrm d\Omega_{d-1}^2\right), \qquad \tau\leq 0,

and a scalar with m2L2=Δ(Δ−d)m^2L^2=\Delta(\Delta-d) on the standard branch Δ>d/2\Delta>d/2. With the GKPW convention ZE[J]=⟨exp⁡(∫JO)⟩Z_E[J]=\langle\exp(\int J\mathcal O)\rangle, the boundary source prepares the unnormalized ket

∣J−⟩=Tτexp⁡ ⁣[∫−∞0dτ dΩ J−(τ,Ω)OE(τ,Ω)]∣0⟩.\lvert J_-\rangle =\mathcal T_\tau\exp\!\left[ \int_{-\infty}^{0}\mathrm d\tau\,\mathrm d\Omega\, J_-(\tau,\Omega)\mathcal O_E(\tau,\Omega) \right]\lvert 0\rangle .

Near the conformal boundary, with defining function z∼2e−ρz\sim2e^{-\rho},

ϕE=zd−ΔJ−(τ,Ω)+zΔA−(τ,Ω)+⋯ .\phi_E =z^{d-\Delta}J_-(\tau,\Omega) +z^\Delta A_-(\tau,\Omega)+\cdots .

The bulk cap path integral is not a single number or a unique endpoint field. It is the functional

ΨJ−bulk[φ]=∫ϕE∣τ=0=φϕE∼zd−ΔJ−regular at the capDϕE e−SE[ϕE].\Psi^{\mathrm{bulk}}_{J_-}[\varphi] = \int_{\substack{\phi_E|_{\tau=0}=\varphi\\ \phi_E\sim z^{d-\Delta}J_-\\ \text{regular at the cap}}} \mathcal D\phi_E\,e^{-S_E[\phi_E]} .

For each fixed endpoint configuration φ\varphi, regularity and J−J_- determine the saddle, when it is unique. The shared endpoint is integrated over—or extremized at leading large NN—only when the cap is glued to the remaining contour. Confusing these two stages incorrectly makes the source appear to fix φ\varphi before gluing. The state/wavefunctional construction and the matching data at contour junctions are developed in Skenderis and van Rees 2009, §2.1 and §2.2.1, pp. 7–11 (Open PDF).

A reflected future cap,

J+(τ,Ω)=J−∗(−τ,Ω),J_+(\tau,\Omega)=J_-^*(-\tau,\Omega),

prepares the adjoint bra. Reflection does not normalize the state: one must still use ∣J^⟩=∣J⟩/⟨J∣J⟩\lvert\widehat J\rangle=\lvert J\rangle/\sqrt{\langle J\vert J\rangle}. Two independent caps instead compute a transition matrix element ⟨Ψ+∣⋯∣Ψ−⟩\langle\Psi_+\rvert\cdots\lvert\Psi_-\rangle; they do not by themselves define a Hermitian, positive, unit-trace density matrix.

The roles of the data are worth separating before doing the continuation:

What each part of the preparation contour fixes
Contour part Data held fixed What it determines
Past Euclidean cap boundary source J− and endpoint field φ ket wavefunctional as a function of φ
Join one shared endpoint field, integrated or extremized compatible classical field and momentum data at saddle level
Lorentzian branch real-time source and later insertions evolution and contour-ordered observables
Reflected future cap the reflected complex-conjugate source the adjoint bra, but not automatic normalization

Use the site’s (+−−−)(+---) convention after continuing τ=it\tau=i t, equivalently t=−iτt=-i\tau. Direct substitution gives

dsE2∣τ=it=−dsL2,dsL2=L2(cosh⁡2ρ dt2−dρ2−sinh⁡2ρ dΩd−12).\left.\mathrm ds_E^2\right|_{\tau=i t}=-\mathrm ds_L^2, \qquad \mathrm ds_L^2=L^2\left( \cosh^2\rho\,\mathrm dt^2-\mathrm d\rho^2 -\sinh^2\rho\,\mathrm d\Omega_{d-1}^2\right).

Let hh be the positive spatial metric on the joining slice and define coordinate momenta along increasing τ\tau and tt by

πE=h NE−1∂τϕE,πL=h NL−1∂tϕL.\pi_E=\sqrt h\,N_E^{-1}\partial_\tau\phi_E, \qquad \pi_L=\sqrt h\,N_L^{-1}\partial_t\phi_L .

The lower boundary of the Lorentzian action and the upper boundary of the Euclidean action contribute

δ ⁣(iSL−SE)∣Σ=−∫Σ(iπL+πE)δφ.\left.\delta\!\left(iS_L-S_E\right)\right|_\Sigma =-\int_\Sigma \left(i\pi_L+\pi_E\right)\delta\varphi .

Stationarity of the joined saddle therefore requires

ϕL(0,ρ,Ω)=ϕE(0,ρ,Ω),πL(0,ρ,Ω)=iπE(0,ρ,Ω),\phi_L(0,\rho,\Omega)=\phi_E(0,\rho,\Omega), \qquad \pi_L(0,\rho,\Omega)=i\pi_E(0,\rho,\Omega),

or ∂tϕL=i∂τϕE\partial_t\phi_L=i\partial_\tau\phi_E when the lapses agree. These signs refer to coordinate momenta along increasing coordinates. If both momenta are instead defined with outward normals, the initial Lorentzian normal is past-directed and an extra minus sign appears. The scalar matching conditions follow directly from the joined variational principle; see Skenderis and van Rees 2009, §§3.1.3–3.1.4, eqs. (3.1.10)–(3.1.15), pp. 16–17 (Open PDF).

For source-free Lorentzian evolution, take J−J_- to vanish in a neighborhood of τ=0\tau=0. Compact support in τ1<τ<τ2<0\tau_1<\tau<\tau_2<0 is a clean choice. The continued field then has no Lorentzian non-normalizable coefficient,

ϕL(z,t,Ω)=zΔAL(t,Ω)+⋯ ,\phi_L(z,t,\Omega)=z^\Delta A_L(t,\Omega)+\cdots ,

so the cap has prepared normalizable initial data rather than a force that remains switched on. A source that reaches or crosses the join must instead be included in the junction analysis or treated as a Lorentzian boundary source. This support condition and the field-plus-momentum matching are the essential ingredients of the real-time prescription Skenderis and van Rees 2008, “Prescription” and “Example,” printed pp. 2–4, eqs. (1)–(5) (Open PDF).

One oscillator exposes the source-to-state map

Section titled “One oscillator exposes the source-to-state map”

Before carrying the normalization into AdS, consider a unit-mass oscillator of frequency ω\omega. Its Euclidean operator is

qE(τ)=12ω(ae−ωτ+a†eωτ).q_E(\tau) =\frac{1}{\sqrt{2\omega}} \left(ae^{-\omega\tau}+a^\dagger e^{\omega\tau}\right).

The cap source J−J_- may be complex. Normal-ordering its Euclidean time-ordered exponential produces a source-dependent scalar factor; the remaining annihilation-operator exponential acts trivially on ∣0⟩\lvert0\rangle. The state is therefore

∣J−⟩∝eαa†∣0⟩,α=Jω2ω,Jω=∫−∞0dτ eωτJ−(τ).\lvert J_-\rangle\propto e^{\alpha a^\dagger}\lvert0\rangle, \qquad \alpha=\frac{\mathcal J_\omega}{\sqrt{2\omega}}, \qquad \mathcal J_\omega =\int_{-\infty}^{0}\mathrm d\tau\, e^{\omega\tau}J_-(\tau).

After normalization this is the exact Glauber coherent state of the free oscillator. With the reflected bra, its Lorentzian one-point function and initial data are

qcl(t)=αe−iωt+α∗eiωt2ω,qcl(0)=Re⁡Jωω,pcl(0)=Im⁡Jω.\begin{aligned} q_{\mathrm{cl}}(t) &=\frac{\alpha e^{-i\omega t}+\alpha^*e^{i\omega t}} {\sqrt{2\omega}},\\ q_{\mathrm{cl}}(0)&=\frac{\operatorname{Re}\mathcal J_\omega}{\omega}, & p_{\mathrm{cl}}(0)&=\operatorname{Im}\mathcal J_\omega . \end{aligned}

Thus the Euclidean source does not become a Lorentzian function by a blind substitution τ→it\tau\to it. Its weighted Laplace moment becomes the complex positive-frequency coefficient, and the real and imaginary parts supply the two real pieces of initial data. A real source gives pcl(0)=0p_{\mathrm{cl}}(0)=0; a source phase supplies nonzero initial momentum. In an interacting theory the same construction defines a state, but exact Glauber coherence receives corrections.

Global-AdS modes are weighted Laplace moments

Section titled “Global-AdS modes are weighted Laplace moments”

Let the scalar harmonics on Sd−1S^{d-1} obey

∫dΩ Yℓσ∗(Ω)Yℓ′σ′(Ω)=δℓℓ′δσσ′,\int\mathrm d\Omega\, Y_{\ell\sigma}^*(\Omega)Y_{\ell'\sigma'}(\Omega) =\delta_{\ell\ell'}\delta_{\sigma\sigma'},

where σ\sigma labels the degeneracy at fixed ℓ\ell. Write the Klein–Gordon-normalized positive-frequency bulk modes and their unit one-particle states as

Unℓσ(t,ρ,Ω)=e−iωnℓtfnℓ(ρ)Yℓσ(Ω),ωnℓ=Δ+2n+ℓ,∣nℓσ⟩=anℓσ†∣0⟩,n=0,1,….\begin{aligned} U_{n\ell\sigma}(t,\rho,\Omega) &=e^{-i\omega_{n\ell}t} f_{n\ell}(\rho)Y_{\ell\sigma}(\Omega),\qquad \omega_{n\ell}=\Delta+2n+\ell,\\ \lvert n\ell\sigma\rangle &=a_{n\ell\sigma}^\dagger\lvert0\rangle,\qquad n=0,1,\ldots . \end{aligned}

Global time and ωnℓ\omega_{n\ell} are dimensionless. Define the normalization rather than hiding it by the one-particle matrix element

⟨nℓσ∣OE(τ,Ω)∣0⟩=κnℓeωnℓτYℓσ∗(Ω).\langle n\ell\sigma\vert \mathcal O_E(\tau,\Omega)\lvert0\rangle =\kappa_{n\ell}e^{\omega_{n\ell}\tau} Y_{\ell\sigma}^*(\Omega).

Rotational symmetry makes κnℓ\kappa_{n\ell} independent of σ\sigma once the harmonic phases and one-particle phases are fixed. The complex conjugate on YℓσY_{\ell\sigma} is essential in a complex harmonic basis. At linear order, the source coupling therefore selects

Jℓσ(τ)=∫dΩ Yℓσ∗(Ω)J−(τ,Ω),J_{\ell\sigma}(\tau) =\int\mathrm d\Omega\, Y_{\ell\sigma}^*(\Omega)J_-(\tau,\Omega),

and prepares

αnℓσ=κnℓ∫−∞0dτ eωnℓτJℓσ(τ),ϕL=∑n,ℓ,σ(αnℓσUnℓσ+αnℓσ∗Unℓσ∗).\begin{aligned} \alpha_{n\ell\sigma} &=\kappa_{n\ell} \int_{-\infty}^{0}\mathrm d\tau\, e^{\omega_{n\ell}\tau}J_{\ell\sigma}(\tau),\\ \phi_L &=\sum_{n,\ell,\sigma} \left( \alpha_{n\ell\sigma}U_{n\ell\sigma} +\alpha_{n\ell\sigma}^*U_{n\ell\sigma}^* \right). \end{aligned}

This operational definition includes the scalar-action prefactor, the boundary limit of the radial mode, and the normalization of O\mathcal O. There is no universal factor 1/(2ωnℓ)1/(2\omega_{n\ell}) once the UnℓσU_{n\ell\sigma} are Klein–Gordon normalized. A source in one angular harmonic (ℓ,σ)(\ell,\sigma) generally excites every radial overtone nn; angular localization is not full normal-mode isolation. The general mode transform appears in Botta-Cantcheff, Martínez, and Silva 2016, §3.1, eqs. (3.7)–(3.10), pp. 6–7, and the explicit coherent-state identification in §4, especially eqs. (4.18) and (4.32)–(4.35), pp. 13–17 (Open PDF).

A compact pulse makes the source-free join condition exact. For one oscillator, or for one projected AdS harmonic before multiplication by its AdS normalization, choose the following continuously differentiable test profile:

J−(τ)={jsin⁡2 ⁣[π(τ−τ1)T],τ1<τ<τ2,0,otherwise,T=τ2−τ1,k=2πT,J_-(\tau)= \begin{cases} j\sin^2\!\left[\dfrac{\pi(\tau-\tau_1)}{T}\right], &\tau_1<\tau<\tau_2,\\[6pt] 0,&\text{otherwise}, \end{cases} \qquad T=\tau_2-\tau_1, \qquad k=\frac{2\pi}{T},

with τ2<0\tau_2<0. Direct integration gives the reproducible source-to-state map

Jω=j k22ω(ω2+k2)(eωτ2−eωτ1),α=Jω2ω.\mathcal J_\omega =j\,\frac{k^2}{2\omega(\omega^2+k^2)} \left(e^{\omega\tau_2}-e^{\omega\tau_1}\right), \qquad \alpha=\frac{\mathcal J_\omega}{\sqrt{2\omega}}.

For the concrete choice τ1=−3/ω\tau_1=-3/\omega and τ2=−1/ω\tau_2=-1/\omega,

Jω=jπ22ω(1+π2)(e−1−e−3).\mathcal J_\omega =\frac{j\pi^2}{2\omega(1+\pi^2)} \left(e^{-1}-e^{-3}\right).

The coherent-state calculation gives

(qcl(0),pcl(0))=(Re⁡Jωω,Im⁡Jω).\left(q_{\mathrm{cl}}(0),p_{\mathrm{cl}}(0)\right) =\left( \frac{\operatorname{Re}\mathcal J_\omega}{\omega}, \operatorname{Im}\mathcal J_\omega \right).

An independent check comes from solving the Euclidean oscillator with the reflected source: the Green function e−ω∣τ−τ′∣/(2ω)e^{-\omega\lvert\tau-\tau'\rvert}/(2\omega) gives the same endpoint position, while the joined derivative gives the same momentum. For any source ending at τ2<0\tau_2<0,

∣Jω∣≤eωτ2∫τ1τ2dτ ∣J−(τ)∣,\left|\mathcal J_\omega\right| \leq e^{\omega\tau_2} \int_{\tau_1}^{\tau_2}\mathrm d\tau\,|J_-(\tau)|,

which bounds the raw Laplace moment. A C∞C^\infty bump with the same support may be used when higher source smoothness matters. Marolf et al. derive the linear source-to-initial-data transform in §§2–3, especially eqs. (31)–(38), pp. 11–13 and analyze the tension between sharp localization and perturbative control in §4.1, especially §§4.1.1–4.1.3, pp. 20–26 (Open PDF).

For an AdS mode whose projected source has the same support, the operational normalization above gives

∣αnℓσ∣≤∣κnℓ∣eωnℓτ2∫τ1τ2dτ ∣Jℓσ(τ)∣.|\alpha_{n\ell\sigma}| \leq |\kappa_{n\ell}|e^{\omega_{n\ell}\tau_2} \int_{\tau_1}^{\tau_2}\mathrm d\tau\, |J_{\ell\sigma}(\tau)|.

A reproducible truncation at ωnℓ≤Ωmax⁡\omega_{n\ell}\leq\Omega_{\max} can monitor both the missed coherent occupation—the Klein–Gordon norm squared of the omitted positive-frequency field—and the missed dimensionless energy:

Ntail(Ωmax⁡)=∑n,ℓ,σωnℓ>Ωmax⁡∣αnℓσ∣2,Ht,tail(Ωmax⁡)=∑n,ℓ,σωnℓ>Ωmax⁡ωnℓ∣αnℓσ∣2,Etail=Ht,tailL.\begin{aligned} N_{\mathrm{tail}}(\Omega_{\max}) &=\sum_{\substack{n,\ell,\sigma\\ \omega_{n\ell}>\Omega_{\max}}} |\alpha_{n\ell\sigma}|^2,\\ H_{t,\mathrm{tail}}(\Omega_{\max}) &=\sum_{\substack{n,\ell,\sigma\\ \omega_{n\ell}>\Omega_{\max}}} \omega_{n\ell}|\alpha_{n\ell\sigma}|^2, \qquad E_{\mathrm{tail}}=\frac{H_{t,\mathrm{tail}}}{L}. \end{aligned}

Each sum includes all nn, ℓ\ell, and degeneracy labels σ\sigma above the cutoff. Declare absolute or retained-relative tolerances for both sums, and stop only when both are met and the join residuals ϕL−ϕE\phi_L-\phi_E and πL−iπE\pi_L-i\pi_E vanish to the same numerical accuracy. The physical approximation separately requires a small dimensionless source-induced field amplitude relative to the nonlinear scale and small total bulk energy for negligible backreaction.

A Gaussian is useful for exposing a common error, but it is not compactly supported. For

J−(τ)=jexp⁡ ⁣[−(τ−τ0)22σ2],τ≤0,J_-(\tau)=j\exp\!\left[-\frac{(\tau-\tau_0)^2}{2\sigma^2}\right], \qquad \tau\leq0,

the exact half-line moment is

Jω=jσπ2 exp⁡ ⁣(ωτ0+ω2σ22)erfc⁡ ⁣(τ0+ωσ22 σ).\mathcal J_\omega =j\sigma\sqrt{\frac{\pi}{2}}\, \exp\!\left( \omega\tau_0+\frac{\omega^2\sigma^2}{2} \right) \operatorname{erfc}\!\left( \frac{\tau_0+\omega\sigma^2}{\sqrt2\,\sigma} \right).

Replacing the half-line by the full Gaussian gives j2πσexp⁡(ωτ0+ω2σ2/2)j\sqrt{2\pi}\sigma\exp(\omega\tau_0+\omega^2\sigma^2/2) only when the shifted saddle τ0+ωσ2\tau_0+\omega\sigma^2 lies many widths below the join. Merely observing that the unweighted Gaussian is small at τ=0\tau=0 is not enough. At fixed τ0\tau_0 and σ\sigma,

Jω∼jωexp⁡ ⁣[−τ022σ2](ω→∞),\mathcal J_\omega \sim \frac{j}{\omega} \exp\!\left[-\frac{\tau_0^2}{2\sigma^2}\right] \qquad (\omega\to\infty),

so the tiny but nonzero endpoint tail eventually dominates. Taper the Gaussian to zero before the join, or restrict it to a declared finite frequency band; otherwise it is not a uniformly ultraviolet-soft, source-free preparation.

An oriented segment of the complex-time path is a branch. Let C1C_1 run forward in Lorentzian time and C2C_2 return backward; along the full closed contour, every point on C2C_2 is later in contour order than every point on C1C_1. Define Gab=⟨TC Oa(t)Ob(t′)⟩\mathcal G_{ab}=\langle\mathcal T_C\,\mathcal O_a(t)\mathcal O_b(t')\rangle without an overall factor of −i-i.

How branch placement selects a real-time two-point function
Placement Correlator Meaning
Both insertions on C1 𝒢11 = GF time ordered
Both insertions on C2 𝒢22 = GF̄ anti-time ordered
First on C1, second on C2 𝒢12 = G< ⟨𝒪(t′)𝒪(t)⟩
First on C2, second on C1 𝒢21 = G> ⟨𝒪(t)𝒪(t′)⟩
Difference of cross-branch responses GR = +i θ(t − t′)[G> − G<] causal response in the site’s source convention

For a two-point function with one insertion fixed at the origin, the boundary value −iτ=t−i0-i\tau=t-i0 gives G>(t)G^>(t), not the time-ordered function. The opposite side gives G<(t)G^<(t), while the Feynman function is piecewise,

−iτ=t−i0 sgn⁡(t).-i\tau=t-i0\,\operatorname{sgn}(t).

With Fourier convention e−ip0t+ip⋅xe^{-ip^0t+i\mathbf p\cdot\mathbf x} and signature (+−−−)(+---), a free scalar illustrates the distinction:

DF(p)=i(p0)2−p2−m2+i0,retarded poles:−1(p0+i0)2−p2−m2.D_F(p)= \frac{i}{(p^0)^2-\mathbf p^2-m^2+i0}, \qquad \text{retarded poles:}\quad -\frac{1}{(p^0+i0)^2-\mathbf p^2-m^2}.

The retarded denominator has both poles below the real p0p^0 axis. A generic CFT correlator uses the corresponding spectral boundary value rather than this simple free pole. Skenderis and van Rees use the opposite Lorentzian source deformation, S↦S−∫JOS\mapsto S-\int J\mathcal O, so their −iθ-i\theta response translates to the +iθ+i\theta convention used here. The branch dictionary and Euclidean boundary values are derived in Skenderis and van Rees 2009, Appendix A.2–A.3, eqs. (A.2.6)–(A.2.10) and (A.3.1)–(A.3.5), pp. 77–80 (Open PDF).

These changes test whether a calculation has retained the state and contour information:

Move jδ(τ−τ0)j\delta(\tau-\tau_0) from the cap to jδ(t−ts)j\delta(t-t_s) on the Lorentzian branch. The cap gives α=jeωτ0/2ω\alpha=je^{\omega\tau_0}/\sqrt{2\omega}. With the site convention S↦S+∫JqS\mapsto S+\int Jq, the real-time impulse instead gives

p(ts+)−p(ts−)=jp(t_s^+)-p(t_s^-)=j

and leaves the state before tst_s unchanged. This disproves the hypothesis that every source insertion prepares the initial state.

For the vacuum oscillator, reversing the Euclidean boundary value changes

G>(t)=e−iωt2ω⟶G<(t)=eiωt2ω.G^>(t)=\frac{e^{-i\omega t}}{2\omega} \quad\longrightarrow\quad G^<(t)=\frac{e^{i\omega t}}{2\omega}.

The two answers are complex conjugates rather than identical. This disproves the hypothesis that the i0i0 side is irrelevant.

Keep ϕL(0)=ϕE(0)\phi_L(0)=\phi_E(0) but omit the momentum condition. One may then add csin⁡(ωt)c\sin(\omega t) without changing the initial field, while shifting the initial momentum by cωc\omega. This disproves the hypothesis that field continuity alone fixes the state.

The surviving claim is narrower and stronger: a source belongs to the state only when it lies on a preparation segment; an observable is fixed only after its contour branch and boundary value are named; and a second-order Lorentzian problem needs both matched initial data.

Exact oscillator coherence holds in a free theory and at generalized-free leading order. At this order, the normal-ordered scalar excitation energy associated with dimensionless global time is

Ht=∑n,ℓ,σωnℓ∣αnℓσ∣2,Ephys=HtL.H_t=\sum_{n,\ell,\sigma} \omega_{n\ell}|\alpha_{n\ell\sigma}|^2, \qquad E_{\mathrm{phys}}=\frac{H_t}{L}.

Large NN suppresses bulk loops, small source amplitude controls the linearization, and fixed-background evolution additionally requires the following dimensionless ratio to be small:

GNHtLd−1=GNEphysLd−2≪1.\frac{G_NH_t}{L^{d-1}} =\frac{G_NE_{\mathrm{phys}}}{L^{d-2}} \ll1.

These are distinct approximations: large NN alone does not remove classical nonlinearities or backreaction. Interactions mix modes and generate noncoherent corrections. A general mixed state requires an explicit initial-density-matrix kernel or an appropriate closed contour, not merely two unrelated caps.

Boundaries and State Preparation develops the underlying path-integral wavefunctional. The prepared normalizable data feed directly into Heavy States, Coherent States, and Semiclassical Geometries. For doubled real-time branches, continue to Schwinger–Keldysh Bulk Geometries and Holographic Initial States and Euclidean Caps.

Treating the endpoint field as source-determined. The source and regularity determine a saddle only after the endpoint φ\varphi has also been specified. Gluing then integrates or extremizes over the shared φ\varphi.

Equating reflection with normalization. A reflected cap supplies the adjoint bra. Divide by the norm when computing normalized expectation values.

Calling an angular harmonic a normal mode. Fixing (ℓ,σ)(\ell,\sigma) still leaves every radial overtone nn. The factors κnℓ\kappa_{n\ell} and the different Laplace weights determine their amplitudes.

Using one i0i0 prescription for every correlator. Feynman, Wightman, and retarded functions are different boundary values or branch combinations. Name the branches before continuing.

For a unit oscillator, let the Euclidean cap end at τ=0\tau=0 and the Lorentzian segment begin at t=0t=0. Using δSE∣0=pEδq\delta S_E|_{0}=p_E\delta q and δSL∣0=−pLδq\delta S_L|_{0}=-p_L\delta q, vary the joined exponent iSL−SEiS_L-S_E and derive the momentum condition. How does the statement change if both momenta are defined with outward normals?

Solution

The shared endpoint value is integrated over, so its coefficient in the saddle variation must vanish:

δ(iSL−SE)∣0=−(ipL+pE)δq=0.\delta(iS_L-S_E)|_0 =-(ip_L+p_E)\delta q=0.

Therefore pL=ipEp_L=i p_E for momenta defined along increasing tt and τ\tau. The outward normal at the initial Lorentzian boundary points toward decreasing tt, so the outward Lorentzian momentum is −pL-p_L; in that convention the relation is pLout=−ipEoutp_L^{\mathrm{out}}=-i p_E^{\mathrm{out}}. The endpoint field itself is continuous because the two path integrals are glued by integrating over one shared qq.

For the compact sin⁡2\sin^2 pulse above, derive Jω\mathcal J_\omega and evaluate it for τ1=−3/ω\tau_1=-3/\omega, τ2=−1/ω\tau_2=-1/\omega.

Solution

Put x=τ−τ1x=\tau-\tau_1 and use sin⁡2(πx/T)=[1−cos⁡(kx)]/2\sin^2(\pi x/T)=[1-\cos(kx)]/2 with k=2π/Tk=2\pi/T. Then

Jω=jeωτ1∫0Tdx eωxsin⁡2 ⁣(πxT)=jeωτ1eωT−12(1ω−ωω2+k2)=j k22ω(ω2+k2)(eωτ2−eωτ1).\begin{aligned} \mathcal J_\omega &=je^{\omega\tau_1} \int_0^T\mathrm dx\,e^{\omega x}\sin^2\!\left(\frac{\pi x}{T}\right)\\ &=je^{\omega\tau_1} \frac{e^{\omega T}-1}{2} \left(\frac1\omega-\frac{\omega}{\omega^2+k^2}\right)\\ &=j\,\frac{k^2}{2\omega(\omega^2+k^2)} \left(e^{\omega\tau_2}-e^{\omega\tau_1}\right). \end{aligned}

For T=2/ωT=2/\omega, k=πωk=\pi\omega, so

Jω=jπ22ω(1+π2)(e−1−e−3).\mathcal J_\omega =\frac{j\pi^2}{2\omega(1+\pi^2)} \left(e^{-1}-e^{-3}\right).

Complete the square to obtain the exact half-line Gaussian transform. State the condition for replacing it by the full-line integral and find the leading large-ω\omega behavior.

Solution

The exponent is

−(τ−τ0)22σ2+ωτ=−(τ−τ0−ωσ2)22σ2+ωτ0+ω2σ22.-\frac{(\tau-\tau_0)^2}{2\sigma^2}+\omega\tau =-\frac{(\tau-\tau_0-\omega\sigma^2)^2}{2\sigma^2} +\omega\tau_0+\frac{\omega^2\sigma^2}{2}.

Changing variables at the upper limit τ=0\tau=0 gives the stated complementary-error-function result. The full-line approximation requires (τ0+ωσ2)/(2σ)≪−1(\tau_0+\omega\sigma^2)/(\sqrt2\sigma)\ll-1. For a large positive argument, erfc⁡x∼e−x2/(πx)\operatorname{erfc}x\sim e^{-x^2}/(\sqrt\pi x), which yields

Jω∼jσ2τ0+ωσ2exp⁡ ⁣[−τ022σ2]∼jωexp⁡ ⁣[−τ022σ2].\mathcal J_\omega \sim \frac{j\sigma^2}{\tau_0+\omega\sigma^2} \exp\!\left[-\frac{\tau_0^2}{2\sigma^2}\right] \sim \frac{j}{\omega} \exp\!\left[-\frac{\tau_0^2}{2\sigma^2}\right].

For the vacuum oscillator, use G>(t)=e−iωt/(2ω)G^>(t)=e^{-i\omega t}/(2\omega) and G<(t)=eiωt/(2ω)G^<(t)=e^{i\omega t}/(2\omega) to compute GR(t)=+iθ(t)[G>(t)−G<(t)]G_R(t)=+i\theta(t)[G^>(t)-G^<(t)]. Explain why neither Wightman function alone is retarded.

Solution

Their difference is −isin⁡(ωt)/ω-i\sin(\omega t)/\omega, so with the convention in the question,

GR(t)=+θ(t)sin⁡(ωt)ω.G_R(t)=+\theta(t)\frac{\sin(\omega t)}{\omega}.

The step function makes the response vanish before the perturbation, while the commutator removes the state-dependent symmetric part. Each Wightman function is nonzero for both signs of tt and therefore is not by itself a causal response. A source convention S↦S−∫JOS\mapsto S-\int J\mathcal O reverses the overall response sign but not the causal support or pole placement.

The chapter overview contains the structure diagram and validity and failure diagram. They are embedded there once so that their shared chapter-level context is not repeated on every article.

For the chapter-wide comparison of assumptions, counterevidence, falsifiers, and claim ceilings, see the claim-domain table.

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