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Open String Boundary Variation

Physical scope

Classical X-variation of the free Polyakov action on a smooth Lorentzian open strip with no endpoint interaction; no endpoint dynamics or D-brane claim.

Statement

Let Σ=I×[0,π] be a smooth Lorentzian strip with dimensionless coordinates (τ,σ), where I=[τi,τf], and let X∈C2(Σ,R1,D−1) and h∈C1 be the fields of the adopted free Polyakov model, with nondegenerate h of signature (−,+). Assume there is no boundary interaction and that variations vanish on the initial and final time slices. Define Cμ:=−det⁡h hσb∂bXμ and [F]0π:=F(τ,π)−F(τ,0). The X-variation has bulk term T∫ΣδXμ ∂a(−det⁡h hab∂bXμ) d2σ and spatial-boundary flux −T∫I[CμδXμ]0π dτ. This coordinate-density expression applies without a causal-type assumption on the spatial faces. If those faces are timelike for h, equivalently hττ<0 there, put ε=+1 at σ=π and ε=−1 at σ=0, na=ε(dσ)a/hσσ, and ds=−hττ dτ. Then n is the outward unit spacelike conormal and the same flux is −T∫∂Σspatialds nahab∂bXμ δXμ. For each endpoint and target component, Dirichlet data δXμ=0 or natural Neumann data Cμ=0 suffice to annihilate the flux; coordinatewise mixed choices are allowed. On timelike faces the Neumann condition is equivalently nahab∂bXμ=0 for that component. In conformal gauge on the flat strip it reduces to ∂σXμ=0.

Facts & Assumptions

Given: The flat-target model, ℏ=c=1, T=1/(2πα′)>0, the adopted Polyakov action, and variations δX that vanish at τi,τf.

[F1]

Flat Bosonic String Model: X is C2, h is the Lorentzian worldsheet metric, and the open strip has σ∈[0,π] with dimensionless coordinates.

[F2]

String Tension Alpha Prime: T=(2πα′)−1>0.

[A1]

Bosonic Polyakov Model: the adopted action is SP=−T2∫Σ−h hab∂aX⋅∂bX, with no boundary interaction.

[F3]

Conformal Gauge and Residual Symmetry: on the flat strip conformal-gauge patch hab=e2ϕdiag⁡(−1,+1).

Proof

1.1givenA1F2algebra

Varying X in [A1] while holding h fixed gives δSP=−T∫Σ−h hab∂aXμ ∂bδXμ d2σ, because hab is symmetric; [F2] fixes the positive coefficient T=(2πα′)−1.

2.1givenF1step 1.1algebra

Integrate the divergence ∂b(−det⁡h hab∂aXμ δXμ) over the coordinate rectangle. The fundamental theorem of calculus in each variable gives the interior term T∫ΣδXμ ∂b(−det⁡h hab∂aXμ)d2σ and the spatial term −T∫I[CμδXμ]0πdτ; the temporal terms vanish by the Given clause. No unit normal is used in this calculation. On a timelike face, the two-dimensional inverse formula gives hσσ=hττ/det⁡h>0. Thus habnanb=1 and ds na=ε−det⁡h(dσ)a dτ, proving the stated proper-time form on precisely those faces.

3.1givenstep 2.1algebra

For each component and each endpoint, Dirichlet data make the corresponding δXμ factor zero; Neumann data Cμ=0 make its coordinate-density flux coefficient zero; on a timelike face the positive normalizing factors give exactly the equivalent unit-conormal condition. The sum of these endpoint integrands therefore vanishes for coordinatewise mixed choices as well.

4.1F3step 3.1algebra∎

In the conformal gauge [F3], hττ=−e2ϕ<0 and Cμ=∂σXμ. The unit conormal at constant σ is na=±eϕ(dσ)a, so nahab∂bXμ=±e−ϕ∂σXμ. Thus the natural condition is equivalent to ∂σXμ=0.

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