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An outward Euclidean exit cannot return

Statement

Let d≥2 and let Θ⊂Rd be a compact obstacle whose exterior Ω=Rd∖Θ has smooth one-sided boundary. Fix R>0 with Θ⊂BR, where BR={z∈Rd:∣z∣<R} and B‾R={z∈Rd:∣z∣≤R}; thus the compact obstacle is contained in the open ball. Quantify over complete unit-speed generalized rays x:R→Ω‾ in the stationary Euclidean generalized-ray convention. In particular, each ray is defined for all forward times. If ∣x(0)∣≤R and ∣x(τ)∣>R at some τ>0, then ∣x(t)∣>R for every t≥τ and ∣x(t)∣→∞ as t→∞.

More precisely, suppose there is L>0 such that every complete admissible ray y with ∣y(0)∣≤R has a time s∈(0,L] satisfying ∣y(s)∣>R. This is the common exterior-hitting bound. Then every such y remains outside B‾R for all t≥L and tends to spatial infinity. Every complete ray initially outside B‾R also eventually remains outside B‾R and tends to spatial infinity. No common time for this last assertion, measured from the initial point outside the ball, is claimed.

Facts & Assumptions

[F1]

The convention of Independent generalized reflected-ray and GCC convention supplies continuous spatial projections of complete rays on R. In the Euclidean interior its Hamilton rule for p=−τ2+∣ξ∣2 keeps τ and ξ constant, with dt/ds=−2τ and dx/ds=2ξ. A nonzero characteristic covector has ∣ξ∣=∣τ∣>0, so physical-time velocity is the constant unit vector −ξ/τ. Its local rules are stationary, so t↦x(q+t) is again a complete admissible ray for every real q. These are properties of the specified complete curves; no extension of an arbitrary ray segment is used.

[F2]

A compact subset of Euclidean space is closed by In a Hausdorff space a point and a disjoint compact set, and two disjoint compact sets, have disjoint open neighbourhoods; hence every compact subset is closed, and in a compact Hausdorff space the compact subsets are exactly the closed ones, since Euclidean space is Hausdorff (distinct points have disjoint balls of radius one third their distance). Hence Ω is open. Every point with ∣z∣≥R is outside Θ and has an obstacle-free neighborhood in Ω. Smoothness of this exterior is assumed explicitly, as required by the generalized-ray convention.

Proof

Given: The smooth compact-obstacle setting and complete rays specified above, and the exterior-hitting bound when proving the consequence. Goal: No return after exit, divergence to infinity, and eventual escape for all initial locations.

1.1givenF1F2algebra

Fix a ray with ∣x(0)∣≤R and ∣x(τ)∣>R. By continuity, the connected component of {t>0:∣x(t)∣>R} containing τ is an interval (a,b) with 0≤a<τ<b≤∞, and ∣x(a)∣=R. Indeed, if a>0 an exterior value at a would extend the component to the left, whereas a strictly interior value would contradict the exterior points immediately to its right; if a=0, continuity and ∣x(0)∣≤R give the same equality. On (a,b) there is no obstacle boundary. The interior rule gives a single constant unit velocity v on this interval: its locally constant velocities agree on overlapping interior intervals, and the interval is connected. Taking the limit at a gives x(a+s)=x(a)+sv for 0<s<b−a. Expanding the squared norm for arbitrarily small positive s shows x(a)⋅v≥0, since a negative value would give ∣x(a+s)∣2=R2+2s x(a)⋅v+s2<R2 for sufficiently small s.

2.1F1step 1.1algebra

If b<∞, the ray is defined and continuous at b by completeness. The line formula from step 1.1 gives ∣x(b)∣2=R2+2(b−a)x(a)⋅v+(b−a)2>R2, contradicting that b is the right endpoint of the exterior component: continuity would put a whole neighborhood of b in the same exterior set. Thus b=∞. The same formula gives ∣x(a+s)∣2≥R2+s2 for all s>0, proving both no return and divergence to infinity. This is an argument about an already complete ray, not a global existence or continuation theorem.

3.1givenstep 1.1step 2.1

Assume the stated common exterior-hitting bound. For any complete ray y initially in B‾R, take its exterior-hitting time s∈(0,L]. Steps 1.1 and 2.1 imply ∣y(t)∣>R for every t≥s, hence for every t≥L, and ∣y(t)∣→∞. The bound is quantified over complete rays themselves, including every admissible branch at glancing, so no uniqueness of a ray from its initial state is needed.

4.1givenF1F2step 3.1∎

Let x instead start outside B‾R. If it never enters B‾R at a nonnegative time, its whole forward path lies in the interior of Ω, so x(t)=x(0)+tv for a fixed unit vector v; the inequality ∣x(0)+tv∣≥t−∣x(0)∣ proves divergence. Otherwise let q be its first entrance time into B‾R. Continuity gives q>0, q<∞ and ∣x(q)∣=R. Stationarity makes y(t)=x(q+t) a complete admissible ray initially in B‾R. Step 3.1 applies, so x remains outside for all t≥q+L and tends to infinity. This proves the asserted consequence for every initial location.

Depends on

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