PhilArchive
open access
Image-Sum Stress-Energy and Multi-Horizon Structure on the Flat Helical Zn Spacetime
We study a free scalar field on flat 4-dimensional Minkowski spacetime with a Zn helical identification (t, r, ϕ) ∼ (t − l/n, r, ϕ + 2π/n), the minimal exactly solvable model carrying the topological structure of the Zn helical identification program of Refs. [1–3]. Using the method of images we obtain ⟨Tμν⟩ren in closed form. Three results are established. (i) Multi-horizon structure (principal result). For n ≥ 3 the identification produces n − 1 distinct chronology horizons at rc,j = jl/(2n sin(πj/n)), j = 1, . . . , n − 1, and we prove analytically that rc,1 < rc,2 < · · · < rc,n−1, so the horizons are separated in radius and do not accumulate. This has no analogue in single-horizon Misner space. (ii) Invariant-sector weight. Near each rc,j the renormalized stress-energy diverges as σ−2 j ; in the Zn-invariant sector each divergence enters with the projector weight 1/n, and at leading UV order the real invariant-sector energy density equals 1/n times the unrestricted density on the same torus, because the n−1 twisted Fourier sums are purely imaginary [Li−2(e2πij/n) ∈ iR, proved inline]. (iii) The divergence is not removed. The 1/n is a weight on a still-divergent quantity. Consistently with the Kay–Radzikowski–Wald theorem [5], the construction redistributes and re-weights the divergence across n − 1 horizons but does not evade chronology protection. We note that Cramer–Kay [9] proved singularity persists for automorphic fields (all modes present, acquiring phase factors eiθ under the identification); the Zn-projected sector studied here (modes with k ̸≡ m (mod n) absent from the Hilbert space entirely) is a mathematically distinct object, and Cramer– Kay does not apply to it directly. The flat model fixes the topological weight in a fully controlled QFTCS setting; the curved Ori background, with frame-dragging β(r, θ) = −Ω1r2 sinh2 θ solved in the companion paper, carries additional O(β) corrections that are not addressed here. Version note (v4). The mode constraint is corrected to k ≡ m (mod n) (the n = 2 case reduces to k + m ≡ 0 (mod 2)); the 1/n claim is restated as an invariant-sector weight rather than a suppression of the divergence; the Li−2 identity is proved inline; and the corrected Table I values of v2 are retained.
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Quantitative QFTCS Calculation of the Doubly Suppressed KRW Divergence in the Helically Identified Kerr Interior#725776
- Black-Hole First Laws and Horizon Constraints: A Differential Rank Criterion#1122595
- On the Inevitability of Horizon Formation in Gravitational Collapse: A Rigorous Proof of the Weak Cosmic Censorship Conjecture#723040
- Unitary evolution of an evaporating black hole in canonical quantum gravity#1071171
- On the Origin of General Relativity - A projection-based derivation from information geometry#78756
Record · ID 729738
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive