A tweaked black hole that looks like Schwarzschild but isn't

In Lorentz gauge theory, the simplest black hole solution resembles Schwarzschild but has its horizon size and surface gravity rescaled by a parameter A₀. Working through the standard toolkit — Eddington-Finkelstein, Kruskal-Szekeres, and Carter-Penrose diagrams — the analysis confirms the causal skeleton is identical to Schwarzschild (same two exteriors, black-hole and white-hole regions), yet the geometry is physically distinct whenever A₀ ≠ 1. This means Lorentz gauge black holes could in principle be distinguished from general-relativistic ones through measurements sensitive to surface gravity or horizon scale.