Abstract
It is shown that under a set of straightforward propositions there exists, at the event horizon and at nonzero radii inside the event horizon of a nonrotating, uncharged, spherically symmetric black hole (BH), under reasonable curvature constraints, a nonempty set of virtual exchange particle modes which can propagate to the black hole’s exterior. This finding reveals that a BH event horizon is not a one-way membrane, but instead a limited two-way membrane. The paper’s technology also permits presentation of what is called virtual cosmic censorship, which requires that the aforesaid virtual exchange particle mode propagation tend to zero at the singularity limit.
Notes
See [3] for the definition of the term “\(r\)-coordinate”.
Where \(|0_{M}\rangle\) denotes the vacuum state for a flat (Minkowski) space-time region.
Ref. [22], Sec. 17.4; [14], Box 8-1. This paper will only consider tree-level diagram interactions such as depicted in Fig. 2, without closed loops. However, closed-loop Feynman diagrams and their processes must also conserve the overall momentum (see [14], Sec. 8.4.2, 8.4.5–8.4.6 regarding the virtual photon and closed-loop analysis; also [16], Sec. 6.2).
\(\mathfrak{N}\cap\beta^{+}=\emptyset\).
Considering Eq. (3), it is seen that qf-truncation significantly reduces the amplitude for the occurrence of the subject interaction between the source at \(x_{\textrm{eh}}\) and sink at \(y_{+}\).
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Wolk, B.J. The Black Hole Event Horizon as a Limited Two-Way Membrane. Gravit. Cosmol. 29, 79–87 (2023). https://doi.org/10.1134/S0202289323010139
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DOI: https://doi.org/10.1134/S0202289323010139