Radial fall of a test particle onto an evaporating black hole

TL;DR

This paper examines the behavior of a test particle falling into an evaporating black hole, highlighting how black hole evaporation affects the classical understanding of particle infall and horizon crossing.

Contribution

It introduces a simplified model of particle infall into an evaporating black hole, illustrating the impact of black hole evaporation on classical black hole physics.

Findings

Observer sees sudden black hole evaporation during infall

Classical horizon crossing is altered by evaporation effects

Model serves as an educational tool for black hole physics

Abstract

A test particle falling into a classical black hole crosses the event horizon and ends up in the singularity within finite eigentime. In the `more realistic' case of a `classical' evaporating black hole, an observer falling onto a black hole observes a sudden evaporation of the hole. This illustrates the fact that the discussion of the classical process commonly found in the literature may become obsolete when the black hole has a finite lifetime. The situation is basically the same for more complex cases, e.g. where a particle collides with two merging black holes. It should be pointed out that the model used in this paper is mainly of academic interest, since the description of the physics near a black hole horizon still presents a difficult problem which is not yet fully understood, but our model provides a valuable possibility for students to enter the interesting field of black hole physics and to perform numerical calculations of their own which are not very involved from the computational point of view.