Estimates of the total gravitation radiation in the head-on black hole collision

TL;DR

This paper calculates the total gravitational energy emitted during a head-on black hole collision using Robinson-Trautman metrics, providing insights into gravitational wave emission in such extreme events.

Contribution

It introduces a method to estimate gravitational radiation in black hole collisions based on Robinson-Trautman geometries, advancing theoretical understanding.

Findings

Quantitative estimates of gravitational radiation emitted.

Application of Robinson-Trautman metrics to collision scenarios.

Enhanced theoretical framework for gravitational wave predictions.

Abstract

We report on calculations of the total gravitational energy radiated in the head-on black hole collision, where we use the geometry of the Robinson-Trautman metrics.