Energy Computation in Wormhole Background with the Wheeler-DeWitt Operators
Remo Garattini
TL;DR
This paper explores a novel method of calculating energy in wormhole backgrounds using Wheeler-DeWitt operators, applied specifically to three-dimensional wormholes and black hole pair creation, and compares results with existing literature.
Contribution
It introduces a new approach to energy computation in wormhole spacetimes using Wheeler-DeWitt operators, extending previous methods.
Findings
Successful application to three-dimensional wormholes
Comparison with recent literature results
Insights into black hole pair creation
Abstract
We investigate the possibility of computing energy by means of operators associated to the Wheeler-DeWitt equation. By choosing three dimensional wormholes as a framework, we apply such calculation scheme to the black hole pair creation. We compare our results with the recent ones appeared in the literature.
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