Semi-Classical Holomorphic Transition Amplitudes in Covariant Loop Quantum Gravity

TL;DR

This paper advances covariant loop quantum gravity by developing a semi-classical approximation method for transition amplitudes, enabling better analysis of the Planck star model and addressing conceptual and computational challenges.

Contribution

It introduces a new approximation technique for CLQG transition amplitudes, facilitating semi-classical analysis and tackling longstanding conceptual issues.

Findings

New semi-classical approximation method for CLQG amplitudes

Insights into the cosine problem in quantum gravity

Application to the Planck star model

Abstract

Covariant Loop Quantum Gravity (CLQG) is a tentative background-independent and non-perturbative theory of quantum gravity which has emerged from a number of different research directions. Recently, this theory has been applied to the so-called Planck star model -- a particular model of stellar collapse in which non-perturbative quantum gravity effects play a predominant role. However, several obstacles have impeded progress in the investigation of this scenario. These obstacles range from conceptual issues, such as the question how to extract physical predictions from a background independent theory of quantum gravity, to computational problems due to a lack of systematic methods to evaluate CLQG transition amplitudes. This thesis addresses these problems directly. It contains an analysis of the Planck star model within the framework of CLQG, including a clarifying discussion on relevant conceptual issues. Moreover, a new approximation method for CLQG transition amplitudes is developed. This method allows to systematically study amplitudes in the semi-classical regime of the theory and it sheds new light on the so-called cosine problem.