
TL;DR
This paper develops a path integral method to analyze gravitational radiation emitted by quantum bound systems, simplifying calculations by neglecting electromagnetic-gravitational interactions, and confirms previous results for graviton emission intensity.
Contribution
It introduces a novel path integral approach to calculate gravitational radiation from quantum systems in a locally inertial frame, simplifying the analysis.
Findings
Results agree with previous graviton emission intensity calculations.
Method confirms validity of simplified assumptions in gravitational radiation analysis.
Provides a new framework for studying quantum gravitational emissions.
Abstract
A method based on the path integral approach is engaged to consider the gravitational emission from a quantum mechanical bound system in a locally inertial frame. In such a frame, interaction between the electromagnetic (bound potential) and gravitational fields can be neglected resulting in the less mathematical complexity. The final outcome is in agreement with the previous result for the radiation intensity of emitted gravitons due to decay of bound states in TT gauge.
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