Abstract

We extend previous work on the numerical diagonalization of quantum stress tensor operators in the Minkowski vacuum state, which considered operators averaged in a finite time interval, to operators averaged in a finite spacetime region. Since real experiments occur over finite volumes and durations, physically meaningful fluctuations may be obtained from stress tensor operators averaged by compactly supported sampling functions in space and time. The direct diagonalization, via a Bogoliubov transformation, gives the eigenvalues and the probabilities of measuring those eigenvalues in the vacuum state, from which the underlying probability distribution can be constructed. For the normal-ordered square of the time derivative of a massless scalar field in a spherical cavity with finite degrees of freedom, analysis of the tails of these distributions confirms previous results based on the analytical treatment of the high moments. We find that the probability of large vacuum fluctuations is reduced when spatial averaging is included, but the tail still decreases more slowly than exponentially as the magnitude of the measured eigenvalues increases, suggesting vacuum fluctuations may not always be subdominant to thermal fluctuations and opening up the possibility of experimental observation under the right conditions.

Highlights

  • We extend previous work on the numerical diagonalization of quantum stress tensor operators in the Minkowski vacuum state, which considered operators averaged in a finite time interval, to operators averaged in a finite spacetime region

  • Since real experiments occur over finite volumes and durations, physically meaningful fluctuations may be obtained from stress tensor operators averaged by compactly supported sampling functions in space and time

  • The semiclassical theory of gravity, where matter fields are treated as quantum fields, whereas the gravitational field is treated as a classical field, deals with the expectation value of the energy-momentum tensor operator of the matter fields as an approximation to a full theory of quantum gravity [1]

Read more

Summary

INTRODUCTION

The semiclassical theory of gravity, where matter fields are treated as quantum fields, whereas the gravitational field is treated as a classical field, deals with the expectation value of the energy-momentum tensor operator of the matter fields as an approximation to a full theory of quantum gravity [1]. The moments approach applied to quantum stress tensor operators averaged over finite time intervals is further developed in Ref. Large quantum fluctuations of the time derivative of a scalar field averaged over a finite spacetime region lead to a decay rate comparable with the standard rate from the instanton approximation [22]. For operators that are quadratic in the time derivative of a scalar field, the probability distribution falls slower than an exponential function, in which case the decay rate is governed by these quadratic field fluctuations rather than quantum tunneling and linear field fluctuations. Units in which the reduced Planck constant and the speed of light are equal to unity, ħ 1⁄4 c 1⁄4 1, are used throughout the paper

PROBABILITY DISTRIBUTIONS OF QUANTUM STRESS TENSOR OPERATORS
General procedure
Specific case
Construction and approximation of fðωÞ
Construction of gðrÞ or gðkÞ
Averaging PðxÞ
PðxjÞ: j ð79Þ
Results
Findings
OUTLOOK AND DISCUSSION
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call