Abstract

Wavepacket tunneling, in the relativistic limit, is studied via solutions to the Dirac equation for a square barrier potential. Specifically, the arrival time distribution (the time-dependent flux) is computed for wavepackets initiated far away from the barrier, and whose momentum is well below the threshold for above-barrier transmission. The resulting distributions exhibit peaks at shorter times than those of photons with the same initial wavepacket transmitting through a vacuum. However, this apparent superluminality in time is accompanied by very low transmission probabilities. We discuss these observations, and related observations by other authors, in the context of published objections to the notion that tunneling can be superluminal in time. We find that many of these objections are not consistent with our observations, and conclude that post-selected (for transmission) distributions of arrival times can be superluminal. However, the low probability of tunneling means a photon will most likely be seen first and therefore the superluminality does not imply superluminal signaling.

Highlights

  • The phenomenon of quantum tunneling was discovered early on by Hund [1], who considered the spectra of optical isomers, and independently by Mandelstam and Leontowitsch [2], who studied scattering through a barrier potential

  • Could there be a fundamental difference between the tunneling time in a non-relativistic and relativistic theory? This question was addressed by De Leo and Rotelli [34] and separately again a few years later by De Leo [35] using the time-dependent Dirac equation for an electron scattered by a symmetric step potential

  • We find that the resulting time distribution agrees well with conclusions based on the quantum phase time delay

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Summary

September 2020

Keywords: tunneling time, superluminality, time dependent Dirac equation, phase time, momentum filtering Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.

Introduction
The time-dependent Dirac equation
The steepest descent approximation
Numerical evidence for superluminal tunneling transit times
Discussion: interpretations of superluminality in the MacColl–Hartman effect
Final remarks
Full Text
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