The Averaged Null Energy Budget of a Traversable Throat Against the Quantum Inequality

A traversable throat must violate the averaged null energy condition along every ray that passes through it. Quantum field theory permits such violations within limits set by the Ford-Roman inequality, which caps the product of a negative density and the fourth power of its sampling duration. For a one-metre throat crossed at one tenth of light speed over a ten-kilometre internal path, the crossing time is 3.34e-04 seconds, the required averaged deficit is 1.79e+22 in integrated mass-density units, and the inequality allows 1.00e-51: an overrun factor of 1.78e+73. Slower crossings make the overrun worse, not better, because the deficit accumulates while the allowance falls as the inverse cube of the duration. The verdict is plain: within free-field quantum theory, a macroscopic throat open long enough to cross is excluded by the averaged budget, independently of how its exotic matter is sourced. Computed, not measured.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-11-12
DOI
https://doi.org/10.5281/zenodo.24147934
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00
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article

The Averaged Null Energy Budget of a Traversable Throat Against the Quantum Inequality

William Alexander Aldred
Zenodo (CERN European Organization for Nuclear Research)
Black Holes and Theoretical Physics
article

The Averaged Null Energy Budget of a Traversable Throat Against the Quantum Inequality

William Alexander Aldred
article en

Abstract

A traversable throat must violate the averaged null energy condition along every ray that passes through it. Quantum field theory permits such violations within limits set by the Ford-Roman inequality, which caps the product of a negative density and the fourth power of its sampling duration. For a one-metre throat crossed at one tenth of light speed over a ten-kilometre internal path, the crossing time is 3.34e-04 seconds, the required averaged deficit is 1.79e+22 in integrated mass-density units, and the inequality allows 1.00e-51: an overrun factor of 1.78e+73. Slower crossings make the overrun worse, not better, because the deficit accumulates while the allowance falls as the inverse cube of the duration. The verdict is plain: within free-field quantum theory, a macroscopic throat open long enough to cross is excluded by the averaged budget, independently of how its exotic matter is sourced. Computed, not measured.

Zenodo (CERN European Organization for Nuclear Research)
Black Holes and Theoretical Physics
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