Life on a closed timelike curve

Abstract We study the internal dynamics of a hypothetical spaceship traveling on a close timelike curve in an axially symmetric Universe. We choose the curve so that the generator of evolution in proper time is the angular momentum. Using Wigner’s theorem, we prove that the energy levels internal to the spaceship must undergo spontaneous discretization. The level separation turns out to be finely tuned so that, after completing a roundtrip of the curve, all systems are back to their initial state. This implies, for example, that the memories of an observer inside the spaceship are necessarily erased by the end of the journey. More in general, if there is an increase in entropy, a Poincaré cycle will eventually reverse it by the end of the loop, forcing entropy to decrease back to its initial value. We show that such decrease in entropy is in agreement with the eigenstate thermalization hypothesis. The non-existence of time-travel paradoxes follows as a rigorous corollary of our analysis.

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Publication Details

Journal
Classical and Quantum Gravity
Published
2024-11-29
DOI
https://doi.org/10.1088/1361-6382/ad98df
Citations
4
Primary Topic
Earth Systems and Cosmic Evolution
Type
article
Field-Weighted Citation Impact
1.51

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article

Life on a closed timelike curve

Lorenzo Gavassino
4 citations
Classical and Quantum Gravity
Earth Systems and Cosmic Evolution
1.51
article

Life on a closed timelike curve

Lorenzo Gavassino
article en
4 citations

Abstract

Abstract We study the internal dynamics of a hypothetical spaceship traveling on a close timelike curve in an axially symmetric Universe. We choose the curve so that the generator of evolution in proper time is the angular momentum. Using Wigner’s theorem, we prove that the energy levels internal to the spaceship must undergo spontaneous discretization. The level separation turns out to be finely tuned so that, after completing a roundtrip of the curve, all systems are back to their initial state. This implies, for example, that the memories of an observer inside the spaceship are necessarily erased by the end of the journey. More in general, if there is an increase in entropy, a Poincaré cycle will eventually reverse it by the end of the loop, forcing entropy to decrease back to its initial value. We show that such decrease in entropy is in agreement with the eigenstate thermalization hypothesis. The non-existence of time-travel paradoxes follows as a rigorous corollary of our analysis.

Classical and Quantum GravityVol. 42(1)
Vanderbilt University (US)
Vanderbilt University
Sustainable cities and communities
Openalex Percentile: Top 19%
Earth Systems and Cosmic Evolution
1.51
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