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Life on a closed timelike curve

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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 Poincar\'{e} 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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2025 1

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Black Holes Rule Out Heavy Tachyons

gr-qc · 2025-01-20 · conditional · novelty 6.0

Heavy tachyons would make black holes evaporate so fast that observing long-lived stellar-mass black holes rules out tachyon masses above about 3 billion GeV.

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  • Black Holes Rule Out Heavy Tachyons gr-qc · 2025-01-20 · conditional · none · ref 2 · internal anchor

    Heavy tachyons would make black holes evaporate so fast that observing long-lived stellar-mass black holes rules out tachyon masses above about 3 billion GeV.