What question did this study set out to answer?

This research aims to compare the entropy of habitable and uninhabited planets within the AUfield hypothesis framework.

January 6, 20260 citationsOpen Access

Comparison of the entropy of an uninhabited and habitable planet in the Acta Universi hypothesis

Key Points

This research aims to compare the entropy of habitable and uninhabited planets within the AUfield hypothesis framework.
Analysis of entropy measures on habitable and uninhabited planets based on the AUfield hypothesis.
Consideration of biological processes versus geological events to quantify entropy production.
Review of relevant data from astrobiology studies to support findings.
Habitable planets exhibit entropy production rates of 10^{30}-10^{50} events/s due to life forms.
Uninhabited planets are limited to 10^{20} events/s due to geological and atmospheric processes.
The data supports the notion that entropy production correlates with the presence of life, labeling these planets as 'thermodynamically alive'.

Abstract

In the Acta Universi (AUfield) hypothesis of D. E. Yashchenko (2025), entropy is a measure of irreversible events recorded in the universal archive of the AU field. On a habitable planet (with life forms), entropy is radically higher due to biological processes (DNA replication, metabolism, consciousness) that generate 10^30-10^50 events/s. On an uninhabited planet (without life), entropy is limited by geological / atmospheric events (erosion, volcanism, ~10 ^ 20 events/s). This is consistent with data from astrobiology 2025: habitable planets have higher entropy production (PEP), which makes them "thermodynamically alive" (Universe Today, 2023; Astrobiology, 2024).

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Dmitry Yashchenko (Sun,) studied this question.

synapsesocial.com/papers/695d855e3483e917927a4c6b https://doi.org/https://doi.org/10.5281/zenodo.18143568

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