What question did this study set out to answer?

To introduce and explore the concept of entropy radiation as proposed by the Acta Universi hypothesis.

January 6, 20260 citationsOpen Access

Entropy emission in the Acta Universi hypothesis

Key Points

To introduce and explore the concept of entropy radiation as proposed by the Acta Universi hypothesis.
Introduced the concept of entropy radiation within the framework of the Acta Universi hypothesis.
Discussed the emission of entropy and electromagnetic radiation from planets.
Analyzed the implications of gravitational-wave anomalies related to entropy emissions.
Proposed that planets emit quanta of accumulated entropy in addition to electromagnetic radiation.
Identified specific frequency ranges for these emissions: 10-1⁵ to 10-3⁰ Hz.
Suggests a detectable gravitational-wave background linked to entropy radiation.

Abstract

For the first time in the history of physics, the Acta Universi hypothesis introduces the concept of entropy radiation — a physical process in which a planet (or any object with a high S_Θ) emits into the surrounding space not only ordinary electromagnetic/gravitational radiation, but also quanta of the accumulated entropy of thought forms in the form of a weak but detectable background. These are radiations in the range of 10-1⁵-10-3⁰ Hz (infra-low frequencies) and anomalies of the gravitational-wave background.

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