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  1. Quantum Mechanics, Formalization and the Cosmological Constant Problem.Jerzy Król & Torsten Asselmeyer-Maluga - 2020 - Foundations of Science 25 (4):879-904.
    Based on formal arguments from Zermelo–Fraenkel set theory we develop the environment for explaining and resolving certain fundamental problems in physics. By these formal tools we show that any quantum system defined by an infinite dimensional Hilbert space of states interferes with the spacetime structure M. M and the quantum system both gain additional degrees of freedom, given by models of Zermelo–Fraenkel set theory. In particular, M develops the ground state where classical gravity vanishes. Quantum mechanics distinguishes set-theoretic random forcing (...)
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  • Random World and Quantum Mechanics.Jerzy Król, Krzysztof Bielas & Torsten Asselmeyer-Maluga - 2023 - Foundations of Science 28 (2):575-625.
    Quantum mechanics (QM) predicts probabilities on the fundamental level which are, via Born probability law, connected to the formal randomness of infinite sequences of QM outcomes. Recently it has been shown that QM is algorithmic 1-random in the sense of Martin–Löf. We extend this result and demonstrate that QM is algorithmic $$\omega$$ -random and generic, precisely as described by the ’miniaturisation’ of the Solovay forcing to arithmetic. This is extended further to the result that QM becomes Zermelo–Fraenkel Solovay random on (...)
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  • Topology and models of ZFC at early Universe.Jerzy Król & Torsten Asselmeyer-Maluga - 2019 - Philosophical Problems in Science 66:15-33.
    Recently the cosmological evolution of the universe has been considered where 3-dimensional spatial topology undergone drastic changes. The process can explain, among others, the observed smallness of the neutrino masses and the speed of inflation. However, the entire evolution is perfectly smooth from 4-dimensional point of view. Thus the raison d’être for such topology changes is the existence of certain non-standard 4-smoothness on R4 already at very early stages of the universe. We show that the existence of such smoothness can (...)
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