Unification of Cosmology and Second Law of Thermodynamics: Solving Cosmological Constant Problem, and Inflation
Holger B. Nielsen, Masao Ninomiya

TL;DR
This paper proposes a unification of the second law of thermodynamics with other physical laws by introducing a probabilistic framework based on the imaginary part of the action, addressing the cosmological constant problem and inflation.
Contribution
It introduces a novel probabilistic law behind the second law of thermodynamics using the imaginary part of the action, providing a new approach to cosmological issues without anthropic reasoning.
Findings
Derives the second law from a probabilistic model involving the imaginary action.
Addresses the cosmological constant problem without anthropic principle.
Suggests a model with a dynamical cosmological constant and a two-sided time universe.
Abstract
We seek here to unify the second law of thermodynamics with the other laws, or at least to put up a law behind the second law of thermodynamics. Assuming no fine tuning, concretely by a random Hamiltonian, we argue just from equations of motion -- but {\em without} second law -- that entropy cannot go first up and then down again except with the rather strict restriction S_{large} \le S_{small 1} + S_{small 2}. Here S_{large} is the "large" entropy in the middle era while S_{small 1} and S_{small 2} are the entropies at certain times before and after the S_{large} - era respectively. From this theorem of "no strong maximum for the entropy" a cyclic time S^1 model world could have entropy at the most varying by a factor two and would not be phenomenologically realistic. With an open ended time axis (-\infty, \infty) ={\bf R} some law behind the second law of thermodynamics is needed if…
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