"Big Bang" as a first-order phase transition in the early Universe
E.A. Pashitskii

TL;DR
The paper proposes that the Big Bang could be a first-order phase transition triggered by a non-linear scalar field interacting with gravity, leading to rapid universe heating and expansion in the early moments.
Contribution
It introduces a model where a scalar field with a linear term in curvature causes a first-order phase transition, offering a new explanation for the Big Bang's origin.
Findings
First-order phase transition occurs at critical scalar curvature R_c<0.
Rapid transition into potential minimum within 10^{-31} seconds.
Transition releases latent heat raising universe temperature to Planck scale.
Abstract
It is argued that the "Big Bang" initiating the creation of our Universe may be a consequence of a first-order phase transition induced by interaction of a fundamental non-linear scalar field with gravitational field. The Lagrangian describing the scalar field f characterized by "imaginary mass" and nonlinearity of type, existing in the space-time with non-zero scalar curvature , is proposed to be augmented with an additional linear term , along with the standard term quadratic in . The term linear in , playing the role of an "external field", leads to a cubic equation in for the extrema of the potential energy of the scalar field and ensures the possibility of a first-order phase transition driven by the parameter proportional to . It is assumed that the early Universe is filled with non-linear scalar…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Earth Systems and Cosmic Evolution
