Thermodynamic Stability of a Multi-Bubble Cosmological Model
G.Horwitz, O.Fonarev
TL;DR
This paper investigates the thermodynamic stability of a cosmological model featuring multiple bubbles, which can lead to thermal inflation through semi-classical gravitational tunneling.
Contribution
It introduces a multi-bubble cosmological model and analyzes its thermodynamic stability considering semi-classical tunneling effects.
Findings
Multibubble solutions can induce thermal inflation.
The model demonstrates conditions for thermodynamic stability.
Semi-classical tunneling plays a key role in inflationary states.
Abstract
Multibubble solutions for a cosmological model which lead to thermal inflationary states due to a semi-classical tunneling of gravity are calculated.
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Taxonomy
TopicsCosmology and Gravitation Theories · Solar and Space Plasma Dynamics · Geophysics and Gravity Measurements