Ginzburg-Landau Theory of Dark Energy: A Framework to Study Both Temporal and Spatial Cosmological Tensions Simultaneously
Abdolali Banihashemi, Nima Khosravi, Amir H. Shirazi

TL;DR
This paper introduces a Ginzburg-Landau based dark energy model that simultaneously addresses both temporal tensions like the Hubble constant discrepancy and spatial anomalies in the CMB, offering a unified theoretical framework.
Contribution
The paper develops a novel dark energy model inspired by phase transition theory, capable of explaining multiple cosmological tensions and anomalies within a single unified framework.
Findings
Model resolves H_0 tension and Lyman-alpha anomaly.
Predicts a transition at redshift z_t=0.738.
Proposes a mechanism for CMB anisotropies and alignments.
Abstract
A dark energy model (DE) is proposed based on Ginzburg-Landau theory of phase transition (GLT). This model, GLTofDE, surprisingly provides a framework to study not only temporal tensions in cosmology e.g. tension but also spatial anomalies of CMB e.g. the hemispherical power asymmetry and quadrupole-octopole alignment. In the mean field (or Landau) approximation of GLTofDE, there is a spontaneously symmetry breaking exactly like the Higgs potential. We modeled this transition, phenomenologically, and showed that GLTofDE can resolve both the tension and Lyman- anomaly in a non-trivial way. According to -analysis the transition happens at while km/s/Mpc and which are consistent with the latest reconstructions. In addition, the GLTofDE proposes a framework to address the CMB…
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