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Entropy and Dark Energy

A special issue of Entropy (ISSN 1099-4300). This special issue belongs to the section "Astrophysics, Cosmology, and Black Holes".

Deadline for manuscript submissions: closed (20 November 2022) | Viewed by 2074

Special Issue Editor


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Guest Editor
Department of Engineering and Design, University of Sussex, Brighton BN1 9QT, UK
Interests: information dark energy; space science instrumentation; particle correlation; magnetosphere physics; space weather

Special Issue Information

Dear Colleagues,

The concordance ɅCDM model has been successful in accounting for much of our known universe. However, the model fails to account for some features, such as the Hubble tension and the σ8 fluctuation parameter tension, features that emerged recently as observational accuracy improved. As the required value of the cosmological constant is still without a satisfactory physical explanation and as cold dark matter particles have yet to be detected, we should consider other possible contributions to the universe energy budget. Landauer’s Principle provides us with an equivalent energy for each bit of entropy/information in the universe. This equivalent energy should be taken into account alongside Einstein’s mc2 equivalent energy of matter. The aim of this Special Issue is to collect works which consider the role that information energy can play as a source of dark energy, and also any possible role of information energy in explaining features previously attributed to dark matter.

Subjects of interest include but are not limited to:

  • Landauer’s Principle, information–energy equivalence;
  • Information content of the universe, total information energy in the universe;
  • Astrophysical and cosmological entropy;
  • Information energy as dark energy;
  • Holographic dark energy models;
  • Comparison of information models with observational data;
  • Information equation of state parameter and universe expansion;
  • Information energy as a solution to tensions and problems of ɅCDM;
  • Can the universe information energy distribution explain H0 directional anisotropies?
  • Does the information energy distribution within galaxies coincide with dark matter attributed effects?
  • Information energy predicted experimental observation signatures for model falsification.

Prof. Dr. Michael Paul Gough
Guest Editor

Manuscript Submission Information

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Keywords

  • Landauer’s Principle
  • universe information content
  • universe information energy contributions
  • information dark energy
  • holographic dark energy
  • Hubble tension

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Published Papers (1 paper)

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Research

25 pages, 896 KiB  
Article
Cosmic and Thermodynamic Consequences of Kaniadakis Holographic Dark Energy in Brans–Dicke Gravity
by Sania, Nadeem Azhar, Shamaila Rani and Abdul Jawad
Entropy 2023, 25(4), 576; https://doi.org/10.3390/e25040576 - 27 Mar 2023
Cited by 4 | Viewed by 1312
Abstract
In this manuscript, we investigate the cosmological and thermodynamic aspects of the Brans–Dicke theory of gravity for a spatially flat FRW universe. We consider a theoretical model for interacting Kaniadakis holographic dark energy with the Hubble horizon as the infrared cutoff. We deal [...] Read more.
In this manuscript, we investigate the cosmological and thermodynamic aspects of the Brans–Dicke theory of gravity for a spatially flat FRW universe. We consider a theoretical model for interacting Kaniadakis holographic dark energy with the Hubble horizon as the infrared cutoff. We deal with two interaction scenarios (Q1 and Q2) between Kaniadakis holographic dark energy and matter. In this context, we study different possible aspects of cosmic evolution through some well-known cosmological parameters such as Hubble (H), deceleration (q), jerk (j), and equation of state (ωd). For both interaction terms, it is observed that the deceleration parameter exhibits early deceleration to the current accelerating universe and also lies within the suggested range of Planck data. The equation of state parameter shows quintessence behavior (for the first interaction term) and phantom-like behavior (for the second interaction term) of the universe. The jerk parameter represents consistency with the ΛCDM model for both interaction terms. In the end, we check the thermodynamic behavior of the underlying model. It is interesting to mention here that the generalized second law of thermodynamics holds for both cases of interaction terms. Full article
(This article belongs to the Special Issue Entropy and Dark Energy)
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