Symmetry in Cosmological Theories and Observations

A special issue of Symmetry (ISSN 2073-8994). This special issue belongs to the section "Physics".

Deadline for manuscript submissions: 30 November 2024 | Viewed by 986

Special Issue Editors


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Guest Editor
Department of Physics, Institute of Basic Science, Sungkyunkwan University, Suwon 16419, Republic of Korea
Interests: dark energy; modified gravity theories; varying speed of light; cosmic microwave background; gravitational waves; cosmological phenomena

E-Mail Website
Guest Editor
Department of Science Education, Jeju National University, Jeju 63243, Republic of Korea
Interests: early universe and late-time cosmology including inflation and dark energy; modified theories of gravity; gravitational waves; black holes

Special Issue Information

Dear Colleagues, 

We are delighted to announce the launch of this Special Issue titled "Symmetry in Cosmological Theories and Observations". The field of cosmology has witnessed remarkable advancements in recent years, reshaping our understanding of the Universe. As cosmological research continues to evolve, it permeates various aspects of science, revolutionizing our comprehension of the cosmos and enhancing our interaction with fundamental physical laws. The study of symmetry and asymmetry plays a pivotal role in diverse domains, ranging from the early Universe, dark matter, and dark energy to cosmic microwave background radiation, gravitational waves, and galaxy formation. The synergy of theoretical advancements, observational data, and increasingly powerful computational methods enables us to push the boundaries of what is attainable and sets the stage for future breakthroughs. This Special Issue aims to explore the profound impact of symmetry (and asymmetry) in cosmological theories and observations, shedding light on emerging trends and cutting-edge research. We invite researchers from the fields of cosmology and astrophysics to contribute their innovative works in the following areas: 

  • Inflationary models and primordial symmetries;
  • Symmetry breaking in the early Universe;
  • Dark matter and dark energy models;
  • Cosmic microwave background radiation;
  • Gravitational waves and their implications for symmetry;
  • Galaxy formation and the large-scale structure of the Universe;
  • Baryogenesis and leptogenesis;
  • Symmetries in high-energy astrophysics;
  • Black holes and their symmetries;
  • Tests of fundamental symmetries using astronomical observations;
  • Symmetry principles in modified gravity theories;
  • Topological defects and cosmic strings;
  • Symmetry in the context of cosmological models;
  • Constraints on symmetry from cosmological data;
  • Symmetries in the evolution of the Universe;
  • The role of symmetry in cosmological perturbations;
  • Asymmetry in cosmic baryon and lepton numbers;
  • Probing cosmological symmetries with next-generation observatories. 

We encourage researchers to submit their original research articles, reviews, or perspectives that explore the role of symmetry (and asymmetry) in cosmological theories and observations. This Special Issue provides an opportunity to share novel insights, methodologies, and applications that will shape the future of the field.

Prof. Dr. Seokcheon Lee
Dr. Gansukh Tumurtushaa
Guest Editors

Manuscript Submission Information

Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 100 words) can be sent to the Editorial Office for announcement on this website.

Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Symmetry is an international peer-reviewed open access monthly journal published by MDPI.

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Keywords

  • inflationary models and primordial symmetries
  • symmetry breaking in the early Universe
  • dark matter and dark energy models
  • cosmic microwave background radiation
  • gravitational waves and their implications for symmetry
  • galaxy formation and the large-scale structure of the Universe
  • baryogenesis and leptogenesis
  • symmetries in high-energy astrophysics
  • black holes and their symmetries
  • tests of fundamental symmetries using astronomical observations
  • symmetry principles in modified gravity theories
  • topological defects and cosmic strings
  • constraints on symmetry from cosmological data
  • symmetries in the evolution of the universe
  • role of symmetry in cosmological perturbations
  • asymmetry in cosmic baryon and lepton numbers
  • probing cosmological symmetries with next-generation observatories

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Published Papers (1 paper)

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Research

15 pages, 1931 KiB  
Article
Observational Constraints and Cosmographic Analysis of f(T,TG) Gravity and Cosmology
by Harshna Balhara, Jainendra Kumar Singh, Shaily and Emmanuel N. Saridakis
Symmetry 2024, 16(10), 1299; https://doi.org/10.3390/sym16101299 - 2 Oct 2024
Cited by 7 | Viewed by 794
Abstract
We perform observational confrontation and cosmographic analysis of f(T,TG) gravity and cosmology. This higher-order torsional gravity is based on both the torsion scalar, as well as on the teleparallel equivalent of the Gauss–Bonnet combination, and gives rise [...] Read more.
We perform observational confrontation and cosmographic analysis of f(T,TG) gravity and cosmology. This higher-order torsional gravity is based on both the torsion scalar, as well as on the teleparallel equivalent of the Gauss–Bonnet combination, and gives rise to an effective dark-energy sector which depends on the extra torsion contributions. We employ observational data from the Hubble function and supernova Type Ia Pantheon datasets, applying a Markov chain Monte Carlo sampling technique, and we provide the iso-likelihood contours, as well as the best-fit values for the parameters of the power-law model, an ansatz which is expected to be a good approximation of most realistic deviations from general relativity. Additionally, we reconstruct the effective dark-energy equation-of-state parameter, which exhibits a quintessence-like behavior, while in the future the Universe enters into the phantom regime, before it tends asymptotically to the cosmological constant value. Furthermore, we perform a detailed cosmographic analysis, examining the deceleration, jerk, snap, and lerk parameters, showing that the transition to acceleration occurs in the redshift range 0.52ztr0.89, as well as the preference of the scenario for quintessence-like behavior. Finally, we apply the Om diagnostic analysis to cross-verify the behavior of the obtained model. Full article
(This article belongs to the Special Issue Symmetry in Cosmological Theories and Observations)
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