Sign in to use this feature.

Years

Between: -

Subjects

remove_circle_outline
remove_circle_outline
remove_circle_outline
remove_circle_outline
remove_circle_outline
remove_circle_outline
remove_circle_outline
remove_circle_outline
remove_circle_outline

Journals

Article Types

Countries / Regions

remove_circle_outline
remove_circle_outline
remove_circle_outline
remove_circle_outline
remove_circle_outline

Search Results (762)

Search Parameters:
Keywords = cosmological model

Order results
Result details
Results per page
Select all
Export citation of selected articles as:
8 pages, 342 KiB  
Article
Should the Evolution of Our Universe Be Treated as an Initial Value Problem?
by Martin Tamm
Symmetry 2025, 17(8), 1258; https://doi.org/10.3390/sym17081258 - 7 Aug 2025
Viewed by 170
Abstract
In classical physics, the traditional way to handle dynamics is to work with initial value problems: Specifying all variables and their time-derivatives at a certain time will, together with the equations of motion, give the state of the system at any time. In [...] Read more.
In classical physics, the traditional way to handle dynamics is to work with initial value problems: Specifying all variables and their time-derivatives at a certain time will, together with the equations of motion, give the state of the system at any time. In this paper, it is questioned whether this is the right way to treat cosmology. The main reason is that cosmology, as opposed to almost all other parts of physics, deals with genuinely global problems. The main example in this paper will be the accelerating expansion. It is not claimed that the model studied here gives any kind of final explanation of this phenomenon. Nevertheless, it shows that what is commonly interpreted as the result of some dark energy, could instead be the result of a global condition for the universe. This model cannot be treated as a classical initial value problem. But an interesting additional property is that it can explain why the rate of acceleration now seems to be decreasing with time. Full article
(This article belongs to the Special Issue Feature Papers in 'Physics' Section 2025)
Show Figures

Figure 1

29 pages, 430 KiB  
Article
Advanced Manifold–Metric Pairs
by Pierros Ntelis
Mathematics 2025, 13(15), 2510; https://doi.org/10.3390/math13152510 - 4 Aug 2025
Viewed by 259
Abstract
This article presents a novel mathematical formalism for advanced manifold–metric pairs, enhancing the frameworks of geometry and topology. We construct various D-dimensional manifolds and their associated metric spaces using functional methods, with a focus on integrating concepts from mathematical physics, field theory, topology, [...] Read more.
This article presents a novel mathematical formalism for advanced manifold–metric pairs, enhancing the frameworks of geometry and topology. We construct various D-dimensional manifolds and their associated metric spaces using functional methods, with a focus on integrating concepts from mathematical physics, field theory, topology, algebra, probability, and statistics. Our methodology employs rigorous mathematical construction proofs and logical foundations to develop generalized manifold–metric pairs, including homogeneous and isotropic expanding manifolds, as well as probabilistic and entropic variants. Key results include the establishment of metrizability for topological manifolds via the Urysohn Metrization Theorem, the formulation of higher-rank tensor metrics, and the exploration of complex and quaternionic codomains with applications to cosmological models like the expanding spacetime. By combining spacetime generalized sets with information-theoretic and probabilistic approaches, we achieve a unified framework that advances the understanding of manifold–metric interactions and their physical implications. Full article
11 pages, 317 KiB  
Article
Phenomenological Charged Extensions of the Quantum Oppenheimer–Snyder Collapse Model
by S. Habib Mazharimousavi
Universe 2025, 11(8), 257; https://doi.org/10.3390/universe11080257 - 4 Aug 2025
Viewed by 188
Abstract
This work presents a semi-classical, quantum-corrected model of gravitational collapse for a charged, spherically symmetric dust cloud, extending the classical Oppenheimer–Snyder (OS) framework through loop quantum gravity effects. Our goal is to study phenomenological quantum modifications to geometry, without necessarily embedding them within [...] Read more.
This work presents a semi-classical, quantum-corrected model of gravitational collapse for a charged, spherically symmetric dust cloud, extending the classical Oppenheimer–Snyder (OS) framework through loop quantum gravity effects. Our goal is to study phenomenological quantum modifications to geometry, without necessarily embedding them within full loop quantum gravity (LQG). Building upon the quantum Oppenheimer–Snyder (qOS) model, which replaces the classical singularity with a nonsingular bounce via a modified Friedmann equation, we introduce electric and magnetic charges concentrated on a massive thin shell at the boundary of the dust ball. The resulting exterior spacetime generalizes the Schwarzschild solution to a charged, regular black hole geometry akin to a quantum-corrected Reissner–Nordström metric. The Israel junction conditions are applied to match the interior APS (Ashtekar–Pawlowski–Singh) cosmological solution to the charged exterior, yielding constraints on the shell’s mass, pressure, and energy. Stability conditions are derived, including a minimum radius preventing full collapse and ensuring positivity of energy density. This study also examines the geodesic structure around the black hole, focusing on null circular orbits and effective potentials, with implications for the observational signatures of such quantum-corrected compact objects. Full article
Show Figures

Figure 1

26 pages, 4349 KiB  
Article
Palazzo Farnese and Dong’s Fortified Compound: An Art-Anthropological Cross-Cultural Analysis of Architectural Form, Symbolic Ornamentation, and Public Perception
by Liyue Wu, Qinchuan Zhan, Yanjun Li and Chen Chen
Buildings 2025, 15(15), 2720; https://doi.org/10.3390/buildings15152720 - 1 Aug 2025
Viewed by 283
Abstract
This study presents a cross-cultural comparison of two fortified residences—Palazzo Farnese in Italy and Dong’s Fortified Compound in China—through a triadic analytical framework encompassing architectural form, symbolic ornamentation, and public perception. By combining field observation, iconographic interpretation, and digital ethnography, the research investigates [...] Read more.
This study presents a cross-cultural comparison of two fortified residences—Palazzo Farnese in Italy and Dong’s Fortified Compound in China—through a triadic analytical framework encompassing architectural form, symbolic ornamentation, and public perception. By combining field observation, iconographic interpretation, and digital ethnography, the research investigates how heritage meaning is constructed, encoded, and reinterpreted across distinct sociocultural contexts. Empirical materials include architectural documentation, decorative analysis, and a curated dataset of 4947 user-generated images and 1467 textual comments collected from Chinese and international platforms between 2020 and 2024. Methods such as CLIP-based visual clustering and BERTopic-enabled sentiment modelling were applied to extract patterns of perception and symbolic emphasis. The findings reveal contrasting representational logics: Palazzo Farnese encodes dynastic authority and Renaissance cosmology through geometric order and immersive frescoes, while Dong’s Compound conveys Confucian ethics and frontier identity via nested courtyards and traditional ornamentation. Digital responses diverge accordingly: international users highlight formal aesthetics and photogenic elements; Chinese users engage with symbolic motifs, family memory, and ritual significance. This study illustrates how historically fortified residences are reinterpreted through culturally specific digital practices, offering an interdisciplinary approach that bridges architectural history, symbolic analysis, and digital heritage studies. Full article
(This article belongs to the Section Architectural Design, Urban Science, and Real Estate)
Show Figures

Figure 1

11 pages, 961 KiB  
Article
Viscous Cosmology in f(Q,Lm) Gravity: Insights from CC, BAO, and GRB Data
by Dheeraj Singh Rana, Sai Swagat Mishra, Aaqid Bhat and Pradyumn Kumar Sahoo
Universe 2025, 11(8), 242; https://doi.org/10.3390/universe11080242 - 23 Jul 2025
Viewed by 272
Abstract
In this article, we investigate the influence of viscosity on the evolution of the cosmos within the framework of the newly proposed f(Q,Lm) gravity. We have considered a linear functional form [...] Read more.
In this article, we investigate the influence of viscosity on the evolution of the cosmos within the framework of the newly proposed f(Q,Lm) gravity. We have considered a linear functional form f(Q,Lm)=αQ+βLm with a bulk viscous coefficient ζ=ζ0+ζ1H for our analysis and obtained exact solutions to the field equations associated with a flat FLRW metric. In addition, we utilized Cosmic Chronometers (CC), CC + BAO, CC + BAO + GRB, and GRB data samples to determine the constrained values of independent parameters in the derived exact solution. The likelihood function and the Markov Chain Monte Carlo (MCMC) sampling technique are combined to yield the posterior probability using Bayesian statistical methods. Furthermore, by comparing our results with the standard cosmological model, we found that our considered model supports the acceleration of the universe in late time. Full article
Show Figures

Figure 1

13 pages, 793 KiB  
Communication
Gamma-Ray Bursts Calibrated by Using Artificial Neural Networks from the Pantheon+ Sample
by Zhen Huang, Xin Luo, Bin Zhang, Jianchao Feng, Puxun Wu, Yu Liu and Nan Liang
Universe 2025, 11(8), 241; https://doi.org/10.3390/universe11080241 - 23 Jul 2025
Viewed by 158
Abstract
In this paper, we calibrate the luminosity relation of gamma−ray bursts (GRBs) by employing artificial neural networks (ANNs) to analyze the Pantheon+ sample of type Ia supernovae (SNe Ia) in a manner independent of cosmological assumptions. The A219 GRB dataset is used to [...] Read more.
In this paper, we calibrate the luminosity relation of gamma−ray bursts (GRBs) by employing artificial neural networks (ANNs) to analyze the Pantheon+ sample of type Ia supernovae (SNe Ia) in a manner independent of cosmological assumptions. The A219 GRB dataset is used to calibrate the Amati relation (Ep-Eiso) at low redshift with the ANN framework, facilitating the construction of the Hubble diagram at higher redshifts. Cosmological models are constrained with GRBs at high redshift and the latest observational Hubble data (OHD) via the Markov chain Monte Carlo numerical approach. For the Chevallier−Polarski−Linder (CPL) model within a flat universe, we obtain Ωm=0.3210.069+0.078h=0.6540.071+0.053w0=1.020.50+0.67, and wa=0.980.58+0.58 at the 1 −σ confidence level, which indicates a preference for dark energy with potential redshift evolution (wa0). These findings using ANNs align closely with those derived from GRBs calibrated using Gaussian processes (GPs). Full article
Show Figures

Figure 1

23 pages, 556 KiB  
Review
Evolving Wormholes in a Cosmological Background
by Mahdi Kord Zangeneh and Francisco S. N. Lobo
Universe 2025, 11(7), 236; https://doi.org/10.3390/universe11070236 - 19 Jul 2025
Viewed by 221
Abstract
Wormholes are non-trivial topological structures that arise as exact solutions to Einstein’s field equations, theoretically connecting distinct regions of spacetime via a throat-like geometry. While static traversable wormholes necessarily require exotic matter that violates the classical energy conditions, subsequent studies have sought to [...] Read more.
Wormholes are non-trivial topological structures that arise as exact solutions to Einstein’s field equations, theoretically connecting distinct regions of spacetime via a throat-like geometry. While static traversable wormholes necessarily require exotic matter that violates the classical energy conditions, subsequent studies have sought to minimize such violations by introducing time-dependent geometries embedded within cosmological backgrounds. This review provides a comprehensive survey of evolving wormhole solutions, emphasizing their formulation within both general relativity and alternative theories of gravity. We explore key developments in the construction of non-static wormhole spacetimes, including those conformally related to static solutions, as well as dynamically evolving geometries influenced by scalar fields. Particular attention is given to the wormholes embedded into Friedmann–Lemaître–Robertson–Walker (FLRW) universes and de Sitter backgrounds, where the interplay between the cosmic expansion and wormhole dynamics is analyzed. We also examine the role of modified gravity theories, especially in hybrid metric–Palatini gravity, which enable the realization of traversable wormholes supported by effective stress–energy tensors that do not violate the null or weak energy conditions. By systematically analyzing a wide range of time-dependent wormhole solutions, this review identifies the specific geometric and physical conditions under which wormholes can evolve consistently with null and weak energy conditions. These findings clarify how such configurations can be naturally integrated into cosmological models governed by general relativity or modified gravity, thereby contributing to a deeper theoretical understanding of localized spacetime structures in an expanding universe. Full article
(This article belongs to the Special Issue Experimental and Observational Constraints on Wormhole Models)
Show Figures

Figure 1

14 pages, 217 KiB  
Article
Eco-Spiritual Threads: Karma, Dharma, and Ecosystem in Amitav Ghosh’s Gun Island
by Muhammad Hafeez ur Rehman
Religions 2025, 16(7), 931; https://doi.org/10.3390/rel16070931 - 18 Jul 2025
Viewed by 381
Abstract
This paper examines Amitav Ghosh’s Gun Island through a Hindu eco-spiritual framework to explore how ancient cosmological concepts illuminate contemporary environmental crises. Building upon the legend of Bonduki Sadagar and Manasa Devi, Ghosh narrates the rupture of sacred human–nature relationships in both colonial [...] Read more.
This paper examines Amitav Ghosh’s Gun Island through a Hindu eco-spiritual framework to explore how ancient cosmological concepts illuminate contemporary environmental crises. Building upon the legend of Bonduki Sadagar and Manasa Devi, Ghosh narrates the rupture of sacred human–nature relationships in both colonial and postcolonial contexts. This study employs a tripartite conceptual lens of karma, dharma, and ecosystem drawn from Hindu philosophy to analyze how the novel frames environmental degradation, human moral failure, and ecological interconnectedness. Karma, as the law of cause and effect, is used to depict the consequences of human exploitation through natural disasters, climate migration, and the collapse of ecosystems. Dharma emerges as a principle advocating ecological responsibility and symbiosis between humans and nonhuman life. This paper argues that Ghosh tactfully intertwines Hindu metaphysics with contemporary ecological science to critique capitalist modernity’s environmental violence. The novel’s depiction of floods, the sinking of Venice, and the global refugee crisis dramatizes karmic consequences, while its evocation of myth–science convergence offers a vision of sacred interdependence. Ultimately, this paper concludes that Gun Island provides an urgent eco-spiritual model for reimagining planetary ethics and responding to the Anthropocene through humility, relationality, and spiritual responsibility. Full article
(This article belongs to the Special Issue Postcolonial Literature and Ecotheology)
18 pages, 1438 KiB  
Article
Maximum Entropy Estimates of Hubble Constant from Planck Measurements
by David P. Knobles and Mark F. Westling
Entropy 2025, 27(7), 760; https://doi.org/10.3390/e27070760 - 16 Jul 2025
Viewed by 1563
Abstract
A maximum entropy (ME) methodology was used to infer the Hubble constant from the temperature anisotropies in cosmic microwave background (CMB) measurements, as measured by the Planck satellite. A simple cosmological model provided physical insight and afforded robust statistical sampling of a parameter [...] Read more.
A maximum entropy (ME) methodology was used to infer the Hubble constant from the temperature anisotropies in cosmic microwave background (CMB) measurements, as measured by the Planck satellite. A simple cosmological model provided physical insight and afforded robust statistical sampling of a parameter space. The parameter space included the spectral tilt and amplitude of adiabatic density fluctuations of the early universe and the present-day ratios of dark energy, matter, and baryonic matter density. A statistical temperature was estimated by applying the equipartition theorem, which uniquely specifies a posterior probability distribution. The ME analysis inferred the mean value of the Hubble constant to be about 67 km/sec/Mpc with a conservative standard deviation of approximately 4.4 km/sec/Mpc. Unlike standard Bayesian analyses that incorporate specific noise models, the ME approach treats the model error generically, thereby producing broader, but less assumption-dependent, uncertainty bounds. The inferred ME value lies within 1σ of both early-universe estimates (Planck, Dark Energy Signal Instrument (DESI)) and late-universe measurements (e.g., the Chicago Carnegie Hubble Program (CCHP)) using redshift data collected from the James Webb Space Telescope (JWST). Thus, the ME analysis does not appear to support the existence of the Hubble tension. Full article
(This article belongs to the Special Issue Insight into Entropy)
Show Figures

Figure 1

23 pages, 2437 KiB  
Article
Elaborating Correlation with Space–Time in the Daoist Body: Following and Reversing Nature
by Jihyun Kim
Religions 2025, 16(7), 890; https://doi.org/10.3390/rel16070890 - 11 Jul 2025
Viewed by 733
Abstract
This article examines Daoist ritual and meditative practices, primarily developed between the fourth and twelft centuries, as cosmotechniques: methods for engaging, recalibrating, and occasionally overturning the spatial and temporal order. It first outlines the cosmological framework of the pre-Qin and Qin–Han periods, in [...] Read more.
This article examines Daoist ritual and meditative practices, primarily developed between the fourth and twelft centuries, as cosmotechniques: methods for engaging, recalibrating, and occasionally overturning the spatial and temporal order. It first outlines the cosmological framework of the pre-Qin and Qin–Han periods, in which space and time were conceived as correlative and qualitative, forming the grounds of Daoist practice. Daoist foundational practices elaborately aligned with this framework but also introduced subtle disruptions that discover the singular space–time for transformation. Through the investigation of bodily cultivation and communal rituals, this study argues for attention to the performative aspect of Daoist practices, aiming to access and enact alternative space–time, and suggesting a dynamic interplay between alignment and disruption. The study further analyzes internal alchemy and visionary practices that engage in radical reversals of natural rhythms—employing fire, dissolution, and systemic negation to reconfigure cosmic flow. As shown here, Daoist practice is not merely contemplative but performative, reconstituting space–time and body. Though not articulated in ecological terms, such practices demonstrate ways of modeling and modulating lifeworlds attuned to the rhythms of nature—pointing to the possibility of reshaping life under unplugged conditions. Full article
Show Figures

Figure 1

19 pages, 1419 KiB  
Article
Revisiting the Relationship Between the Scale Factor (a(t)) and Cosmic Time (t) Using Numerical Analysis
by Artur Chudzik
Mathematics 2025, 13(14), 2233; https://doi.org/10.3390/math13142233 - 9 Jul 2025
Viewed by 555
Abstract
Background: Current cosmological fits typically assume a direct relation between cosmic time (t) and the scale factor (a(t)), yet this ansatz remains largely untested across diverse observations. Objectives: We (i) test whether a single power-law scaling [...] Read more.
Background: Current cosmological fits typically assume a direct relation between cosmic time (t) and the scale factor (a(t)), yet this ansatz remains largely untested across diverse observations. Objectives: We (i) test whether a single power-law scaling (a(t)tα) can reproduce late- and early-time cosmological data and (ii) explore whether a dynamically evolving (α(t)), modeled as a scalar–tensor field, naturally induces directional asymmetry in cosmic evolution. Methods: We fit a constant-α model to four independent datasets: 1701 Pantheon+SH0ES supernovae, 162 gamma-ray bursts, 32 cosmic chronometers, and the Planck 2018 TT spectrum (2507 points). The CMB angular spectrum is mapped onto a logarithmic distance-like scale (μ=log10D), allowing for unified likelihood analysis. Each dataset yields slightly different preferred values for H0 and α; therefore, we also perform a global combined fit. For scalar–tensor dynamics, we integrate α(t) under three potentials—quadratic, cosine, and parity breaking (α3sinα)—and quantify directionality via forward/backward evolution and Lyapunov exponents. Results: (1) The constant-α model achieves good fits across all datasets. In combined analysis, it yields H070kms1Mpc1 and α1.06, outperforming ΛCDM globally (ΔAIC401254), though ΛCDM remains favored for some low-redshift chronometer data. High-redshift GRB and CMB data drive the improved fit. Numerical likelihood evaluations are approximately three times faster than for ΛCDM. (2) Dynamical α(t) models exhibit time-directional behavior: under asymmetric potentials, forward evolution displays finite Lyapunov exponents (λL103), while backward trajectories remain confined (λL<0), realizing classical arrow-of-time emergence without entropy or quantum input. Limitations: This study addresses only homogeneous background evolution; perturbations and physical derivations of potentials remain open questions. Conclusions: The time-scaling approach offers a computationally efficient control scenario in cosmological model testing. Scalar–tensor extensions naturally introduce classical time asymmetry that is numerically accessible and observationally testable within current datasets. Code and full data are available. Full article
Show Figures

Figure 1

12 pages, 1540 KiB  
Review
Gravitational Waves: Echoes of the Biggest Bangs Since the Big Bang and/or BSM Physics?
by John Ellis
Universe 2025, 11(7), 213; https://doi.org/10.3390/universe11070213 - 26 Jun 2025
Viewed by 718
Abstract
“If one could ever prove the existence of gravitational waves, the processes responsible for their generation would probably be much more curious and interesting than even the waves themselves.” (Gustav Mie, 1868–1957). The discovery of gravitational waves has opened new windows on [...] Read more.
“If one could ever prove the existence of gravitational waves, the processes responsible for their generation would probably be much more curious and interesting than even the waves themselves.” (Gustav Mie, 1868–1957). The discovery of gravitational waves has opened new windows on astrophysics, cosmology and physics beyond the Standard Model (BSM). Measurements by the LIGO, Virgo and KAGRA Collaborations of stellar–mass binaries and neutron star mergers have shown that gravitational waves travel at close to the velocity of light and constrain BSM possibilities, such as a graviton mass and Lorentz violation in gravitational wave propagation. Follow-up measurements of neutron star mergers have provided evidence for the production of heavy elements, possibly including some essential for human life. The gravitational waves in the nanoHz range observed by Pulsar Timing Arrays (PTAs) may have been emitted by supermassive black hole binaries, but might also have originated from BSM cosmological scenarios such as cosmic strings, or phase transitions in the early Universe. The answer to the question in the title may be provided by gravitational-wave detectors at higher frequencies, such as LISA and atom interferometers. KCL-PH-TH/2024-05. Full article
Show Figures

Figure 1

44 pages, 683 KiB  
Review
Structural Stability and General Relativity
by Spiros Cotsakis
Universe 2025, 11(7), 209; https://doi.org/10.3390/universe11070209 - 26 Jun 2025
Viewed by 308
Abstract
We review recent developments in structural stability as applied to key topics in general relativity. For a nonlinear dynamical system arising from the Einstein equations by a symmetry reduction, bifurcation theory fully characterizes the set of all stable perturbations of the system, known [...] Read more.
We review recent developments in structural stability as applied to key topics in general relativity. For a nonlinear dynamical system arising from the Einstein equations by a symmetry reduction, bifurcation theory fully characterizes the set of all stable perturbations of the system, known as the ‘versal unfolding’. This construction yields a comprehensive classification of qualitatively distinct solutions and their metamorphoses into new topological forms, parametrized by the codimension of the bifurcation in each case. We illustrate these ideas through bifurcations in the simplest Friedmann models, the Oppenheimer-Snyder black hole, the evolution of causal geodesic congruences in cosmology and black hole spacetimes, crease flow on event horizons, and the Friedmann–Lemaître equations. Finally, we list open problems and briefly discuss emerging aspects such as partial differential equation stability of versal families, the general relativity landscape, and potential connections between gravitational versal unfoldings and those of the Maxwell, Dirac, and Schrödinger equations. Full article
Show Figures

Figure 1

30 pages, 8134 KiB  
Article
Visual Alchemy: Alchemical Yijing Diagrams 丹道易圖 in the Illustrated Commentary on the Wuzhen Pian Based on the Zhouyi 周易悟真篇圖注
by Xin He
Religions 2025, 16(7), 812; https://doi.org/10.3390/rel16070812 - 20 Jun 2025
Viewed by 1175
Abstract
The Illustrated Commentary on the Wuzhen Pian Based on the Zhouyi (周易悟真篇圖注 Zhouyi Wuzhen Pian Tuzhu), authored by the Ming dynasty Confucian scholar Cheng Yiming 程易明, is an illustrated alchemical text that integrates the elixir methodology of Wuzhen pian 悟真篇 (the [...] Read more.
The Illustrated Commentary on the Wuzhen Pian Based on the Zhouyi (周易悟真篇圖注 Zhouyi Wuzhen Pian Tuzhu), authored by the Ming dynasty Confucian scholar Cheng Yiming 程易明, is an illustrated alchemical text that integrates the elixir methodology of Wuzhen pian 悟真篇 (the Awakening to Reality) with the images and numbers (xiangshu 象數) system of The Book of Changes (Zhouyi 周易). Centered on Daoist alchemical theory and elucidated through “Yijing diagrams” (yitu 易圖, diagrams based on the Yijing), it stands as a masterpiece within the tradition of alchemical Yijing studies (dandao yixue 丹道易學). Building on a review of the scholarly history of The Wuzhen Pian, this article focuses on the alchemical Yijing diagrams (dandao yitu 丹道易圖) in the Illustrated Commentary, exploring their terminological definitions, theoretical origins, and diagrammatic systems. By analyzing the structure of cosmology and internal alchemy practice theory (neidan gongfulun 內丹工夫論) as presented in these diagrams, this article demonstrates that the Illustrated Commentary not only inherits the theoretical legacy of early Yijing diagram scholars such as Chen Tuan (陳摶) and Yu Yan (俞琰), but also displays a unique systematic and intuitive approach to illustrating neidan practices through xiangshu diagrams (象數圖解). Notably, diagrams such as “Mundane Continuation vs. Alchemical Inversion” (shunfan nixian 順凡逆仙), the “Three-Five-One Mathematical Model” (sanwuyi shuli moxing 三五一數理模型), and the “Fire Phases” (huohou 火候) reveal attempts to construct an alchemical theoretical system centered on Yijing diagrams. The article further posits that the Illustrated Commentary bridges the gap between images–numbers Yijing studies (xiangshu yixue 象數易學) and alchemical visual hermeneutics, offering a fresh perspective centered on internal alchemy for the study of “Yijing Diagram Studies” (yitu xue 易圖學). Full article
Show Figures

Figure 1

50 pages, 8738 KiB  
Review
From Barthel–Randers–Kropina Geometries to the Accelerating Universe: A Brief Review of Recent Advances in Finslerian Cosmology
by Amine Bouali, Himanshu Chaudhary, Lehel Csillag, Rattanasak Hama, Tiberiu Harko, Sorin V. Sabau and Shahab Shahidi
Universe 2025, 11(7), 198; https://doi.org/10.3390/universe11070198 - 20 Jun 2025
Cited by 1 | Viewed by 417
Abstract
We present a review of recent developments in cosmological models based on Finsler geometry, as well as geometric extensions of general relativity formulated within this framework. Finsler geometry generalizes Riemannian geometry by allowing the metric tensor to depend not only on position but [...] Read more.
We present a review of recent developments in cosmological models based on Finsler geometry, as well as geometric extensions of general relativity formulated within this framework. Finsler geometry generalizes Riemannian geometry by allowing the metric tensor to depend not only on position but also on an additional internal degree of freedom, typically represented by a vector field at each point of the spacetime manifold. We examine in detail the possibility that Finsler-type geometries can describe the physical properties of the gravitational interaction, as well as the cosmological dynamics. In particular, we present and review the implications of a particular implementation of Finsler geometry, based on the Barthel connection, and of the (α,β) geometries, where α is a Riemannian metric, and β is a one-form. For a specific construction of the deviation part β, in these classes of geometries, the Barthel connection coincides with the Levi–Civita connection of the associated Riemann metric. We review the properties of the gravitational field, and of the cosmological evolution in three types of geometries: the Barthel–Randers geometry, in which the Finsler metric function F is given by F=α+β, in the Barthel–Kropina geometry, with F=α2/β, and in the conformally transformed Barthel–Kropina geometry, respectively. After a brief presentation of the mathematical foundations of the Finslerian-type modified gravity theories, the generalized Friedmann equations in these geometries are written down by considering that the background Riemannian metric in the Randers and Kropina line elements is of Friedmann–Lemaitre–Robertson–Walker type. The matter energy balance equations are also presented, and they are interpreted from the point of view of the thermodynamics of irreversible processes in the presence of particle creation. We investigate the cosmological properties of the Barthel–Randers and Barthel–Kropina cosmological models in detail. In these scenarios, the additional geometric terms arising from the Finslerian structure can be interpreted as an effective geometric dark energy component, capable of generating an effective cosmological constant. Several cosmological solutions—both analytical and numerical—are obtained and compared against observational datasets, including Cosmic Chronometers, Type Ia Supernovae, and Baryon Acoustic Oscillations, using a Markov Chain Monte Carlo (MCMC) analysis. A direct comparison with the standard ΛCDM model is also carried out. The results indicate that Finslerian cosmological models provide a satisfactory fit to the observational data, suggesting they represent a viable alternative to the standard cosmological model based on general relativity. Full article
(This article belongs to the Special Issue Cosmological Models of the Universe)
Show Figures

Figure 1

Back to TopTop