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<title>J. O. Seti — Neckpinch</title><link>https://neckpinch.com/authors/j-o-seti/</link><description>New arXiv papers by J. O. Seti, from Neckpinch</description>
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<item><title>Nonmetric geometric flows and quasicrystalline topological phases for dark energy and dark matter in f(Q) cosmology</title><link>https://neckpinch.com/papers/2410.03700/</link><guid isPermaLink="false">arxiv:2410.03700</guid><pubDate>Tue, 24 Sep 2024 00:00:00 GMT</pubDate><description>L. Bubuianu, E. Nurlan, J. O. Seti, S. Vacaru, E. V. Veliev — We elaborate on nonmetric geometric flow theory and metric-affine gravity with applications in modern cosmology. Two main motivations for our research follow from the facts that 1) cosmological models for f(Q) modified gravity theories, MGTs, are efficient for describing recent observational data provided by the James Webb Space Telescope; and 2) the statistical thermodynamic properties of such nonmetric locally anisotropic cosmological models can be studied using generalizations of the concept of G. Perelman entropy. We derive nonmetric distorted R. Hamilton and Ricci soliton equations in such canonical nonholonomic variables when corresponding systems of nonlinear PDEs can be decoupled and integrated in general off-diagonal forms. This is possible if we develop and apply the anholonomic frame and connection deformation method involving corresponding types of generating functions and generating sources encoding nonmetric distortions. Using such generic off-diagonal solutions (when the coefficients of metrics and connections may depend generically on all spacetime coordinates), we model accelerating cosmological scenarios with quasi-periodic gravitational and (effective) matter fields; and study topological and nonlinear geometric properties of respective dark energy and dark matter, DE and DM, models. As explicit examples, we analyze some classes of nonlinear symmetries defining topological quasicrystal, QC, phases which can modified to generate other types of quasi-periodic and locally anisotropic structures. The conditions when such nonlinear systems possess a behaviour which is similar to that of the Lambda cold dark matter (ΛCDM) scenario are stated. We conclude that nonmetric geometric and cosmological flows can be considered as an alternative to the ΛCDM concordance models and speculate on how such theories can be elaborated.</description><category>Anisotropic &amp; nonlocal flows</category><category>Ricci solitons</category><category>Perelman entropy</category><category>Physics</category></item>
<item><title>Nonassicative cosmological solitonic R-flux deformations in gauge gravity and G. Perelman geometric flow thermodynamics</title><link>https://neckpinch.com/papers/2410.03698/</link><guid isPermaLink="false">arxiv:2410.03698</guid><pubDate>Tue, 24 Sep 2024 00:00:00 GMT</pubDate><description>L. Bubuianu, J. O. Seti, S. Vacaru, E. V. Veliev — We elaborate on a model of nonassociative and noncommutative gauge gravity for the de Sitter gauge group SO(4,1) embedding extensions of the affine structure group Af(4,1) and the Poincaré group ISO(3,1). In string theory, such nonassociative gauge gravity theories are determined by star product R-flux deformations. They are new avenues to quantum gravity and geometric and quantum information theories. We analyze physically important and geometric thermodynamic properties of new classes of generic off-diagonal cosmological solitonic solutions encoding nonassociative effective sources. Particularly, we focus on modelling by such solutions of locally anisotropic and inhomogeneous dark matter and dark energy structures generated as nonassociative solitonic hierarchies. Such accelerating cosmological evolution scenarios can&apos;t be described in the framework of the Bekenstein-Hawking thermodynamic formalism. This motivates a change in the gravitational thermodynamic paradigm by considering nonassociative and relativistic generalizations of the concept of W-entropy in the theory of Ricci flows. Finally, we compute the corresponding modified G. Perelman&apos;s thermodynamic variables and analyze the temperature-like evolution of cosmological constants determined by nonassociative cosmological flows.</description><category>Ricci flow</category><category>Perelman entropy</category><category>Homogeneous spaces</category><category>Physics</category></item>
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