Dark energy and accelerating cosmological evolution from osculating Barthel–Kropina geometry

نویسندگان

چکیده

Finsler geometry is an important extension of Riemann geometry, in which to each point the spacetime manifold arbitrary internal variable associated. Interesting geometries, with many physical applications, are Randers and Kropina type respectively. A subclass geometries represented by osculating spaces, a function base coordinates only. In one introduces Barthel connection, has remarkable property that it Levi-Civita connection Riemannian metric. present work we consider gravitational cosmological implications Barthel-Kropina geometry. We assume this Ricci curvatures related matter energy-momentum tensor standard Einstein equations. The generalized Friedmann equations obtained considering background metric Friedmann-Lemaitre-Robertson-Walker type. energy balance equation also derived. properties model investigated detail, shown admits de Sitter solution, effective dark component can be generated. Several solutions numerically integrating comparison two specific classes models observational data $\Lambda$CDM performed, turns out give satisfactory description observations.

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Dark Energy and Dark Matter from Cosmological Observations

The introduction of new observational techniques has in the past few years moved cosmology into the era of precision science. With the advent of precision measurements of the cosmic microwave background (CMB), large scale structure (LSS) of galaxies, and distant type Ia supernovae, a new paradigm of cosmology has been established. In this new standard model, the geometry is flat so that Ωtotal ...

متن کامل

Cosmological Evolution of Interacting Dark Energy in Lorentz Violation

The cosmological evolution of an interacting scalar field model in which the scalar field interacts with dark matter, radiation, and baryon via Lorentz violation is investigated. We propose a model of interaction through the effective coupling β̄. Using dynamical system analysis, we study the linear dynamics of an interacting model and show that the dynamics of critical points are completely con...

متن کامل

Supernovae, Dark Energy, and the Accelerating Universe: The Status of the Cosmological Parameters

I was asked to present the status of the cosmological parameters, and in particular the status of the recent results concerning the accelerating universe—and the possible cosmological constant or dark energy that is responsible for the universe’s acceleration. This result comes most directly from the recent type Ia supernova work, so although I will mention a few of the approaches to the cosmol...

متن کامل

Dark Energy and the Accelerating Universe

Ten years ago, the discovery that the expansion of the universe is accelerating put in place the last major building block of the present cosmological model, in which the universe is composed of 4% baryons, 20% dark matter, and 76% dark energy. At the same time, it posed one of the most profound mysteries in all of science, with deep connections to both astrophysics and particle physics. Cosmic...

متن کامل

The Hubble Constant and Dark Energy from Cosmological Distance Measures

We study how the determination of the Hubble constant from cosmological distance measures is affected by models of dark energy and vice versa. For this purpose, constraints on the Hubble constant and dark energy are investigated using the cosmological observations of cosmic microwave background, baryon acoustic oscillations and type Ia suprenovae. When one investigates dark energy, the Hubble c...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: European Physical Journal C

سال: 2022

ISSN: ['1434-6044', '1434-6052']

DOI: https://doi.org/10.1140/epjc/s10052-022-10318-9