Results 51 to 60 of about 12,766 (215)
Abstract Current observations show that a significant fraction of the Universe is composed of dark energy and dark matter. In this paper, the simultaneous effects of these dark sectors on the Euler–Heisenberg black hole are investigated, using the quintessence matter field and perfect fluid to model them. In particular, the black hole's thermodynamics,
Bilel Hamil, Bekir Can Lütfüoğlu
wiley +1 more source
Generalization of the Randall‐Sundrum Model Using Gravitational Model F(T, Θ)
In this letter, we explore a generalized model based on two scenarios including the Randall‐Sundrum model and gravity model F(T, Θ). We first study the standard Randall‐Sundrum gravitational model and then add a function containing two parameters as torsion and trace energy‐momentum tensor to the main action of the model.
S. Davood Sadatian +2 more
wiley +1 more source
The standard cosmological model is in the midst of a stress test, thanks to the tension between supernova-based measurements of the Hubble constant H _0 and inferences of its values from cosmic microwave background (CMB) anisotropies.
Kazem Rezazadeh +2 more
doaj +1 more source
Status on Bidimensional Dark Energy Parameterizations Using SNe Ia JLA and BAO Datasets
Using current observations of forecast type Ia supernovae (SNe Ia) Joint Lightcurve Analysis (JLA) and baryon acoustic oscillations (BAO), in this paper we investigate six bidimensional dark energy parameterizations in order to explore which has more ...
Celia Escamilla-Rivera
doaj +1 more source
On the Square Speed of Sound in High‐Energy Collisions: Range of Values and How to Understand It
After reviewing the sound speeds in various forms and conditions of matter, we investigate the sound speed of hadronic matter that has decoupled from the hot and dense system formed during high‐energy collisions. We comprehensively consider factors such as energy loss of the incident beam, rapidity shift of leading nucleons, and the Landau hydrodynamic
Ting-Ting Duan +3 more
wiley +1 more source
Inflation in f(R, ϕ) Gravity with Exponential Model
We are taking action of f(R) gravity with a nonminimal coupling to a massive inflaton field. A f(R, ϕ) model is chosen which leads to the scalar-tensor theory which can be transformed to Einstein frame by conformal transformation. To avoid the vagueness of the frame dependence, we evaluate the exact analytical solutions for inflationary era in Jordan ...
Farzana Kousar +3 more
wiley +1 more source
Cosmological extrapolation of MOND
Regime of MOND, which is used in astronomy to describe the gravitating systems of island type without the need to postulate the existence of a hypothetical dark matter, is generalized to the case of homogeneous distribution of usual matter by introducing
Amanullah R +21 more
core +1 more source
Features of the Acoustic Mechanism of Core-Collapse Supernova Explosions [PDF]
In the context of 2D, axisymmetric, multi-group, radiation/hydrodynamic simulations of core-collapse supernovae over the full 180$^{\circ}$ domain, we present an exploration of the progenitor dependence of the acoustic mechanism of explosion.
A. Burrows +7 more
core +2 more sources
Systematic Dynamical Analysis in Palatini f(R) Gravity
This paper aims to explore the evolution of the universe in the background of Palatini f(R) gravity. Considering Amendola Gannouji Polarski Tsujikawa (AGPT) f(R) gravity model, we perform a dynamical system analysis within the FLRW universe in order to analyze the impacts of this gravity model on large‐scale structure and dynamics of universe. With the
Fizza Saeed +3 more
wiley +1 more source
We find that combined Planck cosmic microwave background, baryon acoustic oscillations, and supernovae data analyzed under Λ cold dark matter (ΛCDM) are in 4.9σ tension with the extended Baryon Oscillation Spectroscopic Survey (eBOSS) Lyα forest in ...
Keir K. Rogers, Vivian Poulin
doaj +1 more source

