Bulk Viscous Fluid in Symmetric Teleparallel Cosmology: Theory versus Experiment
نویسندگان
چکیده
The standard formulation of General Relativity Theory, in the absence a cosmological constant, is unable to explain responsible mechanism for observed late-time cosmic acceleration. On other hand, by inserting constant Einstein's field equations it possible describe acceleration, but suffers from an unprecedented fine-tunning problem. This motivates one modify space-time geometry Relativity. $f(Q)$ modified theory gravity alternative Relativity, where non-metricity scalar $Q$ candidate gravitational interactions. In present work we consider Friedmann-Lem\^aitre-Robertson-Walker model dominated bulk viscous fluid with functional form $f(Q)=\alpha Q^n$, $\alpha$ and $n$ are free parameters model. We constrain our recent Pantheon supernovae data set 1048 points, Hubble 31 points baryon acoustic oscillations consisting six points. For higher values redshift, clear that cosmology better fits than cosmology. evolution deceleration parameter redshift properly predicts transition decelerated accelerated phases universe expansion. Also, density, pressure effective equation state redshift. Those show viscosity valid acquire negative drive expansion efficiently.We also examine behavior different energy conditions test viability Furthermore, statefinder diagnostics investigated order distinguish among dark models.
منابع مشابه
Bulk viscous cosmology.
The full causal Müller-Israel-Stewart (MIS) theory of dissipative processes in relativistic fluids is applied to a flat, homogeneous and isotropic universe with bulk viscosity. It is clarified in which sense the so called truncated version is a reasonable limiting case of the full theory. The possibility of bulk viscosity driven inflationary solutions of the full theory is discussed. As long as...
متن کاملWormholes in Bulk Viscous Cosmology
We investigate the effects of the accretion of phantom energy with non-zero bulk viscosity onto a Morris-Thorne wormhole. We have found that if the bulk viscosity is large then the mass of wormhole increases rapidly as compared to small or zero bulk viscosity.
متن کاملNonlocal teleparallel cosmology
Even though it is not possible to differentiate general relativity from teleparallel gravity using classical experiments, it could be possible to discriminate between them by quantum gravitational effects. These effects have motivated the introduction of nonlocal deformations of general relativity, and similar effects are also expected to occur in teleparallel gravity. Here, we study nonlocal d...
متن کاملViscous Brane Cosmology with a Brane-bulk Energy Interchange Term
We assume a flat brane located at y = 0, surrounded by an AdS space, and consider the 5D Einstein equations when the energy flux component of the energy-momentum tensor is related to the Hubble parameter through a constant Q. We calculate the metric tensor, as well as the Hubble parameter on the brane, when Q is small. As a special case, if the brane is tensionless, the influence from Q on the ...
متن کاملAxially Symmetric Solution in Teleparallel Theory of Gravitation
An exact solution has an axial symmetry is obtained in the teleparallel theory of grav-itation. The associated metric has the structure function G(ξ) = 1 − ξ 2 − 2mAξ 3. The cubic nature of the structure function can make calculations cumbersome. Using a coordinate transformation we get a tetrad that its associated metric has the structure function in a factorisable form. This new form has the ...
متن کاملذخیره 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: Universe
سال: 2022
ISSN: ['2218-1997']
DOI: https://doi.org/10.3390/universe9010012