Bulk Viscous Flat FLRW Model with Observational Constraints in f(T, B) Gravity

نویسندگان

چکیده

This paper investigates the impact of bulk viscosity within framework f(T,B) gravity. We consider a time-dependent model with particular Hubble parameter expression. Here, we looked into viability well-motivated gravity model, which takes form f=αlog(B)+βT, and has free parameters α β. The 46 observational data (OHD) in range 0≤z≤2.36 were used to constrain achieve solution. have Markov Chain Monte Carlo (MCMC) method estimate observe that appears be good agreement observations. In addition, evaluate effective viscous equation state for model. examined characteristics different energy conditions stability analysis. is valid based on positive behavior null (NEC), weak (WEC), dominant (DEC); however, strong (SEC) are violation, suggesting universe expanding faster. Our was found quintom region. also discussed how tachyon scalar field corresponds

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

Einstein - Æther Gravity : Theory and Observational Constraints

Einstein-aether theory is general relativity coupled to a dynamical unit timelike vector field. A brief review of current theoretical understanding and observational constraints on the four coupling parameters of the theory is given.

متن کامل

3D gravity data-space inversion with sparseness and bound constraints

One of the most remarkable basis of the gravity data inversion is the recognition of sharp boundaries between an ore body and its host rocks during the interpretation step. Therefore, in this work, it is attempted to develop an inversion approach to determine a 3D density distribution that produces a given gravity anomaly. The subsurface model consists of a 3D rectangular prisms of known sizes ...

متن کامل

Wormholes 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 کامل

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 کامل

Second Order Perturbations of Flat Dust Flrw Universes with a Cosmological Constant

We summarize recent results concerning the evolution of second order perturbations in flat dust irrotational FLRW models with Λ 6= 0. We show that asymptotically these perturbations tend to constants in time, in agreement with the cosmic no-hair conjecture. We solve numerically the second order scalar perturbation equation, and very briefly discuss its all time behaviour and some possible impli...

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: Universe

سال: 2022

ISSN: ['2218-1997']

DOI: https://doi.org/10.3390/universe8120650