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Bianchi Type III

Bianchi type-III Cosmological Model with Linear Equation of State in f(R) Gravity

Bianchi type-III Cosmological Model with Linear Equation of State in f(R) Gravity

... Bianchi type-III cosmological model with linear equation of state have investigated in f (R ) theory of gravitation. The models have studied in relation to volumetric power law and exponential law ...

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Bianchi Type-III Universe with Anisotropic Dark Energy and Special form of Deceleration Parameter

Bianchi Type-III Universe with Anisotropic Dark Energy and Special form of Deceleration Parameter

... In the present paper, the Bianchi type-III cosmological models with anisotropic dark energy and special form of deceleration parameter have been studied. To have a general description of an ...

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Bianchi Type  III and Kantowski Sachs Universes with wet Dark Fluid

Bianchi Type III and Kantowski Sachs Universes with wet Dark Fluid

... the Bianchi type- III and Kantowski-Sachs Universes with matter term with dark energy treated as a Dark Fluid satisfying the Equation of state ...

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Cosmic String in Bianchi Type III Space Time with Bulk Viscosity and Magnetic Field

Cosmic String in Bianchi Type III Space Time with Bulk Viscosity and Magnetic Field

... We have discussed LRS Bianchi type III cosmological model for a cloud of string with bulk viscosity and mag- netic field and a model (26) is constructed. We observed from the Equation (27) that if we ...

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On Bianchi Type III String Cloud Universe Containing Strange Quark Matter

On Bianchi Type III String Cloud Universe Containing Strange Quark Matter

... Considering Bianchi type III space-time we present the model Universe containing strange quark matter which is expanding, anisotropic, with a sign of dark energy that help in accelerated expan- sion ...

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Bulk Viscous Anisotropic Cosmological  Models with Generalized Chaplygin Gas with Time Varying Gravitational and  Cosmological Constants

Bulk Viscous Anisotropic Cosmological Models with Generalized Chaplygin Gas with Time Varying Gravitational and Cosmological Constants

... Abstract This paper is devoted to studying the generalized Chaplygin gas models in Bianchi type III spacetime geometry with time varying bulk viscosity, cosmological and gravitational co[r] ...

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Vol 3, No 3 (2012)

Vol 3, No 3 (2012)

... It is well known that spatially homogeneous and a anisotropic cosmological models in the presence of scalar fields play a vital role in the discussion of large scale structure of the universe. With this motivation we ...

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Vol 9, No 2 (2018)

Vol 9, No 2 (2018)

... LRS Bianchi I models with varying gravitational and cosmological ...obtained Bianchi type III bulk viscous barotropic fluid cosmological models with variable G and Λ ...

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Interacting dark fluids in bianchi type-i universe with variable  deceleration parameter

Interacting dark fluids in bianchi type-i universe with variable deceleration parameter

... tests. Bianchi type-III cosmological model in f (R, T) theory of gravity was studied by ...studied Bianchi type-V modified holographic Ricci dark energy model in the modified theory of ...

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Bianchi type v magnetized cosmological model with wet dark fluid in general relativity

Bianchi type v magnetized cosmological model with wet dark fluid in general relativity

... of Bianchi type III have investigated Bianchi type II, III and IX have studied Bianchi type-III non-static ...

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Vacuum solution of bianchi type i model in   theory of gravity

Vacuum solution of bianchi type i model in theory of gravity

... in Bianchi type-V space time. Bianchi type models are among simplest models with anisotropy ...of Bianchi type–I and V space times in metric f (R ) gravity have been explored by ...

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Vol 7, No 3 (2016)

Vol 7, No 3 (2016)

... electromagnetic Bianchi type III cosmological ...of Bianchi typeIII space time presence and absence of magnetic ...studied Bianchi typeIII non-static ...

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LRS Bianchi Type I Universe with Anisotropic Dark Energy in Lyra Geometry

LRS Bianchi Type I Universe with Anisotropic Dark Energy in Lyra Geometry

... After the discovery that the cosmic expansion is acceler- ating [1-3] and the first cosmic microwave background (CMB) radiation observation of a flat universe [4], the current standard model of cosmology implies the ...

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Search | Preprints

Search | Preprints

... Abstract Bianchi type III string cosmological models (massive and geometric) in presence of magnetic field with vacuum energy density following the techniques used by Letelier (1979) and Stachel ...

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Bianchi Type I Cosmological Models with Expansion Driven by Particle Creation

Bianchi Type I Cosmological Models with Expansion Driven by Particle Creation

... Abstract- A study of Bianchi Type I cosmological model is undertaken in the framework of creation of particles. To accommodate the creation of new particles, the universe is regarded as an Open ...

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LRS Bianchi Type – II Model with Dark Matter and Holographic Dark Energy

LRS Bianchi Type – II Model with Dark Matter and Holographic Dark Energy

... Binanchi type V model by considering HEL ...of Bianchi type- V in f (R, T) gravity ...investigated Bianchi type V early model decelerating and late-time accelerating cosmological model ...

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LRS Bianchi Type –I Universe with Magnetized Wet Dark Fluid

LRS Bianchi Type –I Universe with Magnetized Wet Dark Fluid

... Bianchi type models have been studied by several authors in an attempt to understand better the observed small amount of anisotropy in the ...Some Bianchi cosmologies, for example, are natural hosts ...

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Bianchi Type-IX Radiating Cosmological Model in Self-Creation Cosmology

Bianchi Type-IX Radiating Cosmological Model in Self-Creation Cosmology

... radiating Bianchi type-IX cosmological model in Barbers second self-creation theory of gravitation using the law of variation for the Hubbles parameter which yields a constant value of decelerating ...

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Bianchi Type-V Cosmological Model of Universe with Polytropic Equation of State

Bianchi Type-V Cosmological Model of Universe with Polytropic Equation of State

... EoS may correspond to self gravitating Bose-Einstein condenstates with repulsive ( K  0 ) or attractive ( K  0 ) self interaction or have another origin. This EoS also describes radiation (   1 / 3 ) , pressureless ...

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LRS Bianchi Type-I Cosmological Model with Variable Deceleration Parameter

LRS Bianchi Type-I Cosmological Model with Variable Deceleration Parameter

... fluid type by assuming an equation of state linking the pressure p and energy density in order to build an analytical methodsnear the ...of type Ia supernovae by the High-Z Supernovasearch team (Riess et ...

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