ScholarLens Back to search
2004•Communications in Theoretical PhysicsRequires access

Bianchi Type III String Cosmological Model with Bulk Viscosity

Wang Xing-Xiang

Open publisher page 4 citations

Abstract

The Bianchi type III cosmological model for a cloud string with bulk viscosity are presented. To obtain a determinate model, an equation of state and a relation between metric potentials are assumed. The physical and geometric aspects of the model are also discussed. The model describes a shearing non-rotating continuously expanding universe with a big-bang start, and the relation between the coefficient of bulk viscosity and the energy density is .

About this research paper

What this paper is about

The Bianchi type III cosmological model for a cloud string with bulk viscosity are presented. To obtain a determinate model, an equation of state and a relation between metric potentials are assumed. The physical and geometric aspects of the model are also discussed. The model describes a shearing non-rotating continuously expanding universe with a big-bang start, and the relation between the coefficient of bulk viscosity and the energy density is .

Why it matters

OpenAlex reports 4 citations for this work. Citation counts describe recorded attention and do not establish research quality.

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Available abstract

The Bianchi type III cosmological model for a cloud string with bulk viscosity are presented. To obtain a determinate model, an equation of state and a relation between metric potentials are assumed. The physical and geometric aspects of the model are also discussed. The model describes a shearing non-rotating continuously expanding universe with a big-bang start, and the relation between the coefficient of bulk viscosity and the energy density is .

Key concepts: Volume viscosity, Physics, Cosmological model, Equation of state, String (physics), Shearing (physics), Type (biology), Viscosity

Related papers

Related paper 1Related paper 2
Back to paper searchBrowse research topicsOriginal source
Bianchi Type III String Cosmological Model with Bulk Viscosity — Research Paper | ScholarLens