Dust Fluid Cosmological Model | Zendy

Anita Bagora | Zendy; Rakeshwar Purohit | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

Dust Fluid Cosmological Model

Author(s) -

Anita Bagora,

Rakeshwar Purohit

Publication year - 2013

Publication title -

isrn astronomy and astrophysics

Language(s) - English

Resource type - Journals

eISSN - 2090-4746

pISSN - 2090-4738

DOI - 10.1155/2013/293298

Subject(s) - volume viscosity , physics , viscosity , viscous liquid , hubble's law , cosmological constant , zero (linguistics) , cosmological model , constant (computer programming) , classical mechanics , mechanics , cosmology , thermodynamics , astrophysics , dark energy , linguistics , philosophy , computer science , programming language

Bianchi type I tilted bulk viscous fluid cosmological model filled with dust fluid is investigated. We assume that (constant), where is the coefficient of bulk viscosity and is the expansion in the model. It has been assumed that the expansion in the model is only in two directions; that is, one of the components of Hubble parameters is zero. The physical and geometrical aspects of the model in the presence and absence of bulk viscosity are also discussed. Also, we have discussed two special models and their physical properties. From this, we present a particular example based on dust fluid.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research