Hubble Expansion Parameter in a New Model of Dark Energy

Author： Saadat Hassan  

Publisher： Springer Publishing Company

ISSN： 0020-7748

Source： International Journal of Theoretical Physics, Vol.51, Iss.1, 2012-01, pp. : 78-82

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

The cold local Hubble flow as a signature of dark energy

By  

Astronomy & Astrophysics, Vol. 378, Iss. 3, 2001-11 ,pp. : 729-734

Edp Sciences

Access to resources Recommend Favorite

Bianchi Type-I Anisotropic Dark Energy Model with Constant Deceleration Parameter

By Pradhan Anirudh   Amirhashchi H.   Saha Bijan  

International Journal of Theoretical Physics, Vol. 50, Iss. 9, 2011-09 ,pp. : 2923-2938

Springer Publishing Company

Access to resources Recommend Favorite

The Hubble diagram for a system within dark energy: influence of some relevant quantities

By Saarinen J.   Teerikorpi P.  

Astronomy & Astrophysics, Vol. 568, Iss. issue, 2014-08 ,pp. : A33-A33

Edp Sciences

Access to resources Recommend Favorite

The Hubble diagram for a system within dark energy: the location of the zero-gravity radius and the global Hubble rate

By Teerikorpi P.   Chernin A. D.  

Astronomy & Astrophysics, Vol. 516, Iss. issue, 2010-07 ,pp. : A93-A93

Edp Sciences

Access to resources Recommend Favorite

Holographic Dark Energy Model with Time Varying G as Well as c 2 Parameter

By Borah Bharat   Ansari M.  

International Journal of Theoretical Physics, Vol. 53, Iss. 4, 2014-04 ,pp. : 1217-1224

Springer Publishing Company

Access to resources Recommend Favorite