Open AccessSelf-similarity model of nonsingular perfect gas universe
Author(s) -
Lai Xiao-Ming,
Bian Bao-Min,
Yuan Ling,
Yang Juan,
Bian Niu,
Zhenhua Li,
Anzhi He
Publication year - 2008
Publication title -
wuli xuebao
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.199
H-Index - 47
ISSN - 1000-3290
DOI - 10.7498/aps.57.7955
Subject(s) - physics , hubble's law , friedmann–lemaître–robertson–walker metric , metric expansion of space , dimensionless quantity , mathematical physics , universe , deceleration parameter , gravitational field , gravitational constant , particle horizon , physical constant , classical mechanics , quantum mechanics , cosmology , dark energy
The present paper investigates the dimensionless dynamical continuity equation of perfect gas motion in gravitational field. Based on Π axiom of dimensional theory self-similarity of perfect gas universe with gravity and a series of exact solutions of R(t) are deduced. Based on R(t)a non-Euclidean homogeneous space-time coordinate system S(t,ξθφ) can be established. A perfect gas universe solution can be worked out in which there is a constant density ρ the velocity u value being zero and there is a nonzero pressure p. In this solution the red shift z represents the propagating distance r. When z is much less than 1 it is proportional to r (Hubbles law). The Robertson-Walker (k=-1) metric of normal universe model is obtained from homogeneous expanding coordinates and the ratio of expanding rate HF to the Hubble constant H0 decreases notably as the value of z rises. It corresponds to the “universal accelerated expansion” observed in the spectrum of a high-red-shift supernova.