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Outline

MODERN THEORY OF GENERALISED RELATIVITY

2019, Researchgate

Abstract

We consider a (4+D)-dimensional Friedmann-Robertson-Walker type universe having complex scale factor R + iR I , where R is the scale factor corresponding to the usual 4-dimensional Universe while iR I is that of D-dimensional space. It is then compared with (4+D)-dimensional Kaluza-Klein Cosmology having two scale factors R and a(= iR I). It is shown that the rate of compactification of higher dimension depends on extra dimension 'D'. The Wheeler-DeWitt equation is constructed and general solution is obtained. It is found that for D = 6 (i.e. in 10 dimension), the Wheeler-DeWitt equation is symmetric under the exchange of R I R. I. Introduction: In 1915 Einstein published the general theory of relativity. He expected the universe to be 'closed' and to be filled with matter. Now, if we go outside the gravitating sphere, we see the gravitation would be weaker and weaker. According to Einstein's theory of general relativity, the matter-space-time cannot be separated by any cost. Thus, outside the Einstein's universe, where real time cannot be defined, the corresponding space (although, the matter belongs to another phase) must be measured as imaginary. Thus the space-time of the universe is actually a complex space-time. Here we consider the real space-time (unfolded space-time) for Einstein and imaginary space-time (folded space-time) for us. We found a relation between folded and unfolded space-time of the universe by using Wheeler De-Witt equation. The generalized solution for the Einstein field equations for a homogeneous universe was first presented by Alexander Friedmann. The Friedmann equation for the evolution of the cosmic scale factor R(t) which represents the size of the universe, is Differentiating the above equation with respect to time t and since the total matter in a given expanding volume is unchanged, that means = constant. We have, i.e

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