5-dimensional space with a 4-dimensional FRW spacetime as subspace

 

[1]We will wish to find five-d spaces with 4-d subspaces which are familiar to us. For example the metric for a five-dimensional space with a four-dimensional subspace which is homogeneous and isotropic:

 

ds2 = - dt2 + [Rt2/(1+kr2)2](dr2 + r2 dW2) + 5t2 5r2 dX52

 

The Einstein Tensor for Five-Dimensional Spaces

The Einstein tensor components for spherically symmetric 4 and 5 d spaces have a simple relationship to each other (see appendix for derivation).

For the Grr tensor component: the relationship between the r parts of the 4 and 5-d components:

 

5rGrr  =  4rGrr + 2(1/Rt2)(1/Rr2)(5'r/5r)(qr'/qr) ,

 

which for this metric with  Rr = (1+kr2) and qr = r/(1+kr2)  is:

 

5rGrr  =  4rGrr + (2/Rt2)(1+kr2)2(5'r/5r)(1-kr2)/[r(1+kr2)]

=  4rGrr + (2/Rt2)(5'r/5r)(1-k2r4)/r

 

Homogeneous Isotropic Space

 

For the 5-d tensor component to be homogeneous, it must be independent of r, and since the 4-part is homogeneous and r-independent  it must be  that:

 

(5'r/5r)(1-k2r4)/r

is r-independent. That is:

(5'r/5r)(1-k2r4)/r = c ,

 i.e:

  5'r/5r = cr/(1-k2r4).

5'r/5r  = c  [r/(1-k2r4)]

ln5r  = c  [r/(1-k2r4)] + K

The integral can be easily performed using the substitution R = r2 , dR=2rdr.

 

The solution is:

5r = K [(1-kr2)/(1+kr2)]-c/4k

so that the 5-d metric for a homogeneous isotropic space is (squaring 5r makes the exponent -c/2k)

 

ds2 = -dt2 +Rt2/(1+kr2)2 (dr2+r2dW2) + 5t2 K [(1-kr2)/(1+kr2)]-c/2k dX52

 

It is amazing that this solution can be obtained so simply - for an appreciation of how simple our method is, see Chatterjee paper: he bravely solved this using the usual long and tedious calculations.

The other results derived there are also easily found in this way.



[1] Edited excerpt from my file: “Part IV GR book”


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