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N - The Number Of Dimensions
Of Space-Time
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| From the Lagrangian section |
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3.1
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| In a closed system, in general
G does not have a vanishing divergence. Using the Bianchi identities |
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Where a is a constant and
is the cosmological term. |
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| The divergence of this equation
is |
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3.2
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| With the aid of the following
identities |
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| Where f=3 to N, the following
expression arises from equation 3.2 |
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| Which vanishes if 1-3a=3a, ie
a=1/6 |
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| If the energy tensor is traceless
ie |
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| Hence Space-Time is 6D |
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| The divergence of equation 3.2
becomes |
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3.3
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