Changes

Adding this dimension requires adding a new term to the classic space-time interval, and so:

Adding this dimension requires adding a new term to the classic space-time interval, and so:

<math>ds^2 = \Bigg( 1 + \frac{\Phi}{c^2}\Bigg)c^2dt^2 - dr^2 + \Bigg(1 + \frac{\Psi}{\tau^2}\Bigg) \tau dv^2</math>

<math>ds^2 = \Bigg( 1 + \frac{\Phi}{c^2}\Bigg)c^2dt^2 - dr^2 + \Bigg(1 + \frac{\Psi}{\tau^2}\Bigg) \tau^2 dv^2</math>

where r is the distance of the object from [[earth]] (or more properly, our [[galaxy]]).

where r is the distance of the object from [[earth]] (or more properly, our [[galaxy]]).