According to
general relativity calculations, as one passes the event horizon (the point of no return) of a black hole, space and time switch roles.
Not exact matches
Li's solution to this problem is disarmingly simple, but is backed up by
calculations based on Einstein's
general theory of
relativity.
Her
calculations helped Einstein formulate his
general theory of
relativity.
When Albert Einstein first applied his theory of
general relativity to the universe as a whole, to make the
calculations workable, he was forced to assume that one large part looks much like any other large part.
And the amazing thing is that the amount of lensing that we found through these
calculations is consistent with what Einstein's
general relativity theory predicted.
New
calculations extend Einstein's
general theory of
relativity into the universe's first few moments
Leif Svalgaard says: August 7, 2011 at 10:52 am The
calculations at JPL of Mercury's orbit include the
general relativity effects and are correct to a few meters and confirm the precession to a few arc seconds / century.
The
calculations at JPL of Mercury's orbit include the
general relativity effects and are correct to a few meters and confirm the precession to a few arc seconds / century.
Dr. Singer was the first to make the correct
calculations for using atomic clocks in orbit, contributing to the verification of Einstein's
General Theory of
Relativity, and now essential in the GPS system of satellite navigation.