In Gμν=(8πG/c⁴)Tμν, what do the indexed tensors describe?
Which tensor records local curvature measured through infinitesimal parallel-transport loops?
If one vector returns unchanged around one small loop, every local curvature component must be zero.
Circle one: True False
For a nearly static weak field and slow matter, which equation does the Einstein field equation recover?
A vector returns rotated after parallel transport around a small contractible loop in a smooth region. What does this establish?
In the displayed convention Gμν=κTμν, what coupling κ is fixed by matching Newtonian gravity?
With zero cosmological constant, a vacuum region has Rμν=0. Must its full Riemann tensor also vanish?
A student gives Tμν everywhere and claims this alone selects one spacetime metric. What information can still be needed?