Sunday, February 26, 2017

Same Old, Same Old

We have seen this before, with conservation of energy where \(c^2\) is a constant,

\({v}^{2}_{t}+{v}^{2}_{s} = {c}^{2}\)

differentiating both sides with respect to time,

\(2{v}_{t}\cfrac{d{v}_{t}}{dt}+2{v}_{s}\cfrac{d{v}_{s}}{dt} = 0\)

\({v}_{t}\cfrac{d{v}_{t}}{dx}\cfrac{dx}{dt}+{v}_{s}\cfrac{d{v}_{s}}{dt} = 0\)

\({v}_{t}\cfrac{d{v}_{t}}{dx}{v}_{s}+{v}_{s}\cfrac{d{v}_{s}}{dt} = 0\)

\({v}_{t}\cfrac{d{v}_{t}}{dx} = - \cfrac{d{v}_{s}}{dt}=-g\) --- (*)

And

\(E_t=mv_t^2\)

(*) becomes,

\(\cfrac{1}{2}\cfrac{d{v}^2_{t}}{dx}=\cfrac{1}{2m}\cfrac{d\,E_t}{dx} = -g\)

\(-\cfrac{d\,E_t}{dx}=2mg\)

where the minus sign indicates a decreasing time potential field \(E_t\) with \(x\) in the direction of \(g\).

In a gravity well, around a planet or black hole, we also has a time potential well.  This time potential is at its minimum when gravity is at its maximum.

Good day.