Energies associated "with the indicated frame only" include the kinetic energy of motion, as well as potential energies associated with "geometric forces" which arise in accelerated frames and in curved spacetime. Strangely enough, all of these framespecific energies seem to connect to "differentialaging" γ ≡ dt/dτ i.e. via a relation of the form (γ1)mc^{2}. One thing we will try to deal with in these pages is to explore other places where (γ1) comes in handy for describing "indicated frameonly" effects.
local time and motion
An object's momentum p = mw is the product of its frameinvariant restmass m, and its synchronyfree propervelocity w ≡ Δx/Δτ = γv where Lorentzfactor or "speedofmaptime" γ ≡ Δt/Δτ = 1/Sqrt[1(v/c)^{2}] ≥ 1 and coordinatevelocity v ≡ Δx/Δt. Here τ is frameinvariant propertime elapsed on the clocks of our traveler, and t is maptime measured on clocks fixed to the yardsticks used to measure mapposition x.
Greek letter "Delta" (Δ) in front of any thing means "change in" i.e. the difference between final and initial values of that thing. At low speeds, p ≈ mv.
Similarly an object's translational kinetic energy (e.g. in Joules) is
approximately half its mass m times the square of its speed v^{2}, i.e.
 .
where c ≈ 3×10^{8}[m/s] is the spacetime constant that we call lightspeed for historical reasons.
Thus kinetic energy is directly related to the faster passage of map (t) with respect to traveler (τ) time when simultaneity is defined by the mapframe. However, strangely enough, in nonfreefloat or "geometric force" settings (where forces acting on every ounce of your being materialize) a similar relationship linked to your position rather than your speed also materializes.
local time and rotation
An easy to understand example of a geometric force welldepth arises in the case of rotational artificial
gravity, provided at least that we ignore azimuthal forces which also operate as one's radius is changed. It is simpler because the differential aging arises purely from
the tradeoff between kinetic energy in a single freefloat frame, and
geometric "potential energy" whose (negative energy) welldepth to corotating travelers is

Taking the derivative of this, and
dividing by m, gives a simulated gforce as a function of radius of the
form g = γ^{3}ω^{2}r which reduces to the classical value of ω^{2}r when r << c/ω. Note that the γ^{3} factor similarly relates properacceleration to coordinateacceleration in (1+1)D flat spacetime. This "centrifugal acceleration" in an accelerated traveler's frame is perhaps the simplest case of a geometricforce (and associated "potential") linked to differential aging.
local time and work
A similar type of differential aging takes place when an extended object of length L in flat spacetime undergoes constant properacceleration α. One obtains (at least for αL << c^{2}, with details depending on how you define simultaneity) for the "welldepth" or work needed to climb up from the trailing to the leading edge, e.g. of your accelerating spaceship, something like:
 .
Here t_{trailing} might also be thought of as time τ on the clocks of a passenger getting ready to "make the climb" from the trailing to the leading end of her accelerating home. This example is complicated by the fact that no single freefloat frame can be used to see this geometric "potentialenergy" as a direct tradeoff with kinetic energy, as was possible in the rotation case above.
local time and gravity
The accelerated ship example above is transition from the purely kinetic centrifugal potential, and the purely motionless gravitational potential around a spherical object. Here the traveler's separation r, between the center of a massM spherical object with gravitationalacceleration g_{rM}, puts them into a potentialenergy well whose depth (i.e. "escape energy") is:
where here gravity's acceleration is g_{rM} = GM/r^{2} and speedoffartime is Δt_{far}/Δτ = 1/Sqrt[12GM/(c^{2}r)] ≥ 1, Δt_{far} is time elapsed on "Schwarzschild" mapclocks far away from our object, and Δτ
(also used above) is the "proper" timeelapsed on observer clocks
nearer to the object surface. Put another way, acceleration due to
gravity is g_{rM} = (Δt_{far}/Δτ1)c^{2}/r. In other words: On earth stuff falls because when standing "your head ages faster than your feet".
local time and energy overview
Given an energydifference ΔE between states, one can sometimes at least imagine an associated differentialtime ratio like dt/dτ ≈ 1+ΔE/mc^{2}.
Note that the higher and lower energy states change positions in the
kinetic energy case, which is why globalpositioningsystem (GPS)
satellite clocks are sped up by increasing orbitalaltitude, but slowed
down by increasing orbitalspeed.
Thus kineticenergy, and for geometric ("connectioncoefficient") forces potentialenergy and work, may all be intimately linked to local differences in the rate at which time passes! In other words, very small amounts of differential aging (like the dt/dτ ≈ 10^{9} associated with gravity here on earth's surface) can have verysignificant physical consequences.