About GR (kst)

You and I are astronauts, sitting on the pad
and the count-down begins, 5,4,3,2,1...blast-off!
at t=1.

The g-meter goes from 1g to 2,3,4,5g and stabilizes.

A mechanical deformation heated the space-craft
as it strained under the effects of the acceleration,
the space-craft was heated and an extra infared
energy was produced and emitted.

You look out the window and find you're still
sitting on the pad......why?

Answer:
At t=1 the Earth's density increased by factors,
1,2,3,4,5, hence it's mass increased likewise
while the volume and radius remained constant.

Using AE's law G_uv=k*T_uv we would find,

Guv at (t=5) = 5*Guv at (t=1) and

Tuv at (t=5) = 5* Tuv at (t=1).

The later is interesting, because as the acceleration
increased, the space-craft was heated and emitted
quantized radiation in the infared spectrum.

The change in Guv from t=1 to t=5 appeared to the
astronaut's to be acceleration, but in fact, it was a
gravitational change given by,

g00-1 (at t=5) = 5*(g00-1) (at t=1),

as the Earth's density increased.

That's AE's law G_uv =k*T_uv in operation with the
Principle of Equivalence.

Normally GRist's use G_uv=0 and Schwart's Solution,
but in juxtaposition this example demo's the induction
of heat when a change in T_uv occurs and creates
quantum radiation using the differential of the realistic

G_uv =k*T_uv.

The induction needs the relative motion of charges,
therefore the AE law applies to a relation.
((the continuum is being replaced by relations))

That differential that outputs the infared radiation is
discontinuous, aka quantized, hence,

T_uv;w =0 ,however,

T_uv;w is not a constant.

but the integral

$ T_uv;w dx^w = a relative constant .

Physically, we're incrementing the energy in
a volume of spacetime by inducing a quanta
of energy like a photon, or perhaps emitting,
as the spacecraft is deformed, and from various
refs, that constant is relativistic.
Ken S. Tucker

.

Relevant Pages

  • Radiation reaction for a uniformly accelerated charge
    ... "Radiation from a uniformly accelerated charge ... can distinguish a charge in uniform acceleration ... radiates energy ... Boulware, "Radiation from a uniformly accelerated charge", ...
    (sci.physics.research)
  • Re: Q. about max acceleration, Plancks constant, PLUS: help locate Sci Am column (Amtr. Sci)
    ... just that the extra energy will be wasted and have no additional ... velocity increases to increase the velocity of the increasing mass. ... I doubt that such extreme acceleration as he would have been ... Beyond certain frequencies, radiation is ...
    (sci.physics)
  • Re: Acceleration of charge
    ... >Finally, if the charge on the rocket radiates, then the energy ... >does the rocket's acceleration decrease as the generator separates ... You can't transform away EM radiation by a frame shift. ...
    (sci.physics.relativity)
  • Re: Electromagnetic radiation of planets
    ... Since a planet is constantly being accelerated in its orbit ... into the Sun as they lose energy through radiation? ... but the acceleration of a planet in a ...
    (sci.physics)
  • Radiation reaction and the equivalence principle (again!)
    ... the radiation reaction force on a charged particle. ... the radiation reaction force vanishes for uniform acceleration. ... the charge will be steadily radiating energy off into the surrounding ...
    (sci.physics.research)