Energy of a Particle in Free Fall
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In this page an expression
is found for the energy of a stream of photons originating at infinity as
measured by an observer in a spaceship in free-fall. The observer falls from
rest at infinity. The observer is assumed to be falling radially inward toward a
massive spherical body. The Schwarzschild Metric describes the space-time
geometry near a such a body and is given by
Since the Schwarzschild
metric is not an explicit function of time the energy of the falling observer
(i.e. the spaceship), Eobs,
is conserved. Let Pobs
º
m0Uobs
equal the
four-momentum of the spaceship having a four-velocity and proper mass which are,
respectively, Uobs
and m0.
where m = gm0.
Since the motion is radial
The 4-momentum of the
free-fall observer is therefore
The energy of the observer
is defined as Eobs
= (Pobs)0
where
Since Eobs
is constant and has the value m0c2
at infinity and at rest, it follows that Eobs
= m0c2.
To find g we use the
Schwarzschild metric and set df
= dq = 0 and
since the geodesic will be timelike we set ds2
= c2dt2
in Eq. (1) to give
where s
º
1 - GM/c2r.
Divide Eq. (5) through by c2dt2
to give
where br
º dr/d(ct) and
Solving for br
gives
Let the four-momentum of
the photon be P º
(mc, pr,
0, 0). Then the energy of the photon as measured by the observer in
free-fall, Ep,
is given by
The quantity P0
is the energy of the photon. Since this is a constant it has the same value as
it has at infinity and therefore
The quantity P1
has the value given by
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