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Original by Michael Weiss
The Twin Paradox: The "General Relativity" Explanation
Calling this the "General Relativity Explanation" raises some
people's hackles; I'll say why below. That's
why "General Relativity" is in quotes, and why "gravitational" is in
scare-quotes for much of this entry.
Some background
This explanation relies on a couple of assertions that are true, according
to GR. (We postpone asking what SR has to say about these assertions.)
- Free choice of reference
frames: You can
describe the physics of a situation in pretty much any reference frame
you like, but some frames demand the introduction of force fields that
don't show up in other frames. You can call these "pseudo-force
fields", or even "gravitational fields".
- Uniform "gravitational" time
dilation: Say you have two
identically constructed clocks. One is deep down in a uniform "gravitational"
potential well (or "pseudo-potential" well, if you prefer); the other
is higher up. If the two clocks compare rates by sending light signals
back and forth, then both will agree that the lower clock runs slower
than the higher clock.
I've phrased these statements as carefully as I know how, short of
resorting to formal mathematics. The short and sloppy versions say,
"You can use accelerated frames of reference, so long as you throw in
some pseudo-force fields"; and "Time runs slower as you descend into the
potential well of a uniform pseudo-force field."
Older books called our first assertion the General Principle of
Relativity, but that term has fallen into disuse. It may remind you
of the Principle of Equivalence, but that's really something
different. The short and sloppy version of that says you
can't distinguish a gravitational field due to matter from a
pseudo-force field. We won't need the Principle of Equivalence here,
so I won't bother with a more careful statement. Even so, you can
probably see the connections: without Equivalence, uniform
"gravitational" time dilation has nothing whatever to do with
gravity. (Call it "pseudo-force time dilation" instead.)
OK, now for the twin paradox
Our usual version, that is.
We'll pick a frame of reference in which Stella is at rest the whole
time! When she ignites her thrusters for the Turnaround, she is
forced to assume that a uniform "gravitational" field suddenly
permeates the universe; the field exactly cancels the force of her
thrusters, so she stays motionless.
Not so Terence. The field causes him to accelerate, but he feels
nothing new since he's in free-fall (or rather the Earth as a whole
is). There's an enormous potential difference between him and Stella:
remember, he's light-years from Stella, in a uniform "gravitational"
field! Stella's at the bottom of the well, he's at the top (or they
would be, if the well weren't bottomless and topless). So
by uniform "gravitational" time dilation, he ages years during Stella's
Turnaround.
Short and sweet, once you have the background! As an added bonus, the
"GR" explanation makes short work of Time Gap and Distance Dependence
Objections. The Time Gap Objection
invites us to consider the limit of an instantaneous Turnaround. But
in that limit, the "gravitational" field becomes infinitely strong,
and so does the time dilation. So Terence ages years in an instant
--- physically unrealistic, but so is instantaneous Turnaround.
The Distance Dependence Objection
finds it odd that Terence's Turnaround ageing should depend on how far
he is from Stella when it happens, and not just on Stella's measurement
of the Turnaround time. No mystery: uniform "gravitational" time dilation
depends on the "gravitational" potential difference, which depends on
the distance.
You may be bothered by the Big Coincidence: how come the uniform
"gravitational" field happens to spring up just as Stella engages her
thrusters? You might as well ask children on a merry-go-round why
centrifugal force suddenly appears when the carnival operator cranks
up the engine. There's a reason such forces have had to endure the
derisive prefix "pseudo" in so many books.
You may find uniform "gravitational" time dilation, the
second assertion, a mite too convenient. Where
did it come from? Is it just a fudge factor that Einstein introduced
to resolve the twin paradox? Not at all. Einstein gave a couple of
derivations for it, having nothing to do with the twin paradox. These
arguments don't need the Principle of Equivalence. I won't repeat
Einstein's arguments (chase down some of the references if you're
curious), but I do have a bit more to say about this effect in the
section titled Too Many Explanations.
Gravitation time dilation without scare quotes (i.e., fields
due to matter) is a different story. These fields are never uniform,
and the derivations just mentioned don't work. The essence of
Einstein's first insight into General Relativity was this: (a) you can
derive time dilation for uniform "gravitational" fields; (b) the
Principle of Equivalence then implies time dilation for gravitational
fields (no scare-quotes). A stunning achievement, but irrelevant to
the twin paradox.
Einstein worked on incorporating gravitation into relativity theory
from 1907 to 1915; by 1915, General Relativity had assumed pretty much
its modern form. (Oh, the mathematicians found some spots to apply
polish and gold-plating, but the conceptual foundations remain the
same.) If you asked him to list the crucial features of General
Relativity in 1907, and again in 1915, you'd probably get very
different lists. Certainly modern physicists have a different list
from Einstein's 1907 list.
Here's my version of Einstein's 1907 list (without worrying too much
about the fine points):
- General Principle of Relativity
- All motion is relative, not just uniform
motion. You will have to include so-called pseudo-forces, however
(like centrifugal force or Coriolis force).
- Principle of Equivalence
- Gravity is not essentially different from any pseudo-force.
The General Principle of Relativity plays a key role in the "GR"
explanation of the twin paradox. And this principle gave General
Relativity its name. So there's certainly historical justification
for the term "GR explanation". Even in 1916, Einstein continued to
single out the General Principle of Relativity as a central feature of
the new theory. (See for example the first three sections of his 1916
paper, "The Foundation of the General Theory of Relativity", or his
popular exposition Relativity.)
Here's the modern physicist's list (again, not sweating the fine
points):
- Spacetime Structure
- Spacetime is a 4-dimensional Riemannian manifold. If you want to
study it with coordinates, you may use any
smooth set of charts (aka local coordinate systems). (This free
choice is what has become of the General Principle of Relativity.)
- Principle of Equivalence
- The metric of spacetime induces a Minkowski metric on the tangent
spaces. In other words, to a first-order approximation, a small patch
of spacetime looks like a small patch of Minkowski spacetime. Freely
falling bodies follow geodesics.
- Gravitation = Curvature
- A gravitational field due to matter exhibits itself as curvature
in spacetime. In other words, once we subtract off the first-order
effects by using a free-falling frame of reference, the remaining
second-order effects betray the presence of a (true) gravitational field.
The third feature finds its precise mathematical expression in the
Einstein field equations. This feature looms so large in the final
formulation of GR, that most physicists reserve the term
"gravitational field" for the fields produced by matter. The phrases
"flat portion of spacetime", and "spacetime without gravitational
fields" are synonymous in modern parlance. "SR" and "flat spacetime"
are also synonymous, or nearly so; one can quibble over whether flat
spacetime with a non-trivial topology (for example, cylindrical
spacetime) counts as "SR". Incidentally, the "modern" usage appeared
quite early. Eddington's book The Mathematical Theory of
Relativity (1922) defines Special Relativity as the theory of
flat spacetime.
So modern usage demotes the uniform "gravitational" field back to its
old status as a pseudo-field, with all the pejorative connotations of
the prefix "pseudo". And the hallmark of a truly GR problem
(i.e., not SR) is that spacetime is not flat. By
contrast, the free choice of charts --- the modern form of the General
Principle of Relativity --- doesn't pack much of a punch. You can use
curvilinear coordinates in flat spacetime. (If you use polar
coordinates in plane geometry, have you suddenly departed the kingdom
of Euclid?)
The usual version of the twin paradox qualifies as a pure SR problem,
by modern standards. Spacetime is ordinary flat Minkowski spacetime.
Stella's frame of reference is just a curvilinear coordinate system.
The Spacetime Diagram Explanation is
closer to the spirit of GR (vintage 1916) than the so-called "GR"
explanation. Spacetime, geodesics, and the invariant interval: that's
the core of GR.
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