In General > s.a. kinematics
of special relativity.
* In R3:
An element R of
SO(3), which can be parametrized by Euler angles, R(
,
,
)
= R3(
) R1(
)
R3(
).
* Vector fields: In generalized
Cartesian coordinates,
1 =
(0; 0, z, –y) ,
2
= (0; –z, 0, x) ,
3
= (0; y, –x, 0) ;
in spherical coordinates,
1 =
(0; 0, sin
, cot
cos
) ,
2
= (0; 0, –cos
, cot
sin
) ,
3
= (0; 0, 0, –1) .
* Of a world-line: Its
meaning is well-defined, not just wrt something – it can be measured
by a spiked sphere with springs and beads; To define it quantitatively,
introduce 3 orthogonal vectors ua, va and wa
on the
world-line; The rate of change of these vectors measures the rotation;
There is no rotation iff
m
m
ua =
a (umAm),
m
m va =
a (vmAm),
and
m
m wa =
a (wmAm),
where
a is
the unit tangent to the world-line.
* Measurement: The most
sensitive instruments are laser gyroscopes, and
atom interferometers; The latter have sensitivities of one-hundredth of a
degree/min
[@ Lenef et al PRL(97)
+ pn(97)feb],
and potentially much less.
> Related concepts
and systems: see angular momentum; stars.
Rotational Invariance in Physics > see realism; spherical symmetry; [symmetry].
References > s.a. time [rotating clocks].
@ General: Walker 90; Malament gq/00-in
[general relativity criteria vs intuition]; Bel gq/03 [Wilson-Wilson,
Michelson-Morley experiments].
@ Related topics: Hawking Obs(69) [of the universe].
@ Teaching: Silva & Tavares AJP(07) [angular momentum and angular velocity]
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Send feedback and suggestions to bombelli at olemiss.edu – Modified
20 jun 2008