Rotation  

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]


Main pageAbbreviationsJournalsCommentsOther sitesAcknowledgements
Send feedback and suggestions to bombelli at olemiss.edu – Modified 20 jun 2008