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{{expert-subject|1=physics|date=April 2012}}
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The '''tennis racket theorem''' is a result in [[classical mechanics]] describing movement of a rigid body with three distinct [[Angular momentum|angular momenta]].  It also dubbed '''Dzhanibekov effect''' named after [[Russian people|Russian]] [[astronaut]] [[Vladimir Dzhanibekov]] who discovered the theorem's consequences while in space in 1985.<ref>[http://oko-planet.su/science/sciencehypothesis/15090-yeffekt-dzhanibekova-gajka-dzhanibekova.html]</ref>
 
== Qualitative Proof ==
The tennis racket theorem can be qualitatively analysed with the help of [[Euler's equations (rigid body dynamics)|Euler's equations]].
 
Under torque free conditions, they take the following form:
:<math>
\begin{align}
I_1\dot{\omega}_{1}&=(I_2-I_3)\omega_2\omega_3~~~~~~~~~~~~~~~~~~~~\text{(1)}\\
I_2\dot{\omega}_{2}&=(I_3-I_1)\omega_3\omega_1~~~~~~~~~~~~~~~~~~~~\text{(2)}\\
I_3\dot{\omega}_{3}&=(I_1-I_2)\omega_1\omega_2~~~~~~~~~~~~~~~~~~~~\text{(3)}
\end{align}
</math>
 
 
Let <math> I_1 > I_2 > I_3 </math>
 
Consider the situation when the object is rotating about axis with moment of inertia <math>I_1</math>. To determine the nature of equilibrium, assume small initial angular velocities along the other two axes. As a result, according to equation (1), <math>~\dot{\omega}_{1}</math> is very small. Therefore the time dependence of <math>~\omega_1</math> may be neglected.
 
Now, differentiating equation (2) and substituting <math>\dot{\omega}_3</math> from equation (3),
:<math>
\begin{align}
I_2 I_3 \ddot{\omega}_{2}&= (I_3-I_1) (I_1-I_2) \omega_1\omega_{2}\\
\text{i.e.}~~~~ \ddot{\omega}_2 &= \text{(negative quantity)} \times \omega_2
\end{align}
</math>
 
Note that <math>\omega_2</math> is being opposed and so rotation around this axis is stable for the object.
 
Similar reasoning also gives that rotation  around axis with moment of inertia <math>I_3</math> is also stable.
 
Now apply the same thing to axis with moment of inertia <math>I_2</math>. This time <math>\dot{\omega}_{2}</math> is very small. Therefore the time dependence of <math>~\omega_2</math> may be neglected.
 
Now, differentiating equation (1) and substituting <math>\dot{\omega}_3</math> from equation (3),
:<math>
\begin{align}
I_1 I_3 \ddot{\omega}_{1}&= (I_2-I_3) (I_1-I_2) \omega_1\omega_{2}\\
\text{i.e.}~~~~ \ddot{\omega}_1 &= \text{(positive quantity)} \times \omega_1
\end{align}
</math>
 
Note that <math>\omega_1</math> is '''not''' opposed and so rotation around this axis is '''unstable'''. Therefore even a small disturbance along other axes causes the object to 'flip'.
 
== See also ==
*[[Euler angles]]
*[[Moment of inertia]]
*[[Poinsot's ellipsoid]]
*[[Polhode]]
 
== References ==
{{reflist}}
* Mark S. Ashbaugh, Carmen C. Chicone and Richard H. Cushman,  [http://math.ucalgary.ca/files/publications/cushman/tennis.pdf The  Twisting  Tennis  Racket], ''Journal of Dynamics and Differential Equations'', Volume 3, Number 1, 67-85 (1991). 
* [http://www.youtube.com/watch?v=L2o9eBl_Gzw Dzhanibekov effect video] demonstrated on the [[International Space Station]]
 
 
 
{{classicalmechanics-stub}}
[[Category:Classical mechanics]]
[[Category:Physics theorems]]

Latest revision as of 23:05, 4 December 2014

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