Dance Of The Spaghetti

When we cook spaghetti, noodles loosen up as they take on water, and undergo a beautiful choreography driven by the thermal energy of the boiling water. Although they become more flexible, they still maintain some structure, i.e. they are smooth curves.

We can make a crude model of the spaghetti noodle as a chain of N N short rods of length δ l \delta l that are connected end to end, but otherwise free to rotate about the connections. Under these assumptions, calculate the root mean squared distance (in cm \si{\centi\meter} ) between the ends of the noodle (i.e. the blue and red balls in the diagram) as it dances in the pot.

Details and Assumptions :

  • δ l = 1 mm \delta l = 1 \si{\milli\meter} .
  • N = 350 N = 350 .
  • Ignore the nasty issue of the fact that spaghetti cannot pass through itself.
  • Assume the spaghetti is alone in the pot ​and doesn't interact with the walls.


The answer is 1.870828693.

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1 solution

Josh Silverman Staff
Jul 22, 2016

The displacement d \vec{d} between the start and end of a dancing spaghetti noodle can be written as the sum of displacements between the end points of the small, contiguous rods. If we write the displacement vector between hinge i 1 i-1 and hinge i i as r i \vec{r}_i , we have d = i r i \vec{d} = \sum_i\vec{r}_i .

The square of this is then d 2 = ( r 1 + r 2 + + r N ) ( r 1 + r 2 + + r N ) = ( r 1 2 + r 2 2 + + r N 2 ) + ( r 1 r 2 + r 1 r 3 + + r N 1 r N ) = N δ l 2 + δ l 2 i j cos θ i j \begin{aligned} \vec{d}^2 &= \left(\vec{r}_1 + \vec{r}_2 + \ldots + \vec{r}_N\right)\cdot\left(\vec{r}_1 + \vec{r}_2 + \ldots + \vec{r}_N\right) \\ &= \left(r_1^2 + r_2^2 + \ldots + r_N^2\right) + \left(\vec{r}_1\cdot\vec{r}_2 + \vec{r}_1\cdot\vec{r}_3+\ldots + \vec{r}_{N-1}\cdot\vec{r}_N\right) \\ &= N\delta l^2 + \delta l^2\sum_{i\neq j} \cos\theta_{ij} \end{aligned} where θ i j \theta_{ij} is the angle between displacement vectors i i and j j .

We must average this expression over all possible realizations to find the mean squared distance d 2 \langle d^2\rangle . As there is no correlation between adjacent displacement vectors (and no long range correlation either), we have d 2 = N δ l 2 + δ l 2 i j cos θ i j zero = N δ l 2 \begin{aligned} \langle d^2 \rangle &= N\delta l^2 + \delta l^2 \sum_{ij}\overbrace{\langle\cos\theta_{ij}\rangle}^{\textrm{zero}} \\ &= N\delta l^2 \end{aligned} So that the root mean squared distance is simply N δ l \sqrt{N}\delta l .

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