Philip Wood said:
Sorry if this seems patronising, but you do seem very keen to get to the bottom of this stuff.
Of course i am. I am sure you didn't pick that value for radius of gyration randomly. I want to be able to understand the calculations myself.
Philip Wood said:
\frac{L}{\sqrt{12}} is what's called the 'radius of gyration' of the rod about its centre.
I found how the number was obtained. It seems that i was just picking a radius away from my chosen pivot point; which is wrong? It seems that we have to calculate this radius by integrating the stick.
dm = \frac{M}{L}dr
I = \int_{\frac{-L}{2}}^{\frac{L}{2}} r^2 dm = \frac{M}{L} \int_{\frac{-L}{2}}^{\frac{L}{2}} r^2dr
I = \frac{M}{L} \frac{r^3}{3} |_{\frac{-L}{2}}^{\frac{L}{2}} = \frac{M}{3L} (\frac{L^3}{8} + \frac{L^3}{8}) = M \frac{L^2}{12}
However, i question that if finding the radius of gyration this way is really correct? Here is a simple example i am going to use. Assume that our problem, point A is a fixed pivot point. And i am going to try to find the torque of the stick when gravity is the only relevant force.
\tau = \alpha I = \frac{a_t}{r} mr^2 = F_t r
-First, let's calculate the inertia and radius of gyration; with the fixed pivot point A. So the points of integration are from 0 to L.
I = \int_{0}^{L} r^2 dm = \frac{M}{L} \int_{0}^{L} r^2dr = \frac{M}{L} \frac{r^3}{3} |_{0}^{L} = \frac{M}{3L} (L^3 - 0) = M \frac{L^2}{3}
-Therefore the radius of gyration when the pivot is at the end of the stick is: \frac{L}{\sqrt{3}}
-The tangent acceleration that can be obtained by the geometry is equals: a_t = -gcos(\theta)
-Then the torque equals: \tau = \alpha I = \frac{-gcos(\theta)}{\frac{L}{\sqrt{3}}}M \frac{L^2}{3} = \frac{-\sqrt{3}LMgcos(\theta)}{3}
-But the torque is also equals: \tau = F_t r = -Mgcos(\theta) \frac{L}{2}
-Or even if i use the radius of gyration instead of a distance between the pivot and the center of mass: \tau = F_t r = -Mgcos(\theta) \frac{L}{\sqrt{3}}
-Even if i do a mix and match on the torque that contains moment of inertia: \tau = \alpha I = \frac{-gcos(\theta)}{\frac{L}{2}}M \frac{L^2}{3} = \frac{-2LMgcos(\theta)}{3}
One last thing, it took me to try it with a different notation to actually find out that this is wrong:
Philip Wood said:
You agree that y = \frac{L}{2}sin\theta ?
In that case \dot{y} = \frac{L}{2}cos\theta \dot{θ}.
This is what you are doing:
x = y^2
\frac{dx}{dz} = \frac{d}{dz}(y^2) = 2y \frac{dy}{dz} which is wrong