Feynman’s Lectures Exercises 2.14 and 2.15

If the weights W1W_1 and W2W_2 move the distance ss along the plane to the left, their corresponding difference in height are:

Δh1=s⋅sin⁡θ,Δh2=−s⋅sin⁡θ\Delta h_1 = s \cdot \sin{\theta} , \quad \Delta h_2 = - s \cdot \sin{\theta}

Then, the difference in potential energy of the system is:

ΔEp=Δh1W1−Δh2W2\Delta E_p = \Delta h_1 W_1 - \Delta h_2 W_2

By the definition of work:

F⋅s=ΔEpF \cdot s = \Delta E_p

Then:

F=ΔEps=sin⁡θ⋅m1⋅g−sin⁡θ⋅m2⋅g=sin⁡θ⋅g⋅(m1−m2)\begin{aligned} F &= \frac{\Delta E_p}{s} \\[10pt] &= \sin{\theta} \cdot m_1 \cdot g - \sin{\theta} \cdot m_2 \cdot g \\[10pt] &= \sin{\theta} \cdot g \cdot (m_1 - m_2) \end{aligned}

For the acceleration along the plane, using a=Fma = \frac{F}{m} and the total mass m=m1+m2m = m_1 + m_2, the acceleration is:

a=sin⁡θ⋅g⋅m1−m2m1+m2a = \sin{\theta} \cdot g \cdot \frac{m_1 - m_2}{m_1+m_2}

For the motion over distance DD, starting from rest:

D=at22D = \frac{at^2}{2}

Thus:

t2=2Dat=2Da\begin{aligned} t^2 &= \frac{2D}{a} \\[10pt] t &= \sqrt{\frac{2D}{a}} \end{aligned}

The speed at time tt is given by:

v=at=a⋅2Da=2Da=2D⋅sin⁡θ⋅g⋅m1−m2m1+m2\begin{aligned} v &= at \\[0pt] &= a \cdot \sqrt{\frac{2D}{a}} \\[10pt] &= \sqrt{2Da} \\[2pt] &= \sqrt {2D \cdot \sin{\theta} \cdot g \cdot \frac{m_1 - m_2}{m_1 + m_2}} \end{aligned}

For Exercise 2.15, the acceleration is given by:

a=12⋅g⋅(sin⁡θ−sin⁡ϕ)a = \frac{1}{2} \cdot g \cdot (\sin{\theta} - \sin{\phi})

Substituting this into the expression for speed, we get:

v=g⋅D⋅(sin⁡θ−sin⁡ϕ)v = \sqrt{g \cdot D \cdot (\sin{\theta} - \sin{\phi})}
Oct 17, 2024 #physics