Question
Question: A small block slides down from rest at point A on the surface of a smooth circular cylinder, as show...
A small block slides down from rest at point A on the surface of a smooth circular cylinder, as shown. At point B, the block falls off (leaves) the cylinder. The equation relating the angles θ1 and θ2 is given by
एक छोटा ब्लॉक बिन्दु A से विरामावस्था से एक चिकने वृत्तीय बेलन पर फिसलता है जैसा कि चित्र में दर्शाया गया है। बिन्दु B पर ब्लॉक बेलन की सतह को छोड़ देता है। कोण θ1 तथा θ2 को सम्बन्धित करने वाली समीकरण होगी ?

2 \cos \theta_1 = 3 \cos \theta_2
Solution
The problem involves a small block sliding down a smooth circular cylinder from rest at point A and leaving the cylinder at point B. We need to find the relationship between the angles θ1 (position of A) and θ2 (position of B), both measured from the vertical axis. Let R be the radius of the cylinder and m be the mass of the block.
1. Conservation of Mechanical Energy (from A to B): The block starts from rest at A, so its initial velocity vA=0. Let's set the potential energy reference at the center of the cylinder.
- At point A:
- Potential Energy PEA=mgRcosθ1.
- Kinetic Energy KEA=0.
- Total Energy EA=mgRcosθ1.
- At point B:
- Potential Energy PEB=mgRcosθ2.
- Let vB be the velocity of the block at B.
- Kinetic Energy KEB=21mvB2.
- Total Energy EB=mgRcosθ2+21mvB2.
Since the surface is smooth (frictionless), mechanical energy is conserved: EA=EB mgRcosθ1=mgRcosθ2+21mvB2 Rearranging to find vB2: 21mvB2=mgR(cosθ1−cosθ2) vB2=2gR(cosθ1−cosθ2) (Equation 1)
2. Newton's Second Law at point B (where the block leaves the cylinder): At point B, the forces acting on the block are:
- Gravitational force mg acting vertically downwards.
- Normal force N acting radially outwards.
For circular motion, the net radial force provides the centripetal force mvB2/R. The component of gravity along the radius towards the center is mgcosθ2. Applying Newton's second law in the radial direction: mgcosθ2−N=RmvB2
The block leaves the cylinder when the normal force N becomes zero. Setting N=0: mgcosθ2=RmvB2 Rearranging to find vB2: vB2=gRcosθ2 (Equation 2)
3. Relating θ1 and θ2: Equate the expressions for vB2 from Equation 1 and Equation 2: 2gR(cosθ1−cosθ2)=gRcosθ2 Divide both sides by gR: 2(cosθ1−cosθ2)=cosθ2 2cosθ1−2cosθ2=cosθ2 2cosθ1=3cosθ2
This is the equation relating the angles θ1 and $\theta_2.