NSEP 2015 Problem 3 | Rotational Motion

Try out this problem on the concept of Angular momentum from National Standard Examination in Physics 2015-2016.

NSEP 2015-16 ~ Problem 3


A particle of mass 10g starts from rest at $t=0$s from point (0m, 4m) and gets accelerated at $0.5m/ s^2$ along $x-\sqrt{3}y + 4\sqrt{3}=0$ in XY plane. The angular momentum of the particle about the origin (in SI units) at $t=2$s is
(a) $-0.01\sqrt{3} \hat{k}$
(b) $-0.02\sqrt{3}\hat{k}$
(c) Zero
(d) $-20\sqrt{3}\hat{k}$

Key Concepts


Circular Motion

Center of Curvature for generalised motion

Vector and their Components

Suggested Book | Source | Answer


Concept of Physics H.C. Verma

University Physics by H. D. Young and R.A. Freedman

Fundamental of Physics D. Halliday, J. Walker and R. Resnick

National Standard Examination in Physics(NSEP) 2015-2016

Option-(b) $-0.02\sqrt{3}\hat{k}$

Try with Hints


The first thing to remember is that Even if a particle is not moving in a circle, then also it can have circular motion, i.e., Angular Momentum, Torque, Centripetal forces can exist.

This is the case because any random curves can be approximated bu circles. Even straight lines are circles with radius $\to \infty$.

You can use the circle's centre as the centre of rotation or you can also use the origin. Using the origin is often easier as the positions can be directly given using position vectors.

In our problem, The motion is happening on the line $y = \frac{x}{\sqrt{3}}+4$.

If at any moment of time it's velocity along the curve is $\vec{v}=v_x \hat{i}+v_y \hat{j}$ and it's position vector is $\vec{r}=x \hat{i}+y \hat{j}$ then, It's angular momentum ($\vec{L}$) with respect to origin can be given by,

$$\vec{L} = m(\vec{v}\times \vec{r}) $$

where m is the mass of the particle.

From the previous image, if $(x,y)$ is then they must satisfy $y = \frac{x}{\sqrt{3}}+4$. Differentiating with respect to time,

$$\frac{dy}{dt} = \frac{1}{\sqrt{3}}\frac{dx}{dt} \to v_y = \frac{v_x}{\sqrt{3}}$$

Again differentiating w.r.t time,

$$a_y = \frac{a_x}{\sqrt{3}}$$ where $\vec{a} = a_x\hat{i}+a_y\hat{j}$ is the acceleration (we will not need this but I think it should be written here as we can also use this in solution).

Now at $t=0$, $v_x=0$. Hence, at $t=2s$, $v_x $=$ a_xt $= $a\cos(30^{\circ})t $= $0.5\frac{\sqrt{3}}{2} 2 $= $\frac{\sqrt{3}}{2}$

Now, $x$ = $v_x(t=0 )t+\frac{1}{2}a_x t^2$ = $0 + \frac{1}{2}a\cos(30^{\circ})2^2$ = $\frac{\sqrt{3}}{2} $

Then, $v_y = \frac{v_x}{\sqrt{3}}= \frac{1}{2}$ and $y = \frac{x}{\sqrt{3}} + 4 = \frac{1}{2} + 4 = \frac{9}{2}$.

Hence, $\vec{r}$ = $\frac{\sqrt{3}}{2}\hat{i} + \frac{9}{2}\hat{j}$ and $\vec{v}$ = $\frac{\sqrt{3}}{2}\hat{i} + \frac{1}{2}\hat{j}$.

$\vec{L}$=$m(\vec{r} \times \vec{v})$=$-m 2 \sqrt{3} \hat{k}$=$-\left(\frac{10}{1000}\right) 2 \sqrt{3} \hat{k}$=$-0.02 \sqrt{3} \hat{k}$

Note: The answer is asked in S.I unit. So, m = 10g = $\frac{10}{1000}$kg = 0.01.

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NSEP 2015 Problem 2 | Rotational Motion

Try out this problem on Rotational Motion from National Standard Examination in Physics 2015-2016.

NSEP 2015-16 ~ Problem 2


A body of mass m and radius R rolling horizontally without slipping at a speed v climbs a ramp to a height $\frac{3v^2}{4g}$. The rolling body can be
(a) A Sphere
(b) A circular Ring
(c) A Spherical Shell
(d) A Circular Disc

Key Concepts


Rotational Mechanics

Rolling without Slipping

Energy Conservation

Suggested Book | Source | Answer


Concept of Physics H.C. Verma

University Physics by H. D. Young and R.A. Freedman

Fundamental of Physics D. Halliday, J. Walker and R. Resnick

National Standard Examination in Physics(NSEP) 2015-2016

Option-(d) A Circular Disc

Try with Hints


Notice that It's a motion without slipping. This implies that the point of contact between the body and the ground has zero relative velocity.

If the relative velocity between the ground and object is 0, then we can use the relation $v = \omega R$, where $\omega $ is the angular velocity.

We know the kinetic energy for the rotational motion is,

$$K_{rot} = \frac{1}{2}I^2 \omega = \frac{Iv^2}{2R^2}$$

Hence, the total kinetic energy is,

$K_{\text {tot }}=K_{\text {linear }}+K_{\text {rot }}$=$\frac{1}{2} m v^{2}+\frac{I v^{2}}{2 R^{2}}$=$\frac{m v^{2}}{2}\left(1+\frac{I}{m R^{2}}\right)$

The object can only go upto the height $\frac{3v^2}{4g}$. At that height it's kinetic energy will be zero and all the energy will be potential energy. So, the potential energy at that height is,

$$ V = mgh = mg\frac{3v^2}{4g} = \frac{3}{4}mv^2 $$

Using the conservation of energy,

$\frac{m v^{2}}{2}\left(1+\frac{I}{m R^{2}}\right)=\frac{3}{4} m v^{2} \rightarrow I$

$=\frac{1}{2} m R^{2}$

We know this is the Moment of Inertia of a Circular disc. Hence, the object is a circular disc.

There is a nice way to remember those moment of inertia values of some standard bodies. , Maybe we will see that in some later blog.

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