Question 705046

SCQHARD

A particle of mass mm is moving in a potential V(r)=−krV(r) = -\frac{k}{r}, where kk is a positive constant. If L⃗\vec{L} and p⃗\vec{p} denote the angular momentum and linear momentum respectively, the value of α\alpha for which A⃗=L⃗×p⃗+αmkr^\vec{A} = \vec{L} \times \vec{p} + \alpha mk \hat{r} is a constant of motion, is

(A)

-2

(B)

-1

(C)

2

(D)

1

Detailed Solution

Step 1: Identify the Force

The given potential is V(r)=−krV(r) = -\frac{k}{r}.

The central force is the negative gradient of this potential:

F⃗=−∇V(r)=−ddr(−kr)r^=−kr2r^\vec{F} = -\nabla V(r) = -\frac{d}{dr} \left(-\frac{k}{r} \right) \hat{r} = -\frac{k}{r^2} \hat{r}

According to Newton's Second Law, the force is equal to the rate of change of linear momentum (p⃗\vec{p}):

dp⃗dt=−kr2r^\frac{d\vec{p}}{dt} = -\frac{k}{r^2} \hat{r}

Step 2: Angular Momentum Property

For a central force, the torque is zero (τ⃗=r⃗×F⃗=0\vec{\tau} = \vec{r} \times \vec{F} = 0). Therefore, the angular momentum L⃗\vec{L} is conserved (constant in time):

dL⃗dt=0\frac{d\vec{L}}{dt} = 0

Step 3: Set up the Constant of Motion Condition

We are given that A⃗\vec{A} is a constant of motion, which means its time derivative must be zero:

dA⃗dt=ddt(L⃗×p⃗+αmkr^)=0\frac{d\vec{A}}{dt} = \frac{d}{dt} (\vec{L} \times \vec{p} + \alpha m k \hat{r}) = 0

First, let's evaluate the time derivative of L⃗×p⃗\vec{L} \times \vec{p}:

ddt(L⃗×p⃗)=dL⃗dt×p⃗+L⃗×dp⃗dt\frac{d}{dt} (\vec{L} \times \vec{p}) = \frac{d\vec{L}}{dt} \times \vec{p} + \vec{L} \times \frac{d\vec{p}}{dt}

Since dL⃗dt=0\frac{d\vec{L}}{dt} = 0, the first term vanishes:

ddt(L⃗×p⃗)=L⃗×(−kr2r^)=−kr2(L⃗×r^)\frac{d}{dt} (\vec{L} \times \vec{p}) = \vec{L} \times \left( -\frac{k}{r^2} \hat{r} \right) = -\frac{k}{r^2} (\vec{L} \times \hat{r})

Step 4: Solve the Vector Triple Product

We know that L⃗=r⃗×p⃗=m(r⃗×r⃗˙)\vec{L} = \vec{r} \times \vec{p} = m(\vec{r} \times \dot{\vec{r}}). Substituting this into the cross product:

L⃗×r^=m(r⃗×r⃗˙)×r^=−m[r^×(r⃗×r⃗˙)]\vec{L} \times \hat{r} = m(\vec{r} \times \dot{\vec{r}}) \times \hat{r} = -m \left[ \hat{r} \times (\vec{r} \times \dot{\vec{r}}) \right]

Now, apply the vector triple product identity, A⃗×(B⃗×C⃗)=B⃗(A⃗⋅C⃗)−C⃗(A⃗⋅B⃗)\vec{A} \times (\vec{B} \times \vec{C}) = \vec{B}(\vec{A} \cdot \vec{C}) - \vec{C}(\vec{A} \cdot \vec{B}):

=−m[r⃗(r^⋅r⃗˙)−r⃗˙(r^⋅r⃗)]= -m \left[ \vec{r}(\hat{r} \cdot \dot{\vec{r}}) - \dot{\vec{r}}(\hat{r} \cdot \vec{r}) \right]

Using the standard properties r^⋅r⃗=r\hat{r} \cdot \vec{r} = r and r^⋅r⃗˙=r˙\hat{r} \cdot \dot{\vec{r}} = \dot{r}:

=−m[r⃗r˙−r⃗˙r]=m[rr⃗˙−r⃗r˙]= -m [ \vec{r}\dot{r} - \dot{\vec{r}}r ] = m [ r\dot{\vec{r}} - \vec{r}\dot{r} ]

Step 5: Re-substitute and Recognize the Derivative

Substitute this result back into the derivative equation from Step 3: ddt(L⃗×p⃗)=−kr2×m[rr⃗˙−r⃗r˙]=−mk[rr⃗˙−r⃗r˙r2]\frac{d}{dt} (\vec{L} \times \vec{p}) = -\frac{k}{r^2} \times m [ r\dot{\vec{r}} - \vec{r}\dot{r} ] = -mk \left[ \frac{r\dot{\vec{r}} - \vec{r}\dot{r}}{r^2} \right]

The expression inside the bracket is exactly the quotient rule applied to the time derivative of the unit vector r^\hat{r} (where r^=r⃗r\hat{r} = \frac{\vec{r}}{r}):

ddt(r⃗r)=rr⃗˙−r⃗r˙r2=dr^dt\frac{d}{dt} \left( \frac{\vec{r}}{r} \right) = \frac{r\dot{\vec{r}} - \vec{r}\dot{r}}{r^2} = \frac{d\hat{r}}{dt}

Thus, the equation simplifies to:

ddt(L⃗×p⃗)=−mkdr^dt\frac{d}{dt} (\vec{L} \times \vec{p}) = -mk \frac{d\hat{r}}{dt} Rearranging the terms:

ddt(L⃗×p⃗+mkr^)=0\frac{d}{dt} (\vec{L} \times \vec{p} + mk \hat{r}) = 0

Final Step: Compare to Find α\alpha Our derived constant vector is: L⃗×p⃗+mkr^\vec{L} \times \vec{p} + mk \hat{r}

The vector given in the problem is: A⃗=L⃗×p⃗+αmkr^\vec{A} = \vec{L} \times \vec{p} + \alpha m k \hat{r}

By directly comparing the two expressions, we get:

αmkr^=mkr^\alpha m k \hat{r} = m k \hat{r}

α=1\alpha = 1

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