Sigma Percentile
JEE Advanced 1998
LEVELJEE Advanced

Animated Solution for Physics - Work, Energy, and Power: A particle of mass is moving along the positive X-axis under the influence of a force where . At time , it is at and its velocity . (a) Find its velocity when it reaches . (b) Find the time at which it reaches .

Visualized Solution

Analyzing the Setup

  • Particle of mass starts from rest at .
  • Force is always negative (since and ).
  • The particle will accelerate towards the origin (negative X-direction).

Work-Energy Theorem

  • To find the velocity at , we use the Work-Energy Theorem: .
  • .
  • Since , the work done equals the final kinetic energy.

Setting up the Integral

  • Substitute the force expression into the work integral.
  • .
  • We can pull the constants out: .

Evaluating the Work Done

  • The integral of is .
  • .
  • .

Velocity at

  • Equate work to kinetic energy: .
  • Given and , we get .
  • .
  • Since the particle moves in the negative X-direction, .

General Velocity Function

  • For part (b), we need the time to reach . First, find velocity as a function of .
  • Integrate from to an arbitrary position .
  • .

Expression for

  • .
  • Since , we have .
  • Taking the square root and choosing the negative sign (moving left): .

Kinematic Relation

  • Velocity is the rate of change of position: .
  • Therefore, .
  • We need to separate variables to solve for time .

Separating Variables

  • Rearrange to isolate : .
  • Integrate both sides from the initial state () to the final state ().
  • .

Trigonometric Substitution

  • The integral is a classic form solved by trigonometric substitution.
  • Let .
  • Then the differential is .

Transforming the Integral

  • Substitute : .
  • The integrand becomes: .
  • Using the double angle identity: .

Changing the Limits

  • Initial limit: .
  • Final limit: .
  • The time integral is .

Evaluating the Time Integral

  • Integrate: .
  • Apply limits: .
  • .

Final Calculation

  • .
  • .
  • Substituting and : .

The Sigma Insight: Work Done by Forces

Solution Diagram

The Journey to the Origin

A Tale of Work, Energy, and Calculus
Imagine a particle resting peacefully on the positive X-axis at . Suddenly, it experiences a force pulling it towards the origin. But this isn't just any constant force; it's a force that grows stronger as the particle gets closer to the origin, given by the inverse-square law .
Because the force is variable, we cannot rely on our standard kinematic equations like . Those are strictly reserved for constant acceleration. Instead, we must summon the elegant power of the Work-Energy Theorem and Calculus.

Part A

The Work-Energy Theorem
To find the velocity of the particle when it reaches , we need to calculate the work done by this variable force. The Work-Energy Theorem states that the net work done on an object equals its change in kinetic energy:
Since the particle starts from rest, , meaning the work done will directly equal the final kinetic energy. Let's set up the integral for the work done as the particle moves from to :
Pulling the constant out of the integral, we are left with integrating , which is simply .
Evaluating the limits, we get .
Now, we equate this work to the kinetic energy:
Given that and , the ratio is exactly . Therefore, , which gives . Since the force is pulling the particle in the negative X-direction, we must choose the negative root.
The velocity at is .

Part B

The Kinematic Differential Equation
Now for the real challenge: finding the exact time it takes to reach . To find time, we first need velocity as a general function of position, . We repeat our Work-Energy integration, but this time, we integrate from to an arbitrary position :
Equating this to kinetic energy and substituting , we get:
Taking the negative square root (because it's moving left), we find our velocity function:
Velocity is fundamentally the rate of change of position, . This gives us a beautiful, yet intimidating, differential equation:

The Calculus Climax

To solve for time, we separate the variables, moving all terms to one side and to the other:
Integrating both sides from the initial state () to the final state ():
This integral is a classic candidate for trigonometric substitution. The term in the denominator screams for the Pythagorean identity. Let's substitute . This means the differential becomes .
The square root simplifies beautifully:
Multiplying this by our new , the integrand transforms into:
Using the double-angle identity, .
We must also update our limits. When , , so . When , , so , which means .
Our time integral is now a straightforward trigonometric evaluation:
Integrating yields . Applying the limits:
Substituting the approximate values and , we get:
The particle reaches at exactly . A perfect harmony of physics and calculus!

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