Analyzing the Setup
Welcome, future engineers! Today, we are not just solving a kinematics problem; we are dissecting the very geometry of motion. Imagine two particles, A and B, standing at the starting line.
They are about to embark on a journey where they accelerate from rest to a common final velocity, v. They do so with different accelerations, f and f′. This is a classic JEE Advanced scenario where the algebra can get messy if you dive in blindly, but if you look at it through the lens of a velocity-time graph, the complexity melts away.
Phase 1
The Velocity-Time Landscape
Let us visualize this. On a velocity-time graph, the vertical axis is velocity, and the horizontal axis is time. Both particles start at the origin (0,0).
Since they accelerate constantly, their paths are straight lines. The slope of these lines represents the acceleration. We are told that particle A takes m seconds more than B to reach the same speed v.
This means A's line is 'gentler'—it has a smaller slope, f, while B's line is steeper, with slope f′. This geometric intuition is our first victory.
Phase 2
The Algebra of Time
Now, let us translate this into the language of equations. For any object starting from rest with constant acceleration a, the first equation of motion is v=u+at. Since u=0, we have v=at, or t=av.
For particle A, the time taken is tA=fv. For particle B, the time taken is tB=f′v.
We are given that A takes m seconds more than B, so tA−tB=m. Substituting our expressions, we get:
Factoring out v, we arrive at our first pillar of truth:
v(ff′f′−f)=m(Equation 1)
Phase 3
The Geometry of Distance
Next, we look at the distance covered. In a velocity-time graph, the distance is the area under the line. For a triangle with base t and height v, the area is:
Since t=av, the distance is s=2av2. Thus, the distance for A is sA=2fv2, and for B, it is sB=2f′v2.
We are told A covers n units more than B, so sA−sB=n. Substituting our expressions:
Factoring out 2v2, we get our second pillar:
2v2(ff′f′−f)=n(Equation 2)
Phase 4
The Elegant Cancellation
Here is where the magic happens. Look at Equation 1 and Equation 2. They share the exact same term: ff′f′−f.
This is not a coincidence; it is the symmetry of the problem. If we divide Equation 2 by Equation 1, that entire complex term vanishes:
v(ff′f′−f)2v2(ff′f′−f)=mn
This simplifies to 2v=mn, which gives us the final velocity:
The Final Result
We are almost home. Substitute v=m2n back into Equation 1:
Multiply both sides by m and rearrange:
And there it is! We have arrived at the solution. This result is not just a collection of variables; it is a testament to the power of looking for symmetry in physics. When you face these problems in the exam, do not just calculate—observe. The math will always reward you for it.