The Symphony of Conservation Laws
In physics, conservation laws are the ultimate cheat codes. They allow us to bypass complex, time-dependent equations and jump straight to profound conclusions about a system's behavior. In this beautiful problem, we are presented with four distinct trajectories of a particle. Our mission is to act as cosmic detectives and determine which physical quantities—linear momentum (p), angular momentum (L), kinetic energy (K), potential energy (U), and total energy (E)—remain invariant as the particle dances through space.
Before we dive into the math, let's establish our ground rules:
- Linear Momentum (p) is conserved if and only if the velocity vector v is strictly constant in both magnitude and direction.
- Kinetic Energy (K) is conserved if the speed ∣v∣ is constant.
- Angular Momentum (L) is conserved if the net torque τ=r×F is zero. This happens when the force is zero or when it is a central force (parallel or anti-parallel to r).
- Total Energy (E) is conserved if the force acting on the particle is either zero or conservative.
- Potential Energy (U) is conserved if both E and K are conserved, since E=K+U.
Let's analyze each path one by one.
Path A
The Straight Line (The Trivial Case)
The position vector is given by:
Taking the first derivative with respect to time, we find the velocity:
Notice that the velocity is a constant vector! Because v is constant, the linear momentum p=mv is conserved. Since the velocity vector doesn't change, its magnitude (speed) is also constant, meaning the kinetic energy K is conserved.
Differentiating velocity gives us acceleration:
With zero acceleration, the net force F is zero. A zero force field is trivially conservative, so the total energy E is conserved. Since both E and K are constant, the potential energy U must also be constant.
Finally, let's check angular momentum:
L=m(r×v)=m(αti^+βtj^)×(αi^+βj^)=0
The cross product of parallel vectors is zero, so L is constantly zero. Thus, for Path A, all quantities (p, q, r, s, t) are conserved.
Path B
The Elliptical Dance
Here, the position vector traces an ellipse:
The velocity is:
The velocity vector is clearly changing with time, so linear momentum p is not conserved. What about speed? The square of the speed is:
∣v∣2=ω2(α2sin2ωt+β2cos2ωt)
Because we are given that $\alpha
eq \beta$, this expression fluctuates over time. Therefore, kinetic energy K is not conserved.
Let's find the acceleration:
a=−αω2cosωti^−βω2sinωtj^=−ω2r
This is a profound result! The force F=−mω2r is a central force directed towards the origin. All central forces are conservative, so the total energy E is conserved. However, since K fluctuates, the potential energy U must also fluctuate to keep E constant.
What about angular momentum? Since the force is anti-parallel to the position vector r, the torque r×F is zero. We can verify this mathematically:
This is a constant vector! Thus, for Path B, only angular momentum and total energy (q, t) are conserved.
Path C
The Perfect Circle
This path is a special case of Path B where the semi-major and semi-minor axes are equal:
The velocity is:
The direction of velocity is constantly changing as the particle moves in a circle, so linear momentum p is not conserved. However, the speed is:
This is a constant! Therefore, kinetic energy K is conserved.
Just like in Path B, the acceleration is a=−ω2r, which means the force is central and conservative. Total energy E is conserved. Since both E and K are constant, the potential energy U must also be constant.
Angular momentum is also conserved for the exact same reason as Path B:
Thus, for Path C, angular momentum, kinetic energy, potential energy, and total energy (q, r, s, t) are conserved.
Path D
The Parabolic Arc
Finally, we have a parabolic trajectory:
The velocity is:
The velocity vector changes with time, so linear momentum p is not conserved. The speed squared is ∣v∣2=α2+β2t2, which grows with time. Thus, kinetic energy K is not conserved.
Differentiating velocity gives the acceleration:
The acceleration is a constant vector! A constant force field (like uniform gravity) is always conservative, meaning the total energy E is conserved. Since K is changing, U must also be changing.
Let's check angular momentum:
L=m(r×v)=m(αti^+2βt2j^)×(αi^+βtj^)=21mαβt2k^
The angular momentum depends on t2, so it is not conserved. Thus, for Path D, only total energy (t) is conserved.
The Grand Conclusion
By systematically applying the definitions of conservation laws, we have successfully decoded the physics of all four paths:
- Path A: p, q, r, s, t
- Path B: q, t
- Path C: q, r, s, t
- Path D: t
This perfectly matches option (a). This problem is a masterclass in understanding how mathematical trajectories dictate the physical realities of energy and momentum!