The Cosmic Billiards
A Collision in Free Space
Imagine two celestial bodies, or perhaps just two simple billiard balls, gliding towards each other in the vast emptiness of free space. There is no gravity pulling them down, no friction slowing them down, and absolutely no external forces interfering with their cosmic dance.
The first ball carries a momentum of p1=pi^, moving steadily along the positive x-axis. The second ball mirrors this exactly, carrying a momentum of p2=−pi^, moving along the negative x-axis.
What happens when we look at the system as a whole? The total initial momentum is simply the vector sum of the two:
Pinitial=p1+p2=pi^−pi^=0
The Master Key
Conservation of Momentum
Because our system exists in free space, isolated from the rest of the universe, it obeys one of the most sacred laws of physics: the Conservation of Linear Momentum. This law dictates that if no net external force acts on a system, its total momentum must remain constant forever.
Therefore, no matter how chaotic or explosive the collision between these two balls might be, the total momentum after the collision must still be exactly zero. If we denote their final momenta as p1′ and p2′, we arrive at our master equation:
The Anatomy of a Zero Vector
For a three-dimensional vector to be truly zero, it is not enough for just one part of it to vanish. A vector is composed of independent directions: the x-direction (i^), the y-direction (j^), and the z-direction (k^).
If the total final momentum is zero, it means that the sum of the i^ components must be zero, the sum of the j^ components must be zero, and the sum of the k^ components must be zero. They cannot compensate for each other. A movement in the x-direction cannot cancel out a movement in the y-direction.
With this strict mathematical filter, let's interrogate the given options to see which final states are physically allowed, keeping in mind the crucial constraint: all constants (p,a1,a2,b1,b2,c1,c2) are strictly non-zero.
Interrogating the Options
Option (a): The Lone k-cap
Let's add the final momenta given in option (a):
p1′+p2′=(a1+a2)i^+(b1+b2)j^+c1k^
Look closely at the k^ component. It is simply c1. For this entire vector to be zero, we are forced to conclude that c1=0. However, the problem explicitly forbids any of these constants from being zero! Because this state requires a zero constant to exist, it violates our constraints. Thus, option (a) is not allowed.
Option (b): The Perfect Counterbalance
Now, let's look at option (b):
For this to be zero, we need c1+c2=0, which means c1=−c2. Can two non-zero numbers add up to zero? Absolutely! If c1=5 and c2=−5, the condition is perfectly met without violating the non-zero rule. Therefore, this state is physically allowed.
Option (c): The Symmetrical Dance
Adding the vectors in option (c) yields:
p1′+p2′=(a1+a2)i^+(b1+b2)j^+(c1−c1)k^
The k^ component beautifully cancels itself out immediately. We are left needing a1=−a2 and b1=−b2. Just like in option (b), we can easily find non-zero numbers that satisfy these equations. This state is perfectly allowed.
Option (d): The Double Trouble
Finally, let's examine option (d):
p1′+p2′=(a1+a2)i^+(b1+b1)j^=(a1+a2)i^+2b1j^
Focus on the j^ component: 2b1. For the total momentum to be zero, we must have 2b1=0, which inescapably means b1=0. Once again, we hit a brick wall. The problem states b1 must be non-zero. Because this state forces b1 to be zero, it is physically impossible under the given constraints. Thus, option (d) is not allowed.
The Final Verdict
The question cleverly asks us to identify the options that are not allowed. Through our rigorous application of momentum conservation and vector independence, we discovered that options (a) and (d) force our non-zero constants to become zero. Therefore, they represent impossible physical realities and are the correct answers to this problem.