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Neutral Particle A neutral particle is at rest in a uniform magnetic field \(\vec{B}\). At time \(t=0\) it decays into two charged particles, each of mass \(m\). (a) If the charge of one of the particles is \(+q\), what is the charge of the other? (b) The two particles move off in separate paths, both of which lie in the plane perpendicular to \(\vec{B}\). At a later time the particles collide. Express the time from decay until collision in terms of \(m,|\vec{B}|\), and \(|q|\)

Short Answer

Expert verified
The charge of the other particle is \(-q\). The time from decay until collision is \(\frac{\pi m}{|q| B}\).

Step by step solution

01

Understanding the Charge Conservation

The initial neutral particle has no net charge. According to the law of charge conservation, the total charge must remain zero after the decay. Since one of the decay particles has a charge of +q, the other must have a charge of -q to keep the total charge zero.
02

Analyzing the Motion of Charged Particles

Since the magnetic field, \(\textbf{B}\), is uniform and the particles are moving perpendicularly to \(\textbf{B}\), each particle will travel in a circular path. Let's denote the radius of the circular path as \(r\). The centripetal force for a charged particle in a magnetic field is given by: \[ r = \frac{mv}{|q|B} \] where \(v\) is the velocity of the particle, \(m\) is its mass, and \(q\) is its charge.
03

Time Period of Circular Motion

The time period \(T\) for one full revolution of a charged particle in a magnetic field is: \[ T = \frac{2 \pi r}{v} \] Using the expression for \(r\) from Step 2, we get: \[ T = \frac{2 \pi }{|q|B} \times \frac{mv}{v} = \frac{2 \pi m}{|q|B} \] Thus, the time period \(T\) is \(\frac{2 \pi m}{|q| B}\).
04

Collision Time Calculation

Since the particles start from the same point, they will collide when each has completed exactly half a revolution in opposite directions. This means they will collide at half the time period. Therefore, the collision time \(t_{collision}\) is half of \(T\): \[ t_{collision} = \frac{T}{2} = \frac{2 \pi m}{|q| B} \times \frac{1}{2} = \frac{\pi m}{|q| B} \]

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Charge Conservation
The law of charge conservation is crucial in understanding the behavior of charged particles in any physical process. When a neutral particle decays, the total charge before and after the event must remain the same. In the given exercise, the initial neutral particle has no net charge.

According to charge conservation, if one of the resultant particles from the decay carries a charge of \(+q\), the other must carry a charge of \-q\ to ensure the total charge remains zero. This principle guarantees that the net charge doesn't change, maintaining equilibrium in the system.

Think of charge conservation like balancing a see-saw: if you add a weight on one side, you must add an equal weight on the other to keep it balanced.
Circular Motion
When charged particles move in a uniform magnetic field, they experience a force perpendicular to both their velocity and the magnetic field. This force makes them travel in circular paths. For a particle of mass \(m\) and charge \(q\), moving with velocity \(v\) perpendicular to the magnetic field \(B\), the centripetal force is provided by the magnetic force, given by:

\[ r = \frac{mv}{|q|B} \]

This radius \(r\) represents the distance from the center of the circular path to the moving particle. The key insight here is that the magnetic force is always perpendicular to the velocity of the particle, causing it to move in a circular trajectory.

Imagine it like swinging a ball on a string in a circle; the tension in the string (analogous to the magnetic force) pulls the ball inward, keeping it in its circular path.
Collision Time Calculation
Understanding the time it takes for the particles to collide is essential. Both particles move in circles due to the magnetic field, and their time period \(T\) for one complete revolution is:

\[ T = \frac{2 \pi m}{|q|B} \]

This formula tells us how long it takes a charged particle to go around its circular path once. For the particles to collide, each must travel half a revolution from their starting points in opposite directions. Thus, the collision time \((t_{collision})\) will be exactly half of the time period:

\[ t_{collision} = \frac{T}{2} = \frac{2 \pi m}{|q|B} \times \frac{1}{2} = \frac{\pi m}{|q| B} \]

Think of it like two runners starting at the same point on a circular track but running in opposite directions; they will meet halfway around the circle, meaning it takes them half the total revolution time to collide.

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Most popular questions from this chapter

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