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In a region of space, a uniform magnetic...

In a region of space, a uniform magnetic field `B` is along positive x-axis. Electrons are ernit.u.d from the origin with speed `u` at different, angles. Show that the paraxial electrons are refocused on the x-axis at a distance `(2pimv)/(Be)`. Here, `m` is the mass of electron and e the charge on it.

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To solve the problem, we need to analyze the motion of electrons emitted from the origin in a uniform magnetic field directed along the positive x-axis. The goal is to show that paraxial electrons refocus on the x-axis at a distance of \( \frac{2\pi mv}{Be} \). ### Step-by-Step Solution: 1. **Understanding the Setup**: - We have a uniform magnetic field \( \mathbf{B} \) directed along the positive x-axis. - Electrons are emitted from the origin with speed \( u \) at different angles \( \theta \). 2. **Motion of Electrons in a Magnetic Field**: - When charged particles (like electrons) move in a magnetic field, they experience a magnetic force given by: \[ \mathbf{F} = q(\mathbf{v} \times \mathbf{B}) \] - Here, \( q \) is the charge of the electron, \( \mathbf{v} \) is the velocity vector of the electron, and \( \mathbf{B} \) is the magnetic field vector. 3. **Determining the Components of Velocity**: - The velocity \( \mathbf{u} \) can be decomposed into components: - \( u_x = u \cos \theta \) (along the x-axis) - \( u_y = u \sin \theta \) (along the y-axis) 4. **Radius of Circular Motion**: - The electrons will undergo circular motion in the plane perpendicular to the magnetic field. The radius \( r \) of this circular motion is given by: \[ r = \frac{mv}{eB} \] - Here, \( m \) is the mass of the electron, \( v \) is the speed of the electron, \( e \) is the charge of the electron, and \( B \) is the magnetic field strength. 5. **Time Period of Circular Motion**: - The time period \( T \) for one complete revolution is given by: \[ T = \frac{2\pi m}{eB} \] 6. **Distance Traveled in the x-direction**: - The distance traveled along the x-axis during one complete revolution can be calculated as: \[ \text{Distance} = \text{Velocity in x-direction} \times \text{Time Period} \] - The velocity in the x-direction is \( u \cos \theta \), so: \[ \text{Distance} = (u \cos \theta) \times T = (u \cos \theta) \times \frac{2\pi m}{eB} \] 7. **Focusing Condition for Paraxial Electrons**: - For paraxial electrons, we consider \( \theta \) to be very small (close to zero). Thus, \( \cos \theta \approx 1 \). - Therefore, the distance becomes: \[ \text{Distance} = u \times \frac{2\pi m}{eB} \] 8. **Final Distance for Paraxial Electrons**: - Since we are interested in the distance where the electrons refocus on the x-axis, we can set \( u = v \) (the speed of the electrons): \[ \text{Distance} = \frac{2\pi mv}{eB} \] Thus, we have shown that paraxial electrons are refocused on the x-axis at a distance \( \frac{2\pi mv}{eB} \).

To solve the problem, we need to analyze the motion of electrons emitted from the origin in a uniform magnetic field directed along the positive x-axis. The goal is to show that paraxial electrons refocus on the x-axis at a distance of \( \frac{2\pi mv}{Be} \). ### Step-by-Step Solution: 1. **Understanding the Setup**: - We have a uniform magnetic field \( \mathbf{B} \) directed along the positive x-axis. - Electrons are emitted from the origin with speed \( u \) at different angles \( \theta \). ...
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