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An electron is launched with velocity ve...

An electron is launched with velocity `vec v` in a uniform magnetic field `vec B.` The angle `theta` between `vec v and vec B` lies between 0 and `pi /2`. Its velocity vector `vec v` returns to its initial value in a time interval of

A

`(2pi m)/(eB)`

B

`(2xx2pi m)/(eB)`

C

`(pi m)/(eB)`

D

depends upon between `vec v and vec B`

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The correct Answer is:
To solve the problem, we need to determine the time interval after which the velocity vector of an electron, launched in a uniform magnetic field, returns to its initial value. ### Step-by-Step Solution: 1. **Understanding the Motion**: When an electron moves in a magnetic field, it experiences a magnetic force that acts perpendicular to its velocity. This causes the electron to move in a circular path. The angle θ between the velocity vector (v) and the magnetic field vector (B) is between 0 and π/2. 2. **Components of Velocity**: The velocity vector can be decomposed into two components: - The component parallel to the magnetic field: \( v \cos \theta \) - The component perpendicular to the magnetic field: \( v \sin \theta \) 3. **Magnetic Force**: The magnetic force acting on the electron due to the perpendicular component of its velocity is given by: \[ F = q(v \sin \theta)B \] where \( q \) is the charge of the electron (denoted as \( e \)). 4. **Centripetal Force**: This magnetic force provides the necessary centripetal force for circular motion: \[ F = \frac{mv^2}{r} \] where \( m \) is the mass of the electron and \( r \) is the radius of the circular path. 5. **Setting Forces Equal**: By equating the magnetic force to the centripetal force, we have: \[ e(v \sin \theta)B = \frac{mv^2}{r} \] 6. **Solving for Radius**: Rearranging the equation gives: \[ r = \frac{mv}{eB \sin \theta} \] 7. **Finding the Time Period**: The time period \( T \) for one complete revolution (the time after which the velocity vector returns to its initial value) is given by: \[ T = \frac{2\pi r}{v_{\text{perpendicular}}} \] where \( v_{\text{perpendicular}} = v \sin \theta \). Substituting the expression for \( r \): \[ T = \frac{2\pi \left(\frac{mv}{eB \sin \theta}\right)}{v \sin \theta} = \frac{2\pi m}{eB \sin \theta} \] 8. **Conclusion**: The time interval after which the velocity vector of the electron returns to its initial value is: \[ T = \frac{2\pi m}{eB \sin \theta} \]

To solve the problem, we need to determine the time interval after which the velocity vector of an electron, launched in a uniform magnetic field, returns to its initial value. ### Step-by-Step Solution: 1. **Understanding the Motion**: When an electron moves in a magnetic field, it experiences a magnetic force that acts perpendicular to its velocity. This causes the electron to move in a circular path. The angle θ between the velocity vector (v) and the magnetic field vector (B) is between 0 and π/2. 2. **Components of Velocity**: ...
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