LEVELJEE Advanced
Visualized Solution
The Sigma Insight: Motion of a Charge in Magnetic Fields
The journey of a charged particle through a magnetic field is one of the most elegant dances in physics. It is a perfect interplay between linear momentum and a perpendicular force, resulting in a flawless circular trajectory. Let's dive deep into this problem and uncover the beautiful geometry hidden within!
The Physics of the Dance
When a charged particle enters a uniform magnetic field, it experiences a magnetic force given by the Lorentz force law:
Because this force is always perpendicular to the velocity vector, it does no work on the particle. The kinetic energy and speed remain absolutely constant. Instead of speeding up or slowing down, the particle is constantly pulled sideways, forcing it into a circular path. The magnetic force acts as the centripetal force:
From this, we can easily find the radius of the circular path:
Let's substitute the given values into our master equation:
This radius is the key to unlocking the rest of the problem. No matter which way the magnetic field points, the particle will always travel along a circle of radius .
Case (a)
The Inward Magnetic Field
Imagine the magnetic field pointing directly into the page. As the positively charged particle enters at point with a velocity angled at to the boundary, the right-hand rule tells us that the magnetic force will push it upwards and to the left.
The particle will curve into the magnetic field region, trace out an arc, and eventually exit at point . But how much of the circle does it trace?
If we draw perpendiculars from the velocity vectors at and , they intersect at the center of the circle, . Because the entry angle is , the geometry forms a perfect right isosceles triangle between the center and the boundary. The angle subtended by the arc at the center is exactly .
This means the particle completes exactly th of a full circle!
Because of the beautiful symmetry of the circle, the particle must exit at the exact same angle it entered. Therefore, the exit angle is simply:
To find the distance between the entry and exit points, , we can use the geometry of our right isosceles triangle. The distance is the base of the triangle formed by the center and the two points on the boundary:
Case (b)
The Outward Magnetic Field
Now, let's flip the script. What happens if the magnetic field points out of the page?
The velocity is the same, but the magnetic field is reversed. According to the right-hand rule, the magnetic force also reverses direction! Instead of being pushed to the left, the particle is now pushed to the right, deeper into the magnetic field region.
It will still travel in a circle of radius , but its journey will be much longer. It will curve to the right, complete a large loop, and finally strike the boundary again.
How much of the circle does it complete this time? Since the arc from Case (a) is now the only part of the circle that lies outside the magnetic field, the particle must travel through the remaining portion of the circle.
An angle of corresponds to exactly th of a full circle!
To find the time spent in the magnetic field, we first need the time period for a full circle:
Since the particle only completes th of the circle, the time spent is:
Let's plug in our values and bring it home:
And there we have it! By simply understanding the geometry of circular motion and the right-hand rule, we've completely unraveled the particle's journey.
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