This is an old revision of the document!
Radius of Circular Motion in a Magnetic Field
Suppose you have a moving charge q in a magnetic field →B=−Bˆz. The charge has a speed of →v=vˆx. What does the motion of the charge look like? What if the charge enters the field from a region with 0 magnetic field?
Facts
- There is a charge q.
- The charge has velocity vˆx.
- The charge is in a field →B=−Bˆz.
Lacking
- The motion of the charge.
- How the motion differs if the charge enter from outside the region where the field exists.
Approximations & Assumptions
- The field is constant.
- In the case where the particle comes from outside, the field is a step function – it goes immediately from 0 to B, and we can draw a boundary.
Representations
- We represent the magnetic force on a moving charge as
→F=q→v×→B
- We represent the two situations below.
Solution
Let's start with the first case, when the magnetic field exists all around the charge.
We can recall an earlier example where we had to find the force on a similar charge. One approach we took to find the direction of force was the Right Hand Rule. Remember that the force here will be →F=q→v×→B
So, the force on the charge is at first perpendicular to its motion. The trickiest part of finding magnetic force is the cross-product. You may remember from the math review that there are a couple ways to do the cross product. Below, we show how to use vector components, for which it's helpful to rewrite →v and →B with their components.
→v=⟨10,0,0⟩ m/s→B=⟨0,4⋅10−4,0⟩ T→v×→B=⟨vyBz−vzBy,vzBx−vxBz,vxBy−vyBx⟩=⟨0,0,4⋅10−3⟩ T⋅m/s
Alternatively, we could use the whole vectors and the angle between them. We find that we obtain the same result for the cross product. One would need to use the Right Hand Rule to find that the direction of the cross product is +ˆz. The magnitude is given by
|→v×→B|=|→v||→B|sinθ=(10 m/s)(4⋅10−4 T)sin90o=4⋅10−3 T⋅m/s
We get the same answer with both methods. Now, for the force calculation:
→FB=q→v×→B=1.5 mC ⋅4⋅10−3 T⋅m/s ˆz=6μN
Notice that the sin90o term evaluates to 1. This is the maximum value it can be, and we get this value because the velocity and the B-field are exactly perpendicular. Any other orientation would have yielded a weaker magnetic force. In fact, in the second case, when the velocity is parallel to the magnetic field, the cross product evaluates to 0. See below for the calculations.
→v=⟨0,−10,0⟩ m/s→B=⟨0,4⋅10−4,0⟩ T→v×→B=⟨vyBz−vzBy,vzBx−vxBz,vxBy−vyBx⟩=⟨0,0,0⟩
Or, with whole vectors:
|→v×→B|=|→v||→B|sinθ=(10 m/s)(4⋅10−4 T)sin0=0
When the velocity is parallel to the magnetic field, →FB=0.