Lorentz force - particle in an odd magnetic field

In summary, the magnetic flux density in the quadrupole lens affects the path of the particles. Without the effect of the magnetic flux density, the particles would follow a straight path. However, with the effect of the magnetic flux density, the particles’ paths are affected and they must solve three differential equations in order to determine their coordinates at any given time.
  • #1
Toby_phys
26
0

Homework Statement


Particles of mass ##m## and charge ##q## are initially traveling in a beam along the ##z## direction with speed ##v## when they enter a long magnetic quadrupole lens, where there is no E-field and the magnetic flux density is ##B = Ay\hat{i} + Ax\hat{j}##, and where A is a positive constant. Neglecting edge effects of the magnet, write down the equations of motion for one of the particles. Solve these equations under the assumption that the particle’s path always makes a small angle with the ##z##-direction, and that the particle had ##x = x_0## and ##y = y_0## before entering the magnetic field.

Homework Equations


We have the Lorentz force in the absence of any electric fields:

$$
\mathbf{F}=q\mathbf{v\times B}
$$

We have Newtons 2nd law:

$$\mathbf{F}=m\mathbf{a}$$

The Attempt at a Solution


Equating the Lorentz force with Newtons second law:

$$
\begin{align}
m\mathbf{a} &= \begin{bmatrix}
V_x \\
V_y \\
V_z
\end{bmatrix}
\times
\begin{bmatrix}
Ay \\
Ax \\
0
\end{bmatrix}&=\begin{bmatrix}
-AxV_z \\
AyV_z \\
AxV_x-AyV_y
\end{bmatrix}
\end{align}
$$

Which gets us 3 differential equations:
$$ m \ddot{x}=-Ax\dot{z}$$
$$m \ddot{y}=Ay\dot{z} $$
$$m \ddot{z}=Ax\dot{x}-Ay\dot{y} $$I couldn't see how to progress from here. Any help would be appreciated. thank you.
 
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  • #2
I think the key to solving this is here
Toby_phys said:
... under the assumption that the particle’s path always makes a small angle with the z-direction,
In the first two equations you can approximate ##\dot{z} \approx v_0##. In this approximation you have two decoupled differential equations which you can easily solve for ##x(t)## and ##y(t)##. Put these back in the third equation which will take the form ##m\ddot{z}=f(t)##.

Edited for language clarifications.
 
Last edited:

1. What is the Lorentz force?

The Lorentz force is the force experienced by a charged particle moving in an electric and magnetic field. It is given by the equation F = q(E + v x B), where q is the charge of the particle, E is the electric field, v is the velocity of the particle, and B is the magnetic field.

2. How does the Lorentz force affect a particle in an odd magnetic field?

In an odd magnetic field, the direction of the magnetic field changes in space or time. This causes the particle to experience a force that is not constant in magnitude or direction, resulting in a complex motion. This can lead to the particle following a curved or spiral-like path instead of a straight line.

3. What is an example of an odd magnetic field?

An example of an odd magnetic field is a magnetic field that changes rapidly in time, such as a rotating or oscillating magnetic field. Another example is a magnetic field that varies in space, such as a non-uniform magnetic field.

4. Can the Lorentz force be used to manipulate particles?

Yes, the Lorentz force can be used to manipulate the motion of charged particles. This is the principle behind devices such as particle accelerators and mass spectrometers. By controlling the strength and direction of the electric and magnetic fields, scientists can manipulate the path of particles and study their properties.

5. How does the Lorentz force impact the behavior of particles in a magnetic field?

The Lorentz force causes charged particles to move in a circular or helical path in a uniform magnetic field. In a non-uniform magnetic field, the particle may also experience a force perpendicular to its velocity, causing it to accelerate or decelerate. The Lorentz force also plays a crucial role in the interactions between particles, such as in the formation of plasma and the behavior of cosmic rays.

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