The syllabus for the mid-term exam has been posted under “Beskjeder” on the course pages.

There are some serious errors with the FYS1120 schedule on the course pages.

The following groups have been added as a mistake and will be removed:

• Øvelser Datalab – tir 0815-1000, tor 1815-2100
• Obligatorisk undervisning 3 – man 1215-1230
• Gruppe 3 – man 1815-2100

We’re sorry about the inconvenience.

This means that the following groups are the only ones that will be held:

• Gruppe 1 – tir 1215-1700
• Gruppe 2 – ons 1215-1700

In addition, we note that there is only one oblig in this course. The exact deadline for this oblig will be announced.

This is the last week before the exam, and as you can see from the schedule there will be no group sessions this week. If you need help, we encourage you to contact the group teachers or the lecturer directly.

Good luck with the final exam!

The solutions are meant as a guide on one way to think when solving different problems in electromagnetism, and they are not guaranteed to be clean of errors. When you stumble across an answer or a piece of logic you do not agree with it is most likely you who are correct.

You can help us in identifying errors in the solutions by posting on the weekly post.  This might even trigger a discussion which everyone will learn from and appreciate!

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The syllabus for the midterm exam is up to and including chapter 26, except section 26.4 and 26.5, which are about RC-circuits and power distribution systems.

Good luck!

Kinematics is all about motion. And since we are now moving away from pure electrostatics, it is about time to introduce some motion of particles.

In exercise set 6 we ask you to simulate the motion of a particle in an electric field using numeric methods. This is likely something you have seen before, so we’ll just briefly restate the most important concepts here.

Numerical integration

To determine the motion of any particle, we need to find the position as a function of time. This is usually done by observing that the double derivative of the position, namely the acceleration, can be integrated over time to give back the position. However, evaluating the integral

$$\mathbf r(t) = \int \int \mathbf a(t, \mathbf v(t), \mathbf r(t)) ~dt~dt$$

is no trivial task, except for the cases where $\mathbf a$ is constant. That’s why numerical integration is so useful when working with more complicated problems, especially when $\mathbf a$ is a function of $\mathbf r$ and $\mathbf v$.

In numerical integration, we divide the time into discrete steps, where we at each step recalculate the acceleration, velocity and position. One of the simplest of these schemes is the Euler-Cromer scheme.

In the Euler-Cromer scheme, we increase the current velocity by adding the acceleration at each time step. The acceleration is then a function of the current time, and the position and velocity at the previous time step.

$$\mathbf v(t_{i+1}) = \mathbf v(t_i) + \mathbf a(t_{i}, \mathbf r(t_i), \mathbf v(t_i)) \cdot \Delta t$$

Similarily, we find the position using the velocity we just calculated for the current time step:

$$\mathbf r(t_{i+1}) = \mathbf r(t_i) + \mathbf v(t_{i+1}) \cdot \Delta t$$

We have to do this from the first step in time till the last, and in terms of code this is translated into a for-loop. In Python we may express this as a small script:

from pylab import *

dt = 1e-3
t0 = 0
t1 = 10
t = linspace(t0, t1, (t1 - t0)/dt)

r1 = zeros((len(t),3))
v1 = zeros((len(t),3))

r1[0] = [0.0, 0.0, 0.0]
v1[0] = [0.0, 0.0, 0.0]

for i in range(len(t)-1): 
    a1 = array([5.0, 0.0, 0.0])
    v1[i+1] = v1[i] + a1*dt
    r1[i+1] = r1[i] + v1[i+1]*dt

figure()
plot(t, r1[:,0], label="Motion in x direction")
xlabel("$t$",fontsize=16)
ylabel("$x$",fontsize=16)
legend()
show()

To run this in an IPython terminal, just save it to file a file named “kinematics.py” and launch it by running the following commands in the folder where you saved the file:

ipython --pylab
run kinematics.py

Here we are using vectors, generated by linspace. The linspace function does in this case generate an array of 3-dimensional vectors, where the first argument, len(t), tells linspace that we want as many such vectors as there are time steps. The second argument, 3, tells linspace that each vector is three-dimensional.

The reason for using vectors (instead of 3 arrays of length len(t)) is that it makes it simple to write the following two statements in a way that is easy to read and remember:

r1[0] = [0.0, 0.0, 0.0]
v1[0] = [0.0, 0.0, 0.0]

This sets the first vectors of our position and velocity, also known as the initial conditions. In this case we have chosen the components of both to be $x = 0$, $y = 0$ and $z = 0$.

The for-loop is basically what we defined as the Euler-Cromer scheme above, with a constant acceleration vector in the $x$-direction:

for i in range(len(t)-1): 
    a1 = array([5.0, 0.0, 0.0])
    v1[i+1] = v1[i] + a1*1e-4
    r1[i+1] = r1[i] + v1[i+1]*dt

At each time step the position and velocity is not only calculated, but stored to an array that makes it readily available for plotting. The plotting is done for the first component of all $\mathbf r$-vectors as a function of t:

plot(t, r1[:,0], label="Motion in x direction")

A plot showing the $x$-component of the particle’s position as function of time $t$.

This results in a plot looking something like this:

For the case where we are working with a more physical problem, we would have to calculate the force $\mathbf F$ at each time step and find the acceleration from Newton’s second law, $\mathbf a = \frac{F}{m}$.

You should now be ready to play around with your own kinematic problems.

We have decided that the oblig can be done in any programming language you like, including Python and Matlab. This means that there will be no need for functions specific to Python or Mayavi to get the oblig approved, and that we will help you with both Matlab and Python during the group sessions.

Just note that if you choose any other language than Python or Matlab, you are a bit on your own when it comes to support. You will also have to make sure that your language of choice generates good-looking plots that meets all requirements such as legend, named axes, etc.

Note also that there is a numeric exercise in set number 6 that might be useful to have done before the oblig is published.

The oblig will be published shortly after the mid-term exam.

Last weekend Fysisk fagutvalg arranged the annual cabin trip, and in that regard Jørgen Midtbø held a lecture on Maxwell’s equations. Those of you who were there are already familiar with the content, but for the rest of you we post the note from this lecture that may be useful to read through. You can find the note here

• Maxwell’s equations 

Enjoy!