Ph110B-15
| Differences between revisions 50 and 58 (spanning 8 versions) | Back to page |
|
Size: 1306
Comment:
|
Size: 1056
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 5: | Line 5: |
| * The final exam is [[Homework+|here]]. Good luck!—~-''<<DateTime(2015-06-05T10:02:14-0700)>>''-~ * In today's class, the discussion on $\delta S$ when it is related to the end point variations of $\delta t$ and $\delta \vec r$ did not go so well. I apologize. That is an important topic, although it may be optional for this level. Here is a [[Lecture+#Note|cleaned up and clarified version of that discussion]]!—~-''<<DateTime(2015-06-02T12:39:12-0700)>>''-~ |
* [[Homework+#final|The solutions to the final]] had been posted. Any extra credit materials should be submitted by the end of today (~ 5 PM; either in my mailbox or by email).—~-''<<DateTime(2015-06-12T11:41:04-0700)>>''-~ |
Welcome to Phys 110B, 2015!
The solutions to the final had been posted. Any extra credit materials should be submitted by the end of today (~ 5 PM; either in my mailbox or by email).—11:41AM, Jun 12, 2015
What is this course about?
Classical electrodynamics is all about the light. And electrons and other charged particles... In this course, we will start with Maxwell's equations—something of a monument in the history of physics—and study some conclusions that we can draw from them. By doing so, we will learn about the light, or the electronmagnetic field, and its interaction with charged particles within the realm of “classical” physics. We will learn conservation principles, waves, radiation, and end with the special relativistic view of light.