Ph110B-15
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| == Welcome to Phys 110b, 2015! == | == Welcome to Phys 110B, 2015! == |
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| <<fl(W)>>elcome to the 2nd part of Classical Electrodynamics! The syllabus has been updated with the correct office hour information. However, there is no office hour today (Mar 31), as I have a dentist appointment.—~-''<<DateTime(2015-03-31T12:12:16-0700)>>''-~ |
* This course had been closed for a while now. Good luck, everyone!—~-''<<DateTime(2016-01-24T18:14:55-0700)>>''-~ |
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| <<h(<div style="margin-top: -1.0em; text-align: right;">)>>~-[[OldNews|Archived news items can be found here]].-~<<h(</div>)>> | |
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| <<fl(C)>>lassical electrodynamics is all about light. And, electrons and other charged particles... In this course, we will study the consequences of Maxwell's equations—something of a monument in the history of physics. We will learn conservation principles, waves, radiation, and end with the special relativistic view of light. | <<fl(C)>>lassical 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. |
Welcome to Phys 110B, 2015!
This course had been closed for a while now. Good luck, everyone!—6:14PM, Jan 24, 2016
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.