PHYS 320: Mathematical Physics 
Seth MajorIn this course we will review, learn, and practice a number of mathematical tools which have practical use for physicists. The idea will be that these tools will be of use, not only in your remaining studies at Hamilton, but also in graduate school. A "pedestrian guide'' to the mathematics, the course focus on the implementation of the methods and applications rather than proofs and placing the results in context within mathematics. So, even if you have had a course in one or more of the topics, the emphasis and even some of the methods will be new. I also hope that you will master much of the material so that you can easily use in research, further studies, or elsewhere in life. The course is in lecture/discussion format punctuated by short presentations. I strongly encourage folks to ask questions and make observations. Much of the class time is spent making connections to physics. The course is somewhat unusual in that one first encounters new material in the reading and in a small number of problems. In class we focus on filling out understanding, answering questions, embellishing the material, and working through more examples. Course information (pdf):Questions, Problems and Reading (pdf):PS 1 (February 20)
PS 2 (March 13)
No daily questions due the Monday after break.
Some recent topics:
Handy links:The NIST Digital Library of Mathematical Functions. Referenced links:The 2015 Special Functions presentation list. Here's the Physics Today article by Michael Berry on Special Functions. Let me know if the link doesn't work for you. Reading (3.9 MB pdf) on SturmLiouville theory from Arfken and Weber. Reading on the Frobenious method from Arfken. An example of the method starts on page 395. The Bessely initial condition algebra for the "linearly lengthening pendulum". What do 3D parabolic coordinates look like? Reading on vector differentiation, particularly time dependent basis vectors (from Potter and Goldberg) Dirac Notation Primer (There is also a little bit on the notation in Boas, see page 181.) Power spectrum (CMBR) WMAP (5 yr results). The black body spectrum from COBE which helped win the 2006 Nobel Prize BBC news on the Earth's geoid. Here's a page with the expansion of the Earth's gravitational potential in terms of associated Legendre polynominals. Lovely Simulations of hydrogenic orbitals from falstad.com
Math Methods Poetry (pdf):

Last modified 13 March2015