Condensed matter theory is an enormous, rich, evolving field which is impossible for a single professor to explain or even describe in a single graduate course. In order to help our students navigate this varied terrain, Cornell's condensed-matter theory group has developed Basic Training in Condensed-Matter Theory, a challenging, modular course taught once per year by a rotation of four condensed-matter theorists. Students are exposed to a different set of active research areas each year, and learn sophisticated analytical and numerical methods in the extensive exercises. This year our course replaces the traditional many-body physics course 654, and will incorporate some of the tools and concepts from that field. Tentatively, we plan to cover
Jan 21 - Feb 13 | James Sethna (sethna@lassp.cornell.edu, Clark 528) | Continuum Theories of Crystal Defects | Grader: Yong Chen (yc355@cornell.edu) |
Feb 18 - Mar 13 | Erich Mueller (em256@cornell.edu, Clark 514a) | Probes of Cold Atoms | Grader: Stefan Natu (ssn8@cornell.edu) |
Mar 25 - April 10 | Craig Fennie (fennie@cornell.edu, Clark 226) | Competing Ferroic orders: the magnetoelectric effect | Grader: Johannes Lischner (jl597@cornell.edu) |
April 15 - May 1 | Eun-Ah Kim (eun-ah.kim@cornell.edu, Clark 507) | Quantum Criticality | Grader: Kaden Hazzard (kh279@cornell.edu) |
For more information, please contact any of the instructors.
Teaser 1: | Due Wednesday April 15 | Teaser 1 |
Syllabus | Wednesday April 15 | Syllabus |
Syllabus | Wednesday April 15 | Lecture 1 |
Homework 1: | Due May 1, 2009 | Homework 1 |
Teaser 1: | Due Friday April 3 | Teaser 1 | Solutions |
March 25 | Lecture 1 |
April 1 | Lecture 2 |
April 3 | Lecture 3 |
April 8 | Lecture 4 |
April 10 | Lecture 5 |
Teaser 1: | Due Wednesday Feb 18 | teaser1.pdf |
Teaser 2: | Due Friday Feb 20 | teaser2.pdf |
Teaser 3: | Due Wednesday Feb 25 | teaser3.pdf |
Teaser 4: | Due Friday Feb 27 | teaser4.pdf |
Teaser 4: | Due Friday Mar 3, 2009 | teaser5.pdf |
image.dat |
Lecture 1: | Wednesday Feb 18 | OpticalAbs.pdf |
Lecture 2: | Wednesday Feb 20 | CollectiveModes.pdf |
Lecture 4: | Wednesday Feb 25 | Helium.pdf |
Jan 21, 2009 |
Q: Why do continuum theories work? A: Because we are interested in slow long length-scale properties. Q: What are the relevant continuum fields for any system?A: Conserved quantities (density, energy density, momentum density) and broken symmetries (magnetism, superconducting order,...). teaser: Why can't we run faster than the speed of sound |
Jan 22, 2009 |
Q: Why are we so weak?
A: dislocations. Q: Why are we so strong?A: composite materials. Discussion of how to generate most general continuum free energy consistent with symmetries. Example (multiferroics). Discussion of boundary terms. Teaser: Boundary terms can stabilize defects. |