Fundamentally, a plasma is an *N*-body system of mobile charged
particles and electromagnetic fields. The basic equations that describe the
system classically are the Lorentz-force equation and the (microscopic)
Maxwell equations. Unfortunately, for a macroscopic amount of plasma, a
complete global simulation of such a large *N*-body system by direct
integration of the Maxwell-Lorentz equations is impractical, even with the
most powerful computers, and even if we could solve the system exactly we
would have far more information than we would typically require. For these
reasons a variety of statistical models of plasma dynamics have been
developed.

Statistical models range from kinetic models which contain essentially all the relevant physical phenomena, but are still largely unsolvable (except for simple geometries and/or relatively small systems and short times), to fluid models which selectively remove small-scale physics, but are more tractable and yield very useful large-scale solutions. Hybrid kinetic-fluid plasma models are a useful and popular alternative for some applications. Methods to obtain and solve the best plasma model for a given situation are often at the forefront of current plasma physics research. These methods require a thorough understanding of the basic equations of plasma physics and the physical content of those equations.

In this course we will begin from first principles with the fundamental microscopic equations and then systematically derive the major equations in current use in plasma physics research. This approach is in contrast to most introductory plasma physics courses (including some taught by the instructor of this course), in which various approximate plasma models are presented with a minimal discussion of their theoretical foundations and in which the overall logical structure of theoretical plasma physics is often obscured. While this introductory treatment is arguably the best way to economically present the main physics while avoiding too much mathematics, a more systematic and mathematically-sophisticated approach is appropriate for a more advanced course such as this. The physical content of the main equations will be discussed in terms of general properties of the equations and in terms of waves and instabilities for a given plasma model.

We will consider the main plasma kinetic equations (Klimontovich, Liouville, BBGKY, Balescu-Lenard, Fokker-Planck, and Vlasov), the Vlasov theory of waves and instabilities (including a detailed treatment of Landau damping), and connections to fluid plasma models. We may also include other topics of special interest, such as an introduction to gyrokinetic theory or to phase-space Lagrangian guiding center theory, as time allows.

**Preface**- Objectives of this course
- Reference list
- Electromagnetic units

- Introduction
- Definition of a plasma
- Classical, ideal plasmas
- Classification of plasmas
- An overview of theoretical plasma physics

- Foundations of Plasma Kinetic Theory
- The Klimontovich formulation
- The plasma kinetic equation
- Ensemble averages and measurements
- The Liouville equation
- An elementary treatment of collisions

- The BBGKY Hierarchy
- Derivation of the BBGKY hierarchy
- The
*k=1*BBGKY equation - The Vlasov equation from BBGKY
- Equations for the phase-space density and pair-correlation function

- The Balescu-Lenard Equation
- Introduction
- The Bogoliubov hierarchy of time scales
- Fourier and Laplace transforms
- The Balescu-Lenard collision term

- Connections to Fluid Models
- Introduction and review of the ideal MHD equations
- The starting equations
- Two-fluid equations
- Low-frequency, long-wavelength assumptions
- Single-fluid equations
- The ideal MHD limit
- Validity of the ideal MHD model
- MHD and guiding center currents

- Basic Equations for Linear Waves in Plasmas
- The dielectric tensor, wave equation, and general dispersion relation
- Dispersion relations for weak damping or growth
- A simple example: waves in a cold unmagnetized plasma

**Linear Waves in Vlasov Plasmas**- The dielectric tensor for unmagnetized Vlasov plasma
- Landau's initial-value calculation and Landau damping
- The dielectric function and the electrostatic dispersion relation
- Electrostatic waves in unmagnetized Vlasov plasma
- Electromagnetric waves in unmagnetized Vlasov plasma
- Waves in magnetized Vlasov plasma

**Course Prerequisites:** There are no formal prerequisites, but
experience in
PHYS 480 Introduction to Plasma Physics,
PHYS 515 Classical Mechanics,
and PHYS 532 Classical Electrodynamics, or equivalent courses, is helpful.

**Credit:** 3 semester hours

**Course Web Page:** http://aachan.web.rice.edu/phys519

**Format:** A lecture course with problem sets, a midterm exam,
a class presentation, and a final exam.

** Textbooks: ** There are no required textbooks. A reference list will be
distributed and discussed in class.

** Course Instructor: **

**Office Hours:**
I am available at most times during the week, but you should email or
telephone first to confirm that I will be in the office.

*
Any student with a disability requiring accommodations in this course is
encouraged to contact me after class or during office hours.
Additionally, students should contact Rice Disability Support
Services.
*

I plan to assign a homework set about every week and a half, usually due within one week of assignment. Homework sets will be distributed in class and they will also be available from the course web page.

**Homework Policy:**
Students are encouraged to discuss the problems with their classmates and
with the instructor, but they must write up their homework solutions
*independently*. Of course, you must not look at homework solutions from
previous years.

**Late Policy:**
The grade for late homework will be multiplied by a decaying
exponential with a time constant of five days. Late homework must be given
directly to the grader, with the date and time written on the front page.

Grading Weights: | Homework: | 50% |
---|---|---|

Midterm Exam: | 15% | |

Class Presentation: | 10% | |

Final Exam: | 25% |

**Class Presentation:** A presentation on some aspect of basic plasma
physics relevant to topics covered in this class. To be given near the end of
the semester, on a topic chosen by the student and approved by the
instructor.

**Auditors:** To receive a passing grade auditors must attend more
than half of the lectures and give one class presentation. Auditors are
encouraged, but not required, to do the homework sets.