Syllabus
Course Objectives
We will cover the exciting phenomena happening
at the end of a star's life: supernova explosions and gamma-ray
bursts, and the formation and properties of compact remnants (white dwarfs,
neutron stars, and black holes). This will lead us to topics at the
current frontier of astrophysics. You will learn to look at the physics
behind these cutting-edge phenomena, and make things as simple as possible,
but still capture the important effects.
Texts
All texts will be placed on reserve in the PMA (RLM 4th floor)
and Astronomy Peridier (RLM 15.202) libraries.
The required text is (available at the Co-op):
Rosswog/Brueggen (RB), Introduction to High-Energy Astrophysics, Cambridge University Press
In addition, this text is highly recommended:
A.C. Phillips (ACP), The Physics of Stars (2nd edition), Wiley
Grading
Your final grade will be based on a point system:
Class Participation
10
2 In-class Exams
2x20
Homework
40
Numerical Project
10
We won't have a Final Exam.
The following grading scheme will be used:
A
=
85-100 B
=
70-84 C
=
60-69 D
=
50-59
Any score below 50 is failing.
Class Participation
10% of your grade will be based on your
class participation. You will participate by solving in-class puzzles.
Class Attendance
It is important that you come to class. You will not be successful
otherwise in following the course material. In addition, we will
have unannounced quizzes. If you miss one, there will be no make-up quiz.
Policies
There will be make-up exams ONLY for students with valid
excuses. Scholastic dishonesty, in particular any plagiarism, will be prosecuted in accordance with the university
guidelines.
