PHYS 234: HIGH ENERY ASTRO

University of California, Santa Barbara

Accretion power in a range of astrophysical contexts, from quasars to galactic black holes. Rapid release of thermonuclear energy, Type I X-ray bursts, classical novae, Type Ia supernovae. Relativistic jets from black holes, non-thermal radiation processes, physics of gamma-ray bursts.

Average GPA: 3.61

Grade distribution records: 89 students across 7 terms.

Grade distribution

GradeStudentsPercent
A+1516.9%
A2932.6%
A-1921.3%
B+1112.4%
B1112.4%
C+11.1%
F22.2%
S11.1%

Based on 89 student grade records across 7 terms and 3 professors.

Instructors

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