HIGH ENERGY ASTROPHYSICS

Name: HIGH ENERGY ASTROPHYSICS
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Rating: 4.4 (158 reviews)

PHYSICS 772

과목 설명

Interactions among the particles, fields, and radiation of interstellar and intergalactic space. Gamma-ray, x-ray, and cosmic ray production, propagation, and detection. Knowledge of electrodynamics (such asPHYSICS 322) strongly encouraged.

선수과목

Graduate/professional standing

충족 요건

This course does not satisfy any prerequisites.

학점

미보고

개설 시기

미보고

평점

3.67

4.76% 과거 데이터 대비

수료율

100%

1.94% 과거 데이터 대비

A 비율

41.67%

15.5% 과거 데이터 대비

학급 규모

-31.65% 과거 데이터 대비

Cumulative Grade Distribution

강사 (2026 Summr)

다음 사이트의 평점순으로 정렬 Rate My Professors

유사 과목

THE INTERSTELLAR MEDIUM I: BASIC PROCESSES

ASTRON 720

Observational techniques for interstellar medium studies, overview of the role of interstellar gas in galaxies, dynamics, energetics, major theories of structure and evolution, introduction to star formations and supernova remnant evolution.

EXPERIMENTAL METHODS IN NUCLEAR-, PARTICLE-, AND ASTROPHYSICS

PHYSICS 736

Interaction of particles with matter; detector techniques at colliding beam machines, in nuclear and particle physics, astrophysics, and cosmology; experimental strategies in detector design; principles of simulation and Monte Carlo methods, error analysis and statistical techniques in data analysis. Knowledge of introductory particle physics (such asPHYSICS 535) strongly encouraged.

SEMINAR IN ASTROPHYSICS

ASTRON/PHYSICS 910

Current topics in astrophysics.

THE PHYSICAL UNIVERSE

ASTRON 200

Modern astrophysics involves applying physical principles to understand astronomical phenomena. Includes the solar system, stars, nebulae, galaxies, and cosmology, with emphasis on origins and evolution. Some nighttime observation with telescopes required.

BASIC ASTROPHYSICS II

ASTRON 702

Basic particle and fluid dynamics of stellar and gaseous systems in astrophysics. Review of gravitational dynamics, 2-body relaxation, phase space, basic equations of fluid dynamics, waves, shocks, winds accretion, instabilities.