Fall 1997, TR 2:00-3:15pm, in G027
Professor Andrew J. S. Hamilton
JILA, room A706
This is an elective for graduate students. The course is taught every two years, and a tradition has developed that the emphasis of the course alternates between Galaxies one time, and Cosmology the next. This time the course will concentrate on COSMOLOGY. As regards the Astro Comps I exam, a consistent attempt has been made to choose questions accessible to either flavor of course.
We will deemphasize General Relativity, but we will not avoid it altogether. Some familiarity with GR may be useful. We will not cover the high energy particle physics which lies behind much of the work being done by physicists on inflation and the very early Universe.
I hope that, although the emphasis is on astrophysics, this course will also appeal to physics graduate students.
Astrophysical cosmology is a rapidly developing field, fuelled by ever improving observations of the Cosmic Microwave Background and of the distribution of galaxies in the Universe. In particular, notable advances are anticipated from the MAP (Microwave Anisotropy Probe) satellite planned for launch in Fall 2000, and from the SDSS (Sloan Digital Sky Survey) (for details see the Black Book) which plans to obtain 5 color photometry for 100 million stars, galaxies, and quasars, mostly in the North galactic hemisphere, and to obtain redshifts (spectra) for about 1 million galaxies and quasars. A prominent aim of the course is to provide the student with the background necessary to understand how these and related surveys will contribute to our understanding of the origin, evolution, and structure of the Universe at large. |
Topics
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Texts There are several recently published graduate level texts on Cosmology, and more are about to be published.
In addition the WWW is proving an ever growing, ever more useful up to date resource.
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Updated 09/24/97