Physics 162
Galaxies & Cosmology
H. E. Smith Spring 2005
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Physics 162 - Research Paper
Due: Thursday, May 26 |
As described in class, 40% of your grade in Physics 162 will be determined
by a Research Paper on a subject related to Galaxies & Cosmology. A
brief description of your intended project should be submitted by
Thursday, Apr 28. A 1 page description, neatly handwritten
is adequate. Please be as specific as possible about approach, references,
etc. Following is a list of possible topics that I believe are tractable
in terms of material available, proper scope, etc. This list is by no
means exhaustive and you need not be constrained by it, but remember the
following guidelines:
- The topic should be restricted so that you can treat it in some detail in
10 typed pages. It must have some direct tie in to the subject matter of
the course --- Galaxies and Cosmology --- but need not be a subject that we
cover in class.
- You must go deeper into any subject than class lectures.
(It is advisable here to check carefully into areas in cosmology, which
we will cover later in the course.)
- Check for yourself that there is adequate reference
material available, ranging from semi-popular to scientific journals.
- You must use as primary reference material at least one significant
paper in one of the astrophysics journals, many of which are available online.
These include:
Other places to look are
Astro-Ph - the LANL Astrophysics Preprint Database and the
Astrophysics Data
Service Abstract Database which may be searched by Author, Title, Text
with links to online papers and scanned versions for the past 20 years.
If you have questions please consult with Prof. Smith
Here's an index of recent
Scientific American articles online which is one way way to start
your search. See also our index of popular
Astronomy
Publications.
Your papers descriptions will be returned in about a week with comments about
approach, appropriateness of subject, and suggested references.
Potential Paper Topics
The Evolution of Stellar Populations in Galaxies
Chemical Evolution of Galaxies
Galaxy Collisions and Mergers
Star Formation in Galaxies
Black Holes in Galaxy Nuclei
Galaxy Formation
Production of the Light Elements (D,Li,B,Be) in the Big Bang
The Spectrum of the Microwave Background Radiation
Microwave Background Fluctuations
The Cosmic Background at X-ray, or UV, or Infrared
wavelengths.
The Star Formation History of the Universe
Tests of Cosmological Models - Choose one and discuss in detail
Large Scale Structure in the Universe: concentrate either on
Local Large Scale Structure or the Development of Structure in CDM
Cosmology
Gravitational Lenses
Gamma-Ray Bursts
Ph 162 Home
Gene Smith
Last
modified: Tues., 29 March 2005