Samsara |
Astronomy 323: Cosmology
|
Make-up of Universe from WMAP Observation of CMBR
|
Astronomy 323: Cosmology
is an intermediate course on the structure and evolution of the Universe.
The past 20 years has seen an explosion in our understanding of the contents,
formation, and evolution of our Universe and universes in general.
Changes in our understanding of fundamental physics, combined with
discoveries from space and ground-based telescopes, have led to a radically
different model of our Universe and our place in the Universe.
Cosmology is the meeting point of observational astronomy,
mathematics, and particle physics. More so than in the past,
cosmology directly engages nature
with foundations based in observation and experience. The
goals of this course are to: (1) gain an understanding of basic
mathematics that underlies cosmologywith ;
(2) understand the properties of the objects that make up our Universe,
(3) formulate a coherent philosophy for interpreting the observational
evidence of the hot Big Bang and relating this worldview to new areas
of research.
The interplay between
technology (telescopes, space observatories) and knowledge gained about
the Universe is a key theme to the course. Prerequisites, Physics 253,
and Math 253. Suggested Corequisites: Physics 351, Math 256 (familiarity
with one-dimensional ordinary differential equations).
Instructor: James N. Imamura
Office: 444 Willamette Hall
E-mail: imamura@uoregon.edu
Phone: 541-346-5212
Office Hours:
Course: ASTR 323, Cosmology
Course CRN: 26976
Text: B. Ryden, Introduction to Cosmology
Class: 14:00-15:50, MW
Room: 147 Willamette Hall
|
Grades and Points:
Your grade will be based on the cumulative number of points earned over the
quarter, there will be two (2) in-term exams, six (6) homework
assignments, and a
Final Examination
Test 1 = 60 points
Test 2 = 60 points
Homework/In-class exercises = 10 points per
exercise ===> 60 total points
Final Examination =
80 points
Total points = 60+60+60+80 = 260 points
The grading scale for each exam may slide as driven by
the class performance.
Tests:
Test 1: February 7, Wednesday
Test 2: March 7, Wednesday
Final Examination: March 19, Monday, 14:45
Week | Material
| Reading |
Date |
Notes |
Homework |
1 |
Introduction |
Chap 2: Olbers' Paradox,
Hubble's Law, Cosmic Microwave Background, Make-up of the
Universe |
2018.1.8,2018.1.10 | |
|
2 |
Newton, Einstein, Space-time, and Friedmann equations |
Chap 3: Newton versus Einstein, Chap 4: Cosmic Dynamics
| 2018.1.10,2018.1.17
|
|
|
3,4,5 |
World Views of the Universe |
Chap 5: Single-Component Universes, and Multiple-Component
Universes
| 2018.1.22-2018.2.5
|
|
|
6 |
Fate of the Universe |
Chap 6: Measuring Cosmological Parameters
|
2018.2.12,2018.2.14 |
|
|
7,8 |
Fate of the Universe |
Chap 6: Measuring Cosmological Parameters, Chap 7: Dark Matter
|
2018.2.19,2018.2.26 |
|
|
8-10 |
History of the Universe |
Chap 8: The Cosmic Microwave Bckground,
Chap 9: Nucleosynthesis & the Early Universe,
Chap 10: Inflation & the Early Universe,
Chap 11: The Formation of Structure
| 2018.2.26-
|
|
HW 6--due: |