Cosmology W13 - Physics Department, UCSB
Cosmology W13 - Physics Department, UCSB Cosmology W13 - Physics Department, UCSB
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27.09.2014
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Physics 236 • Grading: – Class par^cipa^on 10% – Homework 20% – Midterm Exam 20% – Final Exam 20% – Presenta^ons 20% – Par^cipa^ons to your colleagues’ presenta^ons 10% • Homework: – assigned on wednesday, due the following Monday – Graded by pairs of students (sign up!)
Physics 236: the big ques^on
- Page 1 and 2: Lecture 1: January 9 2013 Cosm
- Page 3: Physics 236 • Textbook: - Gala
- Page 7 and 8: Physics 236: more specifically
- Page 9 and 10: Tradi^onal Observa^onal Founda^on
- Page 11 and 12: Physics 236: open problems with
- Page 13 and 14: Cosmological Principle • Physic
- Page 15 and 16: Some useful concepts/units • P
- Page 17 and 18: Olbers’ paradox. The night sky
- Page 19 and 20: Olbers’ paradox. What does the sk
- Page 21 and 22: Olbers’ paradox. The Big-Bang sol
- Page 23 and 24: Cosmic Microwave Background
- Page 25 and 26: Cosmic Microwave Background
- Page 27 and 28: Anisotropies of the CMB BenneZ
- Page 29 and 30: Basic Phenomenology: LSS
- Page 31 and 32: Basic Phenomenology: galaxies
- Page 33 and 34: Basic Phenomenology: galaxies
- Page 35 and 36: Spiral galaxies • Like our ve
- Page 37 and 38: Luminosity func^on
- Page 39 and 40: Stellar mass func^on What about
- Page 41 and 42: Examples of cluster in the op^
- Page 43 and 44: Examples of cluster in the X-
- Page 45: The end
<strong>Physics</strong> 236: the big ques^on
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