Physics 10-B,     Winter  2004
55 Roessler,    TuTh    3:10-4:30pm
Syllabus

Teacher: Professor Ling-Lie Chau
Office: 431 Phy/Geo; phone: 752-2715; e-mail: chau@physics.ucdavis.edu
Office hours:  431 Phys/Geo; TuTh 4:30-5pm-extendable; or by appointment.

 
The Cosmos and String Theory (the Theory of Everything)

Veil Nebula



Goals of the Course
* Learning, as non-scientists, up-to-date information and current understanding of our universe.
* Cultivating logical and creative thinking.
* Developing the ability to do “back-of-the-envelope” numerical estimates (two significant figures).
* Promoting self-discipline and participation skills and spirit.
* Making it a real life time enriching experiece.

 Course Outline
  · Powers of 10, Significant Figures, and Units.
  · Our Place in the Universe
  · The Science of Astronomy
  · A Universe of Matter and Energy
  · The Universal Law of Motion
  · Light: The Cosmic Messenger
  · Space and Time
  · Spacetime and Gravity
  · Building Blocks of the University
  · Our Star, and Properties of Stars
  · Galaxies, From Here to Horizon
  · Dark Matter, Dark Energy and the Fate of the Universe
  · The Beginning of Time

Textbooks:
* J. Bennett, M. Donahue, N. Schneider, and M. Voit, “The Cosmic Perspective,” 3RD ed., 2004.
* B. Greene,
    “The Elegant Universe: Superstrings, Hidden Dimensions, and the Quest for the Ultimate Theory,” 1999, with the 2003 Preface.

Reading Assignments

Discussion Groups:
Teaching Assistant: Mr. Steve Tappel
Office: Room 410 Phy/Geo; phone: 530-750-2144; e-mail: tappel@physics.ucdavis.edu
Office hours:  158 Roessler; W 7-7:30pm-extendable; or by appointment.

· Discussion group B01 (CRN 53095): Tu 5:10-6:00pm, 130 Phys/Geo
· Discussion group B02 (CRN 53096): Tu 6:10-7:00pm, 130 Phys/Geo
· Discussion group B03 (CRN 53097): W 5:10-6:00pm, 140 Phys/Geo
· Discussion group B04 (CRN 53098): W 6:10-7:00pm, 158 Roessler


Reference Web Sites  

Fractals: math, art, & infinite possibilitues
Indras Pearls : math, art, & infintie possibilities
Escher's endless gallery view  
Escher's Official Site  
Simulation of the End of the Cosmic Dark Age, by Gnedin of  Colorado U
Cosmic Reionization: the End of the Cosmic Dark Age, observation by Becker et al & by Djorgovski et al, 2001 

 Dark 
Energy Fills the Cosmos,  LBL, Berkeley, 1999
 
Picture above: Veil Nebula, 2.5 kly away in the direction of the Swan (Cygnus), remenats of supernovae 25 kyr ago
.
Nobel Prizes
Nobel Laureates in Physics
to my.ucdavis.edu
to UCD Library Home

Books reserved for phy010B at Shields
to Patricia Schwarz's web, Superstring
to collection of superstring sites
to Cambridge U Superstring web
to Wright's Cosmology Tutorial
to Hubble Space Telescope Public Pictures
to Astronomy Picture of the Day
to Imagine Site of NASA
to Home page of NASA
to site about geometry & fate of the universe
to site of Particle Data Group
to Chau's Davis Honors Challenge 2001 web
to Chau's Davis Honors Challenge 2002 web    

List of 10C (C for constancy)    
10C/C0: To begin with  
10C/C1: G, Newton's law of motion & universal law of gravity  
10C/C2-4: c, Maxwell's eqs for E&M;  h, Planck's work;  E=mc^2, Einstein's special relativity  
10C/C5-8: General Relativity; Quantum Physics; Building Blocks of the Universe; Standard Model & Gauge Principle
10C/C9-10: Grand Unification (GUT); The Theory of Everything (TOE)    

Guidelines for study and for exam preparation

 

Class Activities  


Cosmic Microwave (CMB) Anisotropy
Simulation of the End of the Cosmic Dark Age, by Gnedin of  Colorado U
Cosmic Reionization: the End of the Cosmic Dark Age, observation by Becker et al & by Djorgovski et al, 2001  
Class 20, 3/16/04, Final Exam Reminder; Hightlights; & concluding matters
 
Class 19, 3/11/04, Announcemetnts & Preview

Make-up Discussion Sessions & office hr, Thu, 3/11/04; HW9, Comments & minor typos  
Class 18, 3/9/04, preview; handing out graded Quiz 3, etc.

Class 17, 3/4/03, Quiz 3
3/2/04 news, Water on Mars
Hint to HW8, SA8.2    
 
Class 16, 3/2/04,
Highlights; Announcements and Preview
Class 15, 2/26/04, Highlights; a bonus challenge; & Announcements & Preview
Blackhole in NGC613, 65 Mly away  
Periodic Table from cs.ubc.ca web site
Wave Packet animations, Rochester U web site
Hints to HW7
Class 14, 2/24/05; Highlights ; New Policies & Reminders; Preview

particle physics, SLAC, Stanford, CA
particle physics, CERN, European Center
particle physics, Fermilab, IL
All about known matter: ParticleDataGroup educational site
Class 13, 2/19/04: Quiz2;
S4 of TB1: Building Blocks of the U    
Futherest object (a galaxy, 13 Gyr away, Z~7) observed through gravitational lensing, by Richard Ellis at al.
Futherest object, from Astro-picture-of-the-day
Class 12, 2/17/04: Spactime & Gravity; Review for Quiz2
Class 11, 2/12/04; Reminder of Quiz 2
   
Hulse & Taylor: new type of pulsar & gravitational radiation
Rubbia & van der Meer: discovering force particles (W & Z) of electroweak force, adding to the photon
Glashow, Salam, & Weinberg: electroweak theory

Yang & Lee: parity violation; Yang & Mills: gauge symmetry

Penzias & Wilson: discovering cosmic microwave background
Bethe: explaination of star energy  
Pauli, 1945 Nobel Prize: exclusion principle; quantum physics; proposed neutirno
Davisson & Thomson, 1927 Nobel Prize, showed the wave property of electron in the 1920'  

Schroedinger's wave eq. for partivles in 1926 & Dirac's anti-matter in 1928 & 1930, etc. 1933 Nobel Prize.  
De Broglie, Nobel Prize 1929: theoretical discovery of wave properties of particles in 192
Heisenberg: uncertainty relations, etc.
Einstein: photo electric effect, special & general relativity, Brownian motion, etc.
Michelson & Morley: Observing constant c, indepent of motions of an observer
 
J.J. Thomson, 1906 Nobel Prize: Discovered electron in 1897
Lorentz of the Lorentz transformation, a forerunner of Einstein and his special relativity

Class 10, 2/10/04, 
Beginning of 10C list; Comments & hints about SA5.2 of HW5    
Class 9, 2/8/04
Class 8, 2/3/04    

Class 7, 1/29/04,
Quiz 1
Class 6, 1/27/04
Class 5, 1/22/04

Class 4, 1/20/04
MSNBC: Symphony of Everything
Class 3, 1/15/04

The Ptolemy Univers

Ptolemy, Copernicus, Brahe, Kepler, Galileo, Newton
 
Class 2, 1/13/04

1 L = 10^-3 m^3 = 10^3 cm^3, also see a web about liter


Class 1, 1/8/04  
Useful web site on units: site of Rowlett at U of N Carolina 
Useful web site on fundamental constants: site of Particle Data Group
Useful web site on latest estimate of age of the universe
Units confusion bunrt the $125M Mars Polar Lander
 


Directives:
See Syllabus
Further Guidelines for Homework

 
Important e-mails
e1,1/3/04: Welcome, Mars, & No 1/7/04 discussion meetings
e2, 1/8/04: After-class web update; Careful reading of Syllabus due to complete by 1/13/04
e3, 1/9/04: Class web address modified; Bonus pts for during-class conributions


Copyright c 2004 by Professor Ling-Lie Chau. Copyrights reserved for all original material presented in this course. Request for permission or further information should be addressed to Professor Ling-Lie Chau.