User contributions for ScottMiller
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22 April 2010
- 15:4215:42, 22 April 2010 diff hist +164 Phy5646 →'''<span style="color:#2B65EC">Second Quantization</span>'''
- 15:3415:34, 22 April 2010 diff hist +180 Phy5646 →'''<span style="color:#2B65EC">Second Quantization</span>'''
- 15:3115:31, 22 April 2010 diff hist +354 Phy5646 →'''Many Particle Systems and Identical Particles'''
4 December 2009
- 11:5011:50, 4 December 2009 diff hist +8 Phy5645 →Transmission-Reflection, S-matrix
- 11:2111:21, 4 December 2009 diff hist +19 Phy5645 →Stability of Matter
3 December 2009
- 15:5815:58, 3 December 2009 diff hist +4 Phy5645 →Generalized derivation
- 15:5715:57, 3 December 2009 diff hist +16 Phy5645 →Orbital angular momentum eigenfunctions
- 15:5515:55, 3 December 2009 diff hist +8 Phy5645 →Eigenvalue quantization
- 15:5415:54, 3 December 2009 diff hist +19 Phy5645 →WKB
- 15:4915:49, 3 December 2009 diff hist −4 Phy5645 →Motion in electromagnetic field
- 15:4715:47, 3 December 2009 diff hist +5 Phy5645/Particle in Uniform Magnetic Field No edit summary
- 15:4515:45, 3 December 2009 diff hist +54 Phy5645 →Motion in electromagnetic field
- 15:4015:40, 3 December 2009 diff hist +18 Phy5645 →Gauge
- 15:3715:37, 3 December 2009 diff hist +8 Phy5645 →Saddle point action
- 15:3515:35, 3 December 2009 diff hist +135 Phy5645 →Coherent states
- 15:2515:25, 3 December 2009 diff hist +20 Phy5645 →Harmonic oscillator spectrum and eigenstates
- 15:1815:18, 3 December 2009 diff hist +2 Phy5645 →Problems
- 15:1815:18, 3 December 2009 diff hist +6 Phy5645 →Feynman path integrals
- 15:1715:17, 3 December 2009 diff hist +2 Phy5645 →The Interaction Picture
- 15:1615:16, 3 December 2009 diff hist +15 Phy5645 →The Interaction Picture
- 15:1515:15, 3 December 2009 diff hist +200 Phy5645 →The Heisenberg Equation of Motion
- 15:0815:08, 3 December 2009 diff hist +4 Phy5645 →The Law of Calculation for Operators
- 15:0715:07, 3 December 2009 diff hist +36 Phy5645 →Motion in a periodic potential
- 15:0615:06, 3 December 2009 diff hist +6 Phy5645/Square Wave Potential Problem No edit summary
- 15:0215:02, 3 December 2009 diff hist +4 Phy5645 →Scattering states
- 15:0115:01, 3 December 2009 diff hist +4 Phy5645 →Basic Properties
- 14:5714:57, 3 December 2009 diff hist +111 Phy5645 →Schrödinger equation
- 14:4514:45, 3 December 2009 diff hist −150 Phy5645 →Schrödinger equation
- 14:4214:42, 3 December 2009 diff hist +2 Phy5645 →Schrödinger equation
- 14:4014:40, 3 December 2009 diff hist +1 Phy5645 →Schrödinger equation
- 14:3714:37, 3 December 2009 diff hist +2 Phy5645 →Schrödinger equation
2 December 2009
- 16:1016:10, 2 December 2009 diff hist +1,752 Phy5645 →Central potential scattering and phase shifts
- 15:0815:08, 2 December 2009 diff hist +62 Phy5645 →Central potential scattering and phase shifts
- 15:0715:07, 2 December 2009 diff hist +1,910 N Worked Problem for Scattering on a Delta-Shell Potential New page: Consider an attractive delta-shell potential (<math>\lambda > 0</math>) of the form: <math>V(\textbf{r})=-\frac{\hbar^2 \lambda}{2m} \delta(r-a)</math> 1) Derive the equation for the pha...
- 14:5914:59, 2 December 2009 diff hist +1,846 Phy5645/Problem3 No edit summary current
- 13:4613:46, 2 December 2009 diff hist +64 N Phy5645/Problem3 New page: Consider an attractive delta-shell potential (<math>\lambda > 0)
10 October 2009
- 14:1014:10, 10 October 2009 diff hist +82 Phy5645 →Motion in a periodic potential
- 14:0614:06, 10 October 2009 diff hist −1 Phy5645/Square Wave Potential Problem No edit summary
- 14:0214:02, 10 October 2009 diff hist +3,078 N Phy5645/Square Wave Potential Problem New page: 2. consider an infinite series of dirac delta function potential wells in one dimension such that: <math> ~V(x+a) = V(x) </math> solve for <math> ~\psi(x+a)</math> in terms <math>\psi(x)...
- 13:0213:02, 10 October 2009 diff hist +8 Phy5645 →UV Catastrophe (Black Body Radiation)
- 13:0113:01, 10 October 2009 diff hist +86 Phy5645 →UV Catastrophe (Black Body Radiation)
- 12:5912:59, 10 October 2009 diff hist +786 N Talk:Phy5645 New page: Given that Planck's energy distribution equation is: <math> \rho_{Planck} = \frac{2c^2}{\lambda^5}\frac{h}{e^\frac{hc}{\lambda k T}-1}</math> show that in the long wavelength limit this ...
13 September 2009
- 13:1513:15, 13 September 2009 diff hist +1,345 Phy5645 →Photoelectric Effect
- 12:3612:36, 13 September 2009 diff hist +1 m Phy5645 →UV Catastrophe (Black Body Radiation)
- 12:3512:35, 13 September 2009 diff hist −1 m Phy5645 →UV Catastrophe (Black Body Radiation)
- 12:3412:34, 13 September 2009 diff hist +15 Phy5645 →UV Catastrophe (Black Body Radiation)
- 12:3312:33, 13 September 2009 diff hist −1 m Phy5645 →UV Catastrophe (Black Body Radiation)
- 12:3212:32, 13 September 2009 diff hist −3 Phy5645 →UV Catastrophe (Black Body Radiation)
- 12:3112:31, 13 September 2009 diff hist +1,661 Phy5645 →UV Catastrophy (Blackbody Radiation)
8 September 2009
- 08:5408:54, 8 September 2009 diff hist +26 Phy5645 →Stationary states