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[LECS/CM-06001] Scattering Theory --- Basic DefinitionsNode id: 6192page |
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24-04-18 03:04:31 |
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[DOC/LOG-2024-03] LOG, HISTORY and INFORMATIONNode id: 6086pageThe workflow, time allotment to different activities of Proofs program are divided into several compartments.
This is a log file |
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24-04-18 03:04:26 |
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[NOTES/CM-06003] Particles --- Which area is the cross section?Node id: 6197pageFor scattering of particles, we explain which area is scattering cross section. |
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24-04-17 23:04:25 |
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[NOTES/CM-06002] Scattering of WavesNode id: 6193pageThe definition of scattering cross section for waves is given and the interpretation as an area is explained. |
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24-04-17 23:04:48 |
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[NOTES/CM-06004] Node id: 6194page |
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24-04-17 19:04:38 |
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[LECS/CM-06004] Centre of Mass and Laboratory FramesNode id: 6196page |
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24-04-17 07:04:09 |
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Trying TOC Scattering Theory --- Basic Definitions Node id: 6195page |
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24-04-16 21:04:49 |
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[NOTES/CM-05009] Keplar Problem --- Solving Differential EquationNode id: 6191pageDifferential equation for orbits is solved. The orbits are shown to be conic sections. Kepler's three laws are proved. Some properties of hyperbolic orbits are derived.$\newcommand{\pp}[2][]{\frac{\partial#1}{\partial #2}} \newcommand{\PP}[2][]{\frac{\partial^2#1}{\partial #2^2}} \newcommand{\dd}[2][]{\frac{d#1}{d #2}} \newcommand{\DD}[2][]{\frac{d^2#1}{d #2^2}}$ |
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24-04-14 15:04:28 |
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[NOTES/CM-05006] Effective Potential for Spherically Symmetric ProblemsNode id: 6180pageUsing angular momentum conservation it is shown that orbits for a spherically symmetric potential lie in a plane; This makes it possible to work in plane polar coordinates. The equation for radial motion becomes similar to that in one dimension with potential replaced by an effective potential. An expression for the effective potential is obtained. |
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24-04-14 08:04:31 |
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\(\S 16.4\) Hydrogen atom Energy LevelsNode id: 856page |
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24-04-13 06:04:34 |
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\(\S16.1\) General Properties of Spherically Symmetric Potential Problems Node id: 853page |
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24-04-13 06:04:02 |
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[NOTES/CM-02004] Integration of EOM by QuadraturesNode id: 6043page$\newcommand{\dd}[2][]{\frac{d #1}{d #2}};\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}};$ We discuss an example of particle in two dimensions in a potential independent of \(\theta\). By working in plane polar coordinates, we show how solution of equations of motion can be reduced to quadratures. |
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24-04-13 05:04:40 |
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[NOTES/QM-12002] Free Particle Wave PacketsNode id: 6187page$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}}\newcommand{\dd}[2][]{\frac{d#1}{d#2}}\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}\newcommand{\average}[2]{\langle#1|#2|#1\rangle}$
A particle with localized position is described by a wave packet in quantum mechanics. Taking a free Gaussian wave packet, its wave function at arbitrary time is computed. It is fund that the average value of position varies with time like position of a classical particle. The average vale of momentum remains constant and the uncertainty \(\Delta x\) increases with time. |
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24-04-13 01:04:13 |
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[NOTES/ME-02001] Rotation of Coordinate AxesNode id: 5656page$\newcommand{\mid}{|}$
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24-04-12 17:04:43 |
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[NOTES/QM-12003] Propagator for Free ParticleNode id: 6189page$\newcommand{\Prime}{{^\prime}} \newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}} \newcommand{\xbf}{{\mathbf x}}$
The Green function and the propagator for time dependent Schr\:{o}dinger equation are defined. The time dependent Schr\"{o}dinger equation is soled to obtain the solution for propagator. |
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24-04-12 01:04:00 |
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[NOTES/QM-12001] Free Particle Energy Eigenfunctions and eigenvaluesNode id: 6186page$\newcommand{\DD}[2][]{\frac{d^2#1}{d#2^2}}\newcommand{\kbf}{{\mathbf k}}\newcommand{\xbf}{{\mathbf x}}\newcommand{\rbf}{{\mathbf r}}\newcommand{\Prime}{{^\prime}}$
The energy eigenvalues and eigenfunctions are obtained for a free particle in one dimension. Properties and delta function normalization are discussed. It is shown that the energy eigenvalue must be positive. The free particle solution in three dimension is briefly given. |
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24-04-11 11:04:21 |
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2. Density Matrix --- Lecture Given at Univ Hyd 2024 --- Refresher Course Node id: 6063page |
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24-04-11 03:04:11 |
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[DOC/FBI-ToProcess]Node id: 6185pageThis page contains list of Fully Baked Resources to Process.
- These are mostly lectures notes for courses and are scattered over different Folders in Laptop WorkSpace
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24-04-10 08:04:40 |
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Test and Examination PapersNode id: 2491curated_contentFor Downloads Open Attached File(s) Tab |
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24-04-10 06:04:14 |
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[NOTES/QM-11001] Time Dependent Schrodinger Equation :Solution for Wave function at time \(t\)Node id: 4729page$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle} \newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}} \newcommand{\dd}[2][]{\frac{d#1}{d#2}} \newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}} newcommand{\average}[2]{\langle#1|#2|#1\rangle}$
We show how solution of time dependent Schrodinger equation can be found. Explicit expression for the wave function at arbitrary time \(t\) is obtained in terms of energy eigen functions and eigen values. |
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24-04-09 20:04:32 |
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