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[2003SM/LNP-01] Lecture 01--ProbabilityNode id: 5524pageThe basic notions of probability theory, simple events, sample space and ensemble, are introduced. The probability of compound events, independent events and joint and conditional probability are defined. Examples are given to illustrate the basic concepts.
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22-07-03 23:07:09 |
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[1998TH/LNP-19]-Carnot Heat EngineNode id: 5589page |
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22-07-17 18:07:05 |
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[NOTES/QM-09005] Schr\"{o}dinger Picture ---- Important PointsNode id: 4708page
The time evolution of a general quantum system is reviewed in an abstract setting. The eigen states of energy are seen to have all properties that make them qualify for being called stationary states.The stationary states have the property that all observable quantities remain constant in time.
$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}$ $\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}$ $\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}}$ $\newcommand{\dd}[2][]{\frac{d#1}{d#2}}$ $\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}$ $\newcommand{\average}[2]{\langle#1|#2|#1\rangle}$
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24-03-24 05:03:08 |
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[NOTES/ME-02002]-The SO(3) GroupNode id: 5657page |
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22-08-17 16:08:27 |
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[NOTES/EM-07008]-Magnetic Vector PotentialNode id: 5713page
The vector potential is introduced using the Maxwell's equation \(\nabla \times \vec{B}=0\) and the equation \( \nabla \times \vec{B} = \mu_0 \vec{j}\) is derived. The expression for the magnetic field is obtained as volume integral, the Biot Savart law, is derived. The expressions for the magnetic field for the surface current and the line current are given.
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23-03-03 20:03:21 |
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[QUE/SM-08004] SM-PROBLEMNode id: 5093pageShow that the number of photons in a cavity at temperature $T$ and having a unit volume is $$ N\,=\, j \left(\frac{kT}{\hbar c}\right)^3 $$ where $j$ is a numerical constant.
Use the above result to show that the specific heat of a photon gas in proportional to $T^3$
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22-01-09 20:01:49 |
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[QUE/TH-02008] TH-PROBLEMNode id: 5199pageAn approximate equation of state of a real gas at moderate pressures, devised to take into account of the finite size of the molecules, is $P(v-b)=R\theta$, where $R$ and $b$ are constants. Show that
\begin{equation*} \beta = {1/\theta\over 1+bP/(R\theta)}~~,~~~~\chi = {1/P\over1+bP/(R\theta)} \end{equation*}
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22-01-16 17:01:49 |
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[2019CM/HMW-02]Node id: 5345page Classical Mechanics June 1,2009
Tutorial-II
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22-04-03 11:04:03 |
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[NOTES/EM-07004] Stokes TheoremNode id: 6000page
Relationship between the normal to a surface and the orientation of its boundary curve, as they should appear in Stokes theorem are explained.
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23-11-05 07:11:25 |
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[2008EM/QUIZ-01A]Node id: 5409page |
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22-05-11 07:05:55 |
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[1998TH/LNP-11] Lecture -11 Work in ThermodynamicsNode id: 5553page |
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22-07-08 07:07:50 |
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[ACQ/CV-05001] Understanding Relation Between Existence of Derivative and Being AnalyticNode id: 5623page |
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22-08-07 05:08:18 |
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[NOTES/ME-08003]-Effect of Earth's Rotation --Centrifugal ForceNode id: 5687page |
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24-04-08 07:04:57 |
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[NOTES/QM-25003] Charged Particle in E.M. FieldNode id: 4931page$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}$ $\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}$ $\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}}$ $\newcommand{\dd}[2][]{\frac{d#1}{d#2}}$ $\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}$ $\newcommand{\average}[2]{\langle#1|#2|#1\rangle}$ $\newcommand{\ket}[1]{\langle #1\rangle}$ qm-lec-25003
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22-03-12 18:03:00 |
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[NOTES/EM-10008]-Maxwell's Equations for Time Varying Fields and Ampere's LawNode id: 5743page$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}$ $\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}$ $\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}}$ $\newcommand{\dd}[2][]{\frac{d#1}{d#2}}$ $\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}$ $\newcommand{\average}[2]{\langle#1|#2|#1\rangle}$
Several concepts and results valid for static fields need revision when one is considering the situation of time varying fields. Some of these are discussed here
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23-03-03 20:03:05 |
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[NOTES/QCQI-03003] Density Matrix of Mixed State Node id: 5028page$\newcommand{\average}[2]{\langle#1|#2|#1\rangle}$
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22-04-07 13:04:02 |
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[QUE/TH-09001] TH-PROBLEMNode id: 5169pageConsider the following expressions for entropy. Which ones can possibly be a fundamental equation and which ones violate one or more of postulates II,III and IV?
- $S\,=\,K_1\left(NVU\right)^{1/3}$
- $ S\,=\,K_2\left(\frac{NU}{V}\right)^{2/3} $
- $ S\,=\,K_3\left(\frac{V^3}{NU}\right)$
- $ S\,=\,N{\rm{\ln}}\left(\frac{UV}{N^2K_4}\right)$
$K_i$'s are positive constants so that dimensions match. $S,U,N,V $ are the entropy, internal energy, number of particles and volume respectively.
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22-01-13 18:01:44 |
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[QUE/SM-04026] SM-PROBLEMNode id: 5227pageConsider a perfect gas having N particles obeying Maxwell- Boltzmann statistics and is in equilibrium at temperature $T$. Find the average of $\epsilon^r$ ( $r$ is a real number) where $\epsilon $ is the energy of a single particle.
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22-01-23 20:01:26 |
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[NOTES/EM-03020] Proof of Gauss Law from Maxwell's EquationsNode id: 5969pageA vector calculus proof of Gauss law is given starting from the Maxwell's equation \(\text{div} \vec E=\frac{\rho}{\epsilon_0}\)
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23-10-22 21:10:11 |
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[2013EM/HMW-03]Node id: 5377page |
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22-04-17 09:04:54 |
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