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[NOTES/QM-17003] Some Useful Restrictions on CG coefficientsNode id: 4816page$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}$ $\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}$ $\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}}$ $\newcommand{\dd}[2][]{\frac{d#1}{d#2}}$ $\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}$ $\newcommand{\average}[2]{\langle#1|#2|#1\rangle}$ $\newcommand{\ket}[1]{\langle #1\rangle}$ qm-lec-17003
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22-03-04 09:03:10 |
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[NOTES/ME-14006]-Tensor Nature of Moment of InertiaNode id: 5700page |
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22-08-16 16:08:14 |
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[NOTES/EM-11004]-Wave Equation for FieldsNode id: 5756page
The Maxwell's equations in vacuum, in absence of charges and currents are written and are shown to imply wave equation for the electric and magnetic fields. The plane wave solutions, the electromagnetic waves, are shown to travel with a velocity equal to \(1/\sqrt{\mu_0\epsilon_0}\). The numerical value of this expression equals the velocity of light. This leads to the identification of light as electromagnetic waves.
$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}$ $\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}$ $\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}}$ $\newcommand{\dd}[2][]{\frac{d#1}{d#2}}$ $\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}$ $\newcommand{\average}[2]{\langle#1|#2|#1\rangle}$
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23-03-03 21:03:01 |
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[QUE/SM-03004] SM-PROBLEM Node id: 5068pageConsider an isolated system of ideal gas of $N$ molecules contained in a volume $V$ and having an energy $$E=\sum_{i=1}^{3N}\frac{p_i^2}{2m}.$$ Show that the number of states in the energy range $U-\Delta$ and $U$ is of the system is given by\hfill [5] \begin{eqnarray*} \frac{1}{\Gamma(3N/2+1)}\frac{3N\Delta}{2U} \Big(\frac{mU V^{2/3} }{2\pi\hbar^2}\Big)^{3N/2} \end{eqnarray*}
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22-01-13 16:01:30 |
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[QUE/TH-09002] TH-PROBLEMNode id: 5186pageThe equation of state of system is given by ( in standard notation). The internal energy of the system is
$$ P\,=\,\frac{aT^3}{V} $$
$$ U\,=\,BT^n{\ln}(\frac{V}{V_0})\,+\,f(T), $$
where $B\,,n$ and $V_0$ are all constants. $f(T)$ is a function of only $T$. Find $n$ and a relation between $a$ and $B$. ( Use the fact that entropy is a perfect differential.)
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22-01-14 13:01:54 |
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[2003SM/LNP-15] Lecture-15--Quantum Effects in Statistical MechanicsNode id: 5540pageQuantum effects in macroscopic systems appear in two ways. The first the energy levels are quantized. The quantization of energy levels does not need any modification in the framework. Secondly identical nature of particles constituting the system. This requires a new approach to enumerating the microstates. The microstates are not labeled by coordinates and momenta as is the case in classical theory. In quantum theory the microstates are specified by giving the number of particles for different levels.
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22-07-07 07:07:53 |
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[1998TH/LNP-35]-Thermodynamics Applied to RadiationNode id: 5604page |
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22-07-17 19:07:30 |
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[NOTES/QM-11005] TIme Dependent Schr\"{o}dinger Equation --- Propagator Node id: 4733page$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}} \newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}}\newcommand{\dd}[2][]{\frac{d#1}{d#2}}\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}\newcommand{\average}[2]{\langle#1|#2|#1\rangle} \newcommand{\dd}[2][]{\frac{d#1}{d#2}}\newcommand{\Label}[1]{\label{#1}}$
We discuss the solution of time dependent one particle Schrodinger equation and obtain an expression for the propagator giving the time development.
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24-06-23 18:06:49 |
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[NOTES/ME-06001]- Application of Energy Conservation Law Node id: 5672page$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}$ $\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}$ $\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}}$ $\newcommand{\dd}[2][]{\frac{d#1}{d#2}}$ $\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}$ $\newcommand{\average}[2]{\langle#1|#2|#1\rangle}$
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22-08-14 10:08:50 |
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Editing LaTeX ExpressionNode id: 4885page\begin{eqnarray} \frac{\mu V_0}{\hbar^2 k}\left|\int_0^{R_0} \left( e^{2ikr}-1\right) dr\right| &=& \frac{\mu V_0}{\hbar^2 k}\left|\frac{e^{2ikR_0}-1}{2ik} - R_0 \right|\label{E2}\\ &=& \frac{\mu V_0}{2\hbar^2 k^2}\left|e^{2ikR_0}- 2ik R_0 -1 \right|\label{E3} \end{eqnarray}
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21-11-07 18:11:50 |
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[NOTES/EM-09007]-Electromotive ForceNode id: 5728pageThe concept of electromotive force is explained by means of water coller pump analogy.
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22-08-24 17:08:51 |
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21Th-ProbSet8Node id: 5005page |
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21-12-01 20:12:43 |
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[QUE/TH-01003] TH-PROBLEMNode id: 5153pageLet $$\frac{\partial (x,y)}{\partial (a,b)}\,\equiv\,\left|\begin{array}{ll} \frac{\partial x}{\partial a}&\frac{\partial y}{\partial a}\\ \frac{\partial x}{\partial b}&\frac{\partial y}{\partial b}\\ \end{array}\right|$$
Then show that $$ \frac{\partial (x,y)}{\partial (a,b)}\frac{\partial (a,b)}{\partial (c,d)}\,=\,\frac{\partial (x,y)}{\partial (c,d)} $$
Remarks : 1. This can be generalised to higher dimensions.
2. This can be found in books - and is very useful in changing variables in multiple integrals.
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22-01-13 17:01:58 |
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[QUE/TH-07008] TH-PROBLEMNode id: 5214pageA cylinder closed at both ends with adiabatic walls, is divided into two parts by a movable piston. The piston is frictionless and adiabatic. Originally, the pressure, volume, and the temperature of the gas are the same, $(P_0,V_0,T_0)$, on the two sides of the piston. The gas is ideal gas with $C_v$ independent of $T$ and $\gamma=1.5$. By means of a heating coil on the left hand side, heat is slowly supplied to the gas on the left hand side until the pressure reaches ${27\over 8}P_0$.
- what is the entropy change of the gas on the left?
- what is the entropy change of the gas on the right?
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22-01-23 11:01:17 |
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[NOTES/EM-02009] Line Integrals In PhysicsNode id: 5955pageA few examples of problems are given from electromagnetic theory and other areas of physics are given in which the line integral appears.
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23-10-12 17:10:01 |
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[2019EM/QUIZ-09]Node id: 5361pageElectrodynamics Apr 19, 2019 Quiz-IX
The above image is reproduced from a book. Read Example 8.5 carefully. Answer the following questions.
- Do you agree that there is no flux linked with the circuit when key is open?
- Do you agree that there will be induced current when the circuit is closed. But the coil and the magnet remain stationary?
- If you disagree what is the mistake? Does the flux rule apply or not in this case?
- Write any other comment you may have.
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22-04-04 17:04:58 |
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[2018EM/HMW-04]Node id: 5425page |
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22-06-21 08:06:35 |
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[NOTES/EM-01002]- Thomson’s Method for e/mNode id: 5506pageThomson passed electrons through a region having mutually perpendicular electric and magnetic field, and both perpendicular to the velocity of the electrons. The fields were adjusted so as to produce no deflection. This enebled him to measure the \(e/m\) of electrons.
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22-11-17 18:11:52 |
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[NOTES/EM-02006]-Proof of Gauss LawNode id: 5578pageThe Gauss law of electrostatics follows from the Coulomb’s law for a point charge and superposition principle. The proof given here follows Feynman’s lectures. It makes use of two important features of the electric field due to a point charge. These are (i) the magnitude of the field obeying the inverse square law, and (ii) radial direction of the electric field of a point charge. The above two properties are essential to the proof. Gauss law will not hold for hypothetical field, not having both the properties.
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23-10-09 04:10:51 |
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[NOTES/QM-09001] Unitary Operator for Time EvolutionNode id: 4678page $\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}$ $\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}$ $\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}}$ $\newcommand{\dd}[2][]{\frac{d#1}{d#2}}$ $\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}$
That assumption that the superposition principle be preserved under time evolution leads to unitary nature of the them evolution operator. The state vector satisfies differential equation, the Schrodinger equation, with Hamiltonian as the generator of time evolution.
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24-06-22 09:06:43 |
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