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[1998TH/LNP-07] Lecture -7 Mathematical PreparationNode id: 5549page |
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22-07-08 07:07:09 |
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[NOTES/QM-16002] Spherically Symmetric Potentials — Using Spherical Polar CoordinatesNode id: 4781page$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}$ $\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}$ $\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}}$ $\newcommand{\dd}[2][]{\frac{d#1}{d#2}}$ $\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}$ $\newcommand{\average}[2]{\langle#1|#2|#1\rangle}$ qm-lec-16002
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22-03-07 19:03:56 |
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[NOTES/ME-06007]-Node id: 5683page |
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22-08-14 19:08:48 |
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[NOTES/EM-10006]-Maxwell's Fourth Equation, Displacement CurrentNode id: 5739page$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}$ $\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}$ $\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}}$ $\newcommand{\dd}[2][]{\frac{d#1}{d#2}}$ $\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}$ $\newcommand{\average}[2]{\langle#1|#2|#1\rangle}$
We discuss how Maxwell's addition of a displacement current in the fourth equation.
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23-03-03 21:03:00 |
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[NOTES/QCQI-01005] Bloch Sphere Node id: 5022page |
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22-04-07 13:04:01 |
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testing sample Node id: 5818page |
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22-12-02 18:12:57 |
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[QUE/TH-07001] TH-PROBLEMNode id: 5165pageThe tension $\tau$ in an elastic rubber band is given by $$ \tau\,=\,aT\left(\frac{L}{L_0(T)}-\,\left(\frac{L_0(T)}{L}\right)^2\right),$$ where $a$ is a constant, $L_0(T)$is the unstretched length at zero tension, and is a function of temperature only.
- Write the first law using the work done when it is elongated and gets a supply of heat. ( Be careful of signs!)
- Use the first law to write $dF$, where $F$ is the free energy of the rubber band.
- Solve for the free energy $F$ and show that $$ F(T,L)\,-\,F(T,L_0(T))\,=\,aT\left(\frac{L^2}{2L_0(T)}\,+\,\frac{L_0(T)^2}{L^2}\,-\,\frac{3L_0(T)}{2}\right)$$ and the entropy $S$ $$ S(T,L)\,-\,S(T,L_0(T))\,=\,a\left(\frac{3L_0}{2}\,-\,\frac{L_0^2}{L}\,-\,\frac{L^2}{2L_0}\right)\,-\,aT\left(\frac{3}{2}\,-\,\frac{2L_0}{L}\,+\,\frac{L^2}{2L_0^2}\right)\frac{dL_0(T)}{dT} $$
- Find the heat $Q$ transferred to the elastic band when it is stretched from $L_0$ to $L$ isothermally.
- Show that $$ \left(\frac{\partial T}{\partial L}\right)_S \,=\,\frac{aTL_0^2}{c_LL^2}\left(-1\,+\,\left(\frac{L}{L_0}\right)^3\,+\,\frac{Ta}{L_0}\frac{dL_0}{dT}\left(2\,+\,\left(\frac{L}{L_0}\right)^3\right)\right)$$ where $$c_L\,=\,\left(\frac{DQ}{\partial T}\right)_L.$$
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22-01-13 18:01:49 |
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[QUE/SM-04024] SM-PROBLEMNode id: 5223pageConsider a system having 3 non-interacting particles, each having three possible energy levels with energies $0\,,\,2\Delta\,,\,4\Delta$. Let $N_1\,,\,N_2\,,\,N_3$ be the number of particles occupying the energy levels Find the average of $N_1N_2$ when the system is at temperature $T$.
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22-01-23 20:01:46 |
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[NOTES/EM-03015] Energy of a Continuous Charge DistributionNode id: 5965page$\newcommand{\Label}[1]{\label{#1}}\newcommand{\eqRef}[1]{\eqref{#1}}$
The electrostatic energy associated with continuous charge distribution is shown to correspond to energy \(\frac{\epsilon_0}{2} |\vec E|^2\) per unit volume.
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23-10-21 06:10:54 |
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[2013]Node id: 5373page |
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22-04-15 14:04:43 |
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[PSET/EM-01001]Node id: 5435page |
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22-05-21 06:05:52 |
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[2003SM/LNP-22] Lecture 22 -- Perfect Fermi GasNode id: 5521page |
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22-07-04 10:07:32 |
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[1998TH/LNP-17]-Node id: 5587page |
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22-07-17 18:07:32 |
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[NOTES/QM-09003] Solution of TIme Dependent Schrodinger Equation Node id: 4706page$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}$ $\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}$ $\newcommand{\PP}[2][]{\frac{\partial^2 #1}{\partial #2^2}}$ $\newcommand{\dd}[2][]{\frac{d#1}{d#2}}$ $\newcommand{\pp}[2][]{\frac{\partial #1}{\partial #2}}$
A scheme to solve the time dependent Schr\"{o}dinger equation \begin{equation} \label{eq01} i\hbar \dd{t}\ket{\psi} = \hat{H} \ket{\psi} \end{equation} is described. The final solution will be presented in the form, see \eqref{eq14} \begin{equation} \ket{\psi t} = U(t, t_0) \ket{\psi t_0} \label{eq16} \end{equation}where \begin{equation}\label{EQ16A} U(t, t_0) \ket{\psi t_0} = \exp\Big(\frac{-i H(t-t_0)}{\hbar}\Big)\end{equation}
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24-03-23 05:03:26 |
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[LECS/EM-03003]-Electrostatic EnergyNode id: 5653pageThe electrostatic energy of a continuous charge distribution is defined as the energy required to assemble the charges at infinity into the positions as in the given distribution. For a continuous charge distribution it is shown to be \( \dfrac{\epsilon_0}{2}\iiint(\vec E\cdot\vec E) dV\) . Thus a volume of space having nonvanishing electric field has energy density \(\dfrac{\epsilon_0}{2}(\vec E\cdot\vec E)\).The expression for the electrostatic energy reduces to the usual answer \(\frac{1}{2} CV^2\) for a charged parallel plate capacitor. For a uniformly charged sphere of radius \(R\) the electrostatic energy is proved to be equal to \(\frac{3}{5}\Big(\frac{Q^2}{4\pi\epsilon_0 R^2} \Big)\).
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24-03-30 05:03:23 |
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[NOTES/EM-07006]-Lorentz Force on a Current DistributionNode id: 5711page
Starting from Lorentz force per unit volume on a current carrying conductor due to magnetic field is shown to be \(\vec{j}\times\vec{B}\)
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24-03-05 09:03:16 |
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[QUE/SM-04019] SM-PROBLEMNode id: 5091pageThe average kinetic energy of the hydrogen atoms in a certain stellar atmosphere ( assumed to be in equilibrium) is $1$ electron volt.
(a) What is the temperature in Kelvin?
(b) What is the ratio of the number of atoms in the $N=3$ state to the number in the ground state.
(c) Discuss qualitatively the ration of the number of ionized atoms to the atoms in the $N\,=\,3$ state, with out taking the density of states for the ionized atoms, i.e., taking only the Boltzmann factor. ( Taking the density of states has an interesting consequence, first pointed out by Prof. M.N.Saha . Will discuss this in the class)
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22-01-09 20:01:18 |
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[QUE/TH-02006] TH-PROBLEMNode id: 5197pageA metal wire of cross-sectional area 0.0085 cm$^2$ under a tension of 20 N and a temperature of 20$^\circ$C is stretched between two rigid supports 1.2 m apart. If the temperature is reduced to 8$^\circ$C, what is the final tension? (Assume that $\alpha$ and $Y$ remain constant at the values $1.5\times10^{-5}$K$^{-1}$ and $2.0\times10^9$ N/m$^2$ respectively)
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22-01-16 17:01:07 |
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[2019CM/TEST-01]Node id: 5343pageClassical Mechanics July 3, 2019 $\newcommand{\Lsc}{\mathscr L}$
Test-I
- For a system the Hamiltonian is given to be \begin{equation*} H(q,p) = \frac{p^\beta}{\beta} + V(q) \end{equation*}
- Obtain Hamilton's equations of motion.\hfill[3]
- Show that the Lagrangian of the system is given by [4] \[L = \frac{q^\alpha}{\alpha} -V(q)\] where \(\alpha\) is given by \[ \frac{1}{\alpha} + \frac{1}{\beta}=1\]
- Consider a particle of mass $m$ moving in two dimensions in a potential The equation of motion for small oscillations are given to be \begin{eqnarray} m\ddot{x} = \frac{1}{2}\big( 3x + y \big)\\ m\ddot{y} = \frac{1}{2}\big(x + 3 y \big)\\ \end{eqnarray} [5+5+5]
- Find the normal frequencies of vibration in (b).
- Obtain expressions for \(x,y\) in terms of normal coordinates.
- Write the Lagrangian in terms of normal coordinates and verify that it takes the form \[{\Lsc} = \frac{1}{2}(\omega_1^2\dot{Q}_1^2+\omega_2^2\dot{Q}_2^2) - \frac{1}{2}(Q_1^2+Q_2^2)\]
- Find a differential equation for \(f(P)\) so that the transformation[3+2+3] \begin{equation*} q=\frac{f(P)}{m\omega} \sin Q, \quad p= f(P) \cos Q \end{equation*} may be a canonical transformation.
- Solve the differential equation you get subject to condition \(f(0)=0\) and show that \[ f= \sqrt{2m\omega P}\]
- Obtain the type 1 generator for this transformation.
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22-04-01 14:04:43 |
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[NOTES/EM-07014] Conservation Laws for Electromagnetic FieldsNode id: 5998page$\newcommand{\Tca}{\mathcal T}\newcommand{\Pca}{\mathcal P}$
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23-11-04 23:11:23 |
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