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[1998TH/LNP-07] Lecture -7 Mathematical Preparation

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AK-47's picture 22-07-08 07:07:09 n

[NOTES/QM-16002] Spherically Symmetric Potentials — Using Spherical Polar Coordinates

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$\newcommand{\DD}[2][]{\frac{d^2 #1}{d^2 #2}}$ 
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qm-lec-16002

AK-47's picture 22-03-07 19:03:56 y

[NOTES/ME-06007]-

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AK-47's picture 22-08-14 19:08:48 n

[NOTES/EM-10006]-Maxwell's Fourth Equation, Displacement Current

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We discuss how Maxwell's addition of a displacement current in the fourth equation.


 

AK-47's picture 23-03-03 21:03:00 n

[NOTES/QCQI-01005] Bloch Sphere

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AK-47's picture 22-04-07 13:04:01 y

testing sample

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AK-47's picture 22-12-02 18:12:57 n

[QUE/TH-07001] TH-PROBLEM

Node id: 5165page

The 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 $$c_L\,=\,\left(\frac{DQ}{\partial T}\right)_L.$$
AK-47's picture 22-01-13 18:01:49 n

[QUE/SM-04024] SM-PROBLEM

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Consider 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 $T$.

AK-47's picture 22-01-23 20:01:46 n

[NOTES/EM-03015] Energy of a Continuous Charge Distribution

Node id: 5965page

The electrostatic energy  associated with continuous charge distribution is shown to correspond to  energy \(\frac{\epsilon_0}{2} |\vec E|^2\) per unit volume.

AK-47's picture 23-10-21 06:10:54 n

[2013]

Node id: 5373page
AK-47's picture 22-04-15 14:04:43 n

[PSET/EM-01001]

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AK-47's picture 22-05-21 06:05:52 n

[2003SM/LNP-22] Lecture 22 -- Perfect Fermi Gas

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AK-47's picture 22-07-04 10:07:32 n

[1998TH/LNP-17]-

Node id: 5587page
AK-47's picture 22-07-17 18:07:32 n

[NOTES/QM-09003] Solution of TIme Dependent Schrodinger Equation

Node id: 4706page

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}


AK-47's picture 24-03-23 05:03:26 n

[LECS/EM-03003]-Electrostatic Energy

Node id: 5653page

The 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 \(\frac{3}{5}\Big(\frac{Q^2}{4\pi\epsilon_0 R^2} \Big)\).   

AK-47's picture 24-03-30 05:03:23 n

[NOTES/EM-07006]-Lorentz Force on a Current Distribution

Node id: 5711page

Starting from Lorentz force per unit volume on a current carrying conductor due to magnetic field is shown to be \(\vec{j}\times\vec{B}\)


 

AK-47's picture 24-03-05 09:03:16 n

[QUE/SM-04019] SM-PROBLEM

Node id: 5091page

The 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)

AK-47's picture 22-01-09 20:01:18 n

[QUE/TH-02006] TH-PROBLEM

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A 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)

AK-47's picture 22-01-16 17:01:07 n

[2019CM/TEST-01]

Node id: 5343page

Classical Mechanics               July 3, 2019


Test-I

 

  • For a system the Hamiltonian is given to be \begin{equation*} H(q,p) = \frac{p^\beta}{\beta} + V(q) \end{equation*}
    1. Obtain Hamilton's equations of motion.\hfill[3]
    2. 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]
    1. Find the normal frequencies of vibration in (b).
    2. Obtain expressions for \(x,y\) in terms of normal coordinates.
    3. Write the Lagrangian in terms of normal coordinates and verify that it takes the form \[{\Lsc} = \frac{1}{2}(\omega_1^2\dot{Q}_1^2+\omega_2^2\dot{Q}_2^2) - \frac{1}{2}(Q_1^2+Q_2^2)\]
    1. 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.
    2. Solve the differential equation you get subject to condition \(f(0)=0\) and show that \[ f= \sqrt{2m\omega P}\]
    3. Obtain the type 1 generator for this transformation.
AK-47's picture 22-04-01 14:04:43 n

[NOTES/EM-07014] Conservation Laws for Electromagnetic Fields

Node id: 5998page
AK-47's picture 23-11-04 23:11:23 n

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