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[QUE/QFT-06012] QFT-PROBLEM

Node id: 4372page

Let \(\displaystyle N=-\Big(\frac{i\beta\vec{\alpha}\cdot\vec{p} }{2mc}\Big)\, f\Big(\frac{|\vec{p}|}{mc}\Big)\)

  • Prove that \begin{equation} \exp(iN) = \cos\big(\frac{|\vec{p}|f}{2mc} \big) + \frac{\beta\vec{\alpha}\cdot\vec{p}}{|\vec{p}|} \sin \big(\frac{|\vec{p}|f}{2mc} \big), \end{equation} where \(H\) is Dirac Hamiltonian \(H=c\vec{\alpha}.\cdot\vec{p} + \beta mc^2\)
  • Find the real function \(f\) such that \begin{equation} H{'} = e^{iN} H e^{-iN} \end{equation} is free of operators odd operators. For this choice of \(f\) \[ H{'} = \beta c \sqrt{|\vec{p}|^2 + m^2c^2}.\]
shivahcu's picture 22-02-04 21:02:54 n

[QUIZ/ME-08002]

Node id: 4441page
shivahcu's picture 22-03-31 10:03:24 n

LaTeX practise mathematical formula arrays

Node id: 3870page
shivahcu's picture 20-12-18 10:12:48 n

[QUE/ME-08009] ME-PROBLEM

Node id: 3962page

A conical pendulum moves in a circular path of radius \(a\) and string making an angle \(\alpha\) with vertical.

  • Working in the inertial frame, draw a diagram showing the forces acting on the pendulum and prove that the angular frequency \(\omega\) is given by \[ \omega= \sqrt{\frac{g}{L\cos\alpha}}\]
  • Draw the all forces acting on the pendulum as seen from the rotating frame in which the pendulum is at rest. Is the resultant of all forces is zero or not? If it is not zero, how do you explain that the pendulum is at rest in the rotating frame? Give a complete answer.
  • Next consider a third frame rotating with angular velocity \(2\omega\), the direction of the angular velocity is the same as that of the pendulum. What is the motion of the pendulum as seen by an observer in this frame? Does the sum of all forces vanish now or not? Explain observed behaviour of the pendulum using the equation of motion as applicable in this frame.

%FigNoNumX{10,-65}{40}{0}{ConicalPendulum}

shivahcu's picture 22-02-09 08:02:57 n

[QUE/QFT-05006] QFT-PROBLEM

Node id: 4034page

For a free complex Klein Gordon field find the unequal time commutator as \[ \big[\phi(x), \phi(y)\big] = i\Delta(x-y)\] and express your answer for \(\Delta(x)\) as an integral of the form \[\int dq e^{-iqx} \delta(q^2-\mu^2) \epsilon(q_0) \] You need not compute the integral.

  • Argue that the function \(\Delta(x)\) is odd under change of sign of \(x\) and that it is Lorentz invariant.
  • For spacelike \(x\) show that there exists a Lorentz frame such that \(x^\prime =-x\). Hence prove that the function \(\Delta(x)\) vanishes for space like \(x\).
shivahcu's picture 22-02-04 08:02:38 n

[QUE/QFT-01002] QFT-PROBLEM

Node id: 4320page

Compute infinitesimal variations of the Lagrangian density for the Schrodinger field under the Galilean transformation \begin{equation} \vec{x} \longrightarrow \vec{x}{'} = \vec{x} + \vec{v} t \end{equation} and \begin{equation} \psi(\vec{x}) \longrightarrow \psi{'}(\vec{x}{'}) = e^{-im\vec{v}\,^{\prime\,2} t/(2\hbar)} e^{im\vec{v}\cdot\vec{x}/\hbar} \psi(\vec{x}). \end{equation} Verify that the the change in Lagrangian is a total time derivative. Find the corresponding constant of motion.

shivahcu's picture 22-02-06 19:02:03 n

[QUE/CM-02010]

Node id: 4412page
shivahcu's picture 22-03-19 17:03:38 n

[QUE/ME-02006] ME-PROBLEM

Node id: 3935page

Let \({\bf A, B,..}\) be objects with components written as \(\vec{A}=(A_1,A_2,A_3), \vec{B}=(B_1,B_2,B_3)\). Introduce \(\vec{A}{'}=(A_1{'},A_2{'},A_3{'}), \vec{B}{'}=(B_1{'},B_2{'},B_3{'})\) etc. by means of equation \begin{equation}\label{EQ01} \vec{A}{'} = \vec{A} -\sin \alpha (\hat{n}\times\vec{A}) + (1-\cos\alpha) \hat{n}\times (\hat{n}\times\vec{A}). \end{equation} and with similar equations for other vectors.

  • Using vector identities show that
    • \(\vec{A}{'}\cdot\vec{B}{'}=\vec{A}\cdot\vec{B}\);
    • If \(\vec{C}=\vec{A}\times\vec{B}\), then \(\vec{C}{'}\) is given by an equation similar to \eqRef{EQ01}.
  • How is the expression related \( \vec{A}{'}\cdot(\vec{B}{'}\times\vec{C}{'})\) related \( \vec{A}\cdot(\vec{B}\times\vec{C})\)?
shivahcu's picture 22-02-07 19:02:13 n

[QUE/ME-14005] ME-PROBLEM

Node id: 3992page

Question

 Find the moment of inertia tensor of a uniform rectangular plate w.r.t. the centre \(O\) of the plate relative to the axes \(K\) shown in figure. Use parallel axes theorem to find moment of inertia tensor relative to a set of axes \(K_2\) with origin taken as the corner \(E\). The \(Z\)- axis for both systems is perpendicular to the plate and out of the plane of paper.
%FigBelow{10,-25}{40}{0} RectangularPlate

Solution

We shall do it by evaluating the double integral. Divide the plate by lines parallel to the coordinate axes as in %Figref MI-Plate
Consider one rectangular element of sides \((dx, dy)\) at position \((x,y)\). If the mass of the plate is \(M\), the density of the plate is \(\sigma\), then \(4ab\sigma =M\) and the contribution of the rectangular element to \(I_{xx}\) is \(\sigma (dx\,dy) y^2\). Summing over all elements means integrating over \(x, y\) over their respective ranges. Thus %FigBelow{10,-25}{40}{0} RectangularPlate \begin{eqnarray}\nonumber I_{xx} &=& \int_{-a}^a dx \int_{-b}^b dy \sigma y^2 =\int_{-a}^a dx \sigma \frac{2b^3}{3} = \sigma \frac{2b^3}{3} \int_{-a}^a dx\\ &=& \sigma \frac{2b^3}{3} (2a) = \frac{Mb^2}{3} \qquad \HighLight{\mbox{$\because 4\sigma ab=M$}} \end{eqnarray} % Similarly \begin{eqnarray}\nonumber I_{yy} &=& \int_{-a}^a dx \int_{-b}^b dy \sigma x^2 =\int_{-a}^a dx \sigma x^2 (2b) = \sigma \frac{2b^3}{3} \int_{-a}^a dx\qquad \HighLight{\mbox{$\because 4\sigma ab=M$}}\\ &=& \sigma \frac{2a^3}{3} (2b) = \frac{Ma^2}{3} \end{eqnarray} and appealing to the law of perpendicular axes we get \(I_{zz}= M\frac{a^2+b^2}{3}\) The off diagonal term \(I_{xy}\) is \begin{equation} I_{xy} = - \int_{-a}^a dx \int_{-b}^b dy \sigma (xy) \end{equation} which vanishes due to the symmetry of the problem. Also \begin{equation} I_{xz} = - \int_{-a}^a dx \int_{-b}^b dy \sigma (xz) = 0 \end{equation} because \(z=0\) for all rectangular elements of the plate. Thus the moment of inertia tensor w.r.t.the center of mass is given by \begin{equation} \underline{\Ibb} = \frac{M}{6} \begin{pmatrix} b^2 & 0 & 0\\ 0 & a^2 & 0\\ 0 & 0 & a^2+b^2 \end{pmatrix} \end{equation} \paragraph*{MI Tensor relative to a corner} The parallel axes for the inertia tensor states that \begin{equation} I_{jk} = I^\text{cm}_{jk} + \Delta_{jk} \end{equation} where \(\Delta_{jk} =|\vec{a}|^2 \delta_{jk} -a_ja_k\) and \(\vec{a}\) is the position vector of the corner relative to the origin \(O\). For the corner \(E\) we have \(\vec{a}=(-a,-b,0)\) and \(|\vec{a}|^2=(a^2+b^2)\). Therefore, \begin{eqnarray} &\Delta_{xx} = b^2,\qquad \qquad \qquad \Delta _{yy} = a^2,\quad \qquad \Delta_{zz} = (a^2+b^2)&\\ &\qquad\quad\Delta_{xy}=\Delta_{yx}=-ab\qquad \Delta_{yz}=\Delta_{zy}=0\qquad \Delta_{zx}=\Delta_{xz}=0.\qquad\qquad& \end{eqnarray} Thus the moment of inertia tensor w.r.t.the corner at \(E\) is given by \begin{equation} \underline{\Ibb} = \frac{M}{3} \begin{pmatrix} b^2 + 3a^2 & -3ab & 0\\ -3ab & a^2 + 3b^2 & 0\\ 0 & 0 & 4a^2+4b^2 \end{pmatrix}. \end{equation}

shivahcu's picture 22-02-08 08:02:37 n

[QUE/QFT-15014] QFT-PROBLEM

Node id: 4078page

The matrix element for the decay process \(\pi \to \mu + \nu\) is given by
\[ m_{fi} =\frac{g}{\surd 2} \bar{u}^{(r)}(p) (\gamma_\mu iQ_\mu) (1-\gamma_5)v^{(s)}(k)\] for the life time computation we need to take absolute square, to average over initial spin and sum over final spin states. You may assume neutrino to be have a mass \(m_\nu\) and take limit 

shivahcu's picture 22-02-06 20:02:22 n

[QUE/QFT-14001] QFT-PROBLEM

Node id: 4385page

Prove that \begin{equation} \int_{t_0}^ t \, dt_1 \int_{t_0}^ {t_1} dt_2\, H^\prime_I(t_1) H^\prime_I(t_2) = \frac{1}{2} \int_{t_0}^ t \, dt_1 \int_{t_0}^ t \, dt_2 T\big( H^\prime_I(t_1) H^\prime_I(t_2)\big) \end{equation}

shivahcu's picture 22-02-01 19:02:07 n

[LSN/QFT-04002] Some Mathematical Preparation

Node id: 3874page
shivahcu's picture 22-03-29 20:03:39 n

[QUE/ME-08011] ME-PROBLEM

Node id: 3964page

$\newcommand{\Rbb}[]{\mathbb{R}}$

Question

Find rotation matrix for a rotation by an angle \(\alpha\) about the axis \(1,2,1\) where \(\cos\alpha=\frac{3}{5}, \sin\alpha =\frac{4}{5}\).

Solution

The unit vector along the direction \((1,2,1)\) is given by \(\hat{n}=\frac{1}{\sqrt{6}}(1,2,1)\).\\ Under a rotation by an angle \(\alpha\) about axis \(\hat{n}=(n_1,n_2,n_3)\), the new components \(\vec{X}\) are related to old components \(\vec{x}\) by equation \begin{equation} \vec{X} = \vec{x} -\sin \alpha (\hat{n}\times\vec{x}) + (1-\cos\alpha)\hat{n}\times(\hat{n}\times\vec{x})) \end{equation} We compute \[\hat{n}\times\vec{x}=\big({n_2} {x_3}-{n_3} {x_2},{n_3} {x_1}-{n_1} {x_3},{n_1} {x_2}-{n_2} {x_1}\big)\] \begin{eqnarray} (\hat{n}\times(\hat{n}\times\vec{x}))_1&=&{n_2} ({n_1} {x_2}-{n_2} {x_1})-{n_3} ({n_3} {x_1}-{n_1} {x_3})\\ (\hat{n}\times(\hat{n}\times\vec{x}))_2&=&{n_3} ({n_2} {x_3}-{n_3} {x_2})-{n_1} ({n_1} {x_2}-{n_2} {x_1})\\ (\hat{n}\times(\hat{n}\times\vec{x}))_3&=& {n_1} ({n_3} {x_1}-{n_1} {x_3})-{n_2} ({n_2} {x_3}-{n_3} {x_2}) \end{eqnarray} Therefore \begin{eqnarray}\nonumber X_1&=&(1-\cos \alpha ) ({n_2} ({n_1} {x_2}-{n_2} {x_1})-{n_3} ({n_3} {x_1}-{n_1} {x_3}))-\sin \alpha ({n_2} {x_3}-{n_3} {x_2})+{x_1}\\\nonumber X_2&=&(1-\cos \alpha ) ({n_3} ({n_2} {x_3}-{n_3} {x_2})-{n_1} ({n_1} {x_2}-{n_2} {x_1}))-\sin \alpha ({n_3} {x_1}-{n_1} {x_3})+{x_2}\\\nonumber X_3&=& (1-\cos \alpha ) ({n_1} ({n_3} {x_1}-{n_1} {x_3})-{n_2} ({n_2} {x_3}-{n_3} {x_2}))-\sin \alpha ({n_1} {x_2}-{n_2} {x_1})+{x_3} \end{eqnarray} Therefore \begin{equation} \begin{pmatrix} X_1\\X_2\\X_3 \end{pmatrix} = \underline{\Rbb} \begin{pmatrix} x_1\\x_2\\x_3 \end{pmatrix}. \end{equation} where the matrix \(\Rbb\) is given by \begin{eqnarray}\nonumber \begin{pmatrix} -(1-\cos\alpha)(n_2^2+n_3^2) + 1 & (1-\cos\alpha)n_1n_2 + \sin\alpha n_3 & (1-\cos\alpha)n_3n_1 - \sin\alpha n_2\\ (1-\cos\alpha)n_1 n_2 -n_3\sin\alpha & -(1-\cos\alpha)(n_3^2+n_1^2) +1 & (1-\cos\alpha)n_2n_3 + n_1\sin\alpha\\ (1-\cos \alpha)n_1n_3 + n_2 \sin\alpha & (1-\cos\alpha)n_2n_3 -n_1 \sin\alpha & -(1-\cos\alpha)(n_1^2+n_2^2) + 1 \end{pmatrix} \end{eqnarray} Substituting values \begin{equation*} \hat{n}=\frac{1}{\sqrt{6}}(1,2,1),\quad (1-\cos\alpha)=\frac{2}{5}, \quad\sin\alpha=\frac{4}{5} \end{equation*} and simplifying gives % \begin{equation} \left(\begin{array}{ccc} \frac{2}{3} & \frac{2}{15} \left(1+\sqrt{6}\right) & \frac{1}{15} \left(1-4 \sqrt{6}\right) \\[2mm] \frac{2}{15} \left(1-\sqrt{6}\right) & \frac{13}{15} & \frac{2}{15} \left(1+\sqrt{6}\right) \\[2mm] \frac{1}{15} \left(1+4 \sqrt{6}\right) & \frac{2}{15} \left(1-\sqrt{6}\right) & \frac{2}{3} \end{array} \right) \end{equation} 

shivahcu's picture 22-02-09 08:02:45 n

[QUE/QFT-10003] QFT-PROBLEM

Node id: 4047page


For a real free Klein Gordon field, mass \(m\), compute \[ \matrixelement{0}{\phi(x)\phi(y)}{\vec{k}, \vec{q}}\] and show that the result is properly symmetrized wave function for two identical bosons with momenta \(\vec{q},\vec{p}\). Here \(\ket{\vec{k}, \vec{q}}\) is the state with two bosons with momenta \(\vec{k}, \vec{q}\)

shivahcu's picture 22-02-06 20:02:06 n

[QUE/QFT-01004] QFT-PROBLEM

Node id: 4322page

For second quantized Schrodinger field, show that the Galilean boost \[\int d^3 x\psi^\dagger (m~x+ it \hbar \nabla)\psi,\] is a conserved quantity. How do you interpret this conservation law?

shivahcu's picture 22-02-06 19:02:14 n

[QUE/CM-02012]

Node id: 4414page
shivahcu's picture 22-03-19 11:03:50 n

[QUE/ME-02008] ME-PROBLEM

Node id: 3938page

For a four vector \(x=(\vec{x},x_4)\equiv(x_1,x_2,x_3,x_4)\), define a \(2\times2\) matrix \(M\) by \[M = x_\mu\sigma_\mu= x_4 + \vec{x}\cdot\vec{\sigma}\] where \(\sigma_4\) is \(2\times2\) identity matrix and \(\vec{\sigma}\) are Pauli matrices given by \begin{equation*} \sigma_1=\begin{pmatrix}0&1\\1&0\end{pmatrix},\quad \sigma_1=\begin{pmatrix}0&-i\\i&0\end{pmatrix},\quad \sigma_1=\begin{pmatrix}1&0\\0&-1\end{pmatrix} \end{equation*} Also define a matrix \(U\) by \begin{equation*} U = \cos\frac{\alpha}{2} + i\sin\frac{\alpha}{2}(\hat{n}\cdot\vec{\sigma}) \end{equation*} where \(\hat{n}=(n_1,n_2,n_3)\) is a unit vector.

  • Show that \(U\) is unitary and \(\det U=1\).
  • Prove that \(x_\mu = \frac{1}{2} Tr(\sigma_\mu M)\)
  • Let \(M{'}= U M U^\dagger\) Compute \(x_\mu{'} \) and show that \begin{equation} x_4{'}=x_4; \vec{x}{'}=\vec{x}-\sin\alpha(\hat{n}\times\vec{x}) +(1-\cos\alpha)\hat{n}\times(\hat{n} \times\vec{x}) \end{equation}

The last equation shows that to every rotation in three dimensions there are two \(SU(2)\) matrices given by \(\pm U\).

shivahcu's picture 22-02-07 19:02:14 n

[QUE/ME-14007] ME-PROBLEM

Node id: 3994page

Question

Compute moment of inertia tensor of a space station with solar panels as shown in figure. Let us calculate the inertia tensor for the spacecraft with solar panels illustrated in figure. We will consider the body to be a cylinder and the two panels to be rectangular hexahedra, all of uniform density and of the dimensions indicated in figure.
%FigBelow{10,-35}{70}{0} SolarPanels
Let the \(x\)-axis be the axis of the panel passing through the center of the \(b −c\) face and the \(y\)-axis the symmetry axis of the cylinder. Choose the x-axis to be a principal axis for the cylinder. Let the panels each be inclined at angles \(\pi/2-\theta\) to the generators of the cylinder.

Solution

Let B1 be the cylinder and B2 , B3 the (identical) panels. More in Heard's book.\\ William B Heard, "Rigid Body Mechanics" WILEY-VCH Verlag GmbH & Co. KGaA (2006)

shivahcu's picture 22-02-08 08:02:26 n

[LSN/ME-06001] Potential Problems in One Dimension

Node id: 4131page
shivahcu's picture 22-03-29 20:03:00 n

[QUE/QFT-14003] QFT-PROBLEM

Node id: 4387page

$\newcommand{\matrixelement}[3]{\langle#1|#2|#3\rangle}\newcommand{\dd}[2][]{\frac{d#1}{d#2}}$

For a self coupled scalar theory with interaction Lagrangian density given by

\begin{equation} \mathscr {L}_{\text{int}}= \frac{\lambda}{3!}\phi(x)^3 \end{equation}

Compute and write your answers as integrals of expressions involving propagator in position space.
\begin{eqnarray} (a)&&  \int d^4y_1\int d^4y_2\int d^4y_3 \matrixelement{0}{T(\phi(x_1)\phi(x_2) \mathscr{ L}(y_1) \mathscr {L}(y_2)\mathscr {L}(y_3)}{0} \\ (b) && \int d^4y_1 \int d^4y_2\matrixelement{0}{T(\phi(x_1)\phi(x_2)
\mathscr{L}(y_1) \mathscr{L}(y_2)}{0}. \end{eqnarray}

Draw position space Feynman diagram in each case.

shivahcu's picture 22-02-14 21:02:02 n

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