Notices
 

Browse & Filter

For page specific messages
For page author info
Enter a comma separated list of user names.
2644 records found.
Operations
Selected 20 rows in this page.  
Title+Summary Namesort ascending Date

[QUE/ME-02001] ME-PROBLEM

Node id: 3930page


Show under an infinitesimal rotation of a vector \(\vec{A}\) about an axis \(\hat{n}\) has the form \(\Delta \vec{A}= c \hat{n}\times{\vec{A}}\), where \(c\) is an infinitesimal constant. }
\Hint{Use the fact that lengths and angles do not change under rotations} \QField{Comment}{ When ever you see an equation of the form \(\Delta \vec{A}= c \hat{n}\times{\vec{A}}\), you should realize that some rotation is taking place. Several examples can be given

  1. A electric dipole placed in an electric field will experience a torque and its equation of motion can be written down as\[ \dd[\vec{p}]{t}\propto \vec{p}\times \vec{E}\] and it will tend to rotate.
  2. A similar statement can be made about magnetic dipole in a magentic field.
  3. A related example is that of spin in a uniform magnetic field. The Hamitonian is of the form \(H=-\vec{\mu}\cdot\vec{B}\) and the equation of motion takes the form \[ i\hbar\dd[\vec{S}]{t} = [\vec{S},H]_- \] With magnetic moment being proportional to the spin \(\vec{S}\), the right hand side becomes proportional to \(\vec{B}\times \vec{S}\).
shivahcu's picture 22-02-07 19:02:06 n

[QUE/ME-14001] ME-PROBLEM

Node id: 3987page



Question

A point of rigid body is pivoted in way that the body can rotate freely about a horizontal axis passing thorough the point of suspension. Show that the frequency of small oscillations is given by \[\omega^2= \frac{Mgh}{Mh^2 + I_1n_1^2+I_2n_2^2+I_3n_3^2}\] where \(I_1, I_2, I_3\) are principal moments of inertia about the centre of mass and \(h\) is distance of centre of mass from the point of suspension. Also \(\hat{n}=(n_1,n_2,n_3)\) is unit vector along the axis of rotation and the components of \(\hat{n}\) are taken w.r.t. the principal axes relative to the centre of mass of the body.
%FigBelow{10,-47}{40}{0}{me-fig-14006}

Solution

This is a problem about rotation of a rigid body about a fixed axis. In this case the axis of rotation is horizontal line passes through the point of suspension. The equation of motion is obtained by equating the rate of change of angular momentum to the torque. The angular momentum is \(I\dot{\theta}\), where \(I\) is the moment of inertia about the axis of rotation. The torque is given by \(Mgh\sin\theta\) and is in the clockwise direction of decreasing \(\theta\). Therefore the equation of motion becomes \begin{equation} \dd[L]{t} = - Mgh \sin\theta\\ \end{equation} Substituting \(L=I\dot{\theta}\) and making small amplitude approximation we get \begin{eqnarray} I \ddot{\theta} + Mgh \theta=0\\ \therefore \qquad \qquad \ddot{\theta} + \frac{Mgh}{I} \theta=0. \end{eqnarray} Thus the angular frequency of oscillations is \(\omega^2=\dfrac{Mgh}{I}\). Using the parallel axes theorem the moment of inertia can be written as \begin{equation} I= I_0 + Mh^2 \end{equation} where \(I_0\) is the moment of inertia about a parallel axis passing through the centre of mass. In terms of the principal moments of inertia the value of \(I_0\) is given by \begin{equation} I =I_1n_1^2 + I_2n_2^2 + I_3n_3^2. \end{equation} Thus we get the final answer \begin{equation} \omega^2=\frac{Mgh}{I_0 + I_1n_1^2 + I_2n_2^2 + I_3n_3^2}. \end{equation}

shivahcu's picture 22-02-07 21:02:17 n

[QUE/QFT-15009] QFT-PROBLEM

Node id: 4073page


Assuming interactions of charged pions to be of the form \(\Lsc_\text{int} (x)= (g/4)(\pi(x)^+\pi(x)^-)^2\) find the \(S\) matrix element for \(\pi-\pi\) scattering \[\pi^+ + \pi^- \longrightarrow \pi^+ + \pi^-\] transition probability per unit time per unit volume for \(\pi - \pi\) scattering. Compute the total cross section for the scattering process and show that \[ \frac{d\sigma}{d\Omega}= \frac{g^2}{64\pi^2 E_\text{cm}^2}\]

shivahcu's picture 22-02-06 19:02:45 n

[QUE/QFT-06009] QFT-PROBLEM

Node id: 4369page

Let \(n^\mu\) be a spacelike four vector satisfying \(n^\mu n_\mu=-1\), show that

  • the eigenvalues of \(\gamma_5n\!\!\!/ \) are \(\pm1\).
  • \((\gamma_5 n\!\!\!/)^2 =1\)
  • If \(p^\mu n_\mu=0\), \(p\!\!\!/\) commutes with \(\gamma_5 n\!\!\!/ \)
  • Free particle solutions \(u(p)\) and \(v(p)\) of Dirac equation \[ (p\!\!\!/ -M )u(p)=0, \qquad (p\!\!\!/  + M)v(p)=0\] can also be taken to be eigenvectors of \(\gamma_5 n\!\!\!/   \)  
shivahcu's picture 22-02-04 09:02:19 n

[QUE/CM-02034]

Node id: 4436page
shivahcu's picture 22-03-19 22:03:39 n

LaTeX PRACTICE

Node id: 3865page
shivahcu's picture 20-12-04 19:12:17 n

[QUE/ME-08006] ME-PROBLEM

Node id: 3959page

In equilibrium a pendulum suspended from an inextensible spring in an accelerating car will not hang vertically. The string will make an angle \(\theta\) with vertical see \Figref{me-fig-08002-Q}.\\ \FigBelow{30,20}{50}{70}{me-fig-08002-Q}{Pendulum in accelerating car}\\ Assume that \(g\) is known and the \(\theta\) is measured by an observer sitting in the car. Then without assuming the gravitational and inertial masses to be equal, which of the following quantity can be related to the angle \(\theta\) ?

  • value of acceleration.
  • value of inertial mass.
  • value of gravitational mass.
  • the ratio of gravitational and inertial masses.

Give a short explanation of your answer.

shivahcu's picture 22-02-08 19:02:01 n

[QUE/QFT-04012] QFT-PROBLEM

Node id: 4025page

$\newcommand{\Lsc}{\mathscr L}$

Consider electron proton scattering to be computed in the second quantized Schrodinger theory. The electrostatic interaction can be modeled as \[ V(\mathbf x_1-\mathbf x_2) = -(Ze^2)\int d\mathbf x_1\,d\mathbf x_2 \frac{\rho_e(\mathbf x_1) \rho_p(\mathbf x_2)}{|\mathbf x_1- \mathbf x_2|}\] This interaction suggests the following interaction term in the second quantized Schrodinger theory. \[ \Lsc_\text{int}=\int d\mathbf x_1d\mathbf x_2 \psi^*(\mathbf x_1)\psi(\mathbf x_1) V(\mathbf x_1-\mathbf x_2)\phi^*(\mathbf x_2)\phi(\mathbf x_2) \] where \(\psi ,\phi\) denote the electron and proton fields respectively, and \[V(\mathbf x_1-\mathbf x_2)=-\frac{(Ze^2)}{|\mathbf x_1- \mathbf x_2|}.\] Compute the electron proton scattering cross section in the center of mass frame. Use Yukawa potential \(V(\mathbf x_1-\mathbf x_2)=-V_0\dfrac{ e^{-\mu|\mathbf x_1-\mathbf x_2|}}{|\mathbf x_1- \mathbf x_2|}\) in \(\Lsc_\text{int}\). Show that in the limit \(\mu\to0\), the differential cross section coincides with the Rutherford scattering cross section.

shivahcu's picture 22-02-05 09:02:12 n

[QUE/CM-02006]

Node id: 4409page
shivahcu's picture 22-03-19 16:03:58 n

[QUE/ME-02003] ME-PROBLEM

Node id: 3932page

Show that the rotation matrix for rotation by an angle \(\pi/3\) about the direction \((1,1,1)\) as the axis of rotation is given by \begin{equation} R = \frac{1}{3}\begin{pmatrix} 2 & 2 & -1\\ -1& 2 & 2 \\2 & -1 & 2 \end{pmatrix} \end{equation}Me-que-02003

shivahcu's picture 22-03-24 09:03:42 n

[QUE/ME-14003] ME-PROBLEM

Node id: 3989page

Question

Show that the moment of inertia tensor of a uniform triangular plate, see figure, with centre of mass chosen as origin is given by \begin{equation} I= \frac{mL^2}{18} \begin{pmatrix} 1 & -\frac{1}{2} & 0\\ -\frac{1}{2} & 1 & 0\\ 0 & 0 & 2 \end{pmatrix}\end{equation} 


Solution

In % Figref{me-fig-14012} OAB is the right angle triangle lamina with two sides of equal length \(L\). We choose the coordinate axes as shown in the figure. The corners of the plate are \((0,0,0),(L,0,0),(l,l,0)\) and the centre of mass has coordinates \((\frac{2L}{3},\frac{L}{3}, 0)\). It is easy to calculate the moment of inertia tensor w.r.t. this set of axes. The inertia tensor relative to the centre of mass will then be found by making use of parallel axes theorem.
% FigBelow{10,-14}{40}{00}{me-fig-14012} Choice of axes
Simplest way to solve the problem is to use double integral. Divide the plate into small rectangular elements as shown, obtain contribution of one such element and perform integrations over a range of \(x\) and \(y\) so as to get sum over all the rectangular elements of the plate. Let the mass per unit area of the plate be \(\sigma\), then \(M=\frac{1}{2}\sigma L^2.\) We first record the expression for moment of inertia tensor for a rigid body consisting of masses \(m_\alpha\) at position \(\vec{r}_\alpha\). \begin{eqnarray} I_{xx} &=& \sum_\alpha m_\alpha \big( \vec{r}\,^2- x_\alpha^2\big) =\sum_\alpha m_\alpha \big( y_\alpha^2+ z_\alpha^2\big)\\ I_{yy} &=& \sum_\alpha m_\alpha \big( \vec{r}\,^2_\alpha- y_\alpha^2\big) =\sum_\alpha m_\alpha \big(x_\alpha^2+ z_\alpha^2\big)\\ I_{zz} &=& \sum_\alpha m_\alpha \big( \vec{r}\,^2_\alpha- z_\alpha^2\big) =\sum_\alpha m_\alpha \big(y_\alpha^2+ z_\alpha^2\big) \end{eqnarray} The contribution of the element \(dx\, dy\) at position \(x,y\) to \(I_{xx}\) is easily written down as, remembering that for points on the plate \(z=0\), we get \begin{eqnarray} dI_{xx}= (\sigma dx\,dy)(\vec{r}^2-x^2) = (\sigma dx\,dy) y^2. \end{eqnarray} For a fixed \(x\), the variable \(y\) takes values from 0 to \(x\) and for the plate \(x\) ranges from 0 to \(L\). Therefore \(I_{xx}\) is given by \begin{eqnarray} I_{xx} &=& \int_0^L dx \int_0^x dy \sigma y^2 = \sigma\int_0^L dx \frac{x^3}{3} = \frac{\sigma L^4}{12} \\ &=& \frac{1}{6}M L^2, \qquad \qquad \because \sigma L^2 =2M. \end{eqnarray} The expression for moment of inertia \(I_{yy}\) \begin{equation} I_{yy} = \sum_\alpha m_\alpha (\vec{r}_\alpha^2 -y_\alpha^2) \end{equation} for the planer lamina problem takes the form \begin{eqnarray} I_{yy} &=& \int_0^L dx \int_0^x dy (\sigma x^2) = \int_0^L dx\, (\sigma {x^2})\times y\Big|_{y=0}^{y=x} = \frac{\sigma L^4}{4}\\ &=& \frac{ML^2}{2}. \end{eqnarray} and \(I_{zz}\) is given by \begin{eqnarray} I_{zz} &=& \int_0^L dx \int_0^x dy \sigma (x^2 + y^2) = \int_0^L \sigma (x^2 y + \frac{y^3}{3})\Big|_{y=0}^{y=x}\\ &=& \int_0^L dx \sigma \frac{4x^3}{3}= \sigma \frac{L^4}{3}\\ &=& \frac{2ML^2}{3}. \end{eqnarray} The off diagonal term \(I_{xy}\) is nonzero and is given by \begin{eqnarray} I_{xy} &=& -\int_0^L dx \int_0^L dy \sigma (\sigma x)\,y = -\int_0^L dx (\sigma x) \times \frac{y^2}{2}\Big|_{y=0}^{y=x}\\ & =& -\int_0^L dx \sigma \frac{x^3}{8} = - \sigma \frac{L^2}{8}\\ &=& - \frac{M L^2}{4}. \end{eqnarray} The parallel axis theorem gives \begin{eqnarray} I^\text{cm}_{jk}= I_{jk} - M (|\vec{a}|^2 \delta_{jk}-a_j a_k) \end{eqnarray} where \(\vec{a}\) is the position vector of the origin \(O\) relative to the centre of mass. In the present case the centre of mass has coordinates \((2L/3,L/3,0)\). Therefore \(\vec{a} = (-2L/3, -L/3,0)\). Thus we get \begin{eqnarray} I^\text{cm}_{xx} &=& I_{xx} - M (L^2/9) = (\frac{1}{6}-\frac{1}{9})ML^2 =\frac{ML^2}{18}\\ I^\text{cm}_{yy} &=& I_{yy} - M (4 L^2/9) = (\frac{1}{2}-\frac{4}{9})ML^2 =\frac{ML^2}{18}\\ I^\text{cm}_{zz}&=& I_{zz} - ML^2{(1+4)L^3}{9} = (\frac{2}{3}-\frac{5}{9})ML^2 = \frac{ML^2}{9}\\ I^\text{cm}_xy &=& I_{xy} -a_xa_y = - \frac{ML^2}{4} -\frac{2ML^2}{9} =(\frac{1}{4}-\frac{2}{9}) ML^2\\ &=& -\frac{ML^2}{36}. \end{eqnarray} Thus the moment of inertia tensor relative to the centre of mass is given by \begin{equation*} \underline{\sf I}=\frac{ML^2}{18} \begin{pmatrix} 1 & -\frac{1}{2} & 0 \\ -\frac{1}{2} & 1 & 0 \\ 0 & 0 & 2 \end{pmatrix} \end{equation*}

shivahcu's picture 22-02-07 21:02:57 n

[QUE/QFT-15011] QFT-PROBLEM

Node id: 4075page

Write the Lagrangian for a nonrelativistic particle moving in a potential \(V(r)\). Using the second quantized formalism compute the scattering cross section in the lowest order in the potential. Show that this result is same as the first Born approximation expression in nonrelativistic, first quantized formulation of quantum mechanics. Taking V(r) as Coulomb potential obtain the Rutherford formula

shivahcu's picture 22-02-06 20:02:32 n

[QUE/QFT-06011] QFT-PROBLEM

Node id: 4371page

Write the transformation properties of free Dirac field of under a Lorentz boost by velocity \(vec{v}=v(0,0,1)\). Show that the Dirac wave function for a particle with momentum \(\vec{p}=p(0,0,1)\) and mass \(m\) can be obtained by applying an appropriate boost on wave function for a particle at rest. Demonstrate this only for positive energy solution with spin along \(z\)-axis

shivahcu's picture 22-02-04 21:02:35 n

[QUIZ/CM-05001]

Node id: 4440page
shivahcu's picture 22-03-31 09:03:20 n

tabs and accordion practise

Node id: 3869page
shivahcu's picture 20-12-06 16:12:13 n

[QUE/ME-08008] ME-PROBLEM

Node id: 3961page

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. [10+10]
shivahcu's picture 22-02-09 08:02:40 n

[QUE/QFT-04014] QFT-PROBLEM

Node id: 4027page



For the classical Schrodinger field\(\psi(x)\) calculate the following Poisson brackets.

  • \(\{N, \psi\}_\text{PB}\) 
  • \(\{ \psi, \Hca\}_\text{PB}\)
  • \(\{\Pca, \psi\}_\text{PB}\) 
  • \(\{\Pca, \Hca\}_\text{PB}\)

where \(N,\Pca\) and \(\Hca\), respectively, are the momentum and the Hamiltonian of the Schrodinger field. \begin{eqnarray}\nonumber N &=&\int \psi^*(x)\psi(x)\, dx; \qquad \Pca = -i\hbar\int\, dx \psi^*(x) \nabla \psi(x)\\\nonumber \Hca &=& \int \Big\{ \frac{\hbar^2}{2m}(\nabla\psi(x))^*(\nabla \psi(x)) + \psi^*(x)V(x)\psi(x)\Big\}. \end{eqnarray}

shivahcu's picture 22-02-05 22:02:41 n

[QUE/CM-02008]

Node id: 4411page
shivahcu's picture 22-03-19 17:03:25 n

[QUE/ME-02005] ME-PROBLEM

Node id: 3934page

Question

 Using the definition of Levi-Civita and Kronecker delta symbols to prove the following identity \begin{eqnarray}\label{EQ01} \epsilon_{i\,j\,k}\,\epsilon_{l\,m\,n}\ &=&\ \begin{vmatrix} \delta_{il}&\delta_{im}&\delta_{in}\\ \delta_{jl}&\delta_{jm}&\delta_{jn}\\ \delta_{kl}&\delta_{km}&\delta_{kn} \end{vmatrix} \end{eqnarray} 

Solution

Interchanging \(i\leftrightarrow j\) in the right hand side amounts to interchange of the first and second rows and therefore the right hand side changes sign. Similar statement holds for exchange of \(i\leftrightarrow k\) and \(i\leftrightarrow k\). Thus the hand side is completely antisymmetric in indices \(i,j,k\). Repeating the above argument we see that the right hand side is totally antisymmetrc in indices \(\ell, m, n \) also. Thus the right hand side must be proportional to \(\epsilon_{i\,j\,k}\,\epsilon_{l\,m\,n}\). Thus \begin{equation} \text{R.H.S. of \eqRef{EQ01}} = K \epsilon_{i\,j\,k}\,\epsilon_{l\,m\,n}\label{EQ02} \end{equation} The constant of proportionality \(K\) is fixed by substituting \(i=1,j=2,k=3, \ell=1, m=2, n=3\) in \eqRef{EQ02}. The right hand side of \eqRef{EQ01} becomes determinant of unit matix and hence equal to 1. The right hand side of \eqRef{EQ02} becomes \(K \epsilon_{123}\epsilon_{123}=K\). This gives \(K=1\) and the proof of \eqRef{EQ01} is complete.

Me-que-02005

shivahcu's picture 22-02-07 19:02:39 n

[QUE/ME-14004] ME-PROBLEM

Node id: 3991page

Question

Three equal masses, connected by light rods, are placed at the vertices of a right angle triangle as shown in figure. The origin of the coordinate system is chosen to coincide with the centre of mass of the system. Obtain the values of moment of inertia tensor components. 

Solution

Method 1:
Let the coordinates of the vertices \(A,B,C\) be \((a,b,0)\), \((a+h,b,0)\) and \((a+h,b+h,0)\). Since the centre of mass is at the origin and all the masses are equal \begin{eqnarray}\nonumber a+(a+h)+(a+h)=0 \Longrightarrow a=-2h/3\\ b+b + b+h=0 \Longrightarrow b=-h/3. \end{eqnarray} Therefore the coordinates of the points \(A,B,C\) are \[\vec{x}_1=(-2h/3, -h/3,0), \vec{x_2}=(h/3,-h/3,0), \vec{x_3}=(h/3, 2h/3). \] The moment of inertia tensor is given by \begin{equation} I_{jk} = \sum m_\alpha ( |\vec{x}_\alpha|^2\delta_{jk} - a_ja_k ). \end{equation} It is obvious that \(I_{13}=I_{31}=I_{23}=I_{32}=0\). Since the inertia tensor is symmetric we need to compute only \(I_{11}, I_{22}, I_{33}\) and \(I_{12}\). Let us write the values needed in a tabular form \begin{equation} \begin{array}{crrcrrrrr} \hline & & & & & \\ \text{Location} & x_1 &\quad x_2 & \quad x_3 & x_1^2 &x_2^2&\quad|\vec{x}|^2 & \quad x_1x_2\\[1mm] A & -\dfrac{2h}{3} & -\dfrac{h}{3} & 0 &\dfrac{4h^2}{9} & \dfrac{h^2}{9}& \dfrac{5h^2}{9}&\dfrac{2h^2}{9} \\[2mm] B & \dfrac{h}{3} & -\dfrac{h}{3} & 0 & \dfrac{h^2}{9}& \dfrac{h^2}{9}&\dfrac{2h^2}{9}&-\dfrac{h^2}{3}\\[2mm] C & \dfrac{h}{3} & \dfrac{2h}{3} & 0 & \dfrac{h^2}{9}&\dfrac{4h^2}{9}& \dfrac{5h^2}{9} & \dfrac{2h^2}{9}\\[3mm] \hline &&&&&&&&\\[-1mm] \sum_\alpha(.) & ... & ... & ... & \dfrac{6h^2}{9} & \dfrac{6h^2}{9} & \dfrac{12h^2}{9} & \dfrac{3h^2}{9} \\[2mm] \hline \end{array} \end{equation} We are now ready to compute the moment of inertia tensor \begin{eqnarray} I_11 &=&m \sum_\alpha \{|x_\alpha|^2 - x_{\alpha1}x_{\alpha1}\} =m\big(\frac{12h^2}{9} - \frac{6h^2}{3}=\frac{2mh^2}{3}\big) = \frac{2mh^2}{3} \\ I_22 &=&m \sum_\alpha \{|x_\alpha|^2 - x_{\alpha2}x_{\alpha2}\} =m\Big(\frac{12h^2}{9} - \frac{6h^2}{3}\Big) = \frac{2mh^2}{3} = \\ I_{33} &=& m\sum_\alpha \{|x_\alpha|^2 - x_{\alpha3}x_{\alpha3}\} =\frac{12mh^2}{9}-0= \frac{4mh^2}{3} \end{eqnarray} \FigBelow{-05,0}{50}{40}{me-fig-14008A}{\(K{'}\) axes} \FigBelow{15,0}{50}{40}{me-fig-14008B}{\(K{'}\) axes}\\

Method 2 :

Choose a convenient set of axes:
We translate the axes from the given origin to vertex \(B\), as shown in
%Figref{me-fig-14008B}. With respect to prime axes, the coordinates of the three vertices \(A,B,C\) are \((-h,0,0),(0,0,0)\) and \((h,0,0)\). Therefore the components of moment of inertia tensor are given by \begin{equation} I_{11}{'}= mh^2, \quad I_{22}=mh^2, \quad I_{33}=2mh^2. \end{equation} All other components are zero. \begin{equation} I{'}_{12}=I{'}_{21}=0, \quad I{'}_{23}=I{'}_{32}=0, \quad I{'}_{31}=I{'}_{13}=0. \end{equation} Now we use parallel axes theorem to get the moment of inertia tensor components w.r.t. the given set with origin at the centre of mass. The coordinates of centre of mass in \(K{'} \) system are given by \(\vec{a}=(h/3,h/3,0)\), and the total mass is \(M=3m\).\\ \noindent To use the parallel axes theorem \begin{equation} I_{jk}= I{'}_{jk} - M ( |a|^2 -a_ja_k), \end{equation} we record the following values computation of inertia tensor. \[|\vec{a}|^2= \frac{2h^2}{9}\qquad |a|^2 -a_1^2= |a|^2-a_2^2= \frac{h^2}{9}, \qquad a_1a_2= \frac{h^2}{9} , \qquad a_1a_3=a_2a_3=0 \] We are now ready to have the answers \begin{eqnarray}\nonumber I_{11} &=&I{'}_{11} - M ( |a|^2 -a_1^2) = mh^2 - (3m) \frac{h^2}{9} = \frac{2mh^2}{3} \\\nonumber I_{22} &=&I{'}_{22} - M ( |a|^2 -a_2^2) = mh^2 - (3m) \frac{h^2}{9} = \frac{2mh^2}{3} \\\nonumber I_{33}&=&I{'}_{33} - M ( |a|^2 -a_3^2) = 2mh^2 -3m \frac{2h^2}{9} = \frac{4mh^2}{3}\\\nonumber I_{12}&=& I{'}_{12} + M ( |a|^2 -a_1a_2) = -(3m)\,\frac{h^2}{9} = -\frac{mh^2}{3}\\\nonumber I_{21}&=&I_{12}=-(3m)\frac{h^2}{9}=-\frac{mh^2}{3}. \end{eqnarray} All other off diagonal components are zero. Thus the inertia tensor is given by \begin{equation} I =\begin{pmatrix} \dfrac{2mh^2}{3} & -\dfrac{mh^2}{3} & 0\\[1.5mm] -\dfrac{mh^2}{3} & \dfrac{2mh^2}{3} & 0\\[1.5mm] 0 & 0 & \dfrac{4mh^2}{3} \end{pmatrix}. \end{equation}

shivahcu's picture 22-02-07 21:02:54 n

Pages

 
X