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Give an account of Heisenberg's Uncertainty principle. Outline an idealised experiment to bring out its significance.

IFoS 2015Paper II4+4=8 marksifos-2015-subject-05-001

Calculate the most probable value of 'r' for an electron in the ground state of the hydrogen atom.

IFoS 2015Paper II10 marksifos-2015-subject-05-004

Find the de Broglie wavelength of a neutron moving with a kinetic energy of 500\text{ eV}. (1\text{ eV} = 1\cdot 602 \times 10^{-19}\text{ J})

IFoS 2015Paper II8 marksifos-2015-subject-05-002

Determine the values of the total angular momentum for a 3d electron.

IFoS 2015Paper II8 marksifos-2015-subject-05-005

Deduce the commutation relations between the components of angular momentum operator \mathbf{L} [L_x, L_y] = i \hbar L_z [L_y, L_z] = i \hbar L_x [L_z, L_x] = i \hbar L_y using the commutation relations [x, p_x] = [y, p_y] = [z, p_z] = i \hbar

IFoS 2015Paper II20 marksifos-2015-subject-05-006

Normalized wave function of a particle is given: \psi(x)=N\exp\left(-\frac{x^2}{2a^2}+ikx\right). Find the expectation value of position.

CSE 2015Paper II10 markscse-2015-subject-05-003

What is Zeeman effect? How can it be understood on the basis of quantum mechanics?

CSE 2015Paper II25 markscse-2015-subject-05-001

Write the time independent Schrödinger equation for a bouncing ball.

CSE 2015Paper II10 markscse-2015-subject-05-004

Solve the Schrödinger equation for a particle in a three-dimensional rectangular potential barrier. Explain the terms degenerate and non-degenerate states in this context.

CSE 2015Paper II30 markscse-2015-subject-05-005

A particle trapped in an infinitely deep square well of width a has a wave function \psi=\left(\frac{2}{a}\right)^{1/2}\sin\left(\frac{\pi x}{a}\right). The walls are suddenly separated by infinite distance. Find the probability of the particle having momentum between p and p+dp.

CSE 2015Paper II10 markscse-2015-subject-05-006

Establish that: hc = 1240\ \mathrm{eV\,nm} = 1240\ \mathrm{MeV\,fm}

CSE 2015Paper II5 markscse-2015-subject-05-007

Derive an expression for the total number of particles N in an ideal Bose gas at any temperature T. Hence, obtain the relation N_0 = N \left[ 1 - \left( \frac{T}{T_0} \right)^{\frac{3}{2}} \right] for the number of particles N_0 in the ground state at T < T_0, the Bose-Einstein condensation temperature, and draw N_0 versus T curve.

IFoS 2015Paper I10+10=20 marksifos-2015-subject-04-004

The vapour pressure of an organic substance is 50\times10^3\ \mathrm{Pa} at 40^{\circ}\mathrm{C}. Its normal boiling point is 80^{\circ}\mathrm{C}. If the substance in vapour phase can be treated like an ideal gas, find the latent heat of vaporization of the substance.

CSE 2015Paper I15 markscse-2015-subject-04-002

For a Van der Waals gas, write down the equation of state. Determine the coefficient of critical expansion \beta.

CSE 2015Paper I15 markscse-2015-subject-04-003

A Van der Waals gas undergoes Joule-Kelvin expansion with a pressure drop of 50\ \mathrm{atm}. If its initial temperature is 300^{\circ}\mathrm{K}, determine its final temperature. (Given Van der Waals constant a=0.136\ \mathrm{Pa\,m^6\,mol^{-1}}, b=36.5\times10^{-6}\ \mathrm{m^3\,mol^{-1}}, C_p=30\ \mathrm{J\,K^{-1}\,mol^{-1}}, R=8.3\ \mathrm{J\,K^{-1}\,mol^{-1}}.)

CSE 2015Paper I10 markscse-2015-subject-04-001

Discuss the consequence following from Joule's free expansion experiments in the context of the internal energy of an ideal gas.

IFoS 2015Paper Iifos-2015-subject-04-001

Start from the equation T dS = C_p dT - T \left( \frac{\partial V}{\partial T} \right)_P dP and get the relation \left( \frac{\partial C_p}{\partial P} \right)_T = -T \left( \frac{\partial^2 V}{\partial T^2} \right)_P Hence, show that the third law of thermodynamics requires for the coefficient of thermal expansion of any substance to vanish at T = 0.

IFoS 2015Paper I5+15=20 marksifos-2015-subject-04-002

Plot the Fermi distribution function versus energy at temperatures T = 0 and T > 0. Explain the nature of the former curve on the basis of the Pauli principle.

IFoS 2015Paper Iifos-2015-subject-04-003

Using Planck's radiation law, deduce Wien's displacement law. How does this law enable one to estimate the surface temperature of the Sun or a star?

CSE 2015Paper I15 markscse-2015-subject-03-010

What are the characteristic features of Rayleigh scattering? A very thin monochromatic beam of light is incident on a particle. Suggest a simple experimental method to ascertain whether the scattering by the particle is of Rayleigh type.

CSE 2015Paper I20 markscse-2015-subject-03-011

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