Quantum Statistics CSIR

Q.No:1 CSIR Dec-2014

An ideal Bose gas is confined inside a container that is connected to a particle reservoir. Each particle can occupy a discrete set of single-particle quantum states. If the probability that a particular quantum state is unoccupied is \(0.1\), then the average number of bosons in that state is
(1) \(8\)
(2) \(9\)
(3) \(10\)
(4) \(11\)

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Option 2

Q.No:2 CSIR June-2015

An ideal Bose gas in d-dimensions obeys the dispersion relation \(\in (\overrightarrow{k}) = Ak^{s}\) where \(A\) and \(s\) are constants. For Bose-Einstein condensation to occur, the occupancy of excited states \(N_{e}=c \int_{0}^{\infty} \frac{\epsilon^{(d-s) / s}}{e^{\beta(\epsilon-\mu)}-1} d \epsilon\) Where \(c\) is a constant, should remain finite even for \(\mu = 0\). This can happen if
(1) \(\frac{d}{s} < \frac{1}{4}\)
(2) \(\frac{1}{4} < \frac{d}{s}<\frac{1}{2}\)
(3) \(\frac{d}{s} > 1\)
(4) \(\frac{1}{2} < \frac{d}{s}<1\)

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Option 3

Q.No:3 CSIR June-2015

The low-energy electronic excitations in a two-dimensional sheet of graphene is given by \(E(\vec{k})=\hbar v k\) where \(v\) is the velocity of the excitations. The density of states is proportional to
(1) \(E\)
(2) \(E^{3/2}\)
(3) \(E^{1/2}\)
(4) \(E^2\)

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Option 1

Q.No:4 CSIR Dec-2015

A thin metal film of dimension \(2 \text{ mm}\times 2 \text{ mm}\) contains \(4\times 10^{12}\) electrons. The magnitude of the Fermi wavevector of the system, in the free electron approximation, is
(1) \(2\sqrt{\pi}\times 10^7 \text{ cm}^{-1}\)
(2) \(\sqrt{2\pi}\times 10^7 \text{ cm}^{-1}\)
(3) \(\sqrt{\pi}\times 10^7 \text{ cm}^{-1}\)
(4) \(2\pi\times 10^7 \text{ cm}^{-1}\)

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Option 2

Q.No:5 CSIR June-2016

Suppose the frequency of phonons in a one-dimensional chain of atoms is proportional to the wavevector. If \(n\) is the number density of atoms and \(c\) is the speed of the phonons, then the Debye frequency is
(1) \(2\pi cn\)
(2) \(\sqrt{2}\pi cn\)
(3) \(\sqrt{3}\pi cn\)
(4) \(\pi cn/2\)

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Option 1

Q.No:6 CSIR June-2016

Consider electrons in graphene, which is a planar monatomic layer of carbon atoms. If the dispersion relation of the electrons is taken to be \(\varepsilon(k)=ck\) (where \(c\) is constant) over the entire \(k\)-space, then the Fermi energy \(\varepsilon_F\) depends on the number density of electrons \(\rho\) as
(1) \(\varepsilon_F \propto \rho^{1/2}\)
(2) \(\varepsilon_F \propto \rho\)
(3) \(\varepsilon_F \propto \rho^{2/3}\)
(4) \(\varepsilon_F \propto \rho^{1/3}\)

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Option 1

Q.No:7 CSIR Dec-2016

The electrons in graphene can be thought of as a two-dimensional gas with a linear energy-momentum relation \(E=|\vec{p}|v\), where \(\vec{p}=(p_x, p_y)\) and \(v\) is a constant. If \(\rho\) is the number of electrons per unit area, the energy per unit area is proportional to
(1) \(\rho^{3/2}\)
(2) \(\rho\)
(3) \(\rho^{1/3}\)
(4) \(\rho^{2}\)

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Option 1

Q.No:8 CSIR June-2017

A gas of photons inside a cavity of volume \(V\) is in equilibrium at temperature \(T\). If the temperature of the cavity is changed to \(2T\), the radiation pressure will change by a factor of
(1) \(2\)
(2) \(16\)
(3) \(8\)
(4) \(4\)

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Option 2

Q.No:9 CSIR June-2017

The single particle energy levels of a non-interacting three-dimensional isotropic system, labelled by momentum \(k\), are proportional to \(k^3\). The ratio \(\bar{P}/\epsilon\) of the average pressure \(\bar{P}\) to the energy density \(\epsilon\) at a fixed temperature, is
(1) \(1/3\)
(2) \(2/3\)
(3) \(1\)
(4) \(3\)

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Option 3

Q.No:10 CSIR Dec-2017

The dispersion relation of a gas of spin-\(\frac{1}{2}\) fermions in two dimensions is \(E=\hbar v|\vec{k}|\), where \(E\) is the energy, \(\vec{k}\) is the wave vector and \(v\) is a constant with the dimension of velocity. If the Fermi energy at zero temperature is \(\epsilon_F\), the number of particles per unit area is
(1) \(\epsilon_F/(4\pi v\hbar)\)
(2) \(\epsilon_F^3/(6\pi^2 v^3 \hbar^2)\)
(3) \(\pi\epsilon_F^{3/2}/(3v^3 \hbar^3)\)
(4) \(\epsilon_F^2/(2\pi v^2 \hbar^2)\)

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Option 4

Q.No:11 CSIR Dec-2017

Consider a quantum system of non-interacting bosons in contact with a particle bath. The probability of finding no particle in a given single particle quantum state is \(10^{-6}\). The average number of particles in that state is of the order of
(1) \(10^3\)
(2) \(10^6\)
(3) \(10^9\)
(4) \(10^{12}\)

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Option 2

Q.No:12 CSIR Dec-2017

A metallic nanowire of length \(l\) is approximated as a one-dimensional lattice of \(N\) atoms with lattice spacing \(a\). If the dispersion of electrons in the lattice is given as \(E(k)=E_0-2t\cos{ka}\), where \(E_0\) and \(t\) are constants, then the density of states inside the nanowire depends on \(E\) as
(1) \(N^3 \sqrt{\frac{t^2}{E-E_0}}\)
(2) \(\sqrt{\left(\frac{E-E_0}{2t}\right)^2-1}\)
(3) \(N^3 \sqrt{\frac{E-E_0}{t^2}}\)
(4) \(\frac{N}{\sqrt{(2t)^2-(E-E_0)^2}}\)

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Option 4

Q.No:13 CSIR June-2018

The number of ways of distributing \(11\) indistinguishable bosons in \(3\) different energy levels is
(1) \(3^{11}\)
(2) \(11^3\)
(3) \(\frac{(13)!}{2!(11)!}\)
(4) \(\frac{(11)!}{3!8!}\)

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Option 3

Q.No:14 CSIR Dec-2018

The heat capacity \(C_V\) at constant volume of a metal, as a function of temperature, is \(\alpha T+\beta T^3\), where \(\alpha\) and \(\beta\) are constants. The temperature dependence of the entropy at constant volume is
(1) \(\alpha T+\frac{1}{3}\beta T^3\)
(2) \(\alpha T+\beta T^3\)
(3) \(\frac{1}{2}\alpha T+\frac{1}{3}\beta T^3\)
(4) \(\frac{1}{2}\alpha T+\frac{1}{4}\beta T^3\)

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Option 1

Q.No:15 CSIR Dec-2018

Consider an ideal Fermi gas in a grand canonical ensemble at a constant chemical potential. The variance of the occupation number of the single particle energy level with mean occupation number \(\bar{n}\) is
(1) \(\bar{n}(1-\bar{n})\)
(2) \(\sqrt{\bar{n}}\)
(3) \(\bar{n}\)
(4) \(\frac{1}{\sqrt{\bar{n}}}\)

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Option 1

Q.No:16 CSIR Dec-2018

At low temperatures, in the Debye approximation, the contribution of the phonons to the heat capacity of a two-dimensional solid is proportional to
(1) \(T^2\)
(2) \(T^3\)
(3) \(T^{1/2}\)
(4) \(T^{3/2}\)

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Option 1

Q.No:17 CSIR Dec-2018

The dispersion relation of optical phonons in a cubic crystal is given by \(\omega(k)=\omega_0-ak^2\) where \(\omega_0\) and \(a\) are positive constants. The contribution to the density of states due to these phonons with frequencies just below \(\omega_0\) is proportional to
(1) \((\omega_0-\omega)^{1/2}\)
(2) \((\omega_0-\omega)^{3/2}\)
(3) \((\omega_0-\omega)^{2}\)
(4) \((\omega_0-\omega)\)

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Option 1

Q.No:18 CSIR Dec-2019

Consider black body radiation in thermal equilibrium contained in a two-dimensional box. The dependence of the energy density on the temperature \(T\) is
(1) \(T^3\)
(2) \(T\)
(3) \(T^2\)
(4) \(T^4\)

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Option 1

Q.No:19 CSIR Dec-2019

For \(T\) much less than the Debye temperature of copper, the temperature dependence of the specific heat at constant volume of copper, is given by (in the following \(a\) and \(b\) are positive constants)
(1) \(aT^3\)
(2) \(aT+bT^3\)
(3) \(aT^2+bT^3\)
(4) \(\exp{\left(-\frac{a}{k_B T}\right)}\)

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Option 2

Q.No:20 Assam CSIR Dec-2019

Two spheres are subjected to black-body radiation at temperatures \(T_1\) and \(T_2\) respectively. For the first sphere only half of its surface is exposed to the radiation, while the full surface of the second sphere is exposed. The ratio of the radii of the spheres are \(R_1/R_2=2\). If the forces due to radiation pressure on the two spheres are the same, the ratio \(T_1/T_2\) is
(1) \(2^{1/4}\)
(2) \(1/\sqrt{2}\)
(3) \(1\)
(4) \(1/2^{1/4}\)

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Option 4

Q.No:21 CSIR June-2020

The temperatures of two perfect black bodies \(A\) and \(B\) are \(400 K\) and \(200 K\), respectively. If the surface area of \(A\) is twice that of \(B\), the ratio of total power emitted by \(A\) to that by \(B\) is
(a) \(4\)
(b) \(2\)
(c) \(32\)
(d) \(16\)

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Option c

Q.No:22 CSIR June-2020

Spin \(\frac{1}{2}\) fermions of mass \(m\) and \(4m\) are in a harmonic potential \(V(x)=\frac{1}{2}kx^2\). Which configuration of \(4\) such particles has the lowest value of the ground state energy?
(a) \(4\) particles of mass \(m\)
(b) \(4\) particles of mass \(4m\)
(c) \(1\) particle of mass \(m\) and \(3\) particles of mass \(4m\)
(d) \(2\) particles of mass \(m\) and \(2\) particles of mass \(4m\)

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Option d

Q.No:23 CSIR Feb-2022

The volume and temperature of a spherical cavity filled with black body radiation are \(V\) and \(300K\) , respectively. If it expands adiabatically to a volume \(2V\) , its temperature will be closest to
(1) \(150\) K
(2) \(300\) K
(3) \(250\) K
(4) \(240\) K

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Option 4

Q.No:24 CSIR Feb-2022

The total number of phonon modes in a solid of volume \(V\) is \(\int_0^{\omega_D}g(\omega)d\omega=3N\), is the number of primitive cells, \(\omega_D\) is the Debye frequency and density of photon modes is \(g(\omega)=AV\omega^2\) (with A>0 a constant). If the density of the solid doubles in a phase transition, the Debye temperature \(\Theta_D\) will
(1) increase by a factor of \(2^{2/3}\)
(2) increase by a factor of \(2^{1/3}\)
(3) decrease by a factor of \(2^{2/3}\)
(4) decrease by a factor of \(2^{1/3}\)

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Option 2

Q.No:25 CSIR Feb-2022

The dispersion relation of a gas of non-interacting bosons in d dimensions \(E(k)=ak^s\) where \(a\) and \(s\) are positive constants, Bose-Einstein condensation will occur for all values of
(1) \(d>s\)
(2) \(d+2>s>d-2\)
(3) \(s>2\) independent of \(d\)
(4) \(d>2\) independent of \(s\)

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Option 1

Q.No:26 CSIR Sep-2022

The energy levels of a system, which is in equilibrium at temperature \(T=1/k_B \beta\), are 0, \(\epsilon\), and \(2\epsilon\). If two identical bosons occupy these energy levels, the probability of the total energy being \(3\epsilon\) is
(1) \(\frac{e^{-3\beta\epsilon}}{1+e^{-\beta\epsilon}+e^{-2\beta\epsilon}+e^{-3\beta\epsilon}+e^{-4\beta\epsilon}}\)
(2) \(\frac{e^{-3\beta\epsilon}}{1+2e^{-\beta\epsilon}+2e^{-2\beta\epsilon}+e^{-3\beta\epsilon}+e^{-4\beta\epsilon}}\)
(3) \(\frac{e^{-3\beta\epsilon}}{e^{-\beta\epsilon}+2e^{-2\beta\epsilon}+e^{-3\beta\epsilon}+e^{-4\beta\epsilon}}\)
(4) \(\frac{e^{-3\beta\epsilon}}{1+e^{-\beta\epsilon}+2e^{-2\beta\epsilon}+e^{-3\beta\epsilon}+e^{-4\beta\epsilon}}\)

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Option 4

Q.No:27 CSIR June-2023

The single particle energies of a system of \(N\) non-interacting fermions of spin \(s\) (at \(T=0\)) are \(E_n=n^2E_0\), \(n=1,2,3...\). The ratio \(\epsilon_F(\frac{3}{2})/\epsilon_F(\frac{1}{2})\) of the Fermi energies for fermions of spin \(3/2\) and spin \(1/2\), is
1) \(1/2\)
2) \(1/4\)
3) \(2\)
4) \(1\)

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Option 2

Q.No:28 CSIR June-2023

The energy levels available to each electron in a system of \(N\) non-interacting electrons are \(E_n=nE_0\) , \(n=0,1,2,...\). A magnetic field, which does not affect the energy spectrum, but completely polarizes the electron spins, is applied to the system. The change in the ground state energy of the system is
1) \(\frac{1}{2}N^2E_0\)
2) \(N^2E_0\)
3) \(\frac{1}{8}N^2E_0\)
4) \(\frac{1}{4}N^2E_0\)

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Option 4

Q.No:29 CSIR June-2023

The dispersion relation of a gas of non-interacting bosons in two dimensions is \(E(k)=c\sqrt{|k|}\), where \(c\) is a positive constant. At low temperatures, the leading dependence of the specific heat on temperature \(T\), is
1) \(T^4\)
2) \(T^3\)
3) \(T^2\)
4) \(T^{3/2}\)

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Option 1

Q.No:30 CSIR June-2023

The dispersion relation of electrons in three dimensions is \(\epsilon(k)=\hbar v_Fk\), where \(v_F\) is the Fermi velocity. If at low temperatures (\(T<<T_F\)) the Fermi energy \(\epsilon_F\) depends on the number density \(n\) as \(\epsilon_F(n)\sim n^\alpha\), the value of \(\alpha\) is
1) \(1/3\)
2) \(2/3\)
3) \(1\)
4) \(3/5\)

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Option 1

Q.No: 31 CSIR june-2023

Two electrons in thermal equilibrium at temperature \(T=k_B/\beta\) can occupy two sites. The energy of the configuration in which they occupy the different sites is \(J\textbf{S}_1\cdot\textbf{S}_2\) (where \(J>0\) is a constant and \(\textbf{S}\) denotes the spin of an electron), while it is \(U\) if they are at the same site. If \(U=10J\), the probability for the system to be in the first excited state is
1) \(e^{-3\beta J/4}/(3e^{\beta J/4}+e^{-3\beta J/4}+2e^{-10\beta J})\)
2) \(3e^{-\beta J/4}/(3e^{-\beta J/4}+e^{3\beta J/4}+2e^{-10\beta J})\)
3) \(e^{-\beta J/4}/(2e^{-\beta J/4}+3e^{3\beta J/4}+2e^{-10\beta J})\)
4) \(3e^{-3\beta J/4}/(2e^{\beta J/4}+3e^{-3\beta J/4}+2e^{-10\beta J})\)

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Option 2

Q.No: 32 CSIR Dce-2023

Each allowed energy level of a system of non-interacting fermions has a degeneracy \( M \). If there are \( N \) fermions and \( R \) is the remainder upon dividing \( N \) by \( M \), then the degeneracy of the ground state is
1) \( R^M \)
2) 1
3) \( M \)
4) \( ^MC_R \)

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Option 4

Q.No: 33 CSIR Dce-2023

A system of non-relativistic and non-interacting bosons of mass \(m\) in two dimensions has a density \(n\). The Bose-Einstein condensation temperature \(T_c\) is
1) \(\frac{12\hbar^2n}{\pi mk_B}\)
2) \(\frac{3\hbar^2n}{\pi mk_B}\)
3) \(\frac{6\hbar^2n}{\pi mk_B}\)
4) \(0\)

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Option 4

Q.No: 34 CSIR Dce-2023

Four distinguishable particles fill up energy levels \(0, \varepsilon, 2\varepsilon\). The number of available microstates for the total energy \(4\varepsilon\) is
1) 20
2) 24
3) 11
4) 19

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Option 4

Q.No: 35 CSIR June-2024

The Debye temperature of a two-dimensional insulator is \(150 \, K\). The ratio of the heat required to raise its temperature from \(1 \, K\) to \(2 \, K\) and from \(2 \, K\) to \(3 \, K\) is
1) \(7:19\)
2) \(3:13\)
3) \(1:1\)
4) \(3:5\)

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Option 1

Q.No: 36 CSIR June-2024

The Debye temperature of a two-dimensional insulator is \(150 \, K\). The ratio of the heat required to raise its temperature from \(1 \, K\) to \(2 \, K\) and from \(2 \, K\) to \(3 \, K\) is
1) \(7:19\)
2) \(3:13\)
3) \(1:1\)
4) \(3:5\)

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Option 1

Q.No: 37 CSIR Dec-2024

For an ideal Bose gas, the density of states is given by \(\rho(E) = C E^{2}\), where \(C\) is a positive constant. Assume that the number of bosons is not conserved. The variation of the specific heat of the gas with temperature \(T\) is closest to
1) \(T^{2}\)
2) \(T^{3}\)
3) \(T\)
4) \(T^{4}\)

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Option 2

Q.No: 38 CSIR Dec-2024

A spherical cavity of volume \(V\) is filled with thermal radiation at temperature \(T\). The cavity expands adiabatically to 8 times its initial volume. If \(\sigma\) is Stefan’s constant and \(c\) is the speed of light in vacuum, what is the closest value of the work done in the process?
1) \(8 \left(\frac{\sigma T^{4} V}{c}\right)\)
2) \(4 \left(\frac{\sigma T^{4} V}{c}\right)\)
3) \(\frac{1}{2} \left(\frac{\sigma T^{4} V}{c}\right)\)
4) \(2 \left(\frac{\sigma T^{4} V}{c}\right)\)

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Option 4

Q.No: 39 CSIR Dec-2024

Consider a free fermion gas in a hypercubic infinite potential well in hypothetical 4-dimensional space. What is the expression for the ground state energy per particle in terms of the Fermi energy \(E_{F}\)? (Ignore spin degeneracy of the fermions)
1) \(\frac{4}{5} E_{F}\)
2) \(\frac{2}{3} E_{F}\)
3) \(\frac{1}{3} E_{F}\)
4) \(\frac{2}{5} E_{F}\)

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Option 2

Q.No: 40 CSIR Dec-2024

Bose condensation experiments are carried out on two samples A and B of an ideal Bose gas. The same gas species is used in both. The condensate densities achieved at a given temperature below the critical temperature are \(n_{A} = 1.80\times 10^{14}\,\text{cm}^{-3}\) and \(n_{B} = 1.44\times 10^{15}\,\text{cm}^{-3}\), respectively. If \(P_{A}\) and \(P_{B}\) are the pressures of the two gas samples, the ratio \(\frac{P_{A}}{P_{B}}\) is
1) \(1\)
2) \(\left(\frac{1}{8}\right)^{3/2}\)
3) \(\left(\frac{1}{8}\right)^{2/3}\)
4) \(8\)

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Option 1

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