Chapter #8 Solutions - Modern Quantum Mechanics - Jim J Napolitano, J J Sakurai - 2nd Edition

1. These exercises are to give you some practice with natural units.(a) Express the proton mass mp = 1.67262158 × 10−27 kg in units of GeV.(b) Assume a particle with negligible mass is confined to a box the size of the proton, around 1 fm = 10−15 m. Use the uncertainty principle estimate the energy of the confined particle. You might be interested to know that the mass, in natural units, of the pion, the lightest strongly interacting particle, is mπ = 135 MeV.(c) String theory concerns the physics at a scale that combines gravity, relativity, and quantum mechanics. Use dimensional analysis to find the “Planck mass” MP, which is formed from G, ħ, and c, and express the result in GeV. Get solution

2. Show that a matrix ημν with the same elements as the metric tensor ημν used in this chapter has the property that ..., the identity matrix. Thus, show that the natural relationship ... in fact holds with this definition. Show also that aμbμ = aμbμ for two four-vectors aμ and bμ. Get solution

3. Show that (8.1.11) is in fact a conserved current when Ψ(x, t) satisfies the Klein-Gordon equation. Get solution

4. Show that (8.1.14) follows from (8.1.8). Get solution

5. Derive (8.1.16a), (8.1.16b), and (8.1.18). Get solution

6. Show that the free-particle energy eigenvalues of (8.1.18) are E = ±Ep and that the eigenfunctions are indeed given by (8.1.21), subject to the normalization that ϒ+τ3ϒ = ±1 for E = ±Ep. Get solution

7. This problem is taken from Quantum Mechanics II: A Second Course in Quantum Theory, 2nd ed., by Rubin H. Landau (1996). A spinless electron is bound by the Coulomb potential V(r) = −Ze2/r in a stationary state of total energy E ≤ m. You can incorporate this interaction into the Klein-Gordon equation by using the covariant derivative with V = −eΦ and A = 0.(a) Assume that the radial and angular parts of the equation separate and that the wave function can be written as e−i Et[ul(r)/r]Ylm(θ, ϕ). Show that the radial equation becomes...where α = e2, γ2 = 4(m2 − E2), and ρ = γr.(b) Assume that this equation has a solution of the usual form of a power series times the ρ → ∞ and ρ → 0 solutions, that is,...and show that...and that only for k+ is the expectation value of the kinetic energy finite and that this solution has a nonrelativistic limit that agrees with the solution found for the Schrödinger equation.(c) Determine the recurrence relation among the ci ’s for this to be a solution of the Klein-Gordon equation, and show that unless the power series terminates, the wave function will have an incorrect asymptotic form.(d) In the case where the series terminates, show that the energy eigenvalue for the k+ solution is...where n is the principal quantum number.(e) Expand E in powers of (Zα)2 and show that the first-order term yields the Bohr formula. Connect the higher-order terms with relativistic corrections, and discuss the degree to which the degeneracy in l is removed.Jenkins and Kunselman, in Phys. Rev. Lett. 17 (1966) 1148, report measurements of a large number of transition energies for π− atoms in large-Z nuclei. Compare some of these to the calculated energies, and discuss the accuracy of the prediction. (For example, consider the 3d →2p transition in 59Co, which emits a photon with energy 384.6 ± 1.0 keV.) You will probably need either to use a computer to carry out the energy differences with high enough precision, or else expand to higher powers of (Zα)2. Get solution

8. Prove that the traces of the γμ, α, and β are all zero. Get solution

9. (a) Derive the matrices γμ from (8.2.10) and show that they satisfy the Clifford algebra (8.2.4).(b) Show that...where I is the 2 × 2 identity matrix, and σi and τi are the Pauli matrices. (The ⊗ notation is a formal way to write our 4 × 4 matrices as 2 × 2 matrices of 2 × 2 matrices.) Get solution

10. Prove the continuity equation (8.2.11) for the Dirac equation. Get solution

11. Find the eigenvalues for the free-particle Dirac equation (8.2.20). Get solution

13. Make use of Problem 8.9 to show that UT as defined by (8.3.28) is just σ2 ⊗ I, up to a phase factor. Get solution

14. Write down the positive-helicity, positive-energy free-particle Dirac spinor wave function Ψ(x, t).(a) Construct the spinors ...Ψ, ...Ψ, ...Ψ.(b) Construct the spinor ...Ψ and interpret it using the discussion of negative-energy solutions to the Dirac equation. Get solution

15. Show that (8.4.38) imply that u(x) and v(x) grow like exponentials if the series (8.4.32) and (8.4.33) do not terminate. Get solution

16. Expand the energy eigenvalues given by (8.4.43) in powers of Zα, and show that the result is equivalent to including the relativistic correction to kinetic energy (5.3.10) and the spin-orbit interaction (5.3.31) to the nonrelativistic energy eigenvalues for the one-electron atom (8.4.44). Get solution

17. The National Institute of Standards and Technology (NIST) maintains a web site with up-to-date high-precision data on the atomic energy levels of hydrogen and deuterium: accompanying table of data was obtained from that web site. It gives the energies of transitions between the (n, l, j) = (1,0,1/2) energy level and the energy level indicated by the columns on the left....(The number in parentheses is the numerical value of the standard uncertainty referred to the last figures of the quoted value.) Compare these values to those predicted by (8.4.43). (You may want to make use of Problem 8.16.) In particular:(a) Compare fine-structure splitting between the n = 2, j = 1/2 and n = 2, j = 3/2 states to (8.4.43).(b) Compare fine-structure splitting between the n = 4, j = 5/2 and n = 4, j = 7/2 states to (8.4.43).(c) Compare the 1S → 2S transition energy to the first line in the table. Use as many significant figures as necessary in the values of the fundamental constants, to compare the results within standard uncertainty.(d) How many examples of the Lamb shift are demonstrated in this table? Identify one example near the top and another near the bottom of the table, and compare their values. Get solution

Chapter #7 Solutions - Modern Quantum Mechanics - Jim J Napolitano, J J Sakurai - 2nd Edition

1. Liquid helium makes a transition to a macroscopic quantum fluid, called superfluid helium, when cooled below a phase-transition temperature T = 2.17K. Calculate the de Broglie wavelength λ = h/p for helium atoms with average energy at this temperature, and compare it to the size of the atom itself. Use this to predict the superfluid transition temperature for other noble gases, and explain why none of them can form superfluids. (You will need to look up some empirical data for these elements.) Get solution

2. (a) N identical spin ... particles are subjected to a one-dimensional simple harmonic-oscillator potential. Ignore any mutual interactions between the particles. What is the ground-state energy? What is the Fermi energy?(b) What are the ground-state and Fermi energies if we ignore the mutual interactions and assume N to be very large? Get solution

3. It is obvious that two nonidentical spin 1 particles with no orbital angular momenta (that is, s-states for both) can form j = 0, j = 1, and j = 2. Suppose, however, that the two particles are identical. What restrictions do we get? Get solution

4. Discuss what would happen to the energy levels of a helium atom if the electron were a spinless boson. Be as quantitative as you can. Get solution

5. Three spin 0 particles are situated at the corners of an equilateral triangle (see the accompanying figure). Let us define the z-axis to go through the center and in the direction normal to the plane of the triangle. The whole system is free to rotate about the z-axis. Using statistics considerations, obtain restrictions on the magnetic quantum numbers corresponding to Jz.... Get solution

6. Consider three weakly interacting, identical spin 1 particles.(a) Suppose the space part of the state vector is known to be symmetrical under interchange of any pair. Using notation |+⟩ |0⟩|+⟩ for particle 1 in ms = +1, particle 2 in ms = 0, particle 3 in ms = +1, and so on, construct the normalized spin states in the following three cases:(i) All three of them in |+⟩.(ii) Two of them in |+⟩, one in |0⟩.(iii) All three in different spin states.What is the total spin in each case?(b) Attempt to do the same problem when the space part is antisymmetrical under interchange of any pair. Get solution

7. Show that, for an operator a that, with its adjoint, obeys the anticommutation relation {a, a†} = aa† + a†a = 1, the operator N = a†a has eigenstates with the eigenvalues 0 and 1. Get solution

8. Suppose the electron were a spin-... particle obeying Fermi-Dirac statistics. Write the configuration of a hypothetical Ne (Z = 10) atom made up of such “electrons” [that is, the analog of (1 s)2 (2s)2 (2p)6]. Show that the configuration is highly degenerate. What is the ground state (the lowest term) of the hypothetical Ne atom in spectroscopic notation (2 S+1LJ, where S, L, and J stand for the total spin, the total orbital angular momentum, and the total angular momentum, respectively) when exchange splitting and spin-orbit splitting are taken into account? Get solution

9. Two identical spin ... fermions move in one dimension under the influence of the infinite-wall potential V = ∞ for x x > L, and V = 0 for 0 ≤ x ≤ L.(a) Write the ground-state wave function and the ground-state energy when the two particles are constrained to a triplet spin state (ortho state).(b) Repeat (a) when they are in a singlet spin state (para state).(c) Let us now suppose that the two particles interact mutually via a very short-range attractive potential that can be approximated by...Assuming that perturbation theory is valid even with such a singular potential, discuss semiquantitatively what happens to the energy levels obtained in (a) and (b). Get solution

10. Prove the relations (7.6.11), and then carry through the calculation to derive (7.6.17). Get solution

Chapter #6 Solutions - Modern Quantum Mechanics - Jim J Napolitano, J J Sakurai - 2nd Edition

1. The Lippmann-Schwinger formalism can also be applied to a one-dimensional transmission-reflection problem with a finite-range potential, V(x) ≠ 0 for 0 x| a only.(a) Suppose we have an incident wave coming from the left: .... How must we handle the singular 1/(E − H0) operator if we are to have a transmitted wave only for x > a and a reflected wave and the original wave for x a? Is the E → E + iε prescription still correct? Obtain an expression for the appropriate Green’s function and write an integral equation for ⟨x|ψ(+)⟩.(b) Consider the special case of an attractive δ-function potential...Solve the integral equation to obtain the transmission and rejection amplitudes. Check your results with Gottfried 1966, p. 52.(c) The one-dimensional δ-function potential with γ > 0 admits one (and only one) bound state for any value of γ. Show that the transmission and rejection amplitudes you computed have bound-state poles at the expected positions when k is regarded as a complex variable. Get solution

2. each of the following ways.(a) By integrating the differential cross section computed using the first-order Born approximation.(b) By applying the optical theorem to the forward-scattering amplitude in the second-order Born approximation. [Note that f (0) is real if the first-order Born approximation is used.] Get solution

3. Estimate the radius of the 40Ca nucleus from the data in Figure 6.6 and compare to that expected from the empirical value ≈ 1.4A1/3 fm, where A is the nuclear mass number. Check the validity of using the fist-order Born approximation for these data. Get solution

4. Consider a potential...where V0 may be positive or negative. Using the method of partial waves, show that for |Vo| ≪ E = ħ2k2/2m and k R ≪ 1, the differential cross section is isotropic and that the total cross section is given by...Suppose the energy is raised slightly. Show that the angular distribution can then be written as...Obtain an approximate expression for B/A. Get solution

5. A spinless particle is scattered by a weak Yukawa potential...where μ > 0 but V0 can be positive or negative. It was shown in the text that the fist-order Born amplitude is given by...(a) Using f(1)(θ) and assuming |δl| ≪ 1, obtain an expression for δl in terms of a Legendre function of the second kind,...(b) Use the expansion prove each assertion.(i) δl is negative (positive) when the potential is repulsive (attractive).(ii) When the de Broglie wavelength is much longer than the range of the potential, δl is proportional to k2l+1. Find the proportionality constant. Get solution

6. Check explicitly the x − Px uncertainty relation for the ground state of a particle confined inside a hard sphere: V = ∞ for r > a, V = 0 for r . (Hint: Take advantage of spherical symmetry.) Get solution

7. Consider the scattering of a particle by an impenetrable sphere...(a) Derive an expression for the s-wave (l = 0) phase shift. (You need not know the detailed properties of the spherical Bessel functions to do this simple problem!)(b) What is the total cross section σ[σ = ∫(dσ/dΩ)dΩ] in the extreme low-energy limit k → 0? Compare your answer with the geometric cross section πa2. You may assume without proof:... Get solution

8. Use δl = Δ(b)|b=1/k to obtain the phase shift δl for scattering at high energies by (a) the Gaussian potential, V = V0 exp(−r2/a2),and (b) the Yukawa potential, V = V0 exp(−μr)/μr. Verify the assertion that δl goes to zero very rapidly with increasing l (k fixed) for l ≫ kR, where R is the “range” of the potential. [The formula for Δ(b) is given in (6.5.14)]. Get solution

9. (a) Prove...where r(r>) stands for the smaller (larger) of r and r′.(b) For spherically symmetrical potentials, the Lippmann-Schwinger equation can be written for spherical waves:...Using (a), show that this equation, written in the x-representation, leads to an equation for the radial function, Al(k; r), as follows:...By taking r very large, also obtain... Get solution

10. Consider scattering by a repulsive δ-shell potential:...(a) Set up an equation that determines the s-wave phase shift δ0 as a function of k (E = ħ2k2/2m).(b) Assume now that γ is very large,...Show that if tan kR is not close to zero, the s-wave phase shift resembles the hard-sphere result discussed in the text. Show also that for tan kR close to (but not exactly equal to) zero, resonance behavior is possible; that is, cot δ0 goes through zero from the positive side as k increases. Determine approximately the positions of the resonances keeping terms of order 1/γ; compare them with the bound-state energies for a particle confined inside a spherical wall of the same radius,...Also obtain an approximate expression for the resonance width Γ defined by...and notice, in particular, that the resonances become extremely sharp as γ becomes large. (Note: For a different more sophisticated approach to this problem, see Gottfried 1966, pp. 131–41, who discusses the analytic properties of the Dl -function defined by Al = jl/Dl.) Get solution

11. A spinless particle is scattered by a time-dependent potential...Show that if the potential is treated to first order in the transition amplitude, the energy of the scattered particle is increased or decreased by ħω. Obtain dσ/dΩ. Discuss qualitatively what happens if the higher-order terms are taken into account. Get solution

12. Show that the differential cross section for the elastic scattering of a fast electron by the ground state of the hydrogen atom is given by...(Ignore the effect of identity.) Get solution

13. Let the energy of a particle moving in a central field be E(J1J2J3), where (J1, J2, J3) are the three action variables. How does the functional form of E specialize for the Coulomb potential? Using the recipe of the action-angle method, compare the degeneracy of the central-field problem to that of the Coulomb problem, and relate it to the vector A.If the Hamiltonian is...,how are these statements changed?Describe the corresponding degeneracies of the central-field and Coulomb problems in quantum theory in terms of the usual quantum numbers (n, l, m) and also in terms of the quantum numbers (k, m, n). Here the second set, (k, m, n), labels the wave functions ....How are the wave functions ... related to Laguerre times spherical harmonics? Get solution

Chapter #5 Solutions - Modern Quantum Mechanics - Jim J Napolitano, J J Sakurai - 2nd Edition

1. A simple harmonic oscillator (in one dimension) is subjected to a perturbation...where b is a real constant.(a) Calculate the energy shift of the ground state to lowest nonvanishing order.(b) Solve this problem exactly and compare with your result obtained in (a). You may assume without proof that... Get solution

2. In nondegenerate time-independent perturbation theory, what is the probability of finding in a perturbed energy eigenstate (|k⟩) the corresponding unperturbed eigenstate (|k(0)⟩)? Solve this up to terms of order λ2. Get solution

3. Consider a particle in a two-dimensional potential...Write the energy eigenfunctions for the ground state and the first excited state. We now add a time-independent perturbation of the form...Obtain the zeroth-order energy eigenfunctions and the first-order energy shifts for the ground state and the first excited state. Get solution

4. Consider an isotropic harmonic oscillator in two dimensions. The Hamiltonian is given by...(a) What are the energies of the three lowest-lying states? Is there any degeneracy?(b) We now apply a perturbation...where δ is a dimensionless real number much smaller than unity. Find the zeroth-order energy eigenket and the corresponding energy to first order [that is, the unperturbed energy obtained in (a) plus the first-order energy shift] for each of the three lowest-lying states.(c) Solve the H0 + V problem exactly. Compare with the perturbation results obtained in (b). [You may use ...] Get solution

5. Establish (5.1.54) for the one-dimensional harmonic oscillator given by (5.1.50) with an additional perturbation ... Show that all other matrix elements Vk0 vanish. Get solution

6. (From Merzbacher 1970.) A slightly anisotropic three-dimensional harmonic oscillator has ωz ≈ ωx = ωy. A charged particle moves in the field of this oscillator and is at the same time exposed to a uniform magnetic field in the x-direction. Assuming that the Zeeman splitting is comparable to the splitting produced by the anisotropy, but small compared to ħω, calculate to first order the energies of the components of the first excited state. Discuss various limiting cases. Get solution

7. A one-electron atom whose ground state is nondegenerate is placed in a uniform electric field in the z-direction. Obtain an approximate expression for the induced electric dipole moment of the ground state by considering the expectation value of ez with respect to the perturbed-state vector computed to first order. Show that the same expression can also be obtained from the energy shift ... of the ground state computed to second order. (Note: α stands for the polarizability.) Ignore spin. Get solution

8. Evaluate the matrix elements (or expectation values) given below. If any vanishes, explain why it vanishes using simple symmetry (or other) arguments.(a) ⟨n = 2, l = 1, m = 0|x|n = 2, l = 0, m = 0⟩.(b) ⟨n = 2, l = 1, m = 0|pz|n = 2, l = 0, m = 0⟩.[In (a) and (b), |nlm⟩ stands for the energy eigenket of a nonrelativistic hydrogen atom with spin ignored.](c) ⟨Lz⟩ for an electron in a central held with ..., l = 4.(d) ⟨singlet, ms = 0|Sz(e–) – Sz(e–)|triplet, ms = 0⟩ for an s-state positronium.(e) ⟨S(1) · S(2)) for the ground state of a hydrogen molecule. Get solution

9. A p-orbital electron characterized by |n, l = 1, m = ±1,0⟩ (ignore spin) is subjected to a potential...(a) Obtain the “correct” zeroth-order energy eigenstates that diagonalize the perturbation. You need not evaluate the energy shifts in detail, but show that the original threefold degeneracy is now completely removed.(b) Because V is invariant under time reversal and because there is no longer any degeneracy, we expect each of the energy eigenstates obtained in (a) to go into itself (up to a phase factor or sign) under time reversal. Check this point explicitly. Get solution

10. Consider a spinless particle in a two-dimensional infinite square well:...(a) What are the energy eigenvalues for the three lowest states? Is there any degeneracy?(b) We now add a potential....Taking this as a weak perturbation, answer the following:(i) Is the energy shift due to the perturbation linear or quadratic in λ for each of the three states?(ii) Obtain expressions for the energy shifts of the three lowest states accurate to order λ. (You need not evaluate integrals that may appear.)(iii) Draw an energy diagram with and without the perturbation for the three energy states. Make sure to specify which unperturbed state is connected to which perturbed state. Get solution

11. The Hamiltonian matrix for a two-state system can be written as...Clearly, the energy eigenfunctions for the unperturbed problems (λ = 0) are given by...(a) Solve this problem exactly to find the energy eigenfunctions ψ1 and ψ2 and the energy eigenvalues E1 and E2.(b) Assuming that ..., solve the same problem using timeindependent perturbation theory up to first order in the energy eigenfunctions and up to second order in the energy eigenvalues. Compare with the exact results obtained in (a).(c) Suppose the two unperturbed energies are “almost degenerate”; that is,...Show that the exact results obtained in (a) closely resemble what you would expect by applying degenerate perturbation theory to this problem with ... set exactly equal to .... Get solution

12. (This is a tricky problem because the degeneracy between the first state and the second state is not removed in first order. See also Gottfried 1966, p. 397, Problem 1.) This problem is from Schiff 1968, p. 295, Problem 4. A system that has three unperturbed states can be represented by the perturbed Hamiltonian matrix...where E2> E1. The quantities a and b are to be regarded as perturbations that are of the same order and are small compared with E2 — E1. Use the second-order nondegenerate perturbation theory to calculate the perturbed eigenvalues. (Is this procedure correct?) Then diagonalize the matrix to find the exact eigenvalues. Finally, use the second-order degenerate perturbation theory. Compare the three results obtained. Get solution

13. Compute the Stark effect for the 2S1/2 and 2P1/2 levels of hydrogen for a field ε sufficiently weak that eεa0 is small compared to the fine structure, but take the Lamb shift δ (δ = 1,057 MHz) into account (that is, ignore 2P3/2 in this calculation). Show that for eεa0 δ, the energy shifts are quadratic in ε, whereas for eεa0 >> δ, they are linear in ε. (The radial integral you need is (2s|r|2p⟩ = ...) Briefly discuss the consequences (if any) of time reversal for this problem. This problem is from Gottfried 1966, Problem 7-3. Get solution

14. Work out the Stark effect to lowest nonvanishing order for the n = 3 level of the hydrogen atom. Ignoring the spin-orbit force and relativistic correction (Lamb shift), obtain not only the energy shifts to lowest nonvanishing order but also the corresponding zeroth-order eigenket. Get solution

15. Suppose the electron had a very small intrinsic electric dipole moment analogous to the spin-magnetic moment (that is, μel proportional to σ). Treating the hypothetical —μel · E interaction as a small perturbation, discuss qualitatively how the energy levels of the Na atom (Z = 11) would be altered in the absence of any external electromagnetic field. Are the level shifts first order or second order? Indicate explicitly which states get mixed with each other. Obtain an expression for the energy shift of the lowest level that is affected by the perturbation. Assume throughout that only the valence electron is subjected to the hypothetical interaction. Get solution

16. Consider a particle bound to a fixed center by a spherically symmetrical potential V (r).(a) Prove...for all s-states, ground and excited.(b) Check this relation for the ground state of a three-dimensional isotropic oscillator, the hydrogen atom, and so on. (Note: This relation has actually been found to be useful in guessing the form of the potential between a quark and an antiquark.) Get solution

17. (a) Suppose the Hamiltonian of a rigid rotator in a magnetic field perpendicular to the axis is of the form (Merzbacher 1970, Problem 17-1)...if terms quadratic in the field are neglected. Assuming B >> C, use perturbation theory to lowest nonvanishing order to get approximate energy eigenvalues.(b) Consider the matrix elements...of a one-electron (for example, alkali) atom. Write the selection rules for Δl, Δml, and Δms. Justify your answer. Get solution

18. Work out the quadratic Zeeman effect for the ground-state hydrogen atom [⟨x|0⟩ = ... due to the usually neglected e2A2/2mec2-term in the Hamiltonian taken to first order. Write the energy shift as...and obtain an expression for diamagnetic susceptibility, χ. The following definite integral may be useful:... Get solution

19. (Merzbacher 1970, p. 448, Problem 11.) For the He wave function, use...with ... as obtained by the variational method. The measured value of the diamagnetic susceptibility is 1.88 × 10−6cm3/mole.Using the Hamiltonian for an atomic electron in a magnetic field, determine, for a state of zero angular momentum, the energy change to order B2 if the system is in a uniform magnetic held represented by the vector potential ...Defining the atomic diamagnetic susceptibility χ by ... calculate χ for a helium atom in the ground state and compare the result with the measured value. Get solution

20. Estimate the ground-state energy of a one-dimensional simple harmonic oscillator a trial function with β to be varied. You may use... Get solution

21. Estimate the lowest eigenvalue (λ) of the differential equation...using the variational method a trial function. (Caution: dψ/dx is discontinuous at x = 0.) Numerical data that may be useful for this problem are...The exact value of the lowest eigenvalue can be shown to be 1.019. Get solution

22. Consider a one-dimensional simple harmonic oscillator whose classical angular frequency is ω0. For t 0 it is known to be in the ground state. For t > 0 there is also a time-dependent potentialV (t) = F0 x cos ωt,where F0 is constant in both space and time. Obtain an expression for the expectation value (x) as a function of time using time-dependent perturbation theory to lowest nonvanishing order. Is this procedure valid for ω ≃ ω0? [You may use... Get solution

23. A one-dimensional harmonic oscillator is in its ground state for t 0. For t ≥ 0 it is subjected to a time-dependent but spatially uniform force (not potential!) in the x-direction,...(a) Using time-dependent perturbation theory to first order, obtain the probability of finding the oscillator in its first excited state for t > 0. Show that the t →∞ (τ finite) limit of your expression is independent of time. Is this reasonable or surprising?(b) Can we find higher excited states? You may use... Get solution

25. The unperturbed Hamiltonian of a two-state system is represented by...There is, in addition, a time-dependent perturbation...(a) At t = 0 the system is known to be in the first state, represented by...Using time-dependent perturbation theory and assuming that ...? is not close to ±ħω derive an expression for the probability that the system is found in the second state represented a function of t(t > 0).(b) Why is this procedure not valid when ... is close to ±ħω? Get solution

26. A one-dimensional simple harmonic oscillator of angular frequency ω is acted upon by a spatially uniform but time-dependent force (not potential)...At t = −∞, the oscillator is known to be in the ground state. Using the time-dependent perturbation theory to first order, calculate the probability that the oscillator is found in the first excited state at t = +∞.Challenge for experts: F(t) is so normalized that the impulse...imparted to the oscillator is always the same—that is, independent of τ; yet for τ ≫l/ω, the probability for excitation is essentially negligible. Is this reasonable? [Matrix element of ... Get solution

27. Consider a particle in one dimension moving under the influence of some timeindependent potential. The energy levels and the corresponding eigenfunctions for this problem are assumed to be known. We now subject the particle to a traveling pulse represented by a time-dependent potential,...(a) Suppose that at t = −∞ the particle is known to be in the ground state whose energy eigenfunction is ⟨x\i⟩ = ui(x). Obtain the probability for finding the system in some excited state with energy eigenfunction ⟨x\i⟩ = u f(x) at t = +∞.(b) Interpret your result in (a) physically by regarding the δ-function pulse as a superposition of harmonic perturbations; recall...Emphasize the role played by energy conservation, which holds even quantum-mechanically as long as the perturbation has been on for a very long time. Get solution

28. A hydrogen atom in its ground state [(n, l, m) = (1,0,0)] is placed between the plates of a capacitor. A time-dependent but spatially uniform electric field (not potential!) is applied as follows:...Using first-order time-dependent perturbation theory, compute the probability for the atom to be found at t ≫ τ in each of the three 2p states: (n, l, m) = (2, 1, ±1 or 0). Repeat the problem for the 2s state: (n, l, m) = (2, 0, 0). You need not attempt to evaluate radial integrals, but perform all other integrations (with respect to angles and time). Get solution

29. Consider a composite system made up of two spin ... objects. For t 0, the Hamiltonian does not depend on spin and can be taken to be zero by suitably adjusting the energy scale. For t > 0, the Hamiltonian is given by...Suppose the system is in |+−⟩ for t 0. Find, as a function of time, the probability for its being found in each of the following states |++⟩, |+−⟩, |−+⟩, and |−−⟩:(a) By solving the problem exactly.(b) By solving the problem assuming the validity of first-order time-dependent perturbation theory with H as a perturbation switched on at t = 0. Under what condition does (b) give the correct results? Get solution

30. Consider a two-level system with E1 2. There is a time-dependent potential that connects the two levels as follows:...At t = 0, it is known that only the lower level is populated—that is, c1(0) = 1, c2(0) = 0.(a) Find |c1(t)|2 and |c2(t)|2 for t > 0 by exactly solving the coupled differential equation...(b) Do the same problem using time-dependent perturbation theory to lowest nonvanishing order. Compare the two approaches for small values of γ. Treat the following two cases separately: (i) ω very different from ω21 and (ii) ω close to ω21.Answer for (a): (Rabi’s formula)... Get solution

31. Show that the slow-turn-on of perturbation V → Veηt (see Baym 1969, p. 257) can generate a contribution from the second term in (5.7.36). Get solution

32. (a) Consider the positronium problem you solved in Chapter 3, Problem 3.4. In the presence of a uniform and static magnetic field B along the z-axis, the Hamiltonian is given by...Solve this problem to obtain the energy levels of all four states using degenerate time-independent perturbation theory (instead of diagonalizing the Hamiltonian matrix). Regard the first and second terms in the expression for H as H0 and V, respectively. Compare your results with the exact expressions...where triplet (singlet) m = 0 stands for the state that becomes a pure triplet (singlet) with m = 0 as B → 0.(b) We now attempt to cause transitions (via stimulated emission and absorption) between the two m = 0 states by introducing an oscillating magnetic field of the “right” frequency. Should we orient the magnetic field along the z-axis or along the x- (or y-) axis? Justify your choice. (The original static field is assumed to be along the z-axis throughout.)(c) Calculate the eigenvectors to first order. Get solution

33. Repeat Problem 5.32, but with the atomic hydrogen Hamiltonian...where in the hyperfine term, AS1 · S2, Si is the electron spin and S2 is the proton spin. [Note that the problem here has less symmetry than the positronium case]. Get solution

34. Consider the spontaneous emission of a photon by an excited atom. The process is known to be an E1 transition. Suppose the magnetic quantum number of the atom decreases by one unit. What is the angular distribution of the emitted photon? Also discuss the polarization of the photon, with attention to angular-momentum conservation for the whole (atom plus photon) system. Get solution

35. Consider an atom made up of an electron and a singly charged (Z = 1) triton (3H). Initially the system is in its ground state (n = 1, l = 0). Suppose the system undergoes beta decay, in which the nuclear charge suddenly increases by one unit (realistically by emitting an electron and an antineutrino). This means that the tritium nucleus (called a triton) turns into a helium (Z = 2) nucleus of mass 3 (3He).(a) Obtain the probability for the system to be found in the ground state of the resulting helium ion. The hydrogenic wave function is given by...(b) The available energy in tritium beta decay is about 18 keV, and the size of the 3He atom is about 1Å. Check that the time scale T for the transformation satisfies the criterion of validity for the sudden approximation. Get solution

37. Consider a neutron in a magnetic field, fixed at an angle θ with respect to the z-axis, but rotating slowly in the ϕ-direction. That is, the tip of the magnetic field traces out a circle on the surface of the sphere at “latitude” π − θ. Explicitly calculate the Berry potential A for the spin-up state from (5.6.23), take its curl, and determine Berry’s Phase γ+. Thus, verify (5.6.42) for this particular example of a curve C. (For hints, see “The Adiabatic Theorem and Berry’s Phase” by B. R. Holstein, Am. J. Phys. 57 (1989) 1079.) Get solution

38. The ground state of a hydrogen atom (n = 1, l = 0) is subjected to a time-dependent potential as follows:...Using time-dependent perturbation theory, obtain an expression for the transition rate at which the electron is emitted with momentum p. Show, in particular, how you may compute the angular distribution of the ejected electron (in terms of θ and ϕ defined with respect to the z-axis). Discuss briefly the similarities and the differences between this problem and the (more realistic) photoelectric effect. (Note: For the initial wave function, see Problem 5.35. If you have a normalization problem, the final wave function may be taken to be...with L very large, but you should be able to show that the observable effects are independent of L.) Get solution

40. Linearly polarized light of angular frequency ω is incident on a one-electron “atom” whose wave function can be approximated by the ground state of a three-dimensional isotropic harmonic oscillator of angular frequency ω0. Show that the differential cross section for the ejection of a photoelectron is given by...provided the ejected electron of momentum ħkf can be regarded as being in a plane-wave state. (The coordinate system used is shown in Figure 5.12.) Get solution

41. Find the probability |ϕ(p′)|2d3p′ of the particular momentum p′ for the ground-state hydrogen atom. (This is a nice exercise in three-dimensional Fourier transforms. To perform the angular integration, choose the z-axis in the direction of p.) Get solution

42. Obtain an expression for τ(2p → 1s) for the hydrogen atom. Verify that it is equal to 1.6 × 10−9s. Get solution

Chapter #4 Solutions - Modern Quantum Mechanics - Jim J Napolitano, J J Sakurai - 2nd Edition

1. Calculate the three lowest energy levels, together with their degeneracies, for the following systems (assume equal-mass distinguishable particles).(a) Three noninteracting spin ... particles in a box of length L.(b) Four noninteracting spin ... particles in a box of length L. Get solution

2. Let ... denote the translation operator (displacement vector d); let ... denote the rotation operator (... and ϕ are the axis and angle of rotation, respectively); and let π denote the parity operator. Which, if any, of the following pairs commute? Why?(a) ... and ... (d and d′ in different directions).(b) ... and ... (... and ... in different directions).(c) ... and π.(d) ... and π. Get solution

3. A quantum-mechanical state |ψ⟩ is known to be a simultaneous eigenstate of two Hermitian operators A and B that anticommute:...What can you say about the eigenvalues of A and B for state |ψ⟩? Illustrate your point using the parity operator (which can be chosen to satisfy π = π−1 = π†) and the momentum operator. Get solution

4. A spin ... particle is bound to a fixed center by a spherically symmetrical potential.(a) Write down the spin-angular function ...(b) Express (σ · x) ... in terms of some other ...(c) Show that your result in (b) is understandable in view of the transformation properties of the operator S · x under rotations and under space inversion (parity). Get solution

5. Because of weak (neutral-current) interactions, there is a parity-violating potential between the atomic electron and the nucleus as follows:...where S and p are the spin and momentum operators of the electron, and the nucleus is assumed to be situated at the origin. As a result, the ground State of an alkali atom, usually characterized by |n, l, j, m⟩, actually contains very tiny contributions from other eigenstates as follows:...On the basis of symmetry considerations alone, what can you say about (n′, l′, j′, m′), which give rise to nonvanishing contributions? Suppose the radial wave functions and the energy levels are all known. Indicate how you may calculate Cn′l′j′m′. Do we get further restrictions on (n′, l′, j′, m′)? Get solution

6. Consider a symmetric rectangular double-well potential:...Assuming that V0 is very high compared to the quantized energies of low-lying states, obtain an approximate expression for the energy splitting between the two lowest-lying states. Get solution

7. (a) Let ψ(x, t) be the wave function of a spinless particle corresponding to a plane wave in three dimensions. Show that ψ*(x, −t) is the wave function for the plane wave with the momentum direction reversed.(b) Let ... be the two-component eigenspinor of σ · ... with eigenvalue +1. Using the explicit form of ... (in terms of the polar and azimuthal angles β and γ that characterize ...), verify that −iσ2χ*... is the two-component eigenspinor with the spin direction reversed. Get solution

8. (a) Assuming that the Hamiltonian is invariant under time reversal, prove that the wave function for a spinless nondegenerate system at any given instant of time can always be chosen to be real.(b) The wave function for a plane-wave state at t = 0 is given by a complex function eip·x/ħ. Why does this not violate time-reversal invariance? Get solution

9. Let ϕ(p′) be the momentum-space wave function for state |α⟩—that is, π(p′) = ⟨p′|α). Is the momentum-space wave function for the time-reversed state Θ|α⟩ given by ϕ(p′), by ϕ(−p′), by ϕ*(p′), or by ϕ*(−p′)? Justify your answer. Get solution

10. (a) What is the time-reversed state corresponding to ...(b) Using the properties of time reversal and rotations, prove...(c) Prove θ|j, m⟩ = i2m|j, −m⟩. Get solution

11. Suppose a spinless particle is bound to a fixed center by a potential V(x) so asymmetrical that no energy level is degenerate. Using time-reversal invariance, prove...for any energy eigenstate. (This is known as quenching of orbital angular momentum.) If the wave function of such a nondegenerate eigenstate is expanded as...what kind of phase restrictions do we obtain on Flm(r)? Get solution

12. The Hamiltonian for a spin 1 system is given by...Solve this problem exactly to find the normalized energy eigenstates and eigen-values. (A spin-dependent Hamiltonian of this kind actually appears in crystal physics.) Is this Hamiltonian invariant under time reversal? How do the normalized eigenstates you obtained transform under time reversal? Get solution

Chapter #3 Solutions - Modern Quantum Mechanics - Jim J Napolitano, J J Sakurai - 2nd Edition

1. Find the eigenvalues and eigenvectors of .... Suppose an electron is in the spin state .... If sy is measured, what is the probability of the result ħ /2? Get solution

2. Find, by explicit construction using Pauli matrices, the eigenvalues for the Hamiltonian...for a spin ... particle in the presence of a magnetic field .... Get solution

3. Consider the 2 × 2 matrix defined by...where a0 is a real number and a is a three-dimensional vector with real components.(a) Prove that U is unitary and unimodular.(b) In general, a 2 × 2 unitary unimodular matrix represents a rotation in three dimensions. Find the axis and angle of rotation appropriate for U in terms of a0, a1, a2, and a3. Get solution

4. The spin-dependent Hamiltonian of an electron-positron system in the presence of a uniform magnetic field in the z-direction can be written as...Suppose the spin function of the system is given by ...(a) Is this an eigenfunction of H in the limit A → 0, eB/mc ≠ 0? If it is, what is the energy eigenvalue? If it is not, what is the expectation value of H?(b) Solve the same problem when eB / mc → 0, A ≠ 0. Get solution

5. Consider a spin 1 particle. Evaluate the matrix elements of... Get solution

6. Let the Hamiltonian of a rigid body be...where K is the angular momentum in the body frame. From this expression obtain the Heisenberg equation of motion for K, and then find Euler’s equation of motion in the correspondence limit. Get solution

7. Let ..., where (α, β, γ) are the Eulerian angles. In order that U represent a rotation (α, β, γ), what are the commutation rules that must be satisfied by the Gk? Relate G to the angular-momentum operators. Get solution

8. What is the meaning of the following equation?...where the three components of A are matrices. From this equation show that matrix elements ‹m| Ak |n› transform like vectors. Get solution

9. Consider a sequence of Euler rotations represented by...Because of the group properties of rotations, we expect that this sequence of operations is equivalent to a single rotation about some axis by an angle θ. Find θ. Get solution

10. (a) Consider a pure ensemble of identically prepared spin ... systems. Suppose the expectation values ⟨Sx⟩ and ⟨Sz⟩ and the sign of ⟨Sy⟩ are known. Show how we may determine the state vector. Why is it unnecessary to know the magnitude of ⟨Sy⟩?(b) Consider a mixed ensemble of spin ... systems. Suppose the ensemble averages [Sx], [Sy], and [Sz] are all known. Show how we may construct the 2 × 2 density matrix that characterizes the ensemble. Get solution

11. (a) Prove that the time evolution of the density operator p (in the Schrödinger picture) is given by...(b) Suppose we have a pure ensemble at t = 0. Prove that it cannot evolve into a mixed ensemble as long as the time evolution is governed by the Schrödinger equation. Get solution

12. Consider an ensemble of spin 1 systems. The density matrix is now a 3 × 3 matrix. How many independent (real) parameters are needed to characterize the density matrix? What must we know in addition to [Sx], [Sy], and [Sz] to characterize the ensemble completely? Get solution

13. An angular-momentum eigenstate |j, m = mmax = j⟩ is rotated by an infinitesimal angle ε about the y-axis. Without using the explicit form of the ... function, obtain an expression for the probability for the new rotated state to be found in the original state up to terms of order ε2. Get solution

14. Show that the 3 × 3 matrices Gi(i = 1, 2, 3) whose elements are given by...where j and k are the row and column indices, satisfy the angular-momentum commutation relations. What is the physical (or geometric) significance of the transformation matrix that connects Gi to the more usual 3 × 3 representations of the angular-momentum operator Ji with J3 taken to be diagonal? Relate your result to...under infinitesimal rotations. (Note: This problem may be helpful in understanding the photon spin.) Get solution

15. (a) Let J be angular momentum. (It may stand for orbital L, spin S, or Jtotal.) Using the fact that Jx, Jy, Jz (J± = Jx ± iJy) satisfy the usual angular-momentum commutation relations, prove...(b) Using (a) (or otherwise), derive the “famous” expression for the coefficient c− that appears in... Get solution

16. Show that the orbital angular-momentum operator L commutes with both the operators p2 and x2; that is, prove (3.7.2). Get solution

17. The wave function of a particle subjected to a spherically symmetrical potential V (r) is given by...(a) Is ψ an eigenfunction of L2? If so, what is the l-value? If not, what are the possible values of l that we may obtain when L2 is measured?(b) What are the probabilities for the particle to be found in various ml states?(c) Suppose it is known somehow that ψ (x) is an energy eigenfunction with eigenvalue E. Indicate how we may find V(r). Get solution

18. A particle in a spherically symmetrical potential is known to be in an eigenstate of L2 and Lz with eigenvalues ħ2l(l + 1) and mħ, respectively. Prove that the expectation values between |lm⟩ states satisfy...Interpret this result semiclassically. Get solution

19. Suppose a half-integer l-value, say ..., were allowed for orbital angular momentum. From...we may deduce, as usual,...Now try to construct Y1/2,−1/2(θ, φ) by (a) applying L− to Y1/2,1/2(θ, φ); and (b) using L−Y1/2,−1/2(θ, φ) = 0. Show that the two procedures lead to contradictory results. (This gives an argument against half-integer l-values for orbital angular momentum.) Get solution

20. Consider an orbital angular-momentum eigenstate |l = 2, m = 0⟩. Suppose this state is rotated by an angle β about the y-axis. Find the probability for the new state to be found in m = 0, ±1, and ±2. (The spherical harmonics for l = 0, 1, and 2 given in Section B.5 in Appendix B may be useful.) Get solution

21. The goal of this problem is to determine degenerate eigenstates of the threedimensional isotropic harmonic oscillator written as eigenstates of L2 and Lz, in terms of the Cartesian eigenstates |nxnynz).(a) Show that the angular-momentum operators are given by...where summation is implied over repeated indices, εijk is the totally antisymmetric symbol, and ... counts the total number of quanta.(b) Use these relations to express the states |qlm⟩ = |01m⟩, m = 0, ±1, in terms of the three eigenstates |nxnynz⟩ that are degenerate in energy. Write down the representation of your answer in coordinate space, and check that the angular and radial dependences are correct.(c) Repeat for |qlm⟩ = |200⟩.(d) Repeat for |qlm⟩ = |02m⟩, with m = 0, 1, and 2. Get solution

22. Follow these steps to show that solutions to Kummer’s Equation (3.7.46) can be written in terms of Laguerre polynomials Ln(x), which are defined according to a generating function as...where 0 t (a) Prove that Ln(0) = n! and L0(x) = 1.(b) Differentiate g(x, t) with respect to x, show that...and find the first few Laguerre polynomials.(c) Differentiate g(x, t) with respect to t and show that...(d) Now show that Kummer’s Equation is solved by deriving...and associate n with the principal quantum number for the hydrogen atom. Get solution

23. What is the physical significance of the Schwinger’s scheme for angular momentum? Give the nonvanishing matrix elements of K±. Get solution

24. We are to add angular momenta j1 = 1 and j2 = 1 to form j = 2, 1, and 0 states. Using either the ladder operator method or the recursion relation, express all (nine) {j, m} eigenkets in terms of |j1 j2;m1m2⟩. Write your answer as...where + and 0 stand for m1,2 = 1, 0, respectively. Get solution

25. (a) Evaluate...for any j (integer or half-integer); then check your answer for ....(b) Prove, for any j,...[Hint: This can be proved in many ways. You may, for instance, examine the rotational properties of ... using the spherical (irreducible) tensor language.] Get solution

26. (a) Consider a system with j = 1. Explicitly write⟨j = 1, m′|Jy|j = 1, m⟩in 3 × 3 matrix form.(b) Show that for j = 1 only, it is legitimate to replace e−iJyβ/ħ by...(c) Using (b), prove... Get solution

27. Express the matrix element ⟨α2β2γ2|J32|α1β1γ1⟩ in terms of a series in... Get solution

28. Consider a system made up of two spin ... particles. Observer A specializes in measuring the spin components of one of the particles (s1z, s1x and so on), while observer B measures the spin components of the other particle. Suppose the system is known to be in a spin-singlet state—that is, Stotal = 0.(a) What is the probability for observer A to obtain s1z = ħ/2 when observer B makes no measurement? Solve the same problem for s1x = ħ/2.(b) Observer B determines the spin of particle 2 to be in the s2z = ħ/2 state with certainty. What can we then conclude about the outcome of observer A’s measurement (i) if A measures s1z; (ii) if A measures s1x ? Justify your answer. Get solution

29. Consider a spherical tensor of rank 1 (that is, a vector)...Using the expression for d(j=1) given in Problem 3.26, evaluate...and show that your results are just what you expect from the transformation properties of Vx, y, z under rotations about the y-axis. Get solution

30. (a) Construct a spherical tensor of rank 1 out of two different vectors U = (Ux, Uy, Uz) and V = (Vx, Vy, Vz). Explicitly write ... in terms of Ux,y z and Ux,y z.(b) Construct a spherical tensor of rank 2 out of two different vectors U and V. Write down explicitly ... in terms of Ux,y,z and Vx,y,z. Get solution

31. Consider a spinless particle bound to a fixed center by a central force potential.(a) Relate, as much as possible, the matrix elements...using only the Wigner-Eckart theorem. Make sure to state under what conditions the matrix elements are nonvanishing.(b) Do the same problem using wave functions ... Get solution

32. (a) Write xy, xz, and (x2 − y2) as components of a spherical (irreducible) tensor of rank 2.(b) The expectation known as the quadrupole moment. Evaluate...where m′ = j, j − 1, j − 2,..., in terms of Q and appropriate Clebsch-Gordan coefficients. Get solution

33. A spin ... nucleus situated at the origin is subjected to an external inhomogeneous electric field. The basic electric quadrupole interaction may by taken to be...where ϕ is the electrostatic potential satisfying Laplace’s equation, and the coordinate axes are chosen such that...Show that the interaction energy can be written as...and express A and B in terms of (∂2ϕ/∂x2)0 and so on. Determine the energy eigenkets (in terms of |m⟩, where m = ... and the corresponding energy eigenvalues. Is there any degeneracy? Get solution

Chapter #2 Solutions - Modern Quantum Mechanics - Jim J Napolitano, J J Sakurai - 2nd Edition

1. Consider the spin-precession problem discussed in the text. It can also be solved in the Heisenberg picture. Using the Hamiltonian...,write the Heisenberg equations of motion for the time-dependent operators Sx(t), Sy(t), and Sz(t). Solve them to obtain Sx, y, z as functions of time. Get solution

2. Look again at the Hamiltonian of Chapter 1, Problem 1.11. Suppose the typist made an error and wrote H as....What principle is now violated? Illustrate your point explicitly by attempting to solve the most general time-dependent problem using an illegal Hamiltonian of this kind. (You may assume H11 = H22 = 0 for simplicity.) Get solution

3. An electron is subject to a uniform, time-independent magnetic field of strength B in the positive z-direction. At t = 0 the electron is known to be in an eigenstate of S · ... with eigenvalue ħ /2, where ... is a unit vector, lying in the xz-plane, that makes an angle ß with the z-axis.(a) Obtain the probability for finding the electron in the Sx = ħ/2 state as a function of time.(b) Find the expectation value of Sx as a function of time.(c) For your own peace of mind, show that your answers make good sense in the extreme cases (i) β→ 0 and (ii) β→π/2. Get solution

4. Derive the neutrino oscillation probability (2.1.65) and use it, along with the data in Figure 2.2, to estimate the values of Δm2c4 (in units of eV2) and θ. Get solution

5. Let x(t) be the coordinate operator for a free particle in one dimension in the Heisenberg picture. Evaluate.... Get solution

6. Consider a particle in one dimension whose Hamiltonian is given by....By calculating [[H, x], x], prove...,where |a'⟩ is an energy eigenket with eigenvalue Ea′. Get solution

7. Consider a particle in three dimensions whose Hamiltonian is given by....By calculating [x · p, H], obtain....In order for us to identify the preceding relation with the quantum-mechanical analogue of the virial theorem, it is essential that the left-hand side vanish. Under what condition would this happen? Get solution

8. Consider a free-particle wave packet in one dimension. At t = 0 it satisfies the minimum uncertainty relation....In addition, we know....Using the Heisenberg picture, obtain ⟨(Δx)2⟩t as a function of t(t ≥ 0) when ⟨ (Δx)2)t = 0 is given. (Hint: Take advantage of the property of the minimum uncertainty wave packet you worked out in Chapter 1, Problem 1.18.) Get solution

9. Let |a'⟩ and |a"⟩ be eigenstates of a Hermitian operator A with eigenvalues a' and a", respectively (a' ≠ a"). The Hamiltonian operator is given by...,where δ is just a real number.(a) Clearly, |a'⟩ and |a"⟩ are not eigenstates of the Hamiltonian. Write down the eigenstates of the Hamiltonian. What are their energy eigenvalues?(b) Suppose the system is known to be in state |a'⟩ at t = 0. Write down the state vector in the Schrödinger picture for t > 0.(c) What is the probability for finding the system in |a"⟩ for t > 0 if the system is known to be in state |a'⟩ at t = 0?(d) Can you think of a physical situation corresponding to this problem? Get solution

11. Using the one-dimensional simple harmonic oscillator as an example, illustrate the difference between the Heisenberg picture and the Schrödinger picture. Discuss in particular how (a) the dynamic variables x and p and (b) the most general state vector evolve with time in each of the two pictures. Get solution

12. Consider a particle subject to a one-dimensional simple harmonic oscillator potential. Suppose that at t = 0 the state vector is given by...,where p is the momentum operator and a is some number with dimension of length. Using the Heisenberg picture, evaluate the expectation value ⟨x⟩ for t ≥ 0. Get solution

13. (a) Write down the wave function (in coordinate space) for the state specified in Problem 2.12 at t = 0. You may use....(b) Obtain a simple expression for the probability that the state is found in the ground state at t = 0. Does this probability change for t > 0? Get solution

14. Consider a one-dimensional simple harmonic oscillator.(a) Using...,evaluate ⟨m|x|n⟩, ⟨m|p|n⟩, ⟨m|{x, p}|n⟩, ⟨m|x2|n⟩, and ⟨m|p2|n⟩.(b) Check that the virial theorem holds for the expectation values of the kinetic energy and the potential energy taken with respect to an energy eigenstate. Get solution

15. (a) Using... (one dimension),prove....(b) Consider a one-dimensional simple harmonic oscillator. Starting with the Schrödinger equation for the state vector, derive the Schrödinger equation for the momentum-space wave function. (Make sure to distinguish the operator p from the eigenvalue p'.) Can you guess the energy eigenfunctions in momentum space? Get solution

16. Consider a function, known as the correlation function, defined by...,where x(t) is the position operator in the Heisenberg picture. Evaluate the correlation function explicitly for the ground state of a one-dimensional simple harmonic oscillator. Get solution

17. Consider again a one-dimensional simple harmonic oscillator. Do the following algebraically—that is, without using wave functions.(a) Construct a linear combination of |0⟩ and |1⟩ such that ⟨x⟩ is as large as possible.(b) Suppose the oscillator is in the state constructed in (a) at t = 0. What is the state vector for t > 0 in the Schrödinger picture? Evaluate the expectation value ⟨x⟩as a function of time for t > 0, using (i) the Schrödinger picture and (ii) the Heisenberg picture.(c) Evaluate ⟨ (Δx)2⟩ as a function of time using either picture. Get solution

19. A coherent state of a one-dimensional simple harmonic oscillator is defined to be an eigenstate of the (non-Hermitian) annihilation operator a:...,where λ is, in general, a complex number.(a) Prove a normalized coherent state.(b) Prove the minimum uncertainty relation for such a state.(c) Write |λ⟩ as....Show that the distribution of |f (n)|2 with respect to n is of the Poisson form. Find the most probable value of n, and hence of E.(d) Show that a coherent state can also be obtained by applying the translation (finite-displacement) operator e−ipl/ħ (where p is the momentum operator and l is the displacement distance) to the ground state. (See also Gottfried 1966, 262-64.) Get solution

20. Let..., ..., ...,where a± and ... are the annihilation and creation operators of two independent simple harmonic oscillators satisfying the usual simple harmonic oscillator commutation relations. Prove..., ..., .... Get solution

21. Derive the normalization constant cn in (2.5.28) by deriving the orthogonality relationship (2.5.29) using generating functions. Start by working out the integral...,and then consider the integral again with the generating functions in terms of series with Hermite polynomials. Get solution

22. Consider a particle of mass m subject to a one-dimensional potential of the following form:....(a) What is the ground-state energy?(b) What is the expectation value ⟨x2⟩ for the ground state? Get solution

23. A particle in one dimension is trapped between two rigid walls:....At t = 0 it is known to be exactly at x = L/2 with certainty. What are the relative probabilities for the particle to be found in various energy eigenstates? Write down the wave function for t ≥ 0. (You need not worry about absolute normalization, convergence, and other mathematical subtleties.) Get solution

24. Consider a particle in one dimension bound to a fixed center by a S-function potential of the form..., (v0 real and positive).Find the wave function and the binding energy of the ground state. Are there excited bound states? Get solution

25. A particle of mass m in one dimension is bound to a fixed center by an attractive δ-function potential:..., ....At t = 0, the potential is suddenly switched off (that is, V = 0 for t > 0). Find the wave function for t > 0. (Be quantitative! But you need not attempt to evaluate an integral that may appear.) Get solution

26. A particle in one dimension (−∞ x ..., ....(a) Is the energy spectrum continuous or discrete? Write down an approximate expression for the energy eigenfunction specified by E. Also sketch it crudely.(b) Discuss briefly what changes are needed if V is replaced by.... Get solution

27. Derive an expression for the density of free-particle states in two dimensions, normalized with periodic boundary conditions inside a box of side length L. Your answer should be written as a function of k (or E) times dEdφ, where φ is the polar angle that characterizes the momentum direction in two dimensions. Get solution

28. Consider an electron confined to the interior of a hollow cylindrical shell whose axis coincides with the z-axis. The wave function is required to vanish on the inner and outer walls, ρ = ρa and ρb, and also at the top and bottom, z = 0 and L.(a) Find the energy eigenfunctions. (Do not bother with normalization.) Show that the energy eigenvalues are given by...,where kmn is the nth root of the transcendental equation....(b) Repeat the same problem when there is a uniform magnetic field B = B... for 0 ρ a. Note that the energy eigenvalues are influenced by the magnetic field even though the electron never “touches” the magnetic field.(c) Compare, in particular, the ground state of the B = 0 problem with that of the B ≠ 0 problem. Show that if we require the ground-state energy to be unchanged in the presence of B, we obtain “flux quantization”.... Get solution

29. Consider a particle moving in one dimension under the influence of a potential V(x). Suppose its wave function can be written as exp[iS(x, t)/ħ]. Prove that S(x, t) satisfies the classical Hamilton-Jacobi equation to the extent that ħ can be regarded as small in some sense. Show how one may obtain the correct wave function for a plane wave by starting with the solution of the classical Hamilton-Jacobi equation with V (x) set equal to zero. Why do we get the exact wave function in this particular case? Get solution

30. Using spherical coordinates, obtain an expression for j for the ground and excited states of the hydrogen atom. Show, in particular, that for ml≠ 0 states, there is a circulating flux in the sense that j is in the direction of increasing or decreasing φ, depending on whether ml is positive or negative. Get solution

31. Derive (2.6.16) and obtain the three-dimensional generalization of (2.6.16). Get solution

32. Define the partition function as...,as in (2.6.20)–(2.6.22). Show that the ground-state energy is obtained by taking....Illustrate this for a particle in a one-dimensional box. Get solution

33. The propagator in momentum space analogous to (2.6.26) is given by ⟨p", t|p', t0⟩. Derive an explicit expression for ⟨p", t|p', t0⟩ for the free-particle case. Get solution

34. (a) Write down an expression for the classical action for a simple harmonic oscillator for a finite time interval.(b) Construct ⟨xn, tn |xn−1, tn−1⟩ for a simple harmonic oscillator using Feynman’s prescription for tn − t n−1 = Δt small. Keeping only terms up to order (Δt)2, show that it is in complete agreement with the t −t0 → 0 limit of the propagator given by (2.6.26). Get solution

35. State the Schwinger action principle (see Finkelstein 1973, p. 155). Obtain the solution for ⟨x2t2|x1t1 ⟩ by integrating the Schwinger principle and compare it with the corresponding Feynman expression for ⟨x2t2|x1t1 ⟩. Describe the classical limits of these two expressions. Get solution

36. Show that the wave-mechanical approach to the gravity-induced problem discussed in Section 2.7 also leads to phase-difference expression (2.7.17). Get solution

37. (a) Verify (2.7.25) and (2.7.27).(b) Verify continuity equation (2.7.30) with j given by (2.7.31). Get solution

38. Consider the Hamiltonian of a spinless particle of charge e. In the presence of a static magnetic field, the interaction terms can be generated by...where A is the appropriate vector potential. Suppose, for simplicity, that the magnetic field B is uniform in the positive z-direction. Prove that the above prescription indeed leads to the correct expression for the interaction of the orbital magnetic moment (e/2mc)L with the magnetic field B. Show that there is also an extra term proportional to B2(x2 + y2), and comment briefly on its physical significance. Get solution

39. An electron moves in the presence of a uniform magnetic field in the z-direction ...(a) Evaluate...where...(b) By comparing the Hamiltonian and the commutation relation obtained in (a) with those of the one-dimensional oscillator problem, show how we can immediately write the energy eigenvalues as...where ħk is the continuous eigenvalue of the pz operator and n is a nonnegative integer including zero. Get solution

40. Consider the neutron interferometer....Prove that the difference in the magnetic fields that produce two successive maxima in the counting rates is given by...where gn(= −1.91) is the neutron magnetic moment in units of −eħ/2mnc. (If you had solved this problem in 1967, you could have published your solution in Physical Review Letters!) Get solution

Chapter #8 Solutions - Modern Quantum Mechanics - Jim J Napolitano, J J Sakurai - 2nd Edition

1. These exercises are to give you some practice with natural units.(a) Express the proton mass mp = 1.67262158 × 10−27 kg in units of...