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:http://physics.nist.gov/PhysRefData/HDEL/data.htmlThe 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
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:http://physics.nist.gov/PhysRefData/HDEL/data.htmlThe 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
