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Exercise 81 obtained formulas for hydrogen like atoms in which the nucleus is not assumed infinite, as in the chapter, but is of mass, m1while m2is the mass of the orbiting negative charge. (a) What percentage error is introduced in the hydrogen ground-state energy by assuming that the proton is of infinite mass? (b) Deuterium is a form of hydrogen in which a neutron joins the proton in the nucleus, making the nucleus twice as massive. Taking nuclear mass into account, by what percent do the ground-state energies of hydrogen and deuterium differ?

Short Answer

Expert verified

Answer:
(a) The energy predicted by ignoring the proton’s finite mass is too high by

(b) The ground state energy of hydrogen is less than 0.02% of the ground state energy of Deuterium.

Step by step solution

01

(a) Percentage error is introduced in the hydrogen ground-state energy:

Effective mass simplifies band structures because modelling the behaviour of a free particle with that mass can be observed easily.

Ifμis the effective mass and m is the mass, the actual energy will be μ/mtimes the hydrogen energy.

Now, if meand mpare the mass of electron and proton,

μm=memp/(me+mp)me=11+me/mp=11+9.11×1031/1.673×10-27=1-0.00054

Hence, the energy predicted by ignoring the proton’s finite mass is too high by 0.054% .

02

(b) Ground state energy of Deuterium and Hydrogen:

Also, the ratio of energies (En) of Deuterium and Hydrogen will be equal to the ratio of their reduced masses (μ).

EDeuterinumEHydrogen=μDeuterinumμHydrogen=memDeut/(memDeut)memp/(me/mp)=1+(me/mp)1+(me/mDeut)EDeuteriumEHydrogen=1+(9.11×10-31/1.673×10-27)1+(9.11×10-31/2×1.673×10-27)=1.00027

Hence, the ground state energy of hydrogen is less than 0.027% of the ground state energy of Deuterium.

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Most popular questions from this chapter

Consider two particles that experience a mutual force but no external forces. The classical equation of motion for particle 1 is v˙1=F2on1/m1, and for particle 2 is v˙2=F1on2/m2, where the dot means a time derivative. Show that these are equivalent to v˙cm=constant, and v˙rel=FMutual/μ .Where, v˙cm=(m1v˙1+m2v˙2)/(m1m2),FMutual=-Fion2andμ=m1m2(m1+m2).

In other words, the motion can be analyzed into two pieces the center of mass motion, at constant velocity and the relative motion, but in terms of a one-particle equation where that particle experiences the mutual force and has the “reduced mass” μ.

Classically, an orbiting charged particle radiates electromagnetic energy, and for an electron in atomic dimensions, it would lead to collapse in considerably less than the wink of an eye.

(a) By equating the centripetal and Coulomb forces, show that for a classical charge -e of mass m held in a circular orbit by its attraction to a fixed charge +e, the following relationship holds

ω=er-3/24πε0m.

(b) Electromagnetism tells us that a charge whose acceleration is a radiates power P=e2a2/6ε0c3. Show that this can also be expressed in terms of the orbit radius as P=e696π2ε03m2c3r4. Then calculate the energy lost per orbit in terms of r by multiplying the power by the period T=2π/ωand using the formula from part (a) to eliminate .

(c) In such a classical orbit, the total mechanical energy is half the potential energy, or Eorbit=-e28πε0r. Calculate the change in energy per change in r : dEorbit/dr. From this and the energy lost per obit from part (b), determine the change in per orbit and evaluate it for a typical orbit radius of 10-10m. Would the electron's radius change much in a single orbit?

(d) Argue that dividing dEorbit/dr by P and multiplying by dr gives the time required to change r by dr . Then, sum these times for all radii from rinitial to a final radius of 0. Evaluate your result for rinitial=10-10m. (One limitation of this estimate is that the electron would eventually be moving relativistically).

Spectral lines are fuzzy due to two effects: Doppler broadening and the uncertainty principle. The relative variation in wavelength due to the first effect (see Exercise 2.57) is given by

λλ=3kBT/mc

Where T is the temperature of the sample and m is the mass of the particles emitting the light. The variation due to the second effect (see Exercise 4.72) is given by

λλ=λ4πc

Where, t is the typical transition time

(a) Suppose the hydrogen in a star has a temperature of 5×104K. Compare the broadening of these two effects for the first line in the Balmer series (i.e.,ni=3nf=2 ). Assume a transition time of 10-8s. Which effect is more important?

(b) Under what condition(s) might the other effect predominate?

Question: Consider a cubic 3D infinite well of side length of L. There are 15 identical particles of mass m in the well, but for whatever reason, no more than two particles can have the same wave function. (a) What is the lowest possible total energy? (b) In this minimum total energy state, at what point(s) would the highest energy particle most likely be found? (Knowing no more than its energy, the highest energy particle might be in any of multiple wave functions open to it and with equal probability.)

Question: The kinetic energy of hydrogen atom wave functions for which lis its minimum value of 0 is all radial. This is the case for the 1s and 2s states. The 2 p state has some rotational kinetic energy and some radial. Show that for very large n, the states of largest allowed lhave essentially no radial kinetic energy. Exercise 55 notes that the expectation value of the kinetic energy (including both rotational and radial) equals the magnitude of the total energy. Compare this magnitude with the rotational energy alone,L2/2mr2
,assuming that n is large. That lis as large as it can be, and thatrn2a0.

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