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In general, we might say that the wavelengths allowed a bound particle are those of a typical standing wave,λ=2L/n , where is the length of its home. Given that λ=h/p, we would have p=nh/2L, and the kinetic energy, p2/2m, would thus be n2h2/8mL2. These are actually the correct infinite well energies, for the argumentis perfectly valid when the potential energy is 0 (inside the well) and is strictly constant. But it is a pretty good guide to how the energies should go in other cases. The length allowed the wave should be roughly the region classically allowed to the particle, which depends on the “height” of the total energy E relative to the potential energy (cf. Figure 4). The “wall” is the classical turning point, where there is nokinetic energy left: E=U. Treating it as essentially a one-dimensional (radial) problem, apply these arguments to the hydrogen atom potential energy (10). Find the location of the classical turning point in terms of E , use twice this distance for (the electron can be on both on sides of the origin), and from this obtain an expression for the expected average kinetic energies in terms of E . For the average potential, use its value at half the distance from the origin to the turning point, again in terms of . Then write out the expected average total energy and solve for E . What do you obtain

for the quantized energies?

Short Answer

Expert verified

The energies of a particle trapped inside a Hydrogen atom are E=6me4n2h2π2ε02

Step by step solution

01

Given data

The momentum of a particle classically bound in a region of length L is

p=nh2L ..... (I)

Here h is the Planck's constant.

02

Hydrogen atom potential energy

The potential energy of a Hydrogen atom of radius r is

U=-e24πε0r ..... (II)

Here e is the magnitude of charge of an electron and ε0 is the permittivity of free space.

03

Step 3:Determining the total energy of a particle stuck inside a Hydrogen atom radius

From equation (II) the radius at which the kinetic energy is zero is

E=e24πε0rmaxrmax=e24πε0E

The classically allowed region is twice this value, that is

L=2rmax=2e24πε0E=e22πε0E

From equation (I), the momentum is

p=nh2×e22πε0E=nhπε0Ee2

The kinetic energy is

T=p22m=nhπε0Ee222m=n2h2π2ε02E22me4

From equation (II), the potential energy at half the classical limit is

Ur=rmax2=-e24πε0rmax2=-e24πε0×12×e24πε0E=-2E

The total energy is then

E=T+U=n2h2π2ε02E22me4-2E3E=n2h2π2ε02E22me4E=6me4n2h2π2ε02

Thus the quantized energies are E=6me4n2h2π2ε02.

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Most popular questions from this chapter

Question: Show that the angular normalization constant in Table 7.3 for the case (l,ml)=(1,0) is correct.

In Table 7.5, the pattern that develops with increasing n suggests that the number of different sets ofl,mlvalues for a given energy level n isn2. Prove this mathematically by summing the allowed values ofmlfor a givenlover the allowed values oflfor a given n.

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.)

Calculate the electric dipole moment p and estimate the transition time for a hydrogen atom electron making an electric dipole transition from the to the (n,l,m)=(2,1,+1) ground state. Comment on the relationship of the result to that in Example 7.11.

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?

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