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Chapter 30: Atomic Physics

38 problems · 5 figures

30-1 §30.1 source ↗

Using the given charge-to-mass ratios for electrons and protons, and knowing the magnitudes of their charges are equal, what is the ratio of the proton’s mass to the electron’s? (Note that since the charge-to-mass ratios are given to only three-digit accuracy, your answer may differ from the accepted ratio in the fourth digit.)

Answer

1 . 84 × 10 3

30-3 §30.1 source ↗

If someone wanted to build a scale model of the atom with a nucleus 1.00 m in diameter, how far away would the nearest electron need to be?

Answer

50 km

30-4 §30.2 source ↗

Rutherford found the size of the nucleus to be about 10−15 m. This implied a huge density. What would this density be for gold?

Answer

6 × 10 20 kg/m 3

30-6 §30.2 source ↗

(a) An aspiring physicist wants to build a scale model of a hydrogen atom for her science fair project. If the atom is 1.00 m in diameter, how big should she try to make the nucleus?

(b) How easy will this be to do?

Answer

(a) 10.0 μm

(b) It isn’t hard to make one of approximately this size. It would be harder to make it exactly 10.0 μm .

30-7 §30.3 source ↗

By calculating its wavelength, show that the first line in the Lyman series is UV radiation.

Answer

1λ= R1nf2−1ni2⇒λ= 1R(ni⋅nf)2ni2−nf2;ni= 2,nf= 1, so that

λ= m 1.097 × 10 7 ( 2 × 1 ) 2 2 2 − 1 2 = 1.22×10−7 m= 122 nm , which is UV radiation.

30-9 §30.3 source ↗

Look up the values of the quantities in aB= h24π2mekqe2, and verify that the Bohr radius aB is 0.529×10−10 m.

Answer

a B = h 2 4π 2 m e kZq e 2 = ( 6.626 × 10 − 34 J·s ) 2 4π 2 ( 9.109 × 10 − 31 kg ) ( 8.988 × 10 9 N · m 2 / C 2 ) ( 1 ) ( 1.602 × 10 − 19 C ) 2 = 0.529× 10 − 10 m

30-11 §30.3 source ↗

If a hydrogen atom has its electron in the n=4 state, how much energy in eV is needed to ionize it?

Answer

0.850 eV

30-13 §30.3 source ↗

Find the radius of a hydrogen atom in the n=2 state according to Bohr’s theory.

Answer

2.12 × 10 –10 m

30-15 §30.3 source ↗

What is the smallest-wavelength line in the Balmer series? Is it in the visible part of the spectrum?

Answer

365 nm

It is in the ultraviolet.

30-17 §30.3 source ↗

Do the Balmer and Lyman series overlap? To answer this, calculate the shortest-wavelength Balmer line and the longest-wavelength Lyman line.

Answer

No overlap

365 nm

122 nm

30-19 §30.3 source ↗

A wavelength of 4.653 μm is observed in a hydrogen spectrum for a transition that ends in the nf=5 level. What was ni for the initial level of the electron?

Answer

7

30-21 §30.3 source ↗

A beryllium ion with a single electron (denoted Be3+) is in an excited state with radius the same as that of the ground state of hydrogen.

(a) What is n for the Be3+ ion?

(b) How much energy in eV is needed to ionize the ion from this excited state?

Answer

(a) 2

(b) 54.4 eV

30-23 §30.3 source ↗

Verify Equations rn=n2ZaB and aB= h24π2mekqe2= 0.529×10−10 m using the approach stated in the text. That is, equate the Coulomb and centripetal forces and then insert an expression for velocity from the condition for angular momentum quantization.

Answer

kZqe2rn2= meV2rn , so that rn= kZqe2meV2= kZqe2me1V2. From the equation mevrn=nh2π , we can substitute for the velocity, giving: rn= kZqe2me⋅4π2me2rn2n2h2 so that rn= n2Zh24π2mekqe2= n2ZaB , where aB= h24π2mekqe2.

30-25 §30.4 source ↗

(a) What is the shortest-wavelength x-ray radiation that can be generated in an x-ray tube with an applied voltage of 50.0 kV? (b) Calculate the photon energy in eV. (c) Explain the relationship of the photon energy to the applied voltage.

Answer

(a) 0.248× 10 −10 m

(b) 50.0 keV

(c) The photon energy is simply the applied voltage times the electron charge, so the value of the voltage in volts is the same as the value of the energy in electron volts.

30-27 §30.4 source ↗

An x ray tube has an applied voltage of 100 kV. (a) What is the most energetic x-ray photon it can produce? Express your answer in electron volts and joules. (b) Find the wavelength of such an X–ray.

Answer

(a) 100×103eV, 1.60×10−14J

(b) 0.124×10−10 m

30-29 §30.4 source ↗

What are the approximate energies of the Kα and Kβ x rays for copper?

Answer

(a) 8.00 keV

(b) 9.48 keV

30-30 §30.5 source ↗

Figure 30.37 shows the energy-level diagram for neon. (a) Verify that the energy of the photon emitted when neon goes from its metastable state to the one immediately below is equal to 1.96 eV. (b) Show that the wavelength of this radiation is 633 nm. (c) What wavelength is emitted when the neon makes a direct transition to its ground state?
Figure 30.37 in the book ↗
Energy levels in helium and neon. In the common helium-neon laser, an electrical discharge pumps energy into the metastable states of both atoms. The gas mixture has about ten times more helium atoms than neon atoms. Excited helium atoms easily de-excite by transferring energy to neon in a collision. A population inversion in neon is achieved, allowing lasing by the neon to occur.

Answer

(a) 1.96 eV

(b) ( 1240 eV·nm ) / ( 1 . 96 eV ) = 633 nm

(c) 60.0 nm

30-32 §30.5 source ↗

Ruby lasers have chromium atoms doped in an aluminum oxide crystal. The energy level diagram for chromium in a ruby is shown in Figure 30.59. What wavelength is emitted by a ruby laser?
Figure 30.59 in the book ↗
Chromium atoms in an aluminum oxide crystal have these energy levels, one of which is metastable. This is the basis of a ruby laser. Visible light can pump the atom into an excited state above the metastable state to achieve a population inversion.

Answer

693 nm

30-34 §30.5 source ↗

Some of the most powerful lasers are based on the energy levels of neodymium in solids, such as glass, as shown in Figure 30.60. (a) What average wavelength light can pump the neodymium into the levels above its metastable state? (b) Verify that the 1.17 eV transition produces 1.06 μm radiation.
Figure 30.60 in the book ↗
Neodymium atoms in glass have these energy levels, one of which is metastable. The group of levels above the metastable state is convenient for achieving a population inversion, since photons of many different energies can be absorbed by atoms in the ground state.

Answer

(a) 590 nm

(b) ( 1240 eV·nm ) / ( 1 . 17 eV ) = 1.06 μm

30-35 §30.8 source ↗

If an atom has an electron in the n=5 state with ml=3, what are the possible values of l?

Answer

l=4, 3 are possible since l<n and ∣ml∣≤l.

30-37 §30.8 source ↗

What are the possible values of ml for an electron in the n=4 state?

Answer

n= 4⇒l= 3, 2, 1, 0⇒ml= ±3,±2, ±1, 0 are possible.

30-39 §30.8 source ↗

(a) Calculate the magnitude of the angular momentum for an l=1 electron. (b) Compare your answer to the value Bohr proposed for the n=1 state.

Answer

(a) 1.49×10−34 J⋅s

(b) 1.06×10−34 J⋅s

30-41 §30.8 source ↗

Repeat Exercise 30.40 for l=3.

Answer

(a) 3.66×10−34 J⋅s

(b) s= 9.13×10−35 J⋅s

(c) LS=123/4=4

30-43 §30.8 source ↗

What angles can the spin s of an electron make with the z-axis?

Answer

θ= 54.7º, 125.3º

30-44 §30.9 source ↗

(a) How many electrons can be in the n=4 shell?

(b) What are its subshells, and how many electrons can be in each?

Answer

(a) 32. (b) 2 in s, 6 in p, 10 in d, and 14 in f, for a total of 32.

30-46 §30.9 source ↗

(a) If one subshell of an atom has 9 electrons in it, what is the minimum value of l? (b) What is the spectroscopic notation for this atom, if this subshell is part of the n=3 shell?

Answer

(a) 2

(b) 3d9

30-48 §30.9 source ↗

Which of the following spectroscopic notations are not allowed? (a) 5 s 1 (b) 1 d 1 (c) 4 s 3 (d) 3 p 7 (e) 5 g 15 . State which rule is violated for each that is not allowed.

Answer

(b) n≥l is violated,

(c) cannot have 3 electrons in s subshell since 3> (2l+1)= 2

(d) cannot have 7 electrons in p subshell since 7> (2l+1)= 2(2+1)= 6

30-50 §30.9 source ↗

(a) Using the Pauli exclusion principle and the rules relating the allowed values of the quantum numbers n,l,ml,ms, prove that the maximum number of electrons in a subshell is 2n2.

(b) In a similar manner, prove that the maximum number of electrons in a shell is 2n2.

Answer

(a) The number of different values of ml is ±l,±(l−1), ...,0 for each l>0 and one for l=0⇒(2l+1). Also an overall factor of 2 since each ml can have ms equal to either +1/2 or − 1/2⇒2(2l+1).

(b) for each value of l, you get 2(2l+1)

= 0, 1, 2, ...,(n–1)⇒2(2)(0)+1+(2)(1)+1+....+(2)(n−1)+1= 21+3+...+(2n−3)+(2n−1) ︸ n terms to see that the expression in the box is =n2, imagine taking (n−1) from the last term and adding it to first term = 21+(n–1)+3+...+(2n−3)+(2n−1)–(n−1)= 2n+3+....+(2n−3)+n. Now take (n−3) from penultimate term and add to the second term 2n+n+...+n+n ︸ n terms = 2n2.

30-52 §30.9 source ↗

Integrated Concepts

The electric and magnetic forces on an electron in the CRT in Figure 30.7 are supposed to be in opposite directions. Verify this by determining the direction of each force for the situation shown. Explain how you obtain the directions (that is, identify the rules used).

Figure 30.7 in the book ↗
This schematic shows the electron beam in a CRT passing through crossed electric and magnetic fields and causing phosphor to glow when striking the end of the tube.

Answer

The electric force on the electron is up (toward the positively charged plate). The magnetic force is down (by the RHR).

30-54 §30.9 source ↗

Integrated Concepts

A galaxy moving away from the earth has a speed of 0.0100c . What wavelength do we observe for an ni=7 to nf=2 transition for hydrogen in that galaxy?

Answer

401 nm

30-56 §30.9 source ↗

Integrated Concepts

In a Millikan oil-drop experiment using a setup like that in Figure 30.9, a 500-V potential difference is applied to plates separated by 2.50 cm. (a) What is the mass of an oil drop having two extra electrons that is suspended motionless by the field between the plates? (b) What is the diameter of the drop, assuming it is a sphere with the density of olive oil?

Figure 30.9 in the book ↗
The Millikan oil drop experiment produced the first accurate direct measurement of the charge on electrons, one of the most fundamental constants in nature. Fine drops of oil become charged when sprayed. Their movement is observed between metal plates with a potential applied to oppose the gravitational force. The balance of gravitational and electric forces allows the calculation of the charge on a drop. The charge is found to be quantized in units of −1.6 × 10 −19 C , thus determining directly the charge of the excess and missing electrons on the oil drops.

Answer

(a) 6.54×10−16 kg

(b) 5.54×10−7 m

30-58 §30.9 source ↗

Integrated Concepts

In a laboratory experiment designed to duplicate Thomson’s determination of qe/me, a beam of electrons having a velocity of 6.00×107m/s enters a 5.00×10−3T magnetic field. The beam moves perpendicular to the field in a path having a 6.80-cm radius of curvature. Determine qe/me from these observations, and compare the result with the known value.

Answer

1 . 76 × 10 11 C/kg , which agrees with the known value of 1 . 759 × 10 11 C/kg to within the precision of the measurement

30-60 §30.9 source ↗

Integrated Concepts

Particles called muons exist in cosmic rays and can be created in particle accelerators. Muons are very similar to electrons, having the same charge and spin, but they have a mass 207 times greater. When muons are captured by an atom, they orbit just like an electron but with a smaller radius, since the mass in aB= h24π2mekqe2= 0.529×10−10 m is 207 me.

(a) Calculate the radius of the n=1 orbit for a muon in a uranium ion (Z=92).

(b) Compare this with the 7.5-fm radius of a uranium nucleus. Note that since the muon orbits inside the electron, it falls into a hydrogen-like orbit. Since your answer is less than the radius of the nucleus, you can see that the photons emitted as the muon falls into its lowest orbit can give information about the nucleus.

Answer

(a) 2.78 fm

(b) 0.37 of the nuclear radius.

30-62 §30.9 source ↗

Integrated Concepts

A carbon dioxide laser used in surgery emits infrared radiation with a wavelength of 10.6 μm . In 1.00 ms, this laser raised the temperature of 1.00 cm3 of flesh to 100ºC and evaporated it.

(a) How many photons were required? You may assume flesh has the same heat of vaporization as water. (b) What was the minimum power output during the flash?

Answer

(a) 1.34×1023

(b) 2.52 MW

30-64 §30.9 source ↗

Integrated Concepts

(a) An excimer laser used for vision correction emits 193-nm UV. Calculate the photon energy in eV.

(b) These photons are used to evaporate corneal tissue, which is very similar to water in its properties. Calculate the amount of energy needed per molecule of water to make the phase change from liquid to gas. That is, divide the heat of vaporization in kJ/kg by the number of water molecules in a kilogram.

(c) Convert this to eV and compare to the photon energy. Discuss the implications.

Answer

(a) 6.42 eV

(b) 7.27×10−20 J/molecule

(c) 0.454 eV, 14.1 times less than a single UV photon. Therefore, each photon will evaporate approximately 14 molecules of tissue. This gives the surgeon a rather precise method of removing corneal tissue from the surface of the eye.

30-66 §30.9 source ↗

Integrated Concepts

A pulsar is a rapidly spinning remnant of a supernova. It rotates on its axis, sweeping hydrogen along with it so that hydrogen on one side moves toward us as fast as 50.0 km/s, while that on the other side moves away as fast as 50.0 km/s. This means that the EM radiation we receive will be Doppler shifted over a range of ±50.0 km/s. What range of wavelengths will we observe for the 91.20-nm line in the Lyman series of hydrogen? (Such line broadening is observed and actually provides part of the evidence for rapid rotation.)

Answer

91.18 nm to 91.22 nm

30-68 §30.9 source ↗

Unreasonable Results

(a) What voltage must be applied to an X-ray tube to obtain 0.0100-fm-wavelength X-rays for use in exploring the details of nuclei? (b) What is unreasonable about this result? (c) Which assumptions are unreasonable or inconsistent?

Answer

(a) 1.24×1011 V

(b) The voltage is extremely large compared with any practical value.

(c) The assumption of such a short wavelength by this method is unreasonable.

30-72 §30.9 source ↗

Critical Thinking (a) For carbon, calculate the energy when an electron falls from n=3 to n=2, then from n=2 to n=1. Then add these for the total energy released in the process. (b) Calculate the energy released when the electron falls directly from n=3 to n=1. (c) Are the energies in part a and in part b the same?

Answer

(a) E=− z 2  n 2 E 3 − E 2 =− 6 2 3 2 − 6 2 2 2 13.6eV=68.0eV                E 3 − E 2 =− 6 2 2 2 − 6 2 1 2 13.6eV=367eV E=435eV

(b) E 3 − E 2 = − 6 2 3 2 − 6 2 1 2 13.6eV= 435eV

(c) Yes.

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Problems and answers are adapted from College Physics 2e by Paul Peter Urone, Roger Hinrichs, Kim Dirks and Manjula Sharma, OpenStax, and are used under the CC BY-NC-SA 4.0 licence. Access for free at https://openstax.org/books/college-physics-2e/pages/1-introduction-to-science-and-the-realm-of-physics-physical-quantities-and-units. Illustrations: Copyright Rice University, OpenStax, under CC BY-NC-SA 4.0 license. This adaptation is released under the same licence, is non-commercial, and is neither affiliated with nor endorsed by OpenStax or Rice University.