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Physics for Scientists and Engineers with Modern Physics

Raymond A. Serway, John W. Jewett, Jr.

Chapter 44

Nuclear Structure - all with Video Answers

Educators


Chapter Questions

02:34

Problem 1

What is the order of magnitude of the number of protons in your body? Of the number of neutrons? Of the number of electrons?

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07:26

Problem 2

Review problem. Singly ionized carbon is accelerated through 1000 $\mathrm{V}$ and passed into a mass spectrometer to determine the isotopes present (see Chapter 29 ). The magnitude of the magnetic field in the spectrometer is 0.200 $\mathrm{T}$ (a) Determine the orbit radii for the 12 $\mathrm{C}$ and the 13 $\mathrm{C}$ isotopes as they pass through the field. (b) Show that the ratio of radii may be written in the form
$$
\frac{r_{1}}{r_{2}}=\sqrt{\frac{m_{1}}{m_{2}}}
$$
and verify that your radii in part (a) agree with this equation.

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06:50

Problem 3

(a) What fraction of the space in a tank of hydrogen gas at $0^{\circ} \mathrm{C}$ and 1 atm is occupied by the hydrogen molecules themselves? Assume each hydrogen atom is a sphere with diameter 0.100 $\mathrm{nm}$ and a hydrogen molecule consists of two such spheres in contact. (b) What fraction of the space within one hydrogen atom is occupied by its nucleus, of radius 1.20 $\mathrm{fm}$ ?

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05:54

Problem 4

In a Rutherford scattering experiment, alpha particles having kinetic energy of 7.70 $\mathrm{MeV}$ are fired toward a gold nucleus. (a) Use energy conservation to determine the distance of closest approach between the alpha particle the and gold nucleus. Assume the nucleus remains at rest. (b) What If? Calculate the de Broglic wavelength for the 7.70 -MeV alpha particle and compare it with the distance
obtained in part (a). (c) Based on this comparison, why is it proper to treat the alpha particle as a particle and not as a wave in the Rutherford scattering experiment?

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05:34

Problem 5

(a) Use energy methods to calculate the distance of closest approach for a head-on collision between an alpha particle having an initial energy of 0.500 $\mathrm{MeV}$ and a gold nucleus ( 197 $\mathrm{Au} )$ at rest. Assume the gold nucleus remains at rest during the collision. (b) What minimum initial speed must the alpha particle have to get as close as 300 $\mathrm{fm}$ ?

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01:36

Problem 6

Find the radius of (a) a nucleus of ${ }_{2}^{4} \mathrm{He}$ and (b) a nucleus of ${ }_{92}^{288} \mathrm{U}$

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01:59

Problem 7

A star ending its life with a mass of two times the Sun's mass is expected to collapse, combining its protons and electrons to form a neutron star. Such a star could be thought of as a gigantic atomic nucleus. If a star of mass $2 \times 1.99 \times 10^{10} \mathrm{kg}$ collapsed into neutrons $\left(m_{m}=\right.$ $1.67 \times 10^{-27} \mathrm{kg} ),$ what would its radius be? Assume $r=$ $r_{0} A^{1 / 3}$

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03:11

Problem 8

Review problem. What would be the gravitational force exerted by each of two golf balls on the other if they were made of nuclear matter? Assume each ball has a $4.30-\mathrm{cm}$ diameter and they are 1.00 $\mathrm{m}$ apart.

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07:15

Problem 9

Calculate the binding energy per nucleon for (a) $^{2} \mathrm{H}$ , (b) $^{4} \mathrm{He},$ (c) $^{56} \mathrm{Fe},$ and $(\mathrm{d})^{2 \mathrm{ss}} \mathrm{U}$

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07:40

Problem 10

The iron isotope stife is near the peak of the stability curve. That is the fundamental reason that iron is more common in the Universe than heavier elements, as the spectra of the Sun and of many other stars reveal. Show that $\$ 6$ has a higher binding energy per nucleon than its neighbors $\$ 0 \mathrm{Mn}$ and $\$ 9 \mathrm{Co}$ . State how your results compare with Figure $44.5 .$

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05:05

Problem 11

Assume a hydrogen atom is a sphere with diameter $0.100 \mathrm{nm}$ and a hydrogen molecule consists of two such spheres in contact.
(a) What fraction of the space in a tank of hydrogen gas at $0^{\circ} \mathrm{C}$ and $1.00 \mathrm{~atm}$ is occupied by the hydrogen molecules themselves?
(b) What fraction of the space within one hydrogen atom is occupied by its nucleus, of radius $1.20 \mathrm{fm} ?$

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04:44

Problem 12

Two nuclei having the same mass number are called isobars. Calculate the difference in binding energy per nucleon for the isobars 23 $\mathrm{Na}$ and $_{12}^{23} \mathrm{Mg}$ . How do you account for the difference?

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03:12

Problem 13

A pair of nuclei for which $Z_{1}=N_{2}$ and $Z_{2}=N_{1}$ are called mirror isobars (the atomic and neutron numbers are interchanged). Binding-cnergy measurements on these nuclei can be used to obtain cvidence of the charge independence of nuclear forces (that is, proton-proton. proton-neutron, and neutron-neutron nuclear forces are equal). Calculate the difference in binding energy for the two mirror isobars 150 and 15 $\mathrm{N}$ . The electric repulsion among eight protons rather than seven accounts for the difference.

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05:44

Problem 14

The energy required to construct a uniformly charged sphere of total charge $Q$ and radius $R$ is $U=3 k, Q^{2} / 5 R,$ where $k,$ is the Coulomb constant (see Problem 64 ). Assume a 40 . Ca nucleus contains 20 protons uniformly distributed in a spherical volume. (a) How much energy is required to counter their electrical repulsion according to the above equation? Suggestion: First calculate the radius of a "Ca nucleus. (b) Calculate the binding energy of $? 0$ Ca. (c) Explain what you can conclude from comparing the result of part (b) with that of part (a).

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02:44

Problem 15

Calculate the minimum energy required to remove a neutron from the $\frac{13}{20} \mathrm{Ca}$ nucleus.

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04:11

Problem 16

(a) In the liquid-drop model of nuclear structure, why does the surfaceffect term $-C_{2} A^{2 / 3}$ have a negative sign? (b) What If? The binding energy of the nucleus increases as the volume-to-surface ratio increases. Calculate this ratio for both spherical and cubical shapes and explain which is more plausible for nuclei.

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02:33

Problem 17

Using the graph in Figure $44.5,$ estimate how much cnergy is released when a nucleus of mass number 200 fissions into two nuclei each of mass number 100 .

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05:24

Problem 18

(a) Use the semiempirical binding-energy formula to compute the binding energy for $\frac{56}{26} \mathrm{Fe}$ . (b) What percentage is contributed to the binding energy by each of the four terms?

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01:33

Problem 19

A sample of radioactive material contains $1.00 \times 10^{15}$ atoms and has an activity of $6.00 \times 10^{11} \mathrm{Bq}$ . What is its half-ife?

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01:29

Problem 20

The half-life of 131 $\mathrm{I}$ is 8.04 days. On a certain day, the activity of an iodine-131 sample is 6.40 $\mathrm{mCi}$ . What is its activity 40.2 days later?

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05:23

Problem 21

A freshly prepared sample of a certain radioactive isotop has an activity of 10.0 $\mathrm{mCi}$ . After 4.00 $\mathrm{h}$ , its activity 8.00 $\mathrm{mCi}$ . (a) Find the decay constant and half-life (b) How many atoms of the isotope were contained in th freshly prepared sample? (c) What is the sample's activity
30.0 $\mathrm{h}$ after it is prepared?

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02:54

Problem 22

From the equation expressing the law of radioactive decay, derive the following useful formulas for the decay constant and the half-life, in terms of the time interval $\Delta t$ during which the decay rate decreases from $R_{0}$ to $R :$
$$
\lambda=\frac{1}{\Delta l} \ln \left(\frac{R_{0}}{R}\right) \quad T_{1 / 2}=\frac{(\ln 2) \Delta t}{\ln \left(R_{0} / R\right)}
$$

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05:27

Problem 23

The radioactive isotope 198 $\mathrm{Au}$ has a half-life of 64.8 $\mathrm{h.} \mathrm{A}$ sample containing this isotope has an initial activity $(t=0)$ of 40.0$\mu \mathrm{Ci}$ . Calculate the number of nuclei that decay in the time interval between $t_{1}=10.0 \mathrm{h}$ and $t_{2}=12.0 \mathrm{h} .$

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02:46

Problem 24

A radioactive nucleus has half-life $T_{1 / 2}$ . A sample contaiing these nuclei has initial activity $R_{0}$ . Calculate the number of nuclei that decay during the interval between the times $t_{1}$ and $t_{2}$ .

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02:50

Problem 25

Consider a radioactive sample. Determine the ratio of the number of nuclei decaying during the first half of its half- life to the number of nuclei decaying during the scondhalf of its half-life.

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19:50

Problem 26

(a) The daughter nucleus formed in radioactive decay is often radioactive. Let $N_{10}$ represent the number of parent nuclei at time $t=0, N_{1}(t)$ the number of parent nuclei at time $t,$ and $\lambda_{1}$ the decay constant of the parent. nuclei at time $t,$ and $\lambda_{1}$ the decay constant of the parent. Suppose the number of daughter nuclei at time $t=0$ is zero. Let $N_{2}(t)$ be the number of daughter nuclei at time t and let $\lambda_{2}$ be the decay constant of the daughter. Show that $N_{2}(t)$ satisfies the differential equation
$$
\frac{d N_{2}}{d t}=\lambda_{1} N_{1}-\lambda_{2} N_{2}
$$
(b) Verify by substitution that this differential equation
has the solution
$$
N_{2}(t)=\frac{N_{10} \lambda_{1}}{\lambda_{1}-\lambda_{2}}\left(e^{-\lambda_{2} t}-e^{-\lambda_{1}}\right)
$$
This equation is the law of successive radioactive decays. (c) $^{218}$ Po decays into $^{214} \mathrm{Pb}$ with a half-life of 3.10 $\mathrm{min}$ , and 214 Pb decays into $^{214}$ Bi with a half-life of 26.8 min. On the same axes, plot graphs of $N_{1}(t)$ for 218 $\mathrm{Po}$ and $N_{0}(t)$ for 214 Pb. Let $N_{10}=1000$ nuclei and choose values of $t$ from 0 to 36 $\mathrm{min}$ in 2 -min intervals. The curve for 214 $\mathrm{Pb}$ at first rises to a maximum and then starts to decay. At what instant $t_{\mathrm{m}}$ is the number of $^{214 \mathrm{Pb} \text { nuclei a maximum? (d) By }}$ applying the condition for a maximum $d N_{2} / d t=0,$ derive a symbolic equation for $t_{m}$ in terms of $\lambda_{1}$ and $\lambda_{2}$ . Explain whether the value obtained in part (c) agrees with this equation.

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05:01

Problem 27

In an experiment on the transport of nutrients in the root structure of a plant, two radioactive nuclides $\mathrm{X}$ and $\mathrm{Y}$ are used. Initially, 2.50 times more nuclei of type $\mathrm{X}$ and $\mathrm{Y}$ present than of type Y Precisely three days later, there are 4.20 times more nuclei of type $\mathrm{X}$ than of type $\mathrm{Y}$ . Isotope $\mathrm{Y}$ has a half-life of $1.60 \mathrm{d} .$ What is the half-life of isotope $\mathrm{X}$ ?

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04:15

Problem 28

Identify the missing nuclide or particle $(\mathrm{X}) :$
(a) $\mathrm{X} \rightarrow_{28}^{65} \mathrm{Ni}+\gamma$
(b) $\frac{215}{84} \mathrm{PO} \rightarrow \mathrm{X}+\alpha$
(c) $\mathrm{X} \rightarrow \underset{2 \mathrm{b}}{\mathrm{s}} \mathrm{Fe}+\mathrm{c}^{+}+\nu$
(d) $_{48}^{109} \mathrm{Cd}+\mathrm{X} \rightarrow_{47}^{109} \mathrm{Ag}+\nu$
(e) $14 \mathrm{N}+\frac{4}{2} \mathrm{He} \rightarrow \mathrm{X}+\frac{17}{8} \mathrm{O}$

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02:12

Problem 29

Find the energy released in the alpha decay
EQUATION NOT COPY
You will find Table 14.2 useful.

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08:00

Problem 30

A living specimen in equilibrium with the atmosphere contains one atom of $^{14} \mathrm{C}$ (half-life = 5730 y) for every $7.7 \times 10^{11}$ stable carbon atoms. An archeological sample of wood (cellulose, $\mathrm{C}_{12} \mathrm{H}_{22} \mathrm{O}_{11} )$ contains 21.0 $\mathrm{mg}$ of carbon. When the sample is placed inside a shielded beta counter with 88.0$\%$ counting efficiency, 837 counts are
accumulated in one week. Assuming the cosmic-ray flux and the Farth's atmosphere have not changed appreciably since the sample was formed, find the age of the sample.

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07:10

Problem 31

A sample consists of $1.00 \times 10^{6}$ radioactive nuclei with a half-life of 10.0 h. No other nuclei are present at time $l=0 .$ The stable daughter nuclei accumulate in the sample as time goes on. (a) Derive an equation giving the number of daughter nuclei $N_{d}$ as a function of time. (b) Sketch or describe a graph of the number of daughter nuclei as a function of time. What are the maximum and minimum numbers of daughter nuclei, and when do they occur? What are the maximum and minimum rates of change in the number of daughter nuclei, and when do they occur?

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02:46

Problem 32

A $^{3} \mathrm{H}$ nucleus beta decays into 3 $\mathrm{He}$ by creating an electron and an antineutrino according to the reaction
$$
_{1}^{3} \mathbf{H} \rightarrow_{2}^{3} \mathbf{H} \mathbf{c}+\mathbf{c}^{-}+\overline{\nu}
$$
The symbols in this reaction refer to nuclei. Write the reaction referring to neutral atoms by adding one clectron to both sides. Then use Table 44.2 to determine the total energy released in this reaction.

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04:01

Problem 33

The nucleus is 0 decays by electron capture. The nuclear reaction is written
$$
_{8}^{15} \mathrm{O}+\mathrm{e}^{-} \rightarrow_{7}^{15} \mathrm{N}+v
$$
(a) Write the process going on for a single particle within the nucleus. (b) Write the decay process referring to neutral atoms. (c) Determine the cnergy of the neutrino. Dis- regard the daughter's recoil.

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06:21

Problem 34

Determinc which decays can occur spontancously:
(a) $_{20}^{40} \mathrm{Ca} \rightarrow \mathrm{e}^{+}+_{19}^{40} \mathrm{K}$
Equation canno't copy

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07:07

Problem 35

Enter the correct isotope symbol in each open square in Figure $\mathrm{P} 44.35,$ which shows the sequences of decays in the natural radioactive series starting with the long-lived iso- tope uranium- 235 and ending with the stable nucleus lead- 207 .

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11:02

Problem 36

A rock sample contains traces of $^{298} \mathrm{U}, 235 \mathrm{U}, 2 \mathrm{s} 2 \mathrm{Th}, 208 \mathrm{Pb}$ $207 \mathrm{Pb},$ and 206 $\mathrm{Pb}$ . Analysis shows that the ratio of the amount of $^{238} \mathrm{U}$ to $^{206} \mathrm{Pb}$ is 1.164 . (a) Assuming the rock originally contained no lead, determine the age of the rock. (b) What should be the ratios of $^{235} \mathrm{U}$ to $^{207} \mathrm{Pb}$ and of $^{234} \mathrm{Th}$ to 20 $\mathrm{sPb}$ so that they would yield the same age for the rock? Ignore the minute amounts of the intermediate decay products in the decay chains. Note: This form of multiple dating gives reliable geological dates.

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05:15

Problem 37

Indocr air pollution. Uranium is naturally present in rock and soil. At one step in its series of radioactive decays, $^{233} \mathrm{U}$ produces the chemically incrt gas radon- $222,$ with a half-life of 3.82 days. The radon sceps out of the ground to mix into the atmosphere, typically making open air radioactive with activity 0.3 $\mathrm{pCi} / \mathrm{L}$ . In homes, 222 $\mathrm{Rn}$ can be a serious pollutant, accumulating to reach much higher activities in enclosed spaces. If the radon radioactivity bexceeds $4 \mathrm{pCi} / \mathrm{L},$ the Environmental Protection Agency suggests taking action to reduce it, such as by reducing infiltration of air from the ground. (a) Convert the activity 4 $\mathrm{pCi} / \mathrm{L}$ to units of becquerels per cubic meter. (b) How many 22 $\mathrm{Rn}$ atoms are in one cubic meter of air displaying this activity? (c) What fraction of the mass of the air does the radon constitute?

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03:38

Problem 38

The most common isotope of radon is $22^{2} \mathrm{Rn}$ , which has half-life 3.82 days. (a) What fraction of the nuclei that were on the Earth one week ago are now undecayed? (b) Of those that existed one year ago? (c) In view of these results, explain why radon remains a problem, contributing significantly to our background radiation exposure.

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04:07

Problem 39

Identify the unknown nuclei and particles $\mathrm{X}$ and $\mathrm{X}^{\prime}$ in the following nuclear reactions:
(a) $\mathrm{X}+{ }_{2}^{4} \mathrm{He} \rightarrow{ }_{12}^{24} \mathrm{Mg}+{ }_{0}^{1} \mathrm{n}$
(b) ${ }_{92}^{295} \mathrm{U}+{ }_{0}^{1} \mathrm{n} \rightarrow{ }_{38}^{90} \mathrm{Sr}+\mathrm{X}+2{ }_{0}^{1} \mathrm{n}$
(c) $2{ }_{1}^{1} \mathrm{H} \rightarrow{ }_{1}^{2} \mathrm{H}+\mathrm{X}+\mathrm{X}^{\prime}$

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06:42

Problem 40

After determining that the Sun has existed for hundreds of millions of years, but before the discovery of nuclear physics, scientists could not explain why the Sun has continued to burn for such a long time interval. For example, if it were a coal fire, it would have burned up in about 3000 yr. Assume the Sun, whose mass is $1.99 \times 10^{30} \mathrm{kg}$ , originally consisted entirely of hydrogen and its total
power output is $3.85 \times 10^{96} \mathrm{W}$ . (a) Assuming the energy- generating mechanism of the Sun is the fusion of hydrogen into helium via the net reaction
$$
4\left(_{1}^{1} \mathrm{H}\right)+2\left(\mathrm{e}^{-}\right) \rightarrow_{2}^{4} \mathrm{He}+2 v+\gamma
$$
calculate the energy (in joules) given off by this reaction. (b) Determine how many hydrogen atoms constitute the Sun. Take the mass of one hydrogen atom to be $1.67 \times 10^{-27} \mathrm{kg} .$ (c) If the total power output remains converted into helium, making the Sun die? The actual projected lifetime of the Sun is about 10 billion years because only the hydrogen in a relatively small core is available as a fuel. Only in the core are temperatures and densities high enough for the fusion reaction to be self-sustaining.

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05:07

Problem 41

Natural gold has only one isotope, 79 $\mathrm{Au}$ . If natural gold is irradiated by a flux of slow neutrons, electrons are emitted. (a) Write the reaction equation. (b) Calculate the maximum energy of the emitted electrons.

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02:57

Problem 42

A beam of 6.61-MeV protons is incident on a target of $\frac{27}{13} \mathrm{Al}$ . Those that collide produce the reaction
$$
\mathrm{p}+\underset{13}{27} \mathrm{Al} \quad \rightarrow \quad_{11}^{27} \mathrm{Si}+\mathrm{n}
$$
Ignoring any recoil of the product nucleus, determine the kinetic energy of the emerging neutrons. You may use Table 44.2 .

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04:09

Problem 43

The following reactions are observed:
$$
_{i}^{9} \mathrm{Be}+\mathrm{n} \rightarrow_{1}^{10} \mathrm{Be}+\gamma \quad Q=6.812 \mathrm{MeV}
$$
$$
_{4}^{9} \mathrm{Be}+\gamma \rightarrow_{4}^{8 \mathrm{E}+\mathrm{n}} \quad Q=-1.665 \mathrm{MeV}
$$
Using the mass of "Be from Table 44.2 , calculate the masses of $^{8} \mathrm{Be}$ and $^{10} \mathrm{Be}$ in unified mass units to four decimal places.

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02:08

Problem 44

(a) Suppose $\frac{10}{5} \mathrm{B}$ is struck by an alpha particle, releasing a proton and a product nucleus in the reaction. What is the product nucleus? (b) An alpha particle and a product nucleus are produced when $\frac{13}{6} \mathrm{C}$ is struck by a proton. What is the product nucleus?

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03:16

Problem 45

The radio frequency at which a nucleus displays resonance absorption between spin states is called the Larmor frequency and is given by
$$
f=\frac{\Delta E}{h}=\frac{2 \mu B}{h}
$$
Calculate the Larmor frequency for (a) free neutrons in a magnetic ficld of 1.00 $\mathrm{T}$ , (b) free protons in a magnetic ficld of 1.00 $\mathrm{T}$ , and $\mathrm{c}$ ) free protons in the Earth's magnetic field at a location where the magnitude of the field is 50.0$\mu \mathrm{T}$ .

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06:51

Problem 46

Construct a diagram like that of Figure 44.18 for the cases when $I$ equals (a) $\frac{5}{2}$ and $(b) 4 .$

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03:16

Problem 47

(a) One method of producing neutrons for experimental use is bombardment of light nuclei with alpha particles. In the method used by James Chadwick in $1932,$ alpha particles emitted by polonium are incident on beryllium nuclei:
$$
{ }_{2}^{4} \mathrm{He}+{ }_{4}^{9} \mathrm{Be} \rightarrow{ }_{6}^{12} \mathrm{C}+{ }_{0}^{1} \mathrm{n}
$$
What is the $Q$ value? (b) Neutrons are also often produced by small-particle accelerators. In one design, deuterons accelerated in a Van de Graaff generator bombard other deuterium nuclei:
$$
{ }_{1}^{2} \mathrm{H}+{ }_{1}^{2} \mathrm{H} \rightarrow{ }_{2}^{3} \mathrm{He}+{ }_{0}^{1} \mathrm{n}
$$
Is this reaction exothermic or endothermic? Calculate its
$Q$ value.

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06:43

Problem 48

As part of his discovery of the neutron in 1932 , James Chadvick determined the mass of the newly identified particle by firing a beam of fast neutrons, all having the same speed, at two different targets and measuring the maximum recoil speeds of the target nuclei. The mum speeds arise when an elastic head-on collision occurs between a neutron and a stationary target nucleus. (a) Represent the masses and final speeds of the two target nuclei as $m_{1}, v_{1}, m_{2},$ and $v_{2}$ and assume Newtonian mechanics applics. Show that the neutron mass can becalculated from the cquation
$$
m_{n}=\frac{m_{1} v_{1}-m_{2} v_{2}}{v_{2}-v_{1}}
$$
(b) Chadwick directed a beam of neutrons (produced from a nuclear reaction) on parafin, which contains hydrogen. The maximum speed of the protons ejected was found to be $3.3 \times 10^{7} \mathrm{m} / \mathrm{s}$ . Because the velocity of the neutrons could not be determined directly, a second experiment was performed using neutrons from the same source and nitrogen nuclei as the target. The maximum recoil speed of the nitrogen nuclei was found to be $4.7 \times 10^{6} \mathrm{m} / \mathrm{s}$ . The masses of a proton and a nitrogen nucleus were taken as 1 $\mathrm{u}$ and 14 $\mathrm{u}$ , respectively. What was Chadwick's value for the neutron mass?

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03:54

Problem 49

When the nuclear reaction represented by Equation 44.27 is endothermic, the reaction energy $Q$ is negative. For the reaction to proceed, the incoming particle must have a minimum energy called the threshold energy, $E_{\mathrm{th}}$ . Some fraction of the energy of the incident particle is transferred to the compound nucleus to conscrve momentum. Therefore, $E_{\text { in }}$ must be greater than the magnitude of $Q$ (a) Show that
$$
E_{\mathrm{th}}=-Q\left(1+\frac{M_{\mathrm{a}}}{M_{\mathrm{X}}}\right)
$$
(b) Calculate the threshold energy of the incident alpha particle in the reaction
$$
_{2}^{4} \mathrm{He}+\frac{14}{7} \mathrm{N} \rightarrow_{8}^{17} \mathrm{O}+_{1}^{1} \mathrm{H}
$$

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05:14

Problem 50

Review problem. (a) Is the mass of a hydrogen atom in its ground state larger or smaller than the sum of the masses of a proton and an electron? (b) What is the mass difference? (c) How large is the difference as a percentage of the total mass: (d) Is it large chough to affect the value of the atomic mass listed to six decimal places in Table 44.2$?$

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02:37

Problem 51

Write the statement of a problem for which the following equation appears in the solution. Determine the value of the unknown in the equation and identify its meaning.
$$\begin{array}{rl}{10.012937 \mathrm{u}+4.002} & {603} & {\mathrm{u}} \\ {} & {=13.003355 \mathrm{u}+1.007825 \mathrm{u}+Q / c^{2}}\end{array}$$

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04:21

Problem 52

A by-product of some fission reactors is the isotope ${ }_{94}^{239} \mathrm{Pu}$, an alpha emitter having a half-life of 24120 yr:
$$
{ }_{94}^{239} \mathrm{Pu} \rightarrow{ }_{92}^{235} \mathrm{U}+\alpha
$$
Consider a sample of $1.00 \mathrm{~kg}$ of pure ${ }_{94}^{239} \mathrm{Pu}$ at $t=0 .$ Calculate (a) the number of ${ }_{94}^{239} \mathrm{Pu}$ nuclei present at $t=0$ and
(b) the initial activity in the sample. (c) What If? For what times interval does the sample have to be stored if a "safe" activity level is $0.100 \mathrm{~Bq}$ ?

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07:13

Problem 53

(a) Find the radius of the ${ }_{6}^{12} \mathrm{C}$ nucleus.
(b) Find the force of repulsion between a proton at the surface of a ${ }_{6}^{12} \mathrm{C}$ nucleus and the remaining five protons.
(c) How much work (in MeV) has to be done to overcome this electric repulsion in transporting the last proton from a large distance up to the surface of the nucleus?
(d) Repeat parts (a), (b), and (c) for ${ }_{92}^{238} \mathrm{U}$.

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08:03

Problem 54

(a) Find the radius of the 12 $\mathrm{C}$ nucleus. (b) Find the force of repulsion between a proton at the surface of a $\frac{12}{b} C$ nucleus and the remaining five protons. (c) How much work (in MeV) has to be done to overcome this electric repulsion in transporting the last proton from a large distance up to the surface of the nucleus? (d) Repeat parts (a) $,$ (b), and (c) for $_{\mathrm{g} 2}^{238} \mathrm{U}$

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05:15

Problem 55

(a) Why is the beta decay $\mathrm{p} \rightarrow \mathrm{n}+\mathrm{e}^{+}+v$ forbidden for a free proton? (b) What If? Why is the same reaction possible if the proton is bound in a nucleus? For example,
the following reaction occurs:
$$
_{7}^{13} \mathrm{N} \rightarrow_{6}^{13} \mathrm{C}+\mathrm{e}^{+}+\nu
$$
(c) How much energy is released in the reaction given in part (b)? Suggestion: Add seven electrons to both sides of the reaction to write it for neutral atoms. You may use Table 44.2 .

Ren Jie Tuieng
Ren Jie Tuieng
Numerade Educator
08:45

Problem 56

The activity of a radioactive sample was measured over 12 $\mathrm{h}$ , with the net count rates shown in the table.

Ren Jie Tuieng
Ren Jie Tuieng
Numerade Educator
05:40

Problem 57

After the sudden release of radioactivity from the Chernobyl nuclear reactor accident in 1986, the radioactivity of milk in Poland rose to 2 000 Bq/L due to iodine-131 present in the grass eaten by dairy cattle. Radioactive iodine, with half-life 8.04 days, is particularly hazardous because the thyroid gland concentrates iodine. The Chernobyl accident caused a measurable increase in thyroid cancers among children in Belarus. (a) For comparison, find the activity of milk due to potassium. Assume 1 liter of milk contains 2.00 g of potassium, of which 0.011 7% is the isotope 40K with a half-life 1.28 109 yr. (b) After
what elapsed time would the activity due to iodine fall below that due to potassium?

Ren Jie Tuieng
Ren Jie Tuieng
Numerade Educator
06:43

Problem 58

When, after a reaction or disturbance of any kind, a nucleus is left in an excited state, it can return to its normal (ground) state by emission of a gamma-ray photon (or several photons). This process is illustrated by Equation 44.24. The emitting nucleus must recoil to conserve both energy and momentum. (a) Show that the recoil energy of the nucleus is
$$
E_{,}=\frac{(\Delta E)^{2}}{2 M c^{2}}
$$
where $\Delta E$ is the difference in energy between the excited and ground states of a nucleus of mass $M .$ (b) Calculate the recoil energy of the s7 Fe nucleus when it decays by gamma emission from the $14.4-\mathrm{keV}$ excited state. For this calculation, take the mass to be 57 u. Suggestions: When writing the equation for conservation of energy, use $(M v)^{2} / 2 M$ for the kinetic energy of the recoiling nucleus, Also, assume $h f \ll M c^{2}$ and use the binomial expansion.

Ren Jie Tuieng
Ren Jie Tuieng
Numerade Educator
04:03

Problem 59

A theory of nuclear astrophysics proposes that all the elements heavier than iron are formed in supernova explosions ending the lives of massive stars. Assume the amounts of 235 $\mathrm{U}$ and $^{238} \mathrm{U}$ were equal at the time of the explosion. How long ago did the star(s) explode that
released the elements that formed our Farth? The pres-ent $^{235} \mathrm{U} /^{258} \mathrm{U}$ ratio is $0.00725 .$ The half-lives of 235 $\mathrm{U}$ and 238 $\mathrm{U}$ are $0.704 \times 10^{9}$ yr and $4.47 \times 10^{9} \mathrm{yr}$

Ren Jie Tuieng
Ren Jie Tuieng
Numerade Educator
05:10

Problem 60

Europeans named a certain direction in the sky as between the horns of Taurus the Bull. On the day they named as July 4, 1054, a brilliant light appeared there. Europeans left no surviving record of the supernova, which could be seen in daylight for some days. As it faded, it remained visible for years, dimming for a time with the 77.1-day half-life of the radioactive cobalt-56 that had been created in the explosion. (a) The remains of the star now form the Crab nebula (see the photographs opening Chapter 34). In it, the cobalt-56 has now decreased to what fraction of its original activity? (b) Suppose an American, of the people called the Anasazi, made a charcoal drawing of the supernova. The carbon-14 in the charcoal has now decayed to what fraction of its original activity?

Ren Jie Tuieng
Ren Jie Tuieng
Numerade Educator
02:24

Problem 61

Review problem. Consider the Bohr model of the hydrogen atom, with the electron in the ground state. The magnetic field at the nucleus produced by the orbiting electron has a value of 12.5 T. (See Problem 1 in Chapter 30.) The proton can have its magnetic moment aligned in either of two directions perpendicular to the plane of the electron’s orbit. The interaction of the proton’s magnetic moment with the electron’s magnetic field causes a differ ence in energy between the states with the two different orientations of the proton’s magnetic moment. Find that energy difference in eV.

Ren Jie Tuieng
Ren Jie Tuieng
Numerade Educator
02:59

Problem 62

Student determination of the half-life of 137Ba. The radioactive barium isotope 137Ba has a relatively short half-life and can be easily extracted from a solution containing its parent cesium (137Cs). This barium isotope is commonly used in an undergraduate laboratory exercise for demonstrating the radioactive decay law. Undergraduate students using modest experimental equipment took the data pre-
sented in Figure $\mathrm{P} 44.62$ . Determine the half-life for the decay of $^{137} \mathrm{Ba}$ using their data.

Ren Jie Tuieng
Ren Jie Tuieng
Numerade Educator
04:02

Problem 63

Free neutrons have a characteristic half-life of 10.4 $\mathrm{min}$ . What fraction of a group of free neutrons with kincticncrgy 0.0400 $\mathrm{cV}$ decays before traveling a distance of 10.0 $\mathrm{km}$ ?

Ren Jie Tuieng
Ren Jie Tuieng
Numerade Educator
13:55

Problem 64

Review problem. Consider a model of the nucleus in which the positive charge $(Z e)$ is uniformly distributed throughout a sphere of radius $R$ . By integrating the encrgy density $\frac{1}{2} \epsilon_{0} E^{2}$ over all space, show that the clectric potential energy may be written
$$
U=\frac{3 Z^{2} e^{2}}{20 \pi \epsilon_{0} R}=\frac{3 k, Z^{2} e^{2}}{5 R}
$$
Problem 62 in Chapter 25 derived the same result by a different method.

Ren Jie Tuieng
Ren Jie Tuieng
Numerade Educator
03:51

Problem 65

In a piece of rock from the Moon, the $\$ 7$ Rb content is assayed to be $1.82 \times 10^{10}$ atoms per gram of material and the $^{87} \mathrm{Sr}$ content is found to be $1.07 \times 10^{9}$ atoms pergram. (a) Calculate the age of the rock. (b) What If? What assumption is implicit in using the radioactive dating method? The relevant decay is $^{87} \mathrm{Rb} \rightarrow^{87} \mathrm{Sr}+\mathrm{e}^{-}+\overline{\nu}$ . The half-life of the decay is 4.75 $\times 10^{10} \mathrm{yr} .$

Ren Jie Tuieng
Ren Jie Tuieng
Numerade Educator
12:47

Problem 66

The ground state of (molar mass 92.910 2 g/mol) decays by electron capture and e emission to energy levels of the daughter (molar mass 92.906 8 g/mol in ground state) at 2.44 MeV, 2.03 MeV, 1.48 MeV, and
1.35 MeV. (a) For which of these levels are electron capture and e decay allowed? (b) Identify the daughter andsketch the decay scheme, assuming all excited states deexcite by direct g decay to the ground state.

Ren Jie Tuieng
Ren Jie Tuieng
Numerade Educator