Phsx 2220 - Homework #13: Nuclear Physics Problems, Assignments of Physics

Homework problems for a nuclear physics course, covering topics such as electron states, quantum numbers, nuclear uncertainty principle, radioactive decay, disintegration energy, atomic masses, and nuclear reactions.

Typology: Assignments

Pre 2010

Uploaded on 07/23/2009

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Phsx 2220 - Homework #13
41-1. How many electron states are there in the following shells:
(a) n = 4; (b) n = 1; (c) n = 3; (d) n = 2?
41-2. What are the four quantum numbers for the two electrons of the
helium atom in its ground state?
43-3. Calculate the distance of closest approach for a head-on collision
between a 5.30 MeV alpha particle and the nucleus of a copper atom.
43-4. Because a nucleon is confined to a nucleus, we can take the
uncertainty in its position to be approximately the nuclear radius
R. What does the uncertainty principle say about the kinetic
energy of a nucleon in a nucleus with, say, A = 100? (Hint: take
the uncertainty in momentum p to be the actual momentum p.)
43-5. Consider an initially pure 3.4 g sample of 67Ga, an isotope that has
a half-life of 78 h. (a) What is its initial decay rate?
(b) What is its decay rate 48 h later?
43-6. A radioactive isotope of mercury, 197Hg, decays into gold, 197Au,
with a disintegration constant of 0.0108 h-1. (a) Calculate its
half-life. What fraction of a sample will remain (b) after three
half-lives and (c) after 10.0 days?
43-7. A 238U nucleus emits a 4.196 MeV alpha particle. Calculate the
disintegration energy Q for this process.
44-8. (a) How many atoms are contained in 1.0 kg of pure 235U? (b) How
much energy, in joules, is released by the complete fissioning of
1.0 kg of 235U? Assume Q = 200 MeV. (c) For how long would this
energy light a 100 W lamp?
44-9. Calculate the energy released in the fission reaction
235U + n –> 141Cs + 93Rb + 2n.
Needed atomic and particle masses are
235U 235.04392 u 93Rb 92.92157 u
141Cs 140.91963 u n 1.00867 u.
44-10. Verify that the fusion of 1.0 kg of deuterium by the reaction
2H + 2H –> 3He + n (Q = +3.27 MeV)
could keep a 100 W lamp burning for 3 x 104 y.
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Phsx 2220 - Homework #

41-1. How many electron states are there in the following shells: (a) n = 4; (b) n = 1; (c) n = 3; (d) n = 2?

41-2. What are the four quantum numbers for the two electrons of the helium atom in its ground state?

43-3. Calculate the distance of closest approach for a head-on collision between a 5.30 MeV alpha particle and the nucleus of a copper atom.

43-4. Because a nucleon is confined to a nucleus, we can take the uncertainty in its position to be approximately the nuclear radius R. What does the uncertainty principle say about the kinetic energy of a nucleon in a nucleus with, say, A = 100? (Hint: take the uncertainty in momentum ∆p to be the actual momentum p.)

43-5. Consider an initially pure 3.4 g sample of 67 Ga, an isotope that has a half-life of 78 h. (a) What is its initial decay rate? (b) What is its decay rate 48 h later?

43-6. A radioactive isotope of mercury, 197 Hg, decays into gold, 197 Au, with a disintegration constant of 0.0108 h -1^. (a) Calculate its half-life. What fraction of a sample will remain (b) after three half-lives and (c) after 10.0 days?

43-7. A 238 U nucleus emits a 4.196 MeV alpha particle. Calculate the disintegration energy Q for this process.

44-8. (a) How many atoms are contained in 1.0 kg of pure 235 U? (b) How much energy, in joules, is released by the complete fissioning of 1.0 kg of 235 U? Assume Q = 200 MeV. (c) For how long would this energy light a 100 W lamp?

44-9. Calculate the energy released in the fission reaction

(^235) U + n –> 141 Cs + 93 Rb + 2n.

Needed atomic and particle masses are

(^235) U 235.04392 u 93 Rb 92.92157 u

(^141) Cs 140.91963 u n 1.00867 u.

44-10. Verify that the fusion of 1.0 kg of deuterium by the reaction

(^2) H + 2 H –> 3 He + n (Q = +3.27 MeV)

could keep a 100 W lamp burning for 3 x 10 4 y.

44-11. Show that the energy released when three alpha particles fuse to form 12 C is 7.27 MeV. The atomic mass of 4 He is 4.0026 u, and that of 12 C is 12.0000 u.

44-12. The Sun has a mass of 2.0 x 10 30 kg and radiates energy at the rate of 3.9 x 10 26 W. (a) At what rate does the Sun transfer its mass to other forms of energy? (b) What fraction of its original mass has the Sun lost in this way since it began to burn hydrogen about 4.5 x 109 y ago?