Physics: Principles and Problems
Physics: Principles and Problems
9th Edition
Elliott, Haase, Harper, Herzog, Margaret Zorn, Nelson, Schuler, Zitzewitz
ISBN: 9780078458132
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Textbook solutions

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Page 805: Section Review

Exercise 9
Step 1
1 of 3
In this problem we are given two pairs of nuclei: 1) $^{12}_6$C and $^{13}_6$C one one side and 2) $^{11}_5$B and $^{11}_6$C. We want to discus their differences and their similarities.
Step 2
2 of 3
The first pair has the same atomic number, i.e. it is essentially the same element, carbon, but it has different number of nucleons, i.e. neutrons.
Step 3
3 of 3
The second pair nuclei have different atomic numbers but the same number of nucleons.
Exercise 10
Step 1
1 of 2
By all means, it is the tritium that has higher binding energy because it will have a larger mass defect. The reason for this is that tritium has 2 neutrons and $^3_2$He has only one and neutrons are heavier than protons.
Result
2 of 2
Tritium has the more negative binding energy.
Exercise 11
Step 1
1 of 1
The reason for this is that at certain cutoff distance, the strong nuclear force will decline sharply whereas the repulsion that protons feel from each other will remain and at certain point it can prevail. It is important to know that electrostatic repulsion is inversely proportional to the square of distance and at very small distance can be significant.
Exercise 12
Step 1
1 of 1
Since the tritium has a neutron more, it has a larger mass defect since neutrons are heavier than protons.
Exercise 13
Step 1
1 of 5
In this problem, we are given a radioactive carbon isotope, $^{14}_6$C and its mass. We want to know the mass defect and the corresponding binding energy of the isotope.
Step 2
2 of 5
The mass defect is defined as the difference between the mass of the atom and the mass of it’s constituents and it can be written as follows

$$
M_d=M-Ztimes(m_p+m_e)-(A-Z)times m_n
$$

Step 3
3 of 5
center{a) In our case we have that }
[M_d=M-6(m_p+m_e)-8m_n=14.003074-6times 1.007825-8times 1.008665]
[boxed{M_d=-0.113196textrm{ u}}]
Step 4
4 of 5
b) The binding energy in MeV is obtained when the mass defect is multiplied by the conversion factor ($1u=931.5$MeV) so that we have

$$
E_B=931.5times M_d=-931.5times 0.113196=boxed{-105.44textrm{ MeV}}
$$

Result
5 of 5
$$
textrm{a) }M_d=-0.113196textrm{ u}
$$

$$
textrm{b) }E_B=-105.44textrm{ MeV}
$$

Exercise 14
Step 1
1 of 1
If we observe the Figure 30.2 which describes the relation between the binding energy per nucleon and the number of nucleons we see that the lowest point is iron. This practically means that elements with lower atomic number than iron will participate in nuclear reactions where their mass increases. Elements with atomic numbers larger than iron will participate in nuclear reactions where the mass is lost. Therefore, we can expect that the heaviest element we could expect in old stars is iron.
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Chapter 1: A Physics Toolkit
Section 1.1: Mathematics and Physics
Section 1.2: Measurement
Section 1.3: Graphing Data
Page 24: Assessment
Page 29: Standardized Test Practice
Chapter 3: Accelerated Motion
Section 3.1: Acceleration
Section 3.2: Motion with Constant Acceleration
Section 3.3: Free Fall
Page 80: Assessment
Page 85: Standardized Test Practice
Chapter 4: Forces in One Dimension
Section 4.1: Force and Motion
Section 4.2: Using Newton’s Laws
Section 4.3: Interaction Forces
Page 112: Assessment
Page 117: Standardized Test Practice
Chapter 5: Forces in Two Dimensions
Section 5.1: Vectors
Section 5.2: Friction
Section 5.3: Force and Motion in Two Dimensions
Page 140: Assessment
Page 145: Standardized Test Practice
Chapter 6: Motion in Two Dimensions
Section 6.1: Projectile Motion
Section 6.2: Circular Motion
Section 6.3: Relative Velocity
Page 164: Assessment
Page 169: Standardized Test Practice
Chapter 7: Gravitation
Section 7.1: Planetary Motion and Gravitation
Section 7.2: Using the Law of Universal Gravitation
Page 190: Assessment
Page 195: Standardized Test Practice
Chapter 8: Rotational Motion
Section 8.1: Describing Rotational Motion
Section 8.2: Rotational Dynamics
Section 8.3: Equilibrium
Page 222: Assessment
Page 227: Standardized Test Practice
Chapter 9: Momentum and Its Conservation
Chapter 10: Energy, Work, and Simple Machines
Section 10.1: Energy and Work
Section 10.2: Machines
Page 278: Assessment
Page 283: Standardized Test Practice
Chapter 11: Energy and Its Conservation
Section 11.1: The Many Forms of Energy
Section 11.2: Conservation of Energy
Page 306: Assessment
Page 311: Standardized Test Practice
Chapter 13: State of Matter
Section 13.1: Properties of Fluids
Section 13.2: Forces Within Liquids
Section 13.3: Fluids at Rest and in Motion
Section 13.4: Solids
Page 368: Assessment
Page 373: Standardized Test Practice
Chapter 14: Vibrations and Waves
Section 14.1: Periodic Motion
Section 14.2: Wave Properties
Section 14.3: Wave Behavior
Page 396: Assessment
Page 401: Section Review
Chapter 15: Sound
Section 15.1: Properties of Detection of Sound
Section 15.2: The Physics of Music
Page 424: Assessment
Page 429: Standardized Test Practice
Chapter 17: Reflections and Mirrors
Section 17.1: Reflection from Plane Mirrors
Section 17.2: Curved Mirrors
Page 478: Assessment
Page 483: Standardized Test Practice
Chapter 18: Refraction and lenses
Section 18.1: Refraction of Light
Section 18.2: Convex and Concave Lenses
Section 18.3: Applications of Lenses
Page 508: Assessment
Page 513: Standardized Test Practice
Chapter 21: Electric Fields
Section 21.1: Creating and Measuring Electric Fields
Section 21.2: Applications of Electric Fields
Page 584: Assessment
Page 589: Standardized Test Practice
Chapter 22: Current Electricity
Section 22.1: Current and Circuits
Section 22.2: Using Electric Energy
Page 610: Assessment
Page 615: Standardized Test Practice
Chapter 23: Series and Parallel Circuits
Section 23.1: Simple Circuits
Section 23.2: Applications of Circuits
Page 636: Assessment
Page 641: Standardized Test Practice
Chapter 24: Magnetic Fields
Section 24.1: Magnets: Permanent and Temporary
Section 24.2: Forces Caused by Magnetic Fields
Page 664: Assessment
Page 669: Standardized Test Practice
Chapter 25: Electromagnetic Induction
Section 25.1: Electric Current from Changing Magnetic Fields
Section 25.2: Changing Magnetic Fields Induce EMF
Page 690: Assessment
Page 695: Standardized Test Practice
Chapter 30: Nuclear Physics
Section 30.1: The Nucleus
Section 30.2: Nuclear Decay and Reactions
Section 30.3: The Building Blocks of Matter
Page 828: Assessment
Page 831: Standardized Test Practice