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

All Solutions

Page 773: Standardized Test Practice

Exercise 1
Step 1
1 of 2
The nuclear model, also known as the planetary model was based on the Rutherford’s experiment. Therefore the correct answer is B.
Result
2 of 2
The correct answer is B.
Exercise 2
Step 1
1 of 3
In this problem, we are given an emission from the mercury atom of a known wavelength for which we should find the corresponding energy. We can do so by using Planck’s formula and inserting $hc=1240times 10^{-9}$ eV$cdot$m.

$$
E=frac{hc}{lambda}
$$

Step 2
2 of 3
center{After we plug in the values we have that }
[E=frac{1240times 10^{-9}}{405times 10^{-9}}=3.06textrm{ eV}]
so the answer is C. \
Result
3 of 3
The correct answer is C.
Exercise 3
Step 1
1 of 4
In this problem we are given the mercury atom that undergoes the deexcitation process from $E_7$to $E_4$ while emitting a photon. We should find the wavelength of the emitted photon.
Step 2
2 of 4
We can do so by using the Planck equation to express the wavelength as follows

$$
lambda=frac{hc}{E_{ph}}
$$

where $hc=1240times 10^{-9}$eV$cdot$m. However, we should find the energy first and we can do that by looking at the diagram of the mercury energy states.

$$
E_{ph}=abs{E_4-E_7}=abs{-4.95+2.48}=2.47textrm{ eV}
$$

Step 3
3 of 4
Now, one can simply insert the given values into the expression for the wavelength to have that

$$
lambda=frac{1240times 10^{-9}}{2.47}=boxed{502textrm{ nm}}
$$

so the correct answer is D.

Result
4 of 4
$$
textrm{D) }lambda=502textrm{ nm}
$$
Exercise 4
Solution 1
Solution 2
Step 1
1 of 2
B) The locations of the electrons around the nucleus are known precisely.
Result
2 of 2
B
Step 1
1 of 1
$mathrm{B}$ is the wrong statement. This is due to the axioms of quantum mechanics. Mainly, we don’t represent a state of a system with precise coordinates (Positions of electrons in this example) and their change in time like we do in classical mechanics.

In quantum mechanics we say that a state of system is represented by a state function $Psi$, which is a function of time and coordinates. Due to Heisenberg’s uncertainty principle, in quantum mechanics, we don’t talk about precise coordinates, but the probability of finding a object in a certain place.

Exercise 5
Step 1
1 of 2
Since the energy of a photon is directly proportional to its frequency according to Planck’s formula we have that the highest energy transition will lead to the highest frequency photon emission. From the graph, we see that $E_{6rightarrow2}$ transition has the largest energy so it will lead to the highest frequency photons. So the correct answer is D.
Result
2 of 2
The correct answer is D.
Exercise 6
Step 1
1 of 4
In this problem, we are given the hydrogen atom that undergoes the deexcitation process from $E_4$to $E_2$ while emitting a photon. We should find the frequency of the emitted photon.
Step 2
2 of 4
We can do so by using the Planck equation to express the frequency as follows

$$
f=frac{E_{ph}}{h}
$$

However, we should find the energy first and we can do that by looking at the diagram of the mercury energy states.

$$
E_{ph}=abs{E_2-E_4}=abs{-3.4+0.85}=2.55textrm{ eV}
$$

Step 3
3 of 4
Now, one can simply insert the given values into the expression for the frequency while converting the energy to Joules to have that

$$
f=frac{2.55 times 1.6times 10^{-19}}{6.63times 10^{-34}}=boxed{6.15times 10^{14}textrm{ Hz}}
$$

so the correct answer is C.

Result
4 of 4
$$
textrm{C) }f=6.15times 10^{14}textrm{ Hz}
$$
Exercise 7
Step 1
1 of 4
In this problem, we are given the hydrogen atom that undergoes the deexcitation process from $E_5$to $E_2$ while emitting a photon. We should find the wavelength of the emitted photon.
Step 2
2 of 4
We can do so by using the Planck equation to express the wavelength as follows

$$
lambda=frac{hc}{E_{ph}}
$$

where $hc=1240times 10^{-9}$eV$cdot$m. However, we should find the energy first and we can do that by looking at the diagram of the mercury energy states.

$$
E_{ph}=abs{E_2-E_5}=abs{-3.40+0.54}=2.86textrm{ eV}
$$

Step 3
3 of 4
Now, one can simply insert the given values into the expression for the wavelength to have that

$$
lambda=frac{1240times 10^{-9}}{2.86}=boxed{434textrm{ nm}}
$$

Result
4 of 4
$$
lambda=434textrm{ nm}
$$
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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