College Physics
Second Edition| ©2018 Roger A. Freedman; Todd Ruskell; Philip R. Kesten; David L. Tauck
Freedman College Physics, Second Edition, is a student-centered text and homework program for introductory, algebra-based physics courses. With a focus on conceptual understanding and biological applications, College Physics makes the relevance of physics clear to students. The Sapl...
Freedman College Physics, Second Edition, is a student-centered text and homework program for introductory, algebra-based physics courses. With a focus on conceptual understanding and biological applications, College Physics makes the relevance of physics clear to students. The Sapling Plus system combines the heavily researched FlipIt Physics prelectures (derived from smartPhysics) with a robust homework system, in which every problem has targeted feedback, a hint, and a fully worked and explained solution.
Freedman, College Physics Second Edition and SaplingPlus
This new integrated learning system brings together a ground-breaking media program with an innovative text presentation of algebra-based Physics. An experienced author team brings together a unique set of expertise and perspectives to help students master concepts and succeed in developing problem-solving skills necessary for College Physics. Now available for the first time with Sapling Plus--an online learning platform that combines the heavily research based FlipItPhysics prelectures (derived from smartPhysics) with the robust Sapling homework system, in which every problem has targeted feedback, hints, and a fully worked and explained solution. This HTML5 platform gives students the ability to actively read with a fully interactive ebook, watch pre-lecture videos and work or review problems with a mobile accessible learning experience. Integration is available with Learning Management Systems to provide single sign on and grade-sync capabilities and compatible with the iClicker 2 and other classroom response systems to provide a seamless full course experience for you and your students.
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Move Learning Forward
Bridge conceptual understanding and problem solving with resources to support active teaching and learning.
Freedman College Physics, Second Edition, is a student-centered text and homework program for introductory, algebra-based physics courses. With a focus on conceptual understanding and biological applications, College Physics makes the relevance of physics clear to students. The Sapling Plus system combines the heavily researched FlipIt Physics prelectures (derived from smartPhysics) with a robust homework system, in which every problem has targeted feedback, a hint, and a fully worked and explained solution.
Freedman, College Physics Second Edition and SaplingPlus
This new integrated learning system brings together a ground-breaking media program with an innovative text presentation of algebra-based Physics. An experienced author team brings together a unique set of expertise and perspectives to help students master concepts and succeed in developing problem-solving skills necessary for College Physics. Now available for the first time with Sapling Plus--an online learning platform that combines the heavily research based FlipItPhysics prelectures (derived from smartPhysics) with the robust Sapling homework system, in which every problem has targeted feedback, hints, and a fully worked and explained solution. This HTML5 platform gives students the ability to actively read with a fully interactive ebook, watch pre-lecture videos and work or review problems with a mobile accessible learning experience. Integration is available with Learning Management Systems to provide single sign on and grade-sync capabilities and compatible with the iClicker 2 and other classroom response systems to provide a seamless full course experience for you and your students.
Features
Education-Research-Based Prelecture Videos (derived from smartPhysics) for Preparing Students Before Class
Bridge Questions connect the Prelecture activity to the classroom experience, providing instructors with valuable insight into student understanding.
Sapling Homework with Robust Feedback, Hints, and Solutions with Every Problem
Set Up - Solve - Reflect Problem Solving Strategy for Worked Examples
Extensive Biological Applications
Outcome-Based Learning Objectives
Got the Concept? Problems Built into the Flow of Text for Checking Conceptual Understanding
Watch Out! boxes draw attention to common student misconceptions and corrects them immediately and help promote a deeper understanding of Physics.
Every chapter section ends with a Take home message is tied to outcome based learning objectives listed at the beginning of each chapter and summarizes the main physics principles a student should have learned.
Media Features housed in SaplingPlus
- Prelectures Videos/Embedded Checkpoints/Bridge Questions
Developed based on research and principles that defined smartPhysics. These Animated, narrated Prelecture videos introduce and overview core physics topics, laying the groundwork for conceptual understanding before students ever set foot in class. Each Prelecture activity is about 15 minutes long, and contains embedded questions that help students check their understanding along the way. Followed up by Bridge Questions which bridge student learning to in class engagement by giving students a means of communicating what they know and don’t know and instructors access to valuable insight to tailor class time. - Interactive eBook
New! For the first time, the ebook is also available through an app which allows students to read offline, have the book read aloud to them, in addition to the highlighting, note taking and keyword search that you have come to expect." - Balloon Art Concept Checks
Designed to guide students through the process of identifying important Physics concepts in key figures and equations. Mirroring the visual narrative in the form of word balloons, these interactive questions reinforce key ideas from the text by highlighting important physics principles in each chapter. - PhET Simulations
New HTML5 PhET Simulations from the University of Colorado at Boulder’s renowned research-based Physics simulations help students gain a visual understanding of concepts and illustrate cause-and-effect relationships. Tutorial questions further encourage this quantitative exploration, while addressing specific problem-solving needs. - P’Casts
250 total whiteboard mobile ready videos. Carefully selected by Physics students and instructors throughout North America to help simulate the experience of watching an instructor walk through the steps and explanation of Physics concepts while solving a problem. - Pocket Worked Examples
All worked examples from College Physics are available as a downloadable item for mobile devices
New to This Edition
- Sapling Plus with Prelectures (derived from smartPhysics) Together in One System
- 200+ New End-of-Chapter Problems
- Roger Freedman’s In-Class Activities
- End-of-Chapter Problems Paired to Worked Examples
- Expanded Optical Instruments Coverage (Chapter 24)
"This book breaks a complex problem apart, and step by step teaches students how to think about a physics problem, rather than just substitute a formula."
-Yiyan Bai: Houston Community College"This book is great for teaching physics the right way."
-Avishek Kumar: Arizona State University"This chapter is very well written and one of the best on Fluids that I have read for a non-calculus based text. The main strengths are: 1. The comprehensiveness of the various topics without the mathematical details. 2. The numerical examples to explain the various topics 3. "Got the Concepts" that challenges the students to think."
-Arup Neogi: University of North Texas"This is an excellent physics textbook. I particularly like the easy-to-understand bubble text to clarify equations and figures, which many students typically spend quite some time to understand. The clearly written example problems and solution steps are also essential for this book, which I expect the students to like a lot…The presentation of this book is outstanding. It will be a good choice for students with wide ranging math and physics backgrounds."
-Fengyuan Yang: The Ohio State University"The worked example in the text are excellent, with more detail and consistency of approach than is typical in a textbook at this level."
-Matthew Craig, Minnesota State University Moorhead"This textbook does a good job of describing the physics concepts while providing many examples of typical problems. The examples are done in a useful way, by not just showing the mathematical steps but also justifying in the text why the steps or approach is taken."
-Jeremy Armstrong, University of Nebraska at Kearney"This is is the best treatment of Maxwell's equations in electromagnetic waves I have ever seen in an algebra-based physics textbook."'
-Lawrence Rees, Brigham Young University


College Physics
Second Edition| ©2018
Roger A. Freedman; Todd Ruskell; Philip R. Kesten; David L. Tauck
Digital Options

iClicker REEF
Stay engaged in class with our student response system, show your instructor that you're listening and prove what you know.


College Physics
Second Edition| 2018
Roger A. Freedman; Todd Ruskell; Philip R. Kesten; David L. Tauck
Table of Contents
1. Introduction to Physics
1-1 Physicists use a special language—part words, part equations—to describe the natural world
1-2 Success in physics requires well-developed problem-solving skills
1-3 Measurements in physics are based on standard units of time, length, and mass
1-4 Correct use of significant figures helps keep track of uncertainties in numerical values
1-5 Dimensional analysis is a powerful way to check the results of a physics calculation
2. Linear Motion
2-1 Studying motion in a straight line is the first step in understanding physics
2-2 Constant velocity means moving at a steady speed in the same direction
2-3 Velocity is the rate of change of position, and acceleration is the rate of change of velocity
2-4 Constant acceleration means velocity changes at a steady rate
2-5 Solving straight-line motion problems: Constant acceleration
2-6 Objects falling freely near Earth’s surface have constant acceleration
3. Motion in Two and Three Dimensions
3-1 The ideas of linear motion help us understand motion in two or three dimensions
3-2 A vector quantity has both a magnitude and a direction
3-3 Vectors can be described in terms of components
3-4 For motion in a plane, velocity and acceleration are vector quantities
3-5 A projectile moves in a plane and has a constant acceleration
3-6 You can solve projectile motion problems using techniques learned for straight-line motion
3-7 An object moving in a circle is accelerating even if its speed is constant
3-8 The vestibular system of the ear allows us to sense acceleration
4. Forces and Motion I: Newton’s Laws
4-1 How objects move is determined by the forces that act on them
4-2 If a net external force acts on an object, the object accelerates
4-3 Mass, weight, and inertia are distinct but related concepts
4-4 Making a free-body diagram is essential in solving any problem involving forces
4-5 Newton’s third law relates the forces that two objects exert on each other
4-6 All problems involving forces can be solved using the same series of steps
5. Forces and Motion II: Applications
5-1 We can use Newton’s laws in situations beyond those we have already studied
5-2 The static friction force changes magnitude to offset other applied forces
5-3 The kinetic friction force on a sliding object has a constant magnitude
5-4 Problems involving static and kinetic friction are like any other problem with forces
5-5 An object moving through air or water experiences a drag force
5-6 In uniform circular motion, the net force points toward the center of the circle
6. Work and Energy
6-1 The ideas of work and energy are intimately related
6-2 The work that a constant force does on a moving object depends on the magnitude and direction of the force
6-3 Kinetic energy and the work-energy theorem give us an alternative way to express Newton’s second law
6-4 The work-energy theorem can simplify many physics problems
6-5 The work-energy theorem is also valid for curved paths and varying forces
6-6 Potential energy is energy related to an object’s position
6-7 If only conservative forces do work, total mechanical energy is conserved
6-8 Energy conservation is an important tool for solving a wide variety of problems
6-9 Power is the rate at which energy is transferred
7. Momentum, Collisions, and Center of Mass
7-1 Newton’s third law helps lead us to the idea of momentum
7-2 Momentum is a vector that depends on an object’s mass, speed, and direction of motion
7-3 The total momentum of a system of objects is conserved under certain conditions
7-4 In an inelastic collision, some of the mechanical energy is lost
7-5 In an elastic collision, both momentum and mechanical energy are conserved
7-6 What happens in a collision is related to the time the colliding objects are in contact
7-7 The center of mass of a system moves as though all of the system’s mass were concentrated there
8. Rotational Motion
8-1 Rotation is an important and ubiquitous kind of motion
8-2 An object’s rotational kinetic energy is related to its angular velocity and how its mass is distributed
8-3 An object’s moment of inertia depends on its mass distribution and the choice of rotation axis
8-4 Conservation of mechanical energy also applies to rotating objects
8-5 The equations for rotational kinematics are almost identical to those for linear motion
8-6 Torque is to rotation as force is to translation
8-7 The techniques used for solving problems with Newton’s second law also apply to rotation problems
8-8 Angular momentum is conserved when there is zero net torque on a system
8-9 Rotational quantities such as angular momentum and torque are actually vectors
9. Elastic Properties of Matter: Stress and Strain
9-1 When an object is under stress, it deforms
9-2 An object changes length when under tensile or compressive stress
9-3 Solving stress-strain problems: Tension and compression
9-4 An object expands or shrinks when under volume stress
9-5 Solving stress-strain problems: Volume stress
9-6 A solid object changes shape when under shear stress
9-7 Solving stress-strain problems: Shear stress
9-8 Objects deform permanently or fail when placed under too much stress
9-9 Solving stress-strain problems: From elastic behavior to failure
10. Gravitation
10-1 Gravitation is a force of universal importance
10-2 Newton’s law of universal gravitation explains the orbit of the Moon
10-3 The gravitational potential energy of two objects is negative and increases toward zero as the objects are moved farther apart
10-4 Newton’s law of universal gravitation explains Kepler’s laws for the orbits of planets and satellites
10-5 Apparent weightlessness can have major physiological effects on space travelers
11. Fluids
11-1 Liquids and gases are both examples of fluids
11-2 Density measures the amount of mass per unit volume
11-3 Pressure in a fluid is caused by the impact of molecules
11-4 In a fluid at rest, pressure increases with increasing depth
11-5 Scientists and medical professionals use various units for measuring fluid pressure
11-6 A difference in pressure on opposite sides of an object produces a net force on the object
11-7 A pressure increase at one point in a fluid causes a pressure increase throughout the fluid
11-8 Archimedes’ principle helps us understand buoyancy
11-9 Fluids in motion behave differently depending on the flow speed and the fluid viscosity
11-10 Bernoulli’s equation helps us relate pressure and speed in fluid motion
11-11 Viscosity is important in many types of fluid flow
11-12 Surface tension explains the shape of raindrops and how respiration is possible
12. Oscillations
12-1 We live in a world of oscillations
12-2 Oscillations are caused by the interplay between a restoring force and inertia
12-3 The simplest form of oscillation occurs when the restoring force obeys Hooke’s law
12-4 Mechanical energy is conserved in simple harmonic motion
12-5 The motion of a pendulum is approximately simple harmonic
12-6 A physical pendulum has its mass distributed over its volume
12-7 When damping is present, the amplitude of an oscillating system decreases over time
12-8 Forcing a system to oscillate at the right frequency can cause resonance
13. Waves
13-1 Waves are disturbances that travel from place to place
13-2 Mechanical waves can be transverse, longitudinal, or a combination of these
13-3 Sinusoidal waves are related to simple harmonic motion
13-4 The propagation speed of a wave depends on the properties of the wave medium
13-5 When two waves are present simultaneously, the total disturbance is the sum of the individual waves
13-6 A standing wave is caused by interference between waves traveling in opposite directions
13-7 Wind instruments, the human voice, and the human ear use standing sound waves
13-8 Two sound waves of slightly different frequencies produce beats
13-9 The intensity of a wave equals the power that it delivers per square meter
13-10 The frequency of a sound depends on the motion of the source and the listener
14. Thermodynamics I
14-1 A knowledge of thermodynamics is essential for understanding almost everything around you—including your own body
14-2 Temperature is a measure of the energy within a substance
14-3 In a gas, the relationship between temperature and molecular kinetic energy is a simple one
14-4 Most substances expand when the temperature increases
14-5 Heat is energy that flows due to a temperature difference
14-6 Energy must enter or leave an object in order for it to change phase
14-7 Heat can be transferred by radiation, convection, or conduction
15. Thermodynamics II
15-1 The laws of thermodynamics involve energy and entropy
15-2 The first law of thermodynamics relates heat flow, work done, and internal energy change
15-3 A graph of pressure versus volume helps to describe what happens in a thermodynamic process
15-4 More heat is required to change the temperature of a gas isobarically than isochorically
15-5 The second law of thermodynamics describes why some processes are impossible
15-6 The entropy of a system is a measure of its disorder
16. Electrostatics I: Electric Charge, Forces, and Fields
16-1 Electric forces and electric charges are all around you—and within you
16-2 Matter contains positive and negative electric charge
16-3 Charge can flow freely in a conductor, but not in an insulator
16-4 Coulomb’s law describes the force between charged objects
16-5 The concept of electric field helps us visualize how charges exert forces at a distance
16-6 Gauss’s law gives us more insight into the electric field
16-7 In certain situations Gauss’s law helps us to calculate the electric field and to determine how charge is distributed
17. Electrostatics II: Electric Potential Energy and Electric Potential
17-1 Electric energy is important in nature, technology, and biological systems
17-2 Electric potential energy changes when a charge moves in an electric field
17-3 Electric potential equals electric potential energy per charge
17-4 The electric potential has the same value everywhere on an equipotential surface
17-5 A capacitor stores equal amounts of positive and negative charge
17-6 A capacitor is a storehouse of electric potential energy
17-7 Capacitors can be combined in series or in parallel
17-8 Placing a dielectric between the plates of a capacitor increases the capacitance
18. Electric Charges in Motion
18-1 Life on Earth and our technological society are only possible because of charges in motion
18-2 Electric current equals the rate at which charge flows
18-3 The resistance to current flow through an object depends on the object’s resistivity and dimensions
18-4 Resistance is important in both technology and physiology
18-5 Kirchhoff’s rules help us to analyze simple electric circuits
18-6 The rate at which energy is produced or taken in by a circuit element depends on current and voltage
18-7 A circuit containing a resistor and capacitor has a current that varies with time
19. Magnetism
19-1 Magnetic forces are interactions between two magnets
19-2 Magnetism is an interaction between moving charges
19-3 A moving point charge can experience a magnetic force
19-4 A mass spectrometer uses magnetic forces to differentiate atoms of different masses
19-5 Magnetic fields exert forces on current-carrying wires
19-6 A magnetic field can exert a torque on a current loop
19-7 Ampère’s law describes the magnetic field created by current-carrying wires
19-8 Two current-carrying wires exert magnetic forces on each other
20. Electromagnetic Induction
20-1 The world runs on electromagnetic induction
20-2 A changing magnetic flux creates an electric field
20-3 Lenz’s law describes the direction of the induced emf
20-4 Faraday’s law explains how alternating currents are generated
21. Alternating-Current Circuits
21-1 Most circuits use alternating current
21-2 We need to analyze ac circuits differently than dc circuits
21-3 Transformers allow us to change the voltage of an ac power source
21-4 An inductor is a circuit element that opposes changes in current
21-5 In a circuit with an inductor and capacitor, charge and current oscillate
21-6 When an ac voltage source is attached in series to an inductor, resistor, and capacitor, the circuit can display resonance
21-7 Diodes are important parts of many common circuits
22. Electromagnetic Waves
22-1 Light is just one example of an electromagnetic wave
22-2 In an electromagnetic plane wave, electric and magnetic fields both oscillate
22-3 Maxwell’s equations explain why electromagnetic waves are possible
22-4 Electromagnetic waves carry both electric and magnetic energy, and come in packets called photons
23. Wave Properties of Light
23-1 The wave nature of light explains much about how light behaves
23-2 Huygens’ principle explains the reflection and refraction of light
23-3 In some cases light undergoes total internal reflection at the boundary between media
23-4 The dispersion of light explains the colors from a prism or a rainbow
23-5 In a polarized light wave, the electric field vector points in a specific direction
23-6 Light waves reflected from the layers of a thin film can interfere with each other, producing dazzling effects
23-7 Interference can occur when light passes through two narrow, parallel slits
23-8 Diffraction is the spreading of light when it passes through a narrow opening
23-9 The diffraction of light through a circular aperture is important in optics
24. Geometrical Optics
24-1 Mirrors or lenses can be used to form images
24-2 A plane mirror produces an image that is reversed back to front
24-3 A concave mirror can produce an image of a different size than the object
24-4 Simple equations give the position and magnification of the image made by a concave mirror
24-5 A convex mirror always produces an image that is smaller than the object
24-6 The same equations used for concave mirrors also work for convex mirrors
24-7 Convex lenses form images like concave mirrors and vice versa
24-8 The focal length of a lens is determined by its index of refraction and the curvature of its surfaces
24-9 A camera and the human eye use different methods to focus on objects at various distances
25. Relativity
25-1 The concepts of relativity may seem exotic, but they’re part of everyday life
25-2 Newton’s mechanics include some ideas of relativity
25-3 The Michelson-Morley experiment shows that light does not obey Newtonian relativity
25-4 Einstein’s relativity predicts that the time between events depends on the observer
25-5 Einstein’s relativity also predicts that the length of an object depends on the observer
25-6 The relative velocity of two objects is constrained by the speed of light, the ultimate speed limit
25-7 The equations for momentum and kinetic energy must be modified at very high speeds
25-8 Einstein’s general theory of relativity describes the fundamental nature of gravity
26. Quantum Physics and Atomic Structure
26-1 Experiments that probe the nature of light and matter reveal the limits of classical physics
26-2 The photoelectric effect and blackbody radiation show that light is absorbed and emitted in the form of photons
26-3 As a result of its photon character, light changes wavelength when it is scattered
26-4 Matter, like light, has aspects of both waves and particles
26-5 The spectra of light emitted and absorbed by atoms show that atomic energies are quantized
26-6 Models by Bohr and Schrödinger give insight into the intriguing structure of the atom
27. Nuclear Physics
27-1 The quantum concepts that help explain atoms are essential for understanding the nucleus
27-2 The strong force holds nuclei together
27-3 The binding energy of nuclei helps explain why some are more stable than others
27-4 The largest nuclei can release energy by undergoing fission and splitting apart
27-5 The smallest nuclei can release energy if they are forced to fuse together
27-6 Unstable nuclei may emit alpha, beta, or gamma radiation
28. Particle Physics
28-1 Studying the ultimate constituents of matter helps reveal the nature of the physical universe
28-2 Most forms of matter can be explained by just a handful of fundamental particles
28-3 Four fundamental forces describe all interactions between material objects
28-4 We live in an expanding universe, and the nature of most of its contents is a mystery
Appendix A SI Units and Conversion Factors
Appendix B Numerical Data
Appendix C Periodic Table of Elements
Math Tutorial MT1
Answers Ans1
Index I1


College Physics
Second Edition| 2018
Roger A. Freedman; Todd Ruskell; Philip R. Kesten; David L. Tauck
Authors

Roger Freedman
Dr. Roger A. Freedman is a Lecturer in Physics at the University of California, Santa Barbara.
He was an undergraduate at the University of California campuses in San Diego and Los Angeles, and did his doctoral research in theoretical nuclear physics at Stanford University. He came to UCSB in 1981 after three years of teaching and doing research at the University of Washington. At UCSB, Dr. Freedman has taught in both the Department of Physics and the College of Creative Studies, a branch of the university intended for highly gifted and motivated undergraduates. In recent years, he has helped to develop computer-based tools for learning introductory physics and astronomy and has been a pioneer in the use of classroom response systems and the “flipped” classroom model at UCSB. Roger holds a commercial pilot’s license and was an early organizer of the San Diego Comic-Con, now the world’s largest popular culture convention.
He was an undergraduate at the University of California campuses in San Diego and Los Angeles, and did his doctoral research in theoretical nuclear physics at Stanford University. He came to UCSB in 1981 after three years of teaching and doing research at the University of Washington. At UCSB, Dr. Freedman has taught in both the Department of Physics and the College of Creative Studies, a branch of the university intended for highly gifted and motivated undergraduates. In recent years, he has helped to develop computer-based tools for learning introductory physics and astronomy and has been a pioneer in the use of classroom response systems and the “flipped” classroom model at UCSB. Roger holds a commercial pilot’s license and was an early organizer of the San Diego Comic-Con, now the world’s largest popular culture convention.

Todd Ruskell
As a Teaching Professor of Physics at the Colorado School of Mines, Todd G. Ruskell focuses on teaching at the introductory level, and continually develops more effective ways to help students learn. One method used in large enrollment introductory courses is Studio Physics. This collaborative, hands-on environment helps students develop better intuition about, and conceptual models of, physical phenomena through an active learning approach. Dr. Ruskell brings his experience in improving students’ conceptual understanding to the text, as well as a strong liberal arts perspective. Dr. Ruskell’s love of physics began with a B.A. in physics from Lawrence University in Appleton, Wisconsin. He went on to receive an M.S. and Ph.D. in optical sciences from the University of Arizona. He has received awards for teaching excellence, including Colorado School of Mines’ Alumni Teaching Award. Dr. Ruskell currently serves on the physics panel and advisory board for the NANSLO (North American Network of Science Labs Online) project.

Philip R. Kesten
Dr. Philip Kesten, Associate Professor of Physics and Associate Provost for Residential Learning Communities at Santa Clara University, holds a B.S. in physics from the Massachusetts Institute of Technology and received his Ph.D. in high energy particle physics from the University of Michigan. Since joining the Santa Clara faculty in 1990, Dr. Kesten has also served as Chair of Physics, Faculty Director of the ATOM and da Vinci Residential Learning Communities, and Director of the Ricard Memorial Observatory. He has received awards for teaching excellence and curriculum innovation, was Santa Clara's Faculty Development Professor for 2004-2005, and was named the California Professor of the Year in 2005 by the Carnegie Foundation for the Advancement of Education. Dr. Kesten is co-founder of Docutek, (A SirsiDynix Company), an Internet software company, and has served as the Senior Editor for Modern Dad, a newsstand magazine.

David L. Tauck
Dr. David Tauck, Associate Professor of Biology, holds both a B.A. in biology and an M.A. in Spanish from Middlebury College. He earned his Ph.D. in physiology at Duke University and completed postdoctoral fellowships at Stanford University and Harvard University in anesthesia and neuroscience, respectively. Since joining the Santa Clara University faculty in 1987, he has served as Chair of the Biology Department, the College Committee on Rank and Tenure, and the Institutional Animal Care and Use Committee; he has also served as president of the local chapter of Phi Beta Kappa. Dr. Tauck currently serves as the Faculty Director in Residence of the da Vinci Residential Learning Community.


College Physics
Second Edition| 2018
Roger A. Freedman; Todd Ruskell; Philip R. Kesten; David L. Tauck
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College Physics
Second Edition| 2018
Roger A. Freedman; Todd Ruskell; Philip R. Kesten; David L. Tauck
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