U Can: Physics I For Dummies

U Can: Physics I For Dummies
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Описание книги

Take the fear out of Physics I If the thought of studying physics makes you sweat, you can finally have something to rest easy about! U Can: Physics I For Dummies takes the intimidation out of this tough subject, offering approachable lessons, examples, and practice opportunities—as well as access to additional practice problems online. With this one-stop resource, you'll find friendly and accessible instruction on everything you'll encounter in your Physics I course and will gain the practice and confidence you need to score high at exam time. Inside this comprehensive study resource, how-to lessons are thoughtfully blended with practical examples and problems to help you put your knowledge to practice and gauge your comprehension of the physics topics presented. Lessons and practice problems are fully integrated and track to a typical Physics I course, giving you one mega-resource that combines the 'how-to' you need with the 'do it' practice you want to keep the physics anxiety at bay. Get up to speed on the basic concepts of physics Grasp physics formulas in a clear and concise manner Explore the newest discoveries in the field Access additional practice problems online If you're looking for an all-inclusive product to help with your Physics I coursework, U Can: Physics I For Dummies has it all—and then some!

Оглавление

Steven Holzner. U Can: Physics I For Dummies

Introduction

About This Book

Foolish Assumptions

Beyond the Book

Where to Go from Here

Part I

Chapter 1. Using Physics to Understand Your World

What Physics Is All About

Observing Objects in Motion

When Push Comes to Shove: Forces

Feeling Hot but Not Bothered: Thermodynamics

Chapter 2. Reviewing Physics Measurement and Math Fundamentals

Measuring the World around You and Making Predictions

Eliminating Some Zeros: Using Scientific Notation

From Meters to Inches and Back Again: Converting Between Units

Checking the Accuracy and Precision of Measurements

Arming Yourself with Basic Algebra

Tackling a Little Trig

Interpreting Equations as Real-World Ideas

Chapter 3. Exploring the Need for Speed

Going the Distance with Displacement

Speed Specifics: What Is Speed, Anyway?

Speeding Up (Or Down): Acceleration

Relating Acceleration, Time, and Displacement

Linking Velocity, Acceleration, and Displacement

Chapter 4. Following Directions: Motion in Two Dimensions

Visualizing Vectors

Putting Vectors on the Grid

A Little Trig: Breaking Up Vectors into Components

Featuring Displacement, Velocity, and Acceleration in 2-D

Accelerating Downward: Motion under the Influence of Gravity

Part II

Chapter 5. When Push Comes to Shove: Force

Newton’s First Law: Resisting with Inertia

Newton’s Second Law: Relating Force, Mass, and Acceleration

Newton’s Third Law: Looking at Equal and Opposite Forces

Chapter 6. Getting Down with Gravity, Inclined Planes, and Friction

Acceleration Due to Gravity: One of Life’s Little Constants

Finding a New Angle on Gravity with Inclined Planes

Getting Sticky with Friction

On the Move: Understanding Static and Kinetic Friction

Chapter 7. Circling around Rotational Motion and Orbits

Centripetal Acceleration: Changing Direction to Move in a Circle

Getting Angular with Displacement, Velocity, and Acceleration

Getting into Angular Velocity

Whipping Around with Angular Acceleration

Connecting Angular Velocity and Angular Acceleration to Angles

Connecting Angular Acceleration and Angle to Angular Velocity

Seeking the Center: Centripetal Force

Letting Gravity Supply Centripetal Force

Chapter 8. Go with the Flow: Looking at Pressure in Fluids

Mass Density: Getting Some Inside Information

Applying Pressure

Buoyancy: Float Your Boat with Archimedes’s Principle

Fluid Dynamics: Going with Fluids in Motion

Getting Up to Speed on Flow and Pressure

Part III

Chapter 9. Getting Some Work Out of Physics

Looking for Work

Making a Move: Kinetic Energy

Energy in the Bank: Potential Energy

Choose Your Path: Conservative versus Nonconservative Forces

Keeping the Energy Up: The Conservation of Mechanical Energy

Powering Up: The Rate of Doing Work

Chapter 10. Putting Objects in Motion: Momentum and Impulse

Looking at the Impact of Impulse

Gathering Momentum

The Impulse-Momentum Theorem: Relating Impulse and Momentum

When Objects Go Bonk: Conserving Momentum

When Worlds (Or Cars) Collide: Elastic and Inelastic Collisions

Chapter 11. Winding Up with Angular Motion

Going from Linear to Rotational Motion

Understanding Tangential Motion

Applying Vectors to Rotation

Doing the Twist: Torque

Spinning at Constant Velocity: Rotational Equilibrium

Chapter 12. Round and Round with Rotational Dynamics

Rolling Up Newton’s Second Law into Angular Motion

Moments of Inertia: Looking into Mass Distribution

Wrapping Your Head around Rotational Work and Kinetic Energy

Can’t Stop This: Angular Momentum

Chapter 13. Springs ’n’ Things: Simple Harmonic Motion

Bouncing Back with Hooke’s Law

Getting Around to Simple Harmonic Motion

Factoring Energy into Simple Harmonic Motion

Swinging with Pendulums

Part IV

Chapter 14. Turning Up the Heat with Thermodynamics

Measuring Temperature

The Heat Is On: Thermal Expansion

Heat: Going with the Flow (of Thermal Energy)

Chapter 15. Here, Take My Coat: How Heat Is Transferred

Convection: Letting the Heat Flow

Too Hot to Handle: Getting in Touch with Conduction

Radiation: Riding the (Electromagnetic) Wave

Chapter 16. In the Best of All Possible Worlds: The Ideal Gas Law

Digging into Molecules and Moles with Avogadro’s Number

Relating Pressure, Volume, and Temperature with the Ideal Gas Law

Tracking Ideal Gas Molecules with the Kinetic Energy Formula

Chapter 17. Heat and Work: The Laws of Thermodynamics

Thermal Equilibrium: Getting Temperature with the Zeroth Law

Conserving Energy: The First Law of Thermodynamics

Flowing from Hot to Cold: The Second Law of Thermodynamics

Going Cold: The Third (And Absolute Last) Law of Thermodynamics

Part V

Chapter 18. Ten Common Mistakes People Make When Solving Problems

Mixing Units

Expressing the Answer in the Wrong Units

Swapping Radians and Degrees

Getting Sines and Cosines Mixed Up

Not Treating Vectors as Vectors

Mixing Up the Signs of the Components of Vectors

Getting the Direction of Forces Wrong

Neglecting Latent Heat

Using the Wrong Temperature in the Ideal Gas Law

Getting the Signs Wrong in the First Law of Thermodynamics

Chapter 19. Ten Wild Physics Theories

Heisenberg Says You Can’t Be Certain

Black Holes Don’t Let Light Out

Gravity Curves Space

You Can Measure a Smallest Distance

Matter and Antimatter Destroy Each Other

Supernovas Are the Most Powerful Explosions

The Universe Starts with the Big Bang and Ends with the Gnab Gib

Most Matter Is Invisible

Microwave Ovens Are Hot Physics

Is the Universe Made to Measure?

About the Authors

Take Dummies with you everywhere you go!

Отрывок из книги

Physics is what it’s all about. What what’s all about? Everything. Physics is present in every action around you. And because physics is everywhere, it gets into some tricky places, which means it can be hard to follow. Studying physics can be even worse when you’re reading some dense textbook that’s hard to follow.

For most people who come into contact with physics, textbooks that land with 1,200-page whumps on desks are their only exposure to this amazingly rich and rewarding field. And what follows are weary struggles as the readers try to scale the awesome bulwarks of the massive tomes. Has no brave soul ever wanted to write a book on physics from the reader’s point of view? Yes, and here we come with such a book.

.....

Going from the linear world to the rotational world turns out to be easy, because there’s a handy physics analog (which is a fancy word for “equivalent”) for everything linear in the rotational world. For example, distance traveled becomes angle turned. Speed in meters per second becomes angular speed in angle turned per second. Even linear acceleration becomes rotational acceleration.

So when you know linear motion, rotational motion just falls in your lap. You use the same equations for both linear and angular motion – just different symbols with slightly different meanings (angle replaces distance, for example). You’ll be looping the loop in no time. Chapter 7 has the details.

.....

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