The range of objects and phenomena studied in physics is immense. From the incredibly short lifetime of a nucleus to the age of the Earth, from the tiny sizes of sub-nuclear particles to the vast distance to the edges of the known universe, from the force exerted by a jumping flea to the force between Earth and the Sun, there are enough factors of 10 to challenge the imagination of even the most experienced scientist. Giving numerical values for physical quantities and equations for physical principles allows us to understand nature much more deeply than does qualitative description alone. To comprehend these vast ranges, we must also have accepted units in which to express them. And we shall find that (even in the potentially mundane discussion of meters, kilograms, and seconds) a profound simplicity of nature appears—all physical quantities can be expressed as combinations of only four fundamental physical quantities: length, mass, time, and electric current.
We define a physical quantity either by specifying how it is measured or by stating how it is calculated from other measurements. For example, we define distance and time by specifying methods for measuring them, whereas we define average speed by stating that it is calculated as distance traveled divided by time of travel.
Measurements of physical quantities are expressed in terms of units, which are standardized values. For example, the length of a race, which is a physical quantity, can be expressed in units of meters (for sprinters) or kilometers (for distance runners). Without standardized units, it would be extremely difficult for scientists to express and compare measured values in a meaningful way. (See [link].)
There are two major systems of units used in the world: SI units (also known as the metric system) and English units (also known as the customary or imperial system). English units were historically used in nations once ruled by the British Empire and are still widely used in the United States. Virtually every other country in the world now uses SI units as the standard; the metric system is also the standard system agreed upon by scientists and mathematicians. The acronym “SI” is derived from the French Système International.
SI Units: Fundamental and Derived Units
[link] gives the fundamental SI units that are used throughout this textbook. This text uses non-SI units in a few applications where they are in very common use, such as the measurement of blood pressure in millimeters of mercury (mm Hg). Whenever non-SI units are discussed, they will be tied to SI units through conversions.
Length | Mass | Time | Electric Current |
meter (m) | kilogram (kg) | second (s) | ampere (A) |
It is an intriguing fact that some physical quantities are more fundamental than others and that the most fundamental physical quantities can be defined only in terms of the procedure used to measure them. The units in which they are measured are thus called fundamental units. In this textbook, the fundamental physical quantities are taken to be length, mass, time, and electric current. (Note that electric current will not be introduced until much later in this text.) All other physical quantities, such as force and electric charge, can be expressed as algebraic combinations of length, mass, time, and current (for example, speed is length divided by time); these units are called derived units.
Units of Time, Length, and Mass: The Second, Meter, and Kilogram
The Second
The SI unit for time, the second(abbreviated s), has a long history. For many years it was defined as 1/86,400 of a mean solar day. More recently, a new standard was adopted to gain greater accuracy and to define the second in terms of a non-varying, or constant, physical phenomenon (because the solar day is getting longer due to very gradual slowing of the Earth’s rotation). Cesium atoms can be made to vibrate in a very steady way, and these vibrations can be readily observed and counted. In 1967 the second was redefined as the time required for 9,192,631,770 of these vibrations. (See [link].) Accuracy in the fundamental units is essential, because all measurements are ultimately expressed in terms of fundamental units and can be no more accurate than are the fundamental units themselves.
The Meter
The SI unit for length is the meter (abbreviated m); its definition has also changed over time to become more accurate and precise. The meter was first defined in 1791 as 1/10,000,000 of the distance from the equator to the North Pole. This measurement was improved in 1889 by redefining the meter to be the distance between two engraved lines on a platinum-iridium bar now kept near Paris. By 1960, it had become possible to define the meter even more accurately in terms of the wavelength of light, so it was again redefined as 1,650,763.73 wavelengths of orange light emitted by krypton atoms. In 1983, the meter was given its present definition (partly for greater accuracy) as the distance light travels in a vacuum in 1/299,792,458 of a second. (See [link].) This change defines the speed of light to be exactly 299,792,458 meters per second. The length of the meter will change if the speed of light is someday measured with greater accuracy.
The Kilogram
The SI unit for mass is the kilogram (abbreviated kg); it is defined to be the mass of a platinum-iridium cylinder kept with the old meter standard at the International Bureau of Weights and Measures near Paris. Exact replicas of the standard kilogram are also kept at the United States’ National Institute of Standards and Technology, or NIST, located in Gaithersburg, Maryland outside of Washington D.C., and at other locations around the world. The determination of all other masses can be ultimately traced to a comparison with the standard mass.
Electric current and its accompanying unit, the ampere, will be introduced in Introduction to Electric Current, Resistance, and Ohm's Law when electricity and magnetism are covered. The initial modules in this textbook are concerned with mechanics, fluids, heat, and waves. In these subjects all pertinent physical quantities can be expressed in terms of the fundamental units of length, mass, and time.
Metric Prefixes
SI units are part of the metric system. The metric system is convenient for scientific and engineering calculations because the units are categorized by factors of 10. [link] gives metric prefixes and symbols used to denote various factors of 10.
Metric systems have the advantage that conversions of units involve only powers of 10. There are 100 centimeters in a meter, 1000 meters in a kilometer, and so on. In nonmetric systems, such as the system of U.S. customary units, the relationships are not as simple—there are 12 inches in a foot, 5280 feet in a mile, and so on. Another advantage of the metric system is that the same unit can be used over extremely large ranges of values simply by using an appropriate metric prefix. For example, distances in meters are suitable in construction, while distances in kilometers are appropriate for air travel, and the tiny measure of nanometers are convenient in optical design. With the metric system there is no need to invent new units for particular applications.
The term order of magnitude refers to the scale of a value expressed in the metric system. Each power of $\text{10}$ in the metric system represents a different order of magnitude. For example, ${\text{10}}^{1},\phantom{\rule{0.25em}{0ex}}{\text{10}}^{2},\phantom{\rule{0.25em}{0ex}}{\text{10}}^{3}$, and so forth are all different orders of magnitude. All quantities that can be expressed as a product of a specific power of $\text{10}$ are said to be of the same order of magnitude. For example, the number $\text{800}$ can be written as $8\times {\text{10}}^{2}$, and the number $\text{450}$ can be written as $4.5\times {\text{10}}^{2}.$ Thus, the numbers $\text{800}$ and $\text{450}$ are of the same order of magnitude: ${\text{10}}^{2}.$ Order of magnitude can be thought of as a ballpark estimate for the scale of a value. The diameter of an atom is on the order of ${\text{10}}^{-9}\text{m,}$ while the diameter of the Sun is on the order of ${\text{10}}^{9}\text{m.}$
Prefix | Symbol | Value See Appendix A for a discussion of powers of 10. |
Example (some are approximate) | |||
exa | E | $${\text{10}}^{\text{18}}$$ | exameter | Em | $${\text{10}}^{\text{18}}\text{m}$$ | distance light travels in a century |
peta | P | $${\text{10}}^{\text{15}}$$ | petasecond | Ps | $${\text{10}}^{\text{15}}\text{s}$$ | 30 million years |
tera | T | $${\text{10}}^{\text{12}}$$ | terawatt | TW | $${\text{10}}^{\text{12}}\text{W}$$ | powerful laser output |
giga | G | $${\text{10}}^{9}$$ | gigahertz | GHz | $${\text{10}}^{9}\text{Hz}$$ | a microwave frequency |
mega | M | $${\text{10}}^{6}$$ | megacurie | MCi | $${\text{10}}^{6}\text{Ci}$$ | high radioactivity |
kilo | k | $${\text{10}}^{3}$$ | kilometer | km | $${\text{10}}^{3}\text{m}$$ | about 6/10 mile |
hecto | h | $${\text{10}}^{2}$$ | hectoliter | hL | $${\text{10}}^{2}\text{L}$$ | 26 gallons |
deka | da | $${\text{10}}^{1}$$ | dekagram | dag | $${\text{10}}^{1}\text{g}$$ | teaspoon of butter |
— | — | $${\text{10}}^{0}$$ (=1) | ||||
deci | d | $${\text{10}}^{-1}$$ | deciliter | dL | $${\text{10}}^{-1}\text{L}$$ | less than half a soda |
centi | c | $${\text{10}}^{-2}$$ | centimeter | cm | $${\text{10}}^{-2}\text{m}$$ | fingertip thickness |
milli | m | $${\text{10}}^{-3}$$ | millimeter | mm | $${\text{10}}^{-3}\text{m}$$ | flea at its shoulders |
micro | µ | $${\text{10}}^{-6}$$ | micrometer | µm | $${\text{10}}^{-6}\text{m}$$ | detail in microscope |
nano | n | $${\text{10}}^{-9}$$ | nanogram | ng | $${\text{10}}^{-9}\text{g}$$ | small speck of dust |
pico | p | $${\text{10}}^{-\text{12}}$$ | picofarad | pF | $${\text{10}}^{-\text{12}}\text{F}$$ | small capacitor in radio |
femto | f | $${\text{10}}^{-\text{15}}$$ | femtometer | fm | $${\text{10}}^{-\text{15}}\text{m}$$ | size of a proton |
atto | a | $${\text{10}}^{-\text{18}}$$ | attosecond | as | $${\text{10}}^{-\text{18}}\text{s}$$ | time light crosses an atom |
Known Ranges of Length, Mass, and Time
The vastness of the universe and the breadth over which physics applies are illustrated by the wide range of examples of known lengths, masses, and times in [link]. Examination of this table will give you some feeling for the range of possible topics and numerical values. (See [link] and [link].)
Unit Conversion and Dimensional Analysis
It is often necessary to convert from one type of unit to another. For example, if you are reading a European cookbook, some quantities may be expressed in units of liters and you need to convert them to cups. Or, perhaps you are reading walking directions from one location to another and you are interested in how many miles you will be walking. In this case, you will need to convert units of feet to miles.
Let us consider a simple example of how to convert units. Let us say that we want to convert 80 meters (m) to kilometers (km).
The first thing to do is to list the units that you have and the units that you want to convert to. In this case, we have units in meters and we want to convert to kilometers.
Next, we need to determine a conversion factor relating meters to kilometers. A conversion factor is a ratio expressing how many of one unit are equal to another unit. For example, there are 12 inches in 1 foot, 100 centimeters in 1 meter, 60 seconds in 1 minute, and so on. In this case, we know that there are 1,000 meters in 1 kilometer.
Now we can set up our unit conversion. We will write the units that we have and then multiply them by the conversion factor so that the units cancel out, as shown:
Note that the unwanted m unit cancels, leaving only the desired km unit. You can use this method to convert between any types of unit.
Click [link] for a more complete list of conversion factors.
Lengths in meters | Masses in kilograms (more precise values in parentheses) | Times in seconds (more precise values in parentheses) | |||
${\text{10}}^{-\text{18}}$ | Present experimental limit to smallest observable detail | $${\text{10}}^{-\text{30}}$$ | Mass of an electron $\left(9\text{.}\text{11}\times {\text{10}}^{-\text{31}}\phantom{\rule{0.25em}{0ex}}\text{kg}\right)$ | $${\text{10}}^{-\text{23}}$$ | Time for light to cross a proton |
$${\text{10}}^{-\text{15}}$$ | Diameter of a proton | $${\text{10}}^{-\text{27}}$$ | Mass of a hydrogen atom $\left(1\text{.}\text{67}\times {\text{10}}^{-\text{27}}\phantom{\rule{0.25em}{0ex}}\text{kg}\right)$ | $${\text{10}}^{-\text{22}}$$ | Mean life of an extremely unstable nucleus |
$${\text{10}}^{-\text{14}}$$ | Diameter of a uranium nucleus | $${\text{10}}^{-\text{15}}$$ | Mass of a bacterium | $${\text{10}}^{-\text{15}}$$ | Time for one oscillation of visible light |
$${\text{10}}^{-\text{10}}$$ | Diameter of a hydrogen atom | $${\text{10}}^{-5}$$ | Mass of a mosquito | $${\text{10}}^{-\text{13}}$$ | Time for one vibration of an atom in a solid |
$${\text{10}}^{-8}$$ | Thickness of membranes in cells of living organisms | $${\text{10}}^{-2}$$ | Mass of a hummingbird | $${\text{10}}^{-8}$$ | Time for one oscillation of an FM radio wave |
$${\text{10}}^{-6}$$ | Wavelength of visible light | $$\text{1}$$ | Mass of a liter of water (about a quart) | $${\text{10}}^{-3}$$ | Duration of a nerve impulse |
$${\text{10}}^{-3}$$ | Size of a grain of sand | $${\text{10}}^{2}$$ | Mass of a person | $$\text{1}$$ | Time for one heartbeat |
$$\text{1}$$ | Height of a 4-year-old child | $${\text{10}}^{3}$$ | Mass of a car | $${\text{10}}^{5}$$ | One day $\left(8\text{.}\text{64}\times {\text{10}}^{4}\phantom{\rule{0.25em}{0ex}}\text{s}\right)$ |
$${\text{10}}^{2}$$ | Length of a football field | $${\text{10}}^{8}$$ | Mass of a large ship | $${\text{10}}^{7}$$ | One year (y) $\left(3\text{.}\text{16}\times {\text{10}}^{7}\phantom{\rule{0.25em}{0ex}}\text{s}\right)$ |
$${\text{10}}^{4}$$ | Greatest ocean depth | $${\text{10}}^{\text{12}}$$ | Mass of a large iceberg | $${\text{10}}^{9}$$ | About half the life expectancy of a human |
$${\text{10}}^{7}$$ | Diameter of the Earth | $${\text{10}}^{\text{15}}$$ | Mass of the nucleus of a comet | $${\text{10}}^{\text{11}}$$ | Recorded history |
$${\text{10}}^{\text{11}}$$ | Distance from the Earth to the Sun | $${\text{10}}^{\text{23}}$$ | Mass of the Moon $\left(7\text{.}\text{35}\times {\text{10}}^{\text{22}}\phantom{\rule{0.25em}{0ex}}\text{kg}\right)$ | $${\text{10}}^{\text{17}}$$ | Age of the Earth |
$${\text{10}}^{\text{16}}$$ | Distance traveled by light in 1 year (a light year) | $${\text{10}}^{\text{25}}$$ | Mass of the Earth $\left(5\text{.}\text{97}\times {\text{10}}^{\text{24}}\phantom{\rule{0.25em}{0ex}}\text{kg}\right)$ | $${\text{10}}^{\text{18}}$$ | Age of the universe |
$${\text{10}}^{\text{21}}$$ | Diameter of the Milky Way galaxy | $${\text{10}}^{\text{30}}$$ | Mass of the Sun $\left(1\text{.}\text{99}\times {\text{10}}^{\text{30}}\phantom{\rule{0.25em}{0ex}}\text{kg}\right)$ | ||
$${\text{10}}^{\text{22}}$$ | Distance from the Earth to the nearest large galaxy (Andromeda) | $${\text{10}}^{\text{42}}$$ | Mass of the Milky Way galaxy (current upper limit) | ||
$${\text{10}}^{\text{26}}$$ | Distance from the Earth to the edges of the known universe | $${\text{10}}^{\text{53}}$$ | Mass of the known universe (current upper limit) |
Suppose that you drive the 10.0 km from your university to home in 20.0 min. Calculate your average speed (a) in kilometers per hour (km/h) and (b) in meters per second (m/s). (Note: Average speed is distance traveled divided by time of travel.)
Strategy
First we calculate the average speed using the given units. Then we can get the average speed into the desired units by picking the correct conversion factor and multiplying by it. The correct conversion factor is the one that cancels the unwanted unit and leaves the desired unit in its place.
Solution for (a)
(1) Calculate average speed. Average speed is distance traveled divided by time of travel. (Take this definition as a given for now—average speed and other motion concepts will be covered in a later module.) In equation form,
(2) Substitute the given values for distance and time.
(3) Convert km/min to km/h: multiply by the conversion factor that will cancel minutes and leave hours. That conversion factor is $\text{60 min/hr}$. Thus,
Discussion for (a)
To check your answer, consider the following:
(1) Be sure that you have properly cancelled the units in the unit conversion. If you have written the unit conversion factor upside down, the units will not cancel properly in the equation. If you accidentally get the ratio upside down, then the units will not cancel; rather, they will give you the wrong units as follows:
which are obviously not the desired units of km/h.
(2) Check that the units of the final answer are the desired units. The problem asked us to solve for average speed in units of km/h and we have indeed obtained these units.
(3) Check the significant figures. Because each of the values given in the problem has three significant figures, the answer should also have three significant figures. The answer 30.0 km/hr does indeed have three significant figures, so this is appropriate. Note that the significant figures in the conversion factor are not relevant because an hour is defined to be 60 minutes, so the precision of the conversion factor is perfect.
(4) Next, check whether the answer is reasonable. Let us consider some information from the problem—if you travel 10 km in a third of an hour (20 min), you would travel three times that far in an hour. The answer does seem reasonable.
Solution for (b)
There are several ways to convert the average speed into meters per second.
(1) Start with the answer to (a) and convert km/h to m/s. Two conversion factors are needed—one to convert hours to seconds, and another to convert kilometers to meters.
(2) Multiplying by these yields
Discussion for (b)
If we had started with 0.500 km/min, we would have needed different conversion factors, but the answer would have been the same: 8.33 m/s.
You may have noted that the answers in the worked example just covered were given to three digits. Why? When do you need to be concerned about the number of digits in something you calculate? Why not write down all the digits your calculator produces? The module Accuracy, Precision, and Significant Figures will help you answer these questions.
Summary
- Physical quantities are a characteristic or property of an object that can be measured or calculated from other measurements.
- Units are standards for expressing and comparing the measurement of physical quantities. All units can be expressed as combinations of four fundamental units.
- The four fundamental units we will use in this text are the meter (for length), the kilogram (for mass), the second (for time), and the ampere (for electric current). These units are part of the metric system, which uses powers of 10 to relate quantities over the vast ranges encountered in nature.
- The four fundamental units are abbreviated as follows: meter, m; kilogram, kg; second, s; and ampere, A. The metric system also uses a standard set of prefixes to denote each order of magnitude greater than or lesser than the fundamental unit itself.
- Unit conversions involve changing a value expressed in one type of unit to another type of unit. This is done by using conversion factors, which are ratios relating equal quantities of different units.
Conceptual Questions
Identify some advantages of metric units.
Problems & Exercises
The speed limit on some interstate highways is roughly 100 km/h. (a) What is this in meters per second? (b) How many miles per hour is this?
- $\text{27}\text{.}\text{8 m/s}$
- $\text{62}\text{.}\text{1 mph}$
A car is traveling at a speed of $\text{33 m/s}$. (a) What is its speed in kilometers per hour? (b) Is it exceeding the $\text{90 km/h}$ speed limit?
Show that $1\text{.}\text{0 m/s}=3\text{.}\text{6 km/h}$. Hint: Show the explicit steps involved in converting $1\text{.}\text{0 m/s}=3\text{.}\text{6 km/h.}$
$\frac{\text{1.0 m}}{\mathrm{s}}=\frac{1\text{.}\text{0 m}}{\mathrm{s}}\times \frac{\text{3600 s}}{\text{1 hr}}\times \frac{\mathrm{1\; km}}{\text{1000 m}}$
$=3\text{.}\text{6 km/h}$.
American football is played on a 100-yd-long field, excluding the end zones. How long is the field in meters? (Assume that 1 meter equals 3.281 feet.)
Soccer fields vary in size. A large soccer field is 115 m long and 85 m wide. What are its dimensions in feet and inches? (Assume that 1 meter equals 3.281 feet.)
length: $\text{377 ft}$; $4\text{.}\text{53}\times {\text{10}}^{3}\text{in}\text{.}$ width: $\text{280ft}$; $3\text{.}3\times {\text{10}}^{3}\text{in}$.
What is the height in meters of a person who is 6 ft 1.0 in. tall? (Assume that 1 meter equals 39.37 in.)
Mount Everest, at 29,028 feet, is the tallest mountain on the Earth. What is its height in kilometers? (Assume that 1 kilometer equals 3,281 feet.)
$8\text{.}\text{847 km}$
The speed of sound is measured to be $\text{342 m/s}$ on a certain day. What is this in km/h?
Tectonic plates are large segments of the Earth’s crust that move slowly. Suppose that one such plate has an average speed of 4.0 cm/year. (a) What distance does it move in 1 s at this speed? (b) What is its speed in kilometers per million years?
(a) $1\text{.}3\times {\text{10}}^{-9}\text{m}$
(b) $\text{40 km/My}$
(a) Refer to [link] to determine the average distance between the Earth and the Sun. Then calculate the average speed of the Earth in its orbit in kilometers per second. (b) What is this in meters per second?
- College Physics
- Preface
- Introduction: The Nature of Science and Physics
- Kinematics
- Introduction to One-Dimensional Kinematics
- Displacement
- Vectors, Scalars, and Coordinate Systems
- Time, Velocity, and Speed
- Acceleration
- Motion Equations for Constant Acceleration in One Dimension
- Problem-Solving Basics for One-Dimensional Kinematics
- Falling Objects
- Graphical Analysis of One-Dimensional Motion
- Two-Dimensional Kinematics
- Dynamics: Force and Newton's Laws of Motion
- Introduction to Dynamics: Newton’s Laws of Motion
- Development of Force Concept
- Newton’s First Law of Motion: Inertia
- Newton’s Second Law of Motion: Concept of a System
- Newton’s Third Law of Motion: Symmetry in Forces
- Normal, Tension, and Other Examples of Forces
- Problem-Solving Strategies
- Further Applications of Newton’s Laws of Motion
- Extended Topic: The Four Basic Forces—An Introduction
- Further Applications of Newton's Laws: Friction, Drag, and Elasticity
- Uniform Circular Motion and Gravitation
- Work, Energy, and Energy Resources
- Linear Momentum and Collisions
- Statics and Torque
- Rotational Motion and Angular Momentum
- Introduction to Rotational Motion and Angular Momentum
- Angular Acceleration
- Kinematics of Rotational Motion
- Dynamics of Rotational Motion: Rotational Inertia
- Rotational Kinetic Energy: Work and Energy Revisited
- Angular Momentum and Its Conservation
- Collisions of Extended Bodies in Two Dimensions
- Gyroscopic Effects: Vector Aspects of Angular Momentum
- Fluid Statics
- Fluid Dynamics and Its Biological and Medical Applications
- Introduction to Fluid Dynamics and Its Biological and Medical Applications
- Flow Rate and Its Relation to Velocity
- Bernoulli’s Equation
- The Most General Applications of Bernoulli’s Equation
- Viscosity and Laminar Flow; Poiseuille’s Law
- The Onset of Turbulence
- Motion of an Object in a Viscous Fluid
- Molecular Transport Phenomena: Diffusion, Osmosis, and Related Processes
- Temperature, Kinetic Theory, and the Gas Laws
- Heat and Heat Transfer Methods
- Thermodynamics
- Introduction to Thermodynamics
- The First Law of Thermodynamics
- The First Law of Thermodynamics and Some Simple Processes
- Introduction to the Second Law of Thermodynamics: Heat Engines and Their Efficiency
- Carnot’s Perfect Heat Engine: The Second Law of Thermodynamics Restated
- Applications of Thermodynamics: Heat Pumps and Refrigerators
- Entropy and the Second Law of Thermodynamics: Disorder and the Unavailability of Energy
- Statistical Interpretation of Entropy and the Second Law of Thermodynamics: The Underlying Explanation
- Oscillatory Motion and Waves
- Introduction to Oscillatory Motion and Waves
- Hooke’s Law: Stress and Strain Revisited
- Period and Frequency in Oscillations
- Simple Harmonic Motion: A Special Periodic Motion
- The Simple Pendulum
- Energy and the Simple Harmonic Oscillator
- Uniform Circular Motion and Simple Harmonic Motion
- Damped Harmonic Motion
- Forced Oscillations and Resonance
- Waves
- Superposition and Interference
- Energy in Waves: Intensity
- Physics of Hearing
- Electric Charge and Electric Field
- Introduction to Electric Charge and Electric Field
- Static Electricity and Charge: Conservation of Charge
- Conductors and Insulators
- Coulomb’s Law
- Electric Field: Concept of a Field Revisited
- Electric Field Lines: Multiple Charges
- Electric Forces in Biology
- Conductors and Electric Fields in Static Equilibrium
- Applications of Electrostatics
- Electric Potential and Electric Field
- Electric Current, Resistance, and Ohm's Law
- Circuits, Bioelectricity, and DC Instruments
- Magnetism
- Introduction to Magnetism
- Magnets
- Ferromagnets and Electromagnets
- Magnetic Fields and Magnetic Field Lines
- Magnetic Field Strength: Force on a Moving Charge in a Magnetic Field
- Force on a Moving Charge in a Magnetic Field: Examples and Applications
- The Hall Effect
- Magnetic Force on a Current-Carrying Conductor
- Torque on a Current Loop: Motors and Meters
- Magnetic Fields Produced by Currents: Ampere’s Law
- Magnetic Force between Two Parallel Conductors
- More Applications of Magnetism
- Electromagnetic Induction, AC Circuits, and Electrical Technologies
- Introduction to Electromagnetic Induction, AC Circuits and Electrical Technologies
- Induced Emf and Magnetic Flux
- Faraday’s Law of Induction: Lenz’s Law
- Motional Emf
- Eddy Currents and Magnetic Damping
- Electric Generators
- Back Emf
- Transformers
- Electrical Safety: Systems and Devices
- Inductance
- RL Circuits
- Reactance, Inductive and Capacitive
- RLC Series AC Circuits
- Electromagnetic Waves
- Geometric Optics
- Vision and Optical Instruments
- Wave Optics
- Introduction to Wave Optics
- The Wave Aspect of Light: Interference
- Huygens's Principle: Diffraction
- Young’s Double Slit Experiment
- Multiple Slit Diffraction
- Single Slit Diffraction
- Limits of Resolution: The Rayleigh Criterion
- Thin Film Interference
- Polarization
- *Extended Topic* Microscopy Enhanced by the Wave Characteristics of Light
- Special Relativity
- Introduction to Quantum Physics
- Atomic Physics
- Introduction to Atomic Physics
- Discovery of the Atom
- Discovery of the Parts of the Atom: Electrons and Nuclei
- Bohr’s Theory of the Hydrogen Atom
- X Rays: Atomic Origins and Applications
- Applications of Atomic Excitations and De-Excitations
- The Wave Nature of Matter Causes Quantization
- Patterns in Spectra Reveal More Quantization
- Quantum Numbers and Rules
- The Pauli Exclusion Principle
- Radioactivity and Nuclear Physics
- Medical Applications of Nuclear Physics
- Particle Physics
- Frontiers of Physics
- Atomic Masses
- Selected Radioactive Isotopes
- Useful Information
- Glossary of Key Symbols and Notation