9.2.3.2. Amplifiers
Table of Contents
Basic idea of amplification
An amplifier is a circuit that takes a small input signal and produces a larger output signal. In operational amplifier circuits, the op amp itself is the active device, but the amount of amplification is usually controlled by external components, most often resistors.
The important point is that an op amp by itself has a very large internal gain, but useful amplifier circuits are made by using feedback. Feedback lets us set a predictable gain and makes the circuit more stable and practical.
If the input signal is a voltage, then the amplifier usually aims to produce an output voltage proportional to that input. This proportionality is called the voltage gain.
For a linear amplifier,
$$
A_v = \frac{V_{\text{out}}}{V_{\text{in}}}
$$
where $A_v$ is the voltage gain.
If $A_v$ is positive, output and input have the same sign.
If $A_v$ is negative, the output is inverted.
Why op amp amplifiers need feedback
An ideal op amp has extremely large open loop gain. That means even a tiny difference between its two input terminals would try to drive the output to a very large value. In practice, without feedback, the output usually saturates near the power supply limits. That is not useful for ordinary signal amplification.
By connecting part of the output back to the input, we create negative feedback. This causes the op amp to adjust its output so that the voltage difference between the two input terminals becomes very small.
In many ideal op amp amplifier circuits, we use two key rules. These belong to ideal op amp behavior, but they are especially important here because they make gain calculations simple.
For an ideal op amp operating with negative feedback,
$$
I_+ = I_- = 0
$$
and
$$
V_+ \approx V_-
$$
This second relation is often called the virtual short condition.
Inverting amplifier
One of the most common op amp amplifier circuits is the inverting amplifier. The input signal goes through a resistor to the inverting input, and another resistor connects the output back to that same input. The noninverting input is connected to ground.
Because the noninverting input is at $0 \, \text{V}$, the inverting input is also held very close to $0 \, \text{V}$ by negative feedback. This point is often called a virtual ground. It is not physically connected to ground, but its voltage is approximately zero.
Using current conservation at the inverting input node gives the gain formula.
$$
\frac{V_{\text{in}} - 0}{R_{\text{in}}} = \frac{0 - V_{\text{out}}}{R_f}
$$
So,
$$
V_{\text{out}} = -\frac{R_f}{R_{\text{in}}} V_{\text{in}}
$$
For the inverting amplifier,
$$
A_v = \frac{V_{\text{out}}}{V_{\text{in}}} = -\frac{R_f}{R_{\text{in}}}
$$
The negative sign means the output is inverted.
Noninverting amplifier
Another very important circuit is the noninverting amplifier. Here the input signal is applied directly to the noninverting input. The inverting input receives a fraction of the output through a resistor network.
The op amp adjusts the output so that the inverting input voltage matches the noninverting input voltage. If the noninverting input is at $V_{\text{in}}$, then the inverting input is also approximately at $V_{\text{in}}$.
If the resistor from output to the inverting input is $R_f$, and the resistor from the inverting input to ground is $R_1$, then the inverting input sees a divided version of the output:
$$
V_- = V_{\text{out}} \frac{R_1}{R_1 + R_f}
$$
Since $V_- \approx V_+ = V_{\text{in}}$,
$$
V_{\text{in}} = V_{\text{out}} \frac{R_1}{R_1 + R_f}
$$
So,
$$
V_{\text{out}} = \left(1 + \frac{R_f}{R_1}\right) V_{\text{in}}
$$
For the noninverting amplifier,
$$
A_v = 1 + \frac{R_f}{R_1}
$$
This gain is positive, so the output is not inverted.
Voltage follower
A special case of the noninverting amplifier is the voltage follower, also called a buffer. In this circuit, the output is connected directly to the inverting input, with no resistor divider. The input signal goes to the noninverting input.
This gives a gain of 1:
$$
V_{\text{out}} = V_{\text{in}}
$$
Why is this useful if it does not increase voltage? Because it can isolate one part of a circuit from another. An ideal op amp has very high input resistance and low output resistance, so the buffer can pass a voltage from one stage to the next without significantly loading the source.
For a voltage follower,
$$
A_v = 1
$$
It does not amplify voltage, but it improves signal transfer between circuits.
Comparing common op amp amplifier types
The three circuits above are the foundation of many analog electronics applications.
| Amplifier type | Input terminal used | Gain formula | Inverts signal |
|---|---|---|---|
| Inverting | Inverting input through resistor | $-\dfrac{R_f}{R_{\text{in}}}$ | Yes |
| Noninverting | Noninverting input directly | $1 + \dfrac{R_f}{R_1}$ | No |
| Voltage follower | Noninverting input directly | $1$ | No |
Input and output limitations
Real op amp amplifiers cannot produce any output voltage whatsoever. The output is limited by the supply voltages. If the circuit tries to produce a larger output than the power supply allows, the output saturates.
For example, if an op amp is powered by $\pm 12 \, \text{V}$, the output cannot usually go beyond those limits, and often not quite all the way to them. So even if the gain formula predicts a certain output, the actual output will flatten if that value is too large.
Suppose an amplifier has gain $10$ and the input is $2 \, \text{V}$. The predicted output is
$$
V_{\text{out}} = 10 \times 2 = 20 \, \text{V}
$$
If the supply does not allow $20 \, \text{V}$, the circuit saturates instead of remaining linear.
Amplifier formulas such as
$$
V_{\text{out}} = A_v V_{\text{in}}
$$
are valid only when the op amp remains in its linear operating region and does not saturate.
Gain in decibels
Amplifier strength is often expressed using decibels, especially when comparing signal levels.
For voltage gain, when the same resistance conditions apply at input and output, the gain in decibels is
$$
G_{\text{dB}} = 20 \log_{10} \left| A_v \right|
$$
If $A_v = 10$, then
$$
G_{\text{dB}} = 20 \log_{10}(10) = 20 \, \text{dB}
$$
If $A_v = 2$, then
$$
G_{\text{dB}} \approx 20 \log_{10}(2) \approx 6.0 \, \text{dB}
$$
This does not replace the ordinary gain formula, but it is a convenient way to describe amplification.
A simple example
Consider an inverting amplifier with $R_{\text{in}} = 2 \, \text{k}\Omega$ and $R_f = 10 \, \text{k}\Omega$.
Its gain is
$$
A_v = -\frac{R_f}{R_{\text{in}}} = -\frac{10}{2} = -5
$$
If the input is
$$
V_{\text{in}} = 0.3 \, \text{V}
$$
then the output is
$$
V_{\text{out}} = -5(0.3) = -1.5 \, \text{V}
$$
The output is five times larger in magnitude and opposite in sign.
Now consider a noninverting amplifier with $R_1 = 1 \, \text{k}\Omega$ and $R_f = 4 \, \text{k}\Omega$.
Its gain is
$$
A_v = 1 + \frac{R_f}{R_1} = 1 + \frac{4}{1} = 5
$$
With the same input, $V_{\text{in}} = 0.3 \, \text{V}$,
$$
V_{\text{out}} = 5(0.3) = 1.5 \, \text{V}
$$
This time the output keeps the same sign as the input.
Practical meaning
In real electronics, amplifier circuits are used to boost weak sensor signals, prepare audio signals, and connect circuit stages without unwanted loading effects. The op amp makes this possible with simple resistor networks that set the desired gain.
The most important skill at this stage is to recognize the circuit form and apply the correct gain relation. Later circuits are often built from these same amplifier ideas.
Key amplifier formulas for ideal op amp circuits:
Inverting amplifier:
$$
V_{\text{out}} = -\frac{R_f}{R_{\text{in}}} V_{\text{in}}
$$
Noninverting amplifier:
$$
V_{\text{out}} = \left(1 + \frac{R_f}{R_1}\right) V_{\text{in}}
$$
Voltage follower:
$$
V_{\text{out}} = V_{\text{in}}
$$
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- ☰ 4. Part III: Thermodynamics
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- ☰ 4.2. Kinetic Theory of Gases
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- ☰ 4.3. Thermodynamics
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- ☰ 5. Part IV: Electricity and Magnetism
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- ☰ 5.3. Capacitance
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- ☰ 5.4. Electric Current and Resistance
- ☰ 5.4.1. Electric Current
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- ☰ 5.5. DC Circuits
- ☰ 5.5.1. Kirchhoff's Laws
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- ☰ 5.5.3. RC Circuits
- ☰ 5.5.4. Measuring Instruments
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- ☰ 5.6. Magnetism
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- ☰ 5.6.4. Force on Current-Carrying Wires
- ☰ 5.6.5. Torque on Current Loops
- ☰ 5.6.6. Biot-Savart Law
- ☰ 5.6.7. Ampère's Law
- ☰ 5.6.8. Solenoids
- ☰ 5.6.9. Magnetic Materials
-
- ☰ 5.7. Electromagnetic Induction
- ☰ 5.7.1. Magnetic Flux
- ☰ 5.7.2. Faraday's Law
- ☰ 5.7.3. Lenz's Law
- ☰ 5.7.4. Motional EMF
- ☰ 5.7.5. Self-Inductance
- ☰ 5.7.6. Mutual Inductance
- ☰ 5.7.7. RL Circuits
- ☰ 5.7.8. LC Oscillations
-
- ☰ 5.8. Alternating Current
- ☰ 5.8.1. AC Voltage and Current
- ☰ 5.8.2. RMS Quantities
- ☰ 5.8.3. Resistors in AC Circuits
- ☰ 5.8.4. Capacitors in AC Circuits
- ☰ 5.8.5. Inductors in AC Circuits
- ☰ 5.8.6. RLC Circuits
- ☰ 5.8.7. Impedance
- ☰ 5.8.8. Resonance
- ☰ 5.8.9. Transformers
-
- ☰ 5.9. Maxwell's Equations and Electromagnetic Waves
- ☰ 5.9.1. Gauss's Law for Electricity
- ☰ 5.9.2. Gauss's Law for Magnetism
- ☰ 5.9.3. Faraday's Law
- ☰ 5.9.4. Ampère-Maxwell Law
- ☰ 5.9.5. Electromagnetic Waves
- ☰ 5.9.6. Speed of Light
- ☰ 5.9.7. Electromagnetic Spectrum
- ☰ 5.9.8. Poynting Vector
- ☰ 5.9.9. Radiation Pressure
-
-
- ☰ 6. Part V: Optics
- ☰ 6.1. Geometrical Optics
- ☰ 6.1.1. Nature of Light
- ☰ 6.1.2. Reflection
- ☰ 6.1.3. Plane Mirrors
- ☰ 6.1.4. Refraction
- ☰ 6.1.5. Snell's Law
- ☰ 6.1.6. Total Internal Reflection
- ☰ 6.1.7. Spherical Mirrors
- ☰ 6.1.8. Thin Lenses
- ☰ 6.1.9. Mirror Equation
- ☰ 6.1.10. Lens Equation
- ☰ 6.1.11. Magnification
- ☰ 6.1.12. Ray Diagrams
- ☰ 6.1.13. Optical Instruments
-
- ☰ 6.2. Wave Optics
- ☰ 6.2.1. Interference
- ☰ 6.2.2. Young's Double-Slit Experiment
- ☰ 6.2.3. Diffraction
- ☰ 6.2.4. Single-Slit Diffraction
- ☰ 6.2.5. Diffraction Gratings
- ☰ 6.2.6. Polarization
- ☰ 6.2.7. Malus's Law
- ☰ 6.2.8. Brewster's Angle
- ☰ 6.2.9. Rayleigh Criterion
- ☰ 6.2.10. Optical Resolution
-
-
- ☰ 7. Part VI: Modern Physics
- ☰ 7.1. Special Relativity
- ☰ 7.1.1. Galilean Relativity
- ☰ 7.1.2. Michelson-Morley Experiment
- ☰ 7.1.3. Einstein's Postulates
- ☰ 7.1.4. Lorentz Transformations
- ☰ 7.1.5. Relativity of Simultaneity
- ☰ 7.1.6. Time Dilation
- ☰ 7.1.7. Length Contraction
- ☰ 7.1.8. Relativistic Velocity Addition
- ☰ 7.1.9. Relativistic Momentum
- ☰ 7.1.10. Relativistic Energy
- ☰ 7.1.11. Mass-Energy Equivalence
- ☰ 7.1.12. Energy-Momentum Relation
- ☰ 7.1.13. Spacetime Diagrams
- ☰ 7.1.14. Light Cones
-
- ☰ 7.2. Introduction to Quantum Physics
- ☰ 7.2.1. Blackbody Radiation
- ☰ 7.2.2. Planck's Hypothesis
- ☰ 7.2.3. Photoelectric Effect
- ☰ 7.2.4. Photon Energy
- ☰ 7.2.5. Photon Momentum
- ☰ 7.2.6. Compton Scattering
- ☰ 7.2.7. de Broglie Wavelength
- ☰ 7.2.8. Matter Waves
- ☰ 7.2.9. Wave-Particle Duality
- ☰ 7.2.10. Double-Slit Experiment
- ☰ 7.2.11. Heisenberg Uncertainty Principle
-
- ☰ 7.3. Quantum Mechanics
- ☰ 7.3.1. Wave Function
- ☰ 7.3.2. Probability Interpretation
- ☰ 7.3.3. Normalization
- ☰ 7.3.4. Schrödinger Equation
- ☰ 7.3.5. Operators and Observables
- ☰ 7.3.6. Expectation Values
- ☰ 7.3.7. Particle in a Box
- ☰ 7.3.8. Finite Potential Wells
- ☰ 7.3.9. Quantum Tunneling
- ☰ 7.3.10. Quantum Harmonic Oscillator
- ☰ 7.3.11. Hydrogen Atom
- ☰ 7.3.12. Quantum Numbers
- ☰ 7.3.13. Angular Momentum
- ☰ 7.3.14. Spin
- ☰ 7.3.15. Stern-Gerlach Experiment
- ☰ 7.3.16. Pauli Exclusion Principle
-
- ☰ 7.4. Atomic Physics
- ☰ 7.4.1. Thomson Atomic Model
- ☰ 7.4.2. Rutherford Atomic Model
- ☰ 7.4.3. Bohr Model
- ☰ 7.4.4. Atomic Spectra
- ☰ 7.4.5. Hydrogen Spectrum
- ☰ 7.4.6. Electron Shells
- ☰ 7.4.7. Orbitals
- ☰ 7.4.8. Electron Configurations
- ☰ 7.4.9. X-Ray Spectra
- ☰ 7.4.10. Atomic Transitions
- ☰ 7.4.11. Lasers
- ☰ 7.4.12. Stimulated Emission
-
-
- ☰ 8. Part VII: Nuclear and Particle Physics
- ☰ 8.1. Nuclear Structure
- ☰ 8.1.1. The Atomic Nucleus
- ☰ 8.1.1.1. Protons and Neutrons
- ☰ 8.1.1.2. Atomic Number
- ☰ 8.1.1.3. Mass Number
- ☰ 8.1.1.4. Isotopes
- ☰ 8.1.1.5. Isotones
- ☰ 8.1.1.6. Isobars
-
- ☰ 8.1.2. Nuclear Size and Density
- ☰ 8.1.2.1. Nuclear Radius
- ☰ 8.1.2.2. Nuclear Density
- ☰ 8.1.2.3. Nuclear Charge Distribution
-
- ☰ 8.1.3. Nuclear Forces
- ☰ 8.1.3.1. Strong Nuclear Force
- ☰ 8.1.3.2. Properties of Nuclear Forces
- ☰ 8.1.3.3. Proton-Neutron Interaction
- ☰ 8.1.3.4. Nuclear Stability
-
- ☰ 8.1.4. Mass and Binding Energy
- ☰ 8.1.4.1. Atomic Mass Units
- ☰ 8.1.4.2. Mass Defect
- ☰ 8.1.4.3. Binding Energy
- ☰ 8.1.4.4. Binding Energy per Nucleon
- ☰ 8.1.4.5. Binding-Energy Curve
-
- ☰ 8.1.5. Nuclear Models
- ☰ 8.1.5.1. Liquid-Drop Model
- ☰ 8.1.5.2. Semi-Empirical Mass Formula
- ☰ 8.1.5.3. Nuclear Shell Model
- ☰ 8.1.5.4. Magic Numbers
- ☰ 8.1.5.5. Collective Model
-
- ☰ 8.1.6. Nuclear Spin and Magnetic Moments
- ☰ 8.1.6.1. Nuclear Angular Momentum
- ☰ 8.1.6.2. Nuclear Spin
- ☰ 8.1.6.3. Nuclear Magnetic Moment
-
-
- ☰ 8.2. Radioactivity and Nuclear Decay
- ☰ 8.2.1. Radioactive Decay
- ☰ 8.2.1.1. Nuclear Instability
- ☰ 8.2.1.2. Random Nature of Decay
- ☰ 8.2.1.3. Decay Constant
-
- ☰ 8.2.2. Radioactive Decay Law
- ☰ 8.2.2.1. Exponential Decay
- ☰ 8.2.2.2. Activity
- ☰ 8.2.2.3. Half-Life
- ☰ 8.2.2.4. Mean Lifetime
-
- ☰ 8.2.3. Alpha Decay
- ☰ 8.2.3.1. Alpha Particles
- ☰ 8.2.3.2. Energy of Alpha Decay
-
- ☰ 8.2.4. Beta Decay
- ☰ 8.2.4.1. Beta-Minus Decay
- ☰ 8.2.4.2. Beta-Plus Decay
- ☰ 8.2.4.3. Electron Capture
- ☰ 8.2.4.4. Neutrinos
- ☰ 8.2.4.5. Energy Spectrum
-
- ☰ 8.2.5. Gamma Decay
- ☰ 8.2.5.1. Nuclear Excited States
- ☰ 8.2.5.2. Gamma-Ray Emission
- ☰ 8.2.5.3. Internal Conversion
-
- ☰ 8.2.6. Decay Chains
- ☰ 8.2.6.1. Parent and Daughter Nuclei
- ☰ 8.2.6.2. Secular Equilibrium
- ☰ 8.2.6.3. Natural Radioactive Series
-
-
- ☰ 8.3. Interaction of Radiation with Matter
- ☰ 8.3.1. Charged Particle Interactions
- ☰ 8.3.1.1. Ionization
- ☰ 8.3.1.2. Excitation
- ☰ 8.3.1.3. Energy Loss
- ☰ 8.3.1.4. Stopping Power
- ☰ 8.3.1.5. Range
-
- ☰ 8.3.2. Heavy Charged Particles
- ☰ 8.3.2.1. Alpha Particles
- ☰ 8.3.2.2. Bragg Curve
- ☰ 8.3.2.3. Bragg Peak
-
- ☰ 8.3.3. Electron Interactions
- ☰ 8.3.3.1. Collisional Energy Loss
- ☰ 8.3.3.2. Bremsstrahlung
- ☰ 8.3.3.3. Electron Range
-
- ☰ 8.3.4. Photon Interactions
- ☰ 8.3.4.1. Pair Production
- ☰ 8.3.4.2. Rayleigh Scattering
-
- ☰ 8.3.5. Attenuation of Radiation
- ☰ 8.3.5.1. Linear Attenuation Coefficient
- ☰ 8.3.5.2. Mass Attenuation Coefficient
- ☰ 8.3.5.3. Exponential Attenuation
- ☰ 8.3.5.4. Half-Value Layer
-
- ☰ 8.3.6. Neutron Interactions
- ☰ 8.3.6.1. Elastic Scattering
- ☰ 8.3.6.2. Inelastic Scattering
- ☰ 8.3.6.3. Neutron Capture
- ☰ 8.3.6.4. Neutron Moderation
-
-
- ☰ 8.4. Radiation Detection and Measurement
- ☰ 8.4.1. Principles of Radiation Detection
- ☰ 8.4.1.1. Energy Deposition
- ☰ 8.4.1.2. Detector Efficiency
- ☰ 8.4.1.3. Energy Resolution
- ☰ 8.4.1.4. Timing Resolution
- ☰ 8.4.1.5. Dead Time
-
- ☰ 8.4.2. Gas-Filled Detectors
- ☰ 8.4.2.1. Ionization Chambers
- ☰ 8.4.2.2. Proportional Counters
- ☰ 8.4.2.3. Geiger-Müller Counters
-
- ☰ 8.4.3. Scintillation Detectors
- ☰ 8.4.3.1. Scintillation Process
- ☰ 8.4.3.2. Organic Scintillators
- ☰ 8.4.3.3. Inorganic Scintillators
- ☰ 8.4.3.4. Photomultiplier Tubes
- ☰ 8.4.3.5. Silicon Photomultipliers
-
- ☰ 8.4.4. Semiconductor Detectors
- ☰ 8.4.4.1. Silicon Detectors
- ☰ 8.4.4.2. Germanium Detectors
- ☰ 8.4.4.3. Electron-Hole Pair Creation
-
- ☰ 8.4.5. Gamma-Ray Spectroscopy
- ☰ 8.4.5.1. Photopeak
- ☰ 8.4.5.2. Compton Continuum
- ☰ 8.4.5.3. Compton Edge
- ☰ 8.4.5.4. Escape Peaks
-
- ☰ 8.4.6. Coincidence Measurements
- ☰ 8.4.6.1. Coincidence Detection
- ☰ 8.4.6.2. Timing Windows
- ☰ 8.4.6.3. True Coincidences
- ☰ 8.4.6.4. Random Coincidences
-
-
- ☰ 8.5. Nuclear Reactions
- ☰ 8.5.1. Principles of Nuclear Reactions
- ☰ 8.5.1.1. Reaction Notation
- ☰ 8.5.1.2. Conservation Laws
- ☰ 8.5.1.3. Reaction Energetics
-
- ☰ 8.5.2. Q-Value
- ☰ 8.5.2.1. Exothermic Reactions
- ☰ 8.5.2.2. Endothermic Reactions
- ☰ 8.5.2.3. Reaction Thresholds
-
- ☰ 8.5.3. Reaction Cross Section
- ☰ 8.5.3.1. Cross Section
- ☰ 8.5.3.2. Reaction Probability
- ☰ 8.5.3.3. Energy Dependence
-
- ☰ 8.5.4. Types of Nuclear Reactions
- ☰ 8.5.4.1. Elastic Scattering
- ☰ 8.5.4.2. Inelastic Scattering
- ☰ 8.5.4.3. Capture Reactions
- ☰ 8.5.4.4. Transfer Reactions
- ☰ 8.5.4.5. Charge-Exchange Reactions
-
- ☰ 8.5.5. Compound Nucleus
- ☰ 8.5.5.1. Formation
- ☰ 8.5.5.2. Decay Channels
- ☰ 8.5.5.3. Resonances
-
-
- ☰ 8.6. Nuclear Fission and Fusion
- ☰ 8.6.1. Nuclear Fission
- ☰ 8.6.1.1. Fission Process
- ☰ 8.6.1.2. Fission Fragments
- ☰ 8.6.1.3. Energy Release
- ☰ 8.6.1.4. Neutron Production
-
- ☰ 8.6.2. Chain Reactions
- ☰ 8.6.2.1. Criticality
- ☰ 8.6.2.2. Multiplication Factor
- ☰ 8.6.2.3. Critical Mass
-
- ☰ 8.6.3. Nuclear Reactors
- ☰ 8.6.3.1. Reactor Components
- ☰ 8.6.3.2. Fuel
- ☰ 8.6.3.3. Moderator
- ☰ 8.6.3.4. Control Rods
- ☰ 8.6.3.5. Coolant
-
- ☰ 8.6.4. Nuclear Fusion
- ☰ 8.6.4.1. Fusion Reactions
- ☰ 8.6.4.2. Coulomb Barrier
-
- ☰ 8.6.5. Stellar Fusion
- ☰ 8.6.5.1. Proton-Proton Chain
- ☰ 8.6.5.2. CNO Cycle
- ☰ 8.6.5.3. Nucleosynthesis
-
- ☰ 8.6.6. Controlled Fusion
- ☰ 8.6.6.1. Magnetic Confinement
- ☰ 8.6.6.2. Tokamaks
- ☰ 8.6.6.3. Inertial Confinement
-
-
- ☰ 8.7. Particle Physics Foundations
- ☰ 8.7.1. From Atoms to Elementary Particles
- ☰ 8.7.1.1. Discovery of the Electron
- ☰ 8.7.1.2. Discovery of the Nucleus
- ☰ 8.7.1.3. Discovery of the Neutron
- ☰ 8.7.1.4. Discovery of Antimatter
-
- ☰ 8.7.2. Classification of Particles
- ☰ 8.7.2.1. Elementary Particles
- ☰ 8.7.2.2. Composite Particles
- ☰ 8.7.2.3. Fermions
- ☰ 8.7.2.4. Bosons
-
- ☰ 8.7.3. Antiparticles
- ☰ 8.7.3.1. Matter and Antimatter
- ☰ 8.7.3.2. Pair Production
- ☰ 8.7.3.3. Annihilation
-
- ☰ 8.7.4. Relativistic Particle Kinematics
- ☰ 8.7.4.1. Four-Momentum
- ☰ 8.7.4.2. Invariant Mass
-
- ☰ 8.7.5. Particle Decays
- ☰ 8.7.5.1. Decay Width
- ☰ 8.7.5.2. Lifetime
- ☰ 8.7.5.3. Branching Ratio
- ☰ 8.7.5.4. Conservation Laws
-
-
- ☰ 8.8. Quarks and Hadrons
- ☰ 8.8.1. Quarks
- ☰ 8.8.1.1. Up Quark
- ☰ 8.8.1.2. Down Quark
- ☰ 8.8.1.3. Strange Quark
- ☰ 8.8.1.4. Charm Quark
- ☰ 8.8.1.5. Top Quark
- ☰ 8.8.1.6. Bottom Quark
-
- ☰ 8.8.2. Quark Properties
- ☰ 8.8.2.1. Mass
- ☰ 8.8.2.2. Flavor
- ☰ 8.8.2.3. Color Charge
-
- ☰ 8.8.3. Hadrons
- ☰ 8.8.3.1. Baryons
- ☰ 8.8.3.2. Mesons
-
- ☰ 8.8.4. Baryon Structure
- ☰ 8.8.4.1. Proton Quark Structure
- ☰ 8.8.4.2. Neutron Quark Structure
- ☰ 8.8.4.3. Other Baryons
-
- ☰ 8.8.5. Meson Structure
- ☰ 8.8.5.1. Pions
- ☰ 8.8.5.2. Kaons
- ☰ 8.8.5.3. Heavy Mesons
-
- ☰ 8.8.6. Confinement
- ☰ 8.8.6.1. Color Confinement
- ☰ 8.8.6.2. Hadronization
- ☰ 8.8.6.3. Jets
-
-
- ☰ 8.9. Leptons and Neutrinos
- ☰ 8.9.1. Charged Leptons
- ☰ 8.9.1.1. Electron
- ☰ 8.9.1.2. Muon
- ☰ 8.9.1.3. Tau
-
- ☰ 8.9.2. Neutrinos
- ☰ 8.9.2.1. Electron Neutrino
- ☰ 8.9.2.2. Muon Neutrino
- ☰ 8.9.2.3. Tau Neutrino
-
- ☰ 8.9.3. Neutrino Interactions
- ☰ 8.9.3.1. Weak Interactions
- ☰ 8.9.3.2. Neutrino Detection
-
- ☰ 8.9.4. Neutrino Oscillations
- ☰ 8.9.4.1. Neutrino Flavor
- ☰ 8.9.4.2. Flavor Oscillation
- ☰ 8.9.4.3. Neutrino Mass
-
-
- ☰ 8.10. Fundamental Interactions
- ☰ 8.10.1. Four Fundamental Interactions
- ☰ 8.10.1.1. Electromagnetism
- ☰ 8.10.1.2. Strong Interaction
- ☰ 8.10.1.3. Weak Interaction
-
- ☰ 8.10.2. Exchange Particles
- ☰ 8.10.2.1. Photons
- ☰ 8.10.2.2. Gluons
- ☰ 8.10.2.3. W Bosons
- ☰ 8.10.2.4. Z Boson
-
- ☰ 8.10.3. Electromagnetic Interaction
- ☰ 8.10.3.1. Photon Exchange
-
- ☰ 8.10.4. Strong Interaction
- ☰ 8.10.4.1. Color Charge
- ☰ 8.10.4.2. Gluons
- ☰ 8.10.4.3. Quantum Chromodynamics
-
- ☰ 8.10.5. Weak Interaction
- ☰ 8.10.5.1. Beta Decay
- ☰ 8.10.5.2. W and Z Bosons
- ☰ 8.10.5.3. Flavor-Changing Processes
-
-
- ☰ 8.11. The Standard Model
- ☰ 8.11.1. Overview of the Standard Model
- ☰ 8.11.1.1. Matter Particles
- ☰ 8.11.1.2. Force Carriers
- ☰ 8.11.1.3. Particle Generations
-
- ☰ 8.11.2. Fermions
- ☰ 8.11.2.1. Quarks
- ☰ 8.11.2.2. Leptons
-
- ☰ 8.11.3. Gauge Bosons
- ☰ 8.11.3.1. Photon
- ☰ 8.11.3.2. Gluons
- ☰ 8.11.3.3. W Bosons
- ☰ 8.11.3.4. Z Boson
-
- ☰ 8.11.4. Higgs Field and Higgs Boson
- ☰ 8.11.4.1. Higgs Field
- ☰ 8.11.4.2. Spontaneous Symmetry Breaking
- ☰ 8.11.4.3. Particle Masses
- ☰ 8.11.4.4. Higgs Boson
-
- ☰ 8.11.5. Standard Model Interactions
- ☰ 8.11.5.1. Electroweak Theory
- ☰ 8.11.5.2. Quantum Chromodynamics
-
- ☰ 8.11.6. Limitations of the Standard Model
- ☰ 8.11.6.1. Gravity
- ☰ 8.11.6.2. Dark Matter
- ☰ 8.11.6.3. Neutrino Masses
- ☰ 8.11.6.4. Matter-Antimatter Asymmetry
-
-
- ☰ 8.12. Symmetries and Conservation Laws
- ☰ 8.12.1. Conservation Laws
- ☰ 8.12.1.1. Energy
-
- ☰ 8.12.2. Particle Quantum Numbers
- ☰ 8.12.2.1. Baryon Number
- ☰ 8.12.2.2. Lepton Number
- ☰ 8.12.2.3. Strangeness
- ☰ 8.12.2.4. Charm
- ☰ 8.12.2.5. Isospin
-
- ☰ 8.12.3. Symmetries
- ☰ 8.12.3.1. Charge Conjugation
- ☰ 8.12.3.2. Parity
- ☰ 8.12.3.3. Time Reversal
-
- ☰ 8.12.4. CP Symmetry
- ☰ 8.12.4.1. CP Conservation
- ☰ 8.12.4.2. CP Violation
- ☰ 8.12.4.3. Matter-Antimatter Asymmetry
-
-
- ☰ 8.13. Particle Accelerators
- ☰ 8.13.1. Principles of Acceleration
- ☰ 8.13.1.1. Electric-Field Acceleration
- ☰ 8.13.1.2. Magnetic-Field Steering
-
- ☰ 8.13.2. Linear Accelerators
- ☰ 8.13.2.1. LINACs
- ☰ 8.13.2.2. Radio-Frequency Acceleration
-
- ☰ 8.13.3. Cyclotrons
- ☰ 8.13.3.1. Cyclotron Principle
- ☰ 8.13.3.2. Cyclotron Frequency
- ☰ 8.13.3.3. Limitations
-
- ☰ 8.13.4. Synchrotrons
- ☰ 8.13.4.1. Circular Accelerators
- ☰ 8.13.4.2. Magnetic Focusing
- ☰ 8.13.4.3. RF Cavities
-
- ☰ 8.13.5. Colliders
- ☰ 8.13.5.1. Fixed-Target Experiments
- ☰ 8.13.5.2. Collider Experiments
- ☰ 8.13.5.3. Center-of-Mass Energy
-
- ☰ 8.13.6. Major Particle Accelerators
- ☰ 8.13.6.1. Large Hadron Collider
- ☰ 8.13.6.2. Electron-Positron Colliders
- ☰ 8.13.6.3. Heavy-Ion Colliders
-
-
- ☰ 8.14. Particle Detectors
- ☰ 8.14.1. Principles of Particle Detection
- ☰ 8.14.1.1. Ionization
- ☰ 8.14.1.2. Excitation
- ☰ 8.14.1.3. Energy Deposition
- ☰ 8.14.1.4. Particle Identification
-
- ☰ 8.14.2. Tracking Detectors
- ☰ 8.14.2.1. Cloud Chambers
- ☰ 8.14.2.2. Bubble Chambers
- ☰ 8.14.2.3. Wire Chambers
- ☰ 8.14.2.4. Silicon Trackers
-
- ☰ 8.14.3. Calorimeters
- ☰ 8.14.3.1. Electromagnetic Calorimeters
- ☰ 8.14.3.2. Hadronic Calorimeters
- ☰ 8.14.3.3. Shower Development
-
- ☰ 8.14.4. Cherenkov Detectors
- ☰ 8.14.4.1. Cherenkov Radiation
- ☰ 8.14.4.2. Particle Velocity Measurement
-
- ☰ 8.14.5. Time-of-Flight Detectors
- ☰ 8.14.5.1. Timing Measurements
- ☰ 8.14.5.2. Particle Identification
-
- ☰ 8.14.6. Modern Detector Systems
- ☰ 8.14.6.1. Tracking
- ☰ 8.14.6.2. Muon Systems
- ☰ 8.14.6.3. Trigger Systems
-
-
-
- ☰ 9. Part VIII: Condensed Matter and Applied Physics
- ☰ 9.1. Solid-State Physics
- ☰ 9.1.1. Crystal Structure
- ☰ 9.1.1.1. Crystal Lattices
- ☰ 9.1.1.2. Unit Cells
- ☰ 9.1.1.3. Bravais Lattices
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- ☰ 9.1.2. Electronic Properties
- ☰ 9.1.2.1. Energy Bands
- ☰ 9.1.2.2. Conductors
- ☰ 9.1.2.3. Insulators
- ☰ 9.1.2.4. Semiconductors
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- ☰ 9.1.3. Semiconductor Physics
- ☰ 9.1.3.1. Intrinsic Semiconductors
- ☰ 9.1.3.2. Doping
- ☰ 9.1.3.3. p-Type Materials
- ☰ 9.1.3.4. n-Type Materials
- ☰ 9.1.3.5. p-n Junctions
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- ☰ 9.1.4. Superconductivity
- ☰ 9.1.4.1. Zero Resistance
- ☰ 9.1.4.2. Meissner Effect
- ☰ 9.1.4.3. Critical Temperature
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- ☰ 9.2. Electronics
- ☰ 9.2.1. Semiconductor Diodes
- ☰ 9.2.1.1. p-n Junction
- ☰ 9.2.1.2. Diode Characteristics
- ☰ 9.2.1.3. Rectifiers
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- ☰ 9.2.2. Transistors
- ☰ 9.2.2.1. Bipolar Junction Transistors
- ☰ 9.2.2.2. Field-Effect Transistors
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- ☰ 9.2.3. Operational Amplifiers
- ☰ 9.2.3.1. Ideal Op-Amp
- ☰ 9.2.3.2. Amplifiers
- ☰ 9.2.3.3. Comparators
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- ☰ 9.2.4. Digital Electronics
- ☰ 9.2.4.1. Binary Numbers
- ☰ 9.2.4.2. Logic Gates
- ☰ 9.2.4.3. Boolean Algebra
- ☰ 9.2.4.4. Basic Digital Circuits
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- ☰ 10. Part IX: Astrophysics and Cosmology
- ☰ 10.1. Astrophysics
- ☰ 10.1.1. Measuring the Universe
- ☰ 10.1.1.1. Astronomical Distances
- ☰ 10.1.1.2. Parallax
- ☰ 10.1.1.3. Luminosity
- ☰ 10.1.1.4. Apparent Brightness
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- ☰ 10.1.2. Stars
- ☰ 10.1.2.1. Stellar Spectra
- ☰ 10.1.2.2. Hertzsprung-Russell Diagram
- ☰ 10.1.2.3. Stellar Evolution
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- ☰ 10.1.3. Stellar Remnants
- ☰ 10.1.3.1. White Dwarfs
- ☰ 10.1.3.2. Neutron Stars
- ☰ 10.1.3.3. Black Holes
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- ☰ 10.1.4. Galaxies
- ☰ 10.1.4.1. Structure of Galaxies
- ☰ 10.1.4.2. Milky Way
- ☰ 10.1.4.3. Galaxy Classification
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- ☰ 10.2. Cosmology
- ☰ 10.2.1. Expanding Universe
- ☰ 10.2.1.1. Hubble's Law
- ☰ 10.2.1.2. Cosmological Redshift
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- ☰ 10.2.2. Big Bang Cosmology
- ☰ 10.2.2.1. Early Universe
- ☰ 10.2.2.2. Cosmic Microwave Background
- ☰ 10.2.2.3. Primordial Nucleosynthesis
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- ☰ 10.2.3. Dark Matter
- ☰ 10.2.3.1. Evidence for Dark Matter
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