8.5.4.2. Inelastic Scattering
Table of Contents
What Inelastic Scattering Means
Inelastic scattering is a type of nuclear reaction in which an incoming particle collides with a nucleus and leaves again, but the nucleus is not left in the same internal state as before. Some of the kinetic energy of the incoming system is converted into internal energy of the nucleus. As a result, the nucleus becomes excited.
A common symbolic form is
$$
a + X \rightarrow a + X^*
$$
Here, $a$ is the incoming projectile, $X$ is the target nucleus, and $X^*$ means the same nucleus in an excited state. The important point is that the identity of the particles does not change, but the internal energy does.
In elastic scattering, kinetic energy is redistributed between projectile and target, but the total kinetic energy in the center-of-mass frame remains the same. In inelastic scattering, part of that kinetic energy is used to excite the nucleus, so the final kinetic energy is smaller.
In inelastic scattering, the target nucleus changes its energy state, even though its nuclear species remains the same.
$$
a + X \rightarrow a + X^*
$$
The final kinetic energy is less than the initial kinetic energy because energy has gone into nuclear excitation.
Energy Transfer in the Collision
When a projectile strikes a nucleus, conservation of energy still holds. However, some of the initial kinetic energy may be converted into excitation energy $E^*$ of the nucleus. If the nucleus is raised to an excited state, then
$$
E_{\text{initial}} = E_{\text{final}} + E^*
$$
where $E^*$ is the excitation energy.
This means that the scattered particle often emerges with reduced speed. Measuring this energy loss is one of the main ways physicists identify inelastic scattering experimentally.
If the excited nucleus later returns to a lower energy state, it often emits a gamma ray. So inelastic scattering is frequently followed by gamma emission:
$$
a + X \rightarrow a + X^*
$$
followed by
$$
X^* \rightarrow X + \gamma
$$
This gamma ray is evidence that the nucleus was excited during the collision.
Comparison with Elastic Scattering
The difference between elastic and inelastic scattering is easier to see in a direct comparison.
| Feature | Elastic Scattering | Inelastic Scattering |
|---|---|---|
| Nuclear identity | Unchanged | Unchanged |
| Nuclear internal state | Unchanged | Changed, excited |
| Kinetic energy in center-of-mass frame | Conserved | Decreases |
| Excitation energy produced | No | Yes |
| Possible later gamma emission | No | Often yes |
In both processes, the projectile and target can remain the same kinds of particles. The key difference is whether internal excitation occurs.
Do not confuse loss of kinetic energy with loss of total energy. In inelastic scattering, total energy is still conserved. The kinetic energy lost by the particles becomes internal excitation energy of the nucleus.
Excited Nuclear States
Nuclei can exist in discrete energy levels, somewhat like atoms. During inelastic scattering, the nucleus absorbs just enough energy to move into one of its allowed excited states.
If the excitation energy is $E^*$, then the scattered projectile must supply at least that energy, together with any energy needed by momentum conservation. Therefore, not every incoming energy can produce a given excitation. The projectile must have sufficient energy.
After excitation, the nucleus usually does not stay excited for long. It returns to a lower state by emitting radiation, most commonly gamma rays.
A simple picture is
Threshold Behavior
Because excitation requires energy, inelastic scattering often has a threshold. If the projectile energy is too low, the nucleus cannot be excited to the desired state, and only elastic scattering may occur.
Suppose the lowest excited state of a nucleus has energy $E_1$. Then the incoming projectile must have enough kinetic energy for that excitation to occur. In practice, the threshold is influenced not only by the excitation energy itself but also by momentum conservation.
This threshold behavior helps reveal the energy levels of nuclei. By varying the projectile energy and watching when new scattered-particle energies or gamma rays appear, physicists can determine excited nuclear states.
Inelastic scattering can occur only when the projectile has enough energy to excite the nucleus to an allowed state.
Common Projectiles
Many kinds of particles can produce inelastic scattering. Frequently used projectiles include neutrons, protons, alpha particles, and electrons. In nuclear physics, neutron and proton inelastic scattering are especially important.
For example,
$$
n + X \rightarrow n + X^*
$$
or
$$
p + X \rightarrow p + X^*
$$
Neutrons are especially useful because they have no electric charge, so they are not repelled by the positive nucleus by Coulomb forces. Charged particles such as protons must overcome electrical repulsion before reaching the nucleus.
Experimental Signatures
Inelastic scattering is identified by the measurable consequences of nuclear excitation. The main signatures are reduced outgoing kinetic energy and gamma radiation from de-excitation.
If a detector measures the energy of the outgoing projectile, several distinct groups may appear. One group can correspond to elastic scattering, where little or no energy is lost to excitation. Other groups can correspond to different excited states of the nucleus.
For example, if the projectile emerges with energy lower by $E^$, that suggests the nucleus absorbed excitation energy $E^$. If a gamma ray of the same energy is later detected, that provides strong confirmation.
A simplified energy-level picture is
Why Inelastic Scattering Is Important
Inelastic scattering is a powerful tool for studying nuclear structure. Because nuclei have specific excited states, observing which excitations occur tells us about the allowed energy levels and properties of the nucleus.
By measuring scattering angles, outgoing energies, and emitted gamma rays, physicists can learn about nuclear shapes, collective motion, and internal arrangements of nucleons. The method acts like a probe of the nucleus.
Inelastic scattering is therefore not just a reaction type, it is also an experimental technique for exploring how nuclei are built.
Simple Summary
In inelastic scattering, the projectile collides with a nucleus and leaves as the same kind of particle, but the nucleus is excited. Some kinetic energy is converted into internal nuclear energy. The reaction is commonly written as
$$
a + X \rightarrow a + X^*
$$
and the excited nucleus often later emits a gamma ray:
$$
X^* \rightarrow X + \gamma
$$
This process differs from elastic scattering because the nucleus changes its internal state. Studying inelastic scattering helps reveal nuclear energy levels and nuclear structure.
Views: 0
Where to Move
Move chapter:
- ☰ 1. Mathematical Foundations of Physics
- ☰ 1.1. Physical Quantities and Units
- ☰ 1.1.1. Physical Quantities
- ☰ 1.1.2. SI Base Units
- ☰ 1.1.3. Derived Units
- ☰ 1.1.4. Unit Conversions
- ☰ 1.1.5. Scientific Notation
- ☰ 1.1.6. Orders of Magnitude
- ☰ 1.1.7. Dimensional Analysis
- ☰ 1.1.8. Significant Figures
- ☰ 1.1.9. Measurement Uncertainty
-
- ☰ 1.2. Scalars and Vectors
- ☰ 1.2.1. Scalars and Vectors
- ☰ 1.2.2. Vector Notation
- ☰ 1.2.3. Vector Addition and Subtraction
- ☰ 1.2.4. Vector Components
- ☰ 1.2.5. Unit Vectors
- ☰ 1.2.6. Dot Product
- ☰ 1.2.7. Cross Product
- ☰ 1.2.8. Applications of Vectors in Physics
-
- ☰ 1.3. Coordinate Systems
- ☰ 1.3.1. Cartesian Coordinates
- ☰ 1.3.2. Polar Coordinates
- ☰ 1.3.3. Cylindrical Coordinates
- ☰ 1.3.4. Spherical Coordinates
- ☰ 1.3.5. Coordinate Transformations
-
- ☰ 1.4. Calculus for Physics
- ☰ 1.4.1. Functions and Graphs
- ☰ 1.4.2. Derivatives
- ☰ 1.4.3. Physical Meaning of Derivatives
- ☰ 1.4.4. Partial Derivatives
- ☰ 1.4.5. Integrals
- ☰ 1.4.6. Physical Meaning of Integrals
- ☰ 1.4.7. Differential Equations
- ☰ 1.4.8. Taylor Series and Approximations
-
-
- ☰ 2. Part I: Classical Mechanics
- ☰ 2.1. Kinematics
- ☰ 2.1.1. Motion in One Dimension
- ☰ 2.1.1.1. Position
- ☰ 2.1.1.2. Distance and Displacement
- ☰ 2.1.1.3. Speed and Velocity
- ☰ 2.1.1.4. Average Velocity
- ☰ 2.1.1.5. Instantaneous Velocity
- ☰ 2.1.1.6. Acceleration
-
- ☰ 2.1.2. Motion with Constant Acceleration
- ☰ 2.1.2.1. Kinematic Equations
- ☰ 2.1.2.2. Free Fall
- ☰ 2.1.2.3. Vertical Motion
- ☰ 2.1.2.4. Position-Time Graphs
- ☰ 2.1.2.5. Velocity-Time Graphs
- ☰ 2.1.2.6. Acceleration-Time Graphs
-
- ☰ 2.1.3. Motion in Two and Three Dimensions
- ☰ 2.1.3.1. Position Vectors
- ☰ 2.1.3.2. Velocity Vectors
- ☰ 2.1.3.3. Acceleration Vectors
- ☰ 2.1.3.4. Relative Motion
-
- ☰ 2.1.4. Projectile Motion
- ☰ 2.1.4.1. Horizontal Projection
- ☰ 2.1.4.2. Oblique Projection
- ☰ 2.1.4.3. Maximum Height
- ☰ 2.1.4.4. Time of Flight
- ☰ 2.1.4.5. Projectile Range
- ☰ 2.1.4.6. Trajectory Equation
-
- ☰ 2.1.5. Circular Motion
- ☰ 2.1.5.1. Angular Position
- ☰ 2.1.5.2. Angular Velocity
- ☰ 2.1.5.3. Angular Acceleration
- ☰ 2.1.5.4. Uniform Circular Motion
- ☰ 2.1.5.5. Centripetal Acceleration
-
-
- ☰ 2.2. Newton's Laws of Motion
- ☰ 2.2.1. Force
- ☰ 2.2.1.1. Concept of Force
- ☰ 2.2.1.2. Fundamental Forces
- ☰ 2.2.1.3. Contact Forces
- ☰ 2.2.1.4. Free-Body Diagrams
-
- ☰ 2.2.2. Newton's First Law
- ☰ 2.2.2.1. Inertia
- ☰ 2.2.2.2. Inertial Reference Frames
- ☰ 2.2.2.3. Equilibrium
-
- ☰ 2.2.3. Newton's Second Law
- ☰ 2.2.3.1. Force, Mass, and Acceleration
- ☰ 2.2.3.2. Net Force
- ☰ 2.2.3.3. Applications of F = ma
-
- ☰ 2.2.4. Newton's Third Law
- ☰ 2.2.4.1. Action-Reaction Pairs
- ☰ 2.2.4.2. Interaction Forces
-
- ☰ 2.2.5. Common Forces
- ☰ 2.2.5.1. Weight
- ☰ 2.2.5.2. Normal Force
- ☰ 2.2.5.3. Tension
- ☰ 2.2.5.4. Spring Force
- ☰ 2.2.5.5. Static Friction
- ☰ 2.2.5.6. Kinetic Friction
- ☰ 2.2.5.7. Drag Force
-
- ☰ 2.2.6. Applications of Newton's Laws
- ☰ 2.2.6.1. Connected Objects
- ☰ 2.2.6.2. Pulley Systems
- ☰ 2.2.6.3. Inclined Planes
- ☰ 2.2.6.4. Elevators
- ☰ 2.2.6.5. Circular Motion
-
-
- ☰ 2.3. Work and Energy
- ☰ 2.3.1. Work
- ☰ 2.3.1.1. Work Done by a Constant Force
- ☰ 2.3.1.2. Work Done by a Variable Force
- ☰ 2.3.1.3. Work from Force-Position Graphs
-
- ☰ 2.3.2. Kinetic Energy
- ☰ 2.3.2.1. Translational Kinetic Energy
- ☰ 2.3.2.2. Work-Energy Theorem
-
- ☰ 2.3.3. Potential Energy
- ☰ 2.3.3.1. Gravitational Potential Energy
- ☰ 2.3.3.2. Elastic Potential Energy
- ☰ 2.3.3.3. Potential-Energy Curves
-
- ☰ 2.3.4. Conservation of Energy
- ☰ 2.3.4.1. Mechanical Energy
- ☰ 2.3.4.2. Conservative Forces
- ☰ 2.3.4.3. Non-Conservative Forces
- ☰ 2.3.4.4. Conservation of Mechanical Energy
- ☰ 2.3.4.5. Energy Dissipation
-
- ☰ 2.3.5. Power
- ☰ 2.3.5.1. Average Power
- ☰ 2.3.5.2. Instantaneous Power
- ☰ 2.3.5.3. Efficiency
-
-
- ☰ 2.4. Momentum and Collisions
- ☰ 2.4.1. Linear Momentum
- ☰ 2.4.1.1. Momentum
- ☰ 2.4.1.2. Momentum and Force
-
- ☰ 2.4.2. Impulse
- ☰ 2.4.2.1. Impulse
- ☰ 2.4.2.2. Impulse-Momentum Theorem
- ☰ 2.4.2.3. Force-Time Graphs
-
- ☰ 2.4.3. Conservation of Momentum
- ☰ 2.4.3.1. Isolated Systems
- ☰ 2.4.3.2. Center-of-Mass Motion
-
- ☰ 2.4.4. Collisions
- ☰ 2.4.4.1. Elastic Collisions
- ☰ 2.4.4.2. Inelastic Collisions
- ☰ 2.4.4.3. Perfectly Inelastic Collisions
- ☰ 2.4.4.4. One-Dimensional Collisions
- ☰ 2.4.4.5. Two-Dimensional Collisions
-
- ☰ 2.4.5. Center of Mass
- ☰ 2.4.5.1. Center of Mass of Particles
- ☰ 2.4.5.2. Center of Mass of Continuous Objects
-
- ☰ 2.4.6. Rocket Motion
- ☰ 2.4.6.1. Variable-Mass Systems
- ☰ 2.4.6.2. Rocket Equation
-
-
- ☰ 2.5. Rotational Motion
- ☰ 2.5.1. Rotational Kinematics
- ☰ 2.5.1.1. Angular Displacement
- ☰ 2.5.1.2. Angular Velocity
- ☰ 2.5.1.3. Angular Acceleration
-
- ☰ 2.5.2. Torque
- ☰ 2.5.2.1. Torque
- ☰ 2.5.2.2. Lever Arm
- ☰ 2.5.2.3. Vector Definition of Torque
-
- ☰ 2.5.3. Moment of Inertia
- ☰ 2.5.3.1. Rotational Inertia
- ☰ 2.5.3.2. Common Moments of Inertia
- ☰ 2.5.3.3. Parallel-Axis Theorem
-
- ☰ 2.5.4. Rotational Dynamics
- ☰ 2.5.4.1. Newton's Second Law for Rotation
- ☰ 2.5.4.2. Rotational Kinetic Energy
- ☰ 2.5.4.3. Work and Power in Rotation
-
- ☰ 2.5.5. Angular Momentum
- ☰ 2.5.5.1. Angular Momentum
- ☰ 2.5.5.2. Conservation of Angular Momentum
-
- ☰ 2.5.6. Rolling Motion
- ☰ 2.5.6.1. Rolling Without Slipping
- ☰ 2.5.6.2. Translational and Rotational Energy
-
- ☰ 2.5.7. Static Equilibrium
- ☰ 2.5.7.1. Conditions for Equilibrium
- ☰ 2.5.7.2. Center of Gravity
- ☰ 2.5.7.3. Stability
-
-
- ☰ 2.6. Gravitation
- ☰ 2.6.1. Newton's Law of Gravitation
- ☰ 2.6.1.1. Universal Gravitation
- ☰ 2.6.1.2. Gravitational Constant
- ☰ 2.6.1.3. Superposition
-
- ☰ 2.6.2. Gravitational Field
- ☰ 2.6.2.1. Gravitational Field Strength
- ☰ 2.6.2.2. Field of Spherical Bodies
-
- ☰ 2.6.3. Gravitational Potential
- ☰ 2.6.3.1. Gravitational Potential Energy
- ☰ 2.6.3.2. Gravitational Potential
-
- ☰ 2.6.4. Planetary Motion
- ☰ 2.6.4.1. Kepler's Laws
- ☰ 2.6.4.2. Circular Orbits
- ☰ 2.6.4.3. Orbital Velocity
- ☰ 2.6.4.4. Orbital Period
-
- ☰ 2.6.5. Satellites and Spaceflight
- ☰ 2.6.5.1. Geostationary Satellites
- ☰ 2.6.5.2. Escape Velocity
- ☰ 2.6.5.3. Orbital Energy
-
-
-
- ☰ 3. Part II: Oscillations, Waves, and Fluids
- ☰ 3.1. Oscillations
- ☰ 3.1.1. Simple Harmonic Motion
- ☰ 3.1.1.1. Periodic Motion
- ☰ 3.1.1.2. Amplitude
- ☰ 3.1.1.3. Frequency and Period
- ☰ 3.1.1.4. Angular Frequency
- ☰ 3.1.1.5. SHM Equation
-
- ☰ 3.1.2. Mass-Spring Systems
- ☰ 3.1.2.1. Hooke's Law
- ☰ 3.1.2.2. Spring Oscillations
- ☰ 3.1.2.3. Energy in SHM
-
- ☰ 3.1.3. Pendulums
- ☰ 3.1.3.1. Simple Pendulum
- ☰ 3.1.3.2. Physical Pendulum
-
- ☰ 3.1.4. Damped Oscillations
- ☰ 3.1.4.1. Damping
- ☰ 3.1.4.2. Critical Damping
-
- ☰ 3.1.5. Forced Oscillations and Resonance
- ☰ 3.1.5.1. Driving Force
- ☰ 3.1.5.2. Resonance
- ☰ 3.1.5.3. Natural Frequency
-
-
- ☰ 3.2. Mechanical Waves
- ☰ 3.2.1. Fundamentals of Waves
- ☰ 3.2.1.1. Transverse Waves
- ☰ 3.2.1.2. Longitudinal Waves
- ☰ 3.2.1.3. Wavelength
- ☰ 3.2.1.4. Frequency
- ☰ 3.2.1.5. Wave Speed
- ☰ 3.2.1.6. Amplitude
-
- ☰ 3.2.2. Mathematical Description of Waves
- ☰ 3.2.2.1. Wave Function
- ☰ 3.2.2.2. Phase
- ☰ 3.2.2.3. Wave Equation
-
- ☰ 3.2.3. Superposition
- ☰ 3.2.3.1. Interference
- ☰ 3.2.3.2. Constructive Interference
- ☰ 3.2.3.3. Destructive Interference
-
- ☰ 3.2.4. Standing Waves
- ☰ 3.2.4.1. Nodes and Antinodes
- ☰ 3.2.4.2. Strings
- ☰ 3.2.4.3. Pipes
- ☰ 3.2.4.4. Harmonics
-
- ☰ 3.2.5. Sound Waves
- ☰ 3.2.5.1. Speed of Sound
- ☰ 3.2.5.2. Sound Intensity
- ☰ 3.2.5.3. Decibels
- ☰ 3.2.5.4. Beats
- ☰ 3.2.5.5. Doppler Effect
-
-
- ☰ 3.3. Fluid Mechanics
- ☰ 3.3.1. Properties of Fluids
- ☰ 3.3.1.1. Density
- ☰ 3.3.1.2. Pressure
- ☰ 3.3.1.3. Compressibility
-
- ☰ 3.3.2. Fluid Statics
- ☰ 3.3.2.1. Hydrostatic Pressure
- ☰ 3.3.2.2. Pascal's Principle
-
- ☰ 3.3.3. Buoyancy
- ☰ 3.3.3.1. Archimedes' Principle
- ☰ 3.3.3.2. Floating and Sinking
-
- ☰ 3.3.4. Fluid Dynamics
- ☰ 3.3.4.1. Flow Rate
- ☰ 3.3.4.2. Continuity Equation
- ☰ 3.3.4.3. Bernoulli's Equation
-
- ☰ 3.3.5. Viscosity
- ☰ 3.3.5.1. Laminar Flow
- ☰ 3.3.5.2. Turbulent Flow
- ☰ 3.3.5.3. Poiseuille's Law
- ☰ 3.3.5.4. Reynolds Number
-
-
-
- ☰ 4. Part III: Thermodynamics
- ☰ 4.1. Temperature and Heat
- ☰ 4.1.1. Temperature and Thermal Equilibrium
- ☰ 4.1.2. Zeroth Law of Thermodynamics
- ☰ 4.1.3. Temperature Scales
- ☰ 4.1.4. Thermal Expansion
- ☰ 4.1.5. Heat and Internal Energy
- ☰ 4.1.6. Specific Heat Capacity
- ☰ 4.1.7. Calorimetry
- ☰ 4.1.8. Phase Changes
- ☰ 4.1.9. Latent Heat
- ☰ 4.1.10. Heat Transfer
-
- ☰ 4.2. Kinetic Theory of Gases
- ☰ 4.2.1. Ideal Gas Law
- ☰ 4.2.2. Molecular Interpretation of Pressure
- ☰ 4.2.3. Temperature and Molecular Kinetic Energy
- ☰ 4.2.4. RMS Molecular Speed
- ☰ 4.2.5. Maxwell-Boltzmann Distribution
- ☰ 4.2.6. Mean Free Path
-
- ☰ 4.3. Thermodynamics
- ☰ 4.3.1. Thermodynamic Systems
- ☰ 4.3.2. First Law of Thermodynamics
- ☰ 4.3.3. Isothermal Processes
- ☰ 4.3.4. Isobaric Processes
- ☰ 4.3.5. Isochoric Processes
- ☰ 4.3.6. Adiabatic Processes
- ☰ 4.3.7. Heat Engines
- ☰ 4.3.8. Carnot Cycle
- ☰ 4.3.9. Refrigerators
- ☰ 4.3.10. Second Law of Thermodynamics
- ☰ 4.3.11. Entropy
- ☰ 4.3.12. Reversible and Irreversible Processes
-
-
- ☰ 5. Part IV: Electricity and Magnetism
- ☰ 5.1. Electric Charge and Electric Field
- ☰ 5.1.1. Electric Charge
- ☰ 5.1.2. Conductors and Insulators
- ☰ 5.1.3. Coulomb's Law
- ☰ 5.1.4. Superposition
- ☰ 5.1.5. Electric Field
- ☰ 5.1.6. Electric Field Lines
- ☰ 5.1.7. Electric Dipoles
- ☰ 5.1.8. Electric Flux
- ☰ 5.1.9. Gauss's Law
-
- ☰ 5.2. Electric Potential
- ☰ 5.2.1. Electric Potential Energy
- ☰ 5.2.2. Electric Potential
- ☰ 5.2.3. Equipotential Surfaces
- ☰ 5.2.4. Relationship Between Potential and Field
- ☰ 5.2.5. Potential of Continuous Charge Distributions
-
- ☰ 5.3. Capacitance
- ☰ 5.3.1. Capacitors
- ☰ 5.3.2. Parallel-Plate Capacitor
- ☰ 5.3.3. Series and Parallel Capacitors
- ☰ 5.3.4. Energy Stored in Capacitors
- ☰ 5.3.5. Dielectrics
- ☰ 5.3.6. Polarization
-
- ☰ 5.4. Electric Current and Resistance
- ☰ 5.4.1. Electric Current
- ☰ 5.4.2. Current Density
- ☰ 5.4.3. Drift Velocity
- ☰ 5.4.4. Resistance
- ☰ 5.4.5. Ohm's Law
- ☰ 5.4.6. Resistivity
- ☰ 5.4.7. Electrical Energy
- ☰ 5.4.8. Electric Power
- ☰ 5.4.9. Electromotive Force
-
- ☰ 5.5. DC Circuits
- ☰ 5.5.1. Kirchhoff's Laws
- ☰ 5.5.2. Multi-Loop Circuits
- ☰ 5.5.3. RC Circuits
- ☰ 5.5.4. Measuring Instruments
-
- ☰ 5.6. Magnetism
- ☰ 5.6.1. Magnetic Fields
- ☰ 5.6.2. Lorentz Force
- ☰ 5.6.3. Motion of Charged Particles
- ☰ 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
-
- ☰ 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
-
- ☰ 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
-
- ☰ 9.1.4. Superconductivity
- ☰ 9.1.4.1. Zero Resistance
- ☰ 9.1.4.2. Meissner Effect
- ☰ 9.1.4.3. Critical Temperature
-
-
- ☰ 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
-
- ☰ 9.2.2. Transistors
- ☰ 9.2.2.1. Bipolar Junction Transistors
- ☰ 9.2.2.2. Field-Effect Transistors
-
- ☰ 9.2.3. Operational Amplifiers
- ☰ 9.2.3.1. Ideal Op-Amp
- ☰ 9.2.3.2. Amplifiers
- ☰ 9.2.3.3. Comparators
-
- ☰ 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
-
-
-
- ☰ 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
-
- ☰ 10.1.2. Stars
- ☰ 10.1.2.1. Stellar Spectra
- ☰ 10.1.2.2. Hertzsprung-Russell Diagram
- ☰ 10.1.2.3. Stellar Evolution
-
- ☰ 10.1.3. Stellar Remnants
- ☰ 10.1.3.1. White Dwarfs
- ☰ 10.1.3.2. Neutron Stars
- ☰ 10.1.3.3. Black Holes
-
- ☰ 10.1.4. Galaxies
- ☰ 10.1.4.1. Structure of Galaxies
- ☰ 10.1.4.2. Milky Way
- ☰ 10.1.4.3. Galaxy Classification
-
-
- ☰ 10.2. Cosmology
- ☰ 10.2.1. Expanding Universe
- ☰ 10.2.1.1. Hubble's Law
- ☰ 10.2.1.2. Cosmological Redshift
-
- ☰ 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
-
- ☰ 10.2.3. Dark Matter
- ☰ 10.2.3.1. Evidence for Dark Matter
-
-
-