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  1. AP Physics 2 Revised
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Glossary

B

Backscattering

Criticality: 2

A specific case of scattering where the scattered particle (e.g., photon) reverses its direction, resulting in the maximum possible change in wavelength.

Example:

When a photon undergoes backscattering (a 180° scattering angle), it transfers the maximum possible energy to the electron.

C

Compton Scattering

Criticality: 3

A phenomenon where a photon collides with a charged particle, typically an electron, resulting in a decrease in the photon's energy (increase in wavelength) and a change in its direction.

Example:

When an X-ray photon interacts with an electron in a material, it undergoes Compton Scattering, losing some energy and deflecting from its original path.

Compton Scattering Equation

Criticality: 3

A formula that quantifies the change in wavelength of a photon after Compton scattering, relating it to Planck's constant, electron mass, speed of light, and the scattering angle.

Example:

Using the Compton Scattering Equation, scientists can precisely predict the wavelength shift of X-rays after they interact with electrons in a material.

Conservation Laws

Criticality: 3

Fundamental principles in physics stating that certain quantities, such as energy and momentum, remain constant in a closed system before and after an interaction.

Example:

The conservation laws of energy and momentum are essential for analyzing collisions in physics, from car crashes to subatomic particle interactions.

E

Electrons

Criticality: 2

Fundamental subatomic particles with a negative electric charge, often involved in interactions with photons.

Example:

In a cathode ray tube, a beam of electrons is accelerated to create an image on the screen.

Energy and Momentum Transfer

Criticality: 3

The process by which energy and momentum are exchanged between interacting particles, such as a photon and an electron during a collision.

Example:

During a game of pool, the cue ball's energy and momentum transfer to the object ball, causing it to move.

F

Frequency

Criticality: 2

The number of complete wave cycles that pass a point per unit of time, inversely related to wavelength for electromagnetic waves.

Example:

As a photon's wavelength increases due to Compton scattering, its frequency decreases, indicating a loss of energy.

M

Mass of the Electron (m_e)

Criticality: 2

The intrinsic mass of an electron, a constant value used in calculations involving electron interactions.

Example:

The mass of the electron is a crucial value in the denominator of the Compton scattering equation, influencing the magnitude of the wavelength shift.

P

Particle-like Behavior

Criticality: 3

The characteristic of light (or other waves) to exhibit properties typically associated with particles, such as discrete energy packets and momentum.

Example:

The photoelectric effect and Compton scattering are key experiments demonstrating the particle-like behavior of light.

Photons

Criticality: 3

Discrete packets or quanta of light energy, demonstrating the particle-like nature of light.

Example:

A laser pointer emits millions of photons every second, each carrying a specific amount of energy.

Planck's Constant (h)

Criticality: 2

A fundamental physical constant that relates the energy of a photon to its frequency, central to quantum mechanics.

Example:

The energy of a single photon of blue light can be calculated by multiplying its frequency by Planck's Constant.

S

Scattering Angle

Criticality: 3

The angle at which a scattered particle (e.g., a photon) deviates from its original direction after a collision.

Example:

A larger scattering angle in Compton scattering indicates that the photon transferred more energy to the electron.

Speed of Light (c)

Criticality: 2

The constant speed at which all electromagnetic waves, including light, travel in a vacuum.

Example:

The speed of light is the ultimate speed limit in the universe, approximately 3 x 10^8 meters per second.

W

Wavelength Change (Δλ)

Criticality: 3

The difference between the initial and final wavelengths of a photon after undergoing Compton scattering.

Example:

A positive wavelength change indicates that the scattered photon has a longer wavelength and thus less energy than the incident photon.