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Glossary

B

Binding Energy (Work Function)

Criticality: 2

The minimum amount of energy required to remove an electron from the surface of a particular metal in the photoelectric effect.

Example:

For an electron to be ejected from a metal, the incoming photon must have energy greater than the metal's binding energy, also known as its work function.

Blackbody

Criticality: 2

An idealized physical body that absorbs all incident electromagnetic radiation, regardless of frequency or angle of incidence, and emits thermal radiation perfectly.

Example:

A theoretical blackbody would absorb all light hitting it, appearing perfectly black, and then emit radiation based solely on its temperature, like a glowing hot piece of metal.

D

Dalton Model

Criticality: 1

An early atomic model proposing that atoms are indivisible, indestructible spheres of a given element, and that atoms of different elements have different masses.

Example:

John Dalton's model helped explain why elements combine in fixed ratios, like how hydrogen and oxygen always form water in a specific proportion, treating each atom as a distinct, indivisible sphere.

E

Electron Orbitals

Criticality: 2

Regions around the nucleus where there is a high probability of finding an electron, described by quantum mechanics rather than fixed paths.

Example:

Instead of electrons orbiting like planets, quantum mechanics describes their probable locations within specific three-dimensional shapes called electron orbitals.

Energy (E)

Criticality: 3

The capacity to do work or produce heat, in the context of light, it refers to the energy carried by photons.

Example:

Ultraviolet light carries more energy per photon than visible light, which is why it can cause sunburn.

F

Frequency (ν)

Criticality: 2

The number of wave cycles that pass a fixed point per unit of time, typically measured in Hertz (Hz) or s^-1.

Example:

A high-pitched sound has a high frequency, meaning more sound waves pass your ear per second.

K

Kinetic Energy (KE)

Criticality: 2

The energy an object possesses due to its motion, specifically referring to the energy of ejected electrons in the photoelectric effect.

Example:

In the photoelectric effect, if a photon has more energy than the binding energy, the excess energy is converted into the kinetic energy of the ejected electron.

N

Nucleus

Criticality: 3

The dense, positively charged center of an atom, containing protons and neutrons, which was discovered by Rutherford's experiment.

Example:

The atom's mass is primarily concentrated in its tiny nucleus, which is why alpha particles were occasionally repelled directly backward during the gold foil experiment.

P

Photoelectric Effect

Criticality: 3

The phenomenon where electrons are ejected from a metal surface when light of a sufficiently high frequency shines on it, demonstrating the particle nature of light.

Example:

Solar panels work because of the photoelectric effect, where photons from sunlight strike a material and knock electrons loose, generating an electric current.

Photons

Criticality: 3

Discrete packets or quanta of light energy, proposed by Einstein to explain the photoelectric effect, demonstrating that light behaves as both a wave and a particle.

Example:

When you see light, you are observing streams of tiny energy packets called photons interacting with your eyes.

Planck's Constant (h)

Criticality: 3

A fundamental physical constant that relates the energy of a photon to its frequency, with a value of approximately 6.626 x 10^-34 Js.

Example:

To calculate the energy of a single photon, you multiply its frequency by Planck's constant, a tiny but crucial number in quantum mechanics.

Planck's Equation (E = hν)

Criticality: 3

An equation stating that the energy (E) of a photon is directly proportional to its frequency (ν), with Planck's constant (h) as the proportionality constant.

Example:

Using Planck's equation, we can determine that a photon of blue light, with its higher frequency, carries more energy than a photon of red light.

Q

Quanta

Criticality: 3

Discrete packets or bundles of energy, as proposed by Max Planck, meaning energy is not continuous but comes in specific, quantized amounts.

Example:

Planck revolutionized physics by suggesting that light energy is not continuous but comes in tiny, indivisible packets called quanta.

R

Rutherford's Gold Foil Experiment

Criticality: 3

A landmark experiment where alpha particles were shot at a thin gold foil, leading to the discovery that atoms are mostly empty space with a tiny, dense, positively charged nucleus.

Example:

The surprising deflection of some alpha particles in Rutherford's gold foil experiment indicated that the atom's positive charge and most of its mass were concentrated in a very small central region.

S

Speed of Light Equation (c = λν)

Criticality: 3

An equation relating the speed of light (c) to its wavelength (λ) and frequency (ν), showing that wavelength and frequency are inversely proportional.

Example:

Using the speed of light equation, we can calculate that radio waves, with their very long wavelengths, must have very low frequencies.

T

Thomson's Plum Pudding Model

Criticality: 1

An atomic model suggesting that an atom is a sphere of uniformly distributed positive charge with negatively charged electrons embedded within it, like raisins in a pudding.

Example:

Before Rutherford, scientists imagined the atom as a diffuse positive cloud with electrons scattered throughout, much like the plum pudding model where the 'plums' are electrons in a positive 'pudding'.

Threshold Frequency

Criticality: 3

The minimum frequency of light required to cause the photoelectric effect, below which no electrons will be ejected, regardless of light intensity.

Example:

Even very bright red light won't cause the photoelectric effect in some metals because its frequency is below the threshold frequency required to eject electrons.

U

Ultraviolet Catastrophe

Criticality: 2

A major discrepancy between classical physics predictions and experimental observations of blackbody radiation, where classical theory predicted infinite energy emission at high frequencies.

Example:

Classical physics failed to explain why hot objects don't emit infinite amounts of high-frequency light, a problem famously known as the ultraviolet catastrophe.

W

Wave-Particle Duality

Criticality: 2

The concept that light and matter exhibit properties of both waves and particles, depending on the experimental conditions.

Example:

The wave-particle duality of light means it can diffract around obstacles like a wave, but also knock electrons off a surface like a particle.

Wavelength (λ)

Criticality: 2

The distance between successive crests or troughs of a wave, typically measured in meters or nanometers.

Example:

Visible light ranges from violet, with a short wavelength, to red, with a long wavelength.