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Glossary

E

Energy Levels

Criticality: 3

Discrete, quantized values of energy that electrons can possess within an atom, rather than a continuous range of energies.

Example:

When an electron in a neon sign jumps between specific energy levels, it emits photons of a characteristic red color.

H

Half-Life

Criticality: 3

The characteristic time it takes for half of the radioactive nuclei in a given sample to undergo radioactive decay.

Example:

If a medical isotope has a half-life of 6 hours, then after 12 hours, only one-quarter of the original sample will remain.

P

Probability Density

Criticality: 3

The square of the absolute value of the wave function (|Ψ|²), which represents the likelihood of finding a particle at a specific location in space.

Example:

A high peak in a probability density plot for an electron in a quantum well indicates a region where the electron is most likely to be found.

R

Radioactive Decay

Criticality: 3

A spontaneous, probabilistic process where an unstable atomic nucleus transforms into a more stable one by emitting particles and energy.

Example:

Carbon-14 undergoes radioactive decay to nitrogen-14, a process used in archaeological dating to determine the age of ancient artifacts.

S

Spectral Lines

Criticality: 3

Distinct lines of light observed in emission or absorption spectra, corresponding to the specific photon energies emitted or absorbed during electron transitions between atomic energy levels.

Example:

Astronomers can identify the chemical composition of distant stars by analyzing the unique pattern of spectral lines in their emitted light.

Spontaneous Emission

Criticality: 2

The process where an electron in an excited atomic state randomly drops to a lower energy level, emitting a photon without any external trigger.

Example:

The glow from a firefly is due to spontaneous emission of light from excited molecules within its body.

Standing Waves

Criticality: 2

Wave patterns that remain in a constant position, formed by the superposition of two waves traveling in opposite directions, used to model electron states in atoms.

Example:

Just like a vibrating guitar string forms standing waves with fixed nodes, electrons in an atom exist in specific orbital patterns that resemble these waves.

Stimulated Absorption

Criticality: 2

The process where an atom in a lower energy state absorbs an incoming photon with precisely the right energy, causing an electron to jump to a higher, excited energy level.

Example:

For a solar cell to work efficiently, its material must exhibit strong stimulated absorption of photons from sunlight.

Stimulated Emission

Criticality: 2

The process where an incoming photon causes an excited atom to emit an identical photon as it transitions to a lower energy state, forming the basis for laser operation.

Example:

Lasers achieve their intense, coherent light by harnessing stimulated emission, where one photon triggers a cascade of identical photons.

W

Wave Function (Ψ)

Criticality: 3

A mathematical description of a quantum particle's state, varying in space and time, which contains all possible information about the particle.

Example:

In a hydrogen atom, the wave function for an electron describes its probability distribution around the nucleus, rather than a fixed orbit.

Wave-Particle Duality

Criticality: 3

The fundamental concept in quantum mechanics that particles can exhibit both wave-like and particle-like properties, depending on how they are observed.

Example:

The famous double-slit experiment beautifully illustrates wave-particle duality, showing electrons behaving as waves when unobserved and as particles when detected.

d

de Broglie Wavelength (λ = h/p)

Criticality: 3

The wavelength associated with a particle, inversely proportional to its momentum (p), demonstrating the wave-like nature of matter.

Example:

A fast-moving electron in an electron microscope has a very short de Broglie wavelength, allowing it to resolve incredibly small structures.