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Vocabulary practice flashcards covering classical mechanics limitations, black body radiation, Planck's quantum theory, the photoelectric effect, Compton scattering, de Broglie matter waves, Heisenberg's uncertainty principle, and Schrödinger's wave mechanics.
Inorganic chemistry
The branch of chemistry that deals with the synthesis and behaviors of inorganic and organometallic compounds.
Classical mechanics
The branch of physics obeyed by macroscopic particles such as planets and rigid bodies, in which the state of a system is defined by specifying all forces acting and all positions and velocities.
Thermal spectrum
The spectrum obtained when the radiated energy emitted from a heated body is passed through a prism.
Black body
An ideal body that completely absorbs radiant energy of all wavelengths, neither reflecting nor transmitting any radiation, thus possessing an absorbance of unity.
Fery's black body
A hollow, double-walled metallic sphere coated inside with lamp black, featuring a narrow opening on one side and a conical projection directly opposite the opening to avoid direct reflection.
Quanta (or photons)
Small packets, bundles, or pulses of energy in which radiant energy is discontinuously emitted or absorbed by a body.
Planck's radiation law
The principle stating that hot bodies, atoms, or molecules emit or absorb radiant energy discontinuously in discrete units called quanta, each having energy E=hν.
Planck's constant (h)
The physical constant relating the energy of a quantum to its radiation frequency, with a value of 6.625×10−27erg sec.
Photoelectric effect
The phenomenon in which electrons are ejected from the surface of a metal when a beam of light of suitable wavelength or frequency falls upon it.
Threshold frequency (cut-off frequency)
The critical or limiting minimum frequency of incident radiation below which no photoelectric effect occurs.
Work function (w)
The portion of an incident photon's energy used to separate and eject an electron from the metal surface, equal to hν0.
Compton effect
The change in radiation frequency or increase in wavelength of high-energy X-rays when they scatter after an elastic collision with an electron.
Compton recoil electron
The electron ejected from a material after acquiring kinetic energy during an elastic collision with an incident X-ray photon.
Wave-particle duality
The principle that radiation and microscopic matter, such as electrons, atoms, and molecules, exhibit both particle and wave characteristics under appropriate conditions.
de Broglie relationship
The expression stating that the momentum (mc or mv) of a moving particle is inversely proportional to the wavelength of its associated wave: λ=mch.
Heisenberg uncertainty principle
The fundamental quantum principle stating that it is impossible to determine simultaneously both the exact position and momentum of an electron with arbitrary accuracy (Δp⋅Δx≥4πh).
Orbit
In Bohr's model, a definite, fixed circular path around the nucleus along which an electron moves with a definite energy and velocity.
Orbital
A three-dimensional space around the nucleus where there is a maximum probability (90–95%) of finding an electron.
Schrödinger wave equation
A differential equation describing subatomic particles and atomic behavior in terms of probability in three-dimensional space around the nucleus.
Wave function (ψ)
The mathematical function describing the state of a quantum system; to be physically acceptable, it must be finite, single-valued, and continuous.
Laplacian operator (∇2)
A differential operator defined in Cartesian coordinates as ∇2=∂x2∂2+∂y2∂2+∂z2∂2.
Hamiltonian operator (H^)
The total energy operator in quantum mechanics used in the eigenvalue form of the Schrödinger wave equation: H^ψ=Eψ.
Eigenvalues
The definite values of total energy (E) for which the Schrödinger wave equation yields physically meaningful and acceptable solutions.
Probability density (ψ2)
A real, non-negative quantity obtained by multiplying ψ by its complex conjugate (ψ∗), representing the probability of finding an electron in three-dimensional space around the nucleus.
Rayleigh-Jeans law
A radiation law stating that the emissive power of a black body at absolute temperature T is directly proportional to T and inversely proportional to the wavelength raised to the fourth power (λ4).
Ultraviolet catastrophe
The breakdown of the Rayleigh-Jeans law at higher radiation frequencies, where it erroneously predicted that the total power radiated by a black body per unit area would be infinite.