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Quantum physics

Showing 1–30 of 63 reference entries

Physics · MeasurementSpeed of light in vacuum

c denotes the speed of light in vacuum. Its numerical value is fixed exactly in SI units.

Definition
Physics · MeasurementPlanck constant

h denotes the Planck constant. Its numerical value is fixed exactly in SI units.

Definition
PhysicsPhoton energy and frequency

One photon's energy is proportional to its frequency.

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Physics · Mathematics & logicInvariant spacetime interval

Lorentz transformations preserve a combined space-time separation.

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PhysicsSchrödinger time evolution

A quantum wavefunction evolves according to its Hamiltonian.

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PhysicsBorn position probability

A normalized wavefunction assigns probabilities to position intervals.

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PhysicsQuantum observable expectations

A state and observable determine the mean of repeated outcomes.

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PhysicsRobertson uncertainty relation

A commutator constrains two outcome spreads in the same state.

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PhysicsSpin one-half and Pauli operators

A spin one-half state has two outcomes along a chosen axis.

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Physics · InformationPure and mixed density operators

A density operator represents quantum statistical states.

Definition
PhysicsIdeal projective measurement

Projectors determine outcome probabilities and conditional states.

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Physics · InformationComposite states and entanglement

A joint pure state can fail to factor into subsystem states.

Definition
PhysicsExchange symmetry of identical particles

Boson and fermion states respond differently to exchange.

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PhysicsHydrogen Coulomb energy levels

The ideal one-electron atom has discrete bound energies.

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Physics · ChemistryAtomic state labels and Pauli occupancy

Quantum labels specify orbitals and spin states.

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PhysicsScattering cross section

Normalize a scattering rate by incident flux.

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PhysicsHamiltonian and unitary quantum evolution

A closed quantum system evolves by iħ d|ψ⟩/dt=H(t)|ψ⟩.

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PhysicsStationary states and spectral superposition

For a time-independent Hamiltonian, an energy eigenstate evolves by a phase exp(−iEt/ħ).

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PhysicsInfinite one-dimensional potential well

With zero potential inside 0<x<L and impenetrable walls, normalized eigenfunctions are √(2/L) sin(nπx/L) and energies are n²π²ħ²/(2mL²), n=1,2,… .

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PhysicsProbability flux and rectangular-barrier tunnelling

A real one-dimensional potential conserves probability current.

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PhysicsQuantum harmonic-oscillator spectrum

For H=p²/(2m)+mω²x²/2 on the real line, normalizable states have E_n=ħω(n+½), n=0,1,… .

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Physics · ChemistryOscillator creation and annihilation operators

For the canonical oscillator, a=√(mω/(2ħ))x+ip/√(2mħω) and its adjoint satisfy [a,a†]=1.

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PhysicsHeisenberg evolution and conserved observables

The Heisenberg observable A_H=U†A_SU obeys dA_H/dt=(i/ħ)[H_H,A_H]+(∂A_S/∂t)_H.

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PhysicsAngular-momentum algebra and ladder spectrum

Quantum angular momentum obeys [J_i,J_j]=iħ ε_ijk J_k.

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PhysicsAddition of quantum angular momenta

Independent commuting angular momenta combine as J=J₁+J₂.

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PhysicsNondegenerate stationary perturbation

For an isolated nondegenerate eigenvalue of H₀ and a small Hermitian perturbation V, the leading energy corrections are ⟨n|V|n⟩ and Σ_{k≠n}|⟨k|V|n⟩|²/(E_n⁰−E_k⁰).

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PhysicsDegenerate stationary perturbation

Inside a degenerate eigenspace of H₀, first-order energy shifts and appropriate zeroth-order states come from diagonalizing the projected Hermitian perturbation PVP.

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PhysicsWeak time-dependent transition amplitudes

Starting in eigenstate i of fixed H₀, a weak perturbation V(t) gives first-order amplitude c_f(t)=−(i/ħ)∫_{t₀}^t V_fi(t′)exp[i(E_f−E_i)(t′−t₀)/ħ]dt′ for f≠i.

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Physics · ChemistryElectric-dipole transition selection rules

In the long-wavelength electric-dipole approximation, atomic transition strength depends on the dipole matrix element.

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Physics · ChemistryVariational ground-energy bound

For a self-adjoint Hamiltonian bounded below, every normalized trial state with a finite energy expectation satisfies ⟨ψ_trial|H|ψ_trial⟩≥E₀.

Mathematical statement