Quantum Physics Formula Reference

Explore the fundamental equations that govern the quantum realm. From Schrödinger's equation to quantum entanglement, master the mathematics of the subatomic world.

Quantum Fundamentals

The building blocks of quantum mechanics

Planck-Einstein Relation

E = hν = ħω
The fundamental relationship between energy and frequency in quantum mechanics. It demonstrates that energy is quantized in discrete packets called quanta.
E = Energy Energy of the photon in Joules (J) h = Planck's constant 6.626 × 10⁻³⁴ J⋅s ν = Frequency Frequency in Hertz (Hz) ħ = Reduced Planck constant h/2π = 1.055 × 10⁻³⁴ J⋅s ω = Angular frequency 2πν in rad/s
Formula Importance 100%

De Broglie Wavelength

λ = h/p = h/(mv)
All matter exhibits wave-like behavior, with wavelength inversely proportional to momentum. This fundamental concept bridges particle and wave nature of matter.
λ = Wavelength h = Planck's constant p = Momentum m = Mass v = Velocity

Heisenberg Uncertainty Principle

Δx ⋅ Δp ≥ ħ/2
The fundamental limit to the precision with which certain pairs of physical properties can be known simultaneously.
Δx = Position uncertainty Δp = Momentum uncertainty ħ = Reduced Planck constant

Photoelectric Effect

Kmax = hν - φ
The kinetic energy of emitted electrons depends on the frequency of incident light, not its intensity. This provided crucial evidence for the quantum nature of light.
Kmax = Maximum kinetic energy h = Planck's constant ν = Light frequency φ = Work function

Wave Mechanics

Mathematical framework of quantum waves

Schrödinger Equation (Time-dependent)

iħ ∂Ψ/∂t = ĤΨ
The fundamental equation of quantum mechanics describing how the quantum state of a physical system changes with time.
i = Imaginary unit ħ = Reduced Planck constant Ψ = Wave function Ĥ = Hamiltonian operator

Schrödinger Equation (Time-independent)

ĤΨ = EΨ
Describes the stationary states of a quantum system, where energy eigenvalues are constant in time.
Ĥ = Hamiltonian operator Ψ = Energy eigenfunction E = Energy eigenvalue

Hamiltonian Operator

Ĥ = -ħ²/2m ∇² + V(x,t)
Represents the total energy of the system, including kinetic and potential energy.
-ħ²/2m ∇² = Kinetic energy operator V(x,t) = Potential energy ∇² = Laplacian operator

Probability Density

ρ = |Ψ(x,t)|² = Ψ*Ψ
The probability of finding a particle at position x at time t.
ρ = Probability density Ψ* = Complex conjugate of Ψ Ψ = Wave function

Normalization Condition

∫ |Ψ(x,t)|² dx = 1
The wave function must be normalized to ensure total probability equals 1.
∫ = Integral over all space |Ψ|² = Probability density

Momentum Operator

p̂ = -iħ∇
The quantum mechanical operator corresponding to classical momentum.
p̂ = Momentum operator ∇ = Gradient operator i = Imaginary unit

Quantum Operators

Mathematical tools for quantum observables

Interactive Operator Visualization

Position (x) ψ(x)

Visualization of a quantum wave function and its probability density

Position Operator

x̂ψ(x) = xψ(x)
In position space, the position operator acts by multiplication with the position coordinate.

Angular Momentum Operator

L̂ = r̂ × p̂ = -iħ(r × ∇)
The cross product of position and momentum operators.

Energy Operator

Ê = iħ ∂/∂t
The operator corresponding to the total energy of the system.

Laplacian Operator

∇² = ∂²/∂x² + ∂²/∂y² + ∂²/∂z²
The differential operator representing the sum of second partial derivatives.

Quantum Applications

Real-world quantum phenomena and applications

Hydrogen Atom Energy Levels

En = -13.6 eV / n²
The energy levels of electron in hydrogen atom, derived from Bohr model.
n = Principal quantum number E = Energy in electron volts

Particle in a Box

En = n²h²/(8mL²)
Energy levels for a particle confined in a 1D box of length L.
n = Quantum number (1,2,3,...) m = Mass of particle L = Length of box

Quantum Tunneling

T ≈ e^(-2κL)
Transmission probability for quantum tunneling through a barrier.
T = Transmission probability κ = Decay constant L = Barrier width

Bell's Inequality

|S| ≤ 2 (Classical) |S| = 2√2 (Quantum)
Distinguishes between quantum and classical predictions for entangled particles.

Fermi-Dirac Distribution

f(E) = 1/[e^(E-EF)/kT + 1]
Probability distribution for fermions at thermal equilibrium.
EF = Fermi energy k = Boltzmann constant T = Temperature

Bose-Einstein Distribution

f(E) = 1/[e^(E-μ)/kT - 1]
Probability distribution for bosons at thermal equilibrium.
μ = Chemical potential k = Boltzmann constant T = Temperature

Interactive Calculators

Apply quantum formulas with real-time calculations

De Broglie Wavelength Calculator

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Energy-Frequency Calculator

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Uncertainty Principle Calculator

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Quantum Physics Timeline

The evolution of quantum mechanics

1900

Max Planck

Introduces quantized energy levels and Planck's constant

1905

Albert Einstein

Explains photoelectric effect, introduces photon concept

1924

Louis de Broglie

Proposes wave-particle duality for matter

1926

Erwin Schrödinger

Develops wave equation for quantum mechanics

1927

Werner Heisenberg

Formulates uncertainty principle

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