Calculate photoelectric threshold frequency, work function, photon energy, kinetic energy of ejected electrons, and stopping voltage using Einstein's photoelectric equation.
The threshold frequency is the minimum frequency of light needed to eject electrons from a material's surface — the foundation of the photoelectric effect that earned Einstein his Nobel Prize. Below this frequency, no electrons are emitted regardless of light intensity. Above it, ejected electrons carry kinetic energy equal to the photon energy minus the material's work function. The Threshold Frequency Calculator performs all photoelectric effect computations.
Einstein's photoelectric equation, E = hf = φ + KE_max, connects photon energy (hf) to the work function (φ) and maximum kinetic energy of ejected photoelectrons. The work function is a material property — metals like cesium have low work functions (~2.1 eV) making them sensitive to visible light, while platinum requires ultraviolet light (~5.6 eV).
This calculator is essential for physics students, researchers working with photodetectors and solar cells, and anyone studying quantum mechanics. Enter any known values to solve for the unknowns: threshold frequency, work function, kinetic energy, stopping voltage, wavelength, or photon energy.
Use this calculator when you need to move between work function, threshold frequency, stopping voltage, and photon energy without re-deriving the photoelectric equation each time. It is useful for quantum-physics problems, detector discussions, and quick material comparisons when you are checking how a material responds to different wavelengths. It also keeps the unit conversions from becoming the whole problem.
E_photon = hf = hc/λ. Threshold frequency: f₀ = φ/h. Max kinetic energy: KE_max = hf - φ. Stopping voltage: V₀ = KE_max/e. Where h = 6.626 × 10⁻³⁴ J·s, c = 3 × 10⁸ m/s, e = 1.602 × 10⁻¹⁹ C.
Result: KE_max = 1.03 eV, Stopping Voltage = 1.03 V
Sodium (φ = 2.28 eV) has threshold frequency 5.51 × 10¹⁴ Hz. Light at 8 × 10¹⁴ Hz (UV) ejects electrons with maximum KE of 1.03 eV. A stopping voltage of 1.03 V would halt all photoelectrons.
The photoelectric effect was first observed by Heinrich Hertz in 1887, but it couldn't be explained by classical physics. Maxwell's wave theory predicted that any frequency of light, given enough intensity, should eject electrons. Instead, experiment showed a sharp cutoff frequency below which no emission occurred, regardless of intensity.
Einstein's 1905 explanation — that light consists of discrete energy quanta (photons) with E = hf — resolved the paradox and launched quantum physics. He received the 1921 Nobel Prize for this work, not for relativity as commonly assumed.
The work function arises from the energy barrier at a material's surface. In metals, electrons exist in a "Fermi sea" of delocalized states. The work function is the energy difference between the Fermi level and the vacuum level (free space). Surface conditions, crystal orientation, adsorbed molecules, and temperature all affect the effective work function.
Semiconductor work functions are more complex, depending on doping, band bending, and surface states. This complexity is exploited in device design — controlling work function alignment between materials is crucial for transistors, LEDs, and solar cells.
Photocathodes in photomultiplier tubes use multi-alkali materials (Na-K-Sb-Cs) with work functions tailored for specific wavelength ranges. CCD and CMOS image sensors use silicon (φ ≈ 4.6 eV for pure Si) with doping and surface treatments to optimize quantum efficiency. X-ray photoelectron spectroscopy (XPS) uses high-energy photons to probe core electron binding energies, providing elemental and chemical state analysis of surfaces with nm-scale depth resolution.
The work function (φ) is the minimum energy needed to remove an electron from a material's surface. It's a material property measured in electron volts (eV). Alkali metals have low work functions (1.9-2.5 eV); noble metals are higher (4.5-5.6 eV).
This was the key quantum insight. Light comes in discrete packets (photons), each with energy E = hf. Below threshold, each photon has insufficient energy to overcome the work function — and electrons can't accumulate energy from multiple photons in normal conditions.
Stopping voltage (V₀) is the minimum reverse voltage needed to stop all photoelectrons. V₀ = KE_max/e. It's measured experimentally by applying increasing reverse voltage until photocurrent drops to zero.
Cesium (~2.1 eV, f₀ ≈ 5.1 × 10¹⁴ Hz) and potassium (~2.3 eV) have the lowest work functions among metals, responding to visible red/orange light. This makes them ideal for photocathodes and photomultiplier tubes.
Photodetectors, solar cells, photomultiplier tubes, night vision devices, and CCD/CMOS camera sensors all rely on the photoelectric effect. It's also the basis for photoelectron spectroscopy (XPS/UPS) used in surface science.
1 eV = 1.602 × 10⁻¹⁹ J. The electron volt is convenient for atomic-scale energies because it matches the energy an electron gains crossing a 1V potential. Photon energies of visible light are 1.7-3.1 eV.