Calculate Photon Energy

Conversion between frequency and photon energy with E = h·f

Photon Energy Calculator (JavaScript)

Planck relation

Photon energy follows E = h·f with Planck's constant h = 6.62607015·10⁻³⁴ J·s.

Result

Example calculations

Example 1: Visible light

Given: f = 600 THz

\[E=h\cdot f=6.626\cdot10^{-34}\cdot6.00\cdot10^{14}\] \[=3.98\cdot10^{-19}\,J\]

Result: E ≈ 2.48 eV

Example 2: Frequency from 2.48 eV

Given: E = 2.48 eV

\[f=\frac{E}{h}=\frac{2.48\cdot1.602\cdot10^{-19}}{6.626\cdot10^{-34}}\] \[\approx6.00\cdot10^{14}\,Hz\]

Result: f ≈ 600 THz

Example 3: UV range

Given: f = 1 PHz = 1000 THz

\[E=h\cdot f\approx6.626\cdot10^{-19}\,J\approx4.14\,eV\]

Interpretation: Higher frequency means higher photon energy.

Formulas and comprehensive description

Photon energy is a quantized energy value of electromagnetic radiation. The Planck relation links frequency directly to energy. It is fundamental in quantum physics, laser technology, spectroscopy, semiconductor physics, and photovoltaics. Increasing frequency increases the energy per photon linearly.

Photon energy
\[E=h\cdot f\]
Frequency
\[f=\frac{E}{h}\]
Planck constant
\[h=6.62607015\cdot10^{-34}\,J\,s\]
eV conversion
\[1\,eV=1.602176634\cdot10^{-19}\,J\]
Practical relevance
In optics, photon energy is commonly expressed in electronvolts. Red light carries lower photon energy than blue or UV light. These differences determine, for example, which materials absorb or emit radiation.

Comprehensive Description

What is Photon Energy?

A photon is the energy quantum of light and electromagnetic radiation. Each photon possesses a characteristic energy E that depends exclusively on its frequency f. Photon energy is quantized – it can only assume discrete values, not arbitrary intermediate values. This is a fundamental concept in quantum mechanics and explains many optical and electronic phenomena.

The Planck Relation: The Fundamental Formula

The energy of a photon is given by the famous Planck-Einstein relation:

\[E = h \cdot f\]
  • E – Photon energy (in Joules J)
  • h – Planck constant = 6.62607015·10⁻³⁴ J·s (a fundamental constant of nature)
  • f – Frequency of light (in Hertz Hz)

This formula shows: Higher frequency → higher photon energy

Alternative Formulas and Quantities

Since frequency and wavelength are related (c = λ·f), photon energy can also be expressed as:

\[E = \frac{h \cdot c}{\lambda}\]
  • c – Speed of light = 3·10⁸ m/s
  • λ – Wavelength of light

Or using the reduced Planck constant ℏ = h/(2π) ≈ 1.055·10⁻³⁴ J·s:

\[E = \hbar \cdot \omega\]

where ω = 2πf is the angular frequency.

Planck's Constants
Quantity Symbol Value Unit
Planck Constant h 6.62607015·10⁻³⁴ J·s
Reduced Planck Constant 1.05457182·10⁻³⁴ J·s
Elementary Charge e 1.602176634·10⁻¹⁹ C
Speed of Light c 299,792,458 m/s
Unit: Electron Volts (eV)

In optics and atomic physics, photon energy is often expressed in electron volts (eV), rather than joules. This is the energy gained by an electron when accelerated through a potential difference of 1 volt:

\[1\,eV = 1.602176634 \times 10^{-19}\,J\]
  • 1 eV ≈ 1.60·10⁻¹⁹ J
  • Conversion: E_{eV} = E_{J} / (1.602·10⁻¹⁹)
  • Advantage: eV values for photons are often simple decimals (e.g., 2.5 eV instead of 4.0·10⁻¹⁹ J)
Photon Energy in the Electromagnetic Spectrum
Spectral Region Wavelength λ Frequency f Photon Energy E
Radio Waves mm to m MHz to GHz µeV to meV
Microwaves µm to mm GHz to THz meV to µeV
Infrared (IR) 700 nm to 1 mm 300 GHz to 430 THz 1.2 meV to 1.8 eV
Visible Light 380–700 nm 430–790 THz 1.8–3.3 eV
Ultraviolet (UV) 10–380 nm 790 THz to 30 PHz 3.3 eV to 120 eV
X-rays 0.01–10 nm 30 PHz to 30 EHz 120 eV to 120 keV
Gamma Rays < 0.01 nm > 30 EHz > 120 keV
Visible Light – Colors and Energies
Color Wavelength Frequency Energy (eV) Energy (Joules)
Red 650 nm 461 THz 1.91 eV 3.06·10⁻¹⁹ J
Orange 600 nm 500 THz 2.07 eV 3.31·10⁻¹⁹ J
Yellow 570 nm 526 THz 2.18 eV 3.49·10⁻¹⁹ J
Green 530 nm 566 THz 2.34 eV 3.75·10⁻¹⁹ J
Blue 470 nm 638 THz 2.64 eV 4.23·10⁻¹⁹ J
Violet 400 nm 750 THz 3.10 eV 4.97·10⁻¹⁹ J
Practical Applications of Photon Energy
  • Photosynthesis: Plants use photons of specific energies (visible light) to build organic compounds
  • Photovoltaics: Solar cells harness photon energy to excite electrons and generate electricity (band gap energy)
  • Semiconductors: LEDs and diode lasers emit photons with precisely defined energy (band gap)
  • Spectroscopy: Atoms and molecules absorb/emit photons with specific energy (characteristic lines)
  • Medicine: UV radiation has high photon energy → can damage DNA or be used for disinfection
  • Quantum Electronics: The photoelectric effect shows: photon energy must exceed work function
The Photoelectric Effect – An Example

Albert Einstein's explanation of the photoelectric effect proved the photon concept:

\[h \cdot f = \Phi + E_{\mathrm{kin}}\]
  • Φ – Work function of the material (energy to free an electron)
  • Ekin – Kinetic energy of the emitted electron

Conclusion: The photon must have sufficient energy (f > Φ/h) to free an electron. One photon can free at most one electron – not "half-photons."

Quantization and Why It Matters

Classical Wave: Energy can assume all values (continuous) Quantized Photon: Energy can only assume discrete values (E = h·f for specific frequencies)

  • This explains why atoms have discrete spectral lines (only certain transitions allowed)
  • This explains why LEDs emit monochromatic light (only one frequency)
  • This is the key to quantum mechanics
Frequently Asked Questions

Q: Can one photon free multiple electrons?

A: No. One photon can excite at most one electron. Multiple photons are required for multi-photon effects (only at very high intensities).

Q: Can intensity affect photon energy?

A: No. The energy of a single photon depends only on its frequency, not on intensity. Higher intensity means more photons, not more energetic photons.

Q: Why is photon energy often expressed in eV?

A: Because eV is the natural unit for light and electronics. An atom with a band gap of 2 eV absorbs photons with at least 2 eV energy – direct comparability.

Summary
Key Points:
  • Planck Relation: E = h·f links frequency and energy
  • Quantization: Photon energy is discrete, not arbitrarily divisible
  • Color Dependence: Red light has less energy than blue light
  • Practical Importance: Determines absorption, emission, LED colors, solar cells
  • eV Unit: Natural for optics and electronics
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