$$E = \frac{hc}{\lambda}= h\nu$$
$h = 6.626\times10^{-34}$ J·s
$c = 2.998\times10^8$ m/s
Photon Flux:
$$\Phi_p = \frac{P \cdot \lambda}{h c A}$$
Molar Photon Rate:
$$n_p = \frac{P \cdot \lambda}{h c N_A}$$
Instantly compute photon energy, flux, irradiance, and photochemical reaction rate from wavelength, source power, beam area, and quantum yield. Covers the full UV–IR spectrum.
$$E = \frac{hc}{\lambda}= h\nu$$
$h = 6.626\times10^{-34}$ J·s
$c = 2.998\times10^8$ m/s
Photon Flux:
$$\Phi_p = \frac{P \cdot \lambda}{h c A}$$
Molar Photon Rate:
$$n_p = \frac{P \cdot \lambda}{h c N_A}$$
The fundamental relationship between a photon's energy (E) and its wavelength (λ) or frequency (ν) is given by Planck's equation. This tells us that shorter wavelengths (bluer light) correspond to higher energy photons.
$$E = \frac{hc}{\lambda}= h\nu$$$E$ = Photon energy (Joules). $h$ = Planck's constant ($6.626 \times 10^{-34}$ J·s). $c$ = Speed of light ($2.998 \times 10^8$ m/s). $\lambda$ = Wavelength (m). $\nu$ = Frequency (Hz).
To find out how many of these photons are delivered by a light source, we calculate the photon flux (Φₚ). This is the number of photons per second per unit area, derived from the total optical power (P) spread over an area (A).
$$\Phi_p = \frac{P \cdot \lambda}{h c A}$$$\Phi_p$ = Photon flux (photons·s⁻¹·m⁻²). $P$ = Total radiant power (Watts). $A$ = Illuminated area (m²). The product $\Phi_p \times A$ gives the total photons per second.
Solar Cell Design: Engineers use these calculations to predict the maximum possible current a solar cell can generate. By knowing the photon flux from the sun at different wavelengths and the material's quantum yield (here called external quantum efficiency), they can model and optimize cell efficiency before fabrication.
Photochemical Reactors: In industrial chemistry driven by light, such as water purification or pharmaceutical synthesis, the reaction rate is directly proportional to the absorbed photon flux. Precise calculation of photon delivery ensures the process is efficient, scalable, and cost-effective.
Biological & Medical Sensing: Techniques like fluorescence microscopy or photodynamic therapy rely on molecules absorbing a specific number of photons to emit light or produce a therapeutic effect. Calculating the local photon flux is critical for determining dosage and imaging sensitivity.
Optical Communications: In fiber optics, data is sent as pulses of light. The number of photons per pulse determines the signal strength and the likelihood of error at the receiver. These calculations are fundamental for designing low-power, high-bandwidth communication systems.
There are a few key points I want you to be especially mindful of when starting to use this tool. First, "the source output power P is not necessarily the total energy reaching the irradiated surface." For example, even if an LED datasheet states "radiant flux 1W," there are losses in the lens or optical system, as well as reflection losses due to the angle of incidence on the surface. In practice, you need to estimate this "optical efficiency" and correct the P value you input into the tool. For instance, if the optical system's transmittance is 80%, you should calculate using an effective P of 0.8W.
Next is the point that "the photon flux is not uniform." The tool gives you a value averaged over the irradiated area A, but an actual laser beam has a Gaussian distribution, and LED light isn't uniform either. To precisely estimate reaction rates, you need to consider the flux distribution across the area. It's entirely possible for the reaction rate at the center to be ten times different from that at the edges.
Finally, a super important fact: "quantum efficiency is wavelength-dependent." While you set a single value in the tool, the actual quantum efficiency of a photocatalyst or solar cell can vary greatly with wavelength. It's common to have 50% at 450nm blue light but only 10% at 650nm red light. Therefore, the "reaction rate calculated for this wavelength" is strictly for that monochromatic light. When using broad-spectrum sunlight, you need to integrate the calculation results for each wavelength.
UV-A photocatalytic reactor: wavelength = 365 nm, optical power = 50 W, illuminated area = 80 cm². Photon energy E = 3.27 eV (1.97 × 10⁻¹⁹ J). Photon flux ≈ 9.2 × 10¹⁷ photons/s. Irradiance = 625 mW/cm². With quantum yield 0.15 (15% of photons drive reaction), effective reaction rate constant increases ~60–90% versus non-photochemical pathway.