Luminous efficacy is a measure of how efficiently a light source produces visible light. It is the ratio of luminous flux to power, measured in lumens per watt in the International System of Units (SI). Depending on context, the power can be either the radiant flux of the source's output, or it can be the total power (electric power, chemical energy, or others) consumed by the source. Which sense of the term is intended must usually be inferred from the context, and is sometimes unclear. The former sense is sometimes called luminous efficacy of radiation, and the latter luminous efficacy of a light source or overall luminous efficacy.

Not all wavelengths of light are equally visible, or equally effective at stimulating human vision, due to the spectral sensitivity of the human eye; radiation in the infrared and ultraviolet parts of the spectrum is useless for illumination. The luminous efficacy of a source is the product of how well it converts energy to electromagnetic radiation, and how well the emitted radiation is detected by the human eye.

Efficacy and efficiency

Luminous efficacy can be normalized by the maximum possible luminous efficacy to a dimensionless quantity called luminous efficiency. The distinction between efficacy and efficiency is not always carefully maintained in published sources, so it is not uncommon to see "efficiencies" expressed in lumens per watt, or "efficacies" expressed as a percentage.

Luminous efficacy of radiation

By definition, light outside the visible spectrum cannot be seen by the standard human vision system, and therefore does not contribute to, and indeed can subtract from, luminous efficacy.

Explanation

The typical response of human vision to light under daytime or bright conditions, as standardized by the CIE in 1924. The horizontal axis is wavelength in nanometers.

Luminous efficacy of radiation measures the fraction of electromagnetic power which is useful for lighting. It is obtained by dividing the luminous flux by the radiant flux. Light wavelengths outside the visible spectrum reduce luminous efficacy, because they contribute to the radiant flux, while the luminous flux of such light is zero. Wavelengths near the peak of the eye's response contribute more strongly than those near the edges.

Wavelengths of light outside of the visible spectrum are not useful for general illumination. Furthermore, human vision responds more to some wavelengths of light than others. This response of the eye is represented by the luminous efficiency function. This is a standardized function representing photopic vision, which models the response of the eye's cone cells, that are active under typical daylight conditions. A separate curve can be defined for dark/night conditions, modeling the response of rod cells without cones, known as scotopic vision. (Mesopic vision describes the transition zone in dim conditions, between photopic and scotopic, where both cones and rods are active.)

Photopic luminous efficacy of radiation has a maximum possible value of 683.002 lm/W, for the case of monochromatic light at a wavelength of 555 nm . Scotopic luminous efficacy of radiation reaches a maximum of 1700 lm/W for monochromatic light at a wavelength of 507 nm.

Mathematical definition

Luminous efficacy (of radiation), denoted K, is defined as

K = Φ v Φ e = ∫ 0 ∞ K ( λ ) Φ e , λ d λ ∫ 0 ∞ Φ e , λ d λ , {\displaystyle K={\frac {\Phi _{\mathrm {v} }}{\Phi _{\mathrm {e} }}}={\frac {\int _{0}^{\infty }K(\lambda )\Phi _{\mathrm {e} ,\lambda }\,\mathrm {d} \lambda }{\int _{0}^{\infty }\Phi _{\mathrm {e} ,\lambda }\,\mathrm {d} \lambda }},}

where

Examples

Photopic vision

TypeLuminous efficacy of radiation (lm/W)Luminous efficiency
Tungsten light bulb, typical, 2800 K152%
Class M star (Antares, Betelgeuse), 3300K304%
Black body, 4000 K, ideal54.78%
Class G star (Sun, Capella), 5800K9313.6%
Black-body, 7000 K, ideal9514%
Black-body, 5800 K, truncated to 400–700 nm (ideal "white" source)25137%
Black-body, 5800 K, truncated to ≥ 2% photopic sensitivity range29243%
Black-body, 2800 K, truncated to ≥ 2% photopic sensitivity range29944%
Black-body, 2800 K, truncated to ≥ 5% photopic sensitivity range34350%
Black-body, 5800 K, truncated to ≥ 5% photopic sensitivity range34851%
Monochromatic source at 540 THz683 (exact)99.9997%
Ideal monochromatic source: 555 nm (in air)683.002100%

Scotopic vision

TypeLuminous efficacy of radiation (lm/W)Luminous efficiency
Ideal monochromatic 507 nm source1699 or 1700100%
Spectral radiance of a black body. Wavelengths outside the visible light band (~380–750nm, bounded within grey dotted lines) have very low luminous efficiency.

Lighting efficiency

Artificial light sources are usually evaluated in terms of luminous efficacy of the source, also sometimes called wall-plug efficacy. This is the ratio between the total luminous flux emitted by a device and the total amount of input power (electrical, etc.) it consumes. The luminous efficacy of the source is a measure of the efficiency of the device with the output adjusted to account for the spectral response curve (the luminosity function). When expressed in dimensionless form (for example, as a fraction of the maximum possible luminous efficacy), this value may be called luminous efficiency of a source, overall luminous efficiency or lighting efficiency.

The main difference between the luminous efficacy of radiation and the luminous efficacy of a source is that the latter accounts for input energy that is lost as heat or otherwise exits the source as something other than electromagnetic radiation. Luminous efficacy of radiation is a property of the radiation emitted by a source. Luminous efficacy of a source is a property of the source as a whole.

Examples

The following table lists luminous efficacy of a source and efficiency for various light sources. Note that all lamps requiring electrical/electronic ballast are unless noted (see also voltage) listed without losses for that, reducing total efficiency.

CategoryTypeOverall luminous efficacy (lm/W)Overall luminous efficiency
CombustionGas mantle1–20.15–0.3%
Incandescent15, 40, 100W tungsten incandescent (230 V)8.0, 10.4, 13.81.2, 1.5, 2.0%
5, 40, 100W tungsten incandescent (120 V)5.0, 12.6, 17.50.7, 1.8, 2.6%
Halogen incandescent100, 200, 500W tungsten halogen (230 V)16.7, 17.6, 19.82.4, 2.6, 2.9%
2.6W tungsten halogen (5.2 V)19.22.8%
Halogen-IR (120 V)17.7–24.52.6–3.5%
Tungsten quartz halogen (12–24 V)243.5%
Photographic and projection lamps355.1%
Light-emitting diodeLED screw base lamp (120 V)10214.9%
5–16W LED screw base lamp (230 V)75–21711–32%
21.5W LED retrofit for T8 fluorescent tube (230V)17225%
Theoretical limit for a white LED with phosphorescence color mixing260–30038.1–43.9%
Red LED 660nm83%
Arc lampCarbon arc lamp2–70.29–1.0%
Xenon arc lamp30–904.4–13.5%
Mercury-xenon arc lamp50–557.3–8%
Ultra-high-pressure (UHP) mercury-vapor arc lamp, free mounted58–788.5–11.4%
Ultra-high-pressure (UHP) mercury-vapor arc lamp, with reflector for projectors30–504.4–7.3%
Fluorescent32W T12 tube with magnetic ballast609%
9–32W compact fluorescent (with ballast)46–758–11.45%
T8 tube with electronic ballast80–10012–15%
PL-S 11W U-tube, excluding ballast loss8212%
T5 tube70–104.210–15.63%
70–150W inductively-coupled electrodeless lighting system71–8410–12%
Gas discharge1400W sulfur lamp10015%
Metal-halide lamp65–1159.5–17%
High-pressure sodium lamp85–15012–22%
Low-pressure sodium lamp100–20015–29%
Plasma display panel2–100.3–1.5%
CathodoluminescenceElectron-stimulated luminescence30–11015%
Ideal sourcesTruncated 5800 K black-body25137%
Green light at 555 nm (maximum possible luminous efficacy by definition)683.002100%

Sources that depend on thermal emission from a solid filament, such as incandescent light bulbs, tend to have low overall efficacy because, as explained by Donald L. Klipstein, "An ideal thermal radiator produces visible light most efficiently at temperatures around 6300 °C (6600 K or 11,500 °F). Even at this high temperature, a lot of the radiation is either infrared or ultraviolet, and the theoretical luminous [efficacy] is 95 lumens per watt. No substance is solid and usable as a light bulb filament at temperatures anywhere close to this. The surface of the sun is not quite that hot." At temperatures where the tungsten filament of an ordinary light bulb remains solid (below 3683 kelvin), most of its emission is in the infrared.

SI photometry units

SI photometry quantitiesvte
QuantityUnitDimensionNotes
NameSymbolNameSymbol
Luminous energyQvlumen secondlm⋅sTJThe lumen second is sometimes called the talbot.
Luminous flux, luminous powerΦvlumen (= candela steradian)lm (= cd⋅sr)JLuminous energy per unit time
Luminous intensityIvcandela (= lumen per steradian)cd (= lm/sr)JLuminous flux per unit solid angle
LuminanceLvcandela per square metrecd/m2 (= lm/(sr⋅m2))L−2⋅JLuminous flux per unit solid angle per unit projected source area. The candela per square metre is sometimes called the nit.
IlluminanceEvlux (= lumen per square metre)lx (= lm/m2)L−2⋅JLuminous flux incident on a surface
Luminous exitance, luminous emittanceMvlumen per square metrelm/m2L−2⋅JLuminous flux emitted from a surface
Luminous exposureHvlux secondlx⋅sL−2⋅TJTime-integrated illuminance
Luminous energy densityωvlumen second per cubic metrelm⋅s/m3L−3⋅TJ
Luminous efficacy (of radiation)Klumen per wattlm/WM−1⋅L−2⋅T3⋅JRatio of luminous flux to radiant flux
Luminous efficacy (of a source)ηlumen per wattlm/WM−1⋅L−2⋅T3⋅JRatio of luminous flux to power consumption
Luminous efficiency, luminous coefficientV1Luminous efficacy normalized by the maximum possible efficacy
See also: SIPhotometryRadiometry

See also

Notes

External links

  • Hyperphysics has these that do not quite comply with the standard definition