Absorbance

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Absorbance, also known as optical density, is a measure of the amount of light absorbed by a sample as it passes through a medium. It is a dimensionless quantity and is commonly used in spectroscopy to quantify the concentration of a solute in a solution. Absorbance is defined by the Beer-Lambert law, which relates the absorbance to the concentration of the absorbing species and the path length of the sample.

Principle[edit]

The principle of absorbance is based on the interaction of light with matter. When light passes through a sample, certain wavelengths are absorbed by the molecules in the sample, while others are transmitted. The absorbance (A) is calculated using the formula:

A = -\log_{10}(T)

where T is the transmittance, defined as the ratio of the transmitted light intensity (I) to the incident light intensity (I_0):

T = \frac{I}{I_0}

Beer-Lambert Law[edit]

The Beer-Lambert law states that absorbance is directly proportional to the concentration (c) of the absorbing species, the path length (l) of the sample, and the molar absorptivity (ε), a constant that depends on the nature of the absorbing species and the wavelength of light:

A = \epsilon \cdot c \cdot l

This law is fundamental in quantitative analysis using spectroscopic techniques.

Applications[edit]

Absorbance measurements are widely used in various fields, including:

Instrumentation[edit]

The primary instrument used to measure absorbance is the spectrophotometer. A spectrophotometer consists of a light source, a monochromator to select the desired wavelength, a sample holder, and a detector to measure the intensity of transmitted light. Modern spectrophotometers can measure absorbance across a wide range of wavelengths, from the ultraviolet (UV) to the visible (Vis) and infrared (IR) regions of the electromagnetic spectrum.

Related Concepts[edit]

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