# UV-Vis Spectrophotometer

Avantes AvaSpec UV-Vis System [SOP]
Wavelength range: 200-1100 nm

Resolution: 0.06-20 nm

Stray light: 0.19-1.0%

Sensitivity: 375,000 (counts/µW/ms integration time)

The UV-Vis (ultraviolet-visible) spectrophotometer is a machine that can measure many optical properties of a sample. These properties include transmittance, absorption, and reflectance of light. The spectroscope is able to analyze both solid and liquid specimens. The machine runs through the AvaSoft 8 software.

## Principle

Components of a typical UV-Vis spectrometer.

A beam of light from a visible and/or UV light source (colored red) is separated into its component wavelengths by a prism or diffraction grating [1]. Each monochromatic (single wavelength) beam in turn is split into two equal intensity beams by a half-mirrored device. One beam, the sample beam (colored magenta), passes through a small transparent container (cuvette) containing a solution of the compound being studied in a transparent solvent. The other beam, the reference (colored blue), passes through an identical cuvette containing only the solvent. The intensities of these light beams are then measured by electronic detectors and compared. The intensity of the reference beam, which should have suffered little or no light absorption, is defined as $\displaystyle{ I_0 }$. The intensity of the sample beam is defined as $\displaystyle{ I }$. Over a short period of time, the spectrometer automatically scans all the component wavelengths in the manner described. The ultraviolet (UV) region scanned is normally from 200 to 400 nm, and the visible portion is from 400 to 800 nm. PMMA, PS, or glass cuvettes are used when the primary wavelengths of interest are in the visible range and quartz cuvettes are used when those wavelengths are between 170 and 300 nm, because they are more transparent to these wavelengths.

Typical UV-Vis absorption plot

## Absorption and Transmittance

If the sample compound does not absorb light of a given wavelength, $\displaystyle{ I_0 = I. }$ However, if the sample compound absorbs light then $\displaystyle{ I \lt I_0 }$, and this difference may be plotted on a graph versus wavelength. Absorption may be presented as transmittance $\displaystyle{ (T = I/I_0) }$ or absorbance $\displaystyle{ (A= log \frac{I_0}{I}) }$. If no absorption has occurred, T = 1.0 and A= 0. Most spectrometers display absorbance on the vertical axis, and the commonly observed range is from 0 (100% transmittance) to 2 (1% transmittance). The wavelength of maximum absorbance is a characteristic value, designated as $\displaystyle{ \lambda_{max} }$.

Different compounds may have very different absorption maxima and absorbances. Intensely absorbing compounds must be examined in dilute solution, so that significant light energy is received by the detector, and this requires the use of completely transparent (non-absorbing) solvents. The most commonly used solvents are water, ethanol, hexane and cyclohexane. Solvents having double or triple bonds, or heavy atoms (e.g. S, Br & I) are generally avoided. Because the absorbance of a sample will be proportional to its molar concentration in the sample cuvette, a corrected absorption value known as the molar absorptivity is used when comparing the spectra of different compounds. Molar Absorptivity $\displaystyle{ (\epsilon) }$ is defined by: $\displaystyle{ \epsilon = \frac{A}{cl} }$, where $\displaystyle{ A }$ = absorbance, $\displaystyle{ c }$ = sample concentration in moles/liter & $\displaystyle{ l }$ = length of light path through the cuvette in cm (1cm for the MILL's UV-Vis) .