Spectroscopy deals with the interaction of electromagnetic radiation with the sample molecules. The different chemical bonds in a molecule will absorb the radiation at different vibrational and rotational wavelengths. This changes the energy levels of the bonds. Absorbed energy can be subsequently emitted. The absorbtion or emission spectrum can therefore reveal the structure and identity of the sample molecule.
Varieties of Spectroscopy
The frequencies of electromagnetic radiation wavelengths used for food authenticity testing applications are Infra-red (IR, approx. 700 – 4000nm), Near Infra-red (NIR, approx. 780 – 2500nm), UV-Visible (approx. 10 – 700nm). The wavelength range chosen will try to be appropriate to determine certain molecular markers in the sample molecules.
Image by the authors
Reference spectra are taken from authentic samples. If the test sample spectrum deviates (usually following chemometric analysis,) it may indicate either adulteration or substitution.
Infra-Red (IR) Spectroscopy
Infra-red spectra show the vibrational absorptions of different molecular bonds. Different types of bonds, in different positions within the molecular structure, give different characteristic peaks. The entire spectrum therefore gives a “fingerprint” of the molecule.Infra-red spectrometers can be miniaturised and used in-situ for rapid screening and testing
Near Infra-Red (NIR) Spectroscopy
NIR spectroscopy is very similar to IR spectroscopy except that it uses a narrower section of the IR spectrum i.e., 1250-4000cm-1 (800-2500nm). This results in the peaks becoming broader than those in IR spectra, and chemometric analysis is essential. Again, it can be used in-situ there are a variety of commercial hand-held NIR spectrometers.
Fourier-Transform Infra-Red (FT-IR) Spectroscopy
FTIR differs from single beam infra-red spectroscopy in that it relies on interference of various frequencies of light to collect a spectrum. The spectrometer consists of a source, beam splitter, two mirrors, a laser and a detector; the beam splitter and mirrors are collectively called the interferometer.
The IR light from the source strikes the beam splitter, which produces two beams of roughly the same intensity. One beam strikes a fixed mirror and returns, while the second strikes a moving mirror. When the two beams are combined by the beam splitter, this gives the interference infra-red beam.
The combined beam is then passed through the sample, where some energy is absorbed, and some is transmitted. The detector records the subsequent intensity. This signal is and processed using a computer. The untangling of the frequencies into a spectrum is done by the Fourier transform algorithm..
A background single beam spectrum is collected without a sample. The ratio of these two spectra gives the sharp spectrum, which can then permit interpretation of the specific stretching and rotating atomic frequencies.
FTIR Images by LibreTexts Chemistry, Howard University,, licensed under Creative Common Attribution
UV-Visible Spectroscopy
UV-Vis spectroscopy measures the amount of discrete wavelengths of UV or visible light that are absorbed by or transmitted through a sample in comparison to a reference or blank sample. Light energy is inversely proportional to its wavelength; thus, shorter wavelengths of light carry more energy and longer wavelengths carry less energy. Hence although IR spectra involve absorption by the stretching and rotation of atoms in a molecule, UV-Vis absorption involves promotion of electrons in a molecule to a higher energy state. UV-Vis spectrometers normally use light with a range of wavelengths from 150/200nm to 700/750nm, (the visible light range is 380-780nm).
The technique can be used quantitatively by measuring the size of absorption peaks.
Raman Spectroscopy
Raman spectroscopy uses intense monochromatic light from a laser to probe the chemical bonds in a sample, generating a spectrum that acts as a fingerprint, which can be used to characterise or identify the compounds in a sample. A visible light wavelengh is usually chosen for food analysis. The high intensity laser light source shines on the sample, which interacts with molecular vibrations, or other excitations in the system, and causes the inelastic scattering of photons, known as Raman scattering. Three types of scattering are produced
- Stokes Raman scattering, which is the scattered light used in Raman spectroscopy with wavelengths greater than the laser light
- Rayleigh scattering, which is the strongest but with wavelengths equal to the laser, and
- Anti-Stokes scattering, with wavelengths less than the laser.
Stokes Raman scattering is when the molecule gains energy from the photon during the scattering (excited to a higher vibrational level) then the scattered photon loses energy, and its wavelength increases. On the other hand, Anti-Stokes Raman scattering is where the molecule loses energy by relaxing to a lower vibrational level, and the scattered photon gains the corresponding energy and its wavelength decreases. Stokes Raman scattering is always more intense than the anti-Stokes and for this reason, it is nearly always the Stokes Raman scattering that is measured in Raman spectroscopy. Even so, it is still relatively weak, which is why an intense laser light, and an optimised detector are required to give the spectrum.
Fluorescence Spectroscopy
Fluorescence spectroscopy is based on absorption of photons from a visual or UV light source, which excite the molecules in the sample from a ground state to an excited electronic state. When the molecule returns back to its ground state, the resulting energy is emitted as a photon, which causes the molecule to fluoresce. The intensities and frequencies of these photons are detected and analysed to give a spectrum, and this can be used to authenticate the sample. Like other forms of spectroscopy, fluorescence spectroscopy gives quantitative results if there has been a quantitative calibration with authentic standards.