disperses light into a spectrum) and then are registered by a CCD detector array that
has a large number of pixels (>1000) in the spectral axis in order to acquire a
high-resolution Raman spectrum. Commonly used laser wavelengths in Raman
spectroscopy include 532 nm (a green diode-pumped Nd:YAG laser) and 785 nm
(an AlGaAs diode laser), which enable the achievement of a lateral resolution of
better than half the wavelength (i.e., 250–350 nm). This sub-cellular resolution is
similar to that attainable influorescence imaging.
Example 9.9What are some optical sources that can be used for Raman
spectroscopy?
Solution: Some common lasers and their selected emission wavelengths that
are applicable to Raman spectroscopy include the following:
- Ar (488 nm, 514.5 nm)
- Kr (530.9 nm, 647.1 nm)
- He–Ne (623 nm)
- Diode lasers (782 nm, 830 nm)
- Nd:YAG (1064 nm)
A general illustration of a microscope system used for Raman spectroscopy is
shown in Fig.9.15. The main microscope components are the following:
- An excitation light source, for example, a 532-nm or a 785-nm laser
- Various reflecting and light-collecting and focusing optical elements; lens #1
can be a cylindrical lens to illuminate the sample with a slice of light or the lens
can be removed so that only a spot of light falls on the sample - An excitation opticalfilter that passes only the selected spectral band (≈40 nm
wide) needed for absorption by thefluorophore being used - A dichroic mirror that blocks light from the excitation wavelengths and passes to
the detector only the spectral region in which thefluorescent emission occurs - A spectrometer that spreads the wavelengths across the face of a detector, such
as a photodiode array, CCD, or PMT
Laser Sample
Spectrometer CCD
Lens #1
Lens #2
Microscope
objective
Fig. 9.15 Diagram of a Dichroic mirror
microscope system used for
Raman spectroscopy
9.6 Raman Spectroscopy 277