Title: Spectroscopy
1Spectroscopy
2Interaction Types
- When light interacts with an object, we can
normally see only reflected or transmitted
radiation. Three phenomena that occur when
electromagnetic radiation interacts with matter
can be defined more precisely as
3Scattering
- When electromagnetic radiation passes through
matter, most of the radiation continues in its
original direction but a small fraction is
scattered in other directions. - Light that is scattered at the same wavelength as
the incoming light is called Rayleigh scattering.
- Light that is scattered in transparent solids due
to vibrations (phonons) is called Brillouin
scattering. Brillouin scattering is typically
shifted by 0.1 to 1 cm-1 from the incident light.
- Light that is scattered due to vibrations in
molecules or optical phonons in solids is called
Raman scattering. Raman scattered light is
shifted by as much as 4000 cm-1 from the incident
light. - The sky is blue because fluctuating particles in
the atmosphere scatter blue light more than red
light
4Absorption
- When atoms or molecules absorb light, the
incoming energy excites a quantized structure to
a higher energy level. The type of excitation
depends on the wavelength of the light. - electrons are promoted to higher orbitals by
ultraviolet or visible light, - vibrations are excited by infrared light, and
- rotations are excited by microwaves.
5Absorption
- An absorption spectrum is the absorption of light
as a function of wavelength. The spectrum of an
atom or molecule depends on its energy level
structure, and absorption spectra are useful for
identifying of compounds.
6Absorption
- Measuring the concentration of an absorbing
species in a sample is accomplished by applying
the Beer-Lambert Law. - Red light absorbed by a piece of glass causes the
transmitted light to be appear blue.
7Emission
- Atoms or molecules that are excited to high
energy levels can decay to lower levels by
emitting radiation (emission or luminescence). - For atoms excited by a high-temperature energy
source this light emission is commonly called
atomic or optical emission (atomic-emission
spectroscopy), and - For atoms excited with light it is called atomic
fluorescence (atomic-fluorescence spectroscopy)
or molecular fluorescence (molecular fluorescence
spectroscopy). - For molecules it is called fluorescence if the
transition is between states of the same spin and
phosphorescence if the transition occurs between
states of different spin. - The emission intensity of an emitting substance
is linearly proportional to analyte concentration
at low concentrations, and is useful for
quantitating emitting species. - A flourescent dye may emit green light after
absorbing blue
8Beer-Lambert Law
- The Beer-Lambert law (or Beer's law) is the
linear relationship between absorbance and
concentration of an absorbing species. The
general Beer-Lambert law is usually written asA
a(l) b cwhere A is the measured
absorbance, a(l) is a wavelength-dependent
absorptivity coefficient, b is the path length,
and c is the analyte concentration.
9Instrumentation
- Experimental measurements are usually made in
terms of transmittance (T), which is defined
asT I / Iowhere I is the light intensity
after it passes through the sample and Io is the
initial light intensity. The relation between A
and T isA -log T - log (I / Io).
10Instrumentation
- Modern absorption instruments can usually display
the data as either transmittance,
-transmittance, or absorbance. An unknown
concentration of an analyte can be determined by
measuring the amount of light that a sample
absorbs and applying Beer's law. If the
absorptivity coefficient is not known, the
unknown concentration can be determined using a
working curve of absorbance versus concentration
derived from standards.
11Working Curve
- A working curve is a plot of the analytical
signal (the instrument or detector response) as a
function of analyte concentration. These working
curves are obtained by measuring the signal from
a series of standards of known concentration. The
working curves are then used to determine the
concentration of an unknown sample, or to
calibrate the linearity of an analytical
instrument.
12Photochemical Interaction
- Another result of the interaction of
electromagnetic interaction with matter is
photochemistry. This is obviously extremely
important in biology (such as in vision and
photosynthesis) but this aspect is not dealt with
here.
13Spectroscopy
- The study of the interaction of Electromagnetic
radiation with matter, excluding chemical effects.
14Spectroscopic Techniques
- Irradiation of a sample with some form of
electromagnetic radiation - Measurement of the scattering, absorption, or
emission in terms of some measured parameters
(e.g., scattering intensity at some angle q,
extinction coefficient at a particular
wavelength, or fluorescent lifetime)
15Spectroscopic Techniques
- The interpretation of these measured parameters
to give useful biological information. - This last stage requires some understanding of
the physical basis of the interaction, whether it
is scattering by electrons or nuclei, absorption
by excitation to a higher vibrational level, or
emission from a triplet state.
16Information Available From Spect.
- Detailed study of scattering, absorption, and
emission yields biological information of various
kinds. This information can be broadly classified
as - structural,
- dynamic,
- energetic,
- analytical.
17Information Available From Spect.
- The information available depends on the
instrument used to make the measurements. - While the eye is exceptionally powerful and
versatile, instruments such as the microscope or
the spectrometer can enhance and quantify the
information discernible.
18Each technique has different advantages and
disadvantages, both experimentally and in the
interpretation of the measurements.
19Information Available From Spectroscopy
- The best techniques for determining structure or
the coordinates of a biological system are
microscopy and diffraction.
20Microscopy
- Light microscopy is a technique that can give
structural information directly and
non-invasively about living systems, but the
resolution that can be achieved ( 1 mm) is not
sufficient to study individual molecules.
21Electron Microscopy
- Electron microscopy can achieve higher resolution
( 2 nm), but the sample must be studied in a
vacuum and is normally covered with a metallic
stain, which causes a problem with regard to the
integrity of the structure determined.
22Diffraction Studies
- Diffraction studies of crystals of pure
macromoleculcs can give structural information to
the atomic level (0.15 nm), but this technique
requires crystals, and the structure is no longer
obtained directly but must be interpreted from an
observed diffraction pattern.
23Other Techniques
- Some techniques that can be used to study
macromolecular structure in solution include - optical activity measurements, which give
information on secondary structure of proteins - fluorescence and nuclear magnetic resonance
(NMR), which can give information about
interactions between pairs of centers - electron paramagnetic resonance (EPR), and
resonance Raman, which can "fingerprint" certain
types of structure around a metal ion or
chromophore and solution scattering, which can
give information about the overall shape of a
molecule in solution. - The structural information available from these
methods is nearly always equivocal, although it
is often very useful and important because it can
be obtained in solution and can be combined with
other information on energetics and dynamics.
24Dymamic Information
- Dynamic information about biological systems can
be obtained in a variety of ways. The best
methods are those that give information in
solution. - Examples are
- dynamic light scattering studies of chemotaxis by
bacteria, - fluorescence depolarization studies of the
rotational diffusion of macromolecules, - EPR spin-label studies of lipid fluidity, and
- studies of the movement of fluorescent labels
with the fluorescence microscope.
25Information About Energetics
- Information about energetics can be obtained by
studying - the influence of environment, such as
temperature, ligand concentration, pH, and ionic
strength of the system. - The techniques of UV / visible spectroscopy,
fluorescence, optical activity, and NMR are all
good for distinguishing between bound and unbound
forms of a ligand or a macromolecule, different
ionization states, and different structural forms
of a macromolecule.
26Analytical Information
- The best methods to obtain analytical
information, by which we mean the identification
of a particular compound and the determination of
its concentration, are - UV/visible Spectroscopy,
- NMR, and
- atomic absorption Spectroscopy (AAS).
- It should also be noted that different methods
operate best in different concentration ranges.
NMR is best for studying changes in the
millimolar range, while flourescence is used to
study much lower concentrations ( 1 mM).
27Properties of EM Radiation
- Electromagnetic radiation is made up of two wave
motions perpendicular to each other. One is a
magnetic (M) wave, the other an electric (E)
wave. The waves are propagated along the
z-direction.
Electromagnetic waves are generated by
oscillating electric or magnetic dipoles and are
propagated through a vacuum at the velocity of
light (c). The energies associated with E. and M
are equal, but most optical effects are concerned
with the electric wave, E.
28Polarization
- Since the E- and the M-components are always
perpendicular to each other, it is sufficient, in
many cases, to consider only the E-component in
describing the wave.
Directions of the electric vector In polarized
and unpolarized light. In unpolarized light (a),
or partly polarized light (c), the oscillations
take place at all angles perpendicular to the
direction of travel In polarized light (a) they
are restricted to one angle.
29Degree of Polarization
- It is convenient to introduce a parameter called
the degree of polarization (P) to describe
situations where the radiation is partially
polarized
30Degree of Polarization
- Illustration of (a) how two beams polarized along
xz and yz, 90phase shifted with respect to each
other, generate a circularly polarized beam (b)
when they are superimposed.
31Frequency, Wavelength, Energy, and Wavenumber
- u c / l
- E hu h 6.63 10-34 J.s
- Expression of the radiation as a frequency (Hz)
gives results with very large numbers therefore
it is common to find, particularly for EM
radiation in the microwave to X-ray range, the
frequency expressed as a wavenumber (cm-1). The
wavenumber (u') is defined as the inverse of the
wavelength in centimeters.
32EM and Scales
33What is Matter?
- There are, two concepts arising from wave
mechanics that are very important - The distribution of a particle in space is given
by the square of its wave-function. This leads to
an understanding of orbitals. - Energy states are quantized thus any system has
certain characteristic energy values or levels.
34What is Matter?
- An understanding of the properties of matter,
whether they are describable by wave mechanics or
not, depends on knowledge about its energy and
its coordinates in space and time (that is, its
shape and dynamic properties), it is important to
realize that the three properties of energy,
shape, and dynamics are closely interdependent.
35energy, shape, and dynamics
- the angle of 105 between the H atoms and the O
atom of the H20 molecule, which arises because
this gives an energy minimum to the molecule - the folding of a polypeptide chain in solution to
give a well-defined globular protein, which also
depends on the energy of the system
36Brownian Motion
- Molecules in solution have kinetic energy because
they undergo Brownian motion, that is, they
rotate and diffuse laterally (translate). In
addition, the molecules vibrate because of their
thermal energy. Thus, dynamic and energetic
properties are also related.
37Interparticle Forces and Energies
- The forces between various particles, such as a
nucleus and an electron or between molecules,
often result in a characteristic behavior for the
energy of the system. - If two particles are far apart, there is no
interaction between them. As the particles
approach, there may be direct attraction of
positive and negative charges or there may be a
change in charge distribution on the particle,
resulting in a net attraction.
38Interparticle Forces and Energies
- The energy of the system decreases until an
equilibrium value of the distance between the
particles is reached. As the particles get closer
than this, they begin to repel each other and the
energy increases.
39Interparticle Forces and Energies
- This sort of behavior is typical of many
situations. Examples include - an electron orbiting a nucleus,
- the interaction between atoms in the formation of
chemical bonds and crystals, - the interaction between molecules in gases and
liquids, and - the specific binding of a substrate to an enzyme.
40Energy Levels
- The energy levels represent the characteristic
states of the molecule.
41Energy Levels
- Although every type of energy is quantized, the
separation between neighboring translational
energy levels is so small that for practical
purposes we can disregard the quantization of the
translational energy.
42The Dependence of the Population of Energy Levels
on Temperature
- The exact distribution will depend on the
temperature (thermal energy) and on the
separation between energy levels (DE) in the
energy ladder. At a given temperature the number
of molecules in an upper state (hupper) relative
to the number in a lower stale (hlower) is given
by Boltzmann distribution law