Title: Spectroscopy
1Spectroscopy
2Outline
- Introduction
- Bohr Model
- Examples
- X-ray spectroscopy
- Raman spectroscopy
- Fluorescent spectroscopy
- Nuclear Resonance Vibrational Spectroscopy
3What Is Spectroscopy?
- It is a study of the interaction between
radiation and matter as a function of wavelength
(?) or frequency (f)
4Spectrum
- A plot of the response as a function of
wavelength, or frequency, or energy is referred
to as a spectrum.
E hf
5What Do We Measure?
- Depends on the type of spectroscopy
- - Electromagnetic spectroscopy (intensity)
- - Electron spectroscopy (intensity)
- - Mass spectrometry (mass)
- - Acoustic spectroscopy (intensity)
- - Dielectric spectroscopy (permittivity)
- - Mechanical spectroscopy (stretch, torsion)
6Spectroscopic Methods
7History
Two of the earliest explanations of the optical
spectrum came from Isaac Newton, when he wrote
his Opticks, and from Goethe, in his Theory of
Colours, although earlier observations had been
made by Roger Bacon who first recognized the
visible spectrum in a glass of water, four
centuries before Newton discovered that prisms
could disassemble and reassemble white light.
8Visible spectrum
9Atomic spectra
- Joseph von Fraunhofer 1814
- the spectrum of sunlight is crossed by dark
lines some wavelengths are missing from the
light that reaches us from the Sun!
10Absorption and Emission Spectra
11Johann Balmer, 1885
- Four visible lines in hydrogen spectrum have been
measured by 1885. - Balmer found the measurements to fit the formula
12Is it a coincidence?
l 397 nm - Violet edge of the spectrum
13Generalized Formula
14Atomic Stability
- Classical electromagnetic theory
- An accelerating charge should emit
electromagnetic waves! -
- All electrons should collapse in about 10-11s!
15Bohrs Explanation of Atomic Stability
- Not all electron orbits are allowed!
- A certain discrete set stationary orbits can
exist. - This results in a discrete set of energies.
- An electron in an allowed state would not emit
radiation. - Radiation is emitted once there is a transition
from one state to another this explains spectra!
16Transitions
17The Bohr Model of Hydrogen Atom
Classical Mechanics
18The Bohr Model of Hydrogen Atom
Quantum Mechanics
19The Bohr Model of Hydrogen Atom
20The Bohr Model of Hydrogen Atom
- Knowing possible radii of the electrons orbit,
we can find possible energies
21The Bohr Model of Hydrogen Atom
- Rydberg constant is in the perfect agreement
with the value obtained by Balmer
22Properties of Bohr Atom
23Example 1
- Helium atom has 2 stationary states 2s and 3p
with energies 20.6 eV and 23.1 eV (from the
ground state) correspondingly. What is a
wavelength of a photon emitted as a result of
such a transition?
24Example 2
- What is the diameter of a hydrogen atom with
n100? - Atoms with this high value of n can exist only
in a good vacuum (interatomic spacing at normal
pressure is about 3 nm)
25Diffraction
- Diffraction and interference are similar
- phenomena.
- Interference is the effect of superposition
- of 2 coherent waves.
- Diffraction is the superposition of many
- coherent waves.
26Spectroscopy. Part II
- Outline
- 1. Diffraction
- 2. X-rays
- 3. X-ray spectroscopy
27Double Slit Experiment
28Double Slit Experiment
29Diffraction Grating
- Consists of a flat barrier which contains many
parallel slits separated by a short distance d. - A parallel monochromatic light beam passing
through the grating is diffracted by an angle ?
2dsin? n? similar to two slit interference. - However, the intensity of the diffracted light is
higher and the peaks are much narrower.
30(No Transcript)
31Compact Disk
- The closely spaced dots act like a diffraction
grating.
32Visible light
- Gratings used to disperse ultraviolet (UV) and
visible light usually contain between 300 and
3000 grooves per millimeter, so the distance
between adjacent grooves is on the order of one
micron. - l 400 - 700 nm 0.4 0.7 micron
33EM Spectrum
34X-ray Spectroscopy
- Originally discovered by Wilhelm Roentgen in the
nineteenth century, X-rays have become one of the
most useful applications of spectroscopy in both
science and medicine.
35X-rays
- X-rays are a form of electromagnetic radiation
with a much higher degree of energy than UV
radiation. This extra energy allows X-rays to be
absorbed by core electrons within atoms. Also,
X-rays can penetrate crystal structures more than
other forms of EM radiation, having a wavelength
on the same order of magnitude as interatomic
distances. This allows the X-rays to be
diffracted, producing diffraction patterns of the
crystal.
36Three Basic Applications of X-rays
- 1. Diffraction of X-rays on crystalline materials
to obtain their crystal structure - 2. Measurement of the energy of emitted X-rays
(X-ray Fluorescence ) - 3. Using X-rays to knock out core electrons of
atoms to provide surface chemical information
from samples (X-ray Photoelectron Spectroscopy)
371. Diffraction
- Braggs law
-
- 2dsin? n?
- Visible light the diffraction of sunlight
through a bird's feather was first reported by
James Gregory in the later 17th century.
381. X-ray Diffraction
- The idea that crystals could be used as a
diffraction grating for X-rays arose in 1912 in a
conversation between Paul Peter Ewald and Max von
Laue.
They shined a beam of X-rays through a sphalerite
crystal and record its diffraction on a
photographic plate.
391. Simple Inorganic Crystals
- Although diamonds and graphite are identical in
chemical composition being both pure carbon
X-ray crystallography revealed the arrangement of
their atoms.
401. X-ray Sources
- Synchrotrons (Argonne, Grenoble, etc)
- X-ray tubes
-
X-rays are made monochromatic and collimated to a
single direction before they are allowed to
strike the crystal.
411. Mounting the Crystal
- Goniometer - is an instrument that allows an
object to be rotated to a precise angular
position.
421. Recording the Reflections
- Photographic film
- Area detector
- Charge Couple Device (CCD) sensor
- One image of spots is insufficient to
reconstruct the whole crystal to collect all the
necessary information, the crystal must be
rotated step-by-step through 180.
432. X-ray Fluorescence
- X-ray fluorescence is the emission of
characteristic "secondary" (or fluorescent)
X-rays from a material that has been excited by
bombarding with high-energy X-rays or gamma rays.
The phenomenon is widely used for elemental
analysis and chemical analysis, particularly in
the investigation of metals, glass, ceramics and
building materials, and for research in
geochemistry, forensic science and archaeology.
442. Electronic orbitals
Each element has electronic orbitals of
characteristic energy. Following removal of an
inner electron by an energetic photon provided by
a primary radiation source, an electron from an
outer shell drops into its place.
452. X-ray Fluorescence Spectrum
- X-ray fluorescence spectrum showing the presence
of different elements.
463. Basic Principles of XPS
473. X-ray Photoelectron Spectroscopy
- Uses soft x-ray (200-2000 eV) radiation to
examine core-level electrons.
483. Analyzing Surface with XPS
- Fracturing
- Cutting or scraping in air or UHV to expose the
bulk chemistry - Ion beam etching
- Changes due to heating
- Changes due to exposure to reactive gases or
solutions - Changes due to exposure to UV
493. Electron Spectroscopy for Chemical Analysis
- XPS detects all elements with 3ltZlt103
- Detection limits for most of the elements are in
the parts per thousand range. - XPS is routinely used to analyze inorganic
compounds, metal alloys, semiconductors,
polymers, glasses, ceramics, bio-materials,
viscous oils, glues, ion modified materials and
many others.
50XPS measures
- elemental composition of the surface
- empirical formula of pure materials
- elements that contaminate a surface
- chemical or electronic state of each element in
the surface - uniformity of elemental composition across the
top surface - uniformity of elemental composition as a function
of ion beam etching
513. Typical XPS spectrum
52