Chapter 8 An Introduction to Optical Atomic Spectrometry 1

Slides:



Advertisements
Similar presentations
Astronomy Notes to Accompany the Text Astronomy Today, Chaisson, McMillan Jim Mims.
Advertisements

Lecture 6 ATOMIC SPECTROSCOPY
The Amazing Spectral Line Begin. Table of Contents A light review Introduction to spectral lines What spectral lines can tell us.
FLAME SPECTROSCOPY The concentration of an element in a solution is determined by measuring the absorption, emission or fluorescence of electromagnetic.
ATOMIC ABSORPTION SPECTROMETER
Atomic Absorption Spectroscopy Prof Dr Hisham E Abdellatef 2011.
AA and Atomic Fluorescence Spectroscopy Chapter 9
Atomic Absorption Spectroscopy (AAS) The Visible Spectra.
427 PHC. Introduction  Spectrometric methods are a large group of analytical methods that are based on atomic and molecular spectroscopy.  Spectroscopy.
427 PHC.  Atomic emission spectroscopy (AES) is based upon emission of electromagnetic radiation by atoms.
PHYS 206 Matter and Light At least 95% of the celestial information we receive is in the form of light. Therefore we need to know what light is and where.
Ahmad Aqel Ifseisi Assistant Professor of Analytical Chemistry College of Science, Department of Chemistry King Saud University P.O. Box 2455 Riyadh
Atomic Spectroscopy: Atomic Emission Spectroscopy
Spectroscopy 1: Rotational and Vibrational Spectra CHAPTER 13.
Atomic spectra are a result of energy level diagrams - quantum theory.
The Photoelectric Effect
OPTICAL ATOMIC SPECTROMETRY Chap 8 Three major types Optical spectrometry Optical spectrometry Mass spectrometry Mass spectrometry (X-ray spectrometry)
Advanced Higher Chemistry Unit 1 Spectroscopy. Spectroscopy  Spectroscopy is used to give information regarding the structure of atoms or molecules.
Atomic Spectroscopy: Atomic Emission Spectroscopy Atomic Absorption Spectroscopy Atomic Fluorescence Spectroscopy * Elemental Analysis * Sample is atomized.
6-1 RFSS: Lecture 6 Gamma Decay Part 2 Readings: Modern Nuclear Chemistry, Chap. 9; Nuclear and Radiochemistry, Chapter 3 Energetics Decay Types Transition.
Ahmad Aqel Ifseisi Assistant Professor of Analytical Chemistry College of Science, Department of Chemistry King Saud University P.O. Box 2455 Riyadh
Chapter 8 An Introduction to Optical Atomic Spectroscopy
4-1 Chap. 7 (Optical Instruments), Chap. 8 (Optical Atomic Spectroscopy) General design of optical instruments Sources of radiation Selection of wavelength.
Spectroscopy and Atomic Structure.
Chapter 4 Spectroscopy Chapter 4 opener. Spectroscopy is a powerful observational technique enabling scientists to infer the nature of matter by the way.
Atomic Emission Spectroscopy
Chapter 4 Spectroscopy.
Atomic Absorption Spectroscopy
New Way Chemistry for Hong Kong A-Level Book 11 Chapter 4 The Electronic Structure of Atoms 4.1The Electromagnetic Spectrum 4.2 Deduction of Electronic.
Spectroscopy and Electron Configurations
1 Components of Optical Instruments Lecture Silicon Diode Transducers A semiconductor material like silicon can be doped by an element of group.
B.SC.II PAPER-B (OPTICS and LASERS)
ANALYTICAL CHEMISTRY CHEM 3811 CHAPTER 20
to Optical Atomic Spectroscopy
Vector coupling of angular momentum. Total Angular Momentum L, L z, S, S z J and J z are quantized Orbital angular momentumSpin angular momentum Total.
Atoms in stellar atmospheres are excited and ionized primarily by collisions between atoms/ions/electrons (along with a small contribution from the absorption.
Atoms in stellar atmospheres are excited and ionized primarily by collisions between atoms/ions/electrons (along with a small contribution from the absorption.
Chapter 10 Atomic Structure and Atomic Spectra. Spectra of complex atoms Energy levels not solely given by energies of orbitals Electrons interact and.
ATOMIC/MOLECULAR SPECTROSCOPY  Various spectroscopic techniques are used to elucidate molecular structures (eg. NMR), to study molecular vibrations (IR.
Fluorescence Spectroscopy
Astrophysics Yr 2 Session 6 Astronomical Spectroscopy.
Atomic Fluorescence Spectroscopy. Background l First significant research by Wineforder and Vickers in 1964 as an analytical technique l Used for element.
1 Introduction to Atomic Spectroscopy Lecture 10.
Quantum Theory Chang Chapter 7 Bylikin et al. Chapter 2.
Spectroscopy Spectral lines The Fraunhofer spectrum Charlotte Moore Sitterly (Allen!) –Multiplet table –Rowland table Formalism of spectroscopy.
atomic excitation and ionisation
Chapter 4 Spectroscopy The beautiful visible spectrum of the star Procyon is shown here from red to blue, interrupted by hundreds of dark lines caused.
Chapter 4.
1.1 What’s electromagnetic radiation
1 Introduction to Atomic Spectroscopy Lecture 10.
Chapter – 7 Line Width Line Width (natural) Oscillator strength
Introduction to Optical Atomic spectrometry
Atomic Structure and Atomic Spectra
Atomic Absorption Spectroscopy.  Qualitative test for metals in solution  Can also be used for coloured lights  This emission of light is called an.
1 Introduction to Atomic Spectroscopy Lecture 10.
MOLECULAR SPECTROSCOPY
The Solar System Lesson2 Q & A
Early models to Quantum Model
What Is Light? Light is formed when electrons drop from the excited state to the ground state. The lines on a bright-line spectrum come from specific energy.
Atomic Emisson spectroscopy (AES)
Chapter 8 An Introduction to Optical Atomic Spectroscopy
Diatomic molecules
Electromagnetic spectrum
Atomic Absorption Spectroscopy
Stars and Galaxies Lesson2 Q & A
Energy and Electrons energy
Atomic Absorption Spectroscopy. Atomic absorption spectroscopy is based on the same principle as the flame test used in qualitative analysis.
5.4 Learning from Light Our goals for learning
Continuous, Emission, and Absorption
Spectroscopy Uses emission and absorption of light by electrons moving between ground and excited state configuration, hence electronic configuration.
Presentation transcript:

Chapter 8 An Introduction to Optical Atomic Spectrometry 1 Chapter 8 An Introduction to Optical Atomic Spectrometry 1 Atomic Spectra

1.1 Energy level diagrams Every element has an unique set of atomic orbitals p, d, f .. split by spin-orbit coupling Spin (s) and orbital (l) motion create magnetic fields that perturb each other (couple) if fields parallel – higher energy if fields antiparallel – lower energy. Define spin-orbit coupling by J (total angular momentum) J = L + S (L=l S= s ) (positive values only) Examples: s electron ( l = 0, s = +1/2 or -1/2) J = 0+ ½ = ½ p electron ( l = 1, s = +1/2 or -1/2) J = 1+1/2 = 3/2 (higher energy ) or J = 1-1/2 = 1/2 (lower energy ) Electronic term symbol 2S+1LJ L written as letter (S, P, D ) instead of number Na = 1s22s22p63s1, L = 0, S= 1/2, 2S1/2 Na* = 1s22s12p63p1, L = 1, S= 1/2, 2P3/2, 1/2

Fig. 8-1 (p.216) Energy level diagrams for Na and Mg+

Fig. 8-1a and 8-2 (p.216-217) Energy level diagram for Mg+, and atomic magnesium

Similar pattern between atoms but different spacing Spectrum of an ion different to that of the corresponding atom Energy levels measured in electron volts (eV) 1eV = 1.602x10-19 Cx1 V(J/C) = 1.602x10-19 J = 96.484 kJ .mol-1 As # of electron increases, # of levels increases, emission spectra become more complex

1.2 Atomic line widths 1.2.1 Line broadening from the uncertainty principle Uncertainty principle: must measure for some minimum time to tell two frequencies apart t  E  h t    1 t: minimum time for measurement : minimum detectable difference in frequencies Shows up in lifetime of excited state - if lifetime infinitely long, E infinitely narrow - if lifetime short, E is broadened  = c/ Differentiating  wrt to  d=-c2d, d   and d    = 2/c natural line widths

1.2.2 Doppler broadening Change in frequency produced by motion relative to detector In gas, broadens line symmetrically because of Maxwell-Boltzman velocity distribution Average velocity of atoms increases as (T)1/2 At room T, line widths 10-2-10-3 A Total line width typically 1-10 A

1.2.3 Pressure broadening Collisions with other atoms transfer small quantities of energy (heat) – ill-defined ground state energy Effects worse at high pressures - for low pressure hollow cathode lamp (1-10 torr) 10-1 -10-2 A - for high pressure Xeon lamps (>10,000 torr) 100-1000 A (continuum radiation!)

1.3 Other effects of temperature Temperature changes # of atoms in ground and excited states changes Emission measurements rely on number of excited atoms, requiring close control of temperature (e.g., at 2500K Na only has 0.02% atoms in first excited state, a rise of 10K in temperature results in 4% increase of excited atoms) Less important in absorption measurement, 99.8% atoms in ground state!

2 Atomization Methods Sample must be converted to gaseous atoms or ions first

Fig. 8-11 (p.226) Pneumatic nebulizers 2.1 Introduction of solution samples Must transfer sample to atomizer Fig. 8-11 (p.226) Pneumatic nebulizers

Fig. 8-10 (p.225) Processes leading to atoms, molecules and ions with continuous sample introduction into a flame.

sputtering 2.2 Introduction of solid sample Fig. 8-12 (p.227) A glow-discharge atomizer