CHAPTER 9 Molecules Rotations Spectra Complex planar molecules

Slides:



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

Molecular Bonds Molecular Spectra Molecules and Solids CHAPTER 10 Molecules and Solids Johannes Diderik van der Waals (1837 – 1923) “You little molecule!”
Lecture 6 nitrogen and ozone photochemistry Regions of Light Absorption of Solar Radiation.
METO 621 Lesson 6. Absorption by gaseous species Particles in the atmosphere are absorbers of radiation. Absorption is inherently a quantum process. A.
Electrons And Light. Electromagnetic Radiation Energy that travels as a wave through space Wavelength –λ – distance between corresponding points on adjacent.
Vibrational Spectroscopy I
METO 621 LESSON 7. Vibrating Rotator If there were no interaction between the rotation and vibration, then the total energy of a quantum state would be.
Spectroscopy. Atoms and Light  Atomic electron energy levels are a source of discrete photon energies.  Change from a high to low energy state produces.
Physics for Scientists and Engineers, 6e Chapter 43 - Molecules and Solids.
Absorption and Emission Spectrum
Dr. Jie ZouPHY Chapter 43 Molecules and Solids.
Quantum Physics. Black Body Radiation Intensity of blackbody radiation Classical Rayleigh-Jeans law for radiation emission Planck’s expression h =
Classical Model of Rigid Rotor
Vibrational Transitions
1 LECTURE # 32 HYDROGEN ATOM PARTICLE DOUBLE-SLIT PROBABILITY PHYS 270-SPRING 2010 Dennis Papadopoulos MAY
Physics and the Quantum Model
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.
Microwave Spectroscopy Rotational Spectroscopy
Spectroscopic Analysis Part 4 – Molecular Energy Levels and IR Spectroscopy Chulalongkorn University, Bangkok, Thailand January 2012 Dr Ron Beckett Water.
Vibrational and Rotational Spectroscopy
Vibrational Spectroscopy
Spectroscopy and Electron Configurations
Properties of Light.
Chapter 4 The Bohr Model of the Atom Part 1. Visible Light.
MOLECULAR SPECTROSCOPY  SPECTROSCOPY IS THAT BRANCH OF SCIENCE WHICH DEALS WITH THE STUDY OF INTERACTION OF ELECTROMAGNETIC RADIATION WITH MATTER.  ELECTROMAGNETIC.
The Electronic Spectra of Coordination Compounds.
Quantum Chemistry Chapter 6. Copyright © Houghton Mifflin Company. All rights reserved.6 | 2 Electromagnetic Radiation.
MOLECULAR SPECTROSCOPY  SPECTROSCOPY IS THAT BRANCH OF SCIENCE WHICH DEALS WITH THE STUDY OF INTERACTION OF ELECTROMAGNETIC RADIATION WITH MATTER.  ELECTROMAGNETIC.
Ch ; Lecture 26 – Quantum description of absorption.
Unit #4 CP Chemistry.  Bohr  Quantum Numbers  Quantum Mechanical Model.
ROTATIONAL SPECTROSCOPY
Rotation and vibration spectra. Rotational States Molecular spectroscopy: We can learn about molecules by studying how molecules absorb, emit, and scatter.
441 Chem Introduction to Spectroscopy CH-1 1. Introduction to Spectroscopy Set of methods where interaction of electromagnetic radiation with chemical.
Topic 13 Quantum and Nuclear physics Atomic spectra and atomic energy states.
Simple Harmonic Oscillator (SHO) Quantum Physics II Recommended Reading: Harris: chapter 4 section 8.
Spectroscopy and Atomic Structure Ch 04.
Chapter 7. Electromagnetic Radiation  aka. Radiant energy or light  A form of energy having both wave and particle characteristics  Moves through a.
MOLECULAR SPECTROSCOPY  SPECTROSCOPY IS THAT BRANCH OF SCIENCE WHICH DEALS WITH THE STUDY OF INTERACTION OF ELECTROMAGNETIC RADIATION WITH MATTER.  ELECTROMAGNETIC.
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 14 The Interstellar Medium. All of the material other than stars, planets, and degenerate objects Composed of gas and dust ~1% of the mass of.
Schrödinger Equation – Model Systems: We have carefully considered the development of the Schrödinger equation for important model systems – the one, two.
Rotation and vibration spectra. Rotational States Molecular spectroscopy: We can learn about molecules by studying how molecules absorb, emit, and scatter.
The Particle Model of Light and Atomic Emission and Absorption
Chapter 8. Molecular Motion and Spectroscopy
10.1Molecular Bonding and Spectra 10.2Stimulated Emission and Lasers Molecules and Solids CHAPTER 10 Molecules and Solids.
MOLECULAR SPECTROSCOPY
Electrons And Light. Electromagnetic Radiation Energy that travels as a wave through space Wavelength –λ – distance between corresponding points on adjacent.
Why do molecules form? Molecular bonds Rotations Vibrations Spectra Complex planar molecules Molecules CHAPTER 9 Molecules Johannes Diderik van der Waals.
The Bohr Model of the Atom
Chem. 133 – 3/9 Lecture.
CHAPTER 10 Molecules Why do molecules form? Molecular bonds Rotations
CHAPTER 9 Molecules Why do molecules form? Molecular bonds Rotations
UNIT IV Molecules.
CHAPTER 6 Structure of the Atom
Bohr Model Of Atom.
Bohr Model Of Atom.
Quantum Theory and The Atom
CHAPTER 10 Molecules Why do molecules form? Molecular bonds Rotations
CHAPTER 9 Molecules Rotations Spectra Complex planar molecules
Waves.
Chapter 4 The Wave Description of Light
Diatomic molecules
Sources of Light and and Blackbody Radiation
Energy and Electrons energy
Tro's "Introductory Chemistry", Chapter 9
Cutnell/Johnson Physics 7th edition
Overview of spectroscopy transitions
5.4 Learning from Light Our goals for learning
Molecular Spectra By – P.V.Koshti.
Presentation transcript:

CHAPTER 9 Molecules Rotations Spectra Complex planar molecules Homework due Wednesday Nov. 5th Only 5 problems: 8, 14, 17, 20, 22 Johannes Diderik van der Waals (1837 – 1923) http://en.wikipedia.org/wiki/Image:Johannes_Diderik_van_der_Waals.jpg “Life ... is a relationship between molecules.”  Linus Pauling

Rotational States Consider diatomic molecules. A diatomic molecule may be thought of as two atoms held together with a massless, rigid rod (rigid rotator model). In a purely rotational system, the kinetic energy is expressed in terms of the angular momentum L and rotational inertia I.

Rotational States L is quantized. where ℓ can be any integer. The energy levels are Erot varies only as a function of the quantum number ℓ. = ħ2/I

Rotational transition energies And there is a selection rule that Dℓ = ±1. Transitions from ℓ +1 to ℓ : Emitted photons have energies at regular intervals:

Vibration and Rotation Combined Note the difference in lengths (DE) for larger values of ℓ. Note the similarity in lengths (DE) for small values of ℓ. DE increases linearly with ℓ. Most transitions are forbidden by the selection rules that require Dℓ = ±1 and Dn = ±1.

Vibration and Rotation Combined The emission (and absorption) spectrum spacing varies with ℓ. The higher the starting energy level, the greater the photon energy. Vibrational energies are greater than rotational energies. For a diatomic molecule, this energy difference results in band structure. The line strengths depend on the populations of the states and the vibrational selection rules, however. Weaker overtones Dn = 3 Dn = 0 Dn = 1 Dn = 2 Energy or Frequency → Dℓ = -1 Dℓ = 1

Vibrational/Rotational Spectrum In the absorption spectrum of HCl, the spacing between the peaks can be used to compute the rotational inertia I. The missing peak in the center corresponds to the forbidden Dℓ = 0 transition. ℓi- ℓf = -1 ℓi- ℓf = 1 ni- nf = 1

Frequencies in Atoms and Molecules Electrons vibrate in their motion around nuclei High frequency: ~1014 - 1017 cycles per second. Nuclei in molecules vibrate with respect to each other Intermediate frequency: ~1011 - 1013 cycles per second. Nuclei in molecules rotate Low frequency: ~109 - 1010 cycles per second.

Including Electronic Energy Levels A typical large molecule’s energy levels: E = Eelectonic + Evibrational + Erotational 2nd excited electronic state Lowest vibrational and rotational level of this electronic “manifold.” Energy 1st excited electronic state Excited vibrational and rotational level Transition There are many other complications, such as spin-orbit coupling, nuclear spin, etc., which split levels. Ground electronic state As a result, molecules generally have very complex spectra.

Studying Vibrations and Rotations Infrared spectroscopy allows the study of vibrational and rotational transitions and states. But it’s often difficult to generate and detect the required IR light. It’s easier to work in the visible or near-IR. DE Input light Output light Raman scattering: If a photon of energy greater than DE is absorbed by a molecule, another photon with ±DE additional energy may be emitted. The selection rules become: Δn = 0, ±2 and Δℓ = 0, ±2

Modeling Very Complex Molecules Sometimes more complex is actually easier! Many large organic (carbon-based) molecules are planar, and the most weakly bound electron is essentially free to move along the perimeter. We call this model the Perimeter Free-Electron Orbital model. plus inner elec-trons This is just a particle in a one-dimensional box! The states are just sine waves. The only difference is that x = L is the same as x = 0. So y doesn’t have to be zero at the boundary, and there is another state, the lowest-energy state, which is a constant:

Auroras http://www.itp.uni-hannover.de/~zawischa/ITP/atoms.html

Typical Aurora Emission Spectrum Intensity http://www.itp.uni-hannover.de/~zawischa/ITP/atoms.html

Species Present in the Atmosphere http://www.itp.uni-hannover.de/~zawischa/ITP/atoms.html

Constituents Contributing to Auroras H N http://www.itp.uni-hannover.de/~zawischa/ITP/atoms.html