* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download Chapter 6
Quantum teleportation wikipedia , lookup
Coherent states wikipedia , lookup
Delayed choice quantum eraser wikipedia , lookup
Relativistic quantum mechanics wikipedia , lookup
Quantum group wikipedia , lookup
Probability amplitude wikipedia , lookup
Renormalization wikipedia , lookup
Copenhagen interpretation wikipedia , lookup
Symmetry in quantum mechanics wikipedia , lookup
Interpretations of quantum mechanics wikipedia , lookup
History of quantum field theory wikipedia , lookup
Canonical quantization wikipedia , lookup
Quantum state wikipedia , lookup
Quantum key distribution wikipedia , lookup
EPR paradox wikipedia , lookup
Ultraviolet–visible spectroscopy wikipedia , lookup
Hidden variable theory wikipedia , lookup
Tight binding wikipedia , lookup
Particle in a box wikipedia , lookup
Molecular orbital wikipedia , lookup
Bohr–Einstein debates wikipedia , lookup
Double-slit experiment wikipedia , lookup
Atomic theory wikipedia , lookup
Quantum electrodynamics wikipedia , lookup
X-ray fluorescence wikipedia , lookup
Matter wave wikipedia , lookup
Hydrogen atom wikipedia , lookup
Atomic orbital wikipedia , lookup
Electron configuration wikipedia , lookup
Theoretical and experimental justification for the Schrödinger equation wikipedia , lookup
Chp 6: Atomic Structure 1. Electromagnetic Radiation 2. Light Energy 3. Line Spectra & the Bohr Model 4. Electron & Wave-Particle Duality 5. Quantum Chemistry & Wave Mechanics 6. Atomic Orbitals 1. Absorption - An Electron Absorbs the Light, Acquiring It’s Energy and Entering an “Excited State” 2. Emission - An Electron “Relaxes” to a Overview Chemical Reactions are a Result of Electron Interactions Between Various Elements Elemental Behavior Is the Result of the Element’s Electronic Structure Periodic Table is Based on an Elements Electronic Structure 1. Light Travels Through Space 2. Light has Color 3. Light has Energy Lower Energy State While Emitting Light 4. Light Energy is Quantized Name Some Characteristics of Light 6.1 Electromagnetic Radiation Wavelength (l) - Distance Between two Peaks Frequency (u) - How Often Waves Goes Through a Complete Cycle (1/sec = hertz) Speed (c) - How Fast Wave Propagates So What Is Light? Spectrum l c u u c l c = 3 X 108 m/sec c=lu 1 6.2 Nature of Matter: WaveParticle Duality Electromagnetic Radiation & Energy Planks Constant relates the Energy of a photon of light to it’s frequency. Light exhibits both wave and particle behavior. E=hu Photon - “Particle of Light” (Einstein) E = nhn, where n = # of photons Einstein’s Photoelectric Effect h=Planck’s Constant h= 6.63X10-34J.sec How do we relate the Energy of light to it’s wavelength? from c lu Eh c l Electromagnetic Radiation & Energy Small Wavelength High Frequency High Energy Large Wavelength Low Frequency Low Energy E=hu Light Intensity I = nhu (n = moles of photons) Think about the video on Einstein’s photoelectric effect and the difference between “intense” red light and “weak” blue light Wavelength (meters) Photon Energy Problem How many photons of microwave radiation (l=125mm) are required to heat 1 L of water from 20.0oC to the boiling point? ELight = q -Use s for specific heat capacity as c is the speed of light nhu = msDT Sodium Line Spectra Sodium gives off yellow light of a specific wavelength of 589.0 nm. What is the frequency of the yellow line spectra of sodium? 2 Sodium Line Spectra Sodium gives off yellow light of a specific wavelength of 589.0 nm. 1. Determine E for a photon of sodium yellow light Bohr Model of Hydrogen Atom Correctly Described the Hydrogen Spectrum Used Concept of Orbits (Wrong) Used Concept of Quantized Energy Levels (Right) 2. Determine E for a mole of photons of sodium yellow light Bohr Equation for Hydrogen Energy of the nth level: RH= Rydberg constant RH=Rhc 1 E n RH ( 2 ) n Bohr Model of Hydrogen Atom nf= 1 for UV light nf= 2 for visible light RH= 2.18x10-18 J Energy for transition ni --> nf: DEni n f En f Eni hu Rh ( DE ni n f hu Rh ( 1 1 ) n 2f ni2 nf= 3 for IR light 1 1 ) ni2 n 2f Bohr Problem: What Is the Energy Level of the Excited State Which Is Responsible for the Blue Green Emission Line at 486.1 nm? That is, what is the initial quantum state; ni? Emission is an exothermic process Absorption is an endothermic process 6.4 Wave-Particle Duality De Broglie’s Hypothesis: All Matter has a Characteristic Wavelength hc E mc2 hv l l h mv v=velocity & mv = momentum Note the inverse relationship between the mass and the wavelength 3 DeBroglie Wavelength of Electron Calculate the DeBroglie Wavelength of an Electron moving at 1.00% the speed of light c = 3x108m/s, m=9.11x10-31kg E = mc2 mc2 = hu E = hu uc c=lu l DeBroglie Wavelength of Electron Calculate the DeBroglie Wavelength of an Electron moving at 1.00% the speed of light c = 3x108m/s, m=9.11x10-31kg mc2 = hc l mv = h mc = h l l Wave-Particle Duality – Electron Diffraction lelec = 2.4 x 10-10m and is diffracted by a crystal like NaCl Wave-Particle Duality Uncertainty The characteristic wavelength of an electron in a hydrogen atom is 240pm The size of an isolated H atom is about 240 pm This leads to an uncertainty in the location of the electron Heisenberg’s Uncertainty Principle You can not simultaneously know both the position and momentum of an electron To measure the position of an electron, you need a wavelength smaller than it’s characteristic wavelength, which is of such a high energy that it alters the electron’s position during the measurement process Physical Meanings of Wave Functions Bohr Model Uses Orbits Quantum Mechanics Uses Orbitals (Y2) Y2 - Probability Distribution Function, Describes the probability of finding an electron in a specific location for a given energy state 4 Quantum Numbers Physical Meanings of Wave Functions Bohr Model Uses Orbits Quantum Mechanics Uses Orbitals (Y2) Orbitals are Probability Distribution Functions - They Represent the Probability of Finding an Electron at a Certain Space in Time Different Orbitals Are Defined by Their Shapes and Distance From the Nucleus Quantum Numbers Bohr Orbits Can Be Described by One Quantum Number, N, the Principle Quantum Number Quantum Mechanics Uses 4 Quantum Numbers n l ml ms - Principle Quantum Number Azimuthal Quantum Number Magnetic Quantum Number Spin Quantum Number (Dirac) n - Principle Quantum Number n has integral values; n = 1,2,3... Each Orbital Can Be Described by It’s Set of Quantum Numbers n correlates to the “shells” and the periods of the periodic table There are n2 orbitals in each shell No Two Electrons Can Have the Same Set of Quantum Numbers l - Azmuthal Quantum Number Describes the shape of the orbital Use letters to designate values of l s: l=0 d: l=2 p: l=1 f: l=3 l has values of 0 to n-1 for each principle level -The 1st Principle Level has l = 0 - the 2nd has l = 0,1 - the 3rd has l = 0,1,2 - the 4th has l = 0,1,2,3 - all the rest have 4 or less 1s 2s, 2p 3s, 3p, 3d 4s, 4p, 4d, 4f The Larger the Value of n, the Greater the Average Distance From the Nucleus & the Greater the Orbital’s Energy ml - Magnetic Quantum Number Describes Orientation in Space There are 2l+1 values of ml for each type of azmuthal quantum number with values ranging form l to -l 1 type of s (l = 0) orbital 3 types of p (l = 1) orbitals 5 types of d (l = 2) orbitals 7 types of f (l=3) orbitals 5 Each Orbital can be identified by it’s Quantum numbers n 6.6 Orbital Shapes & Energies: S Orbitals (l=0) Spherical in Nature l, use letters s,p,d & f Example, 2px “Balloon Diagram” shows region of 90% probability of finding electron ml, describes orientation All Periods Have S Orbitals 1s 2s 3s “Onion Skin” layers of 1st 3 S orbitals s orbital radial probability functions P Orbitals (l=1) There are 3 types of P orbitals 2nd Period & Greater Have P Orbitals Y2 Y2 1s r Y2 2s 3s node nodes r r d Orbitals (l=2) 5 types of d orbitals f orbitals 3rd Period & Greater Have d Orbitals 7 types of f orbitals 4th Period & Greater Have f Orbitals 6