Slide 1Why does Neon Glow?Dilemmas/Flaws of Atomic StructureWave PropertiesClicker 6.1:Speed of WavesRadiation (aka Energy)Max PlankSample ProblemWhat can we learn from White light?Atomic SpectraBohr Model of Hydrogen AtomQuantum StaircaseQuantum StaircaseBohr Spectral LinesCalculating Energy of ElectronsLimitations of Bohr’s ModelWave Behavior of MatterWave Behavior of MatterThe Wavelength of a BaseballThe Uncertainty PrincipleQuantum MechanicsQuantum MechanicsQuantum NumbersQuantum NumbersQuantum Numbers (a closer look at shape)Quantum Numbers (a closer look at shape)Quantum Numbers (a closer look at shape)Quantum Numbers (a closer look at shape)Quantum NumbersQuantum Numbers (a closer look at Orientation)Quantum Numbersn and l for: Hydrogenn and l for: All other elementsn and l for: All other elementsQuantum NumbersPauli Exclusion PrincipleSample ProblemsSample ProblemsSample ProblemsSlide 41Sample ProblemsSample ProblemsSample ProblemsAssigning n & l ValuesClicker 6.6 – 6.8:Electron ConfigurationSample ProblemsSlide 49Clicker 6.12:Clicker 6.13:Clicker 6.14:Electron Configurations Cont’dSample ProblemsOrbital DiagramsSlide 56d-block Electron Configuration Exceptionsd-block Electron Configuration ExceptionsWhen are Elements Magnetic?Clicker 6.15:Valence ElectronsValence ElectronsAdded Info About Valence ElectronsClicker 6.17:Electron Configurations of IONSElectron Configurations of IONSSample Problem1Electronic Structureof AtomsChapter 6Chemistry the Central Scienceby: Brown, Lemay, Bursten, Murphy & WoodwardPresented by: Dr. Stacey GuldeWhy doesNeon Glow?Electrons excited to higher energies by electricityElectrons fall to a lower energy, emitting lightQuantum theory explains the behavior of electrons in atomsWill look at the arrangement of electrons in atoms (Aka: electronic structure of atoms)•Refers to the # of electrons in an atom AND their distribution around the nucleus23Dilemmas/Flaws of Atomic StructureFrom 1890 – 1930 a new theory developed a relationship b/t energy & particlesEnergy – ability to do work, to move matterUsually refer to matter in terms of an object (aka particle)Can also refer to matter in terms of radiation (aka energy)Scientist believed there was NO connection b/t the energy of particles & radiation, b/c of how then movedParticles move in straight linesRadiation moves in wavesWave PropertiesTerminology for discussing waves:Crest – highest point of waveWavelength, (lamda) – distance b/t identical points•Unit = mFrequency, (nu) – # of crests that pass a point in 1 sec•Unit = inverse time, s-1 (cycles per second): Hertz (Hz)4DistancecrestClicker 6.1:Which wave has the following?Longer wavelength Lower frequencyA. Red RedB. Red Blue C. Blue RedD. Blue BlueInverse relationship!Long = Low 5Speed of WavesSpeed of wave – distance traveled per unit of timeSpeed of light (c) = 3.00x108 m/s (in vacuum)•inexact value = s-1 or Hz = m6c cRadiation (aka Energy)Electromagnetic Spectrum – lists the different types ofradiation energyFamiliar with visible light•Eachcolor has adifferentENERGY7HighenergyLowenergyMax PlankMax Plank (1900) – figured out that energy and frequency are relatedRemember: So, 8E = energy of a quantum of light (J)h = Planck’s Constant (6.63 x 10-34 Js) = frequency (Hz or s-1)vhE chcE Sample ProblemGive the amount of energy associated with a radiation that has a wavelength of 575nm. What type of radiation is it?9=575nm mElectro.SpectrumYellow lightE=?hcE nm575 nm1mx9101mx71075.5E sJx 341063.6 smx81000.3mx71075.5JxE191046.310What can we learn from White light?White light produces a Continuous spectrum – we see all colors (rainbow)Each color is a different energy, thus all energies possible11Atomic SpectraLight from a vaporized element, produces an Atomic spectrum – see some colorsOnly specific energies possibleColors given = Line spectrumEach element has a uniquespectrum (fingerprint)656nm486nm434nm410nmBohr Model ofHydrogen AtomNiels Bohr (worked w/Rutherford) suggested a model for existence of the hydrogen line spectrum1. H atom has certain allowable energy levels called stationary states, corresponding to a fixed electron orbit around the nucleus2. The atom doesn‘t give off energy while in a stationary state3. When an atom changes states, it experiences an overall energy equal to the difference between the 2 states1221 StateStateOverallEEE hQuantum StaircaseBohr attributed radiation emission (seeing light) to the dropping of an electron from a high energy state to a lowerGiving off a quantum of energy as lightTHERE IS A CONNECTION b/t PARTICLES & ENERGY!Quantum number, n (1, 2, 3…) = indicates the energy & radius of an electron orbitHigh n values: have high energy, thus a larger radius13Ground state (n = 1) – lowest energy of an electron•Most stable stateExcited state (n > 1) – higher energy level•Stability decreasesElectrons “jump” or leap from oneenergy state to anotherThey are never in-between themDirection matters:Promoting to higher n values: absorbs lightDropping to lower n values: gives off light14Quantum StaircaseBohrSpectral LinesMore energy is given off /absorbed when the dropping/promoting difference between energy levels (n) is large6 1 is larger than2 1 15Calculating Energyof ElectronsRydberg Equation: Calculates the amount (quanta) of energy to move from an initial to a final stateA negative E value indicates energy EMITTED,nfinal < ninitial16E = Energy (J)RH = Rydberg constant (2.18x10-18 J)n = energy levelhchE 2218111018.2initialfinalnnJxELimitations ofBohr’s Model1. Only works for hydrogen 2. Fails for atoms with more than 1 electronDue to:•Electron-electron: repulsions•Electron-nucleus: attractionsFor all other elements, we still use the terms ground/excided17Wave Behavior of MatterDeBroglie (1920’s) – suggested if light (energy) behaves like particles, then maybe particles (electrons) posses wave propertiesElectrons orbiting a nucleus must have a characteristic wavelength He dubbed the wave characteristic of particles: matter waves18Wave Behavior of MatterCombined
View Full Document