The Quantum Mechanical Atom CHAPTER 8 Chemistry: The Molecular Nature of Matter, 6th edition By Jesperson, Brady, & Hyslop CHAPTER 8: Quantum Mechanical Atom Learning Objectives Light as Waves, Wavelength and Frequency The Photoelectric Effect, Light as Particles and the Relationship between Energy and Frequency Atomic Emission and Energy Levels The Bohr Model and its Failures Electron Diffraction and Electrons as Waves Quantum Numbers, Shells, Subshells, and Orbitals Electron Configuration, Noble Gas Configuration and Orbital Diagrams Aufbau Principle, Hund’s Rule, and Pauli Exclusion Principle, Heisenberg Uncertainty Principle Valence vs Inner Core Electrons Nuclear Charge vs Electron Repulsion Periodic Trends: Atomic Radius, Ionization Energy, and Electron Affinity 2 Electron Configurations Periodic Table & Electron Configurations • Divided into regions of 2, 6, 10, and 14 columns • This equals maximum number of electrons in s, p, d, and f sublevels Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 3 Electron Configurations Periodic Table & Electron Configurations Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 4 Electron Configurations Shorthand: Electron Configurations • [noble gas of previous row] and electrons filled in next row • Represents core + outer shell electrons • Use to emphasize that only outer shell electrons react Ex: Group 2 A elements: Z Electron Configuration Abbrev Be 4 1s 22s 2 [He] 2s 2 Mg 12 1s 22s 22p 63s 2 [Ne] 3s 2 Ca 20 1s 22s 22p 63s 23p 64s 2 [Ar] 4s 2 Sr 38 1s 22s 22p 63s 23p 63d 104s 24p 65s 2 [Kr] 5s 2 Ba 56 1s 22s 22p 63s 23p 63d 104s 24p 64d 105s 25p 66s 2 [Xe] 6s 2 Ra 88 1s 22s 22p 63s 23p 63d 104s 24p 64d 104f 145s 25p 6 5d 106s 26p 67s 2 [Rn] 7s 2 Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 5 Electron Configurations Shorthand: Orbital Diagrams Write out lines for orbital beyond Noble gas Higher energy orbital to right Fill from left to right Abbreviated Orbital Diagrams Ru [Kr] 4d S [Ne] 5s 3s 3p Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 6 Electron Configurations Valance Shell Electron Configurations Valence Electrons = Electrons in the outer most shell (ie, highest n) • Here only electrons in outer shell important for bonding • Only electrons in s and p subshells • Valence shell = outer shell = occupied shell with highest n • Result – use even more abbreviated notation for electron configurations • Sn = 5s 25p 2 Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 7 Electron Configurations Element Cr Cu Ag Au Exceptions to the Rules: Electron Configurations Expected [Ar] 3d 44s 2 [Ar] 3d 94s 2 [Kr] 4d 95s 2 [Xe] 5d 96s 2 Experimental [Ar] 3d 54s 1 [Ar] 3d 104s 1 [Kr] 4d 105s 1 [Xe] 5d 106s 1 Exactly filled and exactly half-filled subshells have extra stability Promote one electron into ns orbital to gain this extra stability Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 8 Electron Cloud Heisenberg Uncertainty Principle • Can’t know both exact position and exact speed of subatomic particle simultaneously • Such measurements always have certain minimum uncertainty associated with them h Dx Dmv ³ 4p x = particle position mv = particle momentum = mass × velocity of particle h = Planck’s constant = 6.626 × 10–34 J s Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 9 Electron Cloud Heisenberg Uncertainty Principle Macroscopic scale • Errors in measurements much smaller than measured value Subatomic scale • Errors in measurements equal to or greater than measured value – If you know position exactly, know nothing about velocity – If you know velocity exactly, know nothing about position Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 10 Electron Cloud Heisenberg Uncertainty Principle: Consequences • Can’t talk about absolute position • Can only talk about electron probabilities – Where is e – likely to be? • ψ = wavefunction – Amplitude of electron wave • ψ2 = probability of finding electron at given location • Probability of finding an electron in given region of space equals the square of the amplitude of wave at that point Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 11 Orbitals Electron Cloud Electron dot picture = snapshots – Lots of dots shown by large amplitude of wave function • High probability of finding electrons Electron density – How much of electrons charge packed into given volume • High Probability – High electron density or Large electron density • Low Probability – Low electron density or Small electron density Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 12 Orbitals 1 s Orbital Representations a. Dot-density diagram b. Probability of finding electron around given point, ψ2, with respect to distance from nucleus c. Radial probability distribution = probability of finding electron between r and r + x from nucleus – rmax = Bohr radius Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 13 Orbitals Distribution of Electron Density • Determined by • Electron density Shape Size n Orientation m – No sharp boundary – Gradually fades away • “Shape” – Imaginary surface enclosing 90% of electron density of orbital – Probability of finding electrons is same everywhere on surface Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 14 Orbitals Effect of n on the s Orbital • In any given direction probability of finding electron same • All s orbitals are spherically shaped • Size increases as n increases 15 Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E Orbitals Spherical Nodes • At higher n, now have spherical nodes – Spherical regions of zero probability, inside orbital • Node for electron wave – Imaginary surface where electron density = 0 – 2s, one spherical node, size larger – 3s, two spherical nodes, size larger yet In general: • Number of spherical nodes =n–1 Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 16 Orbitals p Orbitals • Possess one nodal plane through nucleus – Electron density only on two sides of nucleus – Two lobes of electron density • All p orbitals have same overall shape – Size increases as n increases – For 3p have one spherical node Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 17 Orbitals p Orbitals • Constant probability surface for 2p orbital • Simplified p orbital emphasizing directional nature of orbital • All 2p orbitals in p sub shell – One points along each axis 2px 2py Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 2pz 18 Orbitals d Orbitals • Four with four lobes of electron density • One with two lobes and ring of electron density • Result of two nodal planes though nucleus • Number of nodal planes through nucleus = Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 19 Orbitals A. D. Ex: Identify Each Orbital C. B. E. z y x Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 20 Periodic Trends Periodic Properties To explain chemical & physical properties, must first consider amount of positive charge felt by outer electrons (valence electrons) • Core electrons spend most of their time closer to nucleus than valence (outer shell) electrons • Shield or cancel out (screen out, neutralize) some of positive charge of nucleus Effective Nuclear Charge (Zeff) • Net positive charge outer electron feels • Core electrons shield valence electrons from full nuclear charge Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 21 Periodic Trends Shielding • Electrons in same subshell don't shield each other – Same average distance from nucleus – Trying to stay away from each other – Spend very little time one below another • Effective nuclear charge determined primarily by – Difference between charge on nucleus (Z ) and charge on core (number of inner electrons) Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 22 Periodic Trends Atomic Size • Theory suggests sizes of atoms and ions indistinct • Experiment shows atoms/ions behave as if they have definite size – C and H have ~ same distance between nuclei in large number of compounds Atomic Radius (r) • Half of distance between two like atoms – H—H C—C etc. – Usually use units of picometer – 1 pm = 1 × 10–12 m – Range 37 – 270 pm for atoms Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 23 Periodic Trends Atomic Size Increases down Column (group) – Zeff essentially constant – n increases, outer electrons farther away from nucleus and radius increase Decreases across row (period) – n constant – Zeff decreases, outer electrons feel larger Zeff and radius decreases Transition Metals and Inner Transition Metals – Size variations less pronounced as filling core – n same (outer electrons) across row – Decrease in Zeff and r more gradually Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 24 Periodic Trends Atomic & Ionic Radii (in picometers) Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 25 Periodic Trends Ionic Radii • Increases down column (group) • Decreases across row (period) Anions larger than parent atom – Same Zeff, more electrons – Radius expands Cations smaller than parent atom – Same Zeff, less electrons, – Radius contracts Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 26 Periodic Trends • • • • Ionization Energy Energy required to remove electron from gas phase atom Corresponds to taking electron from n to n = First ionization energy M (g) M +(g) + e– IE = E Trends: • Ionization energy decreases down column (group) as n increases • Ionization energy increases across row (period) as Zeff increases Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 27 Periodic Trends First Ionization Energies Largest first ionization energies are in upper right Smallest first ionization energies are in lower left Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 28 Periodic Trends Successive Ionization Energies • Increases slowly as remove each successive electron • See big increase in ionization energy – When break into exactly filled or half filled subshell Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 29 Periodic Trends Successive Ionization Energies Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 30 Periodic Trends Electron Affinity (EA) • Potential energy change associated with addition of one electron to gas phase atom or ion in the ground state X(g) + e– X –(g) • O and F very favorable to add electrons • Comparing first electron affinities usually negative (exothermic) • Larger negative value means more favorable to add electron Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 31 Periodic Trends Electron Affinities Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 32 Periodic Trends Electron Affinity Trends • Electron affinity becomes less exothermic down column (group) as n increases – Electron harder to add as orbital farther from nucleus and feels less positive charge • Electron affinity becomes more exothermic across row (period) as Zeff increases • Easier to attract electrons as positive charge increases Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 33 Periodic Trends Successive Electron Affinities • Addition of first electron – often exothermic • Addition of more than one electron requires energy • Consider addition of electrons to oxygen: Change: EA(kJ/mol) O(g) + e – O–(g) –141 O–(g) + e – O2–(g) +844 Net: O(g) + 2e – O2–(g) +703 Jesperson, Brady, Hyslop. Chemistry: The Molecular Nature of Matter, 6E 34 Problem Set C