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Quantum Mechanical Model and Electronic Structure of Atoms

Learn about the quantum mechanical model of atoms and the electronic structure, including the wave nature of light, line spectra, ionization, quantized energy, photons, and atomic orbitals.

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Quantum Mechanical Model and Electronic Structure of Atoms

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  1. Chapters 7 & 8 Quantum Mechanical Model; Electronic Structure of the Atoms & Periodic Trends

  2. Definitions • Atoms - smallest particles of matter • Matter - has mass, volume and specific position • Energy - no mass; a wave function; delocalized

  3. Einstein’s Contribution • Energy is related to mass as seen in the equation: E = mc2

  4. Law of Conservation of Energy • Energy can never be destroyed. It can only be converted from one form to another.

  5. Forms of Energy • Electromagnetic radiation wavelength, frequency and speed • Light • Heat

  6. Electromagnetic Spectrum • Radio Waves • Microwaves, Radar Rays • Infrared • Visible • UV • X-rays • Gamma Rays

  7. The Wave Nature of Light

  8. The Wave Nature of Light

  9. Chemistry in Color • Specific elements gave color when heated in flame. • Continuous spectrum - e.g., rainbow • Line Spectrum

  10. Line Spectra • Held the key to the structure of the atom!

  11. The Bohr Atom • Bohr:suggested that electrons were responsible for the line spectra. Proposed that electrons traveled around the nucleus of the atom in shells

  12. The Bohr Atom • Bohr:associated each shell w/ a particular energy level. The farther away, the higher the Energy. Allowed electrons to jump from one shell to another. (ground state excited state)

  13. Comparison • Bohr Model similar to model for solar system where the planets revolve in their particular orbits. • Difference: Electrons can jump from one shell to another. The planets do not!

  14. Ionization • An electron can absorb so much energy that it can jump completely from the atom!

  15. Quantized Energy and Photons The Photoelectric Effect and Photons • If light shines on the surface of a metal, there is a point at which electrons are ejected from the metal. • The electrons will only be ejected once the threshold frequency is reached. • Below the threshold frequency, no electrons are ejected. • Above the threshold frequency, the number of electrons ejected depend on the intensity of the light.

  16. Matter and Energy • Matter and Energy are not distinct! • Proof: Matter can absorb or emit energy. • Max Planck’s Postulate: Energy can be gained or lost only in whole numbers or integer multiples, hn.

  17. Wrong assumption • Matter was assumed to transfer any amount of energy because E was continuous.

  18. Quantum • E can be quantized or delivered in small packets of size hn, called a Quantum. • Quanta = photon

  19. Quantum Mechanical Model • De Broglie and Schroedinger • Corrected Bohr’s model • determined that E had wave properties and mass

  20. Quantum Mechanical Model • re-evaluated electron as occupying volume of space instead of shells that were like orbits. • Orbital - volume of space occupied by an electron

  21. Quantum Mechanics and Atomic Orbitals If we solve the Schrödinger equation, we get wave functions and energies for the wave functions. • We call wave functions orbitals. • Orbitals were located in levels.

  22. Quantum Mechanical Model • De Broglie and Schroedinger • Corrected Bohr’s model • determined that E had wave properties and mass

  23. Quantum Mechanical Model • re-evaluated electron as occupying volume of space instead of shells that were like orbits. • Orbital - volume of space occupied by an electron

  24. Quantum Mechanics and Atomic Orbitals If we solve the Schrödinger equation, we get wave functions and energies for the wave functions. • We call wave functions orbitals.

  25. Principal Quantum Number, n • Schrödinger’s equation requires 4 quantum numbers: • Principal Quantum Number, n. This is the same as Bohr’s n. As n becomes larger, the atom becomes larger and the electron is further from the nucleus. N refers to the shell.

  26. Azimuthal Quantum Number, l. • This quantum number depends on the value of n. The values of l begin at 0 and increase to (n - 1). We usually use letters for l (s, p, d and f for l = 0, 1, 2, and 3). Usually we refer to the s, p, d and f-orbitals.

  27. Representations of Orbitals The s-Orbitals

  28. Representations of Orbitals

  29. Representations of Orbitals The p-Orbitals

  30. Magnetic Quantum Number, ml. 3. This quantum number depends on l. The magnetic quantum number has integral values between -l and +l. Magnetic quantum numbers give the 3D orientation of each orbital.

  31. Shape of Orbitals • s - sphere • p - dumbbell • d - double dumbbell

  32. Representations of Orbitals The p-Orbitals • There are three p-orbitals px, py, and pz. • The three p-orbitals lie along the x-, y- and z- axes of a Cartesian system. • The letters correspond to allowed values of ml of -1, 0, and +1. • The orbitals are dumbbell shaped. • As n increases, the p-orbitals get larger. • All p-orbitals have a node at the nucleus.

  33. Representations of Orbitals The p-Orbitals

  34. Representations of Orbitals The d and f-Orbitals • There are five d and seven f-orbitals. • Three of the d-orbitals lie in a plane bisecting the x-, y- and z-axes. • Two of the d-orbitals lie in a plane aligned along the x-, y- and z-axes. • Four of the d-orbitals have four lobes each. • One d-orbital has two lobes and a collar.

  35. Pauli Exclusion Principle • An orbital with a particular orientation can only hold 2 electrons and they must have opposite spins! In short, NO 2 electrons can have the same 4 quantum numbers. • Example: px, py, pz

  36. Rules for Occupancy and Pairing • Opposite spins pair up. • Hund’s Rule: For the same sublevel, each orbital must be occupied singly before pairing can occur. This is the lowest E for an atom configuration.

  37. Heisenberg Uncertainty Principle • “There is a fundamental limitation as to how precisely we can determine the position and momentum of a particle at a given time.” • 90-95% probability of finding the electron in the orbital

  38. Magnetic Spin Quantum Number, ms • Gives insight into the spin of the electron • 2 Possible Values: ½ and – ½

  39. Many-Electron Atoms Orbitals and Their Energies • Orbitals of the same energy are said to be degenerate. • For n 2, the s- and p-orbitals are no longer degenerate because the electrons interact with each other. • Therefore, the Aufbau diagram looks slightly different for many-electron systems.

  40. Energy Levels • The electrons are found at a certain distance from nucleus in their shell(s). • energy level = shell (interchangeable terms) • Electrons in the same shell have the same E.

  41. Heisenberg Uncertainty Principle • “There is a fundamental limitation as to how precisely we can determine the position and momentum of a particle at a given time.” • 90-95% probability of finding the electron in the orbital

  42. Shorthand Notation • Uses the closest noble gas before the given element to represent the inner electrons. • Al = 13 electrons 1s2 2s2 2p6 3s2 3p1 • Shorthand Notation: [Ne] 3s2 3p1 • Neon represents the 10 inner electrons

  43. Periodicity • Valence electrons determined the position of the atoms in the periodic table and predicted the reactivity of the elements.

  44. Periodic Table • Organized according to Electronic Configuration of elements • Based on the Aufbau Principle of building up the number of electrons and protons

  45. Definitions • Core Electrons - inner electrons • Valence Electrons - electrons on the outermost energy level of an atom

  46. Valence Electrons • Are the electrons in the outermost shell • Determines the group where the element belongs in the periodic table. • For ex., 1s22s22p3 = element belongs to Grp V. Outermost level is 2. Add the electrons in 2s and 2p orbitals.

  47. Sample Problem • What is the largest principal quantum number in the ground state electron configuration of iodine ?

  48. Sample Problem • What is the azimuthal quantum number for the orbitals being filled in the Lanthanide series?

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