1010 - de Broglie Hypothesis |
1010 - Relate the Davison-Thomson double slit experiment, explain its observations. |
1020 - Explain de Broglies hypothesis, explain how an electron can have wave properties. |
1030 - Relate and apply de Broglies equation for wave length of particles. |
1040 - Know the complementarity of position and velocity through Heisenbergs equation. |
1050 - Know the similarities and differences in classical and quantum-mechanical concepts of trajectory. |
1060 - Differentiate between deterministic and indeterminacy. |
1020 - Schrodingers Equation |
1010 - Define orbital and wave function. |
1020 - Know the Schrodinger equation is how we calculate energies and orbitals for electrons in atoms. |
1030 - Know the properties and allowed values of the principal quantum number, n. |
1040 - Know the properties, values, and letter designations of the angular momentum quantum number, l. |
1050 - Know the properties and allowed values of the magnetic quantum number, ml. |
1060 - Know and understand how atomic spectroscopy defines the energy levels of electrons in the hydrogen atom. |
1070 - Calculate the energies and wavelengths of emitted and absorbed photons for hydrogen. |
1030 - Atomic Orbitals |
1010 - Define probability density and radial distribution function. |
1020 - Define and understand nodes. |
1030 - Identify the number of nodes in a radial distribution function for an s orbital. |
1040 - Know the shapes of s, p, d, and f orbitals and the relationships to quantum numbers. |
1050 - Know that the shape of an atom is dictated by the combined shapes of the collection of orbitals for that atom. |
1060 - Given a value of the principle quantum number, show the designations of all possible sub-shells. |
1070 - Recognize the orbital shapes associated with each energy level and sublevel. |
1080 - Be able to draw the relative orbital shape and size for s and p orbitals. |
1090 - Define and understand phase. |