Heisenberg
Uncertainty Principle: imposs. to know both p (momentum) of e- and its location in space simultaneously
Quantum Mechanics
Schrodinger’s
wave eq.:
includes wave & particle behavior of e- (see handout)
Method
to determine probability region of e- around nucleus
Quantum Numbers:
|
n
|
principle
Q.N. (Energy level) 1,2,3,… |
|
l |
Azimuthal
Q.N.(sublevel) 0,
1, 2, …(n-1) 0
= s sublevel 1
= p 2
= d 3
= f |
|
ml |
Magnetic Q.N. (orbital,
orientation in space) - l ….+ l (2l +1) Tot
# orbitals in E level = n2 Tot
# e- in E level = 2 n2 |
|
ms |
Electron spin Q.N. +
˝ or – ˝ (↑↓) oppositely
directed magnetic field orientations |
Pauli
Exclusion princ.: no 2 e- can have same 4 Q.N. (orbital can
hold 2e- with opposite spins)
Aufbau
Princ.:
e- fill orbitals in order of increasing E
Hund’s
Rule:
lowest E is attained when e- have same spin in degenerate orbitals (Bus Seat
Rule)
degenerate orbitals: orbitals w/in same
sublevel, have equal E
Effective Nuclear Charge
e-
around nucleus
§
attracted
to nucleus
§
repelled
by ea. other
e-
of outer E levels not as attracted to nucleus as inner
E level e-
(Shielding/screening
effect)
Effective
Nuclear charge:
net positive charge attracting e- to nucleus
Zeff = Z – S
Z
= atomic number (# p+)
S
= avg. # e- between nucleus & e- of concern
*e-
repulsion causes dif E values of s, p, d, f sublevels
e- configurations
arrangement of e- around
nucleus
Core: e- in inner E levels