Download presentation
Presentation is loading. Please wait.
Published byDelphia Richardson Modified over 9 years ago
1
I II III Suggested Reading Pages 104 - 110 Section 4-2 Quantum Theory
2
Came about because classical physics couldn’t explain everything. Why does a metal emit invisible radiation first (IR – heat) and then glow red, and then yellow, and then white? Quantum Theory
3
Quantum Mechanics
4
Heisenberg’s Uncertainty Principle There is a limit to just how precisely we can know both the position and velocity of a particle at a given time.
5
Diffraction: The bending of a wave as it passes by the edge of an object or through a small opening. de Broglie – electrons have wave-like properties. Interference: occurs when waves overlap.
6
Regions around the nucleus of an atom where an electron with a given energy is likely to be found. Atomic Orbital's (electron clouds)
7
Quantum Numbers Describe orbital's and electrons in them 1 st Quantum # = main energy level (n) 2 nd Quantum # = shape ( l ) 3 rd Quantum # = which way it’s pointing(m l ) 4 th Quantum # = which way it’s spinning(m s )
8
principal quantum number “n” Main Energy Level Higher “n” = more energy = farther from nucleus
9
Angular momentum quantum number “ ” Has to be lower than 1 st quantum # Indicates shape = 0 s shaped contains 1 orbit = 1p shaped contains 3 orbits = 2d shaped contains 5 orbits = 3f shaped contains 7 orbits
10
s orbitals Shapes of Orbitals
11
p orbitals Shapes of Orbitals
12
d orbitals Shapes of Orbitals
13
f orbitals Shapes of Orbitals
14
Magnetic quantum number “m ” Tells which way it’s pointed
15
Possible Values of m s = 0 p = -1, 0, +1 d = -2, -1, 0, +1, +2 f = -3, -2, -1, 0, +1, +2, +3
16
Spin quantum numbers m s Represented with up or down arrow Can only be +½ (pointed up) or -½ (pointed down)
18
The rule states that no two electrons may ever have the same four quantum numbers. Pauli exclusion principle
19
4 Minute Review
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.