Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

28
Chapter 7: Atoms and Light

Transcript of Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Page 1: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Chapter 7:

Atoms and Light

Page 2: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Low ν

High ν

Electromagnetic Radiation

Page 3: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

WMHB broadcasts at 89.7 on the FM dial (89.7 MHz). What is the wavelength of the emitted radio waves?

Page 4: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

The AM dial ranges from 500-1800 kHz. What wavelengths does this represent?

A microwave oven (2.4 GHz)?

Page 5: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Electromagnetic Spectrum

Page 6: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Constructive and Destructive Interference

Page 7: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Atomic Spectra

PotassiumHydrogen Helium Lithium Sodium

Page 8: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Atomic Spectra

Page 9: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

The Hydrogen Atomic Spectrum

Page 10: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Quantum Theory (Blackbody Radiation)

Max Planck: E = hν

Page 11: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

The energy required to break a carbon-carbon bond is approximately 360 KJ/mol. What wavelength of electro-magnetic radiation can supply this amount of energy?

Page 12: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

The Photoelectric Effect

• Heinrich Hertz (1888) discovered that light striking the surface of certain metals causes ejection of electrons - the photoelectric effect.

• Electrons were only ejected if the frequency of the light () was above a certain threshold frequency (o)

• The number of electrons ejected were proportional to the intensity of the light

• The velocity (kinetic energy) of the electrons ejected was proportional to the frequency of the light

• Einstein used Planck’s ideas to explain the photoelectric effect:

ΔE = hν-hνo

Page 13: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Emission and Absorption Spectroscopy

Page 14: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

The Bohr Atom

Page 15: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Hydrogen Energy Levels

Page 16: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

A New Quantum Mechanics

Page 17: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

The Heisenberg Uncertainty Principle

Δx Δp ≥ h

Page 18: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Standing Waves

2Ln

= n = 1, 2, 3…

In a standing wave, the nodes remain at a constant position.

Page 19: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Standing Waves

Shrodinger suggested that electrons can be described as standing waves orbiting the nucleus, and used a mathematical equation to represent these waves.

Page 20: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

The Schrodinger Equation: Wave Functions

Ψ (psi), the wave function.Corresponds to a standing wave within

the boundary of the system being described.

The energy of the standing wave increases as we add more nodes.

Page 21: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Probability of Finding an Electron

Page 22: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Quantum Numbers

By using three different quantum numbers, we can describe the wavefunction of any electron in an atom.

n : the principle quantum numberDesignates electronic shell (distance from nucleus), n = 1, 2, 3…

[It also corresponds to the number of radial nodes]

l : The angular momentum quantum numberDesignates the shape of the orbital, l = 0, 1, 2…(n-1)

ml : The magnetic quantum number

Describes the orientation of the orbital; ml = - l …-2, -1, 0, 1, 2…+l

Page 23: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

l = 0, the “s” orbitals

Page 24: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

l = 1, the “p” orbitals

Page 25: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

ml for the “p” orbitals

Page 26: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

l = 2, the “d” orbitals

Page 27: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

Orbital Occupancy

Each orbital (described by 3 quantum numbers) can contain two electrons.

No two electrons can have the same set of quantum numbers.

Therefore…

Page 28: Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.

The Fourth Quantum Number, s

Electrons have a spin of either +1/2 or –1/2. Electrons that occupy the same orbital must have opposite spins.