Consider 3 approaches:
Classical
Bohr Model (old quantum theory)
Full Quantum: Schrödinger Equation
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Classically:
There is no theoretical restriction at all on v or r (there are infinitely many combinations with the same energy).
Hence the energy can take any value - it is
.
As a result transitions should be possible everywhere across the electromagnetic spectrum.
So lets see the spectrum .
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The H-atom Emission Spectrum
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Principles of Quantum Mechanics Quantization
Energy levels
Slide 13
In 1890 Rydberg showed that the frequencies
of all transitions could be fit by a single equation:
Revision
Slide 14
Bohr explained the observed frequencies by restricting the allowed orbits the electron could occupy to particular circular orbits(by quantizing the angular momentum).
His theory gives energy levels:
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Bohr theory works extremely well for the H-atom.
However;
it provides no explanation for the quantization of energy -it just happens to fit the observed spectrum
But, more seriously:
it just doesn’t work at all for any other atoms
Slide 16
Slide 17
Principles of Quantum Mechanics Quantization
Energy levels
Quantum mechanics
Classical mechanics
is continuous
Slide 18
Principles of Quantum Mechanics It’s all about probability
In classical mechanics
Position of object specified
In quantum mechanics
Only
of object at a particular location
Slide 19
Principles of Quantum Mechanics How do we describe the electrons in atoms?
You know: Electrons can be described as
(characterised by mass, momentum, position…)
p = h/l
De Broglie
e-
h = Planck’s constant = 6.626 10-34 Js
However: Electrons can also be described as
(characterised by wavelength, frequency, amplitude)