lecture 15: the hydrogen atom
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Lecture 15: The Hydrogen Atom . J.J. Thomson’s Plum Pudding Model of the Atom (1897). He proposed that the electrons are embedded in a positively charged ‘pudding’. Rutherford’s a Scattering Experiment (1911). - PowerPoint PPT PresentationTRANSCRIPT
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Lecture 15: The Hydrogen Atom
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J.J. Thomson’s Plum Pudding Model of the Atom (1897)
He proposed that the electrons are embedded in a positively charged ‘pudding’
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Rutherford’s Scattering Experiment (1911)
He found that, once in a while, the -particles were scattered backwards by the target
video clip
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Discovery of the Atomic Nucleus
To explain the backscattering, the positive charge must be concentrated in a small region
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Rutherford’s Solar System Model of the Atom
The atom consists of electrons orbiting around a small but dense central nucleus
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Hydrogen Atom is Unstable?
It is known that accelerating charges emit radiation
Thus, electron should emit radiation, lose energy and eventually fall into the nucleus!
Why doesn’t this happen? Shows that something was wrong with this model of the hydrogen atom
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Absorption Spectrum of a Gas
Dark lines will appear in the light spectrum
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Absorption spectrum of Sun
Emission spectra of various elements
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Balmer’s Formula for Hydrogen
Notice there are four bright lines in the hydrogen emission spectrum
Balmer guessed the following formula for the wavelength of these four lines:
where n = 3, 4, 5 and 6
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Bohr’s Model of the Hydrogen Atom(1913)
He proposed that only certain orbits for the electron are allowed
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Bohr’s Empirical Explanation
Electrons can only take discrete energies (energy is related to radius of the orbit)
Electrons can jump between different orbitsdue to the absorption or emission of photons
Dark lines in the absorption spectra are due to photons being absorbed
Bright lines in the emission spectra are due to photons being emitted
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Absorption / Emission of Photonsand Conservation of Energy
Ef - Ei = hf Ei - Ef = hf
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Energy Levels of Hydrogen
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Electron jumping to a higher energy level
E = 12.08 eV
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Spectrum of Hydrogen
Bohr’s formula:
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Hydrogen is therefore a fussy absorber / emitter of light
It only absorbs or emits photons with precisely the right energies dictated by energy conservation
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This explains why some nebulae are red or pink in colour
One of the transitions in the Balmer seriescorresponds to the emission of red light
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Schrödinger’s Improvement to Bohr’s Model
Showed how to obtain Bohr’s formula using the Schrödinger equation
Electron is described by a wave function
Solved for in the electric potential due to the nucleus of the hydrogen atom
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Square Well
Approximate electric (roller coaster) potential by a ‘square well’
System is then identical to the wave equation for a string that is fixed at both ends
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Vibrational Modes of a String
fundamental 2nd harmonic 3rd harmonic 4th harmonic
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Energy Levels in a Box
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Quantum Numbers
Energy levels can only take discrete values
Labelled by a ‘quantum number’ n, which takes values 1, 2, 3, ...
Each level has energy that increases with n
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Ground State (n=1)
Lowest or ground-state energy is non-zero
Electron cannot sit still but must be forever ‘jiggling around’
Expected from the Heisenberg uncertainty principle
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Vibrational Modes of a Rectangular Membrane
(1,1) mode (1,2) mode (2,1) mode (2,2) mode
Vibrational modes of a circular membrane (drum)
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Electron in a Hydrogen Atom
Wave function is like a vibrating string or membrane, but the vibration is in three dimensions
Labelled by three quantum numbers:– n = 1, 2, 3, …– ℓ = 0, 1, …, n-1– m = -ℓ, -ℓ+1, …, ℓ-1, ℓ
For historical reasons, ℓ = 0, 1, 2, 3 is also known as s, p, d, f
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1s Orbital
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Density of the cloud gives probability of where the electron is located
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2s and 2p Orbitals
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Another diagram of 2p orbitals
Note that there are three different configurations corresponding to m = -1, 0, 1
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3d Orbitals
Now there are five different configurations corresponding to m = -2, -1, 0, 1, 2
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4f Orbitals
There are seven different configurations corresponding to m = -3, -2, -1, 0, 1, 2, 3
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Summary
Electron does not fly round the nucleus like the Earth around the Sun (Rutherford, Bohr)
Depending on which energy level it is in, the electron can take one of a number of stationary probability cloud configurations (Schrödinger)