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Chapter 7: Quantum theory of the
atom
Chemistry 1061: Principles of Chemistry I
Andy Aspaas, Instructor
Atomic emission and line spectra
• When different compounds are burned, they give off surprisingly different colors of light
– It can be used to identify certain compounds
• If the emitted light is sent through a prism so the colors are separated, only certain discrete colors of light are given off (atomic line spectrum)
• The color of light can be related to the amount of energy that light contains
The wave nature of light
• Electromagnetic radiation: energy that is in the form of a wave, (visible light, x-rays, radio waves, etc)
• Wavelength, : distance between any two adjacent identical points of a wave
– Visible light, wavelength measured in nm– Radio waves can be measured in m
• Frequency, (nu): number of wavelengths that pass a fixed point in one unit of time (usu. 1 second)
Electromagnetic spectrum
Frequency and wavelength
• All electromagnetic waves travel at the speed of light, c = 3.00 x 108 m/s
• c = , if is in m, and is in sec-1
– Visible light wavelengths are always given in nm, between 400 and 800 nm
– Frequency is usually given in sec-1, or Hz
The particle nature of light
• While light has wave-like properties, it also has particle-like properties
• Photon: discreet particles of energy which make up light (or any electromagnetic radiation)
• The energy of one photon of light is related to the frequency of that lightE = h • (where h is Planck’s constant, 6.63x10-34 J·s)• This relates the wave-like and particle-like
properties of light
More about atomic line spectra
• Heated solid metals emit light of all wavelengths, or a continuous spectrum
– Would form a rainbow if sent through a prism
• Heated gases emit light of only particular wavelengths, or a line spectrum
– Would form only lines of particular colors if sent through a prism
– These lines are associated with energy level transitions
Energy levels
• Electrons can have only specific energy values in an atom (energy levels)
– Energy levels are quantized (only specific allowed values)
• When an electron absorbs energy from the environment, it can be promoted to a higher energy level
• In order for it to return to a lower level, energy must be released in the form of a single photon
– Depending on which levels this transition involves, the photon will have a different amount of energy
H atom energy level calculations
• Energy levels are numbered with integers starting with 1, symbol is n
n = 1, 2, 3, …• The energy of a particular level is given by
E = -(RH) / (n2) where RH = 2.179 x 10-18 J
• The energy of a photon given off can be calculated by subtracting the lower energy level from the higher energy level (energy of a photon is positive)
Quantum mechanics
• Just like light can be wave-like and particle-like, so can electrons
• The most accurate description of an electron’s behavior is using a wave-like interpretation, this is known as quantum mechanics
• An electron can be described by a wavefunction – an equation for the wave that represents an electron
• Only the probability of an electron appearing in a certain place can be calculated
– Heisenberg uncertainty principle says the more precisely you know the position of a small particle, the less precisely you know its momentum
Atomic orbitals
• The 3-dimensional space in which there is a high probability of finding an electron in an atom is referred to as an atomic orbital
• Can be described by three quantum numbers
– Principal quantum number, n: refers to the energy of an electron, it also associates with the size of an orbital (n = 1, 2, 3, 4,…)
Atomic orbitals
• Angular momentum quantum number, l: indicates shape of orbital (l = 0, 1, 2, 3, …. n-1)
– Usually shown by letters: s, p, d, f, and g
• Magnetic quantum number, ml: Distinguishes orbitals of same shape but different position (ml = integers from –l to +l)
• Spin quantum number, ms: indicates which of 2 possible spin states an electron is in, equal to either -1/2 or +1/2
Permissible atomic orbitals for n = 1, 2, 3
n l mlNotation # orbitals
1 0 0 1s 1
2 0 0 2s 1
2 1 -1, 0, +1 2p 3
3 0 0 3s 1
3 1 -1, 0, +1 3p 3
3 2 -2, -1, 0, +1, +2 3d 5
Atomic orbital shapes