The Rutherford Bohr model of
the hydrogen atom.
From Wikipedia, the free encyclopedia
The Atomic Orbital Model is the currently accepted model of the electrons in an atom. It is
sometimes called the Wave Mechanics Model. In the atomic orbital model, the atom consists of
a nucleus surrounded by orbiting electrons.These electrons exist in atomic orbitals, which are a
set of quantum states of the negatively charged electrons trapped in the electrical field generated
by the positively charged nucleus. Classically, the orbits can be likened to the planets orbiting
the sun. However, the atomic orbital model can only be described by quantum mechanics, in
which case the electrons are more accurately described as standing waves surrounding the
nucleus.
1 Historical context
2 Current theory
2.1 Wave-like properties
2.2 Particle-like properties
2.3 Describing the electrons
2.4 Predictions of the model
3 See also
4 External links
Main article: Atomic theory
After the discovery of the photoelectric effect, the connection
between the structure of electrons in atoms and the emission
and absorption spectra of atoms became an increasingly
useful tool in the understanding of electrons in atoms. The
most prominent feature of emission and absorption spectra
was that these spectra contained discrete lines. The
significance of the Bohr model was that it related the lines in
emission and absorption spectra to the energy differences
between the orbits that electrons could take around an atom.
This was achieved by giving the electrons some kind of
wave-like properties. In particular, electrons were assumed to
have a wavelength (a property that had previously been
discovered, but not entirely understood). The Bohr model was
therefore not only a significant step towards the
understanding of electrons in atoms, but also a significant step towards the development of the
wave/particle duality of quantum mechanics.
The premise of the model was that electrons had a wavelength, which was a function of its
momentum, and therefore an orbiting electron would need to orbit at a multiple of the
wavelength. The Bohr model was thus a classical model with an additional constraint provided by
the 'wavelength' argument. In our current understanding of physics, this 'wavelength' argument is
known to be an element of quantum mechanics, and for that reason the Bohr model is called a
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Electron atomic and molecular orbitals. The chart of
orbitals (left) is arranged by increasing energy (see
Madelung rule). Note that atomic orbits are
functions of three variables (two angles, and the
distance from the nucleus, r). These images are
faithful to the angular component of the orbital, but
not entirely representative of the orbital as a whole.
semi-classical model.
The Bohr model was able to explain the emission and absorption spectra of Hydrogen. The
energies of electrons in the n=1, 2, 3, etc. states in the Bohr model match those of current
physics. However, this did not explain similarities between different atoms, as expressed by the
periodic table, such as why Helium (2 electrons), Neon (10 electrons), and Argon (18 electrons)
exhibits similar chemical behaviour. Modern physics explains this by noting that the n=1 state can
hold 2 electrons, the n=2 state can hold 8 electrons, and the n=3 state can hold 8 electrons. In
the end, this was solved by the discovery of modern quantum mechanics and the Pauli Exclusion
Principle.
With the development of quantum
mechanics, it was found that the orbiting
electrons around a nucleus could not be
fully described as particles, but needed to
be explained by the wave-particle duality. In
this sense, the electrons have the following
properties:
Wave-like properties
The electrons do not orbit the nucleus in
the sense of a planet orbiting the sun, but
instead exist as standing waves. The lowest
possible energy an electron can take is
therefore analogous to the fundamental
frequency of a wave on a string. Higher
energy states are then similar to harmonics
of the fundamental frequency.
The electrons are never in a single point
location, although the probability of
interacting with the electron at a single point can be found from the wavefunction of the electron.
Particle-like properties
There is always an integer number of electrons orbiting the nucleus.
Electrons jump between orbitals in a particle-like fashion. For example, if a single photon strikes
the electrons, only a single electron changes states in response to the photon.
The electrons retain particle like-properties such as: each wave state has the same electrical
charge as the electron particle. Each wave state has a single discrete spin (spin up or spin
down).
Describing the electrons
Because the electrons around a nucleus exist as a wave-particle duality, they cannot be
described by a location and momentum. Instead, they are described by a set of quantum
numbers that encompasses both the particle-like nature and the wave-like nature of the
electrons. Each set of quantum numbers corresponds to a wavefunction. The quantum numbers
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are:
The principal quantum number, n, is analogous to the harmonic of the electrons. That is, the n=1
states are analogous to the fundamental frequency of a wave on a string, and the n=2 states are
analogous to the first harmonic, etc.
The azimuthal quantum number, l, describes the orbital angular momentum of each electron.
Note that this has no classical analog. The number l is an integer between 0 and (n - 1).
The magnetic quantum number, ml, describes the magnetic moment of an electron in an arbitrary
direction. The number ml is an integer between -l and l.
The spin quantum number, s, describes the spin of each electron (spin up or spin down). The
number s can be +1⁄2 or -1⁄2.
These quantum numbers can only be determined by a full quantum mechanical analysis of the
atom. There is no way to describe them using classical physical principles. A more technical
analysis of these quantum numbers and how they are derived is given in the atomic orbital article.
Furthermore, the Pauli Exclusion Principle states that no two electrons can occupy the same
quantum state. That is, every electron that is orbiting the same nucleus must have a unique
combination of quantum numbers.
Predictions of the model
Under quantum mechanics, each quantum state has a well-defined energy. When applied to
atomic orbitals, this means that each state has a specific energy, and that if an electron is to
move between states, the energy difference is also very fixed.
Consider two states of the Hydrogen atom:
State 1) n=1, l=0, ml=0 and s=+1⁄2
State 2) n=2, l=0, ml=0 and s=+1⁄2
By quantum theory, state 1 has a fixed energy of E1, and state 2 has a fixed energy of E2. Now,
what would happen if an electron in state 1 were to move to state 2? For this to happen, the
electron would need to gain an energy of exactly E2 - E1. If the electron receives energy that is
less than or greater than this value, it cannot jump from state 1 to state 2. Now, suppose we
irradiate the atom with a broad-spectrum of light. Photons that reach the atom that have an
energy of exactly E2 - E1 will be absorbed by the electron in state 1, and that electron will jump to
state 2. However, photons that are greater or lower in energy cannot be absorbed by the electron,
because the electron can only jump to one of the orbitals, it cannot jump to a state between
orbitals. The result is that only photons of a specific frequency will be absorbed by the atom. This
creates a line in the spectrum, known as an absorption line, which corresponds to the energy
difference between states 1 and 2.
The atomic orbital model thus predicts line spectra, which are observed experimentally. This is
one of the main validations of the atomic orbital model.
The atomic orbital model is nevertheless an approximation to the full quantum theory, which only
recognizes many electron states. The predictions of line spectra are qualitatively useful but are
not quantitatively accurate for atoms and ions other than those containing only one electron.
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Atomic orbital — Details of how atomic orbitals are characterized, and approximations used
to calculate them.
Molecular orbital — Details on the structure of electrons in compounds.
quantum chemistry — Study of how chemical bonds are formed by orbital electrons to form
molecules.
Solid state physics and condensed matter physics — Study of electrons in crystalline
materials.
Bonding in Organic Molecules. Atomic-Orbital Models (http://caltechbook.library.caltech.edu
/122/7/BPOCchapter6.pdf) PDF (1.2MB)
Retrieved from "http://en.wikipedia.org/wiki/Atomic_orbital_model"
Categories: Atomic physics
This page was last modified on 14 November 2010 at 02:51.
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