The Electron
Electron, is lightest stable subatomic particle known. It carries a negative charge of
1.602176634 × 10−19 coulomb, which is considered the basic unit of electric charge. The rest mass of the electron is
9.1093837015 × 10−31 kg, which is only 1/1,836the
mass of a proton. An electron is therefore considered
nearly mass-less in comparison with a proton or a neutron, and the electron mass is not included in
calculating the mass
number of an atom.
During the 1870s, the English chemist
and physicist Sir William
Crookes developed the first
cathode ray tube to have a high
vacuum inside. He then showed
in 1874 that the cathode rays can turn a small paddle wheel when placed in
their path. Therefore, he concluded that the rays carried momentum.
Furthermore, by applying a magnetic field, he was able to deflect the rays,
thereby demonstrating that the beam behaved as though it were negatively
charged.
The German-born British physicist Arthur Schuster expanded upon Crookes' experiments by
placing metal plates parallel to the cathode rays and applying an electric potential between the plates. The field deflected
the rays toward the positively charged plate, providing further evidence that
the rays carried negative charge.
In 1897, the British physicist J. J. Thomson, with his colleagues John S. Townsend and H. A. Wilson, performed experiments indicating that
cathode rays really were unique particles, rather than waves, atoms or
molecules as was believed earlier. Thomson made good estimates of both the
charge e and the mass m, finding that cathode ray particles,
which he called "corpuscles," had perhaps one thousandth of the mass
of the least massive ion known: hydrogen. He showed that their charge-to-mass
ratio, e/m, was independent of cathode material.
The electron's charge was more carefully
measured by the American physicists Robert Millikan and Harvey Fletcher in their oil-drop experiment of 1909, the results of which were
published in 1911.
By 1914, experiments by physicists Ernest Rutherford, Henry Moseley, James Franck and Gustav Hertz had largely established the structure of an atom as a dense nucleus of
positive charge surrounded by lower-mass electrons. In 1913, Danish physicist Niels Bohr postulated that electrons resided in
quantized energy states, with their energies determined by the angular momentum
of the electron's orbit about the nucleus. The electrons could move between
those states, or orbits, by the emission or absorption of photons of specific
frequencies. By means of these quantized orbits, he accurately explained the spectral lines of the hydrogen atom.
Chemical bonds between atoms were
explained by Gilbert
Newton Lewis, who in 1916
proposed that a covalent
bond between two atoms is
maintained by a pair of electrons shared between them
In 1927 George Paget Thomson, discovered the interference effect was
produced when a beam of electrons was passed through thin metal foils and by
American physicists Clinton Davisson and Lester Germer by the reflection of electrons from a
crystal of nickel.
Louis de Broglie hypothesized that under the appropriate
conditions, electrons and other matter would show properties of either
particles or waves.
De Broglie's prediction of a wave nature
for electrons led Erwin Schrödinger to postulate a wave equation for
electrons moving under the influence of the nucleus in the atom. In 1926, this
equation, the Schrödinger
equation, successfully
described how electron waves propagated.
Solutions of Schrödinger's equation, like
Heisenberg's, provided derivations of the energy states of an electron in a
hydrogen atom that were equivalent to those that had been derived first by Bohr
in 1913, and that were known to reproduce the hydrogen spectrum.
The wave-like behavior of a bound
electron is described by a function called an atomic orbital.
Each orbital has its own set of quantum numbers such as energy, angular
momentum and projection of angular momentum, and only a discrete set of these
orbitals exist around the nucleus. According to the Pauli exclusion principle
each orbital can be occupied by up to two electrons, which must differ in their
spin quantum number.
Electrons can transfer between different
orbitals by the emission or absorption of photons with an energy that matches
the difference in potential. Other methods of orbital transfer include
collisions with particles, such as electrons, and the Auger
effect. To escape the
atom, the energy of the electron must be increased above its binding energy
to the atom. This occurs, for example, with the photoelectric effect, where an incident photon exceeding the atom's ionization energy
is absorbed by the electron.
The chemical bond
between atoms occurs as a result of electromagnetic interactions, as described
by the laws of quantum mechanics. The strongest bonds are formed by the sharing or transfer of
electrons between atoms, allowing the formation of molecules. Within a molecule, electrons move
under the influence of several nuclei, and occupy molecular orbitals;
much as they can occupy atomic orbitals in isolated atoms. A fundamental factor
in these molecular structures is the existence of electron pairs.
These are electrons with opposed spins, allowing them to occupy the same
molecular orbital without violating the Pauli exclusion principle (much like in
atoms). Different molecular orbitals have different spatial distribution of the
electron density. For instance, in bonded pairs (i.e. in the pairs that
actually bind atoms together) electrons can be found with the maximal
probability in a relatively small volume between the nuclei. By contrast, in
non-bonded pairs electrons are distributed in a large volume around nuclei.
Since an electron has charge, it has a
surrounding electric field, and if that electron is moving relative to an observer,
said observer will observe it to generate a magnetic field.
Electromagnetic fields produced from other sources will affect the motion of an
electron according to the Lorentz force law.
Electrons radiate or absorb energy in the form of photons when they are accelerated.
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