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Electric Energy and Potential



Potential energy

In discussing gravitational potential energy in PY105, we usually
associated it with a single object. An object near the surface of the
Earth has a potential energy because of its gravitational interaction
with the Earth; potential energy is really not associated with a single
object, it comes from an interaction between objects.

Similarly, there is an electric potential energy associated with
interacting charges. For each pair of interacting charges, the
potential energy is given by:

electric potential energy: PE = k q Q / r

Energy is a scalar, not a vector. To find the total electric potential
energy associated with a set of charges, simply add up the energy
(which may be positive or negative) associated with each pair of

An object near the surface of the Earth experiences a nearly uniform
gravitational field with a magnitude of g; its gravitational potential
energy is mgh. A charge in a uniform electric field E has an electric
potential energy which is given by qEd, where d is the distance moved
along (or opposite to) the direction of the field. If the charge moves
in the same direction as the force it experiences, it is losing
potential energy; if it moves opposite to the direction of the force,
it is gaining potential energy.

The relationship between work, kinetic energy, and potential energy, which was discussed in PY105, still applies:

An example

Two positively-charged balls are tied together by a string. One ball
has a mass of 30 g and a charge of 1 ; the other has a mass of 40 g and
a charge of 2 . The distance between them is 5 cm. The ball with the smaller charge
has a mass of 30 g; the other ball has a mass of 40 g. Initially they
are at rest, but when the string is cut they move apart. When they are
a long way away from each other, how fast are they going?

Let's start by looking at energy. No external forces act on this
system of two charges, so the energy must be conserved. To start with
all the energy is potential energy; this will be converted into kinetic

Energy at the start : KE = 0

PE = k q Q / r = (8.99 x 109) (1 x 10-6) (2 x 10-6) / 0.05 = 0.3596 J

When the balls are very far apart, the r in the equation for
potential energy will be large, making the potential energy negligibly

Energy is conserved, so the kinetic energy at the end is equal to the potential energy at the start:

The masses are known, but the two velocities are not. To solve for the
velocities, we need another relationship between them. Because no
external forces act on the system, momentum will also be conserved.
Before the string is cut, the momentum is zero, so the momentum has to
be zero all the way along. The momentum of one ball must be equal and
opposite to the momentum of the other, so:

Plugging this into the energy equation gives:

Electric potential

Electric potential is more commonly known as voltage. The potential at a point a distance r from a charge Q is given by:

V = k Q / r

Potential plays the same role for charge that pressure does for fluids.
If there is a pressure difference between two ends of a pipe filled
with fluid, the fluid will flow from the high pressure end towards the
lower pressure end. Charges respond to differences in potential in a
similar way.

Electric potential is a measure of the potential energy per unit
charge. If you know the potential at a point, and you then place a
charge at that point, the potential energy associated with that charge
in that potential is simply the charge multiplied by the potential.
Electric potential, like potential energy, is a scalar, not a vector.

connection between potential and potential energy: V = PE / q

Equipotential lines are connected lines of the same potential. These
often appear on field line diagrams. Equipotential lines are always
perpendicular to field lines, and therefore perpendicular to the force
experienced by a charge in the field. If a charge moves along an
equipotential line, no work is done; if a charge moves between
equipotential lines, work is done.

Field lines and equipotential lines for a point charge, and for a constant field between two charged plates, are shown below:

An example : Ionization energy of the electron in a hydrogen atom

In the Bohr model of a hydrogen atom, the electron, if it is in the
ground state, orbits the proton at a distance of r = 5.29 x 10-11 m.
Note that the Bohr model, the idea of electrons as tiny balls orbiting
the nucleus, is not a very good model of the atom. A better picture is
one in which the electron is spread out around the nucleus in a cloud
of varying density; however, the Bohr model does give the right answer
for the ionization energy, the energy required to remove the electron
from the atom.

The total energy is the sum of the electron's kinetic energy and the
potential energy coming from the electron-proton interaction.

The kinetic energy is given by KE = 1/2 mv2.

This can be found by analyzing the force on the electron. This force is
the Coulomb force; because the electron travels in a circular orbit,
the acceleration will be the centripetal acceleration:

Note that the negative sign coming from the charge on the electron
has been incorporated into the direction of the force in the equation

This gives m v2 = k e2 / r, so the kinetic energy is KE = 1/2 k e2 / r.

The potential energy, on the other hand, is PE = - k e2
/ r. Note that the potential energy is twice as big as the kinetic
energy, but negative. This relationship between the kinetic and
potential energies is valid not just for electrons orbiting protons,
but also in gravitational situations, such as a satellite orbiting the

The total energy is:

KE + PE = -1/2 ke2 / r = - 1/2 (8.99 x 109)(1.60 x 10-19) / 5.29 x 10-11

This works out to -2.18 x 10-18 J. This is usually stated in energy units of electron volts (eV). An eV is 1.60 x 10-19
J, so dividing by this gives an energy of -13.6 eV. To remove the
electron from the atom, 13.6 eV must be put in; 13.6 eV is thus the
ionization energy of a ground-state electron in hydrogen.


Subject X2: 

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