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Transcript
The internal energy of a system is the sum of all kinetic and potential
energy in a system.
LEARNING OBJECTIVES [ edit ]
Express the internal energy in terms of kinetic and potential energy
Identify the internal energy as an extensive property
KEY POINTS [ edit ]
While a system does not contain 'heat,' it does contain a total amount of energy called internal
energy.
The internal energy is the energy necessary to create a system, minus the energy necessary to
displace its surroundings.
Most of the time, we are interested in the change in internal energy rather than the total internal
energy.
The first law of thermodynamics, dU
=
Δ
Q
−
Δ
W
, describes small changes in internal energy.
TERMS [ edit ]
internal energy
The sum of all energy present in the system, including kinetic and potential energy; equivalently,
the energy needed to create a system, excluding the energy necessary to displace its surroundings.
isolated system
A system that does not interact with its surroundings, that is, its total energy and mass stay
constant.
Give us feedback on this content: FULL TEXT [edit ]
Internal Energy
James Joule showed that both heat
and work can produce the same change in
the internal energy of a substance,
establishing the principle of the
mechanical equivalence of heat. Heat is
emphatically a quantity that solely
describes energy being transferred. It
makes no sense to speak of the total 'heat'
an object or system contains. However, a
system does contain a quantifiable amount
of energy called the internal energy of a
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system. The internal energy of a system is the quantity that changes with the addition or
subtraction of work or heat. It is closely related to temperature.
Definition
The internal energy is the energy required to create a system, excluding the energy necessary
to displace its surroundings. Internal energy has
two components: kinetic energy andpotential energy. The kinetic energy consists of all the
energy involving the motions of the particles constituting the system, including translation,
vibration, and rotation. The potential energy is associated with the static constituents
of matter, static electric energy of atoms within molecules or crystals, and the energy from
chemical bonds. The equation describing the total internal energy of a system is then:
U = U kinetic + U potential
.
We can also think of the internal energy as the sum of all the energy states of each component
in the system:
U =
∑
i
Ei
.
At any finite temperature, kinetic and potential energies are constantly converted into each
other, but the total energy remains constant in an isolated system. The kinetic energy portion
of internal energy gives rise to the temperature of the system. We can use statistical
mechanics to relate the (somewhat) random motions of particles in a system to the mean
kinetic energy of the ensemble of particles, and thus the empirically measurable quantity
expressed as temperature.
We can see that internal energy is an extensive property: it depends on the size of the system
or on the amount of substance it contains.
In most cases, we are not concerned with the total amount of internal energy in the system,
as it is rarely convenient or necessary to consider all energies belonging to the system.
Rather, we are far more interested in the change in internal energy, given some transfer of
work or heat. This can be expressed as:
U = Q + W mech + W other
Δ
.
Q is heat added to a system and Wmech is the mechanical work performed by the
surroundings due to pressure or volume changes in the system. All other perturbations and
energies added by other processes, such as an electric current introduced into an
electronic circuit, is summarized as the term Wextra.
We can calculate a small change in internal energy of the system by considering the
infinitesimal amount of heat δQ added to the system minus the infinitesimal amount of work
δW done by the system:
dU =
δQ − δW .
This expression is the first law of thermodynamics.
The Sun and Internal Energy
Nuclear fusion in the sun converts nuclear potential energy into available internal energy and keeps
the temperature of the Sun very high.