An integral along a curve. In
-dimensional
Euclidean space
consider a given rectifiable curve
,
,
where
is the arc length; let
be a function defined on
.
The curvilinear integral
is defined by the equality
(the integral on the right is an integral over a real interval), and is called a
line integral of the first kind,
or a
line integral with respect to arc length.
It is the limit of suitable integral sums, which can
be described in terms related to the curve. For example, if

is Riemann-integrable (see
Riemann integral),

is a partition of

,

is its mesh,

,

is the length of the section of

from the point

to the point

,

,
and
then
If the rectifiable curve
is given parametrically by
,
,
and
is a function defined on
,
then the integral
is defined by
(the integral on the right is a
Stieltjes integral),
and is called a
line integral of the second kind
or a
line integral with respect to the coordinate

.
It is also the limit of suitably constructed Riemann sums: If

is a partition of

,

,

,

,
and
then
If

is a continuous function on

,
then the curvilinear integrals
(1)
and
(2)
always exist. If

is the initial point and

the end point of

,
then the curvilinear integrals
(1)
and
(2)
are denoted by
respectively.
Line integrals of the first kind are independent of the orientation of the curve:
but line integrals of the second kind change sign when the orientation is reversed:
If
is a continuously differentiable curve given
by a continuously differentiable representation
,
,
and
is a continuous function on
,
then
and hence the integrals on the right of these equalities
are independent of the choice of the parameter on

.
If

is a unit tangent vector to the curve

,
then the line integral of the second kind may be expressed in
terms of a line integral of the first kind via the formula
If
is given in vector notation
and
is a vector function defined on
,
then, by definition,
The relationship between line integrals and integrals
of other types is established by the
Green formulas
and the
Stokes formula.
Line integrals may be used to calculate the area
of plane domains: If a finite plane domain
is bounded by a simple rectifiable curve
,
then its area is
where the contour

is oriented in the counter-clockwise sense.
If
is a mass distributed over
with linear density
,
then
If

is the intensity of a force field (i.e. the force acting on a unit mass), then
is equal to the work performed by the field in moving a unit mass along

.
Line integrals are used in the theory of vector fields. If
is a continuous vector field defined on some
-dimensional
domain
,
,
then the following three properties are equivalent:
1)
For any closed rectifiable curve
,
(a vector field possessing this property is called a
potential field).
2)
For any pair of points
and any two rectifiable curves
with initial point
and end point
:
3)
There exists in
a function
(called a
potential function
of the field
),
such that
,
i.e.
,
,
and moreover, for any
and any curve
,
If
or
and
is a simply-connected domain
(
)
or a simply-connected surface
(
),
while the field
is continuously differentiable, then the properties 1)–3) are equivalent to the following property:
4)
The rotation of the vector field vanishes in
:
If
is not simply connected, then 4) need not be equivalent
to 1)–3). For example, for the field
defined on the plane punctured at the origin one has

,

,
but