- Source: Separable partial differential equation
A separable partial differential equation can be broken into a set of equations of lower dimensionality (fewer independent variables) by a method of separation of variables. It generally relies upon the problem having some special form or symmetry. In this way, the partial differential equation (PDE) can be solved by solving a set of simpler PDEs, or even ordinary differential equations (ODEs) if the problem can be broken down into one-dimensional equations.
The most common form of separation of variables is simple separation of variables. A solution is obtained by assuming a solution of the form given by a product of functions of each individual coordinate. There is a special form of separation of variables called
R
{\displaystyle R}
-separation of variables which is accomplished by writing the solution as a particular fixed function of the coordinates multiplied by a product of functions of each individual coordinate. Laplace's equation on
R
n
{\displaystyle {\mathbb {R} }^{n}}
is an example of a partial differential equation that admits solutions through
R
{\displaystyle R}
-separation of variables; in the three-dimensional case this uses 6-sphere coordinates.
(This should not be confused with the case of a separable ODE, which refers to a somewhat different class of problems that can be broken into a pair of integrals; see separation of variables.)
Example
For example, consider the time-independent Schrödinger equation
[
−
∇
2
+
V
(
x
)
]
ψ
(
x
)
=
E
ψ
(
x
)
{\displaystyle [-\nabla ^{2}+V(\mathbf {x} )]\psi (\mathbf {x} )=E\psi (\mathbf {x} )}
for the function
ψ
(
x
)
{\displaystyle \psi (\mathbf {x} )}
(in dimensionless units, for simplicity). (Equivalently, consider the inhomogeneous Helmholtz equation.) If the function
V
(
x
)
{\displaystyle V(\mathbf {x} )}
in three dimensions is of the form
V
(
x
1
,
x
2
,
x
3
)
=
V
1
(
x
1
)
+
V
2
(
x
2
)
+
V
3
(
x
3
)
,
{\displaystyle V(x_{1},x_{2},x_{3})=V_{1}(x_{1})+V_{2}(x_{2})+V_{3}(x_{3}),}
then it turns out that the problem can be separated into three one-dimensional ODEs for functions
ψ
1
(
x
1
)
{\displaystyle \psi _{1}(x_{1})}
,
ψ
2
(
x
2
)
{\displaystyle \psi _{2}(x_{2})}
, and
ψ
3
(
x
3
)
{\displaystyle \psi _{3}(x_{3})}
, and the final solution can be written as
ψ
(
x
)
=
ψ
1
(
x
1
)
⋅
ψ
2
(
x
2
)
⋅
ψ
3
(
x
3
)
{\displaystyle \psi (\mathbf {x} )=\psi _{1}(x_{1})\cdot \psi _{2}(x_{2})\cdot \psi _{3}(x_{3})}
. (More generally, the separable cases of the Schrödinger equation were enumerated by Eisenhart in 1948.)
References
Kata Kunci Pencarian:
- Separable partial differential equation
- Partial differential equation
- Numerical methods for partial differential equations
- Laplace's equation
- Separation of variables
- Ordinary differential equation
- Separability
- List of named differential equations
- Helmholtz equation
- Schrödinger equation
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