Ordinary differential equation
In mathematics, an ordinary differential equation (ODE) is a differential equation containing one or more functions of one independent variable and the derivatives of those functions. The term ordinary is used in contrast with the term partial differential equation which may be with respect to more than one independent variable.
- 1 Differential equations
- 2 Background
- 3 Definitions
- 4 Theories
- 5 Existence and uniqueness of solutions
- 6 Reduction of order
- 7 Summary of exact solutions
- 8 Software for ODE solving
- 9 See also
- 10 Notes
- 11 References
- 12 Bibliography
- 13 External links
where , ..., and are arbitrary differentiable functions that do not need to be linear, and are the successive derivatives of the unknown function y of the variable x.
Among ordinary differential equations, linear differential equations play a prominent role for several reasons. Most elementary and special functions that are encountered in physics and applied mathematics are solutions of linear differential equations (see Holonomic function); when physical phenomena are modeled with non-linear equations, they are generally approximated by linear differential equations for an easier solution. The few non-linear ODEs that can be solved explicitly are generally solved by transforming the equation into an equivalent linear ODE (see, for example Riccati equation).
Some ODEs can be solved explicitly in terms of known functions and integrals; when that is not possible, the equation for computing the Taylor series of the solutions may be useful. For applied problems, numerical methods for ordinary differential equations can supply an approximation of the solution.
Ordinary differential equations (ODEs) arise in many contexts of mathematics and social and natural sciences. Mathematical descriptions of change use differentials and derivatives. Various differentials, derivatives, and functions become related via equations, such that a differential equation is a result that describes dynamically changing phenomena, evolution, and variation. Often, quantities are defined as the rate of change of other quantities (for example, derivatives of displacement with respect to time), or gradients of quantities, which is how they enter differential equations.
Specific mathematical fields include geometry and analytical mechanics. Scientific fields include much of physics and astronomy (celestial mechanics), meteorology (weather modelling), chemistry (reaction rates), biology (infectious diseases, genetic variation), ecology and population modelling (population competition), economics (stock trends, interest rates and the market equilibrium price changes).
A simple example is Newton's second law of motion — the relationship between the displacement x and the time t of an object under the force F, is given by the differential equation
which constrains the motion of a particle of constant mass m. In general, F is a function of the position x(t) of the particle at time t; the unknown function x(t) appears on both sides of the differential equation, and is indicated in the notation F(x(t)).
In what follows, let y be a dependent variable and x an independent variable, and y = f(x) is an unknown function of x; the notation for differentiation varies depending upon the author and upon which notation is most useful for the task at hand. In this context, the Leibniz's notation (dy/dx,d2y/dx2,...,dny/dxn) is more useful for differentiation and integration, whereas Lagrange's notation (y′,y′′, ..., y(n)) is more useful for representing derivatives of any order compactly, and Newton's notation is often used in physics for representing derivatives of low order with respect to time.
Given F, a function of x, y, and derivatives of y. Then an equation of the form
There are further classifications:
- A differential equation not depending on x is called autonomous.
A differential equation is said to be linear if F can be written as a linear combination of the derivatives of y:
- If r(x) = 0, and consequently one "automatic" solution is the trivial solution, y = 0. The solution of a linear homogeneous equation is a complementary function, denoted here by yc.
- Nonhomogeneous (or inhomogeneous)
- If r(x) ≠ 0. The additional solution to the complementary function is the particular integral, denoted here by yp.
- A differential equation that cannot be written in the form of a linear combination.
The general solution to a linear equation can be written as y = yc + yp.
System of ODEs
A number of coupled differential equations form a system of equations. If y is a vector whose elements are functions; y(x) = [y1(x), y2(x),..., ym(x)], and F is a vector-valued function of y and its derivatives, then
is an explicit system of ordinary differential equations of order n and dimension m. In column vector form:
These are not necessarily linear; the implicit analogue is:
where 0 = (0, 0, ..., 0) is the zero vector. In matrix form
For a system of the form , some sources also require that the Jacobian matrix be non-singular in order to call this an implicit ODE [system]; an implicit ODE system satisfying this Jacobian non-singularity condition can be transformed into an explicit ODE system. In the same sources, implicit ODE systems with a singular Jacobian are termed differential algebraic equations (DAEs); this distinction is not merely one of terminology; DAEs have fundamentally different characteristics and are generally more involved to solve than (nonsingular) ODE systems. Presumably for additional derivatives, the Hessian matrix and so forth are also assumed non-singular according to this scheme, although note that any ODE of order greater than one can be [and usually is] rewritten as system of ODEs of first order, which makes the Jacobian singularity criterion sufficient for this taxonomy to be comprehensive at all orders.
The behavior of a system of ODEs can be visualized through the use of a phase portrait.
Given a differential equation
a function u: I ⊂ R → R is called a solution or integral curve for F, if u is n-times differentiable on I, and
Given two solutions u: J ⊂ R → R and v: I ⊂ R → R, u is called an extension of v if I ⊂ J and
A solution that has no extension is called a maximal solution. A solution defined on all of R is called a global solution.
A general solution of an nth-order equation is a solution containing n arbitrary independent constants of integration. A particular solution is derived from the general solution by setting the constants to particular values, often chosen to fulfill set 'initial conditions or boundary conditions'. A singular solution is a solution that cannot be obtained by assigning definite values to the arbitrary constants in the general solution.
The theory of singular solutions of ordinary and partial differential equations was a subject of research from the time of Leibniz, but only since the middle of the nineteenth century has it received special attention. A valuable but little-known work on the subject is that of Houtain (1854). Darboux (from 1873) was a leader in the theory, and in the geometric interpretation of these solutions he opened a field worked by various writers, notably Casorati and Cayley. To the latter is due (1872) the theory of singular solutions of differential equations of the first order as accepted circa 1900.
Reduction to quadratures
The primitive attempt in dealing with differential equations had in view a reduction to quadratures; as it had been the hope of eighteenth-century algebraists to find a method for solving the general equation of the nth degree, so it was the hope of analysts to find a general method for integrating any differential equation. Gauss (1799) showed, however, that complex differential equations require complex numbers. Hence, analysts began to substitute the study of functions, thus opening a new and fertile field. Cauchy was the first to appreciate the importance of this view. Thereafter, the real question was no longer whether a solution is possible by means of known functions or their integrals, but whether a given differential equation suffices for the definition of a function of the independent variable or variables, and, if so, what are the characteristic properties.
Two memoirs by Fuchs inspired a novel approach, subsequently elaborated by Thomé and Frobenius. Collet was a prominent contributor beginning in 1869, his method for integrating a non-linear system was communicated to Bertrand in 1868. Clebsch (1873) attacked the theory along lines parallel to those in his theory of Abelian integrals; as the latter can be classified according to the properties of the fundamental curve that remains unchanged under a rational transformation, Clebsch proposed to classify the transcendent functions defined by differential equations according to the invariant properties of the corresponding surfaces f = 0 under rational one-to-one transformations.
From 1870, Sophus Lie's work put the theory of differential equations on a better foundation, he showed that the integration theories of the older mathematicians can, using Lie groups, be referred to a common source, and that ordinary differential equations that admit the same infinitesimal transformations present comparable integration difficulties. He also emphasized the subject of transformations of contact.
Lie's group theory of differential equations has been certified, namely: (1) that it unifies the many ad hoc methods known for solving differential equations, and (2) that it provides powerful new ways to find solutions; the theory has applications to both ordinary and partial differential equations.
A general solution approach uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras, and differential geometry are used to understand the structure of linear and nonlinear (partial) differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform, and finally finding exact analytic solutions to DE.
Symmetry methods have been applied to differential equations that arise in mathematics, physics, engineering, and other disciplines.
Sturm–Liouville theory is a theory of a special type of second order linear ordinary differential equation, their solutions are based on eigenvalues and corresponding eigenfunctions of linear operators defined via second-order homogeneous linear equations. The problems are identified as Sturm-Liouville Problems (SLP) and are named after J.C.F. Sturm and J. Liouville, who studied them in the mid-1800s. SLPs have an infinite number of eigenvalues, and the corresponding eigenfunctions form a complete, orthogonal set, which makes orthogonal expansions possible; this is a key idea in applied mathematics, physics, and engineering. SLPs are also useful in the analysis of certain partial differential equations.
Existence and uniqueness of solutions
There are several theorems that establish existence and uniqueness of solutions to initial value problems involving ODEs both locally and globally; the two main theorems are
Theorem Assumption Conclusion Peano existence theorem F continuous local existence only Picard–Lindelöf theorem F Lipschitz continuous local existence and uniqueness
In their basic form both of these theorems only guarantee local results, though the latter can be extended to give a global result, for example, if the conditions of Grönwall's inequality are met.
Local existence and uniqueness theorem simplified
The theorem can be stated simply as follows. For the equation and initial value problem:
if F and ∂F/∂y are continuous in a closed rectangle
for some h ∈ ℝ where the solution to the above equation and initial value problem can be found. That is, there is a solution and it is unique. Since there is no restriction on F to be linear, this applies to non-linear equations that take the form F(x, y), and it can also be applied to systems of equations.
Global uniqueness and maximum domain of solution
When the hypotheses of the Picard–Lindelöf theorem are satisfied, then local existence and uniqueness can be extended to a global result. More precisely:
For each initial condition (x0, y0) there exists a unique maximum (possibly infinite) open interval
such that any solution that satisfies this initial condition is a restriction of the solution that satisfies this initial condition with domain .
In the case that , there are exactly two possibilities
- explosion in finite time:
- leaves domain of definition:
where Ω is the open set in which F is defined, and is its boundary.
Note that the maximum domain of the solution
- is always an interval (to have uniqueness)
- may be smaller than
- may depend on the specific choice of (x0, y0).
This means that F(x, y) = y2, which is C1 and therefore locally Lipschitz continuous, satisfying the Picard–Lindelöf theorem.
Even in such a simple setting, the maximum domain of solution cannot be all since the solution is
which has maximum domain:
This shows clearly that the maximum interval may depend on the initial conditions; the domain of y could be taken as being but this would lead to a domain that is not an interval, so that the side opposite to the initial condition would be disconnected from the initial condition, and therefore not uniquely determined by it.
The maximum domain is not because
which is one of the two possible cases according to the above theorem.
Reduction of order
Differential equations can usually be solved more easily if the order of the equation can be reduced.
Reduction to a first-order system
Any explicit differential equation of order n,
can be written as a system of n first-order differential equations by defining a new family of unknown functions
for i = 1, 2,..., n. The n-dimensional system of first-order coupled differential equations is then
more compactly in vector notation:
Summary of exact solutions
Some differential equations have solutions that can be written in an exact and closed form. Several important classes are given here.
In the table below, P(x), Q(x), P(y), Q(y), and M(x,y), N(x,y) are any integrable functions of x, y, and b and c are real given constants, and C1, C2,... are arbitrary constants (complex in general). The differential equations are in their equivalent and alternative forms that lead to the solution through integration.
In the integral solutions, λ and ε are dummy variables of integration (the continuum analogues of indices in summation), and the notation ∫xF(λ) dλ just means to integrate F(λ) with respect to λ, then after the integration substitute λ = x, without adding constants (explicitly stated).
Type Differential equation Solution method General solution Separable First-order, separable in x and y (general case, see below for special cases) Separation of variables (divide by P2Q1). First-order, separable in x Direct integration. First-order, autonomous, separable in y Separation of variables (divide by F). First-order, separable in x and y Integrate throughout. General first-order First-order, homogeneous Set y = ux, then solve by separation of variables in u and x. First-order, separable Separation of variables (divide by xy).
If N = M, the solution is xy = C.
Exact differential, first-order
where Y(y) and X(x) are functions from the integrals rather than constant values, which are set to make the final function F(x, y) satisfy the initial equation.
Inexact differential, first-order
Integration factor μ(x, y) satisfying If μ(x, y) can be found: General second-order Second-order, autonomous Multiply both sides of equation by 2dy/dx, substitute , then integrate twice. Linear to nth order First-order, linear, inhomogeneous, function coefficients Integrating factor: Second-order, linear, inhomogeneous, constant coefficients Complementary function yc: assume yc = eαx, substitute and solve polynomial in α, to find the linearly independent functions .
If b2 > 4c, then
If b2 = 4c, then
If b2 < 4c, then
nth-order, linear, inhomogeneous, constant coefficients Complementary function yc: assume yc = eαx, substitute and solve polynomial in α, to find the linearly independent functions .
for αj all different,
for each root αj repeated kj times,
for some αj complex, then setting α = χj + iγj, and using Euler's formula, allows some terms in the previous results to be written in the form
where ϕj is an arbitrary constant (phase shift).
Software for ODE solving
- Maxima, an open-source computer algebra system.
- COPASI, a free (Artistic License 2.0) software package for the integration and analysis of ODEs.
- MATLAB, a technical computing application (MATrix LABoratory)
- GNU Octave, a high-level language, primarily intended for numerical computations.
- Scilab, an open source application for numerical computation.
- Maple, a proprietary application for symbolic calculations.
- Mathematica, a proprietary application primarily intended for symbolic calculations.
- Julia (programming language), a high-level, multi-paradigm, open-source, dynamic programming language primarily intended for numerical computations, although it is flexible enough for general-purpose programming.
- SageMath, an open-source application that uses a Python-like syntax with a wide range of capabilities spanning several branches of mathematics.
- SciPy, a Python package that includes an ODE integration module.
- Chebfun, an open-source package, written in MATLAB, for computing with functions to 15-digit accuracy.
- GNU R, an open source computational environment primarily intended for statistics, which includes package for ODE solving.
- EROS.NET a free ODE solver for .NET.
- Examples of differential equations
- Boundary value problem
- Laplace transform applied to differential equations
- List of dynamical systems and differential equations topics
- Matrix differential equation
- Method of undetermined coefficients
- Numerical methods for ordinary differential equations
- Recurrence relation
- Separation of variables
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|Wikibooks has a book on the topic of: Calculus/Ordinary differential equations|
|Wikimedia Commons has media related to Ordinary differential equations.|
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- Solving an ordinary differential equation in Wolfram|Alpha