Calculus of variations
Part of a series of articles about 
Calculus 

The calculus of variations is a field of mathematical analysis that uses variations, which are small changes in functions and functionals, to find maxima and minima of functionals: mappings from a set of functions to the real numbers.^{ [a]} Functionals are often expressed as definite integrals involving functions and their derivatives. Functions that maximize or minimize functionals may be found using the Euler–Lagrange equation of the calculus of variations.
A simple example of such a problem is to find the curve of shortest length connecting two points. If there are no constraints, the solution is a straight line between the points. However, if the curve is constrained to lie on a surface in space, then the solution is less obvious, and possibly many solutions may exist. Such solutions are known as geodesics. A related problem is posed by Fermat's principle: light follows the path of shortest optical length connecting two points, where the optical length depends upon the material of the medium. One corresponding concept in mechanics is the principle of least/stationary action.
Many important problems involve functions of several variables. Solutions of boundary value problems for the Laplace equation satisfy the Dirichlet principle. Plateau's problem requires finding a surface of minimal area that spans a given contour in space: a solution can often be found by dipping a frame in a solution of soap suds. Although such experiments are relatively easy to perform, their mathematical interpretation is far from simple: there may be more than one locally minimizing surface, and they may have nontrivial topology.
History
The calculus of variations may be said to begin with Newton's minimal resistance problem in 1687, followed by the brachistochrone curve problem raised by Johann Bernoulli (1696).^{ [2]} It immediately occupied the attention of Jakob Bernoulli and the Marquis de l'Hôpital, but Leonhard Euler first elaborated the subject, beginning in 1733. Lagrange was influenced by Euler's work to contribute significantly to the theory. After Euler saw the 1755 work of the 19yearold Lagrange, Euler dropped his own partly geometric approach in favor of Lagrange's purely analytic approach and renamed the subject the calculus of variations in his 1756 lecture Elementa Calculi Variationum.^{ [3]}^{ [4]}^{ [1]}
Legendre (1786) laid down a method, not entirely satisfactory, for the discrimination of maxima and minima. Isaac Newton and Gottfried Leibniz also gave some early attention to the subject.^{ [5]} To this discrimination Vincenzo Brunacci (1810), Carl Friedrich Gauss (1829), Siméon Poisson (1831), Mikhail Ostrogradsky (1834), and Carl Jacobi (1837) have been among the contributors. An important general work is that of Sarrus (1842) which was condensed and improved by Cauchy (1844). Other valuable treatises and memoirs have been written by Strauch (1849), Jellett (1850), Otto Hesse (1857), Alfred Clebsch (1858), and Carll (1885), but perhaps the most important work of the century is that of Weierstrass. His celebrated course on the theory is epochmaking, and it may be asserted that he was the first to place it on a firm and unquestionable foundation. The 20th and the 23rd Hilbert problem published in 1900 encouraged further development.^{ [5]}
In the 20th century David Hilbert, Emmy Noether, Leonida Tonelli, Henri Lebesgue and Jacques Hadamard among others made significant contributions.^{ [5]} Marston Morse applied calculus of variations in what is now called Morse theory.^{ [6]} Lev Pontryagin, Ralph Rockafellar and F. H. Clarke developed new mathematical tools for the calculus of variations in optimal control theory.^{ [6]} The dynamic programming of Richard Bellman is an alternative to the calculus of variations.^{ [7]}^{ [8]}^{ [9]}^{ [b]}
Extrema
The calculus of variations is concerned with the maxima or minima (collectively called extrema) of functionals. A functional maps functions to scalars, so functionals have been described as "functions of functions." Functionals have extrema with respect to the elements y of a given function space defined over a given domain. A functional J [ y ] is said to have an extremum at the function f if ΔJ = J [ y ] − J [ f] has the same sign for all y in an arbitrarily small neighborhood of f .^{ [c]} The function f is called an extremal function or extremal.^{ [d]} The extremum J [ f ] is called a local maximum if ΔJ ≤ 0 everywhere in an arbitrarily small neighborhood of f , and a local minimum if ΔJ ≥ 0 there. For a function space of continuous functions, extrema of corresponding functionals are called weak extrema or strong extrema, depending on whether the first derivatives of the continuous functions are respectively all continuous or not.^{ [11]}
Both strong and weak extrema of functionals are for a space of continuous functions but strong extrema have the additional requirement that the first derivatives of the functions in the space be continuous. Thus a strong extremum is also a weak extremum, but the converse may not hold. Finding strong extrema is more difficult than finding weak extrema.^{ [12]} An example of a necessary condition that is used for finding weak extrema is the Euler–Lagrange equation.^{ [13]}^{ [e]}
Euler–Lagrange equation
Finding the extrema of functionals is similar to finding the maxima and minima of functions. The maxima and minima of a function may be located by finding the points where its derivative vanishes (i.e., is equal to zero). The extrema of functionals may be obtained by finding functions where the functional derivative is equal to zero. This leads to solving the associated Euler–Lagrange equation.^{ [f]}
Consider the functional
where
 x_{1}, x_{2} are constants,
 y (x) is twice continuously differentiable,
 y ′(x) = dy / dx ,
 L(x, y (x), y ′(x)) is twice continuously differentiable with respect to its arguments x, y, y ′.
If the functional J[y ] attains a local minimum at f , and η(x) is an arbitrary function that has at least one derivative and vanishes at the endpoints x_{1} and x_{2} , then for any number ε close to 0,
The term εη is called the variation of the function f and is denoted by δf .^{ [1]}^{ [g]}
Substituting f + εη for y in the functional J[ y ] , the result is a function of ε,
Since the functional J[ y ] has a minimum for y = f , the function Φ(ε) has a minimum at ε = 0 and thus,^{ [h]}
Taking the total derivative of L[x, y, y ′] , where y = f + ε η and y ′ = f ′ + ε η′ are considered as functions of ε rather than x, yields
and since dy /dε = η and dy ′/dε = η' ,
Therefore,
where L[x, y, y ′] → L[x, f, f ′] when ε = 0 and we have used integration by parts on the second term. The second term on the second line vanishes because η = 0 at x_{1} and x_{2} by definition. Also, as previously mentioned the left side of the equation is zero so that
According to the fundamental lemma of calculus of variations, the part of the integrand in parentheses is zero, i.e.
which is called the Euler–Lagrange equation. The left hand side of this equation is called the functional derivative of J[f] and is denoted δJ/δf(x) .
In general this gives a secondorder ordinary differential equation which can be solved to obtain the extremal function f(x) . The Euler–Lagrange equation is a necessary, but not sufficient, condition for an extremum J[f]. A sufficient condition for a minimum is given in the section Variations and sufficient condition for a minimum.
Example
In order to illustrate this process, consider the problem of finding the extremal function y = f (x) , which is the shortest curve that connects two points (x_{1}, y_{1}) and (x_{2}, y_{2}) . The arc length of the curve is given by
with
^{ [i]}
The Euler–Lagrange equation will now be used to find the extremal function f (x) that minimizes the functional A[y ] .
with
Since f does not appear explicitly in L , the first term in the Euler–Lagrange equation vanishes for all f (x) and thus,
Substituting for L and taking the derivative,
Thus
for some constant c. Then
where
Solving, we get
which implies that
is a constant and therefore that the shortest curve that connects two points (x_{1}, y_{1}) and (x_{2}, y_{2}) is
and we have thus found the extremal function f(x) that minimizes the functional A[y] so that A[f] is a minimum. The equation for a straight line is y = f(x). In other words, the shortest distance between two points is a straight line.^{ [j]}
Beltrami's identity
In physics problems it may be the case that , meaning the integrand is a function of and but does not appear separately. In that case, the Euler–Lagrange equation can be simplified to the Beltrami identity^{ [16]}
where is a constant. The left hand side is the Legendre transformation of with respect to .
The intuition behind this result is that, if the variable x is actually time, then the statement implies that the Lagrangian is timeindependent. By Noether's theorem, there is an associated conserved quantity. In this case, this quantity is the Hamiltonian, the Legendre transform of the Lagrangian, which (often) coincides with the energy of the system. This is (minus) the constant in Beltrami's identity.
Euler–Poisson equation
If depends on higherderivatives of , that is, if
then must satisfy the Euler– Poisson equation,
^{ [17]}
Du BoisReymond's theorem
The discussion thus far has assumed that extremal functions possess two continuous derivatives, although the existence of the integral J requires only first derivatives of trial functions. The condition that the first variation vanishes at an extremal may be regarded as a weak form of the Euler–Lagrange equation. The theorem of Du BoisReymond asserts that this weak form implies the strong form. If L has continuous first and second derivatives with respect to all of its arguments, and if
then has two continuous derivatives, and it satisfies the Euler–Lagrange equation.
Lavrentiev phenomenon
Hilbert was the first to give good conditions for the Euler–Lagrange equations to give a stationary solution. Within a convex area and a positive thrice differentiable Lagrangian the solutions are composed of a countable collection of sections that either go along the boundary or satisfy the Euler–Lagrange equations in the interior.
However Lavrentiev in 1926 showed that there are circumstances where there is no optimum solution but one can be approached arbitrarily closely by increasing numbers of sections. The Lavrentiev Phenomenon identifies a difference in the infimum of a minimization problem across different classes of admissible functions. For instance the following problem, presented by Manià in 1934:^{ [18]}
Clearly, minimizes the functional, but we find any function gives a value bounded away from the infimum.
Examples (in onedimension) are traditionally manifested across and , but Ball and Mizel^{ [19]} procured the first functional that displayed Lavrentiev's Phenomenon across and for There are several results that gives criteria under which the phenomenon does not occur  for instance 'standard growth', a Lagrangian with no dependence on the second variable, or an approximating sequence satisfying Cesari's Condition (D)  but results are often particular, and applicable to a small class of functionals.
Connected with the Lavrentiev Phenomenon is the repulsion property: any functional displaying Lavrentiev's Phenomenon will display the weak repulsion property.^{ [20]}
Functions of several variables
For example, if φ(x,y) denotes the displacement of a membrane above the domain D in the x,y plane, then its potential energy is proportional to its surface area:
Plateau's problem consists of finding a function that minimizes the surface area while assuming prescribed values on the boundary of D; the solutions are called minimal surfaces. The Euler–Lagrange equation for this problem is nonlinear:
See Courant (1950) for details.
Dirichlet's principle
It is often sufficient to consider only small displacements of the membrane, whose energy difference from no displacement is approximated by
The functional V is to be minimized among all trial functions φ that assume prescribed values on the boundary of D. If u is the minimizing function and v is an arbitrary smooth function that vanishes on the boundary of D, then the first variation of must vanish:
Provided that u has two derivatives, we may apply the divergence theorem to obtain
where C is the boundary of D, s is arclength along C and is the normal derivative of u on C. Since v vanishes on C and the first variation vanishes, the result is
for all smooth functions v that vanish on the boundary of D. The proof for the case of one dimensional integrals may be adapted to this case to show that
 in D.
The difficulty with this reasoning is the assumption that the minimizing function u must have two derivatives. Riemann argued that the existence of a smooth minimizing function was assured by the connection with the physical problem: membranes do indeed assume configurations with minimal potential energy. Riemann named this idea the Dirichlet principle in honor of his teacher Peter Gustav Lejeune Dirichlet. However Weierstrass gave an example of a variational problem with no solution: minimize
among all functions φ that satisfy and can be made arbitrarily small by choosing piecewise linear functions that make a transition between −1 and 1 in a small neighborhood of the origin. However, there is no function that makes .^{ [k]} Eventually it was shown that Dirichlet's principle is valid, but it requires a sophisticated application of the regularity theory for elliptic partial differential equations; see Jost and Li–Jost (1998).
Generalization to other boundary value problems
A more general expression for the potential energy of a membrane is
This corresponds to an external force density in D, an external force on the boundary C, and elastic forces with modulus acting on C. The function that minimizes the potential energy with no restriction on its boundary values will be denoted by u. Provided that f and g are continuous, regularity theory implies that the minimizing function u will have two derivatives. In taking the first variation, no boundary condition need be imposed on the increment v. The first variation of is given by
If we apply the divergence theorem, the result is
If we first set v = 0 on C, the boundary integral vanishes, and we conclude as before that
in D. Then if we allow v to assume arbitrary boundary values, this implies that u must satisfy the boundary condition
on C. This boundary condition is a consequence of the minimizing property of u: it is not imposed beforehand. Such conditions are called natural boundary conditions.
The preceding reasoning is not valid if vanishes identically on C. In such a case, we could allow a trial function , where c is a constant. For such a trial function,
By appropriate choice of c, V can assume any value unless the quantity inside the brackets vanishes. Therefore, the variational problem is meaningless unless
This condition implies that net external forces on the system are in equilibrium. If these forces are in equilibrium, then the variational problem has a solution, but it is not unique, since an arbitrary constant may be added. Further details and examples are in Courant and Hilbert (1953).
Eigenvalue problems
Both onedimensional and multidimensional eigenvalue problems can be formulated as variational problems.
Sturm–Liouville problems
The Sturm–Liouville eigenvalue problem involves a general quadratic form
where is restricted to functions that satisfy the boundary conditions
Let R be a normalization integral
The functions and are required to be everywhere positive and bounded away from zero. The primary variational problem is to minimize the ratio Q/R among all φ satisfying the endpoint conditions. It is shown below that the Euler–Lagrange equation for the minimizing u is
where λ is the quotient
It can be shown (see Gelfand and Fomin 1963) that the minimizing u has two derivatives and satisfies the Euler–Lagrange equation. The associated λ will be denoted by ; it is the lowest eigenvalue for this equation and boundary conditions. The associated minimizing function will be denoted by . This variational characterization of eigenvalues leads to the Rayleigh–Ritz method: choose an approximating u as a linear combination of basis functions (for example trigonometric functions) and carry out a finitedimensional minimization among such linear combinations. This method is often surprisingly accurate.
The next smallest eigenvalue and eigenfunction can be obtained by minimizing Q under the additional constraint
This procedure can be extended to obtain the complete sequence of eigenvalues and eigenfunctions for the problem.
The variational problem also applies to more general boundary conditions. Instead of requiring that φ vanish at the endpoints, we may not impose any condition at the endpoints, and set
where and are arbitrary. If we set the first variation for the ratio is
where λ is given by the ratio as previously. After integration by parts,
If we first require that v vanish at the endpoints, the first variation will vanish for all such v only if
If u satisfies this condition, then the first variation will vanish for arbitrary v only if
These latter conditions are the natural boundary conditions for this problem, since they are not imposed on trial functions for the minimization, but are instead a consequence of the minimization.
Eigenvalue problems in several dimensions
Eigenvalue problems in higher dimensions are defined in analogy with the onedimensional case. For example, given a domain D with boundary B in three dimensions we may define
and
Let u be the function that minimizes the quotient with no condition prescribed on the boundary B. The Euler–Lagrange equation satisfied by u is
where
The minimizing u must also satisfy the natural boundary condition
on the boundary B. This result depends upon the regularity theory for elliptic partial differential equations; see Jost and Li–Jost (1998) for details. Many extensions, including completeness results, asymptotic properties of the eigenvalues and results concerning the nodes of the eigenfunctions are in Courant and Hilbert (1953).
Applications
Optics
Fermat's principle states that light takes a path that (locally) minimizes the optical length between its endpoints. If the xcoordinate is chosen as the parameter along the path, and along the path, then the optical length is given by
where the refractive index depends upon the material. If we try then the first variation of A (the derivative of A with respect to ε) is
After integration by parts of the first term within brackets, we obtain the Euler–Lagrange equation
The light rays may be determined by integrating this equation. This formalism is used in the context of Lagrangian optics and Hamiltonian optics.
Snell's law
There is a discontinuity of the refractive index when light enters or leaves a lens. Let
where and are constants. Then the Euler–Lagrange equation holds as before in the region where x<0 or x>0, and in fact the path is a straight line there, since the refractive index is constant. At the x=0, f must be continuous, but f' may be discontinuous. After integration by parts in the separate regions and using the Euler–Lagrange equations, the first variation takes the form
The factor multiplying is the sine of angle of the incident ray with the x axis, and the factor multiplying is the sine of angle of the refracted ray with the x axis. Snell's law for refraction requires that these terms be equal. As this calculation demonstrates, Snell's law is equivalent to vanishing of the first variation of the optical path length.
Fermat's principle in three dimensions
It is expedient to use vector notation: let let t be a parameter, let be the parametric representation of a curve C, and let be its tangent vector. The optical length of the curve is given by
Note that this integral is invariant with respect to changes in the parametric representation of C. The Euler–Lagrange equations for a minimizing curve have the symmetric form
where
It follows from the definition that P satisfies
Therefore, the integral may also be written as
This form suggests that if we can find a function ψ whose gradient is given by P, then the integral A is given by the difference of ψ at the endpoints of the interval of integration. Thus the problem of studying the curves that make the integral stationary can be related to the study of the level surfaces of ψ. In order to find such a function, we turn to the wave equation, which governs the propagation of light. This formalism is used in the context of Lagrangian optics and Hamiltonian optics.
Connection with the wave equation
The wave equation for an inhomogeneous medium is
where c is the velocity, which generally depends upon X. Wave fronts for light are characteristic surfaces for this partial differential equation: they satisfy
We may look for solutions in the form
In that case, ψ satisfies
where According to the theory of firstorder partial differential equations, if then P satisfies
along a system of curves (the light rays) that are given by
These equations for solution of a firstorder partial differential equation are identical to the Euler–Lagrange equations if we make the identification
We conclude that the function ψ is the value of the minimizing integral A as a function of the upper end point. That is, when a family of minimizing curves is constructed, the values of the optical length satisfy the characteristic equation corresponding the wave equation. Hence, solving the associated partial differential equation of first order is equivalent to finding families of solutions of the variational problem. This is the essential content of the Hamilton–Jacobi theory, which applies to more general variational problems.
Mechanics
In classical mechanics, the action, S, is defined as the time integral of the Lagrangian, L. The Lagrangian is the difference of energies,
where T is the kinetic energy of a mechanical system and U its potential energy. Hamilton's principle (or the action principle) states that the motion of a conservative holonomic (integrable constraints) mechanical system is such that the action integral
is stationary with respect to variations in the path x(t). The Euler–Lagrange equations for this system are known as Lagrange's equations:
and they are equivalent to Newton's equations of motion (for such systems).
The conjugate momenta P are defined by
For example, if
then
Hamiltonian mechanics results if the conjugate momenta are introduced in place of by a Legendre transformation of the Lagrangian L into the Hamiltonian H defined by
The Hamiltonian is the total energy of the system: H = T + U. Analogy with Fermat's principle suggests that solutions of Lagrange's equations (the particle trajectories) may be described in terms of level surfaces of some function of X. This function is a solution of the Hamilton–Jacobi equation:
Further applications
Further applications of the calculus of variations include the following:
 The derivation of the catenary shape
 Solution to Newton's minimal resistance problem
 Solution to the brachistochrone problem
 Solution to isoperimetric problems
 Calculating geodesics
 Finding minimal surfaces and solving Plateau's problem
 Optimal control
Variations and sufficient condition for a minimum
Calculus of variations is concerned with variations of functionals, which are small changes in the functional's value due to small changes in the function that is its argument. The first variation^{ [l]} is defined as the linear part of the change in the functional, and the second variation^{ [m]} is defined as the quadratic part.^{ [22]}
For example, if J[y] is a functional with the function y = y(x) as its argument, and there is a small change in its argument from y to y + h, where h = h(x) is a function in the same function space as y, then the corresponding change in the functional is
 ^{ [n]}
The functional J[y] is said to be differentiable if
where φ[h] is a linear functional,^{ [o]} h is the norm of h,^{ [p]} and ε → 0 as h → 0. The linear functional φ[h] is the first variation of J[y] and is denoted by,^{ [26]}
The functional J[y] is said to be twice differentiable if
where φ_{1}[h] is a linear functional (the first variation), φ_{2}[h] is a quadratic functional,^{ [q]} and ε → 0 as h → 0. The quadratic functional φ_{2}[h] is the second variation of J[y] and is denoted by,^{ [28]}
The second variation δ^{2}J[h] is said to be strongly positive if
for all h and for some constant k > 0 .^{ [29]}
Using the above definitions, especially the definitions of first variation, second variation, and strongly positive, the following sufficient condition for a minimum of a functional can be stated.
 The functional J[y] has a minimum at y = ŷ if its first variation δJ[h] = 0 at y = ŷ and its second variation δ^{2}J[h] is strongly positive at y = ŷ .^{ [30]} ^{ [r]}^{ [s]}
See also
 First variation
 Isoperimetric inequality
 Variational principle
 Variational bicomplex
 Fermat's principle
 Principle of least action
 Infinitedimensional optimization
 Functional analysis
 Ekeland's variational principle
 Inverse problem for Lagrangian mechanics
 Obstacle problem
 Perturbation methods
 Young measure
 Optimal control
 Direct method in calculus of variations
 Noether's theorem
 De Donder–Weyl theory
 Variational Bayesian methods
 Chaplygin problem
 Nehari manifold
 Hu–Washizu principle
 Luke's variational principle
 Mountain pass theorem
 Category:Variational analysts
 Measures of central tendency as solutions to variational problems
 Stampacchia Medal
 Fermat Prize
 Convenient vector space
Notes
 ^ Whereas elementary calculus is about infinitesimally small changes in the values of functions without changes in the function itself, calculus of variations is about infinitesimally small changes in the function itself, which are called variations.^{ [1]}
 ^ See Harold J. Kushner (2004): regarding Dynamic Programming, "The calculus of variations had related ideas (e.g., the work of Caratheodory, the HamiltonJacobi equation). This led to conflicts with the calculus of variations community."
 ^ The neighborhood of f is the part of the given function space where  y − f < h over the whole domain of the functions, with h a positive number that specifies the size of the neighborhood.^{ [10]}
 ^ Note the difference between the terms extremal and extremum. An extremal is a function that makes a functional an extremum.
 ^ For a sufficient condition, see section Variations and sufficient condition for a minimum.
 ^ The following derivation of the Euler–Lagrange equation corresponds to the derivation on pp. 184–185 of Courant & Hilbert (1953).^{ [14]}
 ^ Note that η(x) and f(x) are evaluated at the same values of x, which is not valid more generally in variational calculus with nonholonomic constraints.
 ^ The product εΦ′(0) is called the first variation of the functional J and is denoted by δJ. Some references define the first variation differently by leaving out the ε factor.
 ^ Note that assuming y is a function of x loses generality; ideally both should be a function of some other parameter. This approach is good solely for instructive purposes.
 ^ As a historical note, this is an axiom of Archimedes. See e.g. Kelland (1843).^{ [15]}
 ^ The resulting controversy over the validity of Dirichlet's principle is explained by Turnbull.^{ [21]}
 ^ The first variation is also called the variation, differential, or first differential.
 ^ The second variation is also called the second differential.
 ^ Note that Δ J[h] and the variations below, depend on both y and h. The argument y has been left out to simplify the notation. For example, Δ J[h] could have been written Δ J[y ; h].^{ [23]}
 ^ A functional φ[h] is said to be linear if φ[αh] = α φ[h] and φ[h_{1} +h_{2}] = φ[h_{1}] + φ[h_{2}] , where h, h_{1}, h_{2} are functions and α is a real number.^{ [24]}
 ^ For a function h = h(x) that is defined for a ≤ x ≤ b, where a and b are real numbers, the norm of h is its maximum absolute value, i.e. h = max h(x) for a ≤ x ≤ b.^{ [25]}
 ^ A functional is said to be quadratic if it is a bilinear functional with two argument functions that are equal. A bilinear functional is a functional that depends on two argument functions and is linear when each argument function in turn is fixed while the other argument function is variable.^{ [27]}

^ For other sufficient conditions, see in
Gelfand & Fomin 2000,
 Chapter 5: "The Second Variation. Sufficient Conditions for a Weak Extremum" – Sufficient conditions for a weak minimum are given by the theorem on p. 116.
 Chapter 6: "Fields. Sufficient Conditions for a Strong Extremum" – Sufficient conditions for a strong minimum are given by the theorem on p. 148.
 ^ One may note the similarity to the sufficient condition for a minimum of a function, where the first derivative is zero and the second derivative is positive.
References
 ^ ^{a} ^{b} Courant & Hilbert 1953, p. 184
 ^ Gelfand, I. M.; Fomin, S. V. (2000). Silverman, Richard A. (ed.). Calculus of variations (Unabridged repr. ed.). Mineola, New York: Dover Publications. p. 3. ISBN 9780486414485.
 ^ ^{a} ^{b} Thiele, Rüdiger (2007). "Euler and the Calculus of Variations". In Bradley, Robert E.; Sandifer, C. Edward (eds.). Leonhard Euler: Life, Work and Legacy. Elsevier. p. 249. ISBN 9780080471297.
 ^ Goldstine, Herman H. (2012). A History of the Calculus of Variations from the 17th through the 19th Century. Springer Science & Business Media. p. 110. ISBN 9781461381068.
 ^ ^{a} ^{b} ^{c} van Brunt, Bruce (2004). The Calculus of Variations. Springer. ISBN 9780387402475.
 ^ ^{a} ^{b} Ferguson, James (2004). "Brief Survey of the History of the Calculus of Variations and its Applications". arXiv: math/0402357.
 ^ Dimitri Bertsekas. Dynamic programming and optimal control. Athena Scientific, 2005.
 ^ Bellman, Richard E. (1954). "Dynamic Programming and a new formalism in the calculus of variations". Proc. Natl. Acad. Sci. 40 (4): 231–235. Bibcode: 1954PNAS...40..231B. doi: 10.1073/pnas.40.4.231. PMC 527981. PMID 16589462.
 ^ "Richard E. Bellman Control Heritage Award". American Automatic Control Council. 2004. Retrieved 20130728.
 ^ Courant, R; Hilbert, D (1953). Methods of Mathematical Physics. I (First English ed.). New York: Interscience Publishers, Inc. p. 169. ISBN 9780471504474.
 ^ Gelfand & Fomin 2000, pp. 12–13
 ^ Gelfand & Fomin 2000, p. 13
 ^ Gelfand & Fomin 2000, pp. 14–15
 ^ Courant, R.; Hilbert, D. (1953). Methods of Mathematical Physics. I (First English ed.). New York: Interscience Publishers, Inc. ISBN 9780471504474.
 ^ Kelland, Philip (1843). Lectures on the principles of demonstrative mathematics. p. 58 – via Google Books.
 ^ Weisstein, Eric W. "Euler–Lagrange Differential Equation". mathworld.wolfram.com. Wolfram. Eq. (5).
 ^ Kot, Mark (2014). "Chapter 4: Basic Generalizations". A First Course in the Calculus of Variations. American Mathematical Society. ISBN 9781470414955.
 ^ Manià, Bernard (1934). "Sopra un esempio di Lavrentieff". Bollenttino dell'Unione Matematica Italiana. 13: 147–153.
 ^ Ball & Mizel (1985). "Onedimensional Variational problems whose Minimizers do not satisfy the EulerLagrange equation". Archive for Rational Mechanics and Analysis. 90 (4): 325–388. Bibcode: 1985ArRMA..90..325B. doi: 10.1007/BF00276295. S2CID 55005550.
 ^ Ferriero, Alessandro (2007). "The Weak Repulsion property". Journal de Mathématiques Pures et Appliquées. 88 (4): 378–388. doi: 10.1016/j.matpur.2007.06.002.
 ^ Turnbull. "Riemann biography". UK: U. St. Andrew.
 ^ Gelfand & Fomin 2000, pp. 11–12, 99
 ^ Gelfand & Fomin 2000, p. 12, footnote 6
 ^ Gelfand & Fomin 2000, p. 8
 ^ Gelfand & Fomin 2000, p. 6
 ^ Gelfand & Fomin 2000, pp. 11–12
 ^ Gelfand & Fomin 2000, pp. 97–98
 ^ Gelfand & Fomin 2000, p. 99
 ^ Gelfand & Fomin 2000, p. 100
 ^ Gelfand & Fomin 2000, p. 100, Theorem 2
Further reading
 Benesova, B. and Kruzik, M.: "Weak Lower Semicontinuity of Integral Functionals and Applications". SIAM Review 59(4) (2017), 703–766.
 Bolza, O.: Lectures on the Calculus of Variations. Chelsea Publishing Company, 1904, available on Digital Mathematics library. 2nd edition republished in 1961, paperback in 2005, ISBN 9781418182014.
 Cassel, Kevin W.: Variational Methods with Applications in Science and Engineering, Cambridge University Press, 2013.
 Clegg, J.C.: Calculus of Variations, Interscience Publishers Inc., 1968.
 Courant, R.: Dirichlet's principle, conformal mapping and minimal surfaces. Interscience, 1950.
 Dacorogna, Bernard: " Introduction" Introduction to the Calculus of Variations, 3rd edition. 2014, World Scientific Publishing, ISBN 9781783265510.
 Elsgolc, L.E.: Calculus of Variations, Pergamon Press Ltd., 1962.
 Forsyth, A.R.: Calculus of Variations, Dover, 1960.
 Fox, Charles: An Introduction to the Calculus of Variations, Dover Publ., 1987.
 Giaquinta, Mariano; Hildebrandt, Stefan: Calculus of Variations I and II, SpringerVerlag, ISBN 9783662032787 and ISBN 9783662062012
 Jost, J. and X. LiJost: Calculus of Variations. Cambridge University Press, 1998.
 Lebedev, L.P. and Cloud, M.J.: The Calculus of Variations and Functional Analysis with Optimal Control and Applications in Mechanics, World Scientific, 2003, pages 1–98.
 Logan, J. David: Applied Mathematics, 3rd edition. WileyInterscience, 2006
 Pike, Ralph W. "Chapter 8: Calculus of Variations". Optimization for Engineering Systems. Louisiana State University. Archived from the original on 20070705.
 Roubicek, T.: " Calculus of variations". Chap.17 in: Mathematical Tools for Physicists. (Ed. M. Grinfeld) J. Wiley, Weinheim, 2014, ISBN 9783527411887, pp. 551–588.
 Sagan, Hans: Introduction to the Calculus of Variations, Dover, 1992.
 Weinstock, Robert: Calculus of Variations with Applications to Physics and Engineering, Dover, 1974 (reprint of 1952 ed.).
External links
 Variational calculus. Encyclopedia of Mathematics.
 calculus of variations. PlanetMath.
 Calculus of Variations. MathWorld.
 Calculus of variations. Example problems.
 Mathematics  Calculus of Variations and Integral Equations. Lectures on YouTube.
 Selected papers on Geodesic Fields. Part I, Part II.