Carlson symmetric form
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In mathematics, the Carlson symmetric forms of
elliptic integral In integral calculus, an elliptic integral is one of a number of related functions defined as the value of certain integrals, which were first studied by Giulio Fagnano and Leonhard Euler (). Their name originates from their originally arising in ...
s are a small canonical set of elliptic integrals to which all others may be reduced. They are a modern alternative to the Legendre forms. The Legendre forms may be expressed in terms of the Carlson forms and vice versa. The Carlson elliptic integrals are: R_F(x,y,z) = \tfrac\int_0^\infty \frac R_J(x,y,z,p) = \tfrac\int_0^\infty \frac R_C(x,y) = R_F(x,y,y) = \tfrac \int_0^\infty \frac R_D(x,y,z) = R_J(x,y,z,z) = \tfrac \int_0^\infty \frac Since R_C and R_D are special cases of R_F and R_J, all elliptic integrals can ultimately be evaluated in terms of just R_F and R_J. The term ''symmetric'' refers to the fact that in contrast to the Legendre forms, these functions are unchanged by the exchange of certain subsets of their arguments. The value of R_F(x,y,z) is the same for any permutation of its arguments, and the value of R_J(x,y,z,p) is the same for any permutation of its first three arguments. The Carlson elliptic integrals are named after Bille C. Carlson (1924-2013).


Relation to the Legendre forms


Incomplete elliptic integrals

Incomplete
elliptic integral In integral calculus, an elliptic integral is one of a number of related functions defined as the value of certain integrals, which were first studied by Giulio Fagnano and Leonhard Euler (). Their name originates from their originally arising in ...
s can be calculated easily using Carlson symmetric forms: :F(\phi,k)=\sin\phi R_F\left(\cos^2\phi,1-k^2\sin^2\phi,1\right) :E(\phi,k)=\sin\phi R_F\left(\cos^2\phi,1-k^2\sin^2\phi,1\right) -\tfrack^2\sin^3\phi R_D\left(\cos^2\phi,1-k^2\sin^2\phi,1\right) :\Pi(\phi,n,k)=\sin\phi R_F\left(\cos^2\phi,1-k^2\sin^2\phi,1\right)+ \tfracn\sin^3\phi R_J\left(\cos^2\phi,1-k^2\sin^2\phi,1,1-n\sin^2\phi\right) (Note: the above are only valid for -\frac2\le\phi\le\frac2 and 0\le k^2\sin^2\phi\le1)


Complete elliptic integrals

Complete
elliptic integral In integral calculus, an elliptic integral is one of a number of related functions defined as the value of certain integrals, which were first studied by Giulio Fagnano and Leonhard Euler (). Their name originates from their originally arising in ...
s can be calculated by substituting φ = π: :K(k)=R_F\left(0,1-k^2,1\right) :E(k)=R_F\left(0,1-k^2,1\right)-\tfrack^2 R_D\left(0,1-k^2,1\right) :\Pi(n,k)=R_F\left(0,1-k^2,1\right)+\tfracn R_J \left(0,1-k^2,1,1-n\right)


Special cases

When any two, or all three of the arguments of R_F are the same, then a substitution of \sqrt = u renders the integrand rational. The integral can then be expressed in terms of elementary transcendental functions. :R_(x,y) = R_(x,y,y) = \frac \int _^ \frac = \int _^ \frac = \begin \frac, & x < y \\ \frac, & x = y \\ \frac, & x > y \\ \end Similarly, when at least two of the first three arguments of R_J are the same, :R_(x,y,y,p) = 3 \int _^ \frac = \begin \frac (R_(x,y) - R_(x,p)), & y \ne p \\ \frac \left( R_(x,y) - \frac \sqrt\right), & y = p \ne x \\ \frac, &y = p = x \\ \end


Properties


Homogeneity

By substituting in the integral definitions t = \kappa u for any constant \kappa, it is found that :R_F\left(\kappa x,\kappa y,\kappa z\right)=\kappa^R_F(x,y,z) :R_J\left(\kappa x,\kappa y,\kappa z,\kappa p\right)=\kappa^R_J(x,y,z,p)


Duplication theorem

:R_F(x,y,z)=2R_F(x+\lambda,y+\lambda,z+\lambda)= R_F\left(\frac,\frac,\frac\right), where \lambda=\sqrt\sqrt+\sqrt\sqrt+\sqrt\sqrt. :\beginR_(x,y,z,p) & = 2 R_(x + \lambda,y + \lambda,z + \lambda,p + \lambda) + 6 R_(d^,d^ + (p - x) (p - y) (p - z)) \\ & = \frac R_\left( \frac,\frac,\frac,\frac\right) + 6 R_(d^,d^ + (p - x) (p - y) (p - z)) \end where d = (\sqrt + \sqrt) (\sqrt + \sqrt) (\sqrt + \sqrt) and \lambda =\sqrt\sqrt+\sqrt\sqrt+\sqrt\sqrt


Series Expansion

In obtaining a
Taylor series In mathematics, the Taylor series or Taylor expansion of a function is an infinite sum of terms that are expressed in terms of the function's derivatives at a single point. For most common functions, the function and the sum of its Taylor ser ...
expansion for R_ or R_ it proves convenient to expand about the mean value of the several arguments. So for R_, letting the mean value of the arguments be A = (x + y + z)/3, and using homogeneity, define \Delta x, \Delta y and \Delta z by :\beginR_(x,y,z) & = R_(A (1 - \Delta x),A (1 - \Delta y),A (1 - \Delta z)) \\ & = \frac R_(1 - \Delta x,1 - \Delta y,1 - \Delta z) \end that is \Delta x = 1 - x/A etc. The differences \Delta x, \Delta y and \Delta z are defined with this sign (such that they are ''subtracted''), in order to be in agreement with Carlson's papers. Since R_(x,y,z) is symmetric under permutation of x, y and z, it is also symmetric in the quantities \Delta x, \Delta y and \Delta z. It follows that both the integrand of R_ and its integral can be expressed as functions of the
elementary symmetric polynomial In mathematics, specifically in commutative algebra, the elementary symmetric polynomials are one type of basic building block for symmetric polynomials, in the sense that any symmetric polynomial can be expressed as a polynomial in elementary sy ...
s in \Delta x, \Delta y and \Delta z which are :E_ = \Delta x + \Delta y + \Delta z = 0 :E_ = \Delta x \Delta y + \Delta y \Delta z + \Delta z \Delta x :E_ = \Delta x \Delta y \Delta z Expressing the integrand in terms of these polynomials, performing a multidimensional Taylor expansion and integrating term-by-term... :\beginR_(x,y,z) & = \frac \int _^\frac dt \\ & = \frac \int _^\left( \frac - \frac + \frac + \frac - \frac + O(E_) + O(\Delta^)\right) dt \\ & = \frac \left( 1 - \frac E_ + \frac E_ + \frac E_^ - \frac E_ E_ + O(E_) + O(\Delta^)\right) \end The advantage of expanding about the mean value of the arguments is now apparent; it reduces E_ identically to zero, and so eliminates all terms involving E_ - which otherwise would be the most numerous. An ascending series for R_ may be found in a similar way. There is a slight difficulty because R_ is not fully symmetric; its dependence on its fourth argument, p, is different from its dependence on x, y and z. This is overcome by treating R_ as a fully symmetric function of ''five'' arguments, two of which happen to have the same value p. The mean value of the arguments is therefore taken to be :A = \frac and the differences \Delta x, \Delta y \Delta z and \Delta p defined by :\beginR_(x,y,z,p) & = R_(A (1 - \Delta x),A (1 - \Delta y),A (1 - \Delta z),A (1 - \Delta p)) \\ & = \frac R_(1 - \Delta x,1 - \Delta y,1 - \Delta z,1 - \Delta p) \end The
elementary symmetric polynomial In mathematics, specifically in commutative algebra, the elementary symmetric polynomials are one type of basic building block for symmetric polynomials, in the sense that any symmetric polynomial can be expressed as a polynomial in elementary sy ...
s in \Delta x, \Delta y, \Delta z, \Delta p and (again) \Delta p are in full :E_ = \Delta x + \Delta y + \Delta z + 2 \Delta p = 0 :E_ = \Delta x \Delta y + \Delta y \Delta z + 2 \Delta z \Delta p + \Delta p^ + 2 \Delta p \Delta x + \Delta x \Delta z + 2 \Delta y \Delta p :E_ = \Delta z \Delta p^ + \Delta x \Delta p^ + 2 \Delta x \Delta y \Delta p + \Delta x \Delta y \Delta z + 2 \Delta y \Delta z \Delta p + \Delta y \Delta p^ + 2 \Delta x \Delta z \Delta p :E_ = \Delta y \Delta z \Delta p^ + \Delta x \Delta z \Delta p^ + \Delta x \Delta y \Delta p^ + 2 \Delta x \Delta y \Delta z \Delta p :E_ = \Delta x \Delta y \Delta z \Delta p^ However, it is possible to simplify the formulae for E_, E_ and E_ using the fact that E_ = 0. Expressing the integrand in terms of these polynomials, performing a multidimensional Taylor expansion and integrating term-by-term as before... :\beginR_(x,y,z,p) & = \frac \int _^\frac dt \\ & = \frac \int _^\left( \frac - \frac + \frac + \frac + \frac + O(E_) + O(\Delta^)\right) dt \\ & = \frac \left( 1 - \frac E_ + \frac E_ + \frac E_^ - \frac E_ - \frac E_ E_ + \frac E_ + O(E_) + O(\Delta^)\right) \end As with R_, by expanding about the mean value of the arguments, more than half the terms (those involving E_) are eliminated.


Negative arguments

In general, the arguments x, y, z of Carlson's integrals may not be real and negative, as this would place a
branch point In the mathematical field of complex analysis, a branch point of a multi-valued function (usually referred to as a "multifunction" in the context of complex analysis) is a point such that if the function is n-valued (has n values) at that point, ...
on the path of integration, making the integral ambiguous. However, if the second argument of R_C, or the fourth argument, p, of R_J is negative, then this results in a simple pole on the path of integration. In these cases the
Cauchy principal value In mathematics, the Cauchy principal value, named after Augustin Louis Cauchy, is a method for assigning values to certain improper integrals which would otherwise be undefined. Formulation Depending on the type of singularity in the integrand ...
(finite part) of the integrals may be of interest; these are :\mathrm\; R_C(x, -y) = \sqrt\,R_C(x + y, y), and :\begin\mathrm\; R_(x,y,z,-p) & = \frac \\ & = \frac \end where :q = y + \frac. which must be greater than zero for R_(x,y,z,q) to be evaluated. This may be arranged by permuting x, y and z so that the value of y is between that of x and z.


Numerical evaluation

The duplication theorem can be used for a fast and robust evaluation of the Carlson symmetric form of elliptic integrals and therefore also for the evaluation of Legendre-form of elliptic integrals. Let us calculate R_F(x,y,z): first, define x_0=x, y_0=y and z_0=z. Then iterate the series :\lambda_n=\sqrt\sqrt+\sqrt\sqrt+\sqrt\sqrt, :x_=\frac, y_=\frac, z_=\frac until the desired precision is reached: if x, y and z are non-negative, all of the series will converge quickly to a given value, say, \mu. Therefore, :R_F\left(x,y,z\right)=R_F\left(\mu,\mu,\mu\right)=\mu^. Evaluating R_C(x,y) is much the same due to the relation :R_C\left(x,y\right)=R_F\left(x,y,y\right).


References and External links


B. C. Carlson, John L. Gustafson 'Asymptotic approximations for symmetric elliptic integrals' 1993 arXivB. C. Carlson 'Numerical Computation of Real Or Complex Elliptic Integrals' 1994 arXivB. C. Carlson 'Elliptic Integrals:Symmetric Integrals' in Chap. 19 of ''Digital Library of Mathematical Functions''. Release date 2010-05-07. National Institute of Standards and Technology.'Profile: Bille C. Carlson' in ''Digital Library of Mathematical Functions''. National Institute of Standards and Technology.
*{{Citation , last1=Press , first1=WH , last2=Teukolsky , first2=SA , last3=Vetterling , first3=WT , last4=Flannery , first4=BP , year=2007 , title=Numerical Recipes: The Art of Scientific Computing , edition=3rd , publisher=Cambridge University Press , publication-place=New York , isbn=978-0-521-88068-8 , chapter=Section 6.12. Elliptic Integrals and Jacobian Elliptic Functions , chapter-url=http://apps.nrbook.com/empanel/index.html#pg=309 * Fortran code from
SLATEC SLATEC Common Mathematical Library is a FORTRAN 77 library of over 1400 general purpose mathematical and statistical routines. The code was developed at US Government research laboratories and is therefore public domain software. "SLATEC" is an a ...
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Elliptic functions