In calculus, the integral of the secant function can be evaluated using a variety of methods and there are multiple ways of expressing the antiderivative, all of which can be shown to be equivalent via
This formula is useful for evaluating various trigonometric integrals. In particular, it can be used to evaluate the
integral of the secant cubed, which, though seemingly special, comes up rather frequently in applications.
Proof that the different antiderivatives are equivalent
The second of these follows by first multiplying top and bottom of the interior fraction by . This gives in the denominator and the result follows by moving the factor of 1/2 into the logarithm as a square root. Leaving out the constant of integration for now,
The third form follows by replacing by and expanding using the
identities for . It may also be obtained directly by means of the following substitutions:
The conventional solution for the
Mercator projection ordinate may be written without the modulus signs since the latitude lies between and ,
The integral of the secant function was one of the "outstanding open problems of the mid-seventeenth century", solved in 1668 by
James Gregory. He applied his result to a problem concerning nautical tables. In 1599,
Edward Wright evaluated the
numerical methods – what today we would call
Riemann sums. He wanted the solution for the purposes of
cartography – specifically for constructing an accurate
Mercator projection. In the 1640s, Henry Bond, a teacher of navigation, surveying, and other mathematical topics, compared Wright's numerically computed table of values of the integral of the
secant with a table of logarithms of the tangent function, and consequently conjectured that
A standard method of evaluating the secant integral presented in various references involves multiplying the numerator and denominator by and then substituting the following to the resulting expression: and . This substitution can be obtained from the derivatives of secant and tangent added together, which have secant as a common factor.
adding them gives
The derivative of the sum is thus equal to the sum multiplied by . This enables multiplying by in the numerator and denominator and performing the following substitutions: and .
The integral is evaluated as follows:
as claimed. This was the formula discovered by James Gregory.
By partial fractions and a substitution (Barrow's approach)
Although Gregory proved the conjecture in 1668 in his Exercitationes Geometricae, the proof was presented in a form that renders it nearly impossible for modern readers to comprehend;
Isaac Barrow, in his Geometrical Lectures of 1670, gave the first "intelligible" proof, though even that was "couched in the geometric idiom of the day." Barrow's proof of the result was the earliest use of
partial fractions in integration. Adapted to modern notation, Barrow's proof began as follows:
by the double-angle formulas. As for the integral of the secant function,
The integral can also be derived by using the a somewhat non-standard version of the Weierstrass substitution, which is simpler in the case of this particular integral, published in 2013, is as follows:
By two successive substitutions
The integral can also be solved by manipulating the integrand and substituting twice. Using the definition , the integral can be rewritten as
Using the identity , the integrand can be written as
Substituting for reduces the integral to
The reduced integral can be evaluated by substituting for and using the identity .
The integral is now reduced to a simple integral and back-substituting gives
which is one of the hyperbolic forms of the integral.
A similar strategy can be used to integrate the cosecant, hyperbolic secant, and hyperbolic cosecant functions.
Gudermannian and Lambertian
The integral of the secant function defines the Lambertian function, which is the inverse of the
This is encountered in the theory of map projections: the
Mercator projection of a point with longitude θ and latitude φ may be written as:
^Edward Wright, Certaine Errors in Navigation, Arising either of the ordinaire erroneous making or vsing of the sea Chart, Compasse, Crosse staffe, and Tables of declination of the Sunne, and fixed Starres detected and corrected, Valentine Simms, London, 1599.
^H. W. Turnbull, editor, The Correspondence of Isaac Newton, Cambridge University Press, 1959–1960, volume 1, pages 13–16 and volume 2, pages 99–100.
^D. T. Whiteside, editor, The Mathematical Papers of Isaac Newton, Cambridge University Press, 1967, volume 1, pages 466–467 and 473–475.