Introduction to the exponential integrals
General
The exponential‐type integrals have a long history. After the early developments of differential calculus, mathematicians tried to evaluate integrals containing simple elementary functions, especially integrals that often appeared during investigations of physical problems. Despite the relatively simple form of the integrands, some of these integrals could not be evaluated through known functions. Examples of integrals that could not be evaluated in known functions are:




L. Euler (1768) introduced the first integral shown in the preceding list. Later L. Mascheroni (1790, 1819) used it and introduced the second and third integrals, and A. M. Legendre (1811) introduced the last integral shown. T. Caluso (1805) used the first integral in an article and J. von Soldner (1809) introduced its notation through symbol li. F. W. Bessel (1812) used the second and third integrals. C. A. Bretschneider (1843) not only used the second and third integrals, but also introduced similar integrals for the hyperbolic functions:
O. Schlömilch (1846) and F. Arndt (1847) widely used such integrals containing the exponential and trigonometric functions. For the exponential, sine, and cosine integrals, J. W. L. Glaisher (1870) introduced the notations , , and . H. Amstein (1895) introduced the branch cut for the logarithmic integral with a complex argument. N. Nielsen (1904) used the notations and for corresponding integrals.
Different notations are used for the previous definite integrals by various authors when they are integrated from to or from to .
Definitions of exponential integrals
The exponential integral , exponential integral , logarithmic integral , sine integral , hyperbolic sine integral , cosine integral , and hyperbolic cosine integral are defined as the following definite integrals, including the Euler gamma constant :
The previous integrals are all interrelated and are called exponential integrals.
Instead of the above classical definitions through definite integrals, equivalent definitions through infinite series can be used, for example, the exponential integral can be defined by the following formula (see the following sections for the corresponding series for the other integrals):
A quick look at the exponential integrals Here is a quick look at the graphics for the exponential integrals along the real axis.
Connections within the group of exponential integrals and with other function groups
Representations through more general functions
The exponential integrals , , , , , , and are the particular cases of the more general hypergeometric and Meijer G functions.
For example, they can be represented through hypergeometric functions or the Tricomi confluent hypergeometric function :
Representations of the exponential integrals and , the sine and cosine integrals and , and the hyperbolic sine and cosine integrals and through classical Meijer G functions are rather simple:
Here is the Euler gamma constant and the complicated‐looking expression containing the two logarithm simplifies piecewise:
But the last four formulas that contain the Meijer G function can be simplified further by changing the classical Meijer functions to the generalized one. These formulas do not include factors and terms :
The corresponding representations of the logarithmic integral through the classical Meijer G function is more complicated and includes composition of the G function and a logarithmic function:
All six exponential integrals of one variable are the particular cases of the incomplete gamma function:
Representations through related equivalent functions
The exponential integral can be represented through the incomplete gamma function or the regularized incomplete gamma function:
Relations to inverse functions
The exponential integral is connected with the inverse of the regularized incomplete gamma function by the following formula:
Representations through other exponential integrals
The exponential integrals , , , , , , and are interconnected through the following formulas:
The bestknown properties and formulas for exponential integrals
Real values for real arguments
For real values of parameter and positive argument , the values of the exponential integral are real (or infinity). For real values of argument , the values of the exponential integral , the sine integral , and the hyperbolic sine integral are real. For real positive values of argument , the values of the logarithmic integral , the cosine integral , and the hyperbolic cosine integral are real.
Simple values at zero
The exponential integrals have rather simple values for argument :
Specific values for specialized parameter
If the parameter equals , the exponential integral can be expressed through an exponential function multiplied by a simple rational function. If the parameter equals , the exponential integral can be expressed through the exponential integral , and the exponential and logarithmic functions:
The previous formulas are the particular cases of the following general formula:
If the parameter equals , the exponential integral can be expressed through the probability integral , and the exponential and power functions, for example:
The previous formulas can be generalized by the following general representation of this class of particular cases:
Analyticity
The exponential integrals , , , , , , and are defined for all complex values of the parameter and the variable . The function is an analytical functions of and over the whole complex ‐ and ‐planes excluding the branch cut on the ‐plane. For fixed , the exponential integral is an entire function of . The sine integral and the hyperbolic sine integral are entire functions of .
Poles and essential singularities
For fixed , the function has an essential singularity at . At the same time, the point is a branch point for generic . For fixed , the function has only one singular point at . It is an essential singular point.
The exponential integral , the cosine integral , and the hyperbolic cosine integral have an essential singularity at .
The function does not have poles and essential singularities.
The sine integral and the hyperbolic sine integral have an essential singularity at .
Branch points and branch cuts
For fixed , the function does not have branch points and branch cuts.
For fixed , not being a nonpositive integer, the function has two branch points and , and branch cuts along the interval . At the same time, the point is an essential singularity for this function.
The exponential integral , the cosine integral, and the hyperbolic cosine integral have two branch points and .
The function has three branch points , , and .
The sine integral and hyperbolic sine integral do not have branch points or branch cuts.
For fixed , not being a nonpositive integer, the function is a single‐valued function on the ‐plane cut along the interval , where it is continuous from above:
The function is a single‐valued function on the ‐plane cut along the interval , where it has discontinuities from both sides:
The function is a single‐valued function on the ‐plane cut along the interval . It is continuous from above along the interval and it has discontinuities from both sides along the interval :
The cosine integral and hyperbolic cosine integral are single‐valued functions on the ‐plane cut along the interval where they are continuous from above:
From below, these functions have discontinuity that are described by the formulas:
Periodicity
The exponential integrals , , , , , , and do not have periodicity.
Parity and symmetry
The exponential integral has mirror symmetry:
The sine integral and the hyperbolic sine integral are odd functions and have mirror symmetry:
The exponential integral , logarithmic integral , cosine integral , and hyperbolic cosine integral have mirror symmetry (except on the branch cut interval (∞, 0)):
Series representations
The exponential integrals , , , , , , and have the following series expansions through series that converge on the whole ‐plane:
Interestingly, closed‐form expressions for the truncated version of the Taylor series at the origin can be expressed through the generalized hypergeometric function , for example:
Asymptotic series expansions
The asymptotic behavior of the exponential integrals , , , , , , and can be described by the following formulas (only the main terms of the asymptotic expansions are given):
The previous formulas are valid in any direction of approaching point to infinity (z∞). In particular cases, these formulas can be simplified to the following relations:
Integral representations
The exponential integrals , , , and can also be represented through the following equivalent integrals:
The symbol in the second and third integrals means that these integrals evaluate as the Cauchy principal value of the singular integral:
.
Transformations
The arguments of the exponential integrals , , , , and that contain square roots can sometimes be simplified:
Identities
The exponential integral satisfies the following recurrence identities:
All of the preceding formulas can be generalized to the following recurrence identities with a jump of length :
Simple representations of derivatives
The derivative of the exponential integral with respect to the variable has a simple representation through itself, but with a different parameter:
The derivative of the exponential integral by its parameter can be represented through the regularized hypergeometric function :
The derivatives of the other exponential integrals , , , , , and have simple representations through simple elementary functions:
The symbolic order derivatives with respect to the variable of all exponential integrals , , , , , , and have the following representations:
Differential equations
The exponential integrals , , , , , and satisfy the following linear differential equations of second or third orders:
where , , and are arbitrary constants.
The logarithmic integral satisfies the following ordinary secondorder nonlinear differential equation:
Applications of exponential integrals
Applications of exponential integrals include number theory, quantum field theory, Gibbs phenomena, and solutions of Laplace equations in semiconductor physics.
