In mathematics, the error function (also called the Gauss error function), often denoted by erf, is a function ${\displaystyle \mathrm {erf} :\mathbb {C} \to \mathbb {C} }$ defined as:^[1] $${\displaystyle \operatorname {erf} z={\frac {2}{\sqrt {\pi }}}\int _{0}^{z}e^{-t^{2}}\,\mathrm {d} t.}$$

Error function
Plot of the error function over real numbers
General information
General definition	${\displaystyle \operatorname {erf} z={\frac {2}{\sqrt {\pi }}}\int _{0}^{z}e^{-t^{2}}\,\mathrm {d} t}$
Fields of application	Probability, thermodynamics, digital communications
Domain, codomain and image
Domain	${\displaystyle \mathbb {R} }$
Image	${\displaystyle \left(-1,1\right)}$
Basic features
Parity	Odd
Specific features
Root	0
Derivative	${\displaystyle {\frac {\mathrm {d} }{\mathrm {d} z}}\operatorname {erf} z={\frac {2}{\sqrt {\pi }}}e^{-z^{2}}}$
Antiderivative	${\displaystyle \int \operatorname {erf} z\,dz=z\operatorname {erf} z+{\frac {e^{-z^{2}}}{\sqrt {\pi }}}+C}$
Series definition
Taylor series	${\displaystyle \operatorname {erf} z={\frac {2}{\sqrt {\pi }}}\sum _{n=0}^{\infty }{\frac {z}{2n+1}}\prod _{k=1}^{n}{\frac {-z^{2}}{k}}}$

The integral here is a complex contour integral which is path-independent because ${\displaystyle \exp(-t^{2})}$ is holomorphic on the whole complex plane ${\displaystyle \mathbb {C} }$. In many applications, the function argument is a real number, in which case the function value is also real.

In some old texts,^[2] the error function is defined without the factor of ${\displaystyle 2/{\sqrt {\pi }}}$. This nonelementary integral is a sigmoid function that occurs often in probability, statistics, and partial differential equations.

In statistics, for non-negative real values of x, the error function has the following interpretation: for a real random variable Y that is normally distributed with mean 0 and standard deviation ${\displaystyle 1/{\sqrt {2}}}$, erf x is the probability that Y falls in the range [−x, x].

Two closely related functions are the complementary error function ${\displaystyle \mathrm {erfc} :\mathbb {C} \to \mathbb {C} }$ is defined as

$${\displaystyle \operatorname {erfc} z=1-\operatorname {erf} z,}$$

and the imaginary error function ${\displaystyle \mathrm {erfi} :\mathbb {C} \to \mathbb {C} }$ is defined as

$${\displaystyle \operatorname {erfi} z=-i\operatorname {erf} iz,}$$

where i is the imaginary unit.

The name "error function" and its abbreviation erf were proposed by J. W. L. Glaisher in 1871 on account of its connection with "the theory of Probability, and notably the theory of Errors."^[3] The error function complement was also discussed by Glaisher in a separate publication in the same year.^[4] For the "law of facility" of errors whose density is given by $${\displaystyle f(x)=\left({\frac {c}{\pi }}\right)^{1/2}e^{-cx^{2}}}$$ (the normal distribution), Glaisher calculates the probability of an error lying between p and q as: $${\displaystyle \left({\frac {c}{\pi }}\right)^{\frac {1}{2}}\int _{p}^{q}e^{-cx^{2}}\,\mathrm {d} x={\tfrac {1}{2}}\left(\operatorname {erf} \left(q{\sqrt {c}}\right)-\operatorname {erf} \left(p{\sqrt {c}}\right)\right).}$$

When the results of a series of measurements are described by a normal distribution with standard deviation σ and expected value 0, then erf (⁠a/σ √2⁠) is the probability that the error of a single measurement lies between −a and +a, for positive a. This is useful, for example, in determining the bit error rate of a digital communication system.

The error and complementary error functions occur, for example, in solutions of the heat equation when boundary conditions are given by the Heaviside step function.

The error function and its approximations can be used to estimate results that hold with high probability or with low probability. Given a random variable X ~ Norm[μ,σ] (a normal distribution with mean μ and standard deviation σ) and a constant L > μ, it can be shown via integration by substitution: $${\displaystyle {\begin{aligned}\Pr[X\leq L]&={\frac {1}{2}}+{\frac {1}{2}}\operatorname {erf} {\frac {L-\mu }{{\sqrt {2}}\sigma }}\\&\approx A\exp \left(-B\left({\frac {L-\mu }{\sigma }}\right)^{2}\right)\end{aligned}}}$$

where A and B are certain numeric constants. If L is sufficiently far from the mean, specifically μ − L ≥ σ√ln k, then:

$${\displaystyle \Pr[X\leq L]\leq A\exp(-B\ln {k})={\frac {A}{k^{B}}}}$$

so the probability goes to 0 as k → ∞.

The probability for X being in the interval [L_a, L_b] can be derived as $${\displaystyle {\begin{aligned}\Pr[L_{a}\leq X\leq L_{b}]&=\int _{L_{a}}^{L_{b}}{\frac {1}{{\sqrt {2\pi }}\sigma }}\exp \left(-{\frac {(x-\mu )^{2}}{2\sigma ^{2}}}\right)\,\mathrm {d} x\\&={\frac {1}{2}}\left(\operatorname {erf} {\frac {L_{b}-\mu }{{\sqrt {2}}\sigma }}-\operatorname {erf} {\frac {L_{a}-\mu }{{\sqrt {2}}\sigma }}\right).\end{aligned}}}$$

Plots in the complex plane

Integrand exp(−z²)

erf z

The property erf (−z) = −erf z means that the error function is an odd function. This directly results from the fact that the integrand e^−t2 is an even function (the antiderivative of an even function which is zero at the origin is an odd function and vice versa).

Since the error function is an entire function which takes real numbers to real numbers, for any complex number z: $${\displaystyle \operatorname {erf} {\overline {z}}={\overline {\operatorname {erf} z}}}$$ where z is the complex conjugate of z.

The integrand f = exp(−z²) and f = erf z are shown in the complex z-plane in the figures at right with domain coloring.

The error function at +∞ is exactly 1 (see Gaussian integral). At the real axis, erf z approaches unity at z → +∞ and −1 at z → −∞. At the imaginary axis, it tends to ±i∞.

The error function is an entire function; it has no singularities (except that at infinity) and its Taylor expansion always converges. For x >> 1, however, cancellation of leading terms makes the Taylor expansion unpractical.

The defining integral cannot be evaluated in closed form in terms of elementary functions (see Liouville's theorem), but by expanding the integrand e^−z2 into its Maclaurin series and integrating term by term, one obtains the error function's Maclaurin series as: $${\displaystyle {\begin{aligned}\operatorname {erf} z&={\frac {2}{\sqrt {\pi }}}\sum _{n=0}^{\infty }{\frac {(-1)^{n}z^{2n+1}}{n!(2n+1)}}\\[6pt]&={\frac {2}{\sqrt {\pi }}}\left(z-{\frac {z^{3}}{3}}+{\frac {z^{5}}{10}}-{\frac {z^{7}}{42}}+{\frac {z^{9}}{216}}-\cdots \right)\end{aligned}}}$$ which holds for every complex number z. The denominator terms are sequence A007680 in the OEIS.

For iterative calculation of the above series, the following alternative formulation may be useful: $${\displaystyle {\begin{aligned}\operatorname {erf} z&={\frac {2}{\sqrt {\pi }}}\sum _{n=0}^{\infty }\left(z\prod _{k=1}^{n}{\frac {-(2k-1)z^{2}}{k(2k+1)}}\right)\\[6pt]&={\frac {2}{\sqrt {\pi }}}\sum _{n=0}^{\infty }{\frac {z}{2n+1}}\prod _{k=1}^{n}{\frac {-z^{2}}{k}}\end{aligned}}}$$ because ⁠−(2k − 1)z²/k(2k + 1)⁠ expresses the multiplier to turn the kth term into the (k + 1)th term (considering z as the first term).

The imaginary error function has a very similar Maclaurin series, which is: $${\displaystyle {\begin{aligned}\operatorname {erfi} z&={\frac {2}{\sqrt {\pi }}}\sum _{n=0}^{\infty }{\frac {z^{2n+1}}{n!(2n+1)}}\\[6pt]&={\frac {2}{\sqrt {\pi }}}\left(z+{\frac {z^{3}}{3}}+{\frac {z^{5}}{10}}+{\frac {z^{7}}{42}}+{\frac {z^{9}}{216}}+\cdots \right)\end{aligned}}}$$ which holds for every complex number z.

The derivative of the error function follows immediately from its definition: $${\displaystyle {\frac {\mathrm {d} }{\mathrm {d} z}}\operatorname {erf} z={\frac {2}{\sqrt {\pi }}}e^{-z^{2}}.}$$ From this, the derivative of the imaginary error function is also immediate: $${\displaystyle {\frac {d}{dz}}\operatorname {erfi} z={\frac {2}{\sqrt {\pi }}}e^{z^{2}}.}$$ An antiderivative of the error function, obtainable by integration by parts, is $${\displaystyle z\operatorname {erf} z+{\frac {e^{-z^{2}}}{\sqrt {\pi }}}.}$$ An antiderivative of the imaginary error function, also obtainable by integration by parts, is $${\displaystyle z\operatorname {erfi} z-{\frac {e^{z^{2}}}{\sqrt {\pi }}}.}$$ Higher order derivatives are given by $${\displaystyle \operatorname {erf} ^{(k)}z={\frac {2(-1)^{k-1}}{\sqrt {\pi }}}{\mathit {H}}_{k-1}(z)e^{-z^{2}}={\frac {2}{\sqrt {\pi }}}{\frac {\mathrm {d} ^{k-1}}{\mathrm {d} z^{k-1}}}\left(e^{-z^{2}}\right),\qquad k=1,2,\dots }$$ where H are the physicists' Hermite polynomials.^[5]

An expansion,^[6] which converges more rapidly for all real values of x than a Taylor expansion, is obtained by using Hans Heinrich Bürmann's theorem:^[7] $${\displaystyle {\begin{aligned}\operatorname {erf} x&={\frac {2}{\sqrt {\pi }}}\operatorname {sgn} x\cdot {\sqrt {1-e^{-x^{2}}}}\left(1-{\frac {1}{12}}\left(1-e^{-x^{2}}\right)-{\frac {7}{480}}\left(1-e^{-x^{2}}\right)^{2}-{\frac {5}{896}}\left(1-e^{-x^{2}}\right)^{3}-{\frac {787}{276480}}\left(1-e^{-x^{2}}\right)^{4}-\cdots \right)\\[10pt]&={\frac {2}{\sqrt {\pi }}}\operatorname {sgn} x\cdot {\sqrt {1-e^{-x^{2}}}}\left({\frac {\sqrt {\pi }}{2}}+\sum _{k=1}^{\infty }c_{k}e^{-kx^{2}}\right).\end{aligned}}}$$ where sgn is the sign function. By keeping only the first two coefficients and choosing c₁ = ⁠31/200⁠ and c₂ = −⁠341/8000⁠, the resulting approximation shows its largest relative error at x = ±1.3796, where it is less than 0.0036127: $${\displaystyle \operatorname {erf} x\approx {\frac {2}{\sqrt {\pi }}}\operatorname {sgn} x\cdot {\sqrt {1-e^{-x^{2}}}}\left({\frac {\sqrt {\pi }}{2}}+{\frac {31}{200}}e^{-x^{2}}-{\frac {341}{8000}}e^{-2x^{2}}\right).}$$

Given a complex number z, there is not a unique complex number w satisfying erf w = z, so a true inverse function would be multivalued. However, for −1 < x < 1, there is a unique real number denoted erf⁻¹ x satisfying $${\displaystyle \operatorname {erf} \left(\operatorname {erf} ^{-1}x\right)=x.}$$

The inverse error function is usually defined with domain (−1,1), and it is restricted to this domain in many computer algebra systems. However, it can be extended to the disk |z| < 1 of the complex plane, using the Maclaurin series^[8] $${\displaystyle \operatorname {erf} ^{-1}z=\sum _{k=0}^{\infty }{\frac {c_{k}}{2k+1}}\left({\frac {\sqrt {\pi }}{2}}z\right)^{2k+1},}$$ where c₀ = 1 and $${\displaystyle {\begin{aligned}c_{k}&=\sum _{m=0}^{k-1}{\frac {c_{m}c_{k-1-m}}{(m+1)(2m+1)}}\\[1ex]&=\left\{1,1,{\frac {7}{6}},{\frac {127}{90}},{\frac {4369}{2520}},{\frac {34807}{16200}},\ldots \right\}.\end{aligned}}}$$

So we have the series expansion (common factors have been canceled from numerators and denominators): $${\displaystyle \operatorname {erf} ^{-1}z={\frac {\sqrt {\pi }}{2}}\left(z+{\frac {\pi }{12}}z^{3}+{\frac {7\pi ^{2}}{480}}z^{5}+{\frac {127\pi ^{3}}{40320}}z^{7}+{\frac {4369\pi ^{4}}{5806080}}z^{9}+{\frac {34807\pi ^{5}}{182476800}}z^{11}+\cdots \right).}$$ (After cancellation the numerator and denominator values in OEIS: A092676 and OEIS: A092677 respectively; without cancellation the numerator terms are values in OEIS: A002067.) The error function's value at ±∞ is equal to ±1.

For |z| < 1, we have erf(erf⁻¹ z) = z.

The inverse complementary error function is defined as $${\displaystyle \operatorname {erfc} ^{-1}(1-z)=\operatorname {erf} ^{-1}z.}$$ For real x, there is a unique real number erfi⁻¹ x satisfying erfi(erfi⁻¹ x) = x. The inverse imaginary error function is defined as erfi⁻¹ x.^[9]

For any real x, Newton's method can be used to compute erfi⁻¹ x, and for −1 ≤ x ≤ 1, the following Maclaurin series converges: $${\displaystyle \operatorname {erfi} ^{-1}z=\sum _{k=0}^{\infty }{\frac {(-1)^{k}c_{k}}{2k+1}}\left({\frac {\sqrt {\pi }}{2}}z\right)^{2k+1},}$$ where c_k is defined as above.

A useful asymptotic expansion of the complementary error function (and therefore also of the error function) for large real x is $${\displaystyle {\begin{aligned}\operatorname {erfc} x&={\frac {e^{-x^{2}}}{x{\sqrt {\pi }}}}\left(1+\sum _{n=1}^{\infty }(-1)^{n}{\frac {1\cdot 3\cdot 5\cdots (2n-1)}{\left(2x^{2}\right)^{n}}}\right)\\[6pt]&={\frac {e^{-x^{2}}}{x{\sqrt {\pi }}}}\sum _{n=0}^{\infty }(-1)^{n}{\frac {(2n-1)!!}{\left(2x^{2}\right)^{n}}},\end{aligned}}}$$ where (2n − 1)!! is the double factorial of (2n − 1), which is the product of all odd numbers up to (2n − 1). This series diverges for every finite x, and its meaning as asymptotic expansion is that for any integer N ≥ 1 one has $${\displaystyle \operatorname {erfc} x={\frac {e^{-x^{2}}}{x{\sqrt {\pi }}}}\sum _{n=0}^{N-1}(-1)^{n}{\frac {(2n-1)!!}{\left(2x^{2}\right)^{n}}}+R_{N}(x)}$$ where the remainder is $${\displaystyle R_{N}(x):={\frac {(-1)^{N}}{\sqrt {\pi }}}2^{1-2N}{\frac {(2N)!}{N!}}\int _{x}^{\infty }t^{-2N}e^{-t^{2}}\,\mathrm {d} t,}$$ which follows easily by induction, writing $${\displaystyle e^{-t^{2}}=-(2t)^{-1}\left(e^{-t^{2}}\right)'}$$ and integrating by parts.

The asymptotic behavior of the remainder term, in Landau notation, is $${\displaystyle R_{N}(x)=O\left(x^{-(1+2N)}e^{-x^{2}}\right)}$$ as x → ∞. This can be found by $${\displaystyle R_{N}(x)\propto \int _{x}^{\infty }t^{-2N}e^{-t^{2}}\,\mathrm {d} t=e^{-x^{2}}\int _{0}^{\infty }(t+x)^{-2N}e^{-t^{2}-2tx}\,\mathrm {d} t\leq e^{-x^{2}}\int _{0}^{\infty }x^{-2N}e^{-2tx}\,\mathrm {d} t\propto x^{-(1+2N)}e^{-x^{2}}.}$$ For large enough values of x, only the first few terms of this asymptotic expansion are needed to obtain a good approximation of erfc x (while for not too large values of x, the above Taylor expansion at 0 provides a very fast convergence).

A continued fraction expansion of the complementary error function was found by Laplace:^[10][11] $${\displaystyle \operatorname {erfc} z={\frac {z}{\sqrt {\pi }}}e^{-z^{2}}{\cfrac {1}{z^{2}+{\cfrac {a_{1}}{1+{\cfrac {a_{2}}{z^{2}+{\cfrac {a_{3}}{1+\dotsb }}}}}}}},\qquad a_{m}={\frac {m}{2}}.}$$

The inverse factorial series: $${\displaystyle {\begin{aligned}\operatorname {erfc} z&={\frac {e^{-z^{2}}}{{\sqrt {\pi }}\,z}}\sum _{n=0}^{\infty }{\frac {\left(-1\right)^{n}Q_{n}}{{\left(z^{2}+1\right)}^{\bar {n}}}}\\[1ex]&={\frac {e^{-z^{2}}}{{\sqrt {\pi }}\,z}}\left[1-{\frac {1}{2}}{\frac {1}{(z^{2}+1)}}+{\frac {1}{4}}{\frac {1}{\left(z^{2}+1\right)\left(z^{2}+2\right)}}-\cdots \right]\end{aligned}}}$$ converges for Re(z²) > 0. Here $${\displaystyle {\begin{aligned}Q_{n}&{\overset {\text{def}}{{}={}}}{\frac {1}{\Gamma {\left({\frac {1}{2}}\right)}}}\int _{0}^{\infty }\tau (\tau -1)\cdots (\tau -n+1)\tau ^{-{\frac {1}{2}}}e^{-\tau }\,d\tau \\[1ex]&=\sum _{k=0}^{n}\left({\frac {1}{2}}\right)^{\bar {k}}s(n,k),\end{aligned}}}$$ zⁿ denotes the rising factorial, and s(n,k) denotes a signed Stirling number of the first kind.^[12][13] There also exists a representation by an infinite sum containing the double factorial: $${\displaystyle \operatorname {erf} z={\frac {2}{\sqrt {\pi }}}\sum _{n=0}^{\infty }{\frac {(-2)^{n}(2n-1)!!}{(2n+1)!}}z^{2n+1}}$$

• Abramowitz and Stegun give several approximations of varying accuracy (equations 7.1.25–28). This allows one to choose the fastest approximation suitable for a given application. In order of increasing accuracy, they are: $${\displaystyle \operatorname {erf} x\approx 1-{\frac {1}{\left(1+a_{1}x+a_{2}x^{2}+a_{3}x^{3}+a_{4}x^{4}\right)^{4}}},\qquad x\geq 0}$$ (maximum error: 5×10⁻⁴)

  where a₁ = 0.278393, a₂ = 0.230389, a₃ = 0.000972, a₄ = 0.078108

  $${\displaystyle \operatorname {erf} x\approx 1-\left(a_{1}t+a_{2}t^{2}+a_{3}t^{3}\right)e^{-x^{2}},\quad t={\frac {1}{1+px}},\qquad x\geq 0}$$ (maximum error: 2.5×10⁻⁵)

  where p = 0.47047, a₁ = 0.3480242, a₂ = −0.0958798, a₃ = 0.7478556

  $${\displaystyle \operatorname {erf} x\approx 1-{\frac {1}{\left(1+a_{1}x+a_{2}x^{2}+\cdots +a_{6}x^{6}\right)^{16}}},\qquad x\geq 0}$$ (maximum error: 3×10⁻⁷)

  where a₁ = 0.0705230784, a₂ = 0.0422820123, a₃ = 0.0092705272, a₄ = 0.0001520143, a₅ = 0.0002765672, a₆ = 0.0000430638

  $${\displaystyle \operatorname {erf} x\approx 1-\left(a_{1}t+a_{2}t^{2}+\cdots +a_{5}t^{5}\right)e^{-x^{2}},\quad t={\frac {1}{1+px}}}$$ (maximum error: 1.5×10⁻⁷)

  where p = 0.3275911, a₁ = 0.254829592, a₂ = −0.284496736, a₃ = 1.421413741, a₄ = −1.453152027, a₅ = 1.061405429

  All of these approximations are valid for x ≥ 0. To use these approximations for negative x, use the fact that erf x is an odd function, so erf x = −erf(−x).

• Exponential bounds and a pure exponential approximation for the complementary error function are given by^[14] $${\displaystyle {\begin{aligned}\operatorname {erfc} x&\leq {\frac {1}{2}}e^{-2x^{2}}+{\frac {1}{2}}e^{-x^{2}}\leq e^{-x^{2}},&\quad x&>0\\[1.5ex]\operatorname {erfc} x&\approx {\frac {1}{6}}e^{-x^{2}}+{\frac {1}{2}}e^{-{\frac {4}{3}}x^{2}},&\quad x&>0.\end{aligned}}}$$
• The above have been generalized to sums of N exponentials^[15] with increasing accuracy in terms of N so that erfc x can be accurately approximated or bounded by 2Q̃(√2x), where $${\displaystyle {\tilde {Q}}(x)=\sum _{n=1}^{N}a_{n}e^{-b_{n}x^{2}}.}$$ In particular, there is a systematic methodology to solve the numerical coefficients {(a_n,b_n)}^N
  _{n = 1} that yield a minimax approximation or bound for the closely related Q-function: Q(x) ≈ Q̃(x), Q(x) ≤ Q̃(x), or Q(x) ≥ Q̃(x) for x ≥ 0. The coefficients {(a_n,b_n)}^N
  _{n = 1} for many variations of the exponential approximations and bounds up to N = 25 have been released to open access as a comprehensive dataset.^[16]
• A tight approximation of the complementary error function for x ∈ [0,∞) is given by Karagiannidis & Lioumpas (2007)^[17] who showed for the appropriate choice of parameters {A,B} that $${\displaystyle \operatorname {erfc} x\approx {\frac {\left(1-e^{-Ax}\right)e^{-x^{2}}}{B{\sqrt {\pi }}x}}.}$$ They determined {A,B} = {1.98,1.135}, which gave a good approximation for all x ≥ 0. Alternative coefficients are also available for tailoring accuracy for a specific application or transforming the expression into a tight bound.^[18]
• A single-term lower bound is^[19] $${\displaystyle \operatorname {erfc} x\geq {\sqrt {\frac {2e}{\pi }}}{\frac {\sqrt {\beta -1}}{\beta }}e^{-\beta x^{2}},\qquad x\geq 0,\quad \beta >1,}$$ where the parameter β can be picked to minimize error on the desired interval of approximation.
• Another approximation is given by Sergei Winitzki using his "global Padé approximations":^{[20][21]: 2–3} $${\displaystyle \operatorname {erf} x\approx \operatorname {sgn} x\cdot {\sqrt {1-\exp \left(-x^{2}{\frac {{\frac {4}{\pi }}+ax^{2}}{1+ax^{2}}}\right)}}}$$ where $${\displaystyle a={\frac {8(\pi -3)}{3\pi (4-\pi )}}\approx 0.140012.}$$ This is designed to be very accurate in a neighborhood of 0 and a neighborhood of infinity, and the relative error is less than 0.00035 for all real x. Using the alternate value a ≈ 0.147 reduces the maximum relative error to about 0.00013.^[22]

  This approximation can be inverted to obtain an approximation for the inverse error function: $${\displaystyle \operatorname {erf} ^{-1}x\approx \operatorname {sgn} x\cdot {\sqrt {{\sqrt {\left({\frac {2}{\pi a}}+{\frac {\ln \left(1-x^{2}\right)}{2}}\right)^{2}-{\frac {\ln \left(1-x^{2}\right)}{a}}}}-\left({\frac {2}{\pi a}}+{\frac {\ln \left(1-x^{2}\right)}{2}}\right)}}.}$$

• An approximation with a maximal error of 1.2×10⁻⁷ for any real argument is:^[23] $${\displaystyle \operatorname {erf} x={\begin{cases}1-\tau &x\geq 0\\\tau -1&x<0\end{cases}}}$$ with $${\displaystyle {\begin{aligned}\tau &=t\cdot \exp \left(-x^{2}-1.26551223+1.00002368t+0.37409196t^{2}+0.09678418t^{3}-0.18628806t^{4}\right.\\&\left.\qquad \qquad \qquad +0.27886807t^{5}-1.13520398t^{6}+1.48851587t^{7}-0.82215223t^{8}+0.17087277t^{9}\right)\end{aligned}}}$$ and $${\displaystyle t={\frac {1}{1+{\frac {1}{2}}|x|}}.}$$
• An approximation of ${\displaystyle \operatorname {erfc} }$ with a maximum relative error less than ${\displaystyle 2^{-53}}$ ${\displaystyle \left(\approx 1.1\times 10^{-16}\right)}$ in absolute value is:^[24] for ${\displaystyle x\geq 0}$, $${\displaystyle {\begin{aligned}\operatorname {erfc} \left(x\right)&=\left({\frac {0.56418958354775629}{x+2.06955023132914151}}\right)\left({\frac {x^{2}+2.71078540045147805x+5.80755613130301624}{x^{2}+3.47954057099518960x+12.06166887286239555}}\right)\\&\left({\frac {x^{2}+3.47469513777439592x+12.07402036406381411}{x^{2}+3.72068443960225092x+8.44319781003968454}}\right)\left({\frac {x^{2}+4.00561509202259545x+9.30596659485887898}{x^{2}+3.90225704029924078x+6.36161630953880464}}\right)\\&\left({\frac {x^{2}+5.16722705817812584x+9.12661617673673262}{x^{2}+4.03296893109262491x+5.13578530585681539}}\right)\left({\frac {x^{2}+5.95908795446633271x+9.19435612886969243}{x^{2}+4.11240942957450885x+4.48640329523408675}}\right)e^{-x^{2}}\\\end{aligned}}}$$ and for ${\displaystyle x<0}$ $${\displaystyle \operatorname {erfc} \left(x\right)=2-\operatorname {erfc} \left(-x\right)}$$
• A simple approximation for real-valued arguments could be done through Hyperbolic functions: $${\displaystyle \operatorname {erf} \left(x\right)\approx z(x)=\tanh \left({\frac {2}{\sqrt {\pi }}}\left(x+{\frac {11}{123}}x^{3}\right)\right)}$$ which keeps the absolute difference ${\displaystyle \left|\operatorname {erf} \left(x\right)-z(x)\right|<0.000358,\,\forall x}$.

The complementary error function, denoted erfc, is defined as

$${\displaystyle {\begin{aligned}\operatorname {erfc} x&=1-\operatorname {erf} x\\[5pt]&={\frac {2}{\sqrt {\pi }}}\int _{x}^{\infty }e^{-t^{2}}\,\mathrm {d} t\\[5pt]&=e^{-x^{2}}\operatorname {erfcx} x,\end{aligned}}}$$ which also defines erfcx, the scaled complementary error function^[25] (which can be used instead of erfc to avoid arithmetic underflow^[25][26]). Another form of erfc x for x ≥ 0 is known as Craig's formula, after its discoverer:^[27] $${\displaystyle \operatorname {erfc} (x\mid x\geq 0)={\frac {2}{\pi }}\int _{0}^{\frac {\pi }{2}}\exp \left(-{\frac {x^{2}}{\sin ^{2}\theta }}\right)\,\mathrm {d} \theta .}$$ This expression is valid only for positive values of x, but it can be used in conjunction with erfc x = 2 − erfc(−x) to obtain erfc(x) for negative values. This form is advantageous in that the range of integration is fixed and finite. An extension of this expression for the erfc of the sum of two non-negative variables is as follows:^[28] $${\displaystyle \operatorname {erfc} (x+y\mid x,y\geq 0)={\frac {2}{\pi }}\int _{0}^{\frac {\pi }{2}}\exp \left(-{\frac {x^{2}}{\sin ^{2}\theta }}-{\frac {y^{2}}{\cos ^{2}\theta }}\right)\,\mathrm {d} \theta .}$$