The Gamma function, Γ \Gamma Γ , is at the heart of important results in mathematics
including the Riemann hypothesis .
It is defined as follows:
Γ : C → C s ↦ ∫ 0 ∞ t s − 1 e − t d t \begin{align}
\Gamma \;\colon \C &\to \C~\nonumber \\
s &\mapsto \int\limits_0^\infty t^{s-1} e^{-t} \, \d t~\label{1}
\end{align} Γ : C s → C ↦ 0 ∫ ∞ t s − 1 e − t d t What makes ( 1 ) \eqref{1} ( 1 ) so interesting?
Basic Properties These are:
Over the positive integers, it simplifies to the factorial function,
shifted by 1 1 1 . Over the negative integers, it diverges. At 0 0 0 , it diverges. It has even more interesting behavior over non-integer
fractions and complex numbers. It converges for all complex numbers s s s with positive real part
(i.e. Re ( s ) > 0 \Re(s) > 0 Re ( s ) > 0 ). It also converges for complex numbers with
negative real part (i.e. Re ( s ) < 0 \Re(s) < 0 Re ( s ) < 0 ) except where
Re ( s ) \Re(s) Re ( s ) is a negative integer or 0 0 0 .
When Re ( s ) \Re(s) Re ( s ) is zero or a negative integer and the imaginary part
of s s s is 0 0 0 , then Γ ( s ) \Gamma(s) Γ ( s ) diverges and is undefined.
Over the Positive Integers Note that the integers are embedded in the complex numbers
as the subset obtained by setting the imaginary part to 0 0 0
and restricting the real part accordingly.
Over the positive integers, Γ \Gamma Γ has two general properties,
outlined below.
Special Case Consider Γ ( n ) \Gamma(n) Γ ( n ) for n = 1 n = 1 n = 1 .
The integral has a surprisingly simple simplification:
Γ ( 1 ) = ∫ 0 ∞ t 1 − 1 e − t d t = ∫ 0 ∞ e − t d t (since t 0 = 1 ) = [ − e − t ] 0 ∞ = 0 − ( − 1 ) = 1 \begin{align}
\Gamma(1) &= \int\limits_0^\infty t^{1-1} e^{-t} \, \d t \\
&= \int\limits_0^\infty e^{-t} \, \d t \;\; \text{(since $t^0 = 1$)} \\
&= \biggl [ -e^{-t} \biggr ]_0^\infty \\
&= 0 - (-1) \\
&= 1
\end{align} Γ ( 1 ) = 0 ∫ ∞ t 1 − 1 e − t d t = 0 ∫ ∞ e − t d t (since t 0 = 1) = [ − e − t ] 0 ∞ = 0 − ( − 1 ) = 1
General Case: Positive Integers Take n n n to be an arbitrary positive integer, i.e. n ∈ N n \in \N n ∈ N and n > 1 n > 1 n > 1 .
To prove that Γ \Gamma Γ is indeed equivalent to the factorial function
(albeit shifted by 1 1 1 ), we need to show that Γ ( n + 1 ) = n Γ ( n ) \Gamma(n+1) = n \Gamma(n) Γ ( n + 1 ) = n Γ ( n ) .
Revisit the definition of Γ \Gamma Γ , applied to n + 1 n+1 n + 1 :
Γ ( n + 1 ) = ∫ 0 ∞ t n e − t d t \begin{align*}
\Gamma(n+1) &= \int\limits_0^\infty t^{n} e^{-t} \, \d t \\
\end{align*} Γ ( n + 1 ) = 0 ∫ ∞ t n e − t d t This integral can be simplified using the rule for integration by parts:
∫ u d v = u v − ∫ v d u \begin{align*}
\int u \, \d v = uv - \int v \, \d u
\end{align*} ∫ u d v = uv − ∫ v d u Take u = t n u = t^n u = t n and d v = e − t d t \d v = e^{-t} \, \d t d v = e − t d t ; then:
d u = d d t t n = n t n − 1 v = ∫ e − t d t = − e − t \begin{align*}
\d u &= \frac{\d}{\d t} t^n = n t^{n-1} \\
v &= \int e^{-t} \, \d t = -e^{-t} \\
\end{align*} d u v = d t d t n = n t n − 1 = ∫ e − t d t = − e − t Thus,
Γ ( n + 1 ) = ∫ 0 ∞ t n e − t d t = ∫ 0 ∞ t n ⏟ u ⋅ e − t ⏟ d v d t = [ − t n e − t ] 0 ∞ ⏟ u v − ∫ 0 ∞ n t n − 1 ⏟ v ⋅ ( − e − t ) ⏟ d u d t = ( 0 − 0 ) − ∫ 0 ∞ − n t n − 1 e − t d t = n ∫ 0 ∞ t n − 1 e − t d t = n ⋅ Γ ( n ) \begin{align*}
\Gamma(n+1) &= \int\limits_0^\infty t^{n} e^{-t} \, \d t \\
&= \int\limits_0^\infty \underbrace{t^n}_{u} \cdot \underbrace{e^{-t}}_{\d v} \, \d t \\
&= \underbrace{\biggl [ -t^n e^{-t} \biggr ]_0^\infty}_{uv}
- \int\limits_0^\infty \underbrace{nt^{n-1}}_{v} \cdot \underbrace{\left(- e^{-t}\right)}_{\d u} \, \d t\\ \\
&= (0 - 0) - \int\limits_0^\infty -nt^{n-1} e^{-t} \, \d t \\
&= n \int\limits_0^\infty t^{n-1} e^{-t} \, \d t \\ \\
&= n \cdot \Gamma(n) \\
\end{align*} Γ ( n + 1 ) = 0 ∫ ∞ t n e − t d t = 0 ∫ ∞ u t n ⋅ d v e − t d t = uv [ − t n e − t ] 0 ∞ − 0 ∫ ∞ v n t n − 1 ⋅ d u ( − e − t ) d t = ( 0 − 0 ) − 0 ∫ ∞ − n t n − 1 e − t d t = n 0 ∫ ∞ t n − 1 e − t d t = n ⋅ Γ ( n ) This is an important identity, usually expressed in any
of the following two forms:
Γ ( n + 1 ) = n Γ ( n ) Γ ( n ) = 1 n Γ ( n + 1 ) \begin{align*}
\Gamma(n+1) &= n \Gamma(n) \\
\Gamma(n) &= \frac{1}{n} \Gamma(n+1)
\end{align*} Γ ( n + 1 ) Γ ( n ) = n Γ ( n ) = n 1 Γ ( n + 1 )
Proof by Induction So far, we have seen the following results:
Γ ( 1 ) = 1 ≡ 0 ! Γ ( n + 1 ) = n Γ ( n ) for n ∈ N > 1 \begin{align*}
\Gamma(1) &= 1 \equiv 0! \\
\Gamma(n+1) &= n \Gamma(n) \; \; \text{for $n \in \N_{>1}$}
\end{align*} Γ ( 1 ) Γ ( n + 1 ) = 1 ≡ 0 ! = n Γ ( n ) for n ∈ N > 1 By induction on n n n ,
suppose we know that Γ ( n ) = ( n − 1 ) ! \Gamma(n) = (n-1)! Γ ( n ) = ( n − 1 )!
(with the base-case being Γ ( 1 ) = 0 ! \Gamma(1) = 0! Γ ( 1 ) = 0 ! ).
We can compute Γ ( n + 1 ) \Gamma(n+1) Γ ( n + 1 ) as follows:
Γ ( n + 1 ) = n ⋅ Γ ( n ) = n ⋅ ( n − 1 ) ! = n ! \begin{align*}
\Gamma(n+1) &= n \cdot \Gamma(n) \\
&= n \cdot (n-1) ! \\
&= n!
\end{align*} Γ ( n + 1 ) = n ⋅ Γ ( n ) = n ⋅ ( n − 1 )! = n ! info
Γ \Gamma Γ was not intended to be a generalization of the factorial function.
The result was a somewhat accidental one, albeit useful.
Over the Reals By restricting Γ \Gamma Γ to the positive integers, we discovered that:
Γ ( n ) = ( n − 1 ) ! for n ∈ N \begin{align*}
\Gamma(n) &= (n-1)! \; \; \text{for $n \in \N$}
\end{align*} Γ ( n ) = ( n − 1 )! for n ∈ N But what happens when we plug in a fraction, say 3 2 \displaystyle \frac{3}{2} 2 3 ?
Γ ( 3 2 ) = Γ ( 1 2 + 1 ) = 1 2 ⋅ Γ ( 1 2 ) = 1 2 ∫ 0 ∞ t − 1 2 e − t d t \begin{align*}
\Gamma \left( \frac{3}{2} \right) &= \Gamma(\frac{1}{2} + 1) \\
&= \frac{1}{2} \cdot \Gamma(\frac{1}{2}) \\
&= \frac{1}{2} \int\limits_0^\infty t^{-\frac{1}{2}} e^{-t} \, \d t \\
\end{align*} Γ ( 2 3 ) = Γ ( 2 1 + 1 ) = 2 1 ⋅ Γ ( 2 1 ) = 2 1 0 ∫ ∞ t − 2 1 e − t d t To simplify the integral, let's try to get rid of the t − 1 2 \displaystyle t^{-\frac{1}{2}} t − 2 1 term
by substituting t = x 2 t = x^2 t = x 2 :
Γ ( 3 2 ) = 1 2 ∫ 0 ∞ t − 1 2 e − x 2 ⋅ 2 t 1 2 d x = ∫ 0 ∞ e − x 2 d x \begin{align*}
\Gamma\left(\frac{3}{2}\right) &= \frac{1}{2} \int\limits_0^\infty t^{-\frac{1}{2}} e^{-x^2} \cdot 2t^\frac{1}{2} \, \d x \\
&= \int\limits_0^\infty e^{-x^2} \, \d x \\
\end{align*} Γ ( 2 3 ) = 2 1 0 ∫ ∞ t − 2 1 e − x 2 ⋅ 2 t 2 1 d x = 0 ∫ ∞ e − x 2 d x This is a familiar integral, known as the Gaussian integral :
I ( a ) = ∫ a a e − x 2 d x I ( ∞ ) = ∫ ∞ ∞ e − x 2 d x I 2 ( ∞ ) = ( ∫ − ∞ ∞ e − x 2 d x ) ⋅ ( ∫ − ∞ ∞ e − y 2 d y ) = ∫ − ∞ ∞ ∫ − ∞ ∞ e − ( x 2 + y 2 ) d x d y = ∫ − ∞ ∞ ∫ − ∞ ∞ e − r 2 r d r d θ = ∫ 0 2 π ∫ 0 ∞ e − r 2 r d r d θ = 2 π ∫ 0 ∞ e − r 2 r d r = 2 π ∫ − ∞ 0 1 2 e u d u (substituting u = − r 2 ) = π [ e u ] − ∞ 0 = π ( e 0 − e − ∞ ) = π ( 1 − 0 ) = π \begin{align*}
I(a) &= \int\limits_a^a e^{-x^2} \, \d x \\ \\
I(\infty) &= \int\limits_\infty^\infty e^{-x^2} \, \d x \\ \\
I^2(\infty) &= \left( \int\limits_{-\infty}^\infty e^{-x^2} \, \d x \right) \cdot \left( \int\limits_{-\infty}^\infty e^{-y^2} \, \d y \right) \\
&= \int\limits_{-\infty}^\infty \int\limits_{-\infty}^\infty e^{-(x^2 + y^2)} \, \d x \, \d y \\
&= \int\limits_{-\infty}^\infty \int\limits_{-\infty}^\infty e^{-r^2} \, r\, \d r \, \d \theta \\
&= \int\limits_0^{2\pi} \int\limits_0^\infty e^{-r^2} \, r\, \d r \, \d \theta \\
&= 2\pi \int\limits_0^\infty e^{-r^2} \, r\, \d r \\
&= 2\pi \int\limits_{-\infty}^0 \frac{1}{2} e^{u} \, \d u \;\; \text{(substituting $u = -r^2$)} \\
&= \pi \biggl [ e^u \biggr ]_{-\infty}^0 \\
&= \pi (e^0 - e^{-\infty}) \\
&= \pi (1 - 0) \\ &= \pi
\end{align*} I ( a ) I ( ∞ ) I 2 ( ∞ ) = a ∫ a e − x 2 d x = ∞ ∫ ∞ e − x 2 d x = − ∞ ∫ ∞ e − x 2 d x ⋅ − ∞ ∫ ∞ e − y 2 d y = − ∞ ∫ ∞ − ∞ ∫ ∞ e − ( x 2 + y 2 ) d x d y = − ∞ ∫ ∞ − ∞ ∫ ∞ e − r 2 r d r d θ = 0 ∫ 2 π 0 ∫ ∞ e − r 2 r d r d θ = 2 π 0 ∫ ∞ e − r 2 r d r = 2 π − ∞ ∫ 0 2 1 e u d u (substituting u = − r 2 ) = π [ e u ] − ∞ 0 = π ( e 0 − e − ∞ ) = π ( 1 − 0 ) = π Since Γ ( 3 2 ) \Gamma(\frac{3}{2}) Γ ( 2 3 ) restricts the integration to [ 0 , ∞ ) [0, \infty) [ 0 , ∞ )
and the function is even :
Γ ( 3 2 ) = 1 2 ∫ − ∞ ∞ e − x 2 d x = 1 2 ⋅ I 2 ( ∞ ) = π 2 \begin{align*}
\Gamma\left(\frac{3}{2}\right) &= \frac{1}{2} \int\limits_{-\infty}^\infty e^{-x^2} \, \d x \\
&= \frac{1}{2} \cdot \sqrt{I^2(\infty)} \\
&= \frac{\sqrt{\pi}}{2} \\
\end{align*} Γ ( 2 3 ) = 2 1 − ∞ ∫ ∞ e − x 2 d x = 2 1 ⋅ I 2 ( ∞ ) = 2 π Other fractions of the form ( n + 1 2 ) , n ∈ N \displaystyle \left(n + \frac{1}{2} \right),\, n \in \N ( n + 2 1 ) , n ∈ N have similar results simplifications:
Γ ( 1 2 ) = π Γ ( 3 2 ) = 1 2 π Γ ( 5 2 ) = 3 4 π Γ ( 7 2 ) = 15 8 π Γ ( 9 2 ) = 105 16 π ⋮ \begin{align*}
\Gamma\left(\frac{1}{2}\right) &= \sqrt{\pi} \\
\Gamma\left(\frac{3}{2}\right) &= \frac{1}{2} \sqrt{\pi} \\
\Gamma\left(\frac{5}{2}\right) &= \frac{3}{4} \sqrt{\pi} \\
\Gamma\left(\frac{7}{2}\right) &= \frac{15}{8} \sqrt{\pi} \\
\Gamma\left(\frac{9}{2}\right) &= \frac{105}{16} \sqrt{\pi} \\
\vdots
\end{align*} Γ ( 2 1 ) Γ ( 2 3 ) Γ ( 2 5 ) Γ ( 2 7 ) Γ ( 2 9 ) ⋮ = π = 2 1 π = 4 3 π = 8 15 π = 16 105 π In general,
Γ ( 1 n ) ∼ n − γ \begin{align*}
\Gamma\parens{\frac{1}{n}} \sim n - \gamma
\end{align*} Γ ( n 1 ) ∼ n − γ where γ \gamma γ is the Euler-Mascheroni constant and ∼ \sim ∼ denotes
asymptotic equivalence .
but unfortunately
the integral has to be computed or simplified directly for each case.
Over the Complexes Γ \Gamma Γ has a meromorphic
extension to the complex numbers, with simple poles at the non-positive integers
and 0 0 0 . It is defined with the same rules and the relation
Γ ( s + 1 ) = s Γ ( s ) \displaystyle \Gamma(s+1) = s \Gamma(s) Γ ( s + 1 ) = s Γ ( s ) holds for all complex numbers s s s .
For example;
Γ ( i ) = ( − 1 + i ) ! ≈ − 0.1549 − 0.4980 i \begin{align*}
\Gamma(i) &= \parens{-1 + i}! \approx -0.1549 - 0.4980i
\end{align*} Γ ( i ) = ( − 1 + i ) ! ≈ − 0.1549 − 0.4980 i Various values of Γ \Gamma Γ are tabulated here .
For some useful applications of Γ \Gamma Γ in the Riemann zeta function,
see this post .