The following is a list of significant formulae involving the mathematical constant π . Many of these formulae can be found in the article Pi , or the article Approximations of π .
Euclidean geometry [ edit ]
π
=
C
d
=
C
2
r
{\displaystyle \pi ={\frac {C}{d}}={\frac {C}{2r}}}
where C is the circumference of a circle , d is the diameter , and r is the radius . More generally,
π
=
L
w
{\displaystyle \pi ={\frac {L}{w}}}
where L and w are, respectively, the perimeter and the width of any curve of constant width .
A
=
π
r
2
{\displaystyle A=\pi r^{2}}
where A is the area of a circle . More generally,
A
=
π
a
b
{\displaystyle A=\pi ab}
where A is the area enclosed by an ellipse with semi-major axis a and semi-minor axis b .
C
=
2
π
agm
(
a
,
b
)
(
a
1
2
−
∑
n
=
2
∞
2
n
−
1
(
a
n
2
−
b
n
2
)
)
{\displaystyle C={\frac {2\pi }{\operatorname {agm} (a,b)}}\left(a_{1}^{2}-\sum _{n=2}^{\infty }2^{n-1}(a_{n}^{2}-b_{n}^{2})\right)}
where C is the circumference of an ellipse with semi-major axis a and semi-minor axis b and
a
n
,
b
n
{\displaystyle a_{n},b_{n}}
are the arithmetic and geometric iterations of
agm
(
a
,
b
)
{\displaystyle \operatorname {agm} (a,b)}
, the arithmetic-geometric mean of a and b with the initial values
a
0
=
a
{\displaystyle a_{0}=a}
and
b
0
=
b
{\displaystyle b_{0}=b}
.
A
=
4
π
r
2
{\displaystyle A=4\pi r^{2}}
where A is the area between the witch of Agnesi and its asymptotic line; r is the radius of the defining circle.
A
=
Γ
(
1
/
4
)
2
2
π
r
2
=
π
r
2
agm
(
1
,
1
/
2
)
{\displaystyle A={\frac {\Gamma (1/4)^{2}}{2{\sqrt {\pi }}}}r^{2}={\frac {\pi r^{2}}{\operatorname {agm} (1,1/{\sqrt {2}})}}}
where A is the area of a squircle with minor radius r ,
Γ
{\displaystyle \Gamma }
is the gamma function .
A
=
(
k
+
1
)
(
k
+
2
)
π
r
2
{\displaystyle A=(k+1)(k+2)\pi r^{2}}
where A is the area of an epicycloid with the smaller circle of radius r and the larger circle of radius kr (
k
∈
N
{\displaystyle k\in \mathbb {N} }
), assuming the initial point lies on the larger circle.
A
=
(
−
1
)
k
+
3
8
π
a
2
{\displaystyle A={\frac {(-1)^{k}+3}{8}}\pi a^{2}}
where A is the area of a rose with angular frequency k (
k
∈
N
{\displaystyle k\in \mathbb {N} }
) and amplitude a .
L
=
Γ
(
1
/
4
)
2
π
c
=
2
π
c
agm
(
1
,
1
/
2
)
{\displaystyle L={\frac {\Gamma (1/4)^{2}}{\sqrt {\pi }}}c={\frac {2\pi c}{\operatorname {agm} (1,1/{\sqrt {2}})}}}
where L is the perimeter of the lemniscate of Bernoulli with focal distance c .
V
=
4
3
π
r
3
{\displaystyle V={4 \over 3}\pi r^{3}}
where V is the volume of a sphere and r is the radius.
S
A
=
4
π
r
2
{\displaystyle SA=4\pi r^{2}}
where SA is the surface area of a sphere and r is the radius.
H
=
1
2
π
2
r
4
{\displaystyle H={1 \over 2}\pi ^{2}r^{4}}
where H is the hypervolume of a 3-sphere and r is the radius.
S
V
=
2
π
2
r
3
{\displaystyle SV=2\pi ^{2}r^{3}}
where SV is the surface volume of a 3-sphere and r is the radius.
Regular convex polygons [ edit ]
Sum S of internal angles of a regular convex polygon with n sides:
S
=
(
n
−
2
)
π
{\displaystyle S=(n-2)\pi }
Area A of a regular convex polygon with n sides and side length s :
A
=
n
s
2
4
cot
π
n
{\displaystyle A={\frac {ns^{2}}{4}}\cot {\frac {\pi }{n}}}
Inradius r of a regular convex polygon with n sides and side length s :
r
=
s
2
cot
π
n
{\displaystyle r={\frac {s}{2}}\cot {\frac {\pi }{n}}}
Circumradius R of a regular convex polygon with n sides and side length s :
R
=
s
2
csc
π
n
{\displaystyle R={\frac {s}{2}}\csc {\frac {\pi }{n}}}
Physics [ edit ]
Λ
=
8
π
G
3
c
2
ρ
{\displaystyle \Lambda ={{8\pi G} \over {3c^{2}}}\rho }
Δ
x
Δ
p
≥
h
4
π
{\displaystyle \Delta x\,\Delta p\geq {\frac {h}{4\pi }}}
R
μ
ν
−
1
2
g
μ
ν
R
+
Λ
g
μ
ν
=
8
π
G
c
4
T
μ
ν
{\displaystyle R_{\mu \nu }-{\frac {1}{2}}g_{\mu \nu }R+\Lambda g_{\mu \nu }={8\pi G \over c^{4}}T_{\mu \nu }}
F
=
|
q
1
q
2
|
4
π
ε
0
r
2
{\displaystyle F={\frac {|q_{1}q_{2}|}{4\pi \varepsilon _{0}r^{2}}}}
μ
0
≈
4
π
⋅
10
−
7
N
/
A
2
{\displaystyle \mu _{0}\approx 4\pi \cdot 10^{-7}\,\mathrm {N} /\mathrm {A} ^{2}}
Approximate period of a simple pendulum with small amplitude:
T
≈
2
π
L
g
{\displaystyle T\approx 2\pi {\sqrt {\frac {L}{g}}}}
Exact period of a simple pendulum with amplitude
θ
0
{\displaystyle \theta _{0}}
(
agm
{\displaystyle \operatorname {agm} }
is the arithmetic–geometric mean ):
T
=
2
π
agm
(
1
,
cos
(
θ
0
/
2
)
)
L
g
{\displaystyle T={\frac {2\pi }{\operatorname {agm} (1,\cos(\theta _{0}/2))}}{\sqrt {\frac {L}{g}}}}
R
3
T
2
=
G
M
4
π
2
{\displaystyle {\frac {R^{3}}{T^{2}}}={\frac {GM}{4\pi ^{2}}}}
F
=
π
2
E
I
L
2
{\displaystyle F={\frac {\pi ^{2}EI}{L^{2}}}}
A puzzle involving "colliding billiard balls":
⌊
b
N
π
⌋
{\displaystyle \lfloor {b^{N}\pi }\rfloor }
is the number of collisions made (in ideal conditions, perfectly elastic with no friction) by an object of mass m initially at rest between a fixed wall and another object of mass b 2N m , when struck by the other object.[1] (This gives the digits of π in base b up to N digits past the radix point.)
Formulae yielding π [ edit ]
Integrals [ edit ]
2
∫
−
1
1
1
−
x
2
d
x
=
π
{\displaystyle 2\int _{-1}^{1}{\sqrt {1-x^{2}}}\,dx=\pi }
(integrating two halves
y
(
x
)
=
1
−
x
2
{\displaystyle y(x)={\sqrt {1-x^{2}}}}
to obtain the area of the unit circle)
∫
−
∞
∞
sech
x
d
x
=
π
{\displaystyle \int _{-\infty }^{\infty }\operatorname {sech} x\,dx=\pi }
∫
−
∞
∞
∫
t
∞
e
−
1
/
2
t
2
−
x
2
+
x
t
d
x
d
t
=
∫
−
∞
∞
∫
t
∞
e
−
t
2
−
1
/
2
x
2
+
x
t
d
x
d
t
=
π
{\displaystyle \int _{-\infty }^{\infty }\int _{t}^{\infty }e^{-1/2t^{2}-x^{2}+xt}\,dx\,dt=\int _{-\infty }^{\infty }\int _{t}^{\infty }e^{-t^{2}-1/2x^{2}+xt}\,dx\,dt=\pi }
∫
−
1
1
d
x
1
−
x
2
=
π
{\displaystyle \int _{-1}^{1}{\frac {dx}{\sqrt {1-x^{2}}}}=\pi }
∫
−
∞
∞
d
x
1
+
x
2
=
π
{\displaystyle \int _{-\infty }^{\infty }{\frac {dx}{1+x^{2}}}=\pi }
[2] [note 2] (see also Cauchy distribution )
∫
−
∞
∞
sin
x
x
d
x
=
π
{\displaystyle \int _{-\infty }^{\infty }{\frac {\sin x}{x}}\,dx=\pi }
(see Dirichlet integral )
∫
−
∞
∞
e
−
x
2
d
x
=
π
{\displaystyle \int _{-\infty }^{\infty }e^{-x^{2}}\,dx={\sqrt {\pi }}}
(see Gaussian integral ).
∮
d
z
z
=
2
π
i
{\displaystyle \oint {\frac {dz}{z}}=2\pi i}
(when the path of integration winds once counterclockwise around 0. See also Cauchy's integral formula ).
∫
0
∞
ln
(
1
+
1
x
2
)
d
x
=
π
{\displaystyle \int _{0}^{\infty }\ln \left(1+{\frac {1}{x^{2}}}\right)\,dx=\pi }
[3]
∫
−
∞
∞
sin
x
x
d
x
=
π
{\displaystyle \int _{-\infty }^{\infty }{\frac {\sin x}{x}}\,dx=\pi }
∫
0
1
x
4
(
1
−
x
)
4
1
+
x
2
d
x
=
22
7
−
π
{\displaystyle \int _{0}^{1}{x^{4}(1-x)^{4} \over 1+x^{2}}\,dx={22 \over 7}-\pi }
(see also Proof that 22/7 exceeds π ).
∫
0
∞
x
α
−
1
x
+
1
d
x
=
π
sin
π
α
,
0
<
α
<
1
{\displaystyle \int _{0}^{\infty }{\frac {x^{\alpha -1}}{x+1}}\,dx={\frac {\pi }{\sin \pi \alpha }},\quad 0<\alpha <1}
∫
0
∞
d
x
x
(
x
+
a
)
(
x
+
b
)
=
π
agm
(
a
,
b
)
{\displaystyle \int _{0}^{\infty }{\frac {dx}{\sqrt {x(x+a)(x+b)}}}={\frac {\pi }{\operatorname {agm} ({\sqrt {a}},{\sqrt {b}})}}}
(where
agm
{\displaystyle \operatorname {agm} }
is the arithmetic–geometric mean ;[4] see also elliptic integral )
Note that with symmetric integrands
f
(
−
x
)
=
f
(
x
)
{\displaystyle f(-x)=f(x)}
, formulas of the form
∫
−
a
a
f
(
x
)
d
x
{\textstyle \int _{-a}^{a}f(x)\,dx}
can also be translated to formulas
2
∫
0
a
f
(
x
)
d
x
{\textstyle 2\int _{0}^{a}f(x)\,dx}
.
Efficient infinite series [ edit ]
∑
k
=
0
∞
k
!
(
2
k
+
1
)
!
!
=
∑
k
=
0
∞
2
k
k
!
2
(
2
k
+
1
)
!
=
π
2
{\displaystyle \sum _{k=0}^{\infty }{\frac {k!}{(2k+1)!!}}=\sum _{k=0}^{\infty }{\frac {2^{k}k!^{2}}{(2k+1)!}}={\frac {\pi }{2}}}
(see also Double factorial )
∑
k
=
0
∞
k
!
(
2
k
)
!
(
25
k
−
3
)
(
3
k
)
!
2
k
=
π
2
{\displaystyle \sum _{k=0}^{\infty }{\frac {k!\,(2k)!\,(25k-3)}{(3k)!\,2^{k}}}={\frac {\pi }{2}}}
∑
k
=
0
∞
(
−
1
)
k
(
6
k
)
!
(
13591409
+
545140134
k
)
(
3
k
)
!
(
k
!
)
3
640320
3
k
=
4270934400
10005
π
{\displaystyle \sum _{k=0}^{\infty }{\frac {(-1)^{k}(6k)!(13591409+545140134k)}{(3k)!(k!)^{3}640320^{3k}}}={\frac {4270934400}{{\sqrt {10005}}\pi }}}
(see Chudnovsky algorithm )
∑
k
=
0
∞
(
4
k
)
!
(
1103
+
26390
k
)
(
k
!
)
4
396
4
k
=
9801
2
2
π
{\displaystyle \sum _{k=0}^{\infty }{\frac {(4k)!(1103+26390k)}{(k!)^{4}396^{4k}}}={\frac {9801}{2{\sqrt {2}}\pi }}}
(see Srinivasa Ramanujan , Ramanujan–Sato series )
The following are efficient for calculating arbitrary binary digits of π :
∑
k
=
0
∞
(
−
1
)
k
4
k
(
2
4
k
+
1
+
2
4
k
+
2
+
1
4
k
+
3
)
=
π
{\displaystyle \sum _{k=0}^{\infty }{\frac {(-1)^{k}}{4^{k}}}\left({\frac {2}{4k+1}}+{\frac {2}{4k+2}}+{\frac {1}{4k+3}}\right)=\pi }
[5]
∑
k
=
0
∞
1
16
k
(
4
8
k
+
1
−
2
8
k
+
4
−
1
8
k
+
5
−
1
8
k
+
6
)
=
π
{\displaystyle \sum _{k=0}^{\infty }{\frac {1}{16^{k}}}\left({\frac {4}{8k+1}}-{\frac {2}{8k+4}}-{\frac {1}{8k+5}}-{\frac {1}{8k+6}}\right)=\pi }
(see Bailey–Borwein–Plouffe formula )
∑
k
=
0
∞
1
16
k
(
8
8
k
+
2
+
4
8
k
+
3
+
4
8
k
+
4
−
1
8
k
+
7
)
=
2
π
{\displaystyle \sum _{k=0}^{\infty }{\frac {1}{16^{k}}}\left({\frac {8}{8k+2}}+{\frac {4}{8k+3}}+{\frac {4}{8k+4}}-{\frac {1}{8k+7}}\right)=2\pi }
∑
k
=
0
∞
(
−
1
)
k
2
10
k
(
−
2
5
4
k
+
1
−
1
4
k
+
3
+
2
8
10
k
+
1
−
2
6
10
k
+
3
−
2
2
10
k
+
5
−
2
2
10
k
+
7
+
1
10
k
+
9
)
=
2
6
π
{\displaystyle \sum _{k=0}^{\infty }{\frac {{(-1)}^{k}}{2^{10k}}}\left(-{\frac {2^{5}}{4k+1}}-{\frac {1}{4k+3}}+{\frac {2^{8}}{10k+1}}-{\frac {2^{6}}{10k+3}}-{\frac {2^{2}}{10k+5}}-{\frac {2^{2}}{10k+7}}+{\frac {1}{10k+9}}\right)=2^{6}\pi }
Plouffe's series for calculating arbitrary decimal digits of π :[6]
∑
k
=
1
∞
k
2
k
k
!
2
(
2
k
)
!
=
π
+
3
{\displaystyle \sum _{k=1}^{\infty }k{\frac {2^{k}k!^{2}}{(2k)!}}=\pi +3}
Other infinite series [ edit ]
ζ
(
2
)
=
1
1
2
+
1
2
2
+
1
3
2
+
1
4
2
+
⋯
=
π
2
6
{\displaystyle \zeta (2)={\frac {1}{1^{2}}}+{\frac {1}{2^{2}}}+{\frac {1}{3^{2}}}+{\frac {1}{4^{2}}}+\cdots ={\frac {\pi ^{2}}{6}}}
(see also Basel problem and Riemann zeta function )
ζ
(
4
)
=
1
1
4
+
1
2
4
+
1
3
4
+
1
4
4
+
⋯
=
π
4
90
{\displaystyle \zeta (4)={\frac {1}{1^{4}}}+{\frac {1}{2^{4}}}+{\frac {1}{3^{4}}}+{\frac {1}{4^{4}}}+\cdots ={\frac {\pi ^{4}}{90}}}
ζ
(
2
n
)
=
∑
k
=
1
∞
1
k
2
n
=
1
1
2
n
+
1
2
2
n
+
1
3
2
n
+
1
4
2
n
+
⋯
=
(
−
1
)
n
+
1
B
2
n
(
2
π
)
2
n
2
(
2
n
)
!
{\displaystyle \zeta (2n)=\sum _{k=1}^{\infty }{\frac {1}{k^{2n}}}\,={\frac {1}{1^{2n}}}+{\frac {1}{2^{2n}}}+{\frac {1}{3^{2n}}}+{\frac {1}{4^{2n}}}+\cdots =(-1)^{n+1}{\frac {B_{2n}(2\pi )^{2n}}{2(2n)!}}}
, where B 2n is a Bernoulli number .
∑
n
=
1
∞
3
n
−
1
4
n
ζ
(
n
+
1
)
=
π
{\displaystyle \sum _{n=1}^{\infty }{\frac {3^{n}-1}{4^{n}}}\,\zeta (n+1)=\pi }
[7]
∑
n
=
2
∞
2
(
3
/
2
)
n
−
3
n
(
ζ
(
n
)
−
1
)
=
ln
π
{\displaystyle \sum _{n=2}^{\infty }{\frac {2(3/2)^{n}-3}{n}}(\zeta (n)-1)=\ln \pi }
∑
n
=
1
∞
ζ
(
2
n
)
x
2
n
n
=
ln
π
x
sin
π
x
,
0
<
|
x
|
<
1
{\displaystyle \sum _{n=1}^{\infty }\zeta (2n){\frac {x^{2n}}{n}}=\ln {\frac {\pi x}{\sin \pi x}},\quad 0<|x|<1}
∑
n
=
0
∞
(
−
1
)
n
2
n
+
1
=
1
−
1
3
+
1
5
−
1
7
+
1
9
−
⋯
=
arctan
1
=
π
4
{\displaystyle \sum _{n=0}^{\infty }{\frac {(-1)^{n}}{2n+1}}=1-{\frac {1}{3}}+{\frac {1}{5}}-{\frac {1}{7}}+{\frac {1}{9}}-\cdots =\arctan {1}={\frac {\pi }{4}}}
(see Leibniz formula for pi )
∑
n
=
0
∞
(
−
1
)
(
n
2
−
n
)
/
2
2
n
+
1
=
1
+
1
3
−
1
5
−
1
7
+
1
9
+
1
11
−
⋯
=
π
2
2
{\displaystyle \sum _{n=0}^{\infty }{\frac {(-1)^{(n^{2}-n)/2}}{2n+1}}=1+{\frac {1}{3}}-{\frac {1}{5}}-{\frac {1}{7}}+{\frac {1}{9}}+{\frac {1}{11}}-\cdots ={\frac {\pi }{2{\sqrt {2}}}}}
(Newton , Second Letter to Oldenburg , 1676)[8]
∑
n
=
0
∞
(
−
1
)
n
3
n
(
2
n
+
1
)
=
1
−
1
3
1
⋅
3
+
1
3
2
⋅
5
−
1
3
3
⋅
7
+
1
3
4
⋅
9
−
⋯
=
3
arctan
1
3
=
π
2
3
{\displaystyle \sum _{n=0}^{\infty }{\frac {(-1)^{n}}{3^{n}(2n+1)}}=1-{\frac {1}{3^{1}\cdot 3}}+{\frac {1}{3^{2}\cdot 5}}-{\frac {1}{3^{3}\cdot 7}}+{\frac {1}{3^{4}\cdot 9}}-\cdots ={\sqrt {3}}\arctan {\frac {1}{\sqrt {3}}}={\frac {\pi }{2{\sqrt {3}}}}}
(Madhava series )
∑
n
=
1
∞
(
−
1
)
n
+
1
n
2
=
1
1
2
−
1
2
2
+
1
3
2
−
1
4
2
+
⋯
=
π
2
12
{\displaystyle \sum _{n=1}^{\infty }{\frac {(-1)^{n+1}}{n^{2}}}={\frac {1}{1^{2}}}-{\frac {1}{2^{2}}}+{\frac {1}{3^{2}}}-{\frac {1}{4^{2}}}+\cdots ={\frac {\pi ^{2}}{12}}}
∑
n
=
1
∞
1
(
2
n
)
2
=
1
2
2
+
1
4
2
+
1
6
2
+
1
8
2
+
⋯
=
π
2
24
{\displaystyle \sum _{n=1}^{\infty }{\frac {1}{(2n)^{2}}}={\frac {1}{2^{2}}}+{\frac {1}{4^{2}}}+{\frac {1}{6^{2}}}+{\frac {1}{8^{2}}}+\cdots ={\frac {\pi ^{2}}{24}}}
∑
n
=
0
∞
(
1
2
n
+
1
)
2
=
1
1
2
+
1
3
2
+
1
5
2
+
1
7
2
+
⋯
=
π
2
8
{\displaystyle \sum _{n=0}^{\infty }\left({\frac {1}{2n+1}}\right)^{2}={\frac {1}{1^{2}}}+{\frac {1}{3^{2}}}+{\frac {1}{5^{2}}}+{\frac {1}{7^{2}}}+\cdots ={\frac {\pi ^{2}}{8}}}
∑
n
=
0
∞
(
(
−
1
)
n
2
n
+
1
)
3
=
1
1
3
−
1
3
3
+
1
5
3
−
1
7
3
+
⋯
=
π
3
32
{\displaystyle \sum _{n=0}^{\infty }\left({\frac {(-1)^{n}}{2n+1}}\right)^{3}={\frac {1}{1^{3}}}-{\frac {1}{3^{3}}}+{\frac {1}{5^{3}}}-{\frac {1}{7^{3}}}+\cdots ={\frac {\pi ^{3}}{32}}}
∑
n
=
0
∞
(
1
2
n
+
1
)
4
=
1
1
4
+
1
3
4
+
1
5
4
+
1
7
4
+
⋯
=
π
4
96
{\displaystyle \sum _{n=0}^{\infty }\left({\frac {1}{2n+1}}\right)^{4}={\frac {1}{1^{4}}}+{\frac {1}{3^{4}}}+{\frac {1}{5^{4}}}+{\frac {1}{7^{4}}}+\cdots ={\frac {\pi ^{4}}{96}}}
∑
n
=
0
∞
(
(
−
1
)
n
2
n
+
1
)
5
=
1
1
5
−
1
3
5
+
1
5
5
−
1
7
5
+
⋯
=
5
π
5
1536
{\displaystyle \sum _{n=0}^{\infty }\left({\frac {(-1)^{n}}{2n+1}}\right)^{5}={\frac {1}{1^{5}}}-{\frac {1}{3^{5}}}+{\frac {1}{5^{5}}}-{\frac {1}{7^{5}}}+\cdots ={\frac {5\pi ^{5}}{1536}}}
∑
n
=
0
∞
(
1
2
n
+
1
)
6
=
1
1
6
+
1
3
6
+
1
5
6
+
1
7
6
+
⋯
=
π
6
960
{\displaystyle \sum _{n=0}^{\infty }\left({\frac {1}{2n+1}}\right)^{6}={\frac {1}{1^{6}}}+{\frac {1}{3^{6}}}+{\frac {1}{5^{6}}}+{\frac {1}{7^{6}}}+\cdots ={\frac {\pi ^{6}}{960}}}
In general,
∑
n
=
0
∞
(
−
1
)
n
(
2
n
+
1
)
2
k
+
1
=
(
−
1
)
k
E
2
k
2
(
2
k
)
!
(
π
2
)
2
k
+
1
,
k
∈
N
0
{\displaystyle \sum _{n=0}^{\infty }{\frac {(-1)^{n}}{(2n+1)^{2k+1}}}=(-1)^{k}{\frac {E_{2k}}{2(2k)!}}\left({\frac {\pi }{2}}\right)^{2k+1},\quad k\in \mathbb {N} _{0}}
where
E
2
k
{\displaystyle E_{2k}}
is the
2
k
{\displaystyle 2k}
th Euler number .[9]
∑
n
=
0
∞
(
1
2
n
)
(
−
1
)
n
2
n
+
1
=
1
−
1
6
−
1
40
−
⋯
=
π
4
{\displaystyle \sum _{n=0}^{\infty }{\binom {\frac {1}{2}}{n}}{\frac {(-1)^{n}}{2n+1}}=1-{\frac {1}{6}}-{\frac {1}{40}}-\cdots ={\frac {\pi }{4}}}
∑
n
=
0
∞
1
(
4
n
+
1
)
(
4
n
+
3
)
=
1
1
⋅
3
+
1
5
⋅
7
+
1
9
⋅
11
+
⋯
=
π
8
{\displaystyle \sum _{n=0}^{\infty }{\frac {1}{(4n+1)(4n+3)}}={\frac {1}{1\cdot 3}}+{\frac {1}{5\cdot 7}}+{\frac {1}{9\cdot 11}}+\cdots ={\frac {\pi }{8}}}
∑
n
=
1
∞
(
−
1
)
(
n
2
+
n
)
/
2
+
1
|
G
(
(
−
1
)
n
+
1
+
6
n
−
3
)
/
4
|
=
|
G
1
|
+
|
G
2
|
−
|
G
4
|
−
|
G
5
|
+
|
G
7
|
+
|
G
8
|
−
|
G
10
|
−
|
G
11
|
+
⋯
=
3
π
{\displaystyle \sum _{n=1}^{\infty }(-1)^{(n^{2}+n)/2+1}\left|G_{\left((-1)^{n+1}+6n-3\right)/4}\right|=|G_{1}|+|G_{2}|-|G_{4}|-|G_{5}|+|G_{7}|+|G_{8}|-|G_{10}|-|G_{11}|+\cdots ={\frac {\sqrt {3}}{\pi }}}
(see Gregory coefficients )
∑
n
=
0
∞
(
1
/
2
)
n
2
2
n
n
!
2
∑
n
=
0
∞
n
(
1
/
2
)
n
2
2
n
n
!
2
=
1
π
{\displaystyle \sum _{n=0}^{\infty }{\frac {(1/2)_{n}^{2}}{2^{n}n!^{2}}}\sum _{n=0}^{\infty }{\frac {n(1/2)_{n}^{2}}{2^{n}n!^{2}}}={\frac {1}{\pi }}}
(where
(
x
)
n
{\displaystyle (x)_{n}}
is the rising factorial )[10]
∑
n
=
1
∞
(
−
1
)
n
+
1
n
(
n
+
1
)
(
2
n
+
1
)
=
π
−
3
{\displaystyle \sum _{n=1}^{\infty }{\frac {(-1)^{n+1}}{n(n+1)(2n+1)}}=\pi -3}
(Nilakantha series)
∑
n
=
1
∞
F
2
n
n
2
(
2
n
n
)
=
4
π
2
25
5
{\displaystyle \sum _{n=1}^{\infty }{\frac {F_{2n}}{n^{2}{\binom {2n}{n}}}}={\frac {4\pi ^{2}}{25{\sqrt {5}}}}}
(where
F
n
{\displaystyle F_{n}}
is the n -th Fibonacci number )
∑
n
=
1
∞
σ
(
n
)
e
−
2
π
n
=
1
24
−
1
8
π
{\displaystyle \sum _{n=1}^{\infty }\sigma (n)e^{-2\pi n}={\frac {1}{24}}-{\frac {1}{8\pi }}}
(where
σ
{\displaystyle \sigma }
is the sum-of-divisors function )
π
=
∑
n
=
1
∞
(
−
1
)
ϵ
(
n
)
n
=
1
+
1
2
+
1
3
+
1
4
−
1
5
+
1
6
+
1
7
+
1
8
+
1
9
−
1
10
+
1
11
+
1
12
−
1
13
+
⋯
{\displaystyle \pi =\sum _{n=1}^{\infty }{\frac {(-1)^{\epsilon (n)}}{n}}=1+{\frac {1}{2}}+{\frac {1}{3}}+{\frac {1}{4}}-{\frac {1}{5}}+{\frac {1}{6}}+{\frac {1}{7}}+{\frac {1}{8}}+{\frac {1}{9}}-{\frac {1}{10}}+{\frac {1}{11}}+{\frac {1}{12}}-{\frac {1}{13}}+\cdots }
(where
ϵ
(
n
)
{\displaystyle \epsilon (n)}
is the number of prime factors of the form
p
≡
1
(
m
o
d
4
)
{\displaystyle p\equiv 1\,(\mathrm {mod} \,4)}
of
n
{\displaystyle n}
)[11] [12]
π
2
=
∑
n
=
1
∞
(
−
1
)
ε
(
n
)
n
=
1
+
1
2
−
1
3
+
1
4
+
1
5
−
1
6
−
1
7
+
1
8
+
1
9
+
⋯
{\displaystyle {\frac {\pi }{2}}=\sum _{n=1}^{\infty }{\frac {(-1)^{\varepsilon (n)}}{n}}=1+{\frac {1}{2}}-{\frac {1}{3}}+{\frac {1}{4}}+{\frac {1}{5}}-{\frac {1}{6}}-{\frac {1}{7}}+{\frac {1}{8}}+{\frac {1}{9}}+\cdots }
(where
ε
(
n
)
{\displaystyle \varepsilon (n)}
is the number of prime factors of the form
p
≡
3
(
m
o
d
4
)
{\displaystyle p\equiv 3\,(\mathrm {mod} \,4)}
of
n
{\displaystyle n}
)[13]
π
=
∑
n
=
−
∞
∞
(
−
1
)
n
n
+
1
/
2
{\displaystyle \pi =\sum _{n=-\infty }^{\infty }{\frac {(-1)^{n}}{n+1/2}}}
π
2
=
∑
n
=
−
∞
∞
1
(
n
+
1
/
2
)
2
{\displaystyle \pi ^{2}=\sum _{n=-\infty }^{\infty }{\frac {1}{(n+1/2)^{2}}}}
[14]
The last two formulas are special cases of
π
sin
π
x
=
∑
n
=
−
∞
∞
(
−
1
)
n
n
+
x
(
π
sin
π
x
)
2
=
∑
n
=
−
∞
∞
1
(
n
+
x
)
2
{\displaystyle {\begin{aligned}{\frac {\pi }{\sin \pi x}}&=\sum _{n=-\infty }^{\infty }{\frac {(-1)^{n}}{n+x}}\\\left({\frac {\pi }{\sin \pi x}}\right)^{2}&=\sum _{n=-\infty }^{\infty }{\frac {1}{(n+x)^{2}}}\end{aligned}}}
which generate infinitely many analogous formulas for
π
{\displaystyle \pi }
when
x
∈
Q
∖
Z
.
{\displaystyle x\in \mathbb {Q} \setminus \mathbb {Z} .}
Some formulas relating π and harmonic numbers are given here . Further infinite series involving π are:[15]
π
=
1
Z
{\displaystyle \pi ={\frac {1}{Z}}}
Z
=
∑
n
=
0
∞
(
(
2
n
)
!
)
3
(
42
n
+
5
)
(
n
!
)
6
16
3
n
+
1
{\displaystyle Z=\sum _{n=0}^{\infty }{\frac {((2n)!)^{3}(42n+5)}{(n!)^{6}{16}^{3n+1}}}}
π
=
4
Z
{\displaystyle \pi ={\frac {4}{Z}}}
Z
=
∑
n
=
0
∞
(
−
1
)
n
(
4
n
)
!
(
21460
n
+
1123
)
(
n
!
)
4
441
2
n
+
1
2
10
n
+
1
{\displaystyle Z=\sum _{n=0}^{\infty }{\frac {(-1)^{n}(4n)!(21460n+1123)}{(n!)^{4}{441}^{2n+1}{2}^{10n+1}}}}
π
=
4
Z
{\displaystyle \pi ={\frac {4}{Z}}}
Z
=
∑
n
=
0
∞
(
6
n
+
1
)
(
1
2
)
n
3
4
n
(
n
!
)
3
{\displaystyle Z=\sum _{n=0}^{\infty }{\frac {(6n+1)\left({\frac {1}{2}}\right)_{n}^{3}}{{4^{n}}(n!)^{3}}}}
π
=
32
Z
{\displaystyle \pi ={\frac {32}{Z}}}
Z
=
∑
n
=
0
∞
(
5
−
1
2
)
8
n
(
42
n
5
+
30
n
+
5
5
−
1
)
(
1
2
)
n
3
64
n
(
n
!
)
3
{\displaystyle Z=\sum _{n=0}^{\infty }\left({\frac {{\sqrt {5}}-1}{2}}\right)^{8n}{\frac {(42n{\sqrt {5}}+30n+5{\sqrt {5}}-1)\left({\frac {1}{2}}\right)_{n}^{3}}{{64^{n}}(n!)^{3}}}}
π
=
27
4
Z
{\displaystyle \pi ={\frac {27}{4Z}}}
Z
=
∑
n
=
0
∞
(
2
27
)
n
(
15
n
+
2
)
(
1
2
)
n
(
1
3
)
n
(
2
3
)
n
(
n
!
)
3
{\displaystyle Z=\sum _{n=0}^{\infty }\left({\frac {2}{27}}\right)^{n}{\frac {(15n+2)\left({\frac {1}{2}}\right)_{n}\left({\frac {1}{3}}\right)_{n}\left({\frac {2}{3}}\right)_{n}}{(n!)^{3}}}}
π
=
15
3
2
Z
{\displaystyle \pi ={\frac {15{\sqrt {3}}}{2Z}}}
Z
=
∑
n
=
0
∞
(
4
125
)
n
(
33
n
+
4
)
(
1
2
)
n
(
1
3
)
n
(
2
3
)
n
(
n
!
)
3
{\displaystyle Z=\sum _{n=0}^{\infty }\left({\frac {4}{125}}\right)^{n}{\frac {(33n+4)\left({\frac {1}{2}}\right)_{n}\left({\frac {1}{3}}\right)_{n}\left({\frac {2}{3}}\right)_{n}}{(n!)^{3}}}}
π
=
85
85
18
3
Z
{\displaystyle \pi ={\frac {85{\sqrt {85}}}{18{\sqrt {3}}Z}}}
Z
=
∑
n
=
0
∞
(
4
85
)
n
(
133
n
+
8
)
(
1
2
)
n
(
1
6
)
n
(
5
6
)
n
(
n
!
)
3
{\displaystyle Z=\sum _{n=0}^{\infty }\left({\frac {4}{85}}\right)^{n}{\frac {(133n+8)\left({\frac {1}{2}}\right)_{n}\left({\frac {1}{6}}\right)_{n}\left({\frac {5}{6}}\right)_{n}}{(n!)^{3}}}}
π
=
5
5
2
3
Z
{\displaystyle \pi ={\frac {5{\sqrt {5}}}{2{\sqrt {3}}Z}}}
Z
=
∑
n
=
0
∞
(
4
125
)
n
(
11
n
+
1
)
(
1
2
)
n
(
1
6
)
n
(
5
6
)
n
(
n
!
)
3
{\displaystyle Z=\sum _{n=0}^{\infty }\left({\frac {4}{125}}\right)^{n}{\frac {(11n+1)\left({\frac {1}{2}}\right)_{n}\left({\frac {1}{6}}\right)_{n}\left({\frac {5}{6}}\right)_{n}}{(n!)^{3}}}}
π
=
2
3
Z
{\displaystyle \pi ={\frac {2{\sqrt {3}}}{Z}}}
Z
=
∑
n
=
0
∞
(
8
n
+
1
)
(
1
2
)
n
(
1
4
)
n
(
3
4
)
n
(
n
!
)
3
9
n
{\displaystyle Z=\sum _{n=0}^{\infty }{\frac {(8n+1)\left({\frac {1}{2}}\right)_{n}\left({\frac {1}{4}}\right)_{n}\left({\frac {3}{4}}\right)_{n}}{(n!)^{3}{9}^{n}}}}
π
=
3
9
Z
{\displaystyle \pi ={\frac {\sqrt {3}}{9Z}}}
Z
=
∑
n
=
0
∞
(
40
n
+
3
)
(
1
2
)
n
(
1
4
)
n
(
3
4
)
n
(
n
!
)
3
49
2
n
+
1
{\displaystyle Z=\sum _{n=0}^{\infty }{\frac {(40n+3)\left({\frac {1}{2}}\right)_{n}\left({\frac {1}{4}}\right)_{n}\left({\frac {3}{4}}\right)_{n}}{(n!)^{3}{49}^{2n+1}}}}
π
=
2
11
11
Z
{\displaystyle \pi ={\frac {2{\sqrt {11}}}{11Z}}}
Z
=
∑
n
=
0
∞
(
280
n
+
19
)
(
1
2
)
n
(
1
4
)
n
(
3
4
)
n
(
n
!
)
3
99
2
n
+
1
{\displaystyle Z=\sum _{n=0}^{\infty }{\frac {(280n+19)\left({\frac {1}{2}}\right)_{n}\left({\frac {1}{4}}\right)_{n}\left({\frac {3}{4}}\right)_{n}}{(n!)^{3}{99}^{2n+1}}}}
π
=
2
4
Z
{\displaystyle \pi ={\frac {\sqrt {2}}{4Z}}}
Z
=
∑
n
=
0
∞
(
10
n
+
1
)
(
1
2
)
n
(
1
4
)
n
(
3
4
)
n
(
n
!
)
3
9
2
n
+
1
{\displaystyle Z=\sum _{n=0}^{\infty }{\frac {(10n+1)\left({\frac {1}{2}}\right)_{n}\left({\frac {1}{4}}\right)_{n}\left({\frac {3}{4}}\right)_{n}}{(n!)^{3}{9}^{2n+1}}}}
π
=
4
5
5
Z
{\displaystyle \pi ={\frac {4{\sqrt {5}}}{5Z}}}
Z
=
∑
n
=
0
∞
(
644
n
+
41
)
(
1
2
)
n
(
1
4
)
n
(
3
4
)
n
(
n
!
)
3
5
n
72
2
n
+
1
{\displaystyle Z=\sum _{n=0}^{\infty }{\frac {(644n+41)\left({\frac {1}{2}}\right)_{n}\left({\frac {1}{4}}\right)_{n}\left({\frac {3}{4}}\right)_{n}}{(n!)^{3}5^{n}{72}^{2n+1}}}}
π
=
4
3
3
Z
{\displaystyle \pi ={\frac {4{\sqrt {3}}}{3Z}}}
Z
=
∑
n
=
0
∞
(
−
1
)
n
(
28
n
+
3
)
(
1
2
)
n
(
1
4
)
n
(
3
4
)
n
(
n
!
)
3
3
n
4
n
+
1
{\displaystyle Z=\sum _{n=0}^{\infty }{\frac {(-1)^{n}(28n+3)\left({\frac {1}{2}}\right)_{n}\left({\frac {1}{4}}\right)_{n}\left({\frac {3}{4}}\right)_{n}}{(n!)^{3}{3^{n}}{4}^{n+1}}}}
π
=
4
Z
{\displaystyle \pi ={\frac {4}{Z}}}
Z
=
∑
n
=
0
∞
(
−
1
)
n
(
20
n
+
3
)
(
1
2
)
n
(
1
4
)
n
(
3
4
)
n
(
n
!
)
3
2
2
n
+
1
{\displaystyle Z=\sum _{n=0}^{\infty }{\frac {(-1)^{n}(20n+3)\left({\frac {1}{2}}\right)_{n}\left({\frac {1}{4}}\right)_{n}\left({\frac {3}{4}}\right)_{n}}{(n!)^{3}{2}^{2n+1}}}}
π
=
72
Z
{\displaystyle \pi ={\frac {72}{Z}}}
Z
=
∑
n
=
0
∞
(
−
1
)
n
(
4
n
)
!
(
260
n
+
23
)
(
n
!
)
4
4
4
n
18
2
n
{\displaystyle Z=\sum _{n=0}^{\infty }{\frac {(-1)^{n}(4n)!(260n+23)}{(n!)^{4}4^{4n}18^{2n}}}}
π
=
3528
Z
{\displaystyle \pi ={\frac {3528}{Z}}}
Z
=
∑
n
=
0
∞
(
−
1
)
n
(
4
n
)
!
(
21460
n
+
1123
)
(
n
!
)
4
4
4
n
882
2
n
{\displaystyle Z=\sum _{n=0}^{\infty }{\frac {(-1)^{n}(4n)!(21460n+1123)}{(n!)^{4}4^{4n}882^{2n}}}}
where
(
x
)
n
{\displaystyle (x)_{n}}
is the Pochhammer symbol for the rising factorial. See also Ramanujan–Sato series .
Machin-like formulae [ edit ]
π
4
=
arctan
1
{\displaystyle {\frac {\pi }{4}}=\arctan 1}
π
4
=
arctan
1
2
+
arctan
1
3
{\displaystyle {\frac {\pi }{4}}=\arctan {\frac {1}{2}}+\arctan {\frac {1}{3}}}
π
4
=
2
arctan
1
2
−
arctan
1
7
{\displaystyle {\frac {\pi }{4}}=2\arctan {\frac {1}{2}}-\arctan {\frac {1}{7}}}
π
4
=
2
arctan
1
3
+
arctan
1
7
{\displaystyle {\frac {\pi }{4}}=2\arctan {\frac {1}{3}}+\arctan {\frac {1}{7}}}
π
4
=
4
arctan
1
5
−
arctan
1
239
{\displaystyle {\frac {\pi }{4}}=4\arctan {\frac {1}{5}}-\arctan {\frac {1}{239}}}
(the original Machin's formula)
π
4
=
5
arctan
1
7
+
2
arctan
3
79
{\displaystyle {\frac {\pi }{4}}=5\arctan {\frac {1}{7}}+2\arctan {\frac {3}{79}}}
π
4
=
6
arctan
1
8
+
2
arctan
1
57
+
arctan
1
239
{\displaystyle {\frac {\pi }{4}}=6\arctan {\frac {1}{8}}+2\arctan {\frac {1}{57}}+\arctan {\frac {1}{239}}}
π
4
=
12
arctan
1
49
+
32
arctan
1
57
−
5
arctan
1
239
+
12
arctan
1
110443
{\displaystyle {\frac {\pi }{4}}=12\arctan {\frac {1}{49}}+32\arctan {\frac {1}{57}}-5\arctan {\frac {1}{239}}+12\arctan {\frac {1}{110443}}}
π
4
=
44
arctan
1
57
+
7
arctan
1
239
−
12
arctan
1
682
+
24
arctan
1
12943
{\displaystyle {\frac {\pi }{4}}=44\arctan {\frac {1}{57}}+7\arctan {\frac {1}{239}}-12\arctan {\frac {1}{682}}+24\arctan {\frac {1}{12943}}}
Infinite products [ edit ]
π
4
=
(
∏
p
≡
1
(
mod
4
)
p
p
−
1
)
⋅
(
∏
p
≡
3
(
mod
4
)
p
p
+
1
)
=
3
4
⋅
5
4
⋅
7
8
⋅
11
12
⋅
13
12
⋯
,
{\displaystyle {\frac {\pi }{4}}=\left(\prod _{p\equiv 1{\pmod {4}}}{\frac {p}{p-1}}\right)\cdot \left(\prod _{p\equiv 3{\pmod {4}}}{\frac {p}{p+1}}\right)={\frac {3}{4}}\cdot {\frac {5}{4}}\cdot {\frac {7}{8}}\cdot {\frac {11}{12}}\cdot {\frac {13}{12}}\cdots ,}
(Euler)
where the numerators are the odd primes; each denominator is the multiple of four nearest to the numerator.
3
π
6
=
(
∏
p
≡
1
(
mod
6
)
p
∈
P
p
p
−
1
)
⋅
(
∏
p
≡
5
(
mod
6
)
p
∈
P
p
p
+
1
)
=
5
6
⋅
7
6
⋅
11
12
⋅
13
12
⋅
17
18
⋯
,
{\displaystyle {\frac {{\sqrt {3}}\pi }{6}}=\left(\displaystyle \prod _{p\equiv 1{\pmod {6}} \atop p\in \mathbb {P} }{\frac {p}{p-1}}\right)\cdot \left(\displaystyle \prod _{p\equiv 5{\pmod {6}} \atop p\in \mathbb {P} }{\frac {p}{p+1}}\right)={\frac {5}{6}}\cdot {\frac {7}{6}}\cdot {\frac {11}{12}}\cdot {\frac {13}{12}}\cdot {\frac {17}{18}}\cdots ,}
π
2
=
∏
n
=
1
∞
(
2
n
)
(
2
n
)
(
2
n
−
1
)
(
2
n
+
1
)
=
2
1
⋅
2
3
⋅
4
3
⋅
4
5
⋅
6
5
⋅
6
7
⋅
8
7
⋅
8
9
⋯
{\displaystyle {\frac {\pi }{2}}=\prod _{n=1}^{\infty }{\frac {(2n)(2n)}{(2n-1)(2n+1)}}={\frac {2}{1}}\cdot {\frac {2}{3}}\cdot {\frac {4}{3}}\cdot {\frac {4}{5}}\cdot {\frac {6}{5}}\cdot {\frac {6}{7}}\cdot {\frac {8}{7}}\cdot {\frac {8}{9}}\cdots }
(see also Wallis product )
π
2
=
∏
n
=
1
∞
(
1
+
1
n
)
(
−
1
)
n
+
1
=
(
1
+
1
1
)
+
1
(
1
+
1
2
)
−
1
(
1
+
1
3
)
+
1
⋯
{\displaystyle {\frac {\pi }{2}}=\prod _{n=1}^{\infty }\left(1+{\frac {1}{n}}\right)^{(-1)^{n+1}}=\left(1+{\frac {1}{1}}\right)^{+1}\left(1+{\frac {1}{2}}\right)^{-1}\left(1+{\frac {1}{3}}\right)^{+1}\cdots }
(another form of Wallis product)
Viète's formula :
2
π
=
2
2
⋅
2
+
2
2
⋅
2
+
2
+
2
2
⋅
⋯
{\displaystyle {\frac {2}{\pi }}={\frac {\sqrt {2}}{2}}\cdot {\frac {\sqrt {2+{\sqrt {2}}}}{2}}\cdot {\frac {\sqrt {2+{\sqrt {2+{\sqrt {2}}}}}}{2}}\cdot \cdots }
A double infinite product formula involving the Thue–Morse sequence :
π
2
=
∏
m
≥
1
∏
n
≥
1
(
(
4
m
2
+
n
−
2
)
(
4
m
2
+
2
n
−
1
)
2
4
(
2
m
2
+
n
−
1
)
(
4
m
2
+
n
−
1
)
(
2
m
2
+
n
)
)
ϵ
n
,
{\displaystyle {\frac {\pi }{2}}=\prod _{m\geq 1}\prod _{n\geq 1}\left({\frac {(4m^{2}+n-2)(4m^{2}+2n-1)^{2}}{4(2m^{2}+n-1)(4m^{2}+n-1)(2m^{2}+n)}}\right)^{\epsilon _{n}},}
where
ϵ
n
=
(
−
1
)
t
n
{\displaystyle \epsilon _{n}=(-1)^{t_{n}}}
and
t
n
{\displaystyle t_{n}}
is the Thue–Morse sequence (Tóth 2020 ).
Arctangent formulas [ edit ]
π
2
k
+
1
=
arctan
2
−
a
k
−
1
a
k
,
k
≥
2
{\displaystyle {\frac {\pi }{2^{k+1}}}=\arctan {\frac {\sqrt {2-a_{k-1}}}{a_{k}}},\qquad \qquad k\geq 2}
π
4
=
∑
k
≥
2
arctan
2
−
a
k
−
1
a
k
,
{\displaystyle {\frac {\pi }{4}}=\sum _{k\geq 2}\arctan {\frac {\sqrt {2-a_{k-1}}}{a_{k}}},}
where
a
k
=
2
+
a
k
−
1
{\displaystyle a_{k}={\sqrt {2+a_{k-1}}}}
such that
a
1
=
2
{\displaystyle a_{1}={\sqrt {2}}}
.
π
2
=
∑
k
=
0
∞
arctan
1
F
2
k
+
1
=
arctan
1
1
+
arctan
1
2
+
arctan
1
5
+
arctan
1
13
+
⋯
{\displaystyle {\frac {\pi }{2}}=\sum _{k=0}^{\infty }\arctan {\frac {1}{F_{2k+1}}}=\arctan {\frac {1}{1}}+\arctan {\frac {1}{2}}+\arctan {\frac {1}{5}}+\arctan {\frac {1}{13}}+\cdots }
where
F
k
{\displaystyle F_{k}}
is the k -th Fibonacci number.
π
=
arctan
a
+
arctan
b
+
arctan
c
{\displaystyle \pi =\arctan a+\arctan b+\arctan c}
whenever
a
+
b
+
c
=
a
b
c
{\displaystyle a+b+c=abc}
and
a
{\displaystyle a}
,
b
{\displaystyle b}
,
c
{\displaystyle c}
are positive real numbers (see List of trigonometric identities ). A special case is
π
=
arctan
1
+
arctan
2
+
arctan
3.
{\displaystyle \pi =\arctan 1+\arctan 2+\arctan 3.}
Complex functions [ edit ]
e
i
π
+
1
=
0
{\displaystyle e^{i\pi }+1=0}
(Euler's identity )
The following equivalences are true for any complex
z
{\displaystyle z}
:
e
z
∈
R
↔
ℑ
z
∈
π
Z
{\displaystyle e^{z}\in \mathbb {R} \leftrightarrow \Im z\in \pi \mathbb {Z} }
e
z
=
1
↔
z
∈
2
π
i
Z
{\displaystyle e^{z}=1\leftrightarrow z\in 2\pi i\mathbb {Z} }
[16]
Also
1
e
z
−
1
=
lim
N
→
∞
∑
n
=
−
N
N
1
z
−
2
π
i
n
−
1
2
,
z
∈
C
.
{\displaystyle {\frac {1}{e^{z}-1}}=\lim _{N\to \infty }\sum _{n=-N}^{N}{\frac {1}{z-2\pi in}}-{\frac {1}{2}},\quad z\in \mathbb {C} .}
Suppose a lattice
Ω
{\displaystyle \Omega }
is generated by two periods
ω
1
,
ω
2
{\displaystyle \omega _{1},\omega _{2}}
. We define the quasi-periods of this lattice by
η
1
=
ζ
(
z
+
ω
1
;
Ω
)
−
ζ
(
z
;
Ω
)
{\displaystyle \eta _{1}=\zeta (z+\omega _{1};\Omega )-\zeta (z;\Omega )}
and
η
2
=
ζ
(
z
+
ω
2
;
Ω
)
−
ζ
(
z
;
Ω
)
{\displaystyle \eta _{2}=\zeta (z+\omega _{2};\Omega )-\zeta (z;\Omega )}
where
ζ
{\displaystyle \zeta }
is the Weierstrass zeta function (
η
1
{\displaystyle \eta _{1}}
and
η
2
{\displaystyle \eta _{2}}
are in fact independent of
z
{\displaystyle z}
). Then the periods and quasi-periods are related by the Legendre identity :
η
1
ω
2
−
η
2
ω
1
=
2
π
i
.
{\displaystyle \eta _{1}\omega _{2}-\eta _{2}\omega _{1}=2\pi i.}
Continued fractions [ edit ]
4
π
=
1
+
1
2
2
+
3
2
2
+
5
2
2
+
7
2
2
+
⋱
{\displaystyle {\frac {4}{\pi }}=1+{\cfrac {1^{2}}{2+{\cfrac {3^{2}}{2+{\cfrac {5^{2}}{2+{\cfrac {7^{2}}{2+\ddots }}}}}}}}}
[17]
ϖ
2
π
=
2
+
1
2
4
+
3
2
4
+
5
2
4
+
7
2
4
+
⋱
{\displaystyle {\frac {\varpi ^{2}}{\pi }}={2+{\cfrac {1^{2}}{4+{\cfrac {3^{2}}{4+{\cfrac {5^{2}}{4+{\cfrac {7^{2}}{4+\ddots \,}}}}}}}}}\quad }
(Ramanujan ,
ϖ
{\displaystyle \varpi }
is the lemniscate constant )[18]
π
=
3
+
1
2
6
+
3
2
6
+
5
2
6
+
7
2
6
+
⋱
{\displaystyle \pi ={3+{\cfrac {1^{2}}{6+{\cfrac {3^{2}}{6+{\cfrac {5^{2}}{6+{\cfrac {7^{2}}{6+\ddots \,}}}}}}}}}}
[17]
π
=
4
1
+
1
2
3
+
2
2
5
+
3
2
7
+
4
2
9
+
⋱
{\displaystyle \pi ={\cfrac {4}{1+{\cfrac {1^{2}}{3+{\cfrac {2^{2}}{5+{\cfrac {3^{2}}{7+{\cfrac {4^{2}}{9+\ddots }}}}}}}}}}}
2
π
=
6
+
2
2
12
+
6
2
12
+
10
2
12
+
14
2
12
+
18
2
12
+
⋱
{\displaystyle 2\pi ={6+{\cfrac {2^{2}}{12+{\cfrac {6^{2}}{12+{\cfrac {10^{2}}{12+{\cfrac {14^{2}}{12+{\cfrac {18^{2}}{12+\ddots }}}}}}}}}}}}
For more on the fourth identity, see Euler's continued fraction formula .
(See also Continued fraction and Generalized continued fraction .)
Iterative algorithms [ edit ]
a
0
=
1
,
a
n
+
1
=
(
1
+
1
2
n
+
1
)
a
n
,
π
=
lim
n
→
∞
a
n
2
n
{\displaystyle a_{0}=1,\,a_{n+1}=\left(1+{\frac {1}{2n+1}}\right)a_{n},\,\pi =\lim _{n\to \infty }{\frac {a_{n}^{2}}{n}}}
a
1
=
0
,
a
n
+
1
=
2
+
a
n
,
π
=
lim
n
→
∞
2
n
2
−
a
n
{\displaystyle a_{1}=0,\,a_{n+1}={\sqrt {2+a_{n}}},\,\pi =\lim _{n\to \infty }2^{n}{\sqrt {2-a_{n}}}}
(closely related to Viète's formula)
ω
(
i
n
,
i
n
−
1
,
…
,
i
1
)
=
2
+
i
n
2
+
i
n
−
1
2
+
⋯
+
i
1
2
=
ω
(
b
n
,
b
n
−
1
,
…
,
b
1
)
,
i
k
∈
{
−
1
,
1
}
,
b
k
=
{
0
if
i
k
=
1
1
if
i
k
=
−
1
,
π
=
lim
n
→
∞
2
n
+
1
2
h
+
1
ω
(
10
…
0
⏟
n
−
m
g
m
,
h
+
1
)
{\displaystyle \omega (i_{n},i_{n-1},\dots ,i_{1})=2+i_{n}{\sqrt {2+i_{n-1}{\sqrt {2+\cdots +i_{1}{\sqrt {2}}}}}}=\omega (b_{n},b_{n-1},\dots ,b_{1}),\,i_{k}\in \{-1,1\},\,b_{k}={\begin{cases}0&{\text{if }}i_{k}=1\\1&{\text{if }}i_{k}=-1\end{cases}},\,\pi ={\displaystyle \lim _{n\rightarrow \infty }{\frac {2^{n+1}}{2h+1}}{\sqrt {\omega \left(\underbrace {10\ldots 0} _{n-m}g_{m,h+1}\right)}}}}
(where
g
m
,
h
+
1
{\displaystyle g_{m,h+1}}
is the h+1-th entry of m-bit Gray code ,
h
∈
{
0
,
1
,
…
,
2
m
−
1
}
{\displaystyle h\in \left\{0,1,\ldots ,2^{m}-1\right\}}
)[19]
∀
k
∈
N
,
a
1
=
2
−
k
,
a
n
+
1
=
a
n
+
2
−
k
(
1
−
tan
(
2
k
−
1
a
n
)
)
,
π
=
2
k
+
1
lim
n
→
∞
a
n
{\displaystyle \forall k\in \mathbb {N} ,\,a_{1}=2^{-k},\,a_{n+1}=a_{n}+2^{-k}(1-\tan(2^{k-1}a_{n})),\,\pi =2^{k+1}\lim _{n\to \infty }a_{n}}
(quadratic convergence)[20]
a
1
=
1
,
a
n
+
1
=
a
n
+
sin
a
n
,
π
=
lim
n
→
∞
a
n
{\displaystyle a_{1}=1,\,a_{n+1}=a_{n}+\sin a_{n},\,\pi =\lim _{n\to \infty }a_{n}}
(cubic convergence)[21]
a
0
=
2
3
,
b
0
=
3
,
a
n
+
1
=
hm
(
a
n
,
b
n
)
,
b
n
+
1
=
gm
(
a
n
+
1
,
b
n
)
,
π
=
lim
n
→
∞
a
n
=
lim
n
→
∞
b
n
{\displaystyle a_{0}=2{\sqrt {3}},\,b_{0}=3,\,a_{n+1}=\operatorname {hm} (a_{n},b_{n}),\,b_{n+1}=\operatorname {gm} (a_{n+1},b_{n}),\,\pi =\lim _{n\to \infty }a_{n}=\lim _{n\to \infty }b_{n}}
(Archimedes' algorithm, see also harmonic mean and geometric mean )[22]
For more iterative algorithms, see the Gauss–Legendre algorithm and Borwein's algorithm .
Asymptotics [ edit ]
(
2
n
n
)
∼
4
n
π
n
{\displaystyle {\binom {2n}{n}}\sim {\frac {4^{n}}{\sqrt {\pi n}}}}
(asymptotic growth rate of the central binomial coefficients )
C
n
∼
4
n
π
n
3
{\displaystyle C_{n}\sim {\frac {4^{n}}{\sqrt {\pi n^{3}}}}}
(asymptotic growth rate of the Catalan numbers )
n
!
∼
2
π
n
(
n
e
)
n
{\displaystyle n!\sim {\sqrt {2\pi n}}\left({\frac {n}{e}}\right)^{n}}
(Stirling's approximation )
∑
k
=
1
n
φ
(
k
)
∼
3
n
2
π
2
{\displaystyle \sum _{k=1}^{n}\varphi (k)\sim {\frac {3n^{2}}{\pi ^{2}}}}
(where
φ
{\displaystyle \varphi }
is Euler's totient function )
∑
k
=
1
n
φ
(
k
)
k
∼
6
n
π
2
{\displaystyle \sum _{k=1}^{n}{\frac {\varphi (k)}{k}}\sim {\frac {6n}{\pi ^{2}}}}
Hypergeometric inversions [ edit ]
With
2
F
1
{\displaystyle {}_{2}F_{1}}
being the hypergeometric function , let
|
q
|
<
1
{\displaystyle \left|q\right|<1}
and
Θ
(
q
)
=
∑
n
=
−
∞
∞
q
n
2
{\displaystyle \Theta (q)=\sum _{n=-\infty }^{\infty }q^{n^{2}}}
.
Then
Θ
(
q
)
2
=
2
F
1
(
1
2
,
1
2
,
1
,
z
)
{\displaystyle \Theta (q)^{2}={}_{2}F_{1}\left({\frac {1}{2}},{\frac {1}{2}},1,z\right)}
where
q
=
exp
(
−
π
2
F
1
(
1
/
2
,
1
/
2
,
1
,
1
−
z
)
2
F
1
(
1
/
2
,
1
/
2
,
1
,
z
)
)
,
z
∈
C
∖
{
0
,
1
}
.
{\displaystyle q=\exp \left(-\pi {\frac {{}_{2}F_{1}(1/2,1/2,1,1-z)}{{}_{2}F_{1}(1/2,1/2,1,z)}}\right),\quad z\in \mathbb {C} \setminus \{0,1\}.}
Similarly, let
|
q
|
<
1
{\displaystyle \left|q\right|<1}
and
H
(
q
)
=
1
+
240
∑
n
=
1
∞
σ
3
(
n
)
q
n
,
{\displaystyle \operatorname {H} (q)=1+240\sum _{n=1}^{\infty }\sigma _{3}(n)q^{n},}
with
σ
3
{\displaystyle \sigma _{3}}
being a divisor function .
Then
H
(
q
)
=
2
F
1
(
1
6
,
5
6
,
1
,
z
)
4
{\displaystyle \operatorname {H} (q)={}_{2}F_{1}\left({\frac {1}{6}},{\frac {5}{6}},1,z\right)^{4}}
where
q
=
exp
(
−
2
π
2
F
1
(
1
/
6
,
5
/
6
,
1
,
1
−
z
)
2
F
1
(
1
/
6
,
5
/
6
,
1
,
z
)
)
,
z
∈
C
∖
{
0
,
1
}
.
{\displaystyle q=\exp \left(-2\pi {\frac {{}_{2}F_{1}(1/6,5/6,1,1-z)}{{}_{2}F_{1}(1/6,5/6,1,z)}}\right),\quad z\in \mathbb {C} \setminus \{0,1\}.}
More formulas of this nature can be given, as explained by Ramanujan's theory of elliptic functions to alternative bases.
Miscellaneous [ edit ]
Γ
(
s
)
Γ
(
1
−
s
)
=
π
sin
π
s
{\displaystyle \Gamma (s)\Gamma (1-s)={\frac {\pi }{\sin \pi s}}}
(Euler's reflection formula, see Gamma function )
π
−
s
/
2
Γ
(
s
2
)
ζ
(
s
)
=
π
−
(
1
−
s
)
/
2
Γ
(
1
−
s
2
)
ζ
(
1
−
s
)
{\displaystyle \pi ^{-s/2}\Gamma \left({\frac {s}{2}}\right)\zeta (s)=\pi ^{-(1-s)/2}\Gamma \left({\frac {1-s}{2}}\right)\zeta (1-s)}
(the functional equation of the Riemann zeta function)
e
−
ζ
′
(
0
)
=
2
π
{\displaystyle e^{-\zeta '(0)}={\sqrt {2\pi }}}
e
ζ
′
(
0
,
1
/
2
)
−
ζ
′
(
0
,
1
)
=
π
{\displaystyle e^{\zeta '(0,1/2)-\zeta '(0,1)}={\sqrt {\pi }}}
(where
ζ
(
s
,
a
)
{\displaystyle \zeta (s,a)}
is the Hurwitz zeta function and the derivative is taken with respect to the first variable)
π
=
B
(
1
/
2
,
1
/
2
)
=
Γ
(
1
/
2
)
2
{\displaystyle \pi =\mathrm {B} (1/2,1/2)=\Gamma (1/2)^{2}}
(see also Beta function )
π
=
Γ
(
3
/
4
)
4
agm
(
1
,
1
/
2
)
2
=
Γ
(
1
/
4
)
4
/
3
agm
(
1
,
2
)
2
/
3
2
{\displaystyle \pi ={\frac {\Gamma (3/4)^{4}}{\operatorname {agm} (1,1/{\sqrt {2}})^{2}}}={\frac {\Gamma \left({1/4}\right)^{4/3}\operatorname {agm} (1,{\sqrt {2}})^{2/3}}{2}}}
(where agm is the arithmetic–geometric mean )
π
=
agm
(
θ
2
2
(
1
/
e
)
,
θ
3
2
(
1
/
e
)
)
{\displaystyle \pi =\operatorname {agm} \left(\theta _{2}^{2}(1/e),\theta _{3}^{2}(1/e)\right)}
(where
θ
2
{\displaystyle \theta _{2}}
and
θ
3
{\displaystyle \theta _{3}}
are the Jacobi theta functions [23] )
π
=
−
K
(
k
)
K
(
1
−
k
2
)
ln
q
,
k
=
θ
2
2
(
q
)
θ
3
2
(
q
)
{\displaystyle \pi =-{\frac {\operatorname {K} (k)}{\operatorname {K} \left({\sqrt {1-k^{2}}}\right)}}\ln q,\quad k={\frac {\theta _{2}^{2}(q)}{\theta _{3}^{2}(q)}}}
(where
q
∈
(
0
,
1
)
{\displaystyle q\in (0,1)}
and
K
(
k
)
{\displaystyle \operatorname {K} (k)}
is the complete elliptic integral of the first kind with modulus
k
{\displaystyle k}
; reflecting the nome -modulus inversion problem)[24]
π
=
−
agm
(
1
,
1
−
k
′
2
)
agm
(
1
,
k
′
)
ln
q
,
k
′
=
θ
4
2
(
q
)
θ
3
2
(
q
)
{\displaystyle \pi =-{\frac {\operatorname {agm} \left(1,{\sqrt {1-k'^{2}}}\right)}{\operatorname {agm} (1,k')}}\ln q,\quad k'={\frac {\theta _{4}^{2}(q)}{\theta _{3}^{2}(q)}}}
(where
q
∈
(
0
,
1
)
{\displaystyle q\in (0,1)}
)[24]
agm
(
1
,
2
)
=
π
ϖ
{\displaystyle \operatorname {agm} (1,{\sqrt {2}})={\frac {\pi }{\varpi }}}
(due to Gauss ,[25]
ϖ
{\displaystyle \varpi }
is the lemniscate constant )
i
π
=
Log
(
−
1
)
=
lim
n
→
∞
n
(
(
−
1
)
1
/
n
−
1
)
{\displaystyle i\pi =\operatorname {Log} (-1)=\lim _{n\to \infty }n\left((-1)^{1/n}-1\right)}
(where
Log
{\displaystyle \operatorname {Log} }
is the principal value of the complex logarithm )[note 3]
1
−
π
2
12
=
lim
n
→
∞
1
n
2
∑
k
=
1
n
(
n
mod
k
)
{\displaystyle 1-{\frac {\pi ^{2}}{12}}=\lim _{n\rightarrow \infty }{\frac {1}{n^{2}}}\sum _{k=1}^{n}(n{\bmod {k}})}
(where
n
mod
k
{\textstyle n{\bmod {k}}}
is the remainder upon division of n by k )
π
=
lim
r
→
∞
1
r
2
∑
x
=
−
r
r
∑
y
=
−
r
r
{
1
if
x
2
+
y
2
≤
r
0
if
x
2
+
y
2
>
r
{\displaystyle \pi =\lim _{r\to \infty }{\frac {1}{r^{2}}}\sum _{x=-r}^{r}\;\sum _{y=-r}^{r}{\begin{cases}1&{\text{if }}{\sqrt {x^{2}+y^{2}}}\leq r\\0&{\text{if }}{\sqrt {x^{2}+y^{2}}}>r\end{cases}}}
(summing a circle's area)
π
=
lim
n
→
∞
4
n
2
∑
k
=
1
n
n
2
−
k
2
{\displaystyle \pi =\lim _{n\rightarrow \infty }{\frac {4}{n^{2}}}\sum _{k=1}^{n}{\sqrt {n^{2}-k^{2}}}}
(Riemann sum to evaluate the area of the unit circle)
π
=
lim
n
→
∞
2
4
n
n
!
4
n
(
2
n
)
!
2
=
lim
n
→
∞
2
4
n
n
(
2
n
n
)
2
=
lim
n
→
∞
1
n
(
(
2
n
)
!
!
(
2
n
−
1
)
!
!
)
2
{\displaystyle \pi =\lim _{n\to \infty }{\frac {2^{4n}n!^{4}}{n(2n)!^{2}}}=\lim _{n\rightarrow \infty }{\frac {2^{4n}}{n{2n \choose n}^{2}}}=\lim _{n\rightarrow \infty }{\frac {1}{n}}\left({\frac {(2n)!!}{(2n-1)!!}}\right)^{2}}
(by combining Stirling's approximation with Wallis product)
π
=
lim
n
→
∞
1
n
ln
16
λ
(
n
i
)
{\displaystyle \pi =\lim _{n\to \infty }{\frac {1}{n}}\ln {\frac {16}{\lambda (ni)}}}
(where
λ
{\displaystyle \lambda }
is the modular lambda function )[26] [note 4]
π
=
lim
n
→
∞
24
n
ln
(
2
1
/
4
G
n
)
=
lim
n
→
∞
24
n
ln
(
2
1
/
4
g
n
)
{\displaystyle \pi =\lim _{n\to \infty }{\frac {24}{\sqrt {n}}}\ln \left(2^{1/4}G_{n}\right)=\lim _{n\to \infty }{\frac {24}{\sqrt {n}}}\ln \left(2^{1/4}g_{n}\right)}
(where
G
n
{\displaystyle G_{n}}
and
g
n
{\displaystyle g_{n}}
are Ramanujan's class invariants )[27] [note 5]
See also [ edit ]
References [ edit ]
^ The relation
μ
0
=
4
π
⋅
10
−
7
N
/
A
2
{\displaystyle \mu _{0}=4\pi \cdot 10^{-7}\,\mathrm {N} /\mathrm {A} ^{2}}
was valid until the 2019 redefinition of the SI base units .
^ (integral form of arctan over its entire domain, giving the period of tan )
^ The
n
{\displaystyle n}
th root with the smallest positive principal argument is chosen.
^ When
n
∈
Q
+
{\displaystyle n\in \mathbb {Q} ^{+}}
, this gives algebraic approximations to Gelfond's constant
e
π
{\displaystyle e^{\pi }}
.
^ When
n
∈
Q
+
{\displaystyle {\sqrt {n}}\in \mathbb {Q} ^{+}}
, this gives algebraic approximations to Gelfond's constant
e
π
{\displaystyle e^{\pi }}
.
^ Galperin, G. (2003). "Playing pool with π (the number π from a billiard point of view)" (PDF) . Regular and Chaotic Dynamics . 8 (4): 375–394. doi :10.1070/RD2003v008n04ABEH000252 .
^ Rudin, Walter (1987). Real and Complex Analysis (Third ed.). McGraw-Hill Book Company. ISBN 0-07-100276-6 . p. 4
^ A000796 – OEIS
^ Carson, B. C. (2010), "Elliptic Integrals" , in Olver, Frank W. J. ; Lozier, Daniel M.; Boisvert, Ronald F.; Clark, Charles W. (eds.), NIST Handbook of Mathematical Functions , Cambridge University Press, ISBN 978-0-521-19225-5 , MR 2723248 .
^ Arndt, Jörg; Haenel, Christoph (2001). π Unleashed . Springer-Verlag Berlin Heidelberg. ISBN 978-3-540-66572-4 . page 126
^ Gourdon, Xavier. "Computation of the n-th decimal digit of π with low memory" (PDF) . Numbers, constants and computation . p. 1.
^ Weisstein, Eric W. "Pi Formulas", MathWorld
^ Chrystal, G. (1900). Algebra, an Elementary Text-book: Part II . p. 335.
^ Eymard, Pierre; Lafon, Jean-Pierre (2004). The Number Pi . American Mathematical Society. ISBN 0-8218-3246-8 . p. 112
^ Cooper, Shaun (2017). Ramanujan's Theta Functions (First ed.). Springer. ISBN 978-3-319-56171-4 . (page 647)
^ Euler, Leonhard (1748). Introductio in analysin infinitorum (in Latin). Vol. 1. p. 245
^ Carl B. Boyer , A History of Mathematics , Chapter 21., pp. 488–489
^ Euler, Leonhard (1748). Introductio in analysin infinitorum (in Latin). Vol. 1. p. 244
^ Wästlund, Johan. "Summing inverse squares by euclidean geometry" (PDF) . The paper gives the formula with a minus sign instead, but these results are equivalent.
^ Simon Plouffe / David Bailey. "The world of Pi" . Pi314.net. Retrieved 2011-01-29 . "Collection of series for π " . Numbers.computation.free.fr. Retrieved 2011-01-29 .
^ Rudin, Walter (1987). Real and Complex Analysis (Third ed.). McGraw-Hill Book Company. ISBN 0-07-100276-6 . p. 3
^ Jump up to: a b Loya, Paul (2017). Amazing and Aesthetic Aspects of Analysis . Springer. p. 589. ISBN 978-1-4939-6793-3 .
^ Perron, Oskar (1957). Die Lehre von den Kettenbrüchen: Band II (in German) (Third ed.). B. G. Teubner. p. 36, eq. 24
^ Vellucci, Pierluigi; Bersani, Alberto Maria (2019-12-01). "$$\pi $$-Formulas and Gray code" . Ricerche di Matematica . 68 (2): 551–569. arXiv :1606.09597 . doi :10.1007/s11587-018-0426-4 . ISSN 1827-3491 . S2CID 119578297 .
^ Abrarov, Sanjar M.; Siddiqui, Rehan; Jagpal, Rajinder K.; Quine, Brendan M. (2021-09-04). "Algorithmic Determination of a Large Integer in the Two-Term Machin-like Formula for π" . Mathematics . 9 (17): 2162. arXiv :2107.01027 . doi :10.3390/math9172162 .
^ Arndt, Jörg; Haenel, Christoph (2001). π Unleashed . Springer-Verlag Berlin Heidelberg. ISBN 978-3-540-66572-4 . page 49
^ Eymard, Pierre; Lafon, Jean-Pierre (2004). The Number Pi . American Mathematical Society. ISBN 0-8218-3246-8 . p. 2
^ Borwein, Jonathan M.; Borwein, Peter B. (1987). Pi and the AGM: A Study in Analytic Number Theory and Computational Complexity (First ed.). Wiley-Interscience. ISBN 0-471-83138-7 . page 225
^ Jump up to: a b Borwein, Jonathan M.; Borwein, Peter B. (1987). Pi and the AGM: A Study in Analytic Number Theory and Computational Complexity (First ed.). Wiley-Interscience. ISBN 0-471-83138-7 . page 41
^ Gilmore, Tomack. "The Arithmetic-Geometric Mean of Gauss" (PDF) . Universität Wien . p. 13.
^ Borwein, J.; Borwein, P. (2000). "Ramanujan and Pi" . Pi: A Source Book . Springer Link. pp. 588–595. doi :10.1007/978-1-4757-3240-5_62 . ISBN 978-1-4757-3242-9 .
^ Eymard, Pierre; Lafon, Jean-Pierre (2004). The Number Pi . American Mathematical Society. ISBN 0-8218-3246-8 . p. 248
Further reading [ edit ]
Borwein, Peter (2000). "The amazing number π " (PDF) . Nieuw Archief voor Wiskunde . 5th series. 1 (3): 254–258. Zbl 1173.01300 .
Kazuya Kato, Nobushige Kurokawa, Saito Takeshi: Number Theory 1: Fermat's Dream. American Mathematical Society, Providence 1993, ISBN 0-8218-0863-X .