List of formulae involving π

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Template:Pi box The following is a list of significant formulae involving the mathematical constant [[pi|Template:Pi]]. Many of these formulae can be found in the article Pi, or the article [[Approximations of π|Approximations of Template:Pi]].

Euclidean geometry

π=Cd=C2r2r+1

where Template:Math is the circumference of a circle, Template:Math is the diameter, and Template:Math is the radius. More generally,

π=Lw

where Template:Math and Template:Math are, respectively, the perimeter and the width of any curve of constant width.

A=πr2

where Template:Math is the area of a circle. More generally,

A=πab

where Template:Math is the area enclosed by an ellipse with semi-major axis Template:Math and semi-minor axis Template:Math.

C=2πagm⁡(a,b)(a12−∑n=2∞2n−1(an2−bn2))

where Template:Math is the circumference of an ellipse with semi-major axis Template:Math and semi-minor axis Template:Math and an,bn are the arithmetic and geometric iterations of agm⁡(a,b), the arithmetic-geometric mean of Template:Math and Template:Math with the initial values a0=a and b0=b.

A=4πr2

where Template:Math is the area between the witch of Agnesi and its asymptotic line; Template:Math is the radius of the defining circle.

A=Γ(1/4)22πr2=πr2agm⁡(1,1/2)

where Template:Math is the area of a squircle with minor radius Template:Math, Γ is the gamma function.

A=(k+1)(k+2)πr2

where Template:Math is the area of an epicycloid with the smaller circle of radius Template:Math and the larger circle of radius Template:Math (k∈ℕ), assuming the initial point lies on the larger circle.

A=(−1)k+38πa2

where Template:Math is the area of a rose with angular frequency Template:Math (k∈ℕ) and amplitude Template:Math.

L=Γ(1/4)2πc=2πcagm⁡(1,1/2)

where Template:Math is the perimeter of the lemniscate of Bernoulli with focal distance Template:Math.

V=43πr3

where Template:Math is the volume of a sphere and Template:Math is the radius.

SA=4πr2

where Template:Math is the surface area of a sphere and Template:Math is the radius.

HV=12π2r4

where Template:Math is the hypervolume of a 3-sphere and Template:Math is the radius.

SV=2π2r3

where Template:Math is the surface volume of a 3-sphere and Template:Math is the radius.

Regular convex polygons

Sum Template:Math of internal angles of a regular convex polygon with Template:Math sides:

S=(n−2)π

Area Template:Math of a regular convex polygon with Template:Math sides and side length Template:Math:

A=ns24cot⁡πn

Inradius Template:Math of a regular convex polygon with Template:Math sides and side length Template:Math:

r=s2cot⁡πn

Circumradius Template:Math of a regular convex polygon with Template:Math sides and side length Template:Math:

R=s2csc⁡πn

Physics

  • Approximate period of a simple pendulum with small amplitude:
    T≈2πLg
  • Period of a spring-mass system with spring constant k and mass m:
    T=2πmk

A puzzle involving "colliding billiard balls":

⌊bNπ⌋

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 b2Nm, 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

Integrals

2∫−111−x2dx=π (integrating two halves y(x)=1−x2 to obtain the area of the unit circle)
∫024−x2dx=π (integrating a quarter of a circle with a radius of two x2+y2=4 to obtain 4π/4)
∫−∞∞sech⁡xdx=π
∫−∞∞∫t∞e−1/2t2−x2+xtdxdt=∫−∞∞∫t∞e−t2−1/2x2+xtdxdt=π
∫−11dx1−x2=π
∫−∞∞dx1+x2=π[2][note 2] (see also Cauchy distribution)
∫−∞∞sin⁡xxdx=π (see Dirichlet integral)
∫−∞∞e−x2dx=π (see Gaussian integral).
∮dzz=2πi (when the path of integration winds once counterclockwise around 0. See also Cauchy's integral formula).
∫0∞ln⁡(1+1x2)dx=π[3]
∫01x4(1−x)41+x2dx=227−π (see also [[Proof that 22/7 exceeds π|Proof that 22/7 exceeds Template:Pi]]).
∫01x2(1+x)41+x2dx=π−1715
∫0∞xα−1x+1dx=πsin⁡πα,0<α<1
∫0∞dxx(x+a)(x+b)=πagm⁡(a,b) (where agm is the arithmetic–geometric mean;[4] see also elliptic integral)

Note that with symmetric integrands f(−x)=f(x), formulas of the form ∫−aaf(x)dx can also be translated to formulas 2∫0af(x)dx.

Efficient infinite series

∑k=0∞k!(2k+1)!!=∑k=0∞2kk!2(2k+1)!=π2 (see also Double factorial)
∑k=0∞k!2k(2k+1)!!=2π33
∑k=0∞k!(2k)!(25k−3)(3k)!2k=π2
∑k=0∞(−1)k(6k)!(13591409+545140134k)(3k)!(k!)36403203k=427093440010005π (see Chudnovsky algorithm)
∑k=0∞(4k)!(1103+26390k)(k!)43964k=980122π (see Srinivasa Ramanujan, Ramanujan–Sato series)

The following are efficient for calculating arbitrary binary digits of Template:Pi:

∑k=0∞(−1)k4k(24k+1+24k+2+14k+3)=π[5]
∑k=0∞116k(48k+1−28k+4−18k+5−18k+6)=π (see Bailey–Borwein–Plouffe formula)
∑k=0∞116k(88k+2+48k+3+48k+4−18k+7)=2π
∑k=0∞(−1)k210k(−254k+1−14k+3+2810k+1−2610k+3−2210k+5−2210k+7+110k+9)=26π

Plouffe's series for calculating arbitrary decimal digits of Template:Pi:[6]

∑k=1∞k2kk!2(2k)!=π+3

Other infinite series

ζ(2)=112+122+132+142+⋯=π26 (see also Basel problem and Riemann zeta function)
ζ(4)=114+124+134+144+⋯=π490
ζ(2n)=∑k=1∞1k2n=112n+122n+132n+142n+⋯=(−1)n+1B2n(2π)2n2(2n)! , where B2n is a Bernoulli number.
∑n=1∞3n−14nζ(n+1)=π[7]
∑n=1∞7n−18nζ(n+1)=(1+2)π
∑n=2∞2(3/2)n−3n(ζ(n)−1)=ln⁡π
∑n=1∞ζ(2n)x2nn=ln⁡πxsin⁡πx,0<|x|<1
∑n=0∞(−1)n2n+1=1−13+15−17+19−⋯=arctan⁡1=π4 (see Leibniz formula for pi)
∑n=0∞(13n+1−13n+2)=1−12+14−15+⋯=π33
∑n=0∞(−1)(n2−n)/22n+1=1+13−15−17+19+111−⋯=π22 (Newton, Second Letter to Oldenburg, 1676)[8]
∑n=0∞(−1)n3n(2n+1)=1−131⋅3+132⋅5−133⋅7+134⋅9−⋯=3arctan⁡13=π23 (Madhava series)
∑n=1∞(−1)n+1n2=112−122+132−142+⋯=π212
∑n=1∞1(2n)2=122+142+162+182+⋯=π224
∑n=0∞(12n+1)2=112+132+152+172+⋯=π28
∑n=0∞((−1)n2n+1)3=113−133+153−173+⋯=π332
∑n=0∞(12n+1)4=114+134+154+174+⋯=π496
∑n=0∞((−1)n2n+1)5=115−135+155−175+⋯=5π51536
∑n=0∞(12n+1)6=116+136+156+176+⋯=π6960

In general,

∑n=0∞(−1)n(2n+1)2k+1=(−1)kE2k2(2k)!(π2)2k+1,k∈ℕ0

where E2k is the 2kth Euler number.[9]

∑n=0∞(12n)(−1)n2n+1=1−16−140−⋯=π4
∑n=0∞1(4n+1)(4n+3)=11⋅3+15⋅7+19⋅11+⋯=π8
∑n=1∞(−1)(n2+n)/2+1|G((−1)n+1+6n−3)/4|=|G1|+|G2|−|G4|−|G5|+|G7|+|G8|−|G10|−|G11|+⋯=3π (see Gregory coefficients)
∑n=0∞(1/2)n22nn!2∑n=0∞n(1/2)n22nn!2=1π (where (x)n is the rising factorial)[10]
∑n=1∞(−1)n+1n(n+1)(2n+1)=π−3 (Nilakantha series)
∑n=1∞F2nn2(2nn)=4π2255 (where F2n is the 2nth Fibonacci number)
∑n=1∞L2nn2(2nn)=π25 (where Ln is the nth Lucas number)
∑n=1∞σ(n)e−2πn=124−18π (where σ is the sum-of-divisors function)
π=∑n=1∞(−1)ε(n)n=1+12+13+14−15+16+17+18+19−110+111+112−113+⋯   (where ε(n) is the number of prime factors of the form p≡1(mod4) of n)[11][12]
π2=∑n=1∞(−1)ε(n)n=1+12−13+14+15−16−17+18+19+⋯   (where ε(n) is the number of prime factors of the form p≡3(mod4) of n)[13]
π=∑n=−∞∞(−1)nn+1/2
π2=∑n=−∞∞1(n+1/2)2[14]

The last two formulas are special cases of

πsin⁡πx=∑n=−∞∞(−1)nn+x(πsin⁡πx)2=∑n=−∞∞1(n+x)2

which generate infinitely many analogous formulas for π when x∈ℚ∖ℤ.

π=∑n=1∞6n2 (derived from Euler's solution to the Basel problem)

Some formulas relating Template:Pi and harmonic numbers are given here. Further infinite series involving π are:[15]

π=1Z Z=∑n=0∞((2n)!)3(42n+5)(n!)6163n+1
π=4Z Z=∑n=0∞(−1)n(4n)!(21460n+1123)(n!)44412n+1210n+1
π=4Z Z=∑n=0∞(6n+1)(12)n34n(n!)3
π=32Z Z=∑n=0∞(5−12)8n(42n5+30n+55−1)(12)n364n(n!)3
π=274Z Z=∑n=0∞(227)n(15n+2)(12)n(13)n(23)n(n!)3
π=1532Z Z=∑n=0∞(4125)n(33n+4)(12)n(13)n(23)n(n!)3
π=8585183Z Z=∑n=0∞(485)n(133n+8)(12)n(16)n(56)n(n!)3
π=5523Z Z=∑n=0∞(4125)n(11n+1)(12)n(16)n(56)n(n!)3
π=23Z Z=∑n=0∞(8n+1)(12)n(14)n(34)n(n!)39n
π=39Z Z=∑n=0∞(40n+3)(12)n(14)n(34)n(n!)3492n+1
π=21111Z Z=∑n=0∞(280n+19)(12)n(14)n(34)n(n!)3992n+1
π=24Z Z=∑n=0∞(10n+1)(12)n(14)n(34)n(n!)392n+1
π=455Z Z=∑n=0∞(644n+41)(12)n(14)n(34)n(n!)35n722n+1
π=433Z Z=∑n=0∞(−1)n(28n+3)(12)n(14)n(34)n(n!)33n4n+1
π=4Z Z=∑n=0∞(−1)n(20n+3)(12)n(14)n(34)n(n!)322n+1
π=72Z Z=∑n=0∞(−1)n(4n)!(260n+23)(n!)444n182n
π=3528Z Z=∑n=0∞(−1)n(4n)!(21460n+1123)(n!)444n8822n

where (x)n is the Pochhammer symbol for the rising factorial. See also Ramanujan–Sato series.

Machin-like formulae

Template:See also

π4=arctan⁡1
π4=arctan⁡12+arctan⁡13
3π4=arctan⁡2+arctan⁡3
π4=2arctan⁡12−arctan⁡17
π4=2arctan⁡13+arctan⁡17
π4=4arctan⁡15−arctan⁡1239 (the original Machin's formula)
π4=5arctan⁡17+2arctan⁡379
π4=6arctan⁡18+2arctan⁡157+arctan⁡1239
π4=12arctan⁡149+32arctan⁡157−5arctan⁡1239+12arctan⁡1110443
π4=44arctan⁡157+7arctan⁡1239−12arctan⁡1682+24arctan⁡112943

Infinite products

π4=(∏p≡1(mod4)pp−1)⋅(∏p≡3(mod4)pp+1)=34⋅54⋅78⋅1112⋅1312⋯, (Euler)

where the numerators are the odd primes; each denominator is the multiple of four nearest to the numerator.

3π6=(∏p≡1(mod6)p∈ℙpp−1)⋅(∏p≡5(mod6)p∈ℙpp+1)=56⋅76⋅1112⋅1312⋅1718⋯
2π225=(∏p≡1(mod5)p∈ℙp2(p−1)2)(∏p≡2,3(mod5)p∈ℙp2p2+1)(∏p≡4(mod5)p∈ℙp2(p+1)2)=45⋅910⋅4950⋅121100⋅169170⋯,

Where p is p also the prime number.

π2=∏n=1∞(2n)(2n)(2n−1)(2n+1)=21⋅23⋅43⋅45⋅65⋅67⋅87⋅89⋯ (see also Wallis product)
π2=∏n=1∞(1+1n)(−1)n+1=(1+11)+1(1+12)−1(1+13)+1⋯ (another form of Wallis product)

Viète's formula:

2π=22⋅2+22⋅2+2+22⋅⋯

A double infinite product formula involving the Thue–Morse sequence:

π2=∏m≥1∏n≥1((4m2+n−2)(4m2+2n−1)24(2m2+n−1)(4m2+n−1)(2m2+n))ϵn,

where ϵn=(−1)tn and tn is the Thue–Morse sequence Template:Harv.

One elegant infinite product formula:

π=∏n=1∞(1+(n+2)+(2n+1)+(2n−1)(n+2)×(2n+1)×(2n−1))

Arctangent formulas

π2k+1=arctan⁡2−ak−1ak,k≥2
π4=∑k≥2arctan⁡2−ak−1ak,

where ak=2+ak−1 such that a1=2.

π2=∑k=0∞arctan⁡1F2k+1=arctan⁡11+arctan⁡12+arctan⁡15+arctan⁡113+⋯

where Fk is the kth Fibonacci number.

π4=arctan⁡ab+c+arctan⁡ba+c,

For Pythagorean triple (a,b,c).

π=arctan⁡a+arctan⁡b+arctan⁡c

whenever a+b+c=abc and a, b, c are positive real numbers (see List of trigonometric identities). A special case is

π=arctan⁡1+arctan⁡2+arctan⁡3.

Complex functions

eiπ+1=0 (Euler's identity)

The following equivalences are true for any complex z:

ez∈ℝ↔ℑz∈πℤ
ez=1↔z∈2πiℤ[16]

Also

1ez−1=limN→∞∑n=−NN1z−2πin−12,z∈ℂ.

Suppose a lattice Ω is generated by two periods ω1,ω2. We define the quasi-periods of this lattice by η1=ζ(z+ω1;Ω)−ζ(z;Ω) and η2=ζ(z+ω2;Ω)−ζ(z;Ω) where ζ is the Weierstrass zeta function (η1 and η2 are in fact independent of z). Then the periods and quasi-periods are related by the Legendre identity:

η1ω2−η2ω1=2πi.
4π=1+122+322+522+722+⋱[17]
ϖ2π=2+124+324+524+724+⋱ (Ramanujan, ϖ is the lemniscate constant)[18]
π=3+126+326+526+726+⋱[17]
π=41+123+225+327+429+⋱
2π=6+2212+6212+10212+14212+18212+⋱
π=4−21+11−11+21−21+31−3⋱
2π=11+11+21+31+31+5⋱ (The partial numerators consist of two interleaved sequences: the sequence of natural numbers and the sequence of odd numbers, alternating by index.)

For more on the fourth identity, see Euler's continued fraction formula.

Iterative algorithms

a0=1,an+1=(1+12n+1)an,π=limn→∞an2n
a1=0,an+1=2+an,π=limn→∞2n2−an (closely related to Viète's formula)
ω(in,in−1,…,i1)=2+in2+in−12+⋯+i12=ω(bn,bn−1,…,b1),ik∈{−1,1},bk={0if ik=11if ik=−1,π=limn→∞2n+12h+1ω(10…0⏟n−mgm,h+1) (where gm,h+1 is the h+1-th entry of m-bit Gray code, h∈{0,1,…,2m−1})[19]
∀k∈ℕ,a1=2−k,an+1=an+2−k(1−tan⁡(2k−1an)),π=2k+1limn→∞an (quadratic convergence)[20]
a1=1,an+1=an+sin⁡an,π=limn→∞an (cubic convergence)[21]
a0=23,b0=3,an+1=hm⁡(an,bn),bn+1=gm⁡(an+1,bn),π=limn→∞an=limn→∞bn (Archimedes' algorithm, see also harmonic mean and geometric mean)[22]

For more iterative algorithms, see the Gauss–Legendre algorithm and Borwein's algorithm.

Asymptotics

(2nn)∼4nπn (asymptotic growth rate of the central binomial coefficients)
Cn∼4nπn3 (asymptotic growth rate of the Catalan numbers)
n!∼2πn(ne)n (Stirling's approximation)
log⁡n!≃(n+12)log⁡n−n+log⁡2π2
∑k=1nφ(k)∼3n2π2 (where φ is Euler's totient function)
∑k=1nφ(k)k∼6nπ2

The symbol ∼ means that the ratio of the left-hand side and the right-hand side tends to one as n→∞.

The symbol ≃ means that the difference between the left-hand side and the right-hand side tends to zero as n→∞.

Hypergeometric inversions

With 2F1 being the hypergeometric function:

∑n=0∞r2(n)qn=2F1(12,12,1,z)

where

q=exp⁡(−π2F1(1/2,1/2,1,1−z)2F1(1/2,1/2,1,z)),z∈ℂ∖{0,1}

and r2 is the sum of two squares function.

Similarly,

1+240∑n=1∞σ3(n)qn=2F1(16,56,1,z)4

where

q=exp⁡(−2π2F1(1/6,5/6,1,1−z)2F1(1/6,5/6,1,z)),z∈ℂ∖{0,1}

and σ3 is a divisor function.

More formulas of this nature can be given, as explained by Ramanujan's theory of elliptic functions to alternative bases.

Perhaps the most notable hypergeometric inversions are the following two examples, involving the Ramanujan tau function τ and the Fourier coefficients j of the J-invariant (Template:Oeis):

∑n=−1∞jnqn=256(1−z+z2)3z2(1−z)2,
∑n=1∞τ(n)qn=z2(1−z)22562F1(12,12,1,z)12

where in both cases

q=exp⁡(−2π2F1(1/2,1/2,1,1−z)2F1(1/2,1/2,1,z)),z∈ℂ∖{0,1}.

Furthermore, by expanding the last expression as a power series in

121−(1−z)1/41+(1−z)1/4

and setting z=1/2, we obtain a rapidly convergent series for e−2π:[note 3]

e−2π=w2+4w6+34w10+360w14+4239w18+⋯,w=1221/4−121/4+1.

Miscellaneous

Γ(s)Γ(1−s)=πsin⁡πs (Euler's reflection formula, see Gamma function)
π=6ζ(2) (derived from Euler's solution to Basel problem, see Riemann zeta function)
π−s/2Γ(s2)ζ(s)=π−(1−s)/2Γ(1−s2)ζ(1−s) (the functional equation of the Riemann zeta function)
e−ζ′(0)=2π
eζ′(0,1/2)−ζ′(0,1)=π (where ζ(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 (see also Beta function)
π=Γ(3/4)4agm⁡(1,1/2)2=Γ(1/4)4/3agm⁡(1,2)2/32 (where agm is the arithmetic–geometric mean)
π=agm⁡(θ22(1/e),θ32(1/e)) (where θ2 and θ3 are the Jacobi theta functions[23])
agm⁡(1,2)=πϖ (due to Gauss,[24] ϖ is the lemniscate constant)
N⁡(2ϖ)=e2π,N⁡(ϖ)=eπ/2 (where N is the Gauss N-function)
iπ=Log⁡(−1)=limn→∞n((−1)1/n−1) (where Log is the principal value of the complex logarithm)[note 4]
1−π212=limn→∞1n2∑k=1n(nmodk) (where nmodk is the remainder upon division of n by k)
π=limr→∞1r2∑x=−rr∑y=−rr{1if x2+y2≤r0if x2+y2>r (summing a circle's area)
π=limn→∞4n2∑k=1nn2−k2 (Riemann sum to evaluate the area of the unit circle)
π=limn→∞24nn!4n(2n)!2=limn→∞24nn(2nn)2=limn→∞1n((2n)!!(2n−1)!!)2 (by combining Stirling's approximation with Wallis product)
π=limn→∞1nln⁡16λ(ni) (where λ is the modular lambda function)[25][note 5]
π=limn→∞24nln⁡(21/4Gn)=limn→∞24nln⁡(21/4gn) (where Gn and gn are Ramanujan's class invariants)[26][note 6]

See also

References

Notes

Template:Reflist

Other

Template:Reflist

Further reading


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