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Mathematical notes related to Wikipedia articles.
Even Madhava series
The Leibniz formula for π is...
![{\displaystyle 1\,-\,{\frac {1}{3}}\,+\,{\frac {1}{5}}\,-\,{\frac {1}{7}}\,+\,{\frac {1}{9}}\,-\,\cdots \;=\;{\frac {\pi }{4}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/1f2c2651b0fd7e6248009af8fb9cfe66868fef32)
Or, using summation notation:
![{\displaystyle \sum _{n=0}^{\infty }\,{\frac {(-1)^{n}}{2n+1}}\;=\;{\frac {\pi }{4}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/1fb844ad6c47c496c58283e2386ba0921c73870e)
But what happens if we use even denominators?
![{\displaystyle {\frac {1}{2}}\,-\,{\frac {1}{4}}\,+\,{\frac {1}{6}}\,-\,{\frac {1}{8}}\,+\,\cdots \;=\;?}](https://wikimedia.org/api/rest_v1/media/math/render/svg/9fd5dffe0d56a6a638e22ad06d68610fa74059e7)
This turns out to be:
![{\displaystyle \sum _{n=1}^{\infty }\,{\frac {(-1)^{n+1}}{2n}}\;=\;{\frac {\ln(2)}{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/a94c73b2a33f1b6fa6ab7bab2ab6f76a1530ae5f)
Of course we can extend this to the Dirichlet beta function series too:
![{\displaystyle \beta (s)=\sum _{n=0}^{\infty }{\frac {(-1)^{n}}{(2n+1)^{s}}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/32628be466e83329848e892f940cbbb3479e62fb)
Noting that
and
where G is Catalan's constant.
This becomes, in even denominator terms:
![{\displaystyle \gamma (s)=\sum _{n=1}^{\infty }{\frac {(-1)^{n+1}}{(2n)^{s}}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/5999a2794de9f117de59abae6c8bbdb53299d10f)
Where
.
may be
, and
may be
where
is Apéry's constant.
This is also comparable to the Dirichlet eta function:
Table of some of the results
s |
![{\displaystyle \beta (s)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/68de1924763654d862b83e5661568fe84479feba) |
![{\displaystyle \gamma (s)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/975845bbbf539a8b1abd61f1c156d58f351fd09b) |
|
1 |
![{\displaystyle {\frac {\pi }{4}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/1f89d7c88c1c93dce69a46052a8e276e231063de) |
![{\displaystyle {\frac {\ln(2)}{2}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/c6b7350132d2e0e6a898409d2603b4f3c3d67a6d) |
|
2 |
![{\displaystyle G}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f5f3c8921a3b352de45446a6789b104458c9f90b) |
![{\displaystyle {\frac {\pi ^{2}}{48}}?}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3eaba61f5c67263de4acb9d4ee2213a2513b7e98) |
|
3 |
![{\displaystyle {\frac {\pi ^{3}}{32}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/83310969c1182bd9654dc32c36210f89a0a2c4e0) |
![{\displaystyle {\frac {3\zeta (3)}{32}}?}](https://wikimedia.org/api/rest_v1/media/math/render/svg/fb965608c9720e8aaa8981f205539e851af3103a) |
|
So these values are 1/2, 1/4, 1/8 as much for
as for
, or apparently:
![{\displaystyle \gamma (s)={\frac {\eta (s)}{2^{s}}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/035eeab5125670a6325ea7a8cd09f596b0a9bee9)