Bernoulli umbra
In Umbral calculus, the Bernoulli umbra {\displaystyle B_{-}} is an umbra, a formal symbol, defined by the relation {\displaystyle \operatorname {eval} B_{-}^{n}=B_{n}^{-}}, where {\displaystyle \operatorname {eval} } is the index-lowering operator,[1] also known as evaluation operator [2] and {\displaystyle B_{n}^{-}} are Bernoulli numbers, called moments of the umbra.[3] A similar umbra, defined as {\displaystyle \operatorname {eval} B_{+}^{n}=B_{n}^{+}}, where {\displaystyle B_{1}^{+}=1/2} is also often used and sometimes called Bernoulli umbra as well. They are related by equality {\displaystyle B_{+}=B_{-}+1}. Along with the Euler umbra, Bernoulli umbra is one of the most important umbras.
In Levi-Civita field, Bernoulli umbras can be represented by elements with power series {\displaystyle B_{-}=\varepsilon ^{-1}-{\frac {1}{2}}-{\frac {\varepsilon }{24}}+{\frac {3\varepsilon ^{3}}{640}}-{\frac {1525\varepsilon ^{5}}{580608}}+\dotsb } and {\displaystyle B_{+}=\varepsilon ^{-1}+{\frac {1}{2}}-{\frac {\varepsilon }{24}}+{\frac {3\varepsilon ^{3}}{640}}-{\frac {1525\varepsilon ^{5}}{580608}}+\dotsb }, with lowering index operator corresponding to taking the coefficient of {\displaystyle 1=\varepsilon ^{0}} of the power series. The numerators of the terms are given in OEIS A118050[4] and the denominators are in OEIS A118051.[5] Since the coefficients of {\displaystyle \varepsilon ^{-1}} are non-zero, the both are infinitely large numbers, {\displaystyle B_{-}} being infinitely close (but not equal, a bit smaller) to {\displaystyle \varepsilon ^{-1}-1/2} and {\displaystyle B_{+}} being infinitely close (a bit smaller) to {\displaystyle \varepsilon ^{-1}+1/2}.
In Hardy fields (which are generalizations of Levi-Civita field) umbra {\displaystyle B_{+}} corresponds to the germ at infinity of the function {\displaystyle \psi ^{-1}(\ln x)} while {\displaystyle B_{-}} corresponds to the germ at infinity of {\displaystyle \psi ^{-1}(\ln x)-1}, where {\displaystyle \psi ^{-1}(x)} is inverse digamma function.
Exponentiation
[edit ]Since Bernoulli polynomials is a generalization of Bernoulli numbers, exponentiation of Bernoulli umbra can be expressed via Bernoulli polynomials:
- {\displaystyle \operatorname {eval} (B_{-}+a)^{n}=B_{n}(a),}
where {\displaystyle a} is a real or complex number. This can be further generalized using Hurwitz Zeta function:
- {\displaystyle \operatorname {eval} (B_{-}+a)^{p}=-p\zeta (1-p,a).}
From the Riemann functional equation for Zeta function it follows that
- {\displaystyle \operatorname {eval} ,円B_{+}^{-p}=\operatorname {eval} {\frac {B_{+}^{p+1}2^{p}\pi ^{p+1}}{\sin(\pi p/2)\Gamma (p)(p+1)}}}
Derivative rule
[edit ]Since {\displaystyle B_{1}^{+}=1/2} and {\displaystyle B_{1}^{-}=-1/2} are the only two members of the sequences {\displaystyle B_{n}^{+}} and {\displaystyle B_{n}^{-}} that differ, the following rule follows for any analytic function {\displaystyle f(x)}:
- {\displaystyle f'(x)=\operatorname {eval} (f(B_{+}+x)-f(B_{-}+x))=\operatorname {eval} \Delta f(B_{-}+x)}
Elementary functions of Bernoulli umbra
[edit ]As a general rule, the following formula holds for any analytic function {\displaystyle f(x)}:
- {\displaystyle \operatorname {eval} f(B_{-}+x)={\frac {D}{e^{D}-1}}f(x).}
This allows to derive expressions for elementary functions of Bernoulli umbra.
- {\displaystyle \operatorname {eval} \cos(zB_{-})=\operatorname {eval} \cos(zB_{+})={\frac {z}{2}}\cot \left({\frac {z}{2}}\right)}
- {\displaystyle \operatorname {eval} \cosh(zB_{-})=\operatorname {eval} \cosh(zB_{+})={\frac {z}{2}}\coth \left({\frac {z}{2}}\right)}
- {\displaystyle \operatorname {eval} e^{zB_{-}}={\frac {z}{e^{z}-1}}}
- {\displaystyle \operatorname {eval} \ln(B_{-}+z)=\psi (z)}
Particularly,
- {\displaystyle \operatorname {eval} \ln B_{+}=-\gamma } [6]
- {\displaystyle \operatorname {eval} {\frac {1}{\pi }}\ln \left({\frac {B_{+}-{\frac {z}{\pi }}}{B_{-}+{\frac {z}{\pi }}}}\right)=\cot z}
- {\displaystyle \operatorname {eval} {\frac {1}{\pi }}\ln \left({\frac {B_{-}+1/2+{\frac {z}{\pi }}}{B_{-}+1/2-{\frac {z}{\pi }}}}\right)=\tan z}
- {\displaystyle \operatorname {eval} \cos(aB_{-}+x)={\frac {a}{2}}\csc \left({\frac {a}{2}}\right)\cos \left({\frac {a}{2}}-x\right)}
- {\displaystyle \operatorname {eval} \sin(aB_{-}+x)={\frac {a}{2}}\cot \left({\frac {a}{2}}\right)\sin x-{\frac {a}{2}}\cos x}
Particularly,
- {\displaystyle \operatorname {eval} \sin B_{-}=-1/2},
- {\displaystyle \operatorname {eval} \sin B_{+}=1/2},
Relations between exponential and logarithmic functions
[edit ]Bernoulli umbra allows to establish relations between exponential, trigonometric and hyperbolic functions on one side and logarithms, inverse trigonometric and inverse hyperbolic functions on the other side in closed form:
- {\displaystyle \operatorname {eval} \left(\cosh \left(2xB_{\pm }\right)-1\right)=\operatorname {eval} {\frac {x}{\pi }}\operatorname {artanh} \left({\frac {x}{\pi B_{\pm }}}\right)=\operatorname {eval} {\frac {x}{\pi }}\operatorname {arcoth} \left({\frac {\pi B_{\pm }}{x}}\right)=x\coth(x)-1}
- {\displaystyle \operatorname {eval} {\frac {z}{2\pi }}\ln \left({\frac {B_{+}-{\frac {z}{2\pi }}}{B_{-}+{\frac {z}{2\pi }}}}\right)=\operatorname {eval} \cos(zB_{-})=\operatorname {eval} \cos(zB_{+})={\frac {z}{2}}\cot \left({\frac {z}{2}}\right)}
References
[edit ]- ↑ Taylor, Brian D. (1998). "Difference Equations via the Classical Umbral Calculus". Mathematical Essays in honor of Gian-Carlo Rota. pp. 397–411. CiteSeerX 10.1.1.11.7516 . doi:10.1007/978-1-4612-4108-9_21. ISBN 978-1-4612-8656-1.
- ↑ Di Nardo, E. (February 14, 2022). "A new approach to Sheppard's corrections". arXiv:1004.4989 [math.ST].
- ↑ "The classical umbral calculus: Sheffer sequences" (PDF). Lecture Notes of Seminario Interdisciplinare di Matematica. 8: 101–130. 2009.
- ↑ Sloane, N. J. A. (ed.), "Sequence A118050", The On-Line Encyclopedia of Integer Sequences , OEIS Foundation
- ↑ Sloane, N. J. A. (ed.), "Sequence A118051", The On-Line Encyclopedia of Integer Sequences , OEIS Foundation
- ↑ Yu, Yiping (2010). "Bernoulli Operator and Riemann's Zeta Function". arXiv:1011.3352 [math.NT].