Power Series Expansion for Hyperbolic Cosine Function

Theorem

The hyperbolic cosine function has the power series expansion:

\(\ds \cosh x\) \(=\) \(\ds \sum_{n \mathop = 0}^\infty \frac {x^{2 n} } {\paren {2 n}!}\)
\(\ds \) \(=\) \(\ds 1 + \frac {x^2} {2!} + \frac {x^4} {4!} + \frac {x^6} {6!} + \cdots\)

valid for all $x \in \R$.


Proof

From Derivative of Hyperbolic Cosine:

$\dfrac \d {\d x} \cosh x = \sinh x$

From Derivative of Hyperbolic Sine:

$\dfrac \d {\d x} \sinh x = \cosh x$


Hence:

$\dfrac {\d^2} {\d x^2} \cosh x = \cosh x$

and so for all $m \in \N$:

\(\ds m = 2 k: \ \ \) \(\ds \dfrac {\d^m} {\d x^m} \cosh x\) \(=\) \(\ds \cosh x\)
\(\ds m = 2 k + 1: \ \ \) \(\ds \dfrac {\d^m} {\d x^m} \cosh x\) \(=\) \(\ds \sinh x\)

where $k \in \Z$.


This leads to the Maclaurin series expansion:

\(\ds \cosh x\) \(=\) \(\ds \sum_{r \mathop = 0}^\infty \paren {\frac {x^{2 k} } {\paren {2 k}!} \map \cosh 0 + \frac {x^{2 k + 1} } {\paren {2 k + 1}!} \map \sinh 0}\)
\(\ds \) \(=\) \(\ds \sum_{r \mathop = 0}^\infty \frac {x^{2 k} } {\paren {2 k}!}\) $\map \sinh 0 = 0$, $\map \cosh 0 = 1$

From Series of Power over Factorial Converges, it follows that this series is convergent for all $x$.

$\blacksquare$


Also see


Sources

  • 1968: Murray R. Spiegel: Mathematical Handbook of Formulas and Tables ... (previous) ... (next): $\S 20$: Series for Hyperbolic Functions: $20.34$
  • 1976: K. Weltner and W.J. Weber: Mathematics for Engineers and Scientists ... (previous) ... (next): $8$. Taylor Series and Power Series: Appendix: Table $8.2$: Power Series of Important Functions
  • 1998: David Nelson: The Penguin Dictionary of Mathematics (2nd ed.) ... (previous) ... (next): hyperbolic functions
  • 2008: David Nelson: The Penguin Dictionary of Mathematics (4th ed.) ... (previous) ... (next): hyperbolic functions
  • 2009: Murray R. Spiegel, Seymour Lipschutz and John Liu: Mathematical Handbook of Formulas and Tables (3rd ed.) ... (previous) ... (next): $\S 22$: Taylor Series: Series for Hyperbolic Functions: $22.34.$