10.16
The binomial series is the Maclaurin series expansion for the function one plus x raised to the power m. The series is infinite when m is not a positive integer because the numerator terms never become zero. It converges when the absolute value of x is less than one.
This series can approximate functions like total energy in special relativity. For an object with rest mass m naught moving at velocity v, total energy depends on its mass, velocity, and the speed of light, c.
To apply the binomial series, the energy expression is rewritten as one plus a small term raised to a power. At velocities slower than c, the magnitude of this term stays below one, satisfying the condition for convergence.
Expanding the expression gives terms with increasing powers of velocity. When v is much less than c, each subsequent term approaches zero. Retaining the first two terms gives an approximation for the total energy.
The first term represents the object's rest energy. Subtracting this from the total energy leaves the second term, which is the classical formula for kinetic energy. This shows how the binomial series approximates complex expressions.
The binomial series extends the familiar binomial theorem from finite polynomial expansions to infinite series expansions. This distinction is important: the binomial theorem applies to positive integer exponents, while the binomial series applies more broadly, including fractional and negative exponents. It is obtained from the Maclaurin series of (1 + x)m, where m is any real exponent, and the expansion converges for |x| < 1.
The familiar binomial theorem is
\begin{equation*}(y+x)^n=\sum_{k=0}^{n}\binom{n}{k}x^k y^{n-k}\end{equation*}
Setting y = 1 gives
\begin{equation*}(1+x)^n=\sum_{k=0}^{n}\binom{n}{k}x^k\end{equation*}
This idea is generalized by considering f(x) = (1 + x)m. Using the Maclaurin series,
\begin{equation*}(1+x)^m=1+m x+\jfrac{m(m-1)}{2!}x^2+\frac{m(m-1)(m-2)}{3!}x^3+\cdots\end{equation*}
In compact form,
\begin{equation*}(1+x)^m=\sum_{k=0}^{\infty}\binom{m}{k}x^k\end{equation*}
where
\begin{equation*}\binom{m}{k}= \frac{m(m-1)(m-2)\cdots(m-k+1)}{k!}\end{equation*}
For a positive integer m, the factors eventually include zero, so the series terminates and becomes the binomial theorem. For negative or noninteger m, the factors do not terminate, giving an infinite binomial series.
The binomial series is the Maclaurin series expansion for the function one plus x raised to the power m. The series is infinite when m is not a positive integer because the numerator terms never become zero. It converges when the absolute value of x is less than one.
This series can approximate functions like total energy in special relativity. For an object with rest mass m naught moving at velocity v, total energy depends on its mass, velocity, and the speed of light, c.
To apply the binomial series, the energy expression is rewritten as one plus a small term raised to a power. At velocities slower than c, the magnitude of this term stays below one, satisfying the condition for convergence.
Expanding the expression gives terms with increasing powers of velocity. When v is much less than c, each subsequent term approaches zero. Retaining the first two terms gives an approximation for the total energy.
The first term represents the object's rest energy. Subtracting this from the total energy leaves the second term, which is the classical formula for kinetic energy. This shows how the binomial series approximates complex expressions.
From Chapter 10:
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