From Cumulants Back to Moments
Cumulants and moments encode the same local information about a distribution when the relevant derivatives exist, but they organize it differently. Cumulants are especially useful in algebraic calculations; moments are often the quantities needed to describe scale, skewness-related features, or expected powers of a random variable. Recovering moments from cumulants is therefore a useful conversion, not a new source of information.
The conversion is governed by set partitions. Each partition groups the indices \(1,\ldots,n\) into blocks; a block of size \(r\) contributes the \(r\)th cumulant. Summing over all such groupings gives the \(n\)th raw moment. Complete Bell polynomials collect these terms compactly.
The neighborhood condition on \(M\) ensures that these derivatives exist and that its Taylor expansion near zero can be used to identify moments. The moment \(m_r\) is raw: it is the expectation of \(X^r\), not of a power of \(X-E[X]\).
The Set-Partition Formula
A set partition of \(\{1,\ldots,n\}\) is a collection of nonempty, disjoint subsets, called blocks, whose union is the whole set. Write \(\Pi_n\) for the set of all such partitions. For a block \(B\), let \(|B|\) denote its number of elements.
Here is why the formula holds. The Taylor expansions at zero are \(M(t)=\sum_{n\geq0}m_n t^n/n!\) and \(K(t)=\sum_{r\geq1}\kappa_r t^r/r!\). Since \(M(t)=e^{K(t)}\), expanding the exponential groups terms according to how many times each cumulant occurs.
\(e^{K(t)}=\sum_{q\geq0}K(t)^q/q!\). The \(q\)th power selects an ordered list of \(q\) cumulant terms.
A selection of orders \(r_1,\ldots,r_q\) contributes only when \(r_1+\cdots+r_q=n\), with product \(\kappa_{r_1}\cdots\kappa_{r_q}/(r_1!\cdots r_q!q!)\).
For a partition with block sizes \(r_1,\ldots,r_q\), the factorials count the ways to assign \(n\) labeled indices to those blocks. The factor \(q!\) removes the ordering of the blocks.
More formally, the number of partitions with exactly \(j_r\) blocks of size \(r\), for each \(r=1,\ldots,n\), is \(\displaystyle \frac{n!}{\prod_{r=1}^n (r!)^{j_r}j_r!}\), provided \(\sum_{r=1}^n rj_r=n\). The factors \(r!\) account for the orderings within blocks, and \(j_r!\) account for the orderings among blocks of equal size. Each such partition contributes \(\prod_{r=1}^n\kappa_r^{j_r}\). Grouping the partition sum by its block counts therefore proves the coefficient formula
These coefficient arguments can be read as Taylor-series calculations near zero: the assumed moment-generating function is finite in a neighborhood of zero, so its derivatives there identify the moments and cumulants. The exponential identity then equates the coefficients at each finite order. This proves the set-partition formula and its Bell-polynomial form. \(\square\)
The First Five Moments
For low orders, listing the partitions makes the formula concrete. At order four, for example, the partitions have block sizes \(1+1+1+1\), \(2+1+1\), \(2+2\), \(3+1\), or \(4\). Their respective contributions are \(\kappa_1^4\), \(6\kappa_1^2\kappa_2\), \(3\kappa_2^2\), \(4\kappa_1\kappa_3\), and \(\kappa_4\).
The coefficients count partitions, not arbitrary algebraic choices. For instance, at order five there are ten partitions with one block of size three and one block of size two, giving \(10\kappa_3\kappa_2\). The coefficient \(5\) on \(\kappa_1\kappa_4\) counts the five choices of the singleton block.
Worked Example: Recovering Moments of a Symmetric Two-Point Variable
Let \(X\) equal \(-1\) or \(1\), each with probability \(1/2\). Its moment-generating function is \(M(t)=\cosh(t)\), so \(K(t)=\log\cosh(t)\). Through order five, its Taylor expansion is \(K(t)=t^2/2-t^4/12+O(t^6)\). Since the coefficient of \(t^r\) in \(K(t)\) is \(\kappa_r/r!\), this gives \(\kappa_1=0\), \(\kappa_2=1\), \(\kappa_3=0\), \(\kappa_4=-2\), and \(\kappa_5=0\).
Substituting these values gives \(m_1=0\), \(m_2=1\), and \(m_3=0\). At order four, \(m_4=3\kappa_2^2+\kappa_4=3-2=1\). At order five, every term is zero, so \(m_5=0\). Directly, the odd powers of \(X\) have expectation zero by symmetry, while \(X^2=X^4=1\); all five results agree.
Worked Example: A Shifted Two-Point Distribution
Let \(Y\) equal \(0\) or \(2\), each with probability \(1/2\). Then \(M_Y(t)=(1+e^{2t})/2=e^t\cosh(t)\), and \(K_Y(t)=t+\log\cosh(t)\). The expansion above gives cumulants \(\kappa_1=1\), \(\kappa_2=1\), \(\kappa_3=0\), \(\kappa_4=-2\), and \(\kappa_5=0\).
The formulas yield \(m_1=1\), \(m_2=1+1=2\), and \(m_3=1+3=4\). Next, \(m_4=1+6+3-2=8\). Finally, \(m_5=1+10+15-10=16\); the other terms vanish because \(\kappa_3=\kappa_5=0\). Direct evaluation gives \(E[Y^r]=(0^r+2^r)/2=2^{r-1}\) for \(r\geq1\), which is \(1,2,4,8,16\) for the five orders.
Worked Example: A Three-Point Distribution
Let \(Z\) take values \(-1,0,1\) with probabilities \(1/4,1/2,1/4\), respectively. Its moment-generating function is \(M_Z(t)=1/2+\cosh(t)/2=1+t^2/4+t^4/48+O(t^6)\). Using \(\log(1+u)=u-u^2/2+O(u^3)\) with \(u=t^2/4+t^4/48+O(t^6)\), we obtain \(K_Z(t)=t^2/4-t^4/96+O(t^6)\). Thus \(\kappa_1=0\), \(\kappa_2=1/2\), \(\kappa_3=0\), \(\kappa_4=-1/4\), and \(\kappa_5=0\).
The first and third moments are zero, and the second is \(m_2=\kappa_2=1/2\). The fourth moment is \(m_4=3\kappa_2^2+\kappa_4=3(1/2)^2-1/4=3/4-1/4=1/2\). The fifth moment is zero because all the terms in its formula contain a zero cumulant. Directly, \(Z^2=Z^4\) equals one with probability \(1/2\), and the distribution is symmetric, confirming the results.
Interpreting the Conversion Carefully
The first two cumulants have familiar interpretations: \(\kappa_1=E[X]\) and \(\kappa_2=\operatorname{Var}(X)\). Consequently, \(m_2=\kappa_1^2+\kappa_2\) is the identity \(E[X^2]=(E[X])^2+\operatorname{Var}(X)\). At higher orders, cumulants should not be mistaken for raw or central moments. For example, \(\kappa_4\) is not generally \(E[X^4]\); the fourth raw moment also includes contributions from lower-order cumulants.
A common mistake is to use the fourth-moment expression for a central moment, or to omit terms because a cumulant looks like a moment of the same order. The correction is to identify the target first: the formulas here recover \(E[X^r]\). If a central moment is needed, it must be computed from the raw moments or derived using the centered variable. Another useful check is the order-two identity: if a proposed formula gives \(m_2=\kappa_2\) when \(\kappa_1\ne0\), it has lost the contribution from the nonzero mean.
The partition form also explains why Bell polynomials are useful. They organize all possible products of cumulants at a given order and keep the integer coefficients attached to the number of ways each block pattern can occur. This makes higher-order calculations systematic: enumerate block sizes, or use the complete Bell polynomial, rather than guessing terms.
Check Your Understanding
Use the set-partition interpretation and the first five formulas to check your reasoning.
- Write the set-partition formula for \(m_3\) and identify the partition that contributes \(\kappa_1\kappa_2\).
- If \(\kappa_1=0\) and \(\kappa_2=4\), what are \(m_2\) and \(m_4\) in terms of \(\kappa_4\)?
- Why does the term \(10\kappa_2\kappa_3\) appear in the formula for \(m_5\)?
- For the distribution on \(-1,0,1\) in the third example, explain why the fifth raw moment is zero using both its symmetry and the cumulant formula.
- Explain why \(\kappa_4\) alone is not generally the fourth raw moment.