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Derivation of the Hopf Model:

To apply system (2) to cross-sectional data, I assume that the realization of system (1) in each district begins at small, random displacements from tex2html_wrap_inline1528 and tex2html_wrap_inline1634 . Each realization then runs for a random time period with positive mean and finite variance. The precise form of the random elements is not important, but it is convenient to assume that the random elements are independently and identically distributed across districts. The result is a data set consisting of the points at which the realizations terminated.

Given only cross-sectional data, the equations of (2) have to be simplified to eliminate parameters that are not uniquely identifiable with such data. Parameters tex2html_wrap_inline1814 , tex2html_wrap_inline1366 and tex2html_wrap_inline1818 are not distinctly defined: replacing tex2html_wrap_inline1814 with tex2html_wrap_inline1822 , tex2html_wrap_inline1366 with tex2html_wrap_inline1826 and tex2html_wrap_inline1818 with tex2html_wrap_inline1830 leaves (2) unchanged. Further, for any choice of tex2html_wrap_inline1638 there is a value of tex2html_wrap_inline1818 that leaves tex2html_wrap_inline1836 invariant. I normalize by setting tex2html_wrap_inline1838 and collapsing tex2html_wrap_inline1836 into a single parameter tex2html_wrap_inline1818 .

The next step is to build in transformations to adjust for the coordinate system used to measure the observations tex2html_wrap_inline1646 and tex2html_wrap_inline1648 . I translate the observations to the origin using tex2html_wrap_inline1654 and tex2html_wrap_inline1656 where tex2html_wrap_inline1668 and tex2html_wrap_inline1670 are parameters with values to be determined. I also allow the form of the periodic orbits (the limit cycles of system (2)) to be elliptical rather than exactly circular. As Figure 2 illustrates, ellipses ought to be better approximations to the form of the orbits than circles would be. In system (2) the appropriate change is to replace tex2html_wrap_inline1856 with tex2html_wrap_inline1858 where tex2html_wrap_inline1860 is a parameter valued in the range tex2html_wrap_inline1862 .

To produce a statistical model I replace the time derivatives dx/dt and dy/dt of system (2) with random variables tex2html_wrap_inline1868 and tex2html_wrap_inline1870 , which I assume to be bivariate normal with expectations tex2html_wrap_inline1872 and covariance matrix tex2html_wrap_inline1874 . I assume that tex2html_wrap_inline1868 and tex2html_wrap_inline1870 are independently and identically distributed across observations. The distributional assumption is justified by the fact that the elliptical orbits are symmetric, and we expect observations to be randomly distributed on orbits near the equilibrium. For observed data tex2html_wrap_inline1646 and tex2html_wrap_inline1648 we now have the bivariate model

  subequations610

where tex2html_wrap_inline1654 , tex2html_wrap_inline1656 . Unknown parameters are tex2html_wrap_inline1888 , tex2html_wrap_inline1890 , tex2html_wrap_inline1818 , tex2html_wrap_inline1860 , tex2html_wrap_inline1668 , tex2html_wrap_inline1670 and tex2html_wrap_inline1900 . Model (4) may be construed as specifying a nonlinear covariance structure.

The bivariate model (4) illustrates the basic method of changing time derivatives into random variables, but we should not expect a bivariate specification to be sufficient to represent the dynamics of system (1) near tex2html_wrap_inline1528 and the Cournot-Nash equilibrium point tex2html_wrap_inline1634 . By the robustness of system (2), we can reasonably treat the dynamics as two-dimensional. But to represent system (2) in terms of the variables of system (1) it is necessary to embed system (2) in a space of dimension greater than two. Because system (2) is valid only in a neighborhood of the equilibrium point, it is reasonable to consider the data for which system (2) is relevant as confined to a compact set that includes tex2html_wrap_inline1540 . Treating that set as a compact manifold in which the flows of system (1) are occurring, we can then use the Whitney embedding theorem (Hirsch 1976, 23-27) to conclude that a four-dimensional model is necessary and sufficient to represent system (2).

Indeed, we have direct evidence from system (1) that two-dimensional models will fail to recover the dynamics. In Figure 2, in the projection into the plane ``contributions to the challenger'' by ``probability that the incumbent wins,'' the flow of system (1) appears to cross itself. The resulting figure `8' pattern is fundamentally unlike the circular pattern of system (2)--a figure `8' cannot be smoothly mapped into a circle. Moreover, by the fundamental uniqueness theorems for differential equations, a flow that crosses itself is impossible (Hirsch and Smale 1974, 161-176). Therefore, even if system (1) were correct, a two-dimensional analysis of the relationship between challenger finances and votes would fail to confirm the dynamics of system (2), leading to the rejection of system (1). But the apparent failure of the model would be an artifact of the chosen pair of variables.

To do a four-dimensional analysis I extend model (4) to define model (3), which in four equations combines the six models of form (4) that can be constructed between pairs of the four observed variables. The log-likelihood, for n observations, is tex2html_wrap_inline1910 . To identify the model I set tex2html_wrap_inline1912 , where k=28 is the number of parameters in model (3). Doing so reduces the log-likelihood to tex2html_wrap_inline1916 .


next up previous
Next: Derivation of the Tests Up: Appendix Previous: Appendix

Walter Mebane
Fri Oct 23 17:45:50 EDT 1998