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Complements versus Substitutes and Trends in Fertility Choice in Dynastic Models

Listed author(s):
  • Larry E. Jones
  • Alice Schoonbroodt

The Barro-Becker model is a simple intuitive model of fertility choice. In its original formulation, however, it has not been very successful at reproducing the changes in fertility choice in response to decreased mortality and increased income growth that demographers have emphasized in explaining the demographic transition. In this paper we show that this is due to an implicit assumption that number and utility of children are complements, which is a byproduct of the high intertemporal elasticity of substitution (IES) typically assumed in the fertility literature. We show that, not only is this assumption not necessary, but both the qualitative and quantitative properties of the model in terms of fertility choice change dramatically when substitutability and high curvature are assumed. To do so, we first derive analytical comparative statics and perform quantitative experiments. We find that if IES is less than one, model predictions of changes in fertility amount to about two-thirds of those observed in U.S. data since 1800. There are two major sources to these predicted changes, the increase in the growth rate of productivity which accounts for about 90 percent of the predicted fall in fertility before 1880, and changes in mortality which account for 90 percent of the predicted change from 1880 to 1950.

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File URL: http://www.nber.org/papers/w13680.pdf
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Paper provided by National Bureau of Economic Research, Inc in its series NBER Working Papers with number 13680.

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Date of creation: Dec 2007
Publication status: published as Larry E. Jones & Alice Schoonbroodt, 2010. "Complements Versus Substitutes And Trends In Fertility Choice In Dynastic Models," International Economic Review, Department of Economics, University of Pennsylvania and Osaka University Institute of Social and Economic Research Association, vol. 51(3), pages 671-699, 08.
Handle: RePEc:nbr:nberwo:13680
Note: CH EFG HE
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