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2017 | OriginalPaper | Buchkapitel

3. From Sunspots to Black Holes: Singular Dynamics in Macroeconomic Models

verfasst von : Paulo B. Brito, Luís F. Costa, Huw D. Dixon

Erschienen in: Sunspots and Non-Linear Dynamics

Verlag: Springer International Publishing

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Abstract

We present conditions for the emergence of singularities in DGE models. We distinguish between slow-fast and impasse singularity types, review geometrical methods to deal with both types of singularity and apply them to DGE dynamics. We find that impasse singularities can generate new types of DGE dynamics, in particular temporary determinacy/indeterminacy. We illustrate the different nature of the two types of singularities and apply our results to two simple models: the Benhabib and Farmer (1994) model and one with a cyclical fiscal policy rule.

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Fußnoten
1
We use the notation for derivatives \(f_{x}\equiv \frac{\partial y}{\partial x }\) and \(f_{xy}\equiv \frac{\partial ^{2}y}{\partial x\partial y}\).
 
2
For simplicity we exclude the existence of periodic solutions, but the analysis can easily be extended to that case.
 
3
Observe that we are now referring to a two-dimensional projection in (KL) of a three-dimensional system in (KLC).
 
4
See Kuehn (2015) for a recent textbook presentation.
 
5
Major references for continuous-time regular dynamics and bifurcations are Guckenheimer and Holmes (1990) or Kuznetsov (2005).
 
6
Recall we are assuming that \(\delta (K,L,\epsilon )\ne 0\).
 
7
A singular impasse point is a point in \(\mathcal {S}\) such that \(\nabla \delta = \mathbf 0 \).
 
8
Indeed, a one-dimensional manifold.
 
9
A zero-dimensional manifold.
 
10
For a proof, see Cardin et al. (2012) inter alia.
 
11
Benhabib and Farmer (1994, p. 34) already noted this behavior for particular values of the parameters: “As \(\chi \) moves below \(-0.015\) the roots both become real but remain negative until at (approximately) \(\chi =-0.05\) [i.e. \(\epsilon =0\)] one root passes through minus infinity and reemerges as a positive real root”. To compare with our results please note that we introduced a slight change in notation: while the authors set \(\chi \) as non-positive we set \(\chi \) as non-negative.
 
12
For another example in a macro model with imperfect competition see Brito et al. (2016).
 
13
Considering that we have an infinitely-lived representative household, it would act as if budget was balanced at all moments in time, i.e. Ricardian equivalence holds.
 
14
One special case is given by \(\phi =G\) and \(\mu =-1\), corresponding to setting the expenditure level.
 
15
We thank an anonymous referee and Nuno Barradas for suggesting this clarification.
 
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Metadaten
Titel
From Sunspots to Black Holes: Singular Dynamics in Macroeconomic Models
verfasst von
Paulo B. Brito
Luís F. Costa
Huw D. Dixon
Copyright-Jahr
2017
DOI
https://doi.org/10.1007/978-3-319-44076-7_3