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On the dynamic properties of Okishio’s Monetarist model

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Abstract

In this paper, we reconsider the Monetarist model that was formulated by Okishio (Econ Rev 30:289–299, 1979; Econ Stud Q 31:1–9, 1980) from analytical point of view. The basic model is formulated by a three-dimensional system of nonlinear differential equations, and the long run equilibrium of this system satisfies the typical Monetarist properties, namely, the ‘natural rate of employment’ is attained, and the rate of price inflation and nominal growth rate are determined by the growth rate of nominal money supply that is set by the central bank at the long run equilibrium point. However, as Okishio (Econ Rev 30:289–299, 1979; Econ Stud Q 31:1–9, 1980) correctly pointed out, the dynamic stability of the long run equilibrium point is ensured only if particular conditions for crucial parameter values are satisfied. We further prove by means of Hopf bifurcation theorem that the business cycles which entail cyclical fluctuations of the main variables occur at some range of parameter values. We also investigate the dynamic behavior of the extended model that consists of four-dimensional nonlinear differential equations. Finally, we briefly argue that the Keynesian coordinated active fiscal and monetary stabilization policies are necessary if the inactive Monetarist fiscal and monetary policies cannot ensure the dynamic stability of the macroeconomic system.

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Notes

  1. Okishio’s main contributions in English are collected in Okishio (1993, 2022).

  2. Section 3 is in fact the refinement of Okishio’s (1979, 1980) analysis of the dynamic behavior of the Monetarist model. Okishio (1980) omitted the detailed mathematical description that supports his assertion on the dynamic properties of the Monetarist model. Although Okishio (1979) includes the mathematical analysis of local stability/instability of the long run equilibrium point, its mathematical description is rather sketchy. Furthermore, Okishio’s (1979, 1980) papers do not refer to the possibility of cyclical fluctuations of the main variables. The main contributions of Sect. 3 of this paper are the detailed mathematical analysis of local stability/instability and the study of the possibility of the endogenous cyclical fluctuations around the long run equilibrium point by means of Hopf bifurcation theorem. The analysis of the endogenous cyclical fluctuations in a Monetarist system is quite rare. In this sense, the analysis of cyclical fluctuations in Sect. 3 may be somewhat interesting.

  3. Usually, the dynamic behavior of the public debt is neglected in a typical Monetarist model. Therefore, the analysis of a Monetarist model with the explicit consideration of public debt accumulation in Sects. 4 and 5 may be somewhat interesting.

  4. Okishio (1979) states that his formulation was inspired by the formulations by Nagatani (1969) and Stein (1974).

  5. In our model, asset market consists of only two types of the financial asset, government bond (public debt) and money following the simplified analytical framework in Keynes’ (1936) tradition. In this case, the so called ‘Walras law in the asset market’, which is expressed by the identity “(excess demand of government bond) + (excess demand of money)\(\equiv\) 0”, is satisfied. This means that the bond market is always in equilibrium whenever the equilibrium condition of the money market (Eq. (9)) is satisfied.

  6. This characteristic of the Neoclassical model is called ‘Say’s law’ (cf. Okishio 1980). In this Neoclassical framework, the existence of firms’ investment function that is independent of households’ saving function is not allowed for.

  7. From Assumption 1 and Lemma 1, \(E_{n} < 0\) follows. From Eqs. (12) and (13), we have \(r_{E} y_{n} = r_{n} y_{E} .\) Therefore, we obtain \(i_{n} = 0.\)

  8. Following Okishio’s (1979, 1980) procedure, we neglect the depreciation of capital stock for simplicity of the analysis, so that in this model, the distinction between gross investment and net investment is not necessaey.

  9. See, for example, Gandolfo(2009) Chap. 18. It must be noted that all of the elements \(F_{ij}\) and \(G_{ij}\) are independent of the parameter value \(\gamma .\)

  10. This stability concept belongs to the ‘Old Keynesian’ tradition that was proposed by Tobin (1994) as well as Friedman’s (1968, 1977) traditional Monetarism, which is in contrast to the stability concept of ‘New Keynesian’ literature such as Galí (2015) and Woodford (2003). So called ‘jump variables’ approach of the ‘New Keynesian’ literature assumes that the initial conditions of some endogenous variables can be freely ‘chosen’ by the economic agents, so that the equilibrium point of the dynamic system can be ‘stable’ even if some of the characteristic roots have positive real parts. In contrast to this treatment, in the traditional approach without ‘jump variables’ that is adopted in this paper, initial conditions of all endogenous variables are fixed, and they cannot be freely ‘chosen’.

  11. See Gandolfo (2009) Chap. 16. The usual expression of the Routh-Hurwitz conditions in the three-dimensional system of differential equations is

    \(a_{1} > 0,\) \(a_{2} > 0,\) \(a_{3} > 0,\) \(a_{1} a_{2} - a_{3} > 0.\;\;\;\;\;\;\;\;\;\;\;\;\;\;({\text{F}}1)\)

    However, it is easy to see that the inequality \(a_{2} > 0\) is automatically satisfied if a set of inequality (67) is satisfied. This means that a set of conditions (67) is equivalent to a set of conditions (F1).

  12. This conclusion applies to Friedman’s (1968, 1977) approach, because Friedman (1968, 1977) adopts the adaptive expectation hypothesis of inflation expectation formation like the present model. On the other hand, the recent mainstream modeling strategy, that includes the so-called ‘New Keynesian’ approach as well as the ‘New Classical’ approach, adopts the ‘rational expectation’ hypothesis of inflation expectation, which assumes that the omniscient economic agents with full information of economic structure can solve the dynamic optimization problem (cf. Woodford 2003, Galí 2015, and Romer 2019). In such an approach, the concept of ‘stability’ and ‘instability’ in traditional dynamic analysis that is adopted in this paper becomes meaningless. However, some Keynesian-oriented economists criticize such an approach from the standpoint of realism. See, for example, Chiarella et al. (2013) as for the critical assessment of such a modeling strategy by the recent mainstream macroeconomics.

  13. See Benhabib and Miyao (1981) and Asada(1995) as relatively early examples of the applications of Hopf bifurcation theorem to macrodynamic analysis.

  14. To find such a critical parameter value numerically is not easy task unless we resort to numerical simulations.

  15. It must be noted that \(B\) is the stock of nominal public debt that is owned by the private sector. In other words, \(B\) does not include the public debt that is owned by the central bank.

  16. This equation is simply a definitional equation, and it is utilized by Asada (2014), Asada et al. (2023), and Wray (2015). Wray (2015) rejects to call it the ‘budget constraint’, because of the reason that theoretically the central bank can issue high-powered money indefinitely. Nevertheless, we adopt the terminology ‘budget constraint’ following the conventional custom. Incidentally, in this model the equilibrium in the market of the government bond is always satisfied because of the ‘Walras law in the asset market’ (see footnote (5)).

  17. We need not make explicit the detailed expressions of \(F_{41} ,\) \(F_{42} ,\) and \(F_{43}\) for our purpose.

  18. In Sect. 5, we shall consider the economic implication of the consumption from the interest income of the public debt.

  19. From Eqs. (16) and (18), \(y = (Y/K)\) becomes constant at the long run equilibrium point. This means that \(\dot{Y}/Y = \dot{K}/K\) at that point.

  20. As for the ‘Domar condition’, see Asada (2014). Blanchard (2023) also uses this inequality extensively as an important condition for the stability of the public debt dynamics. Surprisingly enough, however, he never refers to the term ‘Domar condition’, and he does not include Domar’s contribution in the references in his book.

  21. In these equations, \(h\) becomes constant from Eq. (18).

  22. A salient difference between these two models is that the ‘Domar condition’ is not required as one of the necessary conditions for dynamic stability in MMT type model.

  23. It is easy to see that the condition \(a_{2} > 0\) is automatically satisfied if a set of conditions (133) is satisfied. Therefore, a set of inequalities (133) is equivalent to a set of inequalities \(a_{1} > 0,\)\(a_{2} > 0,\)\(a_{3} > 0,\)\(a_{1} a_{2} - a_{3} = 0.\)

  24. As footnote (23) notes, it is easy to see that the condition \(a_{2} (\varepsilon_{0} ) > 0\) is automatically satisfied if a set of conditions (135) is satisfied.

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Acknowledgements

The author is grateful to two anonymous reviewers for their helpful comments. It is needless to say, however, only the author is responsible for possible remaining errors. This research was financially supported by Chuo University Personal Research Grant 2024.

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Chuo University, Chuo University Personal Grant 2024, Toichiro Asada.

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Appendices

Appendix A

Proof of Lemma 2

Step 1

First, let us consider a special case of \(g_{r} * = 0\) and \(i_{{\pi^{e} }} * = 1.\) In this case, Eq. (61) becomes as follows.

$$ \begin{aligned} F_{11} = & - [\mathop {f_{E} *}\limits_{( + )} \mathop {E_{m} *}\limits_{( + )} + \mathop {g_{{i - \pi^{e} }} *}\limits_{( - )} \mathop {i_{m} *}\limits_{( - )} ]m* < 0, \\ F_{12} = & - \mathop {f_{E} *}\limits_{( + )} \mathop {E_{n} *}\limits_{( - )} m* > 0, \\ F_{13} = & - [\mathop {f_{E} *}\limits_{( + )} \mathop {E_{{\pi^{e} }} *}\limits_{( + )} + 1 - \mathop {g_{{i - \pi^{e} }} *}\limits_{( - )} ]m* < 0, \\ F_{21} = & - \mathop {g_{{i - \pi^{e} }} *}\limits_{( - )} \mathop {i_{m} *}\limits_{( - )} n* < 0, \\ F_{22} = & F_{23} = 0, \\ G_{31} = & \mathop {f_{E} *}\limits_{( + )} \mathop {E_{m} *}\limits_{( + )} > 0, \\ G_{32} = & \mathop {f_{E} *}\limits_{( + )} \mathop {E_{n} *}\limits_{( - )} < 0, \\ G_{33} = & \mathop {f_{E} *}\limits_{( + )} \mathop {E_{{\pi^{e} }} *}\limits_{( + )} > 0. \\ \end{aligned} $$
(114)

Substituting Eq. (114) into Eqs. (63), (64) and (65) in the text, we obtain the following results.

$$ A_{2} = - \mathop {F_{11} }\limits_{( - )} > 0. $$
(115)
$$ \begin{aligned} A_{3} = & - \mathop {F_{13} }\limits_{( - )} \mathop {G_{31} }\limits_{( + )} + (\mathop {F_{11} }\limits_{( - )} + \mathop {F_{22} }\limits_{( - )} )\mathop {G_{33} }\limits_{( + )} \\ = & \mathop {f_{E} *}\limits_{( + )} [ - \mathop {g_{{i - \pi^{e} }} *}\limits_{( - )} \{ \mathop {i_{m} *}\limits_{( - )} \mathop {E_{{\pi^{e} }} *}\limits_{( + )} (m* + n*) + \mathop {E_{m} *}\limits_{( + )} m*\} + \mathop {E_{m} *}\limits_{( + )} m*] \\ = & \mathop {f_{E} *}\limits_{( + )} \left| {g_{{i - \pi^{e} }} *} \right|[\mathop {i_{m} *}\limits_{( - )} \mathop {E_{{\pi^{e} }} *}\limits_{( + )} (m* + n*) + \mathop {E_{m} *}\limits_{( + )} m* + (\mathop {E_{m} *}\limits_{( + )} m*/\left| {g_{{i - \pi^{e} }} *} \right|)]. \\ \end{aligned} $$
(116)
$$ A_{4} = - \mathop {F_{12} }\limits_{( + )} \mathop {F_{21} }\limits_{( - )} > 0. $$
(117)
$$ \begin{aligned} A_{5} = & \left| {\begin{array}{*{20}c} {F_{11} } & {F_{12} } & {F_{13} } \\ {F_{21} } & 0 & 0 \\ {G_{31} } & {G_{32} } & {G_{33} } \\ \end{array} } \right| = - \mathop {F_{21} }\limits_{( - )} (\mathop {F_{12} }\limits_{( + )} \mathop {G_{33} }\limits_{( + )} - \mathop {F_{13} }\limits_{( - )} \mathop {G_{32} }\limits_{( - )} ) \\ = & - \mathop {F_{21} }\limits_{( - )} \{ (1 - \mathop {g_{{i - \pi^{e} }} *}\limits_{( - )} )\mathop {f_{E} *}\limits_{( + )} \mathop {E_{n} *}\limits_{( - )} m*\} < 0. \\ \end{aligned} $$
(118)

Step 2

Equations (115), (117) and (118) imply that we have \(A_{2} > 0,\) \(A_{4} > 0,\) and \(A_{5} < 0\) in a special case of \(g_{r} * = 0\) and \(i_{{\pi^{e} }} * = 1.\) However, by continuity, these inequalities are also satisfied as long as \(g_{r} *\) is sufficiently small and \(i_{{\pi^{e} }} *\) is sufficiently close to 1, even if \(g_{r} > 0\) and \(i_{{\pi^{e} }} * \ne 1.\) Incidentally, we have the following expression in case of \(g_{r} * = 0\) from Eqs. (28) and (34).

$$ \begin{aligned} i_{{\pi^{e} }} * = & \frac{{ - \{ 1 - (1 - \tau )y_{E} *\} y*r_{E} * - (1 - \tau )c_{{\pi^{e} }} *y_{E} *\phi * - \left| {g_{{i - \pi^{e} }} *} \right|y_{E} *\phi *}}{{\{ 1 - (1 - \tau )c*\} y*\phi_{i} * - \left| {g_{{i - \pi^{e} }} *} \right|y_{E} *\phi *}} \\ = & \frac{{[ - \{ 1 - (1 - \tau )y_{E} *y*r_{E} * - (1 - \tau )c_{{\pi^{e} }} *y*y_{E} *\phi *]/\left| {g_{{i - \pi^{e} }} *} \right| - y_{E} *\phi *}}{{\{ 1 - (1 - \tau )c*\} y*\phi_{i} */\left| {g_{{i - \pi^{e} }} *} \right| - y_{E} *\phi *}} \\ \end{aligned} $$
(119)

It follows from Eq. (119) that

$$ \mathop {\lim }\limits_{{\left| {g_{{i - \pi^{e} }} *} \right| \to + \infty }} i_{{\pi^{e} }} * = ( - y_{E} *\phi *)/( - y_{E} *\phi *) = 1. $$
(120)

From continuity, Eq. (120) implies that \(i_{{\pi^{e} }} *\) is sufficiently close to 1 if \(\left| {g_{{i - \pi^{e} }} *} \right|\) is sufficiently large.

Step 3

Finally, we shall turn to the question whether \(A_{3}\) is positive or not. From Eqs. (28), (29), (30) and (33), we obtain the following expressions in case of \(g_{r} * = 0.\)

$$ \begin{aligned} E_{m} * = & \frac{{ - \left| {g_{{i - \pi^{e} }} *} \right|}}{{\{ 1 - (1 - \tau )c*\} y*\phi_{i} * - \left| {g_{{i - \pi^{e} }} *} \right|y_{E} *\phi *}} \\ = & \frac{ - 1}{{\{ 1 - (1 - \tau )c*\} y*\phi_{i} */\left| {g_{{i - \pi^{e} }} *} \right| - y_{E} *\phi *}} \\ \end{aligned} $$
(121)
$$ i_{m} * = \frac{{\{ 1 - (1 - \tau )c*\} y_{E} *}}{{\{ 1 - (1 - \tau )c*\} y*\phi_{i} * - \left| {g_{{i - \pi^{e} }} *} \right|y_{E} *\phi *}} $$
(122)
$$ \begin{aligned} E_{{\pi^{e} }} * = & \frac{{(1 - \tau )y*\phi_{i} * + (\phi_{i} * + \phi_{{\pi^{e} }} *)\left| {g_{{i - \pi^{e} }} *} \right|}}{{\{ 1 - (1 - \tau )c*\} y*\phi_{i} * - \left| {g_{{i - \pi^{e} }} *} \right|y_{E} *\phi *}} \\ = & \frac{{(1 - \tau )y*\phi_{i} */\left| {g_{{i - \pi^{e} }} *} \right| + (\phi_{i} * + \phi_{{\pi^{e} }} *)}}{{\{ 1 - (1 - \tau )c*\} y*\phi_{i} */\left| {g_{{i - \pi^{e} }} *} \right| - y_{E} *\phi *}} \\ \end{aligned} $$
(123)

From these equations, we have the following results.

$$ \mathop {\lim }\limits_{{\left| {g_{{i - \pi^{e} }} *} \right| \to + \infty }} E_{m} * = 1/(\mathop {y_{E} *}\limits_{( + )} \mathop {\phi *}\limits_{( + )} ) > 0 $$
(124)
$$ \mathop {\lim }\limits_{{\left| {g_{{i - \pi^{e} }} *} \right| \to + \infty }} i_{m} * = 0 $$
(125)
$$ \mathop {\lim }\limits_{{\left| {g_{{i - \pi^{e} }} *} \right| \to + \infty }} E_{{\pi^{e} }} * = - (\mathop {\phi_{i} *}\limits_{( - )} + \mathop {\phi_{{\pi^{e} }} *}\limits_{( - )} )/(\mathop {y_{E} *}\limits_{( + )} \mathop {\phi *}\limits_{( + )} ) > 0 $$
(126)

Eqs. (116), (124), (125) and (126) imply that \(A_{3}\) is positive for all sufficiently large values of \(\left| {g_{{i - \pi^{e} }} *} \right|.\) We obtained this conclusion under the assumption of \(g_{r} * = 0.\) However, this conclusion applies even if \(g_{r} * > 0\) as long as \(g_{r} *\) is sufficiently small, by continuity. This completes the proof of Lemma 2. \(\quad \square\)

Appendix B

Proof of Proposition 3

Suppose that \(g_{r} * > 0\) is sufficiently small and \(\left| {g_{{i - \pi^{e} }} *} \right|\) is sufficiently large. Then, we have the following results from Eqs. (63)–(66) and Lemma 2.

$$ a_{1} = - \mathop {A_{1} }\limits_{( + )} \gamma + \mathop {A_{2} }\limits_{( + )} \equiv \Phi_{1} (\gamma );\;\Phi_{1} (0) = \mathop {A_{2} }\limits_{( + )} > 0. $$
(127)
$$ a_{3} = - \gamma \mathop {A_{5} }\limits_{( - )} > 0\;{\text{for all}}\;\gamma > 0. $$
(128)
$$ \begin{aligned} a_{1} a_{2} - a_{3} = & - \mathop {A_{1} }\limits_{( + )} \mathop {A_{3} }\limits_{( + )} \gamma^{2} + ( - \mathop {A_{1} }\limits_{( + )} \mathop {A_{4} }\limits_{( + )} + \mathop {A_{2} }\limits_{( + )} \mathop {A_{3} }\limits_{( + )} + \mathop {A_{5} }\limits_{( - )} )\gamma + \mathop {A_{2} }\limits_{( + )} \mathop {A_{4} }\limits_{( + )} \equiv \Phi_{2} (\lambda ) \\ \Phi_{2} (0) = & \mathop {A_{2} }\limits_{( + )} \mathop {A_{4} }\limits_{( + )} > 0. \\ \end{aligned} $$
(129)

Eq. (128) implies that one of a series of Routh-Hurwitz conditions (67) is always satisfied for all \(\gamma > 0.\) In this case, the local stability conditions of the equilibrium point of the dynamic system (54a)–(54c) can be reduced to the following set of inequalities.

$$ a_{1} \equiv \Phi_{1} (\gamma ) > 0,\;a_{1} a_{2} - a_{3} \equiv \Phi_{2} (\gamma ) > 0 $$
(130)

Eq. (127) means that we have \(\Phi_{1} (\gamma ) > 0\) for all \(\gamma \in (0,\gamma_{1} ),\) \(\Phi_{1} (\gamma_{1} ) = 0,\) and \(\Phi_{1} (\gamma ) < 0\) for all \(\gamma \in (\gamma_{1} , + \infty ),\) where \(\gamma_{1} = A_{2} /A_{1} > 0.\)

On the other hand, Eq. (129) means that \(\Phi_{2} (\gamma )\) is a quadratic function of \(\gamma\) such that \(\Phi_{2} (0) > 0\) and the coefficient of \(\gamma^{2}\) is negative. This means that there exists a positive parameter value \(\gamma_{0}\) such that we have \(\Phi_{2} (\gamma ) > 0\) for all \(\gamma \in (0,\gamma_{0} ),\) \(\Phi_{2} (\gamma_{0} ) = 0,\) and \(\Phi_{2} (\gamma ) < 0\) for all \(\gamma \in (\gamma_{0} , + \infty ).\) Incidentally, we have \(\Phi_{2} (\gamma_{1} ) = - a_{3} < 0,\) so that we obtain the inequality

$$ 0 < \gamma_{0} < \gamma_{1} . $$
(131)

These results imply the following conclusion.

  1. (1)

    The long run equilibrium point of the dynamic system (54a)–(54c) is locally stable if \(\gamma \in (0,\gamma_{0} ),\) because a set of inequalities (130) is satisfied at the open interval \((0,\gamma_{0} ).\)

  2. (2)

    It is locally unstable if \(\gamma \in (\gamma_{0} , + \infty ),\) because we have \(\Phi_{2} (\gamma ) < 0\) at the open interval \((\gamma_{0} , + \infty ).\)

This completes the proof of Proposition 3. \(\quad \square\)

Appendix C: Two useful theorems for the analysis of cyclical fluctuations

In this appendix, we present two theorems that are useful for the analysis of cyclical fluctuations in the dynamic system (54a)–(54c) in the text. Theorem 1 presents a set of sufficient conditions for the existence of the closed orbits in an n-dimensional system of nonlinear differential equations. Theorem 2 presents some useful results in case of three-dimensional system.

Theorem 1

(Hopf bifurcation theorem for an n-dimensional dynamic system, cf. Gandolfo (2009) Chap. 24).

Let \(\dot{x} = f(x;\varepsilon ),\) \(x \in R^{n} ,\) \(\varepsilon \in R\) be an n-dimensional system of differential equations depending upon a parameter \(\varepsilon .\) Suppose that the following conditions (H1)–(H3) are satisfied.

  1. (H1)

    The system has a smooth curve of equilibria given by \(f(x*(\varepsilon );\varepsilon ) = 0.\)

  2. (H2)

    The characteristic equation \(\left| {\lambda I - Df(x*(\varepsilon_{0} );\varepsilon_{0} )} \right| = 0\) has a pair of pure imaginary roots \(\lambda (\varepsilon_{0} ),\) \(\overline{\lambda }(\varepsilon_{0} )\) and no other roots with zero real parts, where \(Df(x*(\varepsilon_{0} );\varepsilon_{0} )\) is the Jacobian matrix of the above system at \((x*(\varepsilon_{0} ),\varepsilon_{0} )\) with the parameter value \(\varepsilon_{0} .\)

  3. (H3)

    \(\left. {\frac{{d\{ {\text{Re}} \lambda (\varepsilon )\} }}{d\varepsilon }} \right|_{{\varepsilon = \varepsilon_{0} }} \ne 0,\) where \({\text{Re}} \lambda (\varepsilon )\) is the real part of \(\lambda (\varepsilon ).\)

Then, there exists a continuous function \(\varepsilon (\xi )\) with \(\varepsilon (0) = \varepsilon_{0} ,\) and for all sufficiently small values of \(\xi \ne 0\) there exists a continuous family of non-constant periodic solutions \(x(t,\xi )\) for the above dynamic system, which collapses to the equilibrium point \(x*(\varepsilon_{0} )\) as \(\xi \to 0.\) The period of the cycle is close to \(2\pi /{\text{Im}} \lambda (\varepsilon_{0} ),\) where \({\text{Im}} \lambda (\varepsilon_{0} )\) is the imaginary part of \(\lambda (\varepsilon_{0} ).\)

Theorem 2

(A theorem that is useful for the analysis of Hopf bifurcation in three-dimensional dynamic system, cf. Asada (1995))

  1. (1)

    Suppose that the coefficients of the characteristic equation

    $$ \lambda^{3} + a_{1} \lambda^{2} + a_{2} \lambda + a_{3} = 0 $$
    (132)

    satisfies the following set of conditions.

    $$ a_{1} > 0,\;a_{3} > 0,\;a_{1} a_{2} - a_{3} = 0 $$
    (133)

    Then, Eq. (132) has a pair of pure imaginary roots and a negative real root.Footnote 23

  2. (2)

    Suppose that the coefficients in Eq. (132) are differentiable functions of a parameter \(\varepsilon ,\) namely,

    $$ a_{1} = a_{1} (\varepsilon ),\;a_{2} = a_{2} (\varepsilon ),\;a_{3} = a_{3} (\varepsilon ). $$
    (134)

Furthermore, suppose that a set of conditions

$$ a_{1} (\varepsilon_{0} ) > 0,\;a_{3} (\varepsilon_{0} ) > 0,\;a_{1} (\varepsilon_{0} )a_{2} (\varepsilon_{0} ) - a_{3} (\varepsilon_{0} ) = 0 $$
(135)

is satisfied at the parameter value \(\varepsilon = \varepsilon_{0} .\)Footnote 24 Theorem 2 (1) implies that the characteristic equation (132) has a pair of pure imaginary roots \(\lambda (\varepsilon_{0} ),\) \(\overline{\lambda }(\varepsilon_{0} )\) and a negative real root at the point \(\varepsilon = \varepsilon_{0} .\) Then, the condition

$$ \left. {\frac{{\partial \{ a_{1} (\varepsilon )a_{2} (\varepsilon ) - a_{3} (\varepsilon )\} }}{\partial \varepsilon }} \right|_{{\varepsilon = \varepsilon_{0} }} \ne 0 $$
(136)

is equivalent to the condition

$$ \left. {\frac{{\partial \{ {\text{Re}} (\lambda (\varepsilon )\} }}{\partial \varepsilon }} \right|_{{\varepsilon = \varepsilon_{0} }} \ne 0, $$
(137)

where \({\text{Re}} \lambda (\varepsilon )\) is the real part of \(\lambda (\varepsilon ).\)

Proof

See Asada (1995). \(\quad \square\)

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Asada, T. On the dynamic properties of Okishio’s Monetarist model. Evolut Inst Econ Rev 22, 229–264 (2025). https://doi.org/10.1007/s40844-024-00295-x

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