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A Two-Sector Growth Model with Credit Market Imperfections and Production Externalities

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Advances in Mathematical Economics

Part of the book series: Advances in Mathematical Economics ((MATHECON,volume 22))

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Abstract

A two-sector dynamic general equilibrium model with financial constraints and production externalities is studied. Agents face idiosyncratic productivity shocks in each period. Agents who draw high productivity borrow resources in the financial market and become capital producers, whereas agents who draw low productivity become lenders. We analyze how the interaction between the extent of financial constraints and sector-specific production externalities affects the characterization of equilibria in a two-sector economy.

JEL Classification: E32, E44, O41

Mathematics Subject Classification (2010): 37N40, 39A30

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Notes

  1. 1.

    In contrast to Woodford [24], Barinci and Chéron [5] consider an economy with increasing return-to-scale production externalities.

  2. 2.

    We do not assume any fixed cost that affects financial constraints.

  3. 3.

    See, for instance, Benhabib and Farmer [6, 7], Benhabib and Nishimura [8], Borldrin and Rustichini [11], Benhabib et al. [10], Nishimura and Shimomura [19], Nishimura and Venditti [20, 21], and Dufourt et al. [15].

  4. 4.

    This type of financial constraints is employed by many researchers such as Aghion et al. [2], Aghion and Banerjee [1], and Aghion et al. [3].

  5. 5.

    The derivation of an optimal portfolio allocation of savings follows Kunieda and Shibata [17]. Although agents who draw Φt = ϕ t are indifferent between initiating a capital production project and lending in the financial market, it is assumed that they lend their savings in the financial market.

  6. 6.

    To be accurate, c 0 is not subject to any history of the stochastic events and ω −1 is empty.

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Acknowledgements

The authors would like to express thanks to Toru Maruyama, who is an editor, for his comments. All remaining errors, if any, are ours. This work is financially supported by the Japan Society for the Promotion of Science, Grants-in-Aid for Scientific Research (Nos. 15H05729, 16H02026, 16H03598, 16K03685).

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Appendix

Appendix

1.1 Proof of Proposition 3.1

It follows from Lemma 3.1 that

$$\displaystyle \begin{aligned} \begin{array}{rcl} &\displaystyle &\displaystyle \int_{\Xi_t}\int_{\Omega^t}s_t(\omega^{t-1})dP^t(\omega^{t-1})dP(\omega_t) \\ &\displaystyle &\displaystyle \qquad \qquad \qquad -\frac{\mu}{1-\mu}\int_{\Omega\setminus \Xi_t}\int_{\Omega^t}s_t(\omega^{t-1})dP^t(\omega^{t-1})dP(\omega_t)=0. \\ {} \end{array} \end{aligned} $$
(34)

where Ξt = {ω t ∈ Ω| Φt(ω t) ≤ ϕ t}. (34) can be rewritten as

$$\displaystyle \begin{aligned} \begin{array}{rcl} &\displaystyle &\displaystyle \int_{\Omega^t}s_t(\omega^{t-1})dP^t(\omega^{t-1})\int_0^{\phi_t}dG(\Phi) \\ &\displaystyle &\displaystyle \qquad \qquad \qquad -\frac{\mu}{1-\mu}\int_{\Omega^t}s_t(\omega^{t-1})dP^t(\omega^{t-1})\int_{\phi_t}^\eta dG(\Phi)=0, \\ \end{array} \end{aligned} $$

which is computed as

$$\displaystyle \begin{aligned} \int_{\Omega^t}s_t(\omega^{t-1})dP^t(\omega^{t-1})\left[G(\phi_t)-\frac{\mu}{1-\mu}(1-G(\phi_t))\right]=0. \end{aligned}$$

Solving the last part, we obtain G(ϕ t) = μ. \(\square \)

1.2 Proof of Lemma 3.2

Because \(R_t(\omega _{t-1})=\max \{r_t, (q_t\Phi _{t-1}(\omega _{t-1})-r_t\mu )/(1-\mu )\}\), it follows that

$$\displaystyle \begin{aligned} \int_{\Omega^t}R_t(\omega_{t-1})s_{t-1}(\omega^{t-2})dP^t(\omega^{t-1})&=\int_{\Omega^t}\max\left\{r_t, \frac{q_t\Phi_{t-1}(\omega_{t-1})-r_t\mu}{1-\mu}\right\} \\ &\times s_{t-1}(\omega^{t-2})dP^t(\omega^{t-1})=:I_t \end{aligned} $$

Define Ξt−1 = {ω t−1 ∈ Ω| Φt−1(ω t−1) ≤ ϕ t−1}, as in the proof of Proposition 3.1. Because ϕ t−1 = r t∕q t, I t can be computed as follows:

$$\displaystyle \begin{aligned} I_t&=\int_{\Omega^{t-1}\times \Xi_{t-1}}r_ts_{t-1}(\omega^{t-2})dP^t(\omega^{t-1}) \notag \\ &+\int_{\Omega^{t-1}\times(\Omega\setminus \Xi_{t-1})}\frac{q_t\Phi_{t-1}(\omega_{t-1})-r_t\mu}{1-\mu}s_{t-1}(\omega^{t-2})dP^t(\omega^{t-1}) \notag \\ &=\int_{\Omega^{t-1}\times(\Omega\setminus \Xi_{t-1})}\frac{q_t\Phi_{t-1}(\omega_{t-1})}{1-\mu}s_{t-1}(\omega^{t-2})dP^t(\omega^{t-1}), {} \end{aligned} $$
(35)

where the second equality of (35) is obtained from Lemma 3.1. Agents who draw Φt−1(ω t−1) > ϕ t−1 invest x t−1(ω t−1) = s t−1(ω t−2)∕(1 − μ), and thus, (35) becomes

$$\displaystyle \begin{aligned} I_t&=\int_{\Omega^{t-1}\times(\Omega\setminus \Xi_{t-1})}\frac{q_t\Phi_{t-1}(\omega_{t-1})}{1-\mu}(1-\mu)x_{t-1}(\omega^{t-1})dP^t(\omega^{t-1}) \notag \\ &=q_t\int_{\Omega^{t-1}\times(\Omega\setminus \Xi_{t-1})}\Phi_{t-1}x_{t-1}(\omega^{t-1})dP^t(\omega^{t-1}). {} \end{aligned} $$
(36)

Because \(k_t=\int _{\Omega ^{t-1}\times (\Omega \setminus \Xi _{t-1})}\Phi _{t-1}x_{t-1}(\omega ^{t-1})dP^t(\omega ^{t-1})\), (36) becomes

$$\displaystyle \begin{aligned} I_t=q_tk_t.~~\square \end{aligned} $$

1.3 Proof of Lemma 3.3

By using Lemma 3.2 and because \(\int _{\Omega ^t}\pi _tdP^t(\omega ^{t-1})=\Pi _t\), the aggregation of (6) across all agents is obtained as follows:

$$\displaystyle \begin{aligned} \int_{\Omega^t}s_t(\omega^{t-1})dP^t(\omega^{t-1})&=\int_{\Omega^t}[R_t(\omega_{t-1})s_{t-1}(\omega^{t-2})+w_t+\pi_t \notag \\ &-p_tc_t(\omega^{t-1})]dP^t(\omega^{t-1}) \notag \\ &=q_tk_t+w_t+\Pi_t-p_tC_t. {} \end{aligned} $$
(37)

From (8), we have \(F^1(l_t^1, k_t^1)+p_tF^2(l_t^2, k_t^2)+(1-\delta )k_t=q_tk_t+w_t+\Pi _t\). Additionally, the consumption goods market-clearing condition leads to \(p_tF^2(l_t^2, k_t^2)=p_tC_t\). Therefore, (37) is transformed into

$$\displaystyle \begin{aligned} \int_{\Omega^t}s_t(\omega^{t-1})dP^t(\omega^{t-1})=F^1(l_t^1, k_t^1)+(1-\delta)k_t.~~~\square {} \end{aligned} $$
(38)

1.4 Proof of Proposition 3.2

Because k t+1 is produced by capital producers who draw an individual-specific productivity, Φt(ω t), that is greater than ϕ t, Lemma 3.3 and the i.i.d. assumption compute k t+1 as follows:

$$\displaystyle \begin{aligned} k_{t+1}&=\int_{\Omega^{t}\times (\Omega\setminus \Xi_t)}\Phi_t(\omega_t)x_t(\omega^t)dP^{t+1}(\omega^t) \notag \\ &=\int_{\Omega\setminus \Xi_t}\int_{\Omega^{t}}\Phi_t(\omega_t)\frac{s_t(\omega^{t-1})}{1-\mu}dP^t(\omega^{t-1})dP(\omega_t) \notag \\ &=\int_{\phi_t}^\eta\frac{\Phi_t(\omega_t)}{1-\mu}dG(\Phi)\int_{\Omega^{t}}s_t(\omega^{t-1})dP(\omega^{t-1}) \notag \\ &=\frac{H(\phi^*)}{1-\mu}(F^1(l_t^1,k_t^1)+(1-\delta)k_t), \notag \end{aligned} $$

where \(H(\phi ^*)=\int _{\phi ^*}^\eta \Phi _t(\omega _t) dG(\Phi )\) because ϕ t = ϕ ∗ in equilibrium. \(\square \).

1.5 Proof of Lemma 3.4

Obviously, M(μ) is continuous in [0, 1). The inverse function theorem implies

$$\displaystyle \begin{aligned} \frac{\partial M(\mu)}{\partial \mu}=\frac{\partial}{\partial \mu}\left(\frac{H(\phi^*)}{1-\mu}\right)&=\frac{-(1-\mu)\phi^*G^\prime(\phi^*)(\partial \phi^*/\partial \mu)+H(\phi^*)}{(1-\mu)^2} \notag \\ &=\frac{\int_{\phi^*}^h\Phi_t(\omega_t)dG(\Phi)-\phi^*(1-G(\phi^*))}{(1-\mu)^2}>0. \notag \end{aligned} $$

Therefore, M(μ) is an increasing function with respect to μ in [0, 1). It is straightforward to verify that M(0) = H(0) is the mean of the idiosyncratic productivity shocks. By applying L’Hôpital’s rule, we obtain limμ→1 M(μ) =limμ→1 G −1(μ)G −1 ′(μ)G ′(ϕ ∗) = η. For the last equality, we have used the inverse function theorem again. \(\square \)

1.6 Proof of Proposition 3.3

Because ϕ t = r t+1∕q(p t+1) and ϕ t = ϕ ∗, it follows that

To derive the last equality, Proposition 3.1 is applied. \(\square \)

1.7 Proof of Lemma 3.5

From Assumption 3.2, it follows that (1 − δ)M(μ) < 1. Then, under Assumption 3.3, from (12), (28), and (29), it follows that \(sign\{k^*-\alpha _K^1w(p^*)/(\alpha _L^1v(p^*))\}=sign\{1-(1-\delta )\beta M(\mu )-\alpha _K^1 \beta (1-(1-\delta )M(\mu ))\}\). Because \(1-(1-\delta )\beta M(\mu )-\alpha _K^1 \beta (1-(1-\delta )M(\mu ))>(1-\alpha _K^1\beta )(1-(1-\delta )M(\mu ))>0\), it follows that \(sign\{k^*-\alpha _K^1w(p^*)/(\alpha _L^1v(p^*))\}>0\). Additionally, it follows that \(sign\{\alpha _K^2w(p^*)/\\ (\alpha _L^2v(p^*))-k^*\}=sign\{1-(1-\delta )M(\mu )\}>0\). \(\square \)

1.8 Proof of Theorem 4.1

To prove Theorem 4.1, two lemmata are prepared.

Lemma A.1

Under Assumptions 2.1 , 3.2 , and 3.3 , it holds that 0 < κ 2 < 1.

Proof

It follows from Assumption 3.2 that 0 < (1 − δ)βM(μ) < 1, which leads to (θ 2 − θ 1)∕(θ 2 − θ 1(1 − δ)βM(μ)) < 1 from Assumptions 2.1, 3.2, and 3.3. Additionally, it follows from Assumption 3.3 that (θ 2 − θ 1)∕(θ 2 − θ 1(1 − δ)βM(μ)) > 0 □

Lemma A.2

Under Assumptions 2.1 , 3.2 , 3.3 , and 4.4 , suppose that the mean of the stochastic productivity shocks, M(0), is smaller than M 1 and that the maximum, η, is greater than M 2 . Then, as the value of μ increases from 0 to 1, the value of κ 1 increases in the ranges, as in the following.

  • As μ increases in [0, μ 1), κ 1 increases in \([\tilde {\kappa }, -1)\).

  • As μ increases in [μ 1, μ 2), κ 1 increases in [−1, 0).

  • As μ increases in [μ 2, 1), κ 1 increases in \([0, \bar {\kappa })\) ,

where \(\tilde {\kappa }:=[(\Delta +\alpha _L^2)(1-\delta )\beta M(0)-\alpha _L^2]/(\beta \Delta )\in (-\infty , -1)\) and \(\bar {\kappa }< 1-(1-\beta )\alpha _L^2/(\beta \Delta )\in (0, 1)\) , which is given when M(μ) = η.

Proof

M(μ) is an increasing function with respect to μ. Then, Fig. 2 and (32) prove the claims. □

Proof of Theorem 4.1

From Lemma A.1, we have |κ 2| < 1. From Lemma A.2, if μ ∈ [0, μ 1), |κ 1| > 1, and if μ ∈ (μ 1, 1), |κ 1| < 1. Therefore, the steady state is a saddle point if μ ∈ [0, μ 1), and the steady state is totally stable if μ ∈ (μ 1, 1). □

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Kunieda, T., Nishimura, K. (2018). A Two-Sector Growth Model with Credit Market Imperfections and Production Externalities. In: Kusuoka, S., Maruyama, T. (eds) Advances in Mathematical Economics. Advances in Mathematical Economics, vol 22. Springer, Singapore. https://doi.org/10.1007/978-981-13-0605-1_5

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