Appendix 1: After the Climate Shift
First note that the optimal choice of fossil fuel E and renewable energy R is made at each point in time, without affecting the dynamics of the problem. Therefore, we can simplify the problem by defining the maximum level of output Y net of input costs and capital depreciation:
$$ Y(K,\pi ) \equiv \mathop {\text{Max}}\limits_{E,R} \;\left[ {(1 - \pi )AF(K,E,R) - dE - cR - \delta K} \right]. $$
(A1)
For brevity, we suppress the arguments A, c and d in the maximal net output function, but note that energy use is given by \( E^{A} = - Y_{d} > 0 \) and \( R^{A} = - Y_{c} > 0, \) where the after-calamity values are denoted with superscript A. Energy use increases with the capital stock K and decreases in the size of the disaster π and the own price, so that \( Y_{iK} < 0 \) and \( Y_{i\pi } > 0,\;i = d,c. \)
The Hamilton–Jacobi–Bellman (HJB) equation in the value function VA is
$$ \rho V^{A} (K,\pi ) = \mathop {\text{Max}}\limits_{C} \;\left[ {U(C) + V_{K}^{A} (K,\pi )\left\{ {Y(K,\pi ) - C} \right\}} \right]. $$
(A2)
Optimality requires \( U'(C^{A} ) = V_{K}^{A} (K,\pi ), \) which gives the policy rule \( C^{A} (K,\pi ). \)
Differentiating (A2) with respect to K, using this optimality condition and a CRRA utility function U, yields a differential equation for consumption after the regime shift CA as a function of K:
$$ \left[ {Y(K,\pi ) - C^{A} (K,\pi )} \right]C_{K}^{A} (K,\pi ) = \sigma \left[ {Y_{K} (K,\pi ) - \rho } \right]C^{A} (K,\pi ), $$
(A3)
where \( \sigma \equiv - U^{\prime } /CU^{{\prime \prime }} > 0 \) is the elasticity of intertemporal substitution. Both relative risk aversion and relative intergenerational inequality aversion are equal 1/σ. Equation (A3) can be written as a saddle-point system of differential equations in C and K as functions of time corresponding to the Keynes–Ramsey rule and the capital dynamics:
$$ \begin{aligned} \dot{C}^{A} (t) & = \sigma \left[ {Y_{K} \left( {K(t),\pi } \right) - \rho } \right]C^{A} (t), \\ \dot{K}(t) & = Y\left( {K(t),\pi } \right) - C^{A} (t),\quad K(T) = K_{T} . \\ \end{aligned} $$
(A4)
The steady-state capital stock \( K^{A*} (\pi ) \) follows from the modified golden rule of capital accumulation \( Y_{K} (K^{A*} ,\pi ) = \rho , \) and is low if the disaster is large and the discount rate is high. As far as the transient phase is concerned, the capital stock is predetermined at time T, but consumption jumps up or jumps down to place the economy on the stable manifold, \( C^{A} (T + ) = C^{A} \left( {K(T + ),\pi } \right)\). It depends on the parameter values whether the consumption jumps up or jumps down. For reasonable parameter values, as in the calibration in this paper, consumption jumps down. Rearranging (A2) gives the value function:
$$ V^{A} (K,\pi ) = \frac{{U\left( {C^{A} (K,\pi )} \right) + U'\left( {C^{A} (K,\pi )} \right)\left[ {Y(K,\pi ) - C^{A} (K,\pi )} \right]}}{\rho }. $$
(A5)
The optimal path along the stable manifold is \( C^{A} (t) = C^{A} \left( {K(t),\pi } \right),\;t \ge T. \) In the sequel of the paper we use the log-linear approximation
$$ C^{A} = C^{A} (K,\pi ) \cong Y\left( {K^{{A^{*} }} (\pi ),\pi } \right)\left( {\frac{K}{{K^{{A^{*} }} (\pi )}}} \right)^{\phi } ,\quad \phi \equiv z\frac{{K^{{A^{*} }} (\pi )}}{{Y\left( {K^{{A^{*} }} (\pi ),\pi } \right)}} > 0, $$
(A6)
where the direction of the stable manifold, \( z \equiv C_{K}^{A} (K^{{A^{*} }} ,\pi ) \), is derived from (A3) with l’Hôpital’s rule:
$$ C_{K}^{A} (K^{{A^{*} }} ,\pi ) = \mathop {\lim }\limits_{{K \to K^{{A^{*} }} }} \frac{{\sigma \left[ {Y_{K} (K,\pi ) - \rho } \right]C_{K}^{A} (K,\pi ) + \sigma Y_{KK} (K,\pi )C^{A} (K,\pi )}}{{Y_{K} (K,\pi ) - C_{K}^{A} (K,\pi )}}. $$
(A7)
This yields the quadratic \( z^{2} - \rho z + \sigma Y_{KK} (K^{{A^{*} }} ,\pi )C^{{A^{*} }} = 0. \) The positive solution yields the slope \( z = \frac{\rho }{2} + \frac{1}{2}\sqrt {\rho^{2} - 4\sigma Y_{KK} (K^{{A^{*} }} ,\pi )C^{{A^{*} }} } > \rho > 0 \) of the stable manifold in the steady state. Although we could solve the after-calamity problem by using value function iteration to solve the HJB equation, the approximation (A6) is accurate and convenient.
Appendix 2: Before the Climate Shift
Again we define \( Y^{B} (.) \) as the maximum level of output net of total input costs and capital depreciation:
$$ Y^{B} (K,\tau ) \equiv \mathop {\text{Max}}\limits_{E,R} \;\left[ {AF(K,E,R) - (d + \tau )E - cR - \delta K} \right], $$
(A.8)
so that the efficiency conditions for energy use are \( AF_{E} = d + \tau \) and AFR = c. The cost of fossil fuel is thus augmented with the social cost of carbon. If carbon is taxed at the social cost of carbon, this condition for the social optimum is replicated in the market.
Differentiating (6) with respect to K and P, using (7), gives the Pontryagin conditions:
$$ \begin{aligned} - \dot{V}_{K}^{B} & = \left[ {Y_{K}^{B} (K,\tau ) - \rho - H(P)} \right]V_{K}^{B} + H(P)V_{K}^{A} (K), \\ \dot{V}_{P}^{B} & = \left[ {\rho + \gamma + H(P)} \right]V_{P}^{B} + H^{\prime}(P)\left[ {V^{B} (K,P) - V^{A} (K)} \right]. \\ \end{aligned} $$
(A.9)
Using (8) and (A.9) yields the differential Eq. (9) for the price of carbon τ. Using (A.9), (7), and a CRRA utility function U with elasticity of intertemporal substitution σ, yields the modified Keynes–Ramsey rule (10).
The accumulation of capital and the stock of carbon can be written as
$$ \begin{aligned} & \dot{K} = Y^{B} (K,\tau ) - \tau Y_{\tau }^{B} (K,\tau ) - C^{B} ,\quad K(0) = K_{0} , \\ & \dot{P} = - \psi Y_{\tau }^{B} (K,\tau ) - \gamma P,\quad P(0) = P_{0} . \\ \end{aligned} $$
(A.10)
The capital dynamics include lump-sum rebates of carbon taxes in a market economy.
The steady state of the 4-dimensional Hamiltonian system (9), (10) and (A.10) is indicated with an asterisk and follows from the modified golden rule of capital accumulation \( Y_{K}^{B} (K^{B*} ,\tau^{B*} ) = \rho - \theta^{B*} \), leading to the precautionary return on capital adjustments \( \theta^{B*} = H(P^{B*} )\left[ {\frac{{V_{K}^{A} (K^{B*} )}}{{U'(C^{B*} )}} - 1} \right], \) the carbon tax
$$ \tau^{B*} = \frac{{\psi H^{\prime}(P^{B*} )\left[ {V^{B} (K^{B*} ,P^{B*} ) - V^{A} (K^{B*} )} \right]}}{{\left[ {\rho + \gamma + H(P^{B*} )} \right]U'(C^{B*} )}} = \frac{{\psi H^{\prime}(P^{B*} )\left[ {U(C^{B*} ) - \rho V^{A} (K^{B*} )} \right]}}{{\left[ {\rho + H(P^{B*} )} \right]\left[ {\rho + \gamma + H(P^{B*} )} \right]U'(C^{B*} )}}, $$
the rate of consumption \( C^{B*} = Y^{B} (K^{B*} ,\tau^{B*} ) - \tau^{B*} Y_{\tau }^{B} (K^{{B^{*} }} ,\tau^{B*} ) \) and the carbon stock \( P^{B*} = - \psi Y_{\tau }^{B} (K^{B*} ,\tau^{B*} )/\gamma \). This gives a target steady state as after the regime shift the system moves to the after-calamity steady state \( K^{A*} . \)
Appendix 3: Calibration
We use a utility function U with constant elasticity of intertemporal substitution σ = 0.5 (and 0.8 in a sensitivity test) and a pure rate of time preference ρ = 0.014. Our parameters and initial values are calibrated to figures for the world economy for the year 2010. Data sources are the BP Statistical Review and the World Bank Development Indicators. Output is AF before and (1–π)AF after the disaster, the Cobb–Douglas production function is \( F(K,E,R) = K^{\alpha } (E^{\omega } R^{(1 - \omega )} )^{\beta } \) with share of capital in value added α = 0.3, share of fossil fuel in energy ω = 0.9614 and share of energy in value added β = 0.0651. The share of fossil fuel and labour in value added are thus βω = 0.0626 and 1 – α – β = 0.6349. We use a depreciation rate for manmade capital of δ = 0.05. Total factor productivity is set to A = 11.9762, so that initial world GDP equals Y0 = 63 trillion US $. The corresponding initial value of the aggregate capital stock is K0 = 200 trillion US $, initial fossil use is E0 = 468.3 million GBTU or 8.3 GtC, and initial renewable energy use is R0 = 9.4 million GBTU. The calibrated production share parameters are compatible with a cost of fossil fuel of d = 9 US $/million BTU or 504 US $/tC and a cost of renewable energy of c = 18 US $/million BTU. For the carbon cycle we have an initial stock of carbon of P0 = 826 GtC or 338 ppm by volume CO2, a rate of decay γ = 0.003, a fraction of carbon staying up in the atmosphere of ψ = 0.5, and an equilibrium climate sensitivity χ = 3 (or 4 in a sensitivity run). The catastrophic shock to total factor productivity is π = 0.2 (or 0.1 in a sensitivity run).
Appendix 4: Proof of Proposition 1
\( V^{A} (K,P,\pi ) \) requires \( \tau^{A} (K,P,\pi ) \equiv - \psi V_{P}^{A} (K,P,\pi )/U'(C) > 0 \) to internalise gradual damages. After-calamity consumption CA(K, P, π) yields
$$ V^{A} (K,P,\pi ) = U\left( {C^{A} (K,P,\pi )} \right)/\rho + U^{\prime } \left( {C^{A} (K,P,\pi )} \right)\left[ {Y^{A} (K,P,\pi ) - C^{A} (K,P,\pi ) + \gamma \tau^{A} (K,P,\pi )P/\psi } \right]/\rho . $$
(A.11)
As a consequence, the second parts of (A.9) and (9) become:
$$ \dot{V}_{P}^{B} = \left[ {\rho + \gamma + H(P)} \right]V_{P}^{B} + H^{\prime}(P)(V^{B} - V^{A} ) - A'FV_{K}^{B} - H(P)V_{P}^{A} , $$
(A.12)
$$ \dot{\tau } = \left[ {Y_{K}^{B} (K,\tau ) + \gamma + H(P) + \theta } \right]\tau - \frac{\psi }{{U'(C^{B} )}}\left[ {H^{\prime}(P)(V^{B} - V^{A} ) - A'FV_{K}^{B} - H(P)V_{P}^{A} } \right]. $$
(A.13)
Integrating (A.13), we get (13). The target before-calamity steady-state carbon tax is
$$ \tau^{B*} = \tau_{\text{conventional}}^{B*} + \tau_{\text{risk-averting}}^{B*} + \tau_{\text{raising-the-stakes}}^{B*} ,\quad {\text{where}}\quad \tau_{\text{conventional}}^{B*} \equiv \frac{{\xi \psi A(P^{B*} )F(K^{B*} ,\tau^{B*} )}}{{\rho + \gamma + H(P^{B*} )}}, $$
$$ \tau_{\text{risk-averting}}^{B*} \equiv \frac{{\psi H^{\prime}(P^{B*} )\left[ {U(C^{B*} ) - \rho V^{A} (K^{B*} ,P^{B*} )} \right]}}{{\left[ {\rho + \gamma + H(P^{B*} )} \right]\left[ {\rho + H(P^{B*} )} \right]U'(C^{B*} )}}, $$
$$ \tau_{\text{raising-the-stakes}}^{B*} \equiv \frac{{H(P^{B*} )\tau^{A} (K^{B*} ,P^{B*} )U'\left( {C^{A} (K^{B*} ,P^{B*} )} \right)}}{{\left[ {\rho + \gamma + H(P^{B*} )} \right]U'(C^{B*} )}}, $$
and A(P)F(K,τ) is the maximum level of gross output.
Appendix 5: Carbon Catastrophes
Our damages and χ = 3 imply \( A\left( {Temp} \right) = \bar{A}\exp \left[ { - \xi \left( {2^{Temp/3} P_{PI} - \bar{P}} \right)} \right]. \) A catastrophic increase in the climate sensitivity (CS) to χ > 4 raises the temperature response and thus increases after-calamity damages as can be seen from substituting the temperature response: \( A(P) = \bar{A}\exp \left[ { - \xi \left( {\left( {P/P_{PI} } \right)^{{\frac{\chi }{3}}} P_{PI} - \bar{P}} \right)} \right]. \) The catastrophic rise in χ pushes up damages (\( A^{\prime } (P) = - \xi (\chi /3)\left( {P/P_{PI} } \right)^{(\chi - 3)/3} A(P) < - \xi A(P) < 0 \)).
Figure 3 indicates that a bigger climate sensitivity of 4 (the dashed line) than our benchmark of 3 (the solid line) leads, for a given carbon stock, to bigger damages, with the hazard function unaltered. A sudden increase in climate sensitivity thus leads to a tougher challenge. Doubling the initial carbon stock induces a 2.0% drop in total factor productivity if climate sensitivity is 3 and a 3.4% drop if the climate sensitivity is 4.