Chapter 16Monetary and Fiscal Theory

Introduction

Chapter 15 took monetary policy as a Taylor rule — a feedback function from inflation and the output gap to the interest rate. This chapter goes deeper. Why do people hold money? What determines the optimal quantity of money? Why do central banks consistently produce too much inflation (time inconsistency)? And how does fiscal policy interact with monetary policy through the government budget constraint?

The chapter's culmination is the Fiscal Theory of the Price Level (FTPL) — the radical claim that, under certain conditions, fiscal policy, not monetary policy, determines the price level.

By the end of this chapter, you will be able to:
  1. Model money demand using CIA and MIU approaches and derive the Friedman rule
  2. Explain time inconsistency and the inflation bias
  3. State and interpret Ricardian equivalence and its failures
  4. Derive the intertemporal government budget constraint
  5. Explain FTPL and distinguish Ricardian from non-Ricardian fiscal regimes
  6. Apply the Ramsey optimal taxation framework

16.1 Why Hold Money?

Cash-in-advance (CIA) constraint. A modeling assumption that consumption purchases require prior accumulation of money: $P_tc_t \leq M_t$. Money is valued not for direct utility but because it is a prerequisite for transactions. The CIA constraint generates money demand as a function of the nominal interest rate.
Money-in-utility (MIU). An alternative money-demand framework where real balances $m = M/P$ enter the utility function directly: $u(c, m)$. Real balances provide "liquidity services" that agents value. The optimal money holding equates the marginal utility of real balances to the opportunity cost $i$ (the nominal interest rate).

Cash-in-Advance (CIA)

The CIA constraint assumes agents must hold money to purchase consumption goods:

$$P_t c_t \leq M_t$$ (Eq. 16.1)

Money is valued because it is required for transactions. When the nominal interest rate $i > 0$, holding money has an opportunity cost (foregone interest), creating a wedge that distorts consumption decisions.

Money-in-Utility (MIU)

An alternative: money directly enters the utility function, capturing the liquidity services it provides:

$$\max \sum_{t=0}^\infty \beta^t u(c_t, M_t/P_t)$$ (Eq. 16.2)

The first-order condition equates the marginal utility of real balances to the opportunity cost of holding money:

$$\frac{u_m(c, m)}{u_c(c, m)} = i_t$$ (Eq. 16.3)

where $m = M/P$ is real balances and $i$ is the nominal interest rate.

The Friedman Rule

Friedman rule. The optimal monetary policy sets the nominal interest rate to zero ($i = 0$), eliminating the opportunity cost of holding money. Since producing money is virtually costless, efficiency requires its "price" (the nominal rate) to equal zero. This implies deflation at the rate of time preference: $\pi^* = -r$.
Superneutrality of money. The property that changes in the money growth rate have no effect on real variables (output, consumption, capital) in the long run. Superneutrality holds in some CIA and MIU models but fails when inflation distorts intertemporal margins (e.g., the Tobin effect on capital accumulation).

The marginal cost of producing money is essentially zero. Efficiency requires that the price of each good equal its marginal cost. The "price" of holding money — the opportunity cost — is the nominal interest rate $i$. Since the marginal cost of money is zero, the efficient price is $i = 0$.

Since the Fisher equation gives $i = r + \pi$, and the real rate $r$ is determined by fundamentals, the Friedman rule implies:

$$\pi^* = -r$$ (Eq. 16.4)

The optimal inflation rate is the negative of the real interest rate — the central bank should deflate at the rate of time preference, making the nominal rate zero and eliminating the distortion from money holding.

16.2 Time Inconsistency and the Inflation Bias

Time inconsistency. A situation where the optimal policy at time $t$ differs from what was planned at time $t-1$. In monetary policy, the central bank has an incentive to announce low inflation but then surprise agents with high inflation to boost output. Rational agents anticipate this, producing an equilibrium with higher inflation and no output gain.
Inflation bias. The excess inflation $\pi^* = bk/a$ that results from discretionary monetary policy in the Barro-Gordon model. The bias arises because the central bank wants output above the natural rate ($k > 0$), but rational agents see through the attempt, leaving only inflation as the outcome.
Central bank independence. Institutional arrangements that insulate monetary policy from political pressure. Rogoff (1985) showed that appointing a "conservative" central banker (one with higher inflation aversion $a$) reduces the inflation bias. Empirically, countries with more independent central banks have lower average inflation.
Rules vs discretion. The fundamental choice in monetary policy design. Rules (like an inflation target or Taylor rule) constrain the central bank but solve the time-inconsistency problem. Discretion allows flexible responses but creates the inflation bias. Modern central banking seeks a middle ground: "constrained discretion."

The Barro-Gordon Model

The central bank minimizes a loss function:

$$L = (y - y^* - k)^2 + a\pi^2$$ (Eq. 16.5)

where $y^*$ is natural output, $k > 0$ reflects the central bank's desire to push output above natural, and $a$ is the weight on inflation. An expectations-augmented Phillips curve links output and inflation:

$$y = y^* + b(\pi - \pi^e)$$ (Eq. 16.6)

Under commitment: The central bank announces $\pi = 0$ and sticks to it. The loss is $k^2$.

Under discretion: In rational expectations equilibrium ($\pi = \pi^e$), the inflation bias emerges:

$$\pi^* = \frac{bk}{a}$$ (Eq. 16.7)

The loss under discretion is $L_{disc} = k^2(1 + b^2/a)$ — strictly worse than commitment. The inflation bias is all cost and no benefit: output stays at $y^*$ under both regimes, but discretion adds gratuitous inflation.

Interactive: Barro-Gordon Inflation Bias

The inflation bias under discretion is $\pi^* = bk/a$. Adjust the central bank's preferences and the Phillips curve slope to see how the bias and losses change.

Flat (0.1)Steep (3.0)
None (0)High (0.10)
Dove (0.10)Hawk (3.00)
Inflation bias: π* = 0.040 (4.0%)  |  Loss (commitment): 0.000400  |  Loss (discretion): 0.001200  |  Cost of discretion: 0.000800

Figure 16.1. Loss under commitment vs. discretion. The gap is the cost of the central bank's inability to commit. A more conservative banker (higher $a$) shrinks the inflation bias. Drag sliders to explore.

Solutions to time inconsistency: (1) Central bank independence (Rogoff, 1985): appoint a "conservative central banker" with higher $a$. (2) Inflation targeting: explicit numerical commitment. (3) Reputation: in repeated interactions, the long-run credibility cost exceeds the short-run gain. (4) Performance contracts (Walsh, 1995): penalties for missing targets.

Example 16.1 — Deriving the Friedman Rule from the MIU Model

Consider utility $u(c, m) = \ln c + \gamma\ln m$ with budget constraint and Fisher equation $i = r + \pi$.

Step 1: FOC for real balances: $\gamma/m = i \cdot (1/c)$, so $m/c = \gamma/i$.

Step 2: Marginal utility of money: $u_m = \gamma/m$. Marginal utility of consumption: $u_c = 1/c$. Optimality: $u_m/u_c = \gamma c/m = i$.

Step 3: The social cost of producing money is zero. Efficiency requires $u_m/u_c = $ marginal cost $= 0$. Therefore $i^* = 0$.

Step 4: From Fisher equation: \$1 = r + \pi^*$, so $\pi^* = -r$. With $r = 4\%$: optimal inflation is $-4\%$/year (deflation). The central bank should shrink the money supply at the rate of time preference.

Example 16.2 — Barro-Gordon Inflation Bias Calculation

Parameters: Phillips curve slope $b = 0.5$, output ambition $k = 0.02$, inflation weight $a = 1.0$.

Step 1: Inflation bias under discretion: $\pi^* = bk/a = 0.5 \times 0.02 / 1.0 = 0.01$ (1% per year).

Step 2: Loss under commitment ($\pi = 0$): $L_c = k^2 = 0.0004$.

Step 3: Loss under discretion: $L_d = k^2(1 + b^2/a) = 0.0004(1 + 0.25) = 0.0005$.

Step 4: Cost of discretion: $L_d - L_c = 0.0001$. Society gets 1% gratuitous inflation with zero output benefit.

Step 5: If a "conservative banker" has $a = 4$: $\pi^* = 0.5 \times 0.02/4 = 0.0025$ (0.25%). The bias shrinks by 75%, justifying central bank independence.

Intertemporal government budget constraint. The requirement that the real value of government debt equals the present value of future primary surpluses: $B_0/P_0 = \sum R_t^{-1}s_t$. This constraint must hold in any equilibrium — the question is whether it is satisfied by fiscal adjustment (Ricardian regime) or price-level adjustment (FTPL).
Seigniorage. Revenue earned by the government from creating money. Real seigniorage is $S = \mu \cdot m(\mu)$, where $\mu$ is the money growth rate and $m(\mu)$ is real money demand. It is effectively an inflation tax on money holders.

16.3 The Government Budget Constraint

The government's flow budget constraint:

$$B_{t+1} = (1 + i_t)B_t + P_t(G_t - T_t) - (M_{t+1} - M_t)$$ (Eq. 16.8)

The intertemporal government budget constraint (IGBC) in real terms:

$$\frac{B_0}{P_0} = \sum_{t=0}^\infty R_t^{-1} s_t$$ (Eq. 16.9)

where $R_t = \prod_{j=0}^{t-1}(1+r_j)$ is the cumulative discount factor and $s_t = T_t - G_t$ is the primary surplus. Real government debt equals the present value of future primary surpluses.

16.4 Ricardian Equivalence

Ricardian equivalence. Barro's (1974) result that, under certain conditions (infinite horizons, lump-sum taxes, no liquidity constraints, perfect capital markets), the timing of taxes does not affect consumption, the real interest rate, or any real variable. A tax cut financed by borrowing is fully offset by increased private saving in anticipation of future taxes.
Liquidity-constrained households. Households that cannot borrow against future income and therefore spend any current windfall (including tax cuts). When a fraction of households are liquidity-constrained, Ricardian equivalence fails partially: a tax cut raises aggregate consumption by the constrained fraction times the tax cut.

When Ricardian Equivalence Fails

The theorem requires strong assumptions. Key failures: (1) Finite horizons / OLG: current generation benefits, future generation pays. (2) Liquidity constraints: credit-constrained households spend windfall tax cuts. (3) Distortionary taxes: timing of income taxes changes relative incentives. (4) Uncertainty about future fiscal policy. (5) Behavioral biases: present-biased agents overconsume windfalls.

Empirically, about 20–40% of U.S. households appear liquidity-constrained (Zeldes, 1989). Tax rebates increase spending by about 20–40% of the rebate amount — inconsistent with full Ricardian equivalence.

Interactive: Ricardian Equivalence Test

What fraction of households are liquidity-constrained? At 0%, full Ricardian equivalence holds and a tax cut has zero effect on consumption. At 100%, the full tax cut is spent (pure Keynesian). The real world is somewhere in between.

0% (Ricardian)100% (Keynesian)
Tax cut = \$100B  |  Consumption increase: \$10.0B (30.0% of tax cut)  |  Saving increase: \$10.0B

Figure 16.2. Consumption response to a \$100B tax cut as a function of the fraction of constrained households. At 0% constrained, agents fully internalize future taxes and save the entire cut (Ricardian equivalence). At 100%, the full cut is spent. Empirical estimates (gray band) suggest 20–40% of households are constrained. Drag the slider to explore.

Example 16.3 — Ricardian Equivalence Test

A government cuts lump-sum taxes by \$100B, financed by issuing bonds. Assume $r = 3\%$ and taxes will increase by \$103B$ next year.

Under Ricardian equivalence: Households receive \$100B today but know they owe \$103B next year (PV = \$100B). They save the entire \$100B. Consumption unchanged: $\Delta C = 0$. Bond market absorbs \$100B in new debt with no change in interest rates.

With 40% liquidity-constrained households: Unconstrained (60%) save the full tax cut. Constrained (40%) spend it all. $\Delta C = 0.4 \times 100B = 40B$. The fiscal multiplier is 0.4, not zero.

Empirical evidence: Johnson, Parker, and Souleles (2006) found that U.S. households spent 20–40% of the 2001 tax rebates within the first quarter, consistent with partial Ricardian equivalence failure.

Fiscal theory of the price level (FTPL). The theory (Leeper 1991, Sims 1994, Cochrane 2001) that, when fiscal policy is "active" (surpluses do not adjust to satisfy the IGBC at the current price level), the price level must adjust to make real debt equal the present value of surpluses: $P_0 = B_0/\sum R_t^{-1}s_t$.
Ricardian regime (passive fiscal / active monetary). A policy configuration where fiscal policy passively adjusts primary surpluses to stabilize debt, while monetary policy actively controls inflation via the Taylor rule ($\phi_\pi > 1$). This is the standard NK setup.
Non-Ricardian regime (active fiscal / passive monetary). A policy configuration where fiscal surpluses are set independently of debt, and the price level adjusts to satisfy the IGBC. Monetary policy is passive ($\phi_\pi < 1$). Inflation becomes a fiscal phenomenon.

16.5 Fiscal Theory of the Price Level (FTPL)

Ricardian vs. Non-Ricardian Regimes

From Eq. 16.9, the IGBC must always hold. In the Ricardian regime, fiscal policy adjusts surpluses to satisfy the IGBC at whatever price level the central bank determines. In the non-Ricardian regime, surpluses are set independently, and the price level adjusts:

$$P_0 = \frac{B_0}{\sum_{t=0}^\infty R_t^{-1} s_t}$$ (Eq. 16.10)

If the government increases debt ($B_0$) without adjusting future surpluses, the price level $P_0$ must rise. Inflation is a fiscal phenomenon, not a monetary one.

Monetary policyFiscal policyOutcome
Active ($\phi_\pi > 1$)Passive (adjusts surpluses)Standard NK: monetary policy determines $\pi$
Passive ($\phi_\pi < 1$)Active (fixed surpluses)FTPL: fiscal policy determines $P$
ActiveActiveNo equilibrium (over-determined)
PassivePassiveIndeterminate (under-determined)

Interactive: FTPL Price Determination

In a non-Ricardian regime, $P = B / PV(\text{surpluses})$. Watch how the price level responds to changes in nominal debt or expected fiscal surpluses.

Low (10)High (300)
Low (10)High (300)
Price level: P = B / PV = 100 / 100 = 1.00  |  Inflation from baseline: 0.0%

Figure 16.3. FTPL price determination. The price level adjusts to equate real government debt with the present value of surpluses. Increasing debt without increasing surpluses causes inflation. Decreasing expected surpluses without reducing debt also causes inflation. Drag the sliders to explore fiscal dominance.

Example 16.4 — FTPL Price Level from Fiscal Surplus Path

A government has nominal debt $B_0 = 100$ and announces a new fiscal plan.

Scenario A (credible surpluses): Primary surpluses of 5 per year forever, $r = 5\%$. $PV(s) = 5/0.05 = 100$. Price level: $P_0 = 100/100 = 1.00$. No inflation.

Scenario B (lower surpluses): Surpluses fall to 4 per year. $PV(s) = 4/0.05 = 80$. Price level: $P_0 = 100/80 = 1.25$. Inflation: 25%.

Scenario C (war or crisis): Government doubles debt to $B_0 = 200$ with unchanged surpluses ($PV = 100$). $P_0 = 200/100 = 2.00$. Inflation: 100%.

Key insight: Under FTPL, inflation is determined by the gap between government liabilities and the present value of surpluses — independent of money supply growth. The central bank's inflation target is overridden by fiscal dominance.

16.6 Seigniorage

Seigniorage — the revenue from printing money — is an inflation tax on money holders. Real seigniorage is:

$$S = \mu \cdot m(\mu)$$ (Eq. 16.12)

where $\mu$ is the money growth rate and $m(\mu)$ is real money demand (decreasing in $\mu$). At low inflation, higher $\mu$ raises revenue. But at high inflation, the tax base ($m$) erodes faster than the rate rises — a seigniorage Laffer curve.

Interactive: Seigniorage Laffer Curve

Real money demand falls exponentially with inflation: $m(\mu) = m_0 \cdot e^{-\alpha \mu}$. Seigniorage revenue $S = \mu \cdot m(\mu)$ is an inverted U. Push inflation too high and you destroy the tax base.

0%100%200%
Money growth: 10%  |  Real money demand: 90.5  |  Seigniorage: 9.05  |  Peak at: μ = 100%

Figure 16.4. The seigniorage Laffer curve. Revenue first rises with inflation, then falls as the real money base is destroyed. Hyperinflation economies (Zimbabwe, Venezuela) operate on the right side of the curve — high inflation, low revenue. Drag the slider to explore.

Ramsey optimal taxation. The problem of choosing tax rates on commodities to raise a given revenue while minimizing total deadweight loss. The solution, the inverse elasticity rule, prescribes higher tax rates on goods with lower demand elasticity, because taxing inelastic goods causes less behavioral distortion.
Inverse elasticity rule. The Ramsey rule $\tau_i/\tau_j = \varepsilon_j/\varepsilon_i$: optimal tax rates are inversely proportional to demand elasticities. Tax inelastic goods more (e.g., food, medicine) and elastic goods less (e.g., luxury goods). This minimizes aggregate DWL but may conflict with equity goals.

16.7 Ramsey Optimal Taxation

How should the government structure taxes to minimize distortions? Ramsey's rule (1927): among commodities, tax those with inelastic demand more heavily (the inverse elasticity rule):

$$\frac{\tau_i}{\tau_j} = \frac{\varepsilon_j}{\varepsilon_i}$$ (Eq. 16.11)

Taxes on inelastic goods cause less behavioral distortion (less DWL, recall Chapter 3). The Ramsey rule minimizes total DWL for a given revenue requirement.

Interactive: Ramsey Optimal Tax

Two goods with different demand elasticities. The inverse elasticity rule says tax the inelastic good more. Compare Ramsey optimal rates to a uniform tax — same revenue, less deadweight loss.

Inelastic (0.10)Elastic (3.00)
Inelastic (0.10)Elastic (3.00)
Ramsey rates: τ1 = 30.0%, τ2 = 10.0%  |  Uniform rate: 20.0%  |  DWL (Ramsey): 5.00  |  DWL (Uniform): 6.00  |  Savings: 16.7%

Figure 16.5. Ramsey optimal tax rates vs. uniform taxation. The Ramsey rule assigns higher tax rates to the more inelastic good, reducing total DWL while raising the same revenue. The further apart the elasticities, the larger the efficiency gain. Drag sliders to change elasticities.

16.8 Fiscal Multipliers

Normal times ($\phi_\pi > 1$): Fiscal multiplier $\approx 0.5$–\$1.0$. Government spending raises aggregate demand, but the central bank raises rates, crowding out investment.

Zero lower bound ($i = 0$): Fiscal multiplier $> 1$, possibly \$1.5$–\$1.0$. The central bank cannot raise rates, so there is no crowding out. Fiscal policy is more effective precisely when it is most needed (Christiano, Eichenbaum & Rebelo, 2011; Woodford, 2011).

Example 16.5 — Ramsey Optimal Tax for Two Goods

Two goods with elasticities $|\varepsilon_1| = 0.5$ (inelastic, e.g., food) and $|\varepsilon_2| = 2.0$ (elastic, e.g., electronics). Revenue target: $R = 400$.

Step 1: Inverse elasticity rule: $\tau_1/\tau_2 = \varepsilon_2/\varepsilon_1 = 2.0/0.5 = 4$. The inelastic good should be taxed 4x more heavily.

Step 2: Revenue constraint: $\tau_1 Q_1 P_1 + \tau_2 Q_2 P_2 = 400$. With base $Q_0 = 100$, $P_0 = 10$, and demand $Q_i \approx Q_0(1 - \varepsilon_i\tau_i)$:

With $\tau_1 = 4\tau_2$: solve numerically to find $\tau_2 \approx 8.3\%$ and $\tau_1 \approx 33.2\%$.

Step 3: DWL comparison. Ramsey: $DWL = 0.5 \times 0.5 \times 0.332^2 \times 1000 + 0.5 \times 2.0 \times 0.083^2 \times 1000 = 27.6 + 6.9 = 34.5$.

Uniform tax ($\tau_1 = \tau_2 = 0.20$): $DWL = 0.5 \times 0.5 \times 0.04 \times 1000 + 0.5 \times 2.0 \times 0.04 \times 1000 = 10 + 40 = 50$.

Result: Ramsey reduces DWL by 31% relative to uniform taxation. The efficiency gain comes from concentrating the tax burden on the less responsive good.

The Historical Lens

Zimbabwe hyperinflation and Japan's lost decades: Two extremes of monetary-fiscal interaction.

Zimbabwe (2007–2008): Peak inflation reached approximately 79.6 billion percent per month in November 2008. The government financed massive fiscal deficits (land reform, military spending) by printing money. As inflation accelerated, the real money base collapsed — the economy moved to the wrong side of the seigniorage Laffer curve. The Zimbabwe dollar became worthless; transactions shifted to U.S. dollars and South African rand. This is the textbook case of fiscal dominance: the central bank was subservient to fiscal needs, and the FTPL equation $P = B/PV(s)$ played out with $PV(s) \to 0$.

Japan (1990s–present): The opposite extreme. Government debt exceeded 250% of GDP, yet inflation remained near zero or negative for decades. The Bank of Japan cut rates to zero in 1999 and implemented massive quantitative easing. Neither fiscal nor monetary expansion produced inflation. Possible explanations: (1) Japanese fiscal surpluses are expected to eventually adjust (Ricardian regime despite high debt). (2) The deflationary equilibrium is self-fulfilling — agents expect zero inflation, which validates itself at the ZLB. (3) Demographic decline reduces the natural rate permanently below zero.

The lesson: Zimbabwe and Japan bracket the spectrum of monetary-fiscal regimes. Zimbabwe shows what happens when fiscal policy dominates and surpluses collapse. Japan shows that even enormous debt need not produce inflation if fiscal credibility is maintained — but also that escaping deflationary equilibria is extraordinarily difficult.

Thread: The Kaelani Republic

Kaelani's government has debt of 85% of GDP. The central bank follows a Taylor rule with $\phi_\pi = 1.5$ (active monetary policy), and the government has announced primary surpluses of 2% of GDP for 15 years.

If the government delivers: Ricardian regime. If surpluses fall short: $P_0 = B_0 / PV(surpluses)$. If surpluses drop from 8.5B KD to 6B KD in PV, prices must rise by \$1.5/6 = 42\%$ — fiscal dominance overrides the inflation target.

About 40% of Kaelani's households are liquidity-constrained, so a tax cut has a positive (but partial) effect on aggregate demand — Ricardian equivalence fails for them.

Summary

Key Equations

LabelEquationDescription
Eq. 16.1$P_tc_t \leq M_t$CIA constraint
Eq. 16.4$\pi^* = -r$Friedman rule
Eq. 16.7$\pi^* = bk/a$Inflation bias under discretion
Eq. 16.9$B_0/P_0 = \sum R_t^{-1}s_t$Intertemporal GBC
Eq. 16.10$P_0 = B_0 / \sum R_t^{-1}s_t$FTPL price determination
Eq. 16.11$\tau_i/\tau_j = \varepsilon_j/\varepsilon_i$Ramsey inverse elasticity rule

Exercises

Practice

  1. In the MIU model, utility is $u(c, m) = \ln c + \gamma \ln m$. The nominal interest rate is $i = 0.05$. Derive the optimal ratio $m/c$. What happens to real balances as $i \to 0$?
  2. In the Barro-Gordon model with $b = 1$, $k = 0.02$, $a = 0.5$: (a) compute the inflation bias under discretion, (b) compute the loss under discretion vs. commitment, (c) how much does society gain from a more conservative central banker with $a = 2$?
  3. A government has real debt $B/P = 100$. Primary surpluses are expected to be 5 per year forever. The real interest rate is $r = 3\%$. (a) What is the PV of surpluses? (b) Does the IGBC hold? (c) If surpluses fall to 2 per year, what must happen to the price level under FTPL?

Apply

  1. The Friedman rule says $i = 0$ is optimal. Japan has had near-zero interest rates for decades. Is Japan implementing the Friedman rule? What other considerations might explain why most central banks target positive nominal rates?
  2. A government cuts taxes by \$100B and finances it by issuing bonds. Analyze the effect on aggregate demand under: (a) full Ricardian equivalence, (b) 50% liquidity-constrained households, (c) the ZLB. In which case is the fiscal multiplier largest?
  3. Using the Leeper taxonomy, classify the current U.S. policy regime. What would it take for the regime to switch from Ricardian to non-Ricardian?

Challenge

  1. Derive the Friedman rule from the MIU model. Show that the optimal nominal rate is zero and that this requires deflation at rate $\rho$.
  2. Prove Ricardian equivalence formally in an infinite-horizon model with lump-sum taxes. Identify the step that fails with finite horizons.
  3. In a Ramsey problem with two goods and linear demand $Q_i = a_i - b_iP_i$, derive the optimal tax rates and verify the inverse elasticity rule.