The Taylor principle and determinacy

@econcortex

2026-09-22

The most important number in The Taylor rule is not 2 percent for r*r^* but the total response of the nominal rate to inflation. Woodford gave the requirement its name: the Taylor principle says the nominal rate must rise by more than one for one with inflation, so that the real rate rises when inflation rises (Woodford, 2001). This lesson shows where the requirement comes from.

The three-equation model

The workhorse New Keynesian model has three log-linear equations (Clarida et al., 1999; Galı́, 2015). Variables are deviations from steady state; xtx_t is the output gap, πt\pi_t inflation, iti_t the nominal rate and rtnr^n_t the natural real rate, which moves with shocks.

xt=𝔼txt+1−1σ(it−𝔼tπt+1−rtn)\begin{equation} x_t = \mathbb{E}_t x_{t+1} - \frac{1}{\sigma}\left(i_t - \mathbb{E}_t \pi_{t+1} - r^n_t\right) \label{eq:is} \end{equation}

The three-equation model (cont.)

πt=β𝔼tπt+1+κxt\begin{equation} \pi_t = \beta\, \mathbb{E}_t \pi_{t+1} + \kappa\, x_t \label{eq:pc} \end{equation}

it=ϕππt+ϕxxt\begin{equation} i_t = \phi_\pi \pi_t + \phi_x x_t \label{eq:rule} \end{equation}

The three-equation model (cont.)

Equation is the dynamic IS curve: demand today depends on expected demand tomorrow and on the gap between the real rate and its natural level. Equation is the New Keynesian Phillips curve with slope κ\kappa and discount factor β\beta. Equation is a Taylor-type rule without the constants, which drop out in deviations.

Why “more than one” matters

Consider a self-fulfilling burst of inflation expectations with no change in fundamentals. Higher expected inflation lowers the real rate in unless the central bank raises iti_t enough. A higher gap raises inflation through , which confirms the expectation. If instead the rule raises the nominal rate by more than the increase in inflation, the real rate rises, the gap falls, inflation falls, and the expectation is refuted. The Taylor principle is what makes sunspot expectations fail.

Why “more than one” matters (cont.)

Theorem (Determinacy condition)

The system – has a unique bounded rational-expectations equilibrium if and only if κ(ϕπ−1)+(1−β)ϕx>0.\begin{equation} \kappa\,(\phi_\pi - 1) + (1 - \beta)\,\phi_x > 0. \label{eq:det} \end{equation} With ϕx=0\phi_x = 0 this reduces to ϕπ>1\phi_\pi > 1, the Taylor principle in its simplest form. A positive response to the output gap relaxes the requirement on ϕπ\phi_\pi slightly, because 1−β1 - \beta is small (Bullard & Mitra, 2002; Woodford, 2003).

Why “more than one” matters (cont.)

The proof works by writing the system as 𝔼tzt+1=Azt\mathbb{E}_t z_{t+1} = A z_t with zt=(xt,πt)′z_t = (x_t, \pi_t)' and checking that both eigenvalues of AA lie outside the unit circle, which is the Blanchard–Kahn condition for two non-predetermined variables. Galí works through the algebra in chapter 4 of his textbook (Galı́, 2015); the condition in is his equation for the contemporaneous rule.

Why “more than one” matters (cont.)

Example (The Taylor coefficients)

With Taylor’s values the total inflation response is ϕπ=1.5\phi_\pi = 1.5 and the gap response ϕx=0.5\phi_x = 0.5 (per year, so 0.1250.125 per quarter in quarterly models). Any plausible κ\kappa and β\beta satisfy with room to spare.

Evidence

Clarida, Galí and Gertler estimated a forward-looking version of the rule for the United States and found that the inflation response was below one in the pre-Volcker period and well above one after 1979 (Clarida et al., 2000). Their reading: before 1979 policy accommodated inflation and left the door open to self-fulfilling fluctuations, afterwards it did not. Their baseline estimates put the response at roughly 0.8 before and roughly 2.2 after; the exact numbers vary with the specification, the sign of the difference does not.

Evidence (cont.)

The interpretation is contested. Real-time data and the Taylor rule shows that with the data the Fed actually saw at the time, the 1970s look less like a failure of the Taylor principle and more like a measurement problem.

Caveats

  • Determinacy is a property of the model. Under learning rather than rational expectations the same condition governs whether agents can learn the equilibrium, which is reassuring (Bullard & Mitra, 2002), but other frictions change the boundary.

  • At the effective lower bound the rule cannot deliver a nominal rate below zero (or slightly below), so the principle cannot be satisfied for large negative shocks. This is why Measuring the policy stance needs tools beyond the policy rate.

Bullard, J., & Mitra, K. (2002). Learning about monetary policy rules. Journal of Monetary Economics, 49(6), 1105–1129. https://doi.org/10.1016/S0304-3932(02)00144-7
Clarida, R., Galı́, J., & Gertler, M. (1999). The science of monetary policy: A New Keynesian perspective. Journal of Economic Literature, 37(4), 1661–1707. https://doi.org/10.1257/jel.37.4.1661
Clarida, R., Galı́, J., & Gertler, M. (2000). Monetary policy rules and macroeconomic stability: Evidence and some theory. Quarterly Journal of Economics, 115(1), 147–180. https://doi.org/10.1162/003355300554692
Galı́, J. (2015). Monetary policy, inflation, and the business cycle: An introduction to the new keynesian framework and its applications (2nd ed.). Princeton University Press.
Woodford, M. (2001). The Taylor rule and optimal monetary policy. American Economic Review, 91(2), 232–237. https://doi.org/10.1257/aer.91.2.232
Woodford, M. (2003). Interest and prices: Foundations of a theory of monetary policy. Princeton University Press.