Abstract
Integrating out high energy degrees of freedom to yield a low energy effective field theory leads to a loss of information with a concomitant increase in entropy. We obtain the effective field theory of a light scalar field interacting with heavy fields after tracing out the heavy degrees of freedom from the time evolved density matrix. The initial density matrix describes the light field in its ground state and the heavy fields in equilibrium at a common temperature $T$. For $T=0$, we obtain the reduced density matrix in a perturbative expansion, it reveals an emergent mixed state as a consequence of the entanglement between light and heavy fields. We obtain the effective action that determines the time evolution of the \emph{reduced} density matrix for the light field in a non-perturbative Dyson resummation of one-loop correlations of the heavy fields. The Von-Neumann \emph{entanglement entropy} associated with the reduced density matrix is obtained for the non-resonant and resonant cases in the asymptotic long time limit. In the non-resonant case the reduced density matrix displays an \emph{incipient} thermalization albeit with a wave-vector, time and coupling dependent \emph{effective temperature} as a consequence of memory of initial conditions. The entanglement entropy is time independent and is the \emph{thermal entropy} for this effective, non-equilibrium temperature. In the resonant case the light field fully \emph{thermalizes} with the heavy fields, the reduced density matrix looses memory of the initial conditions and the entanglement entropy becomes the \emph{thermal entropy} of the light field. We discuss the relation between the entanglement entropy ultraviolet divergences and renormalization.
Highlights
Effective field theory describes physical phenomena below some energy scale or on large spatiotemporal scales and is widely used in different fields
In the previous section we provided a perturbative interpretation of the reduced density matrix and the origin of the entanglement entropy from the coarse graining process; we obtain the time evolution of the full density matrix from the effective action up to second order in the coupling
Our study is motivated by the observation that an effective field theory describing phenomena below some energy scale emerges, fundamentally, from tracing over or coarse graining the high energy degrees of freedom with a concomitant loss of information
Summary
Since at a fundamental level an effective field theory emerges after integrating or tracing out high energy (or short distance) degrees of freedom and describes only the low energy degrees of freedom, the reduction from the full field theory (whatever its origin may be) to the effective one entails a loss of information and a concomitant increase of the entropy. We evolve the initial density matrix in time and trace over the heavy degrees of freedom obtaining the reduced density matrix for the light field, and obtain the Von-Neumann entropy associated with the reduced density matrix in the asymptotic long time limit This entropy is different from the geometric (area) entropy [37,38,39,40] but both originate from tracing out (coarse graining) degrees of freedom. We analyze the emergence of the entanglement entropy upon coarse graining both from a perturbative and nonperturbative point of view The latter allows us to study in detail the effects of thresholds and the case in which the light field thermalizes with the heavy fields
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