Resonance locking and tidal evolution in rotating {\gamma}-Doradus binaries

TL;DR

This study investigates how resonance locking influences tidal interactions and orbital evolution in rotating b3 dordus binaries, revealing its role in angular momentum exchange and system synchronization.

Contribution

It introduces a coupled orbital and stellar oscillation code that models the impact of dynamical tides with multiple forcing frequencies and rotation effects.

Findings

Resonance locking can be stable over long periods in rapidly rotating stars.

It can increase a star's angular momentum by about 70% during the main sequence.

Resonance locking can slow rotational evolution and drive asynchronization in binary systems.

Abstract

In binary systems, studying tidal interactions is key to understanding the evolution of binary populations. The primary dissipation process occurring in stars with radiative envelopes is believed to be radiative damping of high-radial-order tidally excited oscillations, which is in agreement with observations of most binary systems. However, recent studies have suggested that outside this dissipation regime, dynamical tides can act in the opposite manner (a phenomenon known as inverse tides), and resonance locking could significantly impact the orbital evolution of binary systems. We aim to study inverse tides and resonance locking by simultaneously including the effect of all the forcing frequencies and accounting for the effect of the rotation on the forced oscillations. We have developed an orbital evolution code that is coupled to a stellar oscillation code to compute on the fly the impact of dynamical tides on the rotational and orbital evolution of binary systems including multiple simultaneous forcing frequencies. We find that resonance locking can be stable over a long period of time and a source of long-term exchange of angular momentum for rapidly rotating stars. Long-term locking can increase the total angular momentum of a fast-rotating star by approximately 70% during the main sequence. For slow-rotating stars, resonance locking can slow down the rotational evolution of the system over most of the main-sequence phase, even in the presence of strong tidal interactions. This mechanism efficiently drives asynchronisation in binary systems where significant discrepancies already exist between the orbital and rotational frequencies.