Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung

TL;DR

This study uses numerical simulations of binary neutron star mergers to evaluate how nucleon-nucleon-axion bremsstrahlung as a cooling mechanism affects observable signals, finding minimal impact on gravitational waves and ejecta for current detection capabilities.

Contribution

It introduces a phenomenological model of nucleon-nucleon-axion bremsstrahlung into merger simulations to assess its observational signatures.

Findings

Temperature profile of merger remnant is affected by axion cooling.

Impact on gravitational wave signals is too small to constrain axion properties.

Ejecta mass shows negligible change due to axion cooling.

Abstract

The QCD axion is a hypothetical particle motivated by the Strong CP problem of particle physics. One of the primary ways in which its existence can be inferred is via its function as an additional cooling channel in stars, with some of the strongest constraints coming from the supernova observation SN1987A. Multimessenger observations of binary neutron star mergers (such as those of GW170817, AT2017gfo, and GRB170817A) may provide another scenario in which such constraints could be obtained. In particular, the axion could potentially alter the lifetime, the ejection of material, and the emitted gravitational wave signal of the postmerger remnant. In this article, we perform numerical relativity simulations of a binary neutron star merger, including a phenomenological description of the nucleon-nucleon-axion bremsstrahlung to quantify the effects of such a cooling channel on the dynamical evolution. While our simulations show a difference in the temperature profile of the merger remnant, the imprint of the axion via nucleon-nucleon-axion bremsstrahlung on the emitted gravitational wave signal and the ejecta mass is too small to improve constraints on the axion mass with current or future planned detectors. Whilst we consider a limited number of cases, and a simplified cooling model, these broadly represent the "best case" scenario, thus, a more thorough investigation is unlikely to change the conclusions, at least for this particular interaction channel.