Tracing the Trace Anomaly of Dense Matter inside Neutron Stars

TL;DR

This paper develops quasi-universal relations linking the trace anomaly in neutron star matter to observable stellar properties, enabling estimation of the anomaly profile from astrophysical measurements.

Contribution

It introduces new quasi-universal relations connecting the trace anomaly to neutron star observables and applies them to real pulsar data for the first time.

Findings

Estimated the trace anomaly at the center of a 1.4 solar mass neutron star as 0.1770 with uncertainties.

Derived trace anomaly profiles for specific pulsars using mass-radius measurements.

Provided constraints on the trace anomaly from multimessenger observations.

Abstract

The trace anomaly $\Delta$ is an important quantity that measures the broken conformal symmetry in neutron star matter. In this work, we present quasi-universal relations that connect the stellar profile of $\Delta$ to the compactness, moment of inertia, and tidal deformability of neutron stars. We apply the quasi-universal relations to determine the trace anomaly profiles for PSR J0030+0451 and PSR J0740+6620 based on their mass-radius measurements. We also analyze PSR J0737-3039A according to its moment of inertia inferred from Bayesian modeling of nuclear equation of state. A recent multimessenger constraint on the tidal deformability is also studied, resulting in an estimate value of the trace anomaly $\Delta_c = 0.1770^{+0.0365}_{-0.0432}$ at the center of a $1.4M_\odot$ canonical neutron star. It is expected that more precise observations from both electromagnetic and gravitational-wave channels in the future will provide tighter constraints on the behavior of $\Delta$ inside neutron stars.