Trace Anomaly of Cold Dense Matter Constrained by Collective Flow
Bao-An Li

TL;DR
This paper presents the first Bayesian extraction of the trace anomaly of cold dense matter from heavy-ion collision data, showing consistency with neutron star observations and establishing it as a universal macroscopic property.
Contribution
It introduces a novel Bayesian method to determine the trace anomaly from laboratory data, linking heavy-ion collisions with astrophysical observations.
Findings
Trace anomaly from flow data agrees with astrophysical posterior bands within 68% credible intervals.
Heavy-ion collisions and neutron star observations probe the same macroscopic properties of dense matter.
The trace anomaly acts as a composition-insensitive observable bridging different physical environments.
Abstract
The trace anomaly of dense matter, , defined through the ratio of pressure to energy density , quantifies deviations from conformal symmetry and provides a dimensionless measure of the stiffness of the equation of state (EOS) relevant for both neutron stars and heavy-ion collisions. While has recently been inferred from neutron star observations, we report the first Bayesian extraction of the trace anomaly from collective flow observables in intermediate-energy heavy-ion collisions. By employing transport-model simulations that explicitly decouple the cold matter mean-field potential from thermal effects, we directly constrain the EOS of cold dense matter. Remarkably, the trace anomaly inferred from laboratory flow data agrees quantitatively, within credible intervals, with…
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Taxonomy
TopicsHigh-Energy Particle Collisions Research · Pulsars and Gravitational Waves Research · Dust and Plasma Wave Phenomena
