Seminars 李政道研究所-粒子核物理研究所联合演讲

Trace anomaly in neutron stars

by Dr Yuki Fujimoto (Institute for Nuclear Theory, University of Washington)

Asia/Shanghai
Online

Online

Description

Abstract

The recent observational data suggest that the equation of state of neutron star matter stiffens rapidly around a few times the saturation density. We discuss an interpretation that a peak in the sound velocity in neutron star matter, as suggested by the observational data, signifies strongly-coupled conformal matter. The normalized trace anomaly is a dimensionless measure of conformality leading to the derivative and the non-derivative contributions to the sound velocity. We find that the peak in the sound velocity is attributed to the derivative contribution from the trace anomaly that steeply approaches the conformal limit. Smooth continuity to the behavior of high-density QCD implies that the matter part of the trace anomaly may be positive definite. We discuss pros and cons for the trace anomaly being positive semi-definite and a possible implication of the positivity condition of the trace anomaly on the observable quantities of the neutron stars. [arxiv:2207.06753]

Online meeting room

https://cern.zoom.us/j/67311786739?pwd=dktWOC8rOGJrQm1lamFEQzFiQUV6QT09   (ID: 673 1178 6739 Passcode: 606814)

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