1. Topology change, emergent symmetries and compact star matter
- Author
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Yong-Liang Ma, Mannque Rho, Institut de Physique Théorique - UMR CNRS 3681 (IPHT), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)
- Subjects
topology: transition ,symmetry: flavor ,star: compact ,Nuclear Theory ,Emergent symmetry ,[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th] ,QC1-999 ,FOS: Physical sciences ,Compact star ,Topology ,01 natural sciences ,expansion 1/N: color ,topological ,Nuclear Theory (nucl-th) ,effective field theory ,High Energy Physics - Phenomenology (hep-ph) ,0103 physical sciences ,quantum chromodynamics ,Effective field theory ,Saturation (graph theory) ,Stress–energy tensor ,density: high ,010306 general physics ,Topology (chemistry) ,energy: low ,Physics ,High Energy Astrophysical Phenomena (astro-ph.HE) ,condensed matter ,Topology change ,010308 nuclear & particles physics ,Skyrmion ,High Energy Physics::Phenomenology ,General Medicine ,quark hadron ,Nuclear matter ,Compact star matter ,velocity: acoustic ,Baryon ,High Energy Physics - Phenomenology ,topology: effect ,nuclear matter ,tensor: energy-momentum ,[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] ,Astrophysics - High Energy Astrophysical Phenomena ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,saturation: density ,Gravitational wave - Abstract
Topology effects have being extensively studied and confirmed in strongly correlated condensed matter physics. In the large color number limit of QCD, baryons can be regarded as topological objects -- skyrmions -- and the baryonic matter can be regarded as a skyrmion matter. We review in this paper the generalized effective field theory for dense compact-star matter constructed with the robust inputs obtained from the skyrmion approach to dense nuclear matter, relying to possible ``emergent" scale and local flavor symmetries at high density. All nuclear matter properties from the saturation density $n_0$ up to several times $n_0$ can be fairly well described. A uniquely novel -- and unorthdox -- feature of this theory is the precocious appearance of the pseudo-conformal sound velocity $v^2_{s}/c^2 \approx 1/3$, with the non-vanishing trace of the energy momentum tensor of the system. The topology change encoded in the density scaling of low energy constants is interpreted as the quark-hadron continuity in the sense of Cheshire Cat Principle (CCP) at density $\gsim 2n_0$ in accessing massive compact stars. We confront the approach with the data from GW170817 and GW190425., Comment: Version published in AAPPS Bulletin
- Published
- 2021
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