核心概念
本研究採用量子色動力學 (QCD) 微擾模型,並結合最新的粒子數據組數據集,探討了奇異夸克星 (SQS) 的結構特性,特別是通過引入密度相依的有效袋參數來解釋非微擾效應的影響。
統計資料
Λ1.4M⊙ < 580
MT OV > 2M⊙
ms(2GeV ) = 96 MeV
αs(mτ) = 0.314
v2/c2 = 1/3
引述
"This study investigates the structural properties of strange quark stars (SQS) using a Quantum Chromodynamics (QCD) perturbative model combined with the latest Particle Data Group dataset."
"Given the energy scale present in compact stars, QCD perturbation theory alone may not fully explain their structure."
"To account for non-perturbative contributions, we incorporate a density-dependent effective bag parameter, B, and derive the equation of state (EOS) for strange quark matter (SQM)."