Kondo QCD effect in stellar matter
Kondo QCD effect in stellar matter
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发表时间：
2019-01
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通讯作者：
J. C. Macias;F. Navarra
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作者：
J. C. Macias;F. Navarra
研究了含有魅力杂质的轻($u$、$d$和$S$)夸克物质。将这些引起近藤相的杂质加到拉格朗日密度中，得到了状态方程。通过求解通常的TOV方程，研究了近藤位相对夸克星质量比关系的影响。
Light ($u$, $d$ and $s$)\ quark matter containing charm impurities is studied. These impurities, which induce a Kondo phase, are added to the Lagrangian density and the equation of state (EOS) is then derived. The effects of the Kondo phase on the mass-ratio relations of quark stars are examined by solving the usual TOV equations.