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$) we expect the error due to the choice of the adiabatic approximation to be minimal. For the $^{208}$Pb nucleus, the error is of the order $0.25%$ and for the lightest considered nucleus, $^{12}$C, the error is only $0.1%$. Conclusions =========== Using the adiabatic expansion of medium modified nuclear matter equation of state for quark matter recently derived in [@2018PhRvD..97j4051R], we have shown that the quark matter core of massive stars is in stable equilibrium in the presence of nucleon matter, provided that it is stiff enough in itself.
However, it seems like is an HTML5 page and the content can be extracted with the following Python code: totalRows = [getAnyTag(full_html, "a") for full_html in HTMLTABLE] count = sum([1 for c in HTMLTABLE]) (+44) 0800 151 1215 d2c66b5586