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• W3100533248 endingPage "12" @default.
• W3100533248 startingPage "12" @default.
• W3100533248 abstract "Using the idea of a smooth crossover from the hadronic matter with hyperons to quark matter with strangeness, we show that the maximum mass of neutron stars with quark matter core can be larger than those without quark matter core. This is in contrast to the conventional softening of equation of state due to exotic components at high density. Essential conditions to reach our conclusion are (i) the crossover takes place at relatively low densities, around 3 times the normal nuclear density, and (ii) the quark matter is strongly interacting in the crossover region. By these, the pressure of the system can be greater than that of purely hadronic matter in the crossover region and leads to the maximum mass greater than 2 solar mass. This conclusion is insensitive to the different choice of the hadronic equation of state with hyperons. Several implications of this result to the nuclear incompressibility, the hyperon mixing, and the neutrino cooling are also remarked." @default.
• W3100533248 created "2020-11-23" @default.
• W3100533248 creator A5059258606 @default.
• W3100533248 creator A5074770743 @default.
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• W3100533248 date "2013-01-21" @default.
• W3100533248 modified "2023-10-15" @default.
• W3100533248 title "HADRON-QUARK CROSSOVER AND MASSIVE HYBRID STARS WITH STRANGENESS" @default.
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• W3100533248 doi "https://doi.org/10.1088/0004-637x/764/1/12" @default.
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