GW190814: Circumstantial evidence for up-down quark star

نویسندگان

چکیده

Within a confining quark matter model which considers phenomenologically the confinement and asymptotic freedom as well chiral symmetry restoration deconfinement at high baryon density, we find that if up-down ($ud$QM) is more stable than nuclear strange (SQM), maximum mass of static stars with $ud$QM $2.87M_{\odot}$ under agreement both constraints on star tidal deformability from gravitational wave signal GW170817 mass-radius PSR J0030+0451 J0740+6620 measured by NICER. In contrast, conventional SQM while $ud$QM, has only $1.87M_{\odot}$ its radius significantly deviates NICER's constraint. Our results thus provide circumstantial evidence suggesting recently reported GW190814's secondary component $2.59^{+0.08}_{-0.09}M_\odot$ could be an star.

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ژورنال

عنوان ژورنال: Physical review

سال: 2022

ISSN: ['0556-2813', '1538-4497', '1089-490X']

DOI: https://doi.org/10.1103/physrevd.106.083007