Up-down quark stars in the two-families scenario yield tidal deformabilities compatible with GW170817, constraining the effective bag constant to approximately 50 MeV/fm^3.
Terazawa, INS-Report-336 (INS, University of Tokyo, Tokyo) May, 1979
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Probing up-down quark matter via gravitational waves
Up-down quark stars in the two-families scenario yield tidal deformabilities compatible with GW170817, constraining the effective bag constant to approximately 50 MeV/fm^3.