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Hybrid stars rotating

Figure 12. Kepler period versus the rotational mass for purely hadronic stars as well as hybrid stars. The following core compositions are considered i) nucleons and leptons (dotted line) ii) nucleons, hyperons, and leptons (dashed line) in) hadrons, quarks, and leptons (solid line). The shaded area represents the current range of observed data. Figure 12. Kepler period versus the rotational mass for purely hadronic stars as well as hybrid stars. The following core compositions are considered i) nucleons and leptons (dotted line) ii) nucleons, hyperons, and leptons (dashed line) in) hadrons, quarks, and leptons (solid line). The shaded area represents the current range of observed data.
Figure 10. The Mass - radius relation and mass - central energy density dependencies for rotating (dashed lines) and nonrotating (solid lines) hybrid star configurations... Figure 10. The Mass - radius relation and mass - central energy density dependencies for rotating (dashed lines) and nonrotating (solid lines) hybrid star configurations...

See other pages where Hybrid stars rotating is mentioned: [Pg.131]    [Pg.278]    [Pg.371]    [Pg.377]    [Pg.392]    [Pg.394]    [Pg.392]    [Pg.251]   
See also in sourсe #XX -- [ Pg.393 ]




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Hybrid stars

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