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 Date: 2013-07-27 00:52:38Nuclear physics Exotic matter Astrophysics Baryons Star types Neutron star Nucleon Degenerate matter Neutron Physics Matter Particle physics |
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PORTILLO 1 Neutron Star Core Equations of State and the Maximum Neutron Star Mass Stephen K N P ORTILLO | Hadrons baryons mesons fermionsDocID: 1v7xl - View Document |
 | Citation: M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, ) Ξ BARYONS (S = −2, I = 1/2) Ξ 0 = uss,DocID: 1v4xM - View Document |
 | Citation: M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, ) ∆ BARYONS (S = 0, I = 3/2) ∆++ = u u u,DocID: 1uyHK - View Document |
 | Citation: M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, CHARMED BARYONS (C = +1) ++ 0DocID: 1uoXm - View Document |
 | Citation: M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, BOTTOM BARYONS (B = −1) − Λ0b = u d b, Ξ 0b = u s b, Ξ −DocID: 1u7oo - View Document |