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Low‐Mass Neutron Stars and the Equation of State of Dense Matter

  • Authors: J. Carriere, C. J. Horowitz, and J. Piekarewicz

Carriere, Horowitz, & Piekarewicz 2003 The Astrophysical Journal 593 463.

  • Provider: AAS Journals

Caption: Fig. 5.

Radius of a neutron star of mass 1.4 M⊙ as a function of the neutron skin in 208Pb. The solid curve is for the Z271 parameter set with ﹩\Lambda _{v}\neq 0﹩ while the dashed curve uses Z271 with ﹩\Lambda _{s}\neq 0﹩. The dotted curve is for the S271 set and the dot‐dashed curve for NL3, both of these with ﹩\Lambda _{v}\neq 0﹩.

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