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Analytical Representation for Equations of State of Dense Matter

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arxiv 1108.2166 v2 pith:BU3OC4RH submitted 2011-08-10 astro-ph.SR astro-ph.HEastro-ph.IM

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keywords analyticaldenseequationsmatterneutronrepresentationstatederivatives
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We present an analytical unified representation for 22 equations of state (EoS) of dense matter in neutron stars. Such analytical representations can be useful for modeling neutron star structure in modified theories of gravity with high order derivatives.

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Cited by 1 Pith paper

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  1. Neutron Stars in Causal Scalar-Tensor Theories

    gr-qc 2025-05 conditional novelty 6.0 of 10

    Solving modified TOV equations in an anti-screened K-essence scalar-tensor theory, the authors find two solution branches per central density and a critical density cutoff, producing mass-radius predictions that can m...

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