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Innermost stable circular orbits of neutron stars in dilatonic-Einstein-Gauss-Bonnet theory

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arxiv 1812.02686 v1 pith:C5M7MUAF submitted 2018-12-06 gr-qc astro-ph.HEhep-th

classification gr-qcastro-ph.HEhep-th
keywords theorycirculardilatoniceinstein-gauss-bonnetinnermostneutronorbitsrelations
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The innermost stable circular orbits (ISCOs) around rapidly rotating neutron stars are studied in dilatonic Einstein-Gauss-Bonnet theory. Universal relations for properly scaled ISCO properties are extended from General Relativity to dilatonic Einstein-Gauss-Bonnet theory and additional relations are obtained.

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