The Hartle-Thorne slow-rotation expansion is extended to seventh order, yielding analytical exterior metrics and multipole moments up to S7 for isolated neutron stars.
quark stars) The previously discussed matching procedure relied on imposing continuity at R = R∗
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Highly-accurate neutron star modeling in the Hartle-Thorne Approximation
The Hartle-Thorne slow-rotation expansion is extended to seventh order, yielding analytical exterior metrics and multipole moments up to S7 for isolated neutron stars.