Radial oscillation frequencies of neutron stars are computed in Starobinsky and Gauss-Bonnet extended gravity, revealing a dynamical exterior and a low-density plateau in the fundamental mode.
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Radial oscillations of neutron stars in Starobinsky gravity and its Gauss-Bonnet extension
Radial oscillation frequencies of neutron stars are computed in Starobinsky and Gauss-Bonnet extended gravity, revealing a dynamical exterior and a low-density plateau in the fundamental mode.