Massless topological shells inside neutron stars produce non-monotonic shifts in f-mode frequencies and potentially detectable changes in gravitational-wave damping times and strains relative to standard models.
Chandrasekhar, The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity., Astrophys
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Topological Shell Structures in Neutron Stars: Effects on Equilibrium, Oscillations, and Gravitational-Wave Signatures
Massless topological shells inside neutron stars produce non-monotonic shifts in f-mode frequencies and potentially detectable changes in gravitational-wave damping times and strains relative to standard models.