Two-Fluid Radial Stability of Dark-Matter-Admixed Compact Objects: Dark Compact Planets, Dark White Dwarfs, Dark Neutron Stars, and Dark Oysters
hep-ph, astro-ph.HE, astro-ph.SR, gr-qc, nucl-th
Submitted: 2026-10-29
Updated: 2026-10-29
Related papers
- Crowdsourcing Gravitational Waves from Superradiant Axions
- Classification of g-modes for neutron stars with a strong transition: Novel universal relation including slow stable hybrid stars
- Symmetry-Preserving and Scalable Variational Circuits for the Lattice Gross-Neveu Model
- New Bounds on Heavy QCD Axions from Big Bang Nucleosynthesis
- Evidence for Kaluza-Klein excitations of the graviton, gluon and quark at LHC
- LUNAR: a Monte Carlo generator for bound-nucleon decay in liquid argon