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20242026
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astro-ph.HE2026

Universality of dual mass-scaled fundamental modes in two-fluid neutron stars with mirror dark matter

Hajime Sotani, Ankit Kumar

The paper investigates the vibration frequencies of neutron stars containing mirror dark matter using a two‑fluid model, showing that mass‑scaled fundamental frequencies follow uni…

astro-ph.HE2026

Slowly Rotating Two-Fluid Neutron Stars: Coupled Frame-Dragging, Inertia Splitting, and Universal Relations

Ankit Kumar, Hajime Sotani

We develop a fully relativistic framework to study the rotational response of gravitationally coupled two-fluid neutron stars within the slow-rotation approximation. Treating the t…

astro-ph.HE2025

Universal relation involving fundamental modes in two-fluid dark matter admixed neutron stars

Hajime Sotani, Ankit Kumar

We systematically investigate the fundamental oscillation frequencies of dark matter admixed neutron stars, focusing on models with self-interacting fermionic dark matter that coup…

astro-ph.HE2025

Stability analysis of two-fluid neutron stars featuring twin star and ultradense configurations

Ankit Kumar, Hajime Sotani

We perform a detailed analysis of radial oscillations to discuss dynamical stability in two-fluid neutron stars composed of ordinary nuclear matter and a gravitationally coupled da…

astro-ph.HE2025

Asteroseismology and Universal Relations in Neutron Stars with Gravitationally Bound Dark Matter

Ankit Kumar, Hajime Sotani

We investigate the structural, dynamical, and oscillatory properties of neutron stars admixed with dark matter, modeled via a single-fluid formalism where dark matter interacts wit…

astro-ph.HE2025

Emergence of new oscillation modes in dark matter admixed neutron stars

Hajime Sotani, Ankit Kumar

Dark matter admixed neutron stars provide a promising avenue for observationally probing the dark matter characteristic. In this study, we examine non-radial oscillations in neutro…