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Madsen, J · 1992 · DOI 10.1103/physrevd.46.3290

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astro-ph.HE 1

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Modelling Dissipative Dynamics of r-mode Instability in Hybrid Stars

astro-ph.HE · 2026-06-25 · unverdicted · novelty 4.0

Bayesian inference on observational data yields shear viscosity timescale τ_s=(4.99^{+0.49}_{-0.52})×10^8 T^{5/3} s and bulk viscosity timescale for two-layer hybrid stars, giving frequency minima of 451.87 Hz and 517.47 Hz that explain stability of pulsars including XTE J0929-314.

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  • Modelling Dissipative Dynamics of r-mode Instability in Hybrid Stars astro-ph.HE · 2026-06-25 · unverdicted · none · ref 1

    Bayesian inference on observational data yields shear viscosity timescale τ_s=(4.99^{+0.49}_{-0.52})×10^8 T^{5/3} s and bulk viscosity timescale for two-layer hybrid stars, giving frequency minima of 451.87 Hz and 517.47 Hz that explain stability of pulsars including XTE J0929-314.