[Submitted on 15 Dec 2015] (cross-list from astro-ph.SR)
Oscillations of superfluid hyperon stars: decoupling scheme and g-modes
V.A. Dommes · M.E. Gusakov (Ioffe Institute)
We analyse the oscillations of general relativistic superfluid hyperon stars, following the approach suggested by Gusakov & Kantor and Gusakov et al. and generalizing it to the nucleon-hyperon matter. We show that the equations governing the oscillations can be split into two weakly coupled systems with the coupling parameters , , and . The approximation (decoupling approximation) allows one to drastically simplify the calculations of stellar oscillation spectra. An efficiency of the presented scheme is illustrated by the calculation of sound speeds in the nucleon-hyperon matter composed of neutrons (n), protons (p), electrons (e), muons (), as well as , , and -hyperons. However, the gravity oscillation modes (g-modes) cannot be treated within this approach, and we discuss them separately. For the first time we study the composition g-modes in superfluid hyperon stars with the core and show that there are two types of g-modes (`muonic' and `--hyperonic') in such stars. We also calculate the g-mode spectrum and find out that the eigenfrequencies of the superfluid g-modes can be exceptionally large (up to for a considered stellar model).
- Comments:
- 20 pages, 8 figures, published in MNRAS
- Subjects:
- Solar and Stellar Astrophysics (astro-ph.SR); High Energy Astrophysical Phenomena (astro-ph.HE); General Relativity and Quantum Cosmology (gr-qc); Nuclear Theory (nucl-th)
- arXiv:
- 1512.04900 [pdf]