Oscillating Strange Quark Matter Objects Excited in Stellar Systems
arXiv:2002.09593 · doi:10.3847/1538-4357/ab97ab
Abstract
It is shown that strange quark matter (SQM) objects, stars, and planets, can very efficiently convert the mechanical energy into hadronic energy when they oscillate. This is because the mass density at the edge of SQM objects, , is the critical density below which SQM is unstable with respect to decay into photons, hadrons, and leptons. We consider here radial oscillations of SQM objects that could be induced in stellar or planetary systems where tidal interactions are ubiquitous. Oscillations of radius amplitude already result in keV per unit baryon number excitation near the surface of SQM stars. The excitation energy is converted into electromagnetic energy in a short time of 1 ms, during a few oscillations. Higher amplitude oscillations result in faster energy release that could lead to fragmentation or dissolution of SQM stars. This would have significant consequences for hypothetical SQM star binaries and planetary systems of SQM planets with regard to gravitational wave emission.
arXiv comment7 pages, 3 captioned figures, 1 table, accepted for publication in ApJ
References in corpus (7)
- Radial oscillations of relativistic stars
- Discriminating Strange Star Mergers from Neutron Star Mergers by Gravitational-Wave Measurements
- Strange quark matter fragmentation in astrophysical events
- Evolution of Highly Eccentric Binary Neutron Stars Including Tidal Effects
- Coalescence of Strange-Quark Planets with Strange Stars: a New Kind of Sources for Gravitational Wave Bursts
- Searching for strange quark matter objects in exoplanets
- Close-in Exoplanets as Candidates of Strange Quark Matter Objects