[Submitted on 7 Sept 2016] (cross-list from astro-ph.HE)
X-ray bounds on the r-mode amplitude in millisecond pulsars
Kai Schwenzer · Tuğba Boztepe · Tolga Güver · Eda Vurgun
r-mode astroseismology provides a unique way to study the internal composition of compact stars. Due to their precise timing, recycled millisecond radio pulsars present a particularly promising class of sources. Although their thermal properties are still poorly constrained, X-ray data is very useful for astroseismology since r-modes could strongly heat a star. Using known and new upper bounds on the temperatures and luminosities of several non-accreting millisecond radio pulsars we derive bounds on the r-mode amplitude as low as and discuss the impact on scenarios for their internal composition.
- Comments:
- 10 pages, 8 figures
- Subjects:
- High Energy Astrophysical Phenomena (astro-ph.HE); General Relativity and Quantum Cosmology (gr-qc); Nuclear Theory (nucl-th)
- arXiv:
- 1609.01912 [pdf]