Hyperons in Neutron Stars
arXiv:1509.03587 · doi:10.1088/1742-6596/668/1/012031
Abstract
In this work I briefly review some of the effects of hyperons on the properties of neutron and proto-neutron stars. In particular, I revise the problem of the strong softening of the EoS, and the consequent reduction of the maximum mass, induced by the presence of hyperons, a puzzle which has become more intringuing and difficult to solve due the recent measurements of the unusually high masses of the millisecond pulsars PSR J1903+0327 (), PSR J1614-2230 (), and PSR J0348+0432 (). Some of the solutions proposed to tackle this problem are discussed. Finally, I re-examine also the role of hyperons on the cooling properties of newly born neutron stars and on the so-called r-mode instability.
8 pages, 3 figures. Plenary talk at the 15th International Conference on Strangeness in Quark Matter (SQM2015), 6-11 July 2015, JINR, Dubna, Russia. To be published in Journal of Physics: Conference Series (JPCS)
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- Many-body forces in magnetic neutron stars
- Constraints on the muon fraction and density profile in neutron stars
- Delta baryons in neutron stars
- Exploring the effects of Delta Baryons in magnetars
- Phase transition in compact stars: nucleation mechanism and -ray bursts revisited
- Probing the impact of Delta-Baryons on Nuclear Matter and Non-Radial Oscillations in Neutron Stars
- Kaon condensation in skyrmion matter and compact stars
- Quark-Pauli effects in three octet-baryons
- Impact of QCD sum rules coupling constants on neutron stars structure
- The effect of inclusion of resonances in relativistic mean-field model with scaled hadron masses and coupling constants
- The Strange Physics of Dark Baryons