A self-consistent study of magnetic field effects on hybrid stars
arXiv:1702.00386 · doi:10.1088/1742-6596/861/1/012012
Abstract
It is understood that strong magnetic fields affect the structure of neutron stars. Nevertheless, many calculations for magnetized neutron stars are still being performed using symmetric solutions of Einstein's equations. In this conference proceeding, we review why this is not the correct procedure and we also discuss the effects of magnetic fields on the stellar population and temperature profiles.
Prepared for Conference "Compact Stars in the QCD phase diagram V" 23-27 May 2016 GSSI and LNGS (L'Aquila, Italy)
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Cited by in corpus (11)
- What is the magnetic field distribution for the equation of state of magnetized neutron stars?
- Magnetic field distribution in magnetars
- D mesons in strongly magnetized asymmetric nuclear matter
- Open bottom mesons in asymmetric nuclear matter in presence of strong magnetic fields
- Charmonium states in strong magnetic fields
- Tabulated Neutron Star Equations of State Modeled within the Chiral Mean Field Model
- Charmonium decay widths in magnetized matter
- Magnetically supramassive neutron stars
- (Anti)kaon condensation in strongly magnetized dense matter
- Kaons and antikaons in strong magnetic fields
- QCD sum rule analysis of Heavy Quarkonium states in magnetized matter -- effects of (inverse) magnetic catalysis