Article contents
Magnetic Color-flavor-locked Stars
Published online by Cambridge University Press: 20 March 2013
Abstract
Using the solutions of the gap equations of the magnetic-color-flavor-locked (MCFL) phase of paired quark matter in a magnetic field, and taking into consideration the separation between the longitudinal and transverse pressures due to the field-induced breaking of the spatial rotational symmetry, the equation of state (EoS) of the MCFL phase is self-consistently determined. Implications for stellar models of magnetized (self-bound) strange stars and hybrid (MCFL core) stars are discussed.
- Type
- Contributed Papers
- Information
- Copyright
- Copyright © International Astronomical Union 2013
References
- 1
- Cited by