Magnetized color flavor locked state and compact stars

Details Magnetized color flavor locked state and compact stars Magnetized color flavor locked state and compact stars

2010-03-16

arxiv.org/abs/1003.3254v3

Eur.Phys.J.A47:1,2011

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

9 pages, 8 figures, 3 tables; version to be published in The European Physical Journal A

Scientific paper

10.1140/epja/i2011-11001-0

The stability of the color flavor locked phase in the presence of a strong magnetic field is investigated within the phenomenological MIT bag model, taking into account the variation of the strange quark mass, the baryon density, the magnetic field, as well as the bag and gap parameters. It is found that the minimum value of the energy per baryon in a color flavor locked state at vanishing pressure is lower than the corresponding one for unpaired magnetized strange quark matter and, as the magnetic field increases, the energy per baryon decreases. This implies that magnetized color flavor locked matter is more stable and could become the ground state inside neutron stars. The mass-radius relation for such stars is also studied.

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