Instability of Quark Matter Core in a Compact Newborn Neutron Star With Moderately Strong Magnetic Field

Details Instability of Quark Matter Core in a Compact Newborn Neutron Star With Moderately Strong Magnetic Field Instability of Quark Matter Core in a Compact Newborn Neutron Star With Moderately Strong Magnetic Field

2001-10-05

arxiv.org/abs/astro-ph/0110135v1

Pramana60:901-908,2002

Astronomy and Astrophysics

Astrophysics

Six pages REVTEX file, one .eps file (included)

Scientific paper

10.1007/BF02707009

It is explicitly shown that if phase transition occurs at the core of a
newborn neutron star with moderately strong magnetic field strength, which
populates only the electron's Landau levels, then in the $\beta$-equilibrium
condition, the quark core is energetically much more unstable than the neutron
matter of identical physical condition.

Affiliated with

Also associated with

No associations

Rating

Instability of Quark Matter Core in a Compact Newborn Neutron Star With Moderately Strong Magnetic Field does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Instability of Quark Matter Core in a Compact Newborn Neutron Star With Moderately Strong Magnetic Field, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Instability of Quark Matter Core in a Compact Newborn Neutron Star With Moderately Strong Magnetic Field will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-193465