Distinguishing Newly Born Strange Stars from Neutron Stars with g-Mode Oscillations

Details Distinguishing Newly Born Strange Stars from Neutron Stars with g-Mode Oscillations Distinguishing Newly Born Strange Stars from Neutron Stars with g-Mode Oscillations

2008-10-07

arxiv.org/abs/0810.1084v2

Phys.Rev.Lett.101:181102,2008

Physics

Nuclear Physics

Nuclear Theory

9 pages, 1 figure

Scientific paper

10.1103/PhysRevLett.101.181102

The gravity-mode (g-mode) eigenfrequencies of newly born strange quark stars (SQSs) and neutron stars (NSs) are studied. It is found that the eigenfrequencies in SQSs are much lower than those in NSs by almost one order of magnitude, since the components of a SQS are all extremely relativistic particles while nucleons in a NS are non-relativistic. We therefore propose that newly born SQSs can be distinguished from the NSs by detecting the eigenfrequencies of the g-mode pulsations of supernovae cores through gravitational radiation by LIGO-class detectors.

Affiliated with

Also associated with

No associations

Rating

Distinguishing Newly Born Strange Stars from Neutron Stars with g-Mode Oscillations 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 Distinguishing Newly Born Strange Stars from Neutron Stars with g-Mode Oscillations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Distinguishing Newly Born Strange Stars from Neutron Stars with g-Mode Oscillations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-556658