Probing Quark Matter In Neutron Stars

Details Probing Quark Matter In Neutron Stars Probing Quark Matter In Neutron Stars

2001-05-16

arxiv.org/abs/hep-ph/0105158v1

Nucl.Phys. A698 (2002) 440-443

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages, 2 figures. To appear in the proceedings of QM 2001. Uses fleqn.sty and espcrc1.sty

Scientific paper

10.1016/S0375-9474(01)01399-9

The presence of quark matter in neutron star interiors may have distinctive signatures in basic observables such as (i) masses and radii [1], (ii) surface temperatures versus age [2], (iii) spin-down rates of milli-second pulsars [3], and (iv) neutrino luminosities from future galactic core collapse supernovae [4]. I highlight recent developments in some of these areas with a view towards assessing how theory may be confirmed by $\nu-$signals from future galactic supernovae in detectors like SuperK, SNO and others under consideration, including UNO [5], and by multi-wavelength photon observations with new generation satellites such as the HST, Chandra, and XMM.

Affiliated with

Also associated with

No associations

Rating

Probing Quark Matter In Neutron Stars 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 Probing Quark Matter In Neutron Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Probing Quark Matter In Neutron Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-150765