arXiv · hep-ph/0105158
Probing Quark Matter In Neutron Stars
Abstract
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 $ν-$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.
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M. Prakash. 2001-05-16. Probing Quark Matter In Neutron Stars. https://doi.org/10.1016/s0375-9474(01)01399-9
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