@article{oai:iwate-u.repo.nii.ac.jp:00014029,
 author = {Takatsuka, Tatsuyuki and Hatsuda, Tetsuo and Masuda, Kota},
 journal = {AIP Conference Proceedings},
 month = {Jan},
 note = {We propose a new strategy to construct the equation of state (EOS) for neutron stars (NSs) with hadron-quark (H-Q) phase transition, by considering three density-regions. We supplement the EOS at H-Q region, very uncertain due to the confinement-deconfinement problems, by sandwitching in between and matching to the relatively “well known” EOSs, i.e., the EOS at lower densities (H-phase up to several times nuclear density, calculated from a G-matrix approach) and that at ultra high densities (Q-phase, form a view of asymptotic freedom). Here, as a first step, we try a simple case and discuss the maximum mass of NSs.},
 pages = {406--408},
 title = {Maximum mass of neutron stars with quark matter core},
 volume = {1484},
 year = {2012}
}