| Home | Organizers | Proceedings Editors | Proceedings Contributors | Search | | ||
|
|
|||
|
||||
|
|
||||
| Title: | EFFECTS OF QCD PHASE TRANSITION ON THE EJECTED ELEMENTS FROM THE ENVELOPES OF COMPACT STARS | |
| DOI No: | 10.1142/9789812793379_0019 | |
| Source: | PHYSICS OF SELF-ORGANIZATION SYSTEMS (pp 219-225) | |
| Author(s): | N. YASUTAKE
www.heap.phys.waseda.ac.jp/yasutake/opening.html Science and Engineering, Waseda University, Tokyo 169-8555, Japan S. YAMADA Science and Engineering, Waseda University, Tokyo 169-8555, Japan T. NODA Department of Physics, Kyushu University, Fukuoka 810-8560, Japan M. HASHIMOTO Department of Physics, Kyushu University, Fukuoka 810-8560, Japan K. KOTAKE Division of Theoretical Astronomy, National Astronomical Observatory of Japan, Tokyo 181-8588, Japan |
|
| Abstract: | We perform hydrodynamical collapse and bounce simulations of neutron stars induced by QCD phase transition. We study how the phase transition affects the elements of the envelopes and crusts of neutron stars near the epoch of core-bounce. We assume the first-order phase transition, a chirally symmetric quark-gluon plasma for quark phase. The initial elements are adopted from the realistic evolutional calculations of neutron stars containing the cooling effects and the nucleosynthesis of envelope such as type I X-ray burst. We find that the elements of envelope can eject directly (without nucleosynthesis) for such a collapse and bounce by the transition. | |
| Keywords: | QCD phase transition; nucleosynthesis; quark star; neutron star |
|
| Full Text: | View full text in PDF format (148KB) | |
| TOC: | Back to Table of Contents | |
|
||