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AbstractAbstract
[en] Neutron stars represent excellent physical systems for the study of the high density QCD phase transition that might occur in their core. A promising line of research concerns the possible signatures of the dynamics of the formation of quark matter in a neutron star. We review the different signatures that have been recently proposed in connection with explosive phenomena such as supernovae, gamma-ray-bursts, merger of neutron stars. (author)
Original Title
PACS numbers: 97.60.Jd, 21.65.Qr, 97.60.Bw, 98.70.Rz
Primary Subject
Source
Excited QCD 2010 Workshop; Tatranska Lomnica - Stara Lesna (Slovakia); 31 Jan - 6 Feb 2010; DFG GRANT PA 1780/2-1; Also available at http://th-www.if.uj.edu.pl/acta/sup3/pdf/s3p0791.pdf; 27 refs.
Record Type
Journal Article
Literature Type
Conference
Journal
Acta Physica Polonica. Series B, Proceedings Supplement; ISSN 1899-2358;
; v. 3(4); p. 791-796

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