LEADER 03346nam 2200529 450 001 9910164134203321 005 20230422034032.0 010 $a981-4527-20-3 035 $a(CKB)3710000001051513 035 $a(MiAaPQ)EBC4800896 035 $a(WSP)00004189 035 $a(EXLCZ)993710000001051513 100 $a20170217h19991999 uy 0 101 0 $aeng 135 $aurcnu|||||||| 181 $2rdacontent 182 $2rdamedia 183 $2rdacarrier 200 10$aProceedings of strong and electroweak matter '98 $eCopenhagen, Denmark, 2-5 Dec 1998 /$feditors, Jan Ambjorn [and three others] 210 1$aSingapore :$cWorld Scientific,$d1999. 210 4$d©1999 215 $a1 online resource (426 pages) $cillustrations 300 $aTitle from PDF title page (viewed March 30, 2017). 300 $aPapers presented at a conference held on December 2-5, 1998 in Copenhagen, Denmark. 311 $a981-02-4031-7 320 $aIncludes bibliographical references at the end of each chapters. 330 $a"Already in 1997, the topics included in this meeting had been enlarged to include all different phases and phase transitions relevant on laboratory scales or in cosmology. The '98 meeting followed this trend, and there was a balanced combination of the physics associated with both strong and electroweak interactions (and beyond). The main motivation continues to be the understanding of the standard model in ?extreme? situations, particularly relevant on the cosmological scale. Most contributions were in one way or another concerned with the finite-temperature aspects of strong and electroweak interactions, and, as in the previous meeting, one persistent theme was the present understanding of baryon-number asymmetry: how it can be created, and how it can be maintained beyond the earliest stages of the Universe. The recent progress in describing the real-time and nonequilibrium dynamics of the non-Abelian gauge was covered in a number of the main talks, as well as in several shorter contributions and posters. The conference presented examples of impressive analytical progress and equally impressive results from numerical simulations: the two techniques continue to fruitfully complement each other. One completely new theme at this conference was the recent suggestion that finite-density QCD may contain new and interesting condensed phases in the neighborhood of the conventional critical density separating quark matter from hadronic matter. All of these developments, and many more, are reflected in this book."--Publisher's website. 517 3 $aStrong and electroweak matter '98 606 $aElectroweak interactions$vCongresses 606 $aNuclear matter$vCongresses 606 $aNuclear reactions$vCongresses 606 $aNuclear astrophysics$vCongresses 606 $aStandard model (Nuclear physics)$vCongresses 615 0$aElectroweak interactions 615 0$aNuclear matter 615 0$aNuclear reactions 615 0$aNuclear astrophysics 615 0$aStandard model (Nuclear physics) 676 $a539.7544 702 $aAmbjørn$b Jan 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910164134203321 996 $aProceedings of strong and electroweak matter '98$92586257 997 $aUNINA