Strong and electroweak matter 2002 : Heidelberg, Germany, 2-5 October 2002
The SEWM2002 workshop, like the ones before, brought together theoretical physicists working on thermal field theory and, more generally, on (resummation) techniques for deriving effective actions based on QCD and the electroweak standard model of elementary particle physics, but describing nonstand...
Đã lưu trong:
Định dạng: | Sách |
---|---|
Ngôn ngữ: | Undetermined |
Được phát hành: |
Singapore
World Scientific
2003
|
Những chủ đề: | |
Các nhãn: |
Thêm thẻ
Không có thẻ, Là người đầu tiên thẻ bản ghi này!
|
Thư viện lưu trữ: | Trung tâm Học liệu Trường Đại học Cần Thơ |
---|
LEADER | 01315nam a2200205Ia 4500 | ||
---|---|---|---|
001 | CTU_156808 | ||
008 | 210402s9999 xx 000 0 und d | ||
020 | |c 202 | ||
082 | |a 539.7 | ||
082 | |b P963 | ||
245 | 0 | |a Strong and electroweak matter 2002 : | |
245 | 0 | |b Heidelberg, Germany, 2-5 October 2002 | |
245 | 0 | |c edited by Michael G. Schmidt | |
260 | |a Singapore | ||
260 | |b World Scientific | ||
260 | |c 2003 | ||
520 | |a The SEWM2002 workshop, like the ones before, brought together theoretical physicists working on thermal field theory and, more generally, on (resummation) techniques for deriving effective actions based on QCD and the electroweak standard model of elementary particle physics, but describing nonstandard situations. The focus was on the temperature/chemical potential phase diagram of QCD, considered both analytically and with lattice gauge theory, equilibrium and nonequilibrium thermo field theory, and on heavy ion physics. Other related topics were "small x physics" in QCD, electroweak baryogenesis, inflation, and dark energy in the early universe. | ||
650 | |a Nuclear matter,Nuclear reactions,Electroweak interactions,Strong interactions (Nuclear physics),Nuclear astrophysics | ||
904 | |i Bạch Trúc | ||
980 | |a Trung tâm Học liệu Trường Đại học Cần Thơ |