|
|
|
|
| LEADER |
00000cam a22000004a 4500 |
| 001 |
7360067 |
| 005 |
20130308134400.0 |
| 008 |
090305s2008 si a b 001 0 eng c |
| 003 |
ICU |
| 010 |
|
|
|a 2009275808
|
| 020 |
|
|
|a 9812705880
|
| 020 |
|
|
|a 9789812705884
|
| 035 |
|
|
|a (OCoLC)141384778
|
| 035 |
|
|
|a om2254828
|
| 040 |
|
|
|a YDXCP
|b eng
|c YDX
|d DLC
|d BTCTA
|d BAKER
|d YDXCP
|d BWX
|d TXA
|d YOU
|d MUQ
|
| 042 |
|
|
|a pcc
|
| 049 |
|
|
|a CGUA
|
| 050 |
0 |
0 |
|a QC793.3.C54
|b R46 2008
|
| 100 |
1 |
|
|a Rho, Mannque.
|0 http://id.loc.gov/authorities/names/n78008860
|1 http://viaf.org/viaf/29594257
|
| 245 |
1 |
0 |
|a Chiral nuclear dynamics II :
|b from quarks to nuclei to compact stars /
|c Mannque Rho.
|
| 260 |
|
|
|a Singapore ;
|a Hackensack, NJ :
|b World Scientific,
|c c2008.
|
| 300 |
|
|
|a xix, 352 p. :
|b ill. ;
|c 23 cm.
|
| 336 |
|
|
|a text
|b txt
|2 rdacontent
|0 http://id.loc.gov/vocabulary/contentTypes/txt
|
| 337 |
|
|
|a unmediated
|b n
|2 rdamedia
|0 http://id.loc.gov/vocabulary/mediaTypes/n
|
| 338 |
|
|
|a volume
|b nc
|2 rdacarrier
|0 http://id.loc.gov/vocabulary/carriers/nc
|
| 500 |
|
|
|a "Sequel to the previous volume entitled 'Chiral nuclear dynamics' (CND-I for short) that I co-authored with Maciej Nowak and Ismail Zahed."--P. vii.
|
| 500 |
|
|
|a "2nd edition."--T.p. verso.
|
| 504 |
|
|
|a Includes bibliographical references (p. 335-348) and index.
|
| 505 |
0 |
0 |
|a 1. Introduction -- 2. Multi-Facets of QCD in Matter -- 3. Cheshire Cat Phenomenon -- 4. Effective Field Theory for Nuclei -- 5. Hidden Local Symmetry for Hadrons -- 6. Skyrmions -- 7. Hidden Local Symmetry in Hot/Dense Medium -- 8. Hadrons in the Sliding Vacua of Nuclear Matter -- 9. Strangeness in Dense Medium -- 10. Dense Matter for Compact Stars -- 11. Compact Stars.
|
| 520 |
|
|
|a This is the sequel to the first volume to treat in one effective field theory framework the physics of strongly interacting matter under extreme conditions. This is vital for understanding the high temperature phenomena taking place in relativistic heavy ion collisions and in the early Universe, as well as the high-density matter predicted to be present in compact stars. The underlying thesis is that what governs hadronic properties in a heat bath and/or a dense medium is hidden local symmetry which emerges from chiral dynamics of light quark systems and from the duality between QCD in 4D and bulk gravity in 5D as in AdS/QCD. Special attention is paid to hot matter relevant for relativistic heavy ion processes and to dense matter relevant for compact stars that are either stable or on the verge of collapse into black holes.
|
| 650 |
|
0 |
|a Particles (Nuclear physics)
|x Chirality.
|0 http://id.loc.gov/authorities/subjects/sh95003360
|
| 650 |
|
0 |
|a Quantum chromodynamics.
|0 http://id.loc.gov/authorities/subjects/sh85109458
|
| 650 |
|
6 |
|a Chiralité (Physique nucléaire)
|
| 650 |
|
6 |
|a Chromodynamique quantique.
|
| 650 |
|
7 |
|a Particles (Nuclear physics)
|x Chirality.
|2 fast
|0 http://id.worldcat.org/fast/fst01054132
|
| 650 |
|
7 |
|a Quantum chromodynamics.
|2 fast
|0 http://id.worldcat.org/fast/fst01085093
|
| 700 |
1 |
|
|a Nowak, Maciej A.
|t Chiral nuclear dynamics.
|
| 903 |
|
|
|a HeVa
|
| 929 |
|
|
|a cat
|
| 999 |
f |
f |
|i c8f607c3-0709-56d0-bb17-d772169e39cb
|s feaa4bfc-2492-5601-a706-7c525b802e12
|
| 928 |
|
|
|t Library of Congress classification
|a QC793.3.C54 R66 2008
|l ASR
|c ASR-SciASR
|i 5592069
|
| 927 |
|
|
|t Library of Congress classification
|a QC793.3.C54 R66 2008
|l ASR
|c ASR-SciASR
|e SHAP
|e CRERAR
|b 81197686
|i 8483490
|
