Chiral nuclear dynamics II: from quarks to nuclei to compact stars
Gespeichert in:
| 1. Verfasser: | |
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| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Singapore
World Scientific
c2008
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| Schlagworte: | |
| Online-Zugang: | FAW01 FAW02 Volltext |
| Beschreibung: | "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. - "2nd edition."--T.p. verso Includes bibliographical references (p. 335-348) and index 1. Introduction -- 2. Multi-facets of QCD in matter -- 3. Cheshire cat phenomenon. 3.1. Motivation. 3.2. Chiral bag picture. 3.3. Cheshire cat principle in nature. 3.4. CCP and multi-facets of CBM -- 4. Effective field theory for nuclei. 4.1. Role of effective field theory in nuclear physics. 4.2. Standard nuclear physics approach and EFT. 4.3. Chiral lagrangians. 4.4. Pionless EFT ([symbol]/EFT). 4.5. More effective EFT. 4.6. EFT "Completion" of SNPA. 4.7. EFT for heavy nuclei and nuclear matter -- 5. Hidden local symmetry for hadrons. 5.1. Emergence of local flavor symmetry. 5.2. Tower of hidden gauge fields. 5.3. AdS/QCD and hQCD. 5.4. HLS[symbol]from holographic dual QCD. 5.5. Hidden local symmetry and the "vector manifestation". 5.6. Phenomenology with HLS[symbol]. 5.7. HLS with [symbol] and a[symbol]: HLS[symbol] -- - 6. Skyrmions. 6.1. Preliminary remarks. 6.2. Skyrmions in QCD. 6.3. Skyrmions and vector mesons. 6.4. Dense skyrmion matter and chiral transition. 6.5. Holographic skyrmion. 6.6. Neutron stars as giant skyrmions -- 7. Hidden local symmetry in hot/dense medium. 7.1. HLS in heat bath. 7.2. HLS in dense matter. 7.3. Hadronic freedom. 7.4. Applications -- 8. Hadrons in the sliding vacua of nuclear matter. 8.1. Brown-Rho scaling. 8.2. Chiral fermi liquid. 8.3. Observables in finite nuclei. 8.4. Dropping masses and nuclear matter -- 9. Strangeness In dense medium. 9.1. Kaon condensation from matter-free vacuum. 9.2. From the vector manifestation fixed point to kaon condensation. 9.3. Dense kaonic nuclei as strange nuggets: "KaoN" -- 10. Dense matter for compact stars. 10.1. Dense hadronic phase with and without exotica. 10.2. Skyrmion-half-skyrmion transition. 10.3. QCD at high density: Color Superconductivity (CSC). 10.4. CSC at non-asymptotic density -- - 11. Compact stars. 11.1. Objective. 11.2. Star observables. 11.3. Chiral dynamics in the core of compact stars. 11.4. Maximum neutron star mass. 11.5. Formation of double neutron star binaries. 11.6. Neutron stars heavier than M[symbol]. 11.7. Outlook 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 |
| Beschreibung: | 1 Online-Ressource (xix, 352 p.) |
| ISBN: | 1281968153 9781281968159 9789812705884 9789812814746 9812705880 9812814744 |
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| 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. - "2nd edition."--T.p. verso | ||
| 500 | |a Includes bibliographical references (p. 335-348) and index | ||
| 500 | |a 1. Introduction -- 2. Multi-facets of QCD in matter -- 3. Cheshire cat phenomenon. 3.1. Motivation. 3.2. Chiral bag picture. 3.3. Cheshire cat principle in nature. 3.4. CCP and multi-facets of CBM -- 4. Effective field theory for nuclei. 4.1. Role of effective field theory in nuclear physics. 4.2. Standard nuclear physics approach and EFT. 4.3. Chiral lagrangians. 4.4. Pionless EFT ([symbol]/EFT). 4.5. More effective EFT. 4.6. EFT "Completion" of SNPA. 4.7. EFT for heavy nuclei and nuclear matter -- 5. Hidden local symmetry for hadrons. 5.1. Emergence of local flavor symmetry. 5.2. Tower of hidden gauge fields. 5.3. AdS/QCD and hQCD. 5.4. HLS[symbol]from holographic dual QCD. 5.5. Hidden local symmetry and the "vector manifestation". 5.6. Phenomenology with HLS[symbol]. 5.7. HLS with [symbol] and a[symbol]: HLS[symbol] -- | ||
| 500 | |a - 6. Skyrmions. 6.1. Preliminary remarks. 6.2. Skyrmions in QCD. 6.3. Skyrmions and vector mesons. 6.4. Dense skyrmion matter and chiral transition. 6.5. Holographic skyrmion. 6.6. Neutron stars as giant skyrmions -- 7. Hidden local symmetry in hot/dense medium. 7.1. HLS in heat bath. 7.2. HLS in dense matter. 7.3. Hadronic freedom. 7.4. Applications -- 8. Hadrons in the sliding vacua of nuclear matter. 8.1. Brown-Rho scaling. 8.2. Chiral fermi liquid. 8.3. Observables in finite nuclei. 8.4. Dropping masses and nuclear matter -- 9. Strangeness In dense medium. 9.1. Kaon condensation from matter-free vacuum. 9.2. From the vector manifestation fixed point to kaon condensation. 9.3. Dense kaonic nuclei as strange nuggets: "KaoN" -- 10. Dense matter for compact stars. 10.1. Dense hadronic phase with and without exotica. 10.2. Skyrmion-half-skyrmion transition. 10.3. QCD at high density: Color Superconductivity (CSC). 10.4. CSC at non-asymptotic density -- | ||
| 500 | |a - 11. Compact stars. 11.1. Objective. 11.2. Star observables. 11.3. Chiral dynamics in the core of compact stars. 11.4. Maximum neutron star mass. 11.5. Formation of double neutron star binaries. 11.6. Neutron stars heavier than M[symbol]. 11.7. Outlook | ||
| 500 | |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 | ||
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| 650 | 4 | |a Particles (Nuclear physics) |x Chirality | |
| 650 | 4 | |a Quantum chromodynamics | |
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Datensatz im Suchindex
| _version_ | 1804175458103721984 |
|---|---|
| any_adam_object | |
| author | Rho, Mannque |
| author_facet | Rho, Mannque |
| author_role | aut |
| author_sort | Rho, Mannque |
| author_variant | m r mr |
| building | Verbundindex |
| bvnumber | BV043073053 |
| collection | ZDB-4-EBA |
| ctrlnum | (OCoLC)696629748 (DE-599)BVBBV043073053 |
| dewey-full | 539.754822 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 539 - Modern physics |
| dewey-raw | 539.7548 22 |
| dewey-search | 539.7548 22 |
| dewey-sort | 3539.7548 222 |
| dewey-tens | 530 - Physics |
| discipline | Physik |
| format | Electronic eBook |
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| id | DE-604.BV043073053 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T07:16:36Z |
| institution | BVB |
| isbn | 1281968153 9781281968159 9789812705884 9789812814746 9812705880 9812814744 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-028497245 |
| oclc_num | 696629748 |
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| owner_facet | DE-1046 DE-1047 |
| physical | 1 Online-Ressource (xix, 352 p.) |
| psigel | ZDB-4-EBA ZDB-4-EBA FAW_PDA_EBA |
| publishDate | 2008 |
| publishDateSearch | 2008 |
| publishDateSort | 2008 |
| publisher | World Scientific |
| record_format | marc |
| spelling | Rho, Mannque Verfasser aut Chiral nuclear dynamics II from quarks to nuclei to compact stars Mannque Rho Singapore World Scientific c2008 1 Online-Ressource (xix, 352 p.) txt rdacontent c rdamedia cr rdacarrier "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. - "2nd edition."--T.p. verso Includes bibliographical references (p. 335-348) and index 1. Introduction -- 2. Multi-facets of QCD in matter -- 3. Cheshire cat phenomenon. 3.1. Motivation. 3.2. Chiral bag picture. 3.3. Cheshire cat principle in nature. 3.4. CCP and multi-facets of CBM -- 4. Effective field theory for nuclei. 4.1. Role of effective field theory in nuclear physics. 4.2. Standard nuclear physics approach and EFT. 4.3. Chiral lagrangians. 4.4. Pionless EFT ([symbol]/EFT). 4.5. More effective EFT. 4.6. EFT "Completion" of SNPA. 4.7. EFT for heavy nuclei and nuclear matter -- 5. Hidden local symmetry for hadrons. 5.1. Emergence of local flavor symmetry. 5.2. Tower of hidden gauge fields. 5.3. AdS/QCD and hQCD. 5.4. HLS[symbol]from holographic dual QCD. 5.5. Hidden local symmetry and the "vector manifestation". 5.6. Phenomenology with HLS[symbol]. 5.7. HLS with [symbol] and a[symbol]: HLS[symbol] -- - 6. Skyrmions. 6.1. Preliminary remarks. 6.2. Skyrmions in QCD. 6.3. Skyrmions and vector mesons. 6.4. Dense skyrmion matter and chiral transition. 6.5. Holographic skyrmion. 6.6. Neutron stars as giant skyrmions -- 7. Hidden local symmetry in hot/dense medium. 7.1. HLS in heat bath. 7.2. HLS in dense matter. 7.3. Hadronic freedom. 7.4. Applications -- 8. Hadrons in the sliding vacua of nuclear matter. 8.1. Brown-Rho scaling. 8.2. Chiral fermi liquid. 8.3. Observables in finite nuclei. 8.4. Dropping masses and nuclear matter -- 9. Strangeness In dense medium. 9.1. Kaon condensation from matter-free vacuum. 9.2. From the vector manifestation fixed point to kaon condensation. 9.3. Dense kaonic nuclei as strange nuggets: "KaoN" -- 10. Dense matter for compact stars. 10.1. Dense hadronic phase with and without exotica. 10.2. Skyrmion-half-skyrmion transition. 10.3. QCD at high density: Color Superconductivity (CSC). 10.4. CSC at non-asymptotic density -- - 11. Compact stars. 11.1. Objective. 11.2. Star observables. 11.3. Chiral dynamics in the core of compact stars. 11.4. Maximum neutron star mass. 11.5. Formation of double neutron star binaries. 11.6. Neutron stars heavier than M[symbol]. 11.7. Outlook 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 TECHNOLOGY & ENGINEERING / Power Resources / Nuclear bisacsh Particles (Nuclear physics) Chirality Quantum chromodynamics Chirale Symmetrie (DE-588)4274371-0 gnd rswk-swf Elementarteilchen (DE-588)4014413-6 gnd rswk-swf Elementarteilchen (DE-588)4014413-6 s Chirale Symmetrie (DE-588)4274371-0 s 1\p DE-604 Nowak, Maciej A. Sonstige oth World Scientific Sonstige oth http://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&db=nlabk&AN=518599 Aggregator Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Rho, Mannque Chiral nuclear dynamics II from quarks to nuclei to compact stars TECHNOLOGY & ENGINEERING / Power Resources / Nuclear bisacsh Particles (Nuclear physics) Chirality Quantum chromodynamics Chirale Symmetrie (DE-588)4274371-0 gnd Elementarteilchen (DE-588)4014413-6 gnd |
| subject_GND | (DE-588)4274371-0 (DE-588)4014413-6 |
| title | Chiral nuclear dynamics II from quarks to nuclei to compact stars |
| title_auth | Chiral nuclear dynamics II from quarks to nuclei to compact stars |
| title_exact_search | Chiral nuclear dynamics II from quarks to nuclei to compact stars |
| title_full | Chiral nuclear dynamics II from quarks to nuclei to compact stars Mannque Rho |
| title_fullStr | Chiral nuclear dynamics II from quarks to nuclei to compact stars Mannque Rho |
| title_full_unstemmed | Chiral nuclear dynamics II from quarks to nuclei to compact stars Mannque Rho |
| title_short | Chiral nuclear dynamics II |
| title_sort | chiral nuclear dynamics ii from quarks to nuclei to compact stars |
| title_sub | from quarks to nuclei to compact stars |
| topic | TECHNOLOGY & ENGINEERING / Power Resources / Nuclear bisacsh Particles (Nuclear physics) Chirality Quantum chromodynamics Chirale Symmetrie (DE-588)4274371-0 gnd Elementarteilchen (DE-588)4014413-6 gnd |
| topic_facet | TECHNOLOGY & ENGINEERING / Power Resources / Nuclear Particles (Nuclear physics) Chirality Quantum chromodynamics Chirale Symmetrie Elementarteilchen |
| url | http://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&db=nlabk&AN=518599 |
| work_keys_str_mv | AT rhomannque chiralnucleardynamicsiifromquarkstonucleitocompactstars AT nowakmacieja chiralnucleardynamicsiifromquarkstonucleitocompactstars AT worldscientific chiralnucleardynamicsiifromquarkstonucleitocompactstars |