Effective field theories for nuclei and compact-star matter: chiral nuclear dynamics (CND-III)
"Effective field theories have been widely used in nuclear physics. This volume is devoted to exploring the intricate structure of compact-star matter inaccessible directly from QCD. It is principally anchored on hidden symmetries and topology presumed to be encoded in QCD. It differs from stan...
Gespeichert in:
1. Verfasser: | |
---|---|
Format: | Elektronisch E-Book |
Sprache: | English |
Veröffentlicht: |
Singapore
World Scientific Publishing Company Pte Limited
2019
|
Schlagworte: | |
Online-Zugang: | UBY01 Volltext |
Zusammenfassung: | "Effective field theories have been widely used in nuclear physics. This volume is devoted to exploring the intricate structure of compact-star matter inaccessible directly from QCD. It is principally anchored on hidden symmetries and topology presumed to be encoded in QCD. It differs from standard effective field theory and energy density functional approaches in that it exploits renormalization-group flow in the complex "vacuum" sliding with density inferred from topology change identified as a manifestation of baryon-quark continuity in dense matter. It makes a variety of predictions that drastically differ from the conventional treatments that could be tested by upcoming terrestrial and astrophysical experiments. This monograph recounts how to go, in one unique field theoretic formalism in terms of hadronic degrees of freedom, from finite nuclei to dense compact-star matter that could be explored in RIB-type machines in nuclear physics as well as in LIGO-type gravity waves in astrophysics."-- |
Beschreibung: | Includes bibliographical references (pages 339-355) and index Notation and conventions -- Introduction -- The folk theorem in nuclear physics -- Hadron-quark continuity -- Effective field theories for nuclear interactions -- Hidden symmetries in dense matter -- Scale-chiral symmetry -- From skyrmions to dense matter -- Compressed baryonic matter -- Compact stars -- Strangeness in stars -- Epilogue |
Beschreibung: | 1 online resource (378 pages) illustrations (some color) |
ISBN: | 9789813273320 |
Internformat
MARC
LEADER | 00000nmm a2200000zc 4500 | ||
---|---|---|---|
001 | BV046810657 | ||
003 | DE-604 | ||
005 | 20201102 | ||
007 | cr|uuu---uuuuu | ||
008 | 200716s2019 |||| o||u| ||||||eng d | ||
020 | |a 9789813273320 |9 978-981-3273-32-0 | ||
024 | 7 | |a 10.1142/11072 |2 doi | |
035 | |a (ZDB-124-WOP)00011072 | ||
035 | |a (OCoLC)1190923369 | ||
035 | |a (DE-599)BVBBV046810657 | ||
040 | |a DE-604 |b ger |e rda | ||
041 | 0 | |a eng | |
049 | |a DE-706 | ||
082 | 0 | |a 530.14 | |
100 | 1 | |a Ma, Yong-Liang |4 aut | |
245 | 1 | 0 | |a Effective field theories for nuclei and compact-star matter |b chiral nuclear dynamics (CND-III) |c Yong-Liang Ma, Mannque Rho |
264 | 1 | |a Singapore |b World Scientific Publishing Company Pte Limited |c 2019 | |
300 | |a 1 online resource (378 pages) |b illustrations (some color) | ||
336 | |b txt |2 rdacontent | ||
337 | |b c |2 rdamedia | ||
338 | |b cr |2 rdacarrier | ||
500 | |a Includes bibliographical references (pages 339-355) and index | ||
500 | |a Notation and conventions -- Introduction -- The folk theorem in nuclear physics -- Hadron-quark continuity -- Effective field theories for nuclear interactions -- Hidden symmetries in dense matter -- Scale-chiral symmetry -- From skyrmions to dense matter -- Compressed baryonic matter -- Compact stars -- Strangeness in stars -- Epilogue | ||
520 | |a "Effective field theories have been widely used in nuclear physics. This volume is devoted to exploring the intricate structure of compact-star matter inaccessible directly from QCD. It is principally anchored on hidden symmetries and topology presumed to be encoded in QCD. It differs from standard effective field theory and energy density functional approaches in that it exploits renormalization-group flow in the complex "vacuum" sliding with density inferred from topology change identified as a manifestation of baryon-quark continuity in dense matter. It makes a variety of predictions that drastically differ from the conventional treatments that could be tested by upcoming terrestrial and astrophysical experiments. This monograph recounts how to go, in one unique field theoretic formalism in terms of hadronic degrees of freedom, from finite nuclei to dense compact-star matter that could be explored in RIB-type machines in nuclear physics as well as in LIGO-type gravity waves in astrophysics."-- | ||
650 | 4 | |a Field theory (Physics) | |
650 | 4 | |a Quantum chromodynamics | |
650 | 4 | |a Compact objects (Astronomy) | |
650 | 4 | |a Electronic books | |
700 | 1 | |a Rho, Mannque |e Sonstige |4 oth | |
776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe |z 9789813273313 |
776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe |z 9813273313 |
856 | 4 | 0 | |u https://www.worldscientific.com/worldscibooks/10.1142/11072 |x Verlag |z URL des Erstveröffentlichers |3 Volltext |
912 | |a ZDB-124-WOP | ||
999 | |a oai:aleph.bib-bvb.de:BVB01-032219220 | ||
966 | e | |u https://www.worldscientific.com/worldscibooks/10.1142/11072 |l UBY01 |p ZDB-124-WOP |x Verlag |3 Volltext |
Datensatz im Suchindex
_version_ | 1804181615877816320 |
---|---|
adam_txt | |
any_adam_object | |
any_adam_object_boolean | |
author | Ma, Yong-Liang |
author_facet | Ma, Yong-Liang |
author_role | aut |
author_sort | Ma, Yong-Liang |
author_variant | y l m ylm |
building | Verbundindex |
bvnumber | BV046810657 |
collection | ZDB-124-WOP |
ctrlnum | (ZDB-124-WOP)00011072 (OCoLC)1190923369 (DE-599)BVBBV046810657 |
dewey-full | 530.14 |
dewey-hundreds | 500 - Natural sciences and mathematics |
dewey-ones | 530 - Physics |
dewey-raw | 530.14 |
dewey-search | 530.14 |
dewey-sort | 3530.14 |
dewey-tens | 530 - Physics |
discipline | Physik |
discipline_str_mv | Physik |
format | Electronic eBook |
fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>03000nmm a2200445zc 4500</leader><controlfield tag="001">BV046810657</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">20201102 </controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">200716s2019 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789813273320</subfield><subfield code="9">978-981-3273-32-0</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1142/11072</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ZDB-124-WOP)00011072</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1190923369</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV046810657</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-706</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">530.14</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Ma, Yong-Liang</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Effective field theories for nuclei and compact-star matter</subfield><subfield code="b">chiral nuclear dynamics (CND-III)</subfield><subfield code="c">Yong-Liang Ma, Mannque Rho</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Singapore</subfield><subfield code="b">World Scientific Publishing Company Pte Limited</subfield><subfield code="c">2019</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 online resource (378 pages)</subfield><subfield code="b">illustrations (some color)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Includes bibliographical references (pages 339-355) and index</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Notation and conventions -- Introduction -- The folk theorem in nuclear physics -- Hadron-quark continuity -- Effective field theories for nuclear interactions -- Hidden symmetries in dense matter -- Scale-chiral symmetry -- From skyrmions to dense matter -- Compressed baryonic matter -- Compact stars -- Strangeness in stars -- Epilogue</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">"Effective field theories have been widely used in nuclear physics. This volume is devoted to exploring the intricate structure of compact-star matter inaccessible directly from QCD. It is principally anchored on hidden symmetries and topology presumed to be encoded in QCD. It differs from standard effective field theory and energy density functional approaches in that it exploits renormalization-group flow in the complex "vacuum" sliding with density inferred from topology change identified as a manifestation of baryon-quark continuity in dense matter. It makes a variety of predictions that drastically differ from the conventional treatments that could be tested by upcoming terrestrial and astrophysical experiments. This monograph recounts how to go, in one unique field theoretic formalism in terms of hadronic degrees of freedom, from finite nuclei to dense compact-star matter that could be explored in RIB-type machines in nuclear physics as well as in LIGO-type gravity waves in astrophysics."--</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Field theory (Physics)</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Quantum chromodynamics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Compact objects (Astronomy)</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Electronic books</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rho, Mannque</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druck-Ausgabe</subfield><subfield code="z">9789813273313</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druck-Ausgabe</subfield><subfield code="z">9813273313</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://www.worldscientific.com/worldscibooks/10.1142/11072</subfield><subfield code="x">Verlag</subfield><subfield code="z">URL des Erstveröffentlichers</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-124-WOP</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-032219220</subfield></datafield><datafield tag="966" ind1="e" ind2=" "><subfield code="u">https://www.worldscientific.com/worldscibooks/10.1142/11072</subfield><subfield code="l">UBY01</subfield><subfield code="p">ZDB-124-WOP</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield></record></collection> |
id | DE-604.BV046810657 |
illustrated | Illustrated |
index_date | 2024-07-03T14:58:49Z |
indexdate | 2024-07-10T08:54:29Z |
institution | BVB |
isbn | 9789813273320 |
language | English |
oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-032219220 |
oclc_num | 1190923369 |
open_access_boolean | |
owner | DE-706 |
owner_facet | DE-706 |
physical | 1 online resource (378 pages) illustrations (some color) |
psigel | ZDB-124-WOP |
publishDate | 2019 |
publishDateSearch | 2019 |
publishDateSort | 2019 |
publisher | World Scientific Publishing Company Pte Limited |
record_format | marc |
spelling | Ma, Yong-Liang aut Effective field theories for nuclei and compact-star matter chiral nuclear dynamics (CND-III) Yong-Liang Ma, Mannque Rho Singapore World Scientific Publishing Company Pte Limited 2019 1 online resource (378 pages) illustrations (some color) txt rdacontent c rdamedia cr rdacarrier Includes bibliographical references (pages 339-355) and index Notation and conventions -- Introduction -- The folk theorem in nuclear physics -- Hadron-quark continuity -- Effective field theories for nuclear interactions -- Hidden symmetries in dense matter -- Scale-chiral symmetry -- From skyrmions to dense matter -- Compressed baryonic matter -- Compact stars -- Strangeness in stars -- Epilogue "Effective field theories have been widely used in nuclear physics. This volume is devoted to exploring the intricate structure of compact-star matter inaccessible directly from QCD. It is principally anchored on hidden symmetries and topology presumed to be encoded in QCD. It differs from standard effective field theory and energy density functional approaches in that it exploits renormalization-group flow in the complex "vacuum" sliding with density inferred from topology change identified as a manifestation of baryon-quark continuity in dense matter. It makes a variety of predictions that drastically differ from the conventional treatments that could be tested by upcoming terrestrial and astrophysical experiments. This monograph recounts how to go, in one unique field theoretic formalism in terms of hadronic degrees of freedom, from finite nuclei to dense compact-star matter that could be explored in RIB-type machines in nuclear physics as well as in LIGO-type gravity waves in astrophysics."-- Field theory (Physics) Quantum chromodynamics Compact objects (Astronomy) Electronic books Rho, Mannque Sonstige oth Erscheint auch als Druck-Ausgabe 9789813273313 Erscheint auch als Druck-Ausgabe 9813273313 https://www.worldscientific.com/worldscibooks/10.1142/11072 Verlag URL des Erstveröffentlichers Volltext |
spellingShingle | Ma, Yong-Liang Effective field theories for nuclei and compact-star matter chiral nuclear dynamics (CND-III) Field theory (Physics) Quantum chromodynamics Compact objects (Astronomy) Electronic books |
title | Effective field theories for nuclei and compact-star matter chiral nuclear dynamics (CND-III) |
title_auth | Effective field theories for nuclei and compact-star matter chiral nuclear dynamics (CND-III) |
title_exact_search | Effective field theories for nuclei and compact-star matter chiral nuclear dynamics (CND-III) |
title_exact_search_txtP | Effective field theories for nuclei and compact-star matter chiral nuclear dynamics (CND-III) |
title_full | Effective field theories for nuclei and compact-star matter chiral nuclear dynamics (CND-III) Yong-Liang Ma, Mannque Rho |
title_fullStr | Effective field theories for nuclei and compact-star matter chiral nuclear dynamics (CND-III) Yong-Liang Ma, Mannque Rho |
title_full_unstemmed | Effective field theories for nuclei and compact-star matter chiral nuclear dynamics (CND-III) Yong-Liang Ma, Mannque Rho |
title_short | Effective field theories for nuclei and compact-star matter |
title_sort | effective field theories for nuclei and compact star matter chiral nuclear dynamics cnd iii |
title_sub | chiral nuclear dynamics (CND-III) |
topic | Field theory (Physics) Quantum chromodynamics Compact objects (Astronomy) Electronic books |
topic_facet | Field theory (Physics) Quantum chromodynamics Compact objects (Astronomy) Electronic books |
url | https://www.worldscientific.com/worldscibooks/10.1142/11072 |
work_keys_str_mv | AT mayongliang effectivefieldtheoriesfornucleiandcompactstarmatterchiralnucleardynamicscndiii AT rhomannque effectivefieldtheoriesfornucleiandcompactstarmatterchiralnucleardynamicscndiii |