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Effective field theories for nuclei and compact-star matter[electronic resource] :chiral nuclear dynamics (CND-III) /

紀錄類型:	書目-電子資源 : Monograph/item
杜威分類號:	530.14
書名/作者:	Effective field theories for nuclei and compact-star matter : chiral nuclear dynamics (CND-III) // Yong-Liang Ma, Mannque Rho.
作者:	Ma, Yong-Liang.
其他作者:	Rho, Mannque.
出版者:	Singapore : : World Scientific,, c2019.
面頁冊數:	1 online resource (378 p.) : : ill. (some col.)
標題:	Field theory (Physics)
標題:	Quantum chromodynamics.
標題:	Compact objects (Astronomy)
標題:	Electronic books.
ISBN:	9789813273320
書目註:	Includes bibliographical references (p. 339-355) and index.
摘要、提要註:	"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."--
電子資源:	https://www.worldscientific.com/worldscibooks/10.1142/11072#t=toc

Effective field theories for nuclei and compact-star matter[electronic resource] :chiral nuclear dynamics (CND-III) /
Ma, Yong-Liang.

Effective field theories for nuclei and compact-star matterchiral nuclear dynamics (CND-III) /[electronic resource] :Yong-Liang Ma, Mannque Rho. - 1st ed. - Singapore :World Scientific,c2019. - 1 online resource (378 p.) :ill. (some col.)

Includes bibliographical references (p. 339-355) and index.

"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."--

Electronic reproduction.
Singapore :
World Scientific,
[2018]

Mode of access: World Wide Web.

ISBN: 9789813273320Subjects--Topical Terms:

471016
Field theory (Physics)

LC Class. No.: QC173.7 / .M3 2019

Dewey Class. No.: 530.14

Effective field theories for nuclei and compact-star matter[electronic resource] :chiral nuclear dynamics (CND-III) /
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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."-- $c Publisher's website.
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