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Effective field theories for nuclei ...

Ma, Yong-Liang.

Effective field theories for nuclei and compact-star matterchiral nuclear dynamics (CND-III) /

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Effective field theories for nuclei and compact-star matterYong-Liang Ma, Mannque Rho.
其他題名:	chiral nuclear dynamics (CND-III) /
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)
電子資源:	https://www.worldscientific.com/worldscibooks/10.1142/11072#t=toc
ISBN:	9789813273320$q(electronic bk.)

Effective field theories for nuclei and compact-star matterchiral 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: 9789813273320$q(electronic bk.)Subjects--Topical Terms:

208085
Field theory (Physics)

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

Dewey Class. No.: 530.14

Effective field theories for nuclei and compact-star matterchiral nuclear dynamics (CND-III) /
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300 $a 1 online resource (378 p.) : $b ill. (some col.)
504 $a Includes bibliographical references (p. 339-355) and index.
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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