Effective Field Theories for Nuclei and Compact-Star Matter:Chiral Nuclear Dynamics (Cnd-III)

原子核和紧实恒星物质的有效场论:手性核动力学(CND-III)

原子核物理学

原   价:
1499.00
售   价:
1124.00
发货周期:预计3-5周发货
作      者
出  版 社
出版时间
2018年10月16日
装      帧
精装
ISBN
9789813273313
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页      码
380
语      种
英文
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图书简介
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. Key Features: ○Effective theories ○Emergence of hidden symmetries ○Topology change and hadron-quark continuity
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