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Effective Field Theories For Nuclei And Compact-star Matter: Chiral Nuclear Dynamics (Cnd-iii) (Hardcover)
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Effective Field Theories For Nuclei And Compact-star Matter: Chiral Nuclear Dynamics (Cnd-iii) (Hardcover)
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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.
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