000			01647 a2200217 4500
005			20181217152245.0
008			181213b xxu||||| |||| 00| 0 eng d
020			_a9789813273313
040			_cIIT Kanpur
041			_aeng
082			_a571.66 _bM11e
100			_aMa, Yong-Liang
245			_aEffective field theories for nuclei and compact-star matter _bChiral Nuclear Dynamics (CND-lll) _cYong - Liang Ma and Mannque Rho
260			_bWorld Scientific Publishing _c2019 _aLondon
300			_axvii, 359p.
520			_aEffective 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			_aField theory
650			_aQuantum chromodynamics
700			_aRho, Mannque
942			_cBK
999			_c559891 _d559891