Tasting nuclear pasta made with classical molecuar dynamics simulations  

作　　者：Bao-An Li 

机构地区：[1]Department of Physics and Astronomy,Texas A&M University-Commerce,TX 75429-3011,USA

出　　处：《Frontiers of physics》2021年第2期115-117,共3页物理学前沿（英文版）

基　　金：B. A. Li is supported in part by the U.S.D epartm ent of Energy, Office of Science, under Award Number DESC0013702;the CUSTIPEN (China-U.S. Theory Institute for Physics with Exotic Nuclei) under the US D epartment of Energy Grant No. DE-SC0009971.

摘　　要：Nuclear clusters or voids in the inner crust of neutron stars were predicted to have various shapes collectively nicknamed nuclear pasta.The recent review in Ref.[1]by Lopez,Dorso and Frank summarized their systematic investigations into properties especially the mor-phological and thermodynamical phase transitions of the nuclear pasta within a Classical Molecular Dynamics model,providing further stimuli to find more observational evidences of the predicted nuclear pasta in neutron stars.

关 键 词：COLLECTIVE summarized TRANSITIONS 

分 类 号：O57[理学—粒子物理与原子核物理]