Hot Nuclear Matter Equation of State and Finite Temperature Kaon Condensation


Autoria(s): Li, A (Li Ang); Zuo, W (Zuo, Wei); Schulze, HJ (Schulze, H. J.); Lombardo, U (Lombardo, U.)
Data(s)

2008

Resumo

We perform a systematic calculation of the equation of state of asymmetric nuclear matter at finite temperature within the framework of the Brueckner-Hartree-Fock approach with a microscopic three-body force. When applying it to the study of hotka on condensed matter, we find that the thermal effect is more profound in comparison with normal matter, in particular around the threshold density. Also, the increase of temperature makes the equation of state slightly stiffer through suppression of kaon condensation.

National Natural Science Foundation of China 10575119 Knowledge Innovation Project of Chinese Academy of Sciences KJCX3-SYW-N2 European Commission CN/ASIA-LINK/008(94791)

Identificador

http://ir.impcas.ac.cn/handle/113462/5593

http://www.irgrid.ac.cn/handle/1471x/132387

Idioma(s)

英语

Fonte

Li, A (Li Ang); Zuo, W (Zuo, Wei); Schulze, HJ (Schulze, H. J.); Lombardo, U (Lombardo, U.) .Hot Nuclear Matter Equation of State and Finite Temperature Kaon Condensation,CHINESE PHYSICS LETTERS,2008,25 (12 ):4233-4236

Palavras-Chave #NEUTRON-STARS #PROTONEUTRON STARS #EVOLUTION #CHARGE
Tipo

期刊论文