Transition to Δ matter from hot, dense nuclear matter within a relativistic mean field formulation of the nonlinear σ and ω model

Zhuxia Li, Guangjun Mao, Yizhong Zhuo, and Walter Greiner
Phys. Rev. C 56, 1570 – Published 1 September 1997
PDFExport Citation

Abstract

An investigation of the transition to Δ matter is performed based on a relativistic mean field formulation of the nonlinear σ and ω model. We demonstrate that in addition to the Δ-meson coupling, the occurrence of the baryon resonance isomer also depends on the nucleon-meson coupling. Our results show that for the favored phenomenological value of m* and K, the Δ isomer exists at baryon density 2–3ρ0 if β=1.31 is adopted. For universal coupling of the nucleon and Δ, the Δ density at baryon density 2–3ρ0 and temperature 0.4–0.5 fm1 is about normal nuclear matter density, which is in accord with a recent experimental finding.

  • Received 9 January 1997

DOI:https://doi.org/10.1103/PhysRevC.56.1570

©1997 American Physical Society

Authors & Affiliations

Zhuxia Li1,2, Guangjun Mao2,3, Yizhong Zhuo1,2, and Walter Greiner3

  • 1China Institute of Atomic Energy, P.O. Box 275(18), Beijing 102413, People's Republic of China
  • 2Institute of Theoretical Physics, Academia Sinica, P.O. Box 2735, Beijing 100080, People's Republic of China
  • 3Institut für Theoretische Physik, Frankfurt University, D-60054 Frankfurt am Main, Germany

References (Subscription Required)

Click to Expand
Issue

Vol. 56, Iss. 3 — September 1997

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review C

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×