A Criterion to Obtain the Equation of State of Asymmetric Nuclear Matter
スポンサーリンク
概要
- 論文の詳細を見る
A criterion to obtain the equation of state of asymmetric nuclear matter experimentally is discussed from the viewpoint of surface and asymmetry energies in neutron-rich nuclei. A simple analysis with a liquid-drop mass formula suggests that the proton fraction of a nucleus, Z/A, should be as small as 0.3. In the case of Ni isotopes, this corresponds to the neutron number N = 52 and the asymmetry energy per nucleon is 2 MeV. A preliminary result of a systematic study using a macroscopic nuclear model concerning the asymmetry energy is also briefly discussed.
- 2002-12-26
著者
-
Oyamatsu Kazuhiro
Department Of Media Production And Theories Aichi Shukutoku University
-
Oyamatsu Kazuhiro
Department Of Energy Engineering And Science Nagoya University
関連論文
- Development of an Advanced Startup Procedure for a PIUS-type Reactor
- Nonuniform Matter in Neutron Star Crusts Studied by the Variational Method with Thomas-Fermi Calculations(Nuclear Physics)
- Phenomenological Approach to Nuclei and Nuclear Matter(Nuclear Astrophysics,New Frontiers in QCD 2010-Exotic Hadron Systems and Dense Matter-)
- Equation of State of Nuclear Matter, Neutron Rich Nuclei in Laboratories and Pasta Nuclei in Neutron Star Crusts(Proceedings of the YITP Workshop on Nuclear Matter under Extreme Conditions)
- Further Study of the Nuclear Shape in High-Density Matter
- New Method for Calculating Aggregate Fission Product Decay Heat with Full Use of Macroscopic-Measurement Data
- Variational Calculation for the Equation of State of Nuclear Matter(International Workshop on Nuclear Structure-New Pictures in the Extended Isospin Space(NS07)-)
- Saturation of Nuclear Matter and Radii of Unstable Nuclei
- A Criterion to Obtain the Equation of State of Asymmetric Nuclear Matter
- A Criterion to Obtain the Equation of State of Asymmetric Nuclear Matter
- Exploring Neutron-Star Matter Using RI Beam
- Cluster Variation Method for Finite-Temperature Systems. II : Symmetric Nuclear Matter with a Central Potential
- Nonuniform Matter in Neutron Star Crusts Studied by the Variational Method with Thomas-Fermi Calculations
- Equation of State of Nuclear Matter, Neutron Rich Nuclei in Laboratories and Pasta Nuclei in Neutron Star Crusts(Proceedings of the YITP Workshop on Nuclear Matter under Extreme Conditions)