Relativistic Mean Field Theory for Finite Nuclei Hiroshi

Relativistic Mean Field Theory for Finite Nuclei Hiroshi Toki 1/16/2022 Lecture in Osaka on Sept. 8, 2003

Relativistic mean field theory with TM 1 parameter Y. Sugahara and H. Toki Lagrangian Nucl. Phys. A 579 (1994) 557 7 free parameters TM 1 1/16/2022 Lecture in Osaka on Sept. 8, 2003

Dirac Equation 940 Me. V -350 Me. V 280 Me. V Three Body Force (Non-relativistic language) E 0 Three body 2(r/r 0)8/3 E= Me. V Spin-Orbit Force Mayer-Jensen (1949) 1/16/2022 630 Me. V Relativity produces strong three body repulsion Spin-orbit force comes from vector and scalar potential Lecture in Osaka on Sept. 8, 2003

1/16/2022 Lecture in Osaka on Sept. 8, 2003

1/16/2022 Lecture in Osaka on Sept. 8, 2003

Single particle energy TM 1 1/16/2022 Lecture in Osaka on Sept. 8, 2003

1/16/2022 Lecture in Osaka on Sept. 8, 2003

1/16/2022 Lecture in Osaka on Sept. 8, 2003

1/16/2022 Lecture in Osaka on Sept. 8, 2003

1/16/2022 Lecture in Osaka on Sept. 8, 2003

1/16/2022 Lecture in Osaka on Sept. 8, 2003

Equation of state 1/16/2022 Lecture in Osaka on Sept. 8, 2003

Neutron star Rho 0 The central density is about twice of rho 0. 1/16/2022 Lecture in Osaka on Sept. 8, 2003

Supernova explosion The prompt explosion is realized. We shall work out the neutrino reaction rates. 1/16/2022 Lecture in Osaka on Sept. 8, 2003