PPT-Equation of State of Neutron-Rich Matter in the Relativistic Mean-Field Approach

Farrukh J Fattoyev My TAMUC collaborators BA Li W G Newton My outside collaborators C J Horowitz J Piekarewicz G Shen J Xu Texas AampM UniversityCommerce International Workshop on Nuclear Dynamics and Thermodynamics. Ramesh Narayan. Jets are Widespread. Relativistic Jets . occur widely in . accreting black holes (BHs): AGN, XRBs, GRBs. A . common . robust . mechanism . must be producing all these . Jets. Best Bet. . In classical mechanics, the momentum of a particle is defined as a product of its mass and its velocity, . . In an isolated system of particles, with no net force acting on the system, the total momentum of the system remains the same. However , we can see from a simple though experiment that the quantity . Yuri . Lyubarsky. Ben-Gurion University. Beer-. Sheva. , Israel . Universality of . relativistic jets. M 87. M 87. Crab in X-rays. GRBs. t. ime, s. t. ime, s. PKS 2155-304 . Pulsar magnetosphere. Contents. Breakup reactions. of . 14. Be on a proton target. Inelastic scattering (. 14. Be). One-neutron removal reaction (. 13. Be). Y. Kondo. RIKEN . Nishina. Center. 2. Collaborators. Y. Kondo. Chang Ho Hyun. Panagiota. . Papakonstantinou. , . Yeunhwan. Lim, . Young-Ho Song, . Tae-Sun Park. 31th . Reimei. Workshop, Tokai, Japan. January 18, 2016 . Contents. Introduction. Old wisdom. Strategy. Marcella Grasso. Tribute to Daniel Gogny. Outline. Context: . Energy Density Functional . (EDF. ). . . theory. . Mean-field-based models. Beyond the mean field. : Which . interaction . to use? . . In classical mechanics, the momentum of a particle is defined as a product of its mass and its velocity, . . In an isolated system of particles, with no net force acting on the system, the total momentum of the system remains the same. However , we can see from a simple though experiment that the quantity . Mikhail E. . Gusakov. , . Vasiliy. A. . Dommes. Ioffe. Institute. Saint-Petersburg, Russia. Introduction. . It is generally accepted that baryons (neutrons and protons) in the internal layers of neutron stars undergo transition into superfluid/superconducting state at .. Lecture . 3. Books Recommended:. Lectures on Quantum Field Theory by Ashok Das. Advanced Quantum Mechanics by . Schwabl. Relativistic Quantum Mechanics by Greiner. . Quantum Field Theory by Mark . Srednicki. Lecture 4. Books Recommended:. Lectures on Quantum Field Theory by Ashok Das. Advanced Quantum Mechanics by . Schwabl. Relativistic Quantum Mechanics by Greiner. . Quantum Field Theory by Mark . Srednicki. Nuclear. Structure and . Reactions. : Building . Together. for the Future. 9 October 2017 GANIL. Present. . c. ollaborators. . along. . this. . research. line:. ENSAR2. , . JRA . TheoS. . (. Theoretical. Y. . Kanada-En’yo. (Kyoto Univ.). Lesson1: Introduction of cluster phenomena. Lesson2: . Antisymmetrized. molecular dynamics. Lesson3: . clustering in neutron-rich . Be. . 1. Important questions. .  . B. . What observables are sensitive to the EOS and at what densities. ?. 0. Astrophysical observables (neutron stars). . . 1. Binding energies . . 2. Radii of neutron and proton matter in nuclei . and . astrophysical . observations. David E. . Á. lvarez. . C. .. Sept 2013. S. . Kubis. , D. . Blaschke. and T. . Klaehn. The Modern Physics of Compact Stars and Relativistic Gravity. Outline. Introduction to neutron stars.