NuSYM17 - Sciencesconf.org

›8:30 (2h)

Symmetry energy in nuclear structure 2
Marek Ploszajczak (GANIL, Caen, France)

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›8:30 (30min)

Collective excitations as probe of the nuclear effective interaction
Maria Colonna (Laboratori Nazionali del Sud, INFN, Catania, ITALY)

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›9:00 (25min)

Symmetry-motivated tuning effect in particle masses and nuclear data
Sergey Sukhoruchkin (Petersburg Kurchatov Institute, RUSSIA)

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›9:25 (20min)

Nuclear symmetry energy constrained by proton/cluster radioactivity
Xu Chang (Nanjing University, CHINA)

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›9:45 (20min)

Classical vs quantal effects in equilibrium and nonequilibrium dynamics
Hua Zheng (Laboratori Nazionali del Sud, INFN, Catania, ITALY)

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›10:05 (25min)

The 12C+12C and 12C+16O fusion reactions: clusters and astrophysics
Sandrine Courtin (Institut Pluridi. Hubert Curien, Strasbourg, FRANCE)

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›11:00 (1h30)

Transport codes comparison
Betty Tsang (NSCL, Michigan State University, East Lansing, USA)

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›11:00 (15min)

Current status of Transport code Evaluation project (TCEP)
Jun Xu (Shanghai Institute of Applied Physics, CHINA)

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›11:15 (35min)

Results of TCEP HW1 – NN collisions evaluation
YingXun Zhang (China Institute of Atomic Energy, CHINA)

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›11:50 (20min)

Status of HW 2 – Mean field evaluation
Maria Colonna (Laboratori Nazionali del Sud, INFN, Catania, ITALY)

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›12:10 (20min)

Status of HW3 – Pion Production
Akira Ono (Tohoku University Sendai, JAPAN)

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›14:00 (2h20)

Influence of the symmetry energy on the structure of objects and processes in the Femto and astrophysical scales 1
Anthea Fantina (GANIL, Caen, FRANCE)

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›14:00 (30min)

Inhomogeneity growth in two-component fermionic systems
Paolo Napolitani (IPN-Orsay, FRANCE)

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›14:30 (25min)

Fragmentation of Neutron Star Pasta
Claudio Dorso (FCEN, University of Buenos Aires, ARGENTINA)

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›14:55 (25min)

Empirical equation of state for dense nucleonic matter and predictions for NS properties
Francesca Gulminelli (Laboratoire de Physique Corpusculaire de Caen, FRANCE)

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›15:20 (25min)

Crust-core transition in neutron stars revisited
Xavier Vinas (Facultat de Física, Universitat de Barcelona, SPAIN)

›15:40 (20min)

A unified nuclear Equation of State based on empirical parameters constrained by nuclear observables
Debarati Chatterjee (Laboratoire de Physique Corpusculaire de Caen, FRANCE)

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›15:40 (20min)

A unified nuclear Equation of State based on empirical parameters constrained by nuclear observables
Debarati Chatterjee (Laboratoire de Physique Corpusculaire de Caen, FRANCE)

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›16:00 (20min)

The properties of symmetry energy in the saturated Nambu-Jona-Lasinio model
Wei Sina (Southeast University, Nanjing, CHINA)

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›16:50 (1h45)

Influence of the symmetry energy on the structure of objects and processes in the Femto and astrophysical scales 2
Jerzy Lukasik (Institute of Nuclear Physics PAN, POLAND)

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›16:50 (25min)

Geometric approach to pasta phases
Sebastian Kubis (Kraków University of Technology, POLAND)

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›17:15 (20min)

Density and momentum dependence of nuclear symmetry energy in the relativistic Hartree-Fock approximation
Tsuyoshi Miyatsu (Tokyo University of Science, JAPAN)

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›17:35 (20min)

How the structure of nuclei and neutron stars depends on the pressure of asymmetric nuclear matter
Kazuhiro Oyamatsu (Aichi Shukutoku University, JAPAN)

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›17:55 (20min)

Delta matter in asymmetric dense matter
Youngman Kim (Institute for Basic Science, Daejeon, SOUTH KOREA

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›18:15 (20min)

Effect of amplitude in compact star rotation by cosmological parameter
Shougaijam Singh (University of Delhi, INDIA)

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