SCIENCE BRINGS NATIONS TOGETHER International Workshop "Infinite and Finite Nuclear Matter" (INFINUM)

20 Mar 2019, 07:00 → 22 Mar 2019, 17:00 Europe/Moscow

JINR BLTP

The interdisciplinary workshop "Infinite and Finite Nuclear Matter" (INFINUM) is considered as a platform offered to specialists in the physics of atomic nuclei, nuclear matter, heavy ion reactions and astrophysics for the exchange of experience in understanding properties of nuclear systems and nuclear interactions in various media. Scientific program is supposed to include topics of infinite dense matter relevant to neutron stars and heavy-ion collision (equation of state, superconductivity, liquid-gas phase transition, collision dynamics, etc.) and topics of finite nuclei, like structure, excitation energies, decays, energy-density functional, etc. One of the days of the workshop will be dedicated to the memory of our dear friend and colleague Eduard E. Saperstein (1939 - 2018) who made essential contributions to physics of finite Fermi systems.


Organizers:

N. Antonenko (JINR) – co-chairman
E. Kolomeitsev (JINR) – co-chairman
A. Dzhioev (JINR)
Yu. Ivanov (JINR)
S. Nedelko (JINR)
A. Friesen (JINR)
V. Voronin (JINR) — scientific secretary
O. Belova (JINR) — secretary.

Wednesday, 20 March

08:30 → 09:00 Registration

09:00 → 09:30 INFINUM. Introduction

Speaker: Evgeni Kolomeitsev (BLTP/Matej Bel Univ.)

Slides Kolomeitsev-Infinum.ppt

09:30 → 10:00 Cluster viral expansion for quark-nuclear matter

Speaker: David Blaschke (JINR Dubna)

Slides Blaschke-ClusterVirial_2019_Dubna.pdf

10:00 → 10:20 Coffee Break

10:20 → 11:00 Introduction to vorticity in HIC

Speaker: Yuri B. Ivanov (NRC "Kurchatov Institute")

Slides Dubna_20.03.2019-Ivanov.pdf

11:00 → 11:30 Relativistic mean-field models of neutron-star matter and nuclear liquid-gas phase transition

Speaker: Konstantin Maslov (NRNU MEPhI)

Slides Maslov-INFINUM19.pdf

11:30 → 13:00 Lunch

13:00 → 13:40 Advances in predicting nuclear matter at finite temperature

Speaker: Arianna Carbone (ECT*)

Slides Arianna_Dubna_March2019.pdf

13:40 → 14:20 Understanding extreme matter with gravitational waves

Speaker: Jérôme Margueron (IPN Lyon)

Slides 2019-03-Dubna-Margueron.pdf

14:20 → 14:40 Coffee Break

14:40 → 15:10 Close binary stars as source of energy in the universe

Speaker: Gurgen Adamian (BLTP, JINR)

Slides AdamianDubna2019.pdf

15:10 → 15:30 Specific features of spinning gravity and unification on the example of the Kerr-Newman spinning particle

Speaker: Alexander Burinskii (NSI, Russian Academy of Sciences)

Slides conf_talk_Dubna_INFINUM_2019_Burinskii.pdf

15:30 → 15:50 Role of gravitation in elementary particle structure

Speaker: Sergey Manaenkov (Petersburg Nuclear Physics Institute of National Research Centre "Kurchatov Institute")

Slides infinum-manaenkov-19.pdf

15:50 → 16:10 The symmetry energy in neutron stars: constraints from GW170817 and Direct Urca Cooling

Speaker: Dr David Edwin Alvarez Castillo (Joint Institute for Nuclear Research)

Slides Alvarez-Infinum-2019.pdf

Thursday, 21 March

09:00 → 09:30 Macroscopic and microscopic aspects of electron capture by polarized nuclei

Speaker: Alexey Barabanov (NRC "Kurchatov Institute")

Slides Barabanov_2019_03_21.pdf

09:30 → 10:10 Pion degrees of freedom in equilibrium and non-equilibrium nuclear systems

Speaker: Dmitry Voskresensky (NRNU MEPhI)

Slides Dubna2019_Saper_Voskresensky_fin1.pptx

10:10 → 10:30 Coffee Break

10:30 → 11:10 Beyond the mean field in the particle-vibration coupling scheme

Speaker: Marcello Baldo (INFN)

Slides talk_Baldo_Dubna_March_2019.pptx

11:10 → 11:40 Beta decay of very neutron-rich nuclei and Fayans density functional

Speaker: Ivan Borzov (NRC KI and JINR)

Slides Borzov-INFINUM_JINR_2.pptx

11:40 → 13:10 Lunch

13:10 → 13:40 Particle-hole dispersive optical model: unique features and new implementations

Speaker: Mikhail Urin (NRNU MEPhI)

Slides Urin_INFINUM2019.pdf

13:40 → 14:20 Flat bands, baryon asymmetry of Universe, and the violation of time-reversal symmetry

Speaker: Vasily Shaginyan (Petersburg Nuclear Physics Institute, NRC Kurchatov Institute)

Slides Shaginyan-Asym_Universe_PNPI_Dubna_2019.ppt

14:20 → 14:40 Coffe Break

14:40 → 15:10 Anharmonic effects in theory of finite Fermi- systems

Speaker: Sergey Kamerdzhiev (Kurchatov Institute)

15:10 → 15:40 Isotopic trends of nuclear surface properties of spherical nuclei

Speaker: Nikolai Antonenko (BLTP, JINR)

Slides AntonenkoINFINUM.pdf

15:40 → 16:10 Charge-exchange isobaric resonances and local interaction parameters

Speaker: Yuri Lutostansky

Slides +Lutotansky=Sap-2019.pdf

18:00 → 19:30 Banquet

Friday, 22 March

09:00 → 09:40 Single-particle spectral function of the Lambda hyperon in finite nuclei

Speaker: Isaac Vidana (INFN Catania)

Slides vidana.pdf

09:40 → 10:10 Charged-current neutrino opacities for supernova simulations with RPA correlations

Speaker: Alan Dzhioev (Joint Institute for Nuclear Research, Bogoliubov Laboratory of Theoretical Physics)

Slides Dzhioev_INFINUM2019.pdf

10:10 → 10:30 Coffee Break

10:30 → 11:00 Pion condensation in dense baryonic/quark matter with isospin and chiral imbalance

Speaker: Roman Zhokhov-Larionov (IHEP, IZMIRAN)

Slides Zhohov.pdf

11:00 → 11:30 Two-phonon structures of beta-decay rates

Speaker: Alexey Severyukhin (BLTP, JINR)

Slides SeveryukhinINFINUM2019.pdf

11:30 → 13:00 Lunch

13:00 → 13:30 Spreading widths of giant dipole resonance in the lead region

Speaker: Rashid Nazmitdinov (BLTP, JINR< Dubna)

13:30 → 14:00 Properties of isoscalar giant multipole resonances within a semimicroscopic model

Speaker: Mikhail Gorelik (MEPhI)

14:00 → 14:20 Coffee Break

14:20 → 14:50 Damping of giant resonances in open-shell nuclei: a semi-microscopic model

Speaker: Georgy Kolomiytsev (National Research Nuclear University "MEPhI" (Moscow Engineering Physics Institute))

14:50 → 15:20 Relation of toroidal and pygmy dipole resonances

Speaker: Valentin Nesterenko (BLTP, Joint Institute for Nuclear Research)

15:20 → 15:50 Properties and synthesis of magnetized nuclei

Speaker: Vladimir Kondratyev (BLTP)

15:50 → 16:10 Conclusion