3rd Rencontre PhyNuBE: Fission and Nuclear Astrophysics

Europe/Paris
Village CNRS Oléron (France)

Village CNRS Oléron (France)

Village vacances du CAES du CNRS La Vieille Perrotine 17310 Saint-Pierre d'Oléron
Fairouz HAMMACHE (IPN-Orsay), Beatriz Jurado (IN2P3/CENBG), Denis LACROIX (Institut de Physique Nucléaire), Antoine Lemasson (GANIL / CNRS UPR3266), Guillaume Scamps (L2i Toulouse, CNRS/IN2P3, UT3), sorlin olivier (GANIL)
Description

 

The third edition of PhyNuBE of the Groupement de Recherche Resanet will take place at the CNRS center of Oléron (France) between October 6 (arrival) and October 11 (departure). We propose to adress two scientific topics that are nuclear astrophysics and nuclear fission. The meeting will comprise a series of invited overview talks, oral contributions and poster presentations.

 

The PhyNuBe scientific meetings are intended to gather and educate students and senior scientists around major scientific topics of our field, as well as reinforcing links between theory and experiment and encouraging cross-fertilize activities. 

 

The astrophysics part will cover quiescent and explosive burning phases of stars in which nuclear physics plays an essential role, such as massive stars, novae, x-ray bursts, or neutron star mergers. Theoretical aspects of stellar modeling, nuclear reaction rates, and spectroscopy will be covered. Experimentally, results from reaction cross-section measurements of astrophysical relevance involving neutral, charged particles and neutrinos will be presented and confronted to observations.

Concerning fission,  the most relevant experimental programs for measuring fission cross sections, probabilities, fission fragment properties, and the associated emitted particles will be discussed, thus highlighting the related challenges, the solutions provided, and the main results. The advances and challenges in fission theory will also be covered by discussing the latest developments in microscopic dynamical models based on the energy density functional theory and in more phenomenological models. The various talks will also illustrate the importance of the fission process for fundamental nuclear physics, societal applications, and nuclear astrophysics.

A large amount of time will be dedicated to discussions and debates, as well as outdoor activities. Finantial support for local expenses is possible on demand for a limited number of participants. Fees are estimated to 550 euros for a sinle room and 440 euros in twin rooms with double occupancy, both for full board. Bus shuttles are planned to be organized between the train station of La Rochelle and the CNRS center of Oléron. Departures of these shuttles are planned on October 06 and October 11, synchronized with the TGV trains between Paris and La Rochelle (see file 'last announcement' at the bottom of the website for details).

 

Submission abstract: May 4th to July 15th 

Notification of acceptance of abstracts: July 22nd

Registration deadline: August, 31st

 

The PhyNuBE3 meeting is organized under the umbrella of the GDR Resanet by F. Hammache, B. Jurado, D. Lacroix, A. Lemasson, G. Scamps and O. Sorlin.

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Registration
    • 21:00 21:30
      Meeting between organizing committee and students 30m
    • 08:25 08:35
      Welcome Session
    • 08:35 09:35
      Introduction to the r-process nucleosynthesis 1h
      Orateur: Stéphane Goriely (ULB, Bruxelles Belgium)
    • 09:35 10:20
      Masses measurements for nuclear astrophysics 45m
      Orateur: Sara Naimi (IJCLab, Orsay, France)
    • 10:20 10:50
      Pause 30m
    • 10:50 11:35
      Reaction models for astrophysics 45m
      Orateur: Guillaume Hupin (IJClab, Orsay, France)
    • 11:35 12:00
      Discussions
    • 12:00 16:00
      Lunch
    • 16:00 16:50
      Introduction to experiments on nuclear fission P1 50m
      Orateur: Beatriz Jurado (LP2I, Bordeaux, France)
    • 16:50 17:40
      Introduction to the theory of nuclear fission P1 50m
      Orateur: David Regnier (CEA/DAM, Bruyères-le-Châtel, France)
    • 17:40 18:10
      Pause 30m
    • 18:10 18:55
      Fission cross sections, evaluations and measurements 45m
      Orateur: Pierre Tamagno (CEA, Cadarache, France)
    • 18:55 19:15
      Discussions
    • 08:30 09:20
      Introduction to the theory of nuclear fission P2 50m
      Orateur: David Regnier (CEA/DAM, Bruyères-le-Châtel, France)
    • 09:20 10:10
      Introduction to experiments on nuclear fission P2 50m
      Orateur: Beatriz Jurado (LP2I, Bordeaux, France)
    • 10:10 10:40
      Pause 30m
    • 10:40 11:15
      Measurements in inverse kinematics around the Coulomb Barrier at VAMOS 35m
      Orateur: Diego Ramos (GANIL, Caen, France)
    • 11:15 12:00
      Microscopic description of nuclear fission: Recent advances in the TDGCM approach 45m
      Orateur: Nathalie Pillet (CEA/DAM, Bruyères-le-Châtel, France)
    • 12:00 12:20
      Discussions
    • 12:20 15:45
      Lunch 3h 25m
    • 15:45 16:30
      Massive stars modelling: Evolution and nucleosynthesis 45m
      Orateur: Thibaut Dumont (IPHC, Strasbourg, France)
    • 16:30 16:45
      Pause
    • 16:45 17:30
      Direct Measurements of Fusion Reactions of Astrophysics Impact 45m
      Orateur: Marcel Heine (IPHC, Strasbourg, France)
    • 17:30 18:00
      Coincidence measurements of fusion reactions involving carbon and oxygen with the high-precision STELlar LAboratory (STELLA) 30m
      Orateur: Aurélie Bonhomme (IPHC, Strasbourg, France)
    • 18:00 19:30
      Poster Session
    • 08:30 09:15
      The fundamental role of fission during r-process nucleosynthesis 45m
      Orateur: Stéphane Goriely (ULB, Bruxelles Belgium)
    • 09:15 10:00
      The intermediate neutron capture process 45m
      Orateur: Arthur Choplin (ULB, Bruxelles Belgium)
    • 10:00 10:30
      Pause 30m
    • 10:30 11:15
      Neutron sources for the s-process and their experimental study 45m
      Orateur: Fairouz Hammache (IJCLab, Orsay, France)
    • 11:15 11:55
      Study of Pigmy Dipole resonances and their potential roles in nuclear astrophysics 40m
      Orateur: Iolanda Matea (IJCLab, Orsay, France)
    • 11:55 12:15
      Pause: Discussions
    • 12:15 16:00
      Lunch 3h 45m
    • 16:00 16:45
      State of the art on new region around neutron deficient Pb 45m
      Orateur: Christelle Schmitt (IPHC, Strasbourg, France)
    • 16:45 17:15
      Pause 30m
    • 17:15 18:00
      Structure and angular momentum at scission from microscopic models 45m
      Orateur: Guillaume Scamps (L2I Toulouse, France)
    • 18:00 18:30
      Angular momentum and excitation energy of 120Cd/132Sn, 118Pd/134Te neutronless fragmentations in 252Cf(sf) 30m
      Orateur: Alexis Francheteau (GANIL, Caen, France)
    • 18:30 19:00
      Pause: Discussions
    • 08:30 09:15
      Fission-fragment de-excitation as a fission probe 45m
      Orateur: Dr Jon Wilson (IJClab, Orsay, France)
    • 09:15 09:50
      Fission in heavy ion storage ring 35m
      Orateur: Boguslaw Wloch (LP2I, Bordeaux, France)
    • 09:50 10:20
      Pause 30m
    • 10:20 10:45
      Fission studies at at NFS with SCONE 25m

      Fission modeling is still the subject of much work. The objective is to understand the structure and dynamic effects involved in this reaction. From the point of view of fission applications, the objective is to provide precise data on the fission fragments yields and kinetic energies, but also on the emission of neutrons and γ-rays. The work being carried out in numerous laboratories ultimately aims to enable the provision of such data based on theories or phenomenological models. In this presentation I will describe the new results obtained with the large SCONE detector (Solid COunter for NEutrons), based on plastic scintillator bars. The detector design includes a significant amount of Gd, in order to carry out neutron counting with an efficiency of about 70 percent for fission neutrons. In addition, by design, SCONE is also a good γ-ray calorimeter, and in particular the granularity allows to determine the average γ-ray multiplicities. I will present the experimental results of the fast neutron induced fission of uranium 238 campaign performed at the GANIL/NFS facility, for neutron energies ranging from 1 MeV to 30 MeV. The complete distributions of fission neutron multiplicities, the average total radiated γ-ray en ergy, and the average γ-ray multiplicity in the fast neutron induced fission of uranium 238 will be discussed. Furthermore, measuring the different observables continuously as a function of neutron energy makes it possible to study the effects of multi-chances which confer structures into those observables. For the first time the second chance fission probability on uranium 238 was mea- sured experimentally. In a ddition, the re-analysis of old data on uranium 235 and plutonium 239 allowed us to obtain the aforementioned probability also for these two isotopes. These measure- ments open a way to take into account the effects of multi-chance in fission, that overcomplicate the description of the neutron induced fission process. Unfolding these effects will simplify the achievement of more precise models.

      Orateur: Gilbert Bélier (CEA, DAM, DIF)
    • 10:45 11:20
      Measurements in inverse kinematics at relativistic energies (SOFIA) 35m
      Orateur: Audrey Chatillon (CEA/DAM, Bruyères-le-Châtel, France)
    • 11:20 12:00
      Pause
    • 12:00 16:00
      Lunch 4h
    • 16:00 17:00
      Novae & X-ray burst modeling 1h
      Orateur: Jordi Jose (UPC, Barcelona, Spain)
    • 17:00 17:30
      Pause 30m
    • 17:30 18:15
      X-ray bursts studies using indirect methods 45m
      Orateur: Nicolas De Séréville (IJClab, Orsay, France)
    • 18:15 19:00
      Accessing explosive stellar nucleosynthesis from grounded laboratories 45m
      Orateur: Chloé Fougères (CEA/DAM, Bruyères-le-Châtel, France)
    • 19:00 19:20
      Pause
    • 09:00 09:20
      Discussion on Resanet activities 20m
    • 09:20 11:00
      Restitution/Conclusions