Connection between the Reference Parameter Input Library RIPL, GND and nuclear reaction evaluations

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Connection between the Reference Parameter Input Library RIPL, GND and nuclear reaction evaluations Arjan Koning NRG Petten, the Netherlands WPEC SG38 Meeting, OECD/NEA Data Bank May 21-22 2013, Issy-les-Moulineaux

RIPL: The result of 3 IAEA CRP s 2

RIPL segments 1. Masses 2. Discrete levels 3. Neutron resonances 4. Optical model 5. Level densities 6. Gamma-ray strength functions 7. Fission All of these segments are important for nuclear model codes Some of these segments are important for a particle database. Recommendation: force link of particle database with nuclear reaction evaluation Recommendation: try to work with defaults that can be overruled Warning: Unification of the RIPL format has been recommended before by a RIPL-participant. Maybe the time is right now! 3

Masses Everyone (I think) agrees we should adopt experimental masses from the Atomic Mass Evaluation, when available People, especially astrophysicists, disagree on theoretical masses (FRDM, HFB models, Duflo-Zuker formula). RIPL also stores relative isotopic abundances = BNL Nuclear Wallet Cards. Link with nuclear reaction evaluations (NRE): Agree on the (RIPL) default: if no mass is given in the NRE, link to the particle database Allow to overrule default mass choice in NRE. Should Q-values remain implicit (are completely determined by mass choice) or be explicit in an NRE? How to deal with old masses from ENDF-B, JEFF, JENDL, etc.? Any new evaluation made with (at least) TALYS or EMPIRE, uses consistent RIPL values for masses 4

Discrete levels There is one generally adopted source for discrete level information, ENSDF, and in RIPL this is translated into a discrete level database. Unfortunately, less well-defined, or well-agreed, than masses: Unknown energies Unknown spins and parities Unknown branching ratios ~10 units away from stability line: no info at all Do we get halflives from here or from the Decay Data File? Filling these omissions for nuclear reaction evaluations is subjective, e.g. TALYS uses HFB level densities to fill it all. Existing nuclear reaction evaluations often disagree on the level energy and number (!) Can/should we impose the RIPL default on this? 5

Neutron resonance parameters Direct connection with current MF2, also for the average resonance parameters. Evaluators will disagree more than for masses and discrete levels Outside RIPL: bring The Atlas of Neutron Resonances also under the GND umbrella. 6

Optical model parameters All OMP parameterizations must first be used in nuclear model calculations, so no direct link with format issues of nuclear reaction evaluations. Bringing OMP parameters under GND umbrella may be difficult since special software is required to retrieve the parameters. 7

Level density parameters All these parameterizations must first be used in nuclear model calculations, so no direct link with format issues of nuclear reaction evaluations. All tables can be brought under GND umbrella, either for level density parameters or tabulated level densities. 8

Gamma-ray strength functions All these parameterizations must first be used in nuclear model calculations, so no direct link with format issues of nuclear reaction evaluations. All tables can be brought under GND umbrella, either for gamma-ray parameters or tabulated gamma-ray strength functions. 9

Fission parameters All these parameterizations must first be used in nuclear model calculations, so no direct link with format issues of nuclear reaction evaluations. All tables can be brought under GND umbrella, either for fission parameters or tabulated fission level densities, etc. 10

Conclusions - Try to bring large nuclear-structure related databases under GND umbrella: RIPL, Atlas, Radioactive Decay Data file, NUBASE etc. - This will allow users to choose from a variety of sources without (?) caring about read formats. - Question for the link to nuclear reaction evaluations: should we establish defaults for (almost) everything to minimize errors? ( a bit like a TALYS input file..) 11