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Nuclear Structure Data Needs

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Title: Nuclear Structure Data Needs


1
Nuclear Structure Data Needs
  • Filip G. Kondev

kondev_at_anl.gov
Outline
  • What kind of nuclear structure and decay data
    are needed an incomplete list
  • Where to find the relevant data?
  • Suggestions on how to proceed in the future in
    order to update the corresponding nuclear
    astrophysics data libraries with the best
    available nuclear structure data?

Collaborative meeting, Trento, May 28 June 1,
2007
2
What NS data are needed?
  • Priority 1 masses decay data
  • masses, T1/2, decay modes BR and
    delayed-particle emission probabilities
  • Priority 2 level energies, quantum numbers,
    T1/2 of excited states, etc.
  • depends on the site of nucleosynthesis
  • s- and p-processes near the valley of
    stability a lot of data
  • rp-process at the proton-rich side
  • r-process - at the neutron-rich side much
    more data is expected in the future with the RIB
    facilities
  • important for model (cross-section) calculations
    level densities, partition functions, etc.
  • important when we are dealing with isomers
    cosmo-chronometers at the s-process path, but
    also many at the n-rich side
  • including the atomic (electron) environment?

3
Where to find the data ENSDF?
Effort within NSDD network, under auspices of
IAEA. Database is managed by NNDC (BNL)
Contents Evaluated nuclear structure and decay
data for all known nuclei, organized in over 260
mass chains
ENSDF
Reactions (HI,xn?) (p,p) (n, ?), (n,xng) Coul.
Exc. (?,?), (a,xng) (d,p), etc.
Adopted (best values) Levels (E, J?, T1/2, ?, Q,
configurations) Gammas (Eg, BR, M,?, ICC)
Decays ?- ?? ? ?-n etc.
www.nndc.bnl.gov/ensdf
4
Where to find the data - cont?
Atomic Masses (Audi, Wapstra)
Nuclear Science References (NSR)
www.nndc.bnl.gov/ensdf
  • Pros
  • effort that already exists - updated on regular
    basis
  • (NSDD Network under the auspices of IAEA)
  • ALL experimental NS data for ALL nuclei

ENSDF
RIPL
ENDF/JENDL/JEFF
NuBase
  • Cons
  • updating time vary between 6 to 10 years in
    some cases
  • not all data are relevant to the needs of the
    astrophysics community
  • strange format

5
Where to find the data - cont?
http//www.nucleide.org/DDEP_WG/DDEPdata.htm
  • Pros
  • include comprehensive X-ray data
  • updated on regular basis
  • Cons
  • decay data only
  • mostly for NE metrology applications
  • relevant to a handful of s-(p-) process nuclei

6
Where to find the data - cont?
http//amdc.in2p3.fr/web/nubase_en.html
  • Pros
  • based on ENSDF, but updated for recent data
  • Cons
  • updating time 5-8 years
  • no spectral information
  • continuity

Atomic Masses Evaluations?
7
What would be useful to have?
  • although ENSDF is the best source for a variety
    of experimental NS and decay data, effort is
    needed to (i) extract the needed data for
    astrophysics applications in user defined formats
    (ii) to update for recent discoveries (30 new
    isotopes/yr)
  • results from model calculations should be also
    included for many nuclei, especially on the
    neutron-rich side, experimental data do not exist
  • in an ideal case scenario - a merge between
    experimental theoretical data is needed
    development of a dedicated Astrophysics Nuclear
    Structure Data (ANSD) module easily included
    into Reaclib (or any other library)

8
A N Z E E/T T1/2 E/T
Decay Mode E/T Delayed Particle Emission
E/T 0/1 0/1 b-
eb a 0/1 n p a
0/1 77 38 39 0.0 0 63 MS 12
0 0 100 0 0
0 10 1 2.2 0.5 0
9
What Id like to propose?
  • ANL in collaboration with JINA and other
    interested groups can provide the Astrophysics
    Nuclear Structure Data (ANSD) module
  • updates will be provided regularly once a year
  • data will be peer-reviewed by expert(s) in the
    field
  • the ANSD module will be a merge between
    experiment theory - it will include available
    experimental data for all known nuclei, together
    with predictions for those not yet known
  • the corresponding codes used to merge
    (manipulate) the experimental theoretical data
    sets will be provided, together with subroutines
    that can read the corresponding data files

10
What would be the benefits?
  • Comprehensive Complete
  • All related quantities will be provided,
    together with estimates of their uncertainties
  • Reliable
  • Data will be correctly represented
  • Up-to-Date
  • Consequences of new measurements will appear
    promptly regular updates will be provided
  • Accessible
  • Data will be available in an user-defined format
  • You will have all that for FREE sorry no
    charges

11
What about other data?
Priority 2 level energies, quantum numbers, T1/2
of excited states, etc. the needs for dedicated
effort should be driven by the users and modelers
many of those can be find in ENSDF if there
is a need we can provide it
Priority 1 usually a comparison between
experimental and theoretical T1/2 is used to test
the reliability of a particular model - what
about the b-decay strength distributions from
decay schemes TAGS?
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