/
2. General overview of TALYS 2. General overview of TALYS

2. General overview of TALYS - PowerPoint Presentation

pasty-toler
pasty-toler . @pasty-toler
Follow
382 views
Uploaded On 2017-12-14

2. General overview of TALYS - PPT Presentation

Prof Dr AJ Arjan Koning 12 1 International Atomic Energy Agency Vienna 2 Division of Applied Nuclear Physics Department of Physics and Astronomy Uppsala University Uppsala Sweden ID: 615098

general talys energy reaction talys general reaction energy sample production mev manual time output total cases cross spectra input

Share:

Link:

Embed:

Download Presentation from below link

Download Presentation The PPT/PDF document "2. General overview of TALYS" is the property of its rightful owner. Permission is granted to download and print the materials on this web site for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.


Presentation Transcript

Slide1

2. General overview of TALYS

Prof. Dr. A.J. (Arjan) Koning1,21International Atomic Energy Agency, Vienna 2Division of Applied Nuclear Physics, Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden Email: A.koning@iaea.org

EXTEND

European School on Experiment, Theory and Evaluation of Nuclear Data, Uppsala University, Sweden, August 29 - September 2, 2016Slide2

www.talys.eu2Slide3

PLATYPUSSlide4

GENERAL FEATURES

Situation in 1998 !ALICE – LLNL – 1974 – Blann(Mc-)GNASH – LANL – 1977 – Young, Arthur & ChadwickTNG – ORNL – 1980 – FuSTAPRE – Univ. Vienna – 1980 – UhlUNF,MEND – CIAE, Nanking Univ. – 1985 – Cai, ZhangTALYS – NRG/CEA – 1998 – Koning, Hilaire & DuijvestijnModern computers (i.e. speed and memory) available when the code conception was started EXIFON – Univ. Dresden – 1989 – KalkaEMPIRE – ENEA/IAEA/BNL – 1980 – HermanSlide5

GENERAL FEATURES

GNASH Input file before 1998Slide6

GENERAL FEATURES

Ideas behind TALYS conception- TALYS mantra : “ First Completeness then Quality” - Transparent programmingNo NaNsNo CrashWarnings to identify malfunctionsDefault « simple » models which will later be improved (anticipation)All output channels smoothly described No unnecessary assumptionsNo equation simplification (one can recognize a general expression)Many commentsNo implicit definition of variablesThe variables are defined following the order of appearance in subroutinesSlide7

GENERAL FEATURES

What TALYS does !- Simulates a nuclear reaction projectiles : n,p,d,t,3he, 4he and gamma targets : 3 ≤ Z ≤ 110 or 5 ≤ A ≤ 339 (either isotopic or natural)- Incident projectile energy from a few keV up to 200 MeV (code works up to1 GeV but physics?)- TALYS can be used : . In depth single reaction analysis . Global nuclear reaction network calculation (eg astrophysics) . Within a more global code system (reactor physics)

. Without reaction calculation (only structure data provided)

TALYS

is

always

under

development, while a stable version is released

every 2 years.Slide8

GENERAL FEATURES

Technical details- Fortran 77 -  110000 lines (+ 20000 lines of ECIS)- Modern programming- Flexible use and extensive validation - Flexibility : default  4 line idiot proof input (element, mass, projectile, energy) adjustment  300 keywords- >500 pages manual - Drip-line to drip-line calculations help removing bugs - Random input generation to check stability

-

C

ompiled and tested with several compilers and OS

- modular

(312

subroutines)

- Transparent programming (few exceptions)

- Explicit variable names and many comments (30% of total number of lines) Slide9

GENERAL FEATURES

Typical calculation timesNumbers based on a single Intel Xeon X5472 3.0 GhZ processorTime needed to get all cross sections, level densities, spectra, angular distributions. gamma production etc.:14 MeV neutron on non-deformed target: 3 sec.60 incident energies between 0 and 20 MeV:1 min. (Al-27) 4 min. (Pb-208) 10 min. (U-238)100 incident energies between 0 and 200 MeV:20 min. (Al-27) 3-100 hours (U-238) depending on OMP60 incident energies between 0 and 20 MeV for

all

2629

nuclides

,

stable

or

with

t> 1 sec:

about

200

hours

To

obtain

credible

Monte Carlo

based

covariance

data:

multiply

the

above

numbers

by

50-500.Slide10

GENERAL FEATURES

TALYS versions onlinehttp://www.talys.euTALYS 1.0 (ND 2007)TALYS 1.2 (End of 2009) - new keywords (mainly to improve fitting possibilities) - bugs corrected to solve crashes or unphysical results - inclusion of microscopic ph level densities - inclusion of Skm-HFB structure information (def., masses, g strengths) - inclusion of D1MTALYS 1.4 (End of 2011) - new alpha and deuteron OMP - URR extensionTALYS 1.6 (End of 2013) - non-equidistant excitation energy binning possible (extension to energies > 200 MeV) - direct and semi-direct capture added - new microscopic lds from D1M - medical isotope production implemented - coupling to GEF for fission yields doneTALYS

1.8

(End of

2015)

Resolved resonance range added

More extensive GEF and fission possibilities (PFNS) addedSlide11

GENERAL FEATURES

TALYS versions onlinehttp://www.talys.euSlide12

GENERAL FEATURES

TALYS users and publications User feedback via talys mailing list : info@talys.eu to be added to mailing list : talys-l@nrg.eu to inform mailing listPUBLICATIONSSlide13

13

TALYS code schemeSlide14

REACTION MODELS & REACTION CHANNELS

(REMINDER)Optical model+Statistical model+Pre-equilibrium modelsR = sd + s PE + sCN

n +

238

U

Neutron energy (MeV)

Cross section (barn)

=

s

nn’

+

s

nf

+

s

n

g

+ ...Slide15

TIME SCALES AND ASSOCIATED MODELS (1/4)

Typical spectrum shapeAlways evaporation peakDiscrete peaks at forward anglesFlat intermediate regionSlide16

Reaction time

Emission energy

d

2

s

/ d

W

dE

Compound

Nucleus

Pre-equilibrium

Direct

components

TIME SCALES AND ASSOCIATED MODELS (2/4)

MSC

MSD

Low

emission

energy

Reaction

time

 10

-18

s

Isotropic

angular

distribution

High

emission

energy

Reaction

time

 10

-22

s

Anisotropic

angular

distribution

-

forward

peaked

-

oscillatory

behavior

 spin and

parity

of

residual

nucleus

Intermediate

emission

energy

Intermediate

r

eaction

time

Anisotropic

angular

distribution

smoothly

increasing

to

forward

peaked

shape

with

outgoing

energy

Slide17

TIME SCALES AND ASSOCIATED MODELS (4/4)Slide18

GENERAL FEATURES

What TALYS yieldsCross sections : total, reaction, elastic (shape & compound), non-elastic, inelastic (discrete levels & total) total particle production all exclusive reactions (n,nd2a) all exclusive isomer production all exclusive discrete and continuum g-ray production Spectra : elastic and inelastic angular distribution or energy spectra all exclusive double-differential spectra total particle production spectra compound and pre-equilibrium spectra per reaction stage.Fission observables : cross section (total, per chance) fission fragment mass and isotopic yieldsMiscellaneous : recoil cross sections and ddx

particle multiplicities

s and p

wave

functions

and

potential

scattering

radius r’

nuclear

structure

only

(

levels

, Q,

ld

tables, …)

specific

pre-equilibrium

output (ph

lds

,

decay

widths

…)

astrophysical

reaction

ratesSlide19

19

Statistical Analysis of Cross Sections (SACS) by J. Kopecky: (n,p)Trend lineDiscrepant reactionsS=(N-Z)/ASlide20

20

Installing TALYSSlide21

21

TALYS setupSlide22

22

Alternative (manual) setupcd talys/sourceedit machine.freplace the pathname by the total pathname of the structure database on your systemsave machine.fgfortran –c *.fgfortran *.o –o talysmv talys ~/bin or wherever you want to have the executableSlide23

Running the TALYS sample cases

Go to the samples/ directoryverifyWait for 1-2 hours before all 27 sample cases have finished…….or try your own input filesAll 27 sample cases are described in the manual, with input files, output files, plots etc.See talys/doc/talys1.8.pdf23Slide24

24

TALYS sample cases (see manual)232ThSlide25

25

TALYS sample cases (see manual)Slide26

26

TALYS sample cases (see manual)Slide27

27

TALYS sample cases (see manual)19. Unresolved resonance range parameters: n + 136Ba20. Maxwellian averaged cross section at 30 keV: n + 138Ba21. Medical isotope production with p + 100Mo22. Calculations up to 500 MeV for p + 209Bi23. Neutron multiplicities and fission yields for n + 242Pu24. Local parameter adjustment for n + 93Nb25. Direct neutron capture for n + 89YSlide28

28

Sample 1A: simplest case (1 energy)Cd talys/samples/1/a/newAll important results are in the output fileSlide29

29

Sample 1: outputSlide30

30

Sample 1: output (continued)Slide31

31

Sample 8: residual production with protonsCd talys/samples/8/new; talys <input > output(pre-calculated results in talys/samples/8/org)Slide32

32

Residual production c.s. for FePlot: xmgrace rp027056.tot