USCD1238 ALICE2011.
ALICE2011, Particle Spectra from HMS precompound Nucleus Decay
NAME OR DESIGNATION OF PROGRAM, COMPUTER, DESCRIPTION OF PROGRAM OR FUNCTION, METHODS, RESTRICTIONS ON THE COMPLEXITY OF THE PROBLEM, RELATED OR AUXILIARY PROGRAMS, STATUS, REFERENCES, HARDWARE REQUIREMENTS, LANGUAGE, SOFTWARE REQUIREMENTS, NAME AND ESTABLISHMENT OF AUTHORS, MATERIAL, CATEGORIES
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| Program name | Package id | Status | Status date |
|---|---|---|---|
| ALICE2011 | USCD1238/05 | Tested | 15-MAR-2011 |
Machines used:
| Package ID | Orig. computer | Test computer |
|---|---|---|
| USCD1238/05 | IBM PC | Linux-based PC,PC Windows |
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3. DESCRIPTION OF PROGRAM OR FUNCTION
This nuclear model code permits nuclear reaction predictions to be made using the Hybrid model of precompound decay in the HMS Monte-Carlo formulation,plus the Weisskopf-Ewing evaporation and Bohr- Wheeler fission models. The latter may be run in S-wave approximation to estimate angular momentum effects on phase space, including enhancement of gamma ray de-excitation. Multiple emission cascades including photons,n,p,d,t,3He, and 4He are performed, plus the fission channel. Product yields may be calculated, including those of fission fragments. Single and double differential emission spectra are calculated, and user may select to have ENDF format spectra for 1-3 n,p,4He particle emissions output. As a Monte-Carlo method of calculation is used, the history file for each event may be programmed to output any order of ENDF spectra, gated coincidence spectra, etc.
Incident projectiles of photons, neutrons, protons and heavy ions (A>1) are acceptable, as in earlier versions.
This nuclear model code permits nuclear reaction predictions to be made using the Hybrid model of precompound decay in the HMS Monte-Carlo formulation,plus the Weisskopf-Ewing evaporation and Bohr- Wheeler fission models. The latter may be run in S-wave approximation to estimate angular momentum effects on phase space, including enhancement of gamma ray de-excitation. Multiple emission cascades including photons,n,p,d,t,3He, and 4He are performed, plus the fission channel. Product yields may be calculated, including those of fission fragments. Single and double differential emission spectra are calculated, and user may select to have ENDF format spectra for 1-3 n,p,4He particle emissions output. As a Monte-Carlo method of calculation is used, the history file for each event may be programmed to output any order of ENDF spectra, gated coincidence spectra, etc.
Incident projectiles of photons, neutrons, protons and heavy ions (A>1) are acceptable, as in earlier versions.
USCD1238/05
NEW VERSION DIFFERS FROM PREVIOUS VERSION IN THE FOLLOWING FEATURES-------------------------------------------------------------------
The January 2011 version of ALICE has some refinement of Fortran, more enlarged BE (Binding Energy) arrays.
The Oct 2010 version had a modification which gave the option (parm=512) to override the A=12 default mass number as the mass at or below which Fermi decay is implemented using a new coding of K.K. Gudima.
The January 2011 version (like the previous one) differs from earlier versions in allowing isotopic targets to be used except for incident heavy ions (A>1). It contains cluster exit channels on demand, precompound and compound (use PARM=128). An ENDF output for 1,2,3 n,p,alpha out reactions is an option. The logic used could be extended to include other clusters and to increase multiplicities if needed. Some routines have been rewritten in a more modern f95 fortran compiler. Random routine generator has been rewritten.
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4. METHODS
This code predicts the course of nuclear reactions induced by photons, nucleons,or nuclei incident on target isotopes, either single mass or (for A=1 projectiles) natural isotopic mix. The nuclear models used in this process are primarily the Monte-Carlo version of the Hybrid precompound decay model followed by Weisskopf- Ewing evaporation and Bohr-Wheeler fission models. Other models are used in the algorithms for getting fission product mass and charge yields, in the nuclidic masses, fission barriers, level densities, etc. contained in the library files used at time of code execution, or coded as subroutines.
Options are available for shell corrected level densities at time of execution, or these are default selected by the code based on proximity of composite nucleus to closed shell product nuclei.Angular distributions are based on the linear momentum conservation model of Chadwick and Oblozinsky. Cluster exit channels are an option selectable by user.
This code predicts the course of nuclear reactions induced by photons, nucleons,or nuclei incident on target isotopes, either single mass or (for A=1 projectiles) natural isotopic mix. The nuclear models used in this process are primarily the Monte-Carlo version of the Hybrid precompound decay model followed by Weisskopf- Ewing evaporation and Bohr-Wheeler fission models. Other models are used in the algorithms for getting fission product mass and charge yields, in the nuclidic masses, fission barriers, level densities, etc. contained in the library files used at time of code execution, or coded as subroutines.
Options are available for shell corrected level densities at time of execution, or these are default selected by the code based on proximity of composite nucleus to closed shell product nuclei.Angular distributions are based on the linear momentum conservation model of Chadwick and Oblozinsky. Cluster exit channels are an option selectable by user.
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5. RESTRICTIONS ON THE COMPLEXITY OF THE PROBLEM
Excitations below 1 GeV required, but advised to keep under 250 MeV until pion resonances are included for the excitation and decay cascades. The code is intended to be relatively fast in execution and easy to use. Ease of use is achieved by an on- screen input interrogation procedure, with defaults provided if user has no preferences, plus several library files which provide masses, binding energies, fission barriers, natural isotopic abundances of non- mono-isotopic targets, nuclide spins and parities, isomer spins and level energies ( for calculation of isomer yields).
Excitations below 1 GeV required, but advised to keep under 250 MeV until pion resonances are included for the excitation and decay cascades. The code is intended to be relatively fast in execution and easy to use. Ease of use is achieved by an on- screen input interrogation procedure, with defaults provided if user has no preferences, plus several library files which provide masses, binding energies, fission barriers, natural isotopic abundances of non- mono-isotopic targets, nuclide spins and parities, isomer spins and level energies ( for calculation of isomer yields).
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10. REFERENCES
- M.Blann: Phys. Rev.C54(1996)1341.
- M.B. Chadwick and P. Oblozinsky: Phys. Rev.C50,(1994)2490.
- P.Moller, J.R.Nix, W.D.Myers and W.J. Swiatecki: Atomic Data Nucl. Data Tables, 59(1995)185, and private comm. P.Moller, 2002.
- T.M.Shneidman et al.: Phys. Rev. C65,064302(2002).
- M.Blann: Phys. Rev.C54(1996)1341.
- M.B. Chadwick and P. Oblozinsky: Phys. Rev.C50,(1994)2490.
- P.Moller, J.R.Nix, W.D.Myers and W.J. Swiatecki: Atomic Data Nucl. Data Tables, 59(1995)185, and private comm. P.Moller, 2002.
- T.M.Shneidman et al.: Phys. Rev. C65,064302(2002).
USCD1238/05, included references:
- M.Blann, A.A. Konobeev, W.B. Wilson, S.G. Mashnik:Manual for Code Alice version July 7, 2008 (July 27, 2008)
- M.Blann, W.G. Wilson, S.G. Mashnik, A.Y. Konobeev:
Summary of Capabilities of Monte-Carlo HMSALICE Code post-1996 (September 17,
2008)
- M. Blann and A.Y. Konobeev:
Precompound Cluster Decay in HMSAlice (September 22, 2008)
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15. NAME AND ESTABLISHMENT OF AUTHORS
M.Blann (LLNL, Retired),
K.K. Gudima (Institute of Applied Physics, Moldova Academy of Sciences, Kishineu, Moldova),
A.V. Ignatyuk (Institute for Physics and Power Engineering, Obninsk, Russia),
A.Yu. Konobeyev (Karlsruhe Institute of Technology, Karlsruhe, Germany),
V.P. Lunev (Institute for Physics and Power Engineering, Obninsk, Russia),
S.G. Mashnik (LANL, USA),
W.B. Wilson (LANL, USA),
We appreciate contributions from:
D. Madland (LANL,USA),
M. Giaccri-Mauborgne (CEA, Saclay, France)
M.Blann (LLNL, Retired),
K.K. Gudima (Institute of Applied Physics, Moldova Academy of Sciences, Kishineu, Moldova),
A.V. Ignatyuk (Institute for Physics and Power Engineering, Obninsk, Russia),
A.Yu. Konobeyev (Karlsruhe Institute of Technology, Karlsruhe, Germany),
V.P. Lunev (Institute for Physics and Power Engineering, Obninsk, Russia),
S.G. Mashnik (LANL, USA),
W.B. Wilson (LANL, USA),
We appreciate contributions from:
D. Madland (LANL,USA),
M. Giaccri-Mauborgne (CEA, Saclay, France)
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USCD1238/05
abund Input file to read the naturally occuring abundanceshmsalice.jan2011.f Fortran source of Alice as Jan 2011 to be compiled by lahey
Alice_feb_2011.exe Alice executable obtained with lahey futjitsu
angeng Ouput angular energy tabular data
ddcsfcm Output file with double differential fission spectra (com)
ddcsflb Output file with double differential fission spectra (lab)
ddcstotlb Output file with double differential fission + evaporation spectra
ejplanes Output file for internal check
endf Output file for internal check
endv Output file for internal check
engang Output file with energy angular distribution
excdst Output file for check use
excdst1 Output file for check use
exciton Output File for check use
finp Output File for check use
fizej Output File for check use
fizisomr Output File with fission yields
fizisrat Output File with fission isomer ratios
fizybya Output File with fission mass yields
fizylds Output File with fission fragments yields
fizzers Output File
fizzersj Output File
fout Output File
fragss Output File
gammaspec Output File with gamma spectra
gdrparms Input file
insave input file saved
labangd Output File with lab angular data
labengd Output File with energy distribution data
labout Output File
labspec Output file
MASS.TBL Input file with mass excess
mcspec Output check file
outpt Output detailed File
0utpt_linux_alice_jan_2011 Output obtained with linux machine
phtlib Input File
plot Output plot file
pmtable Input mass table File
ratiox Output check File
recoils Output check File
recvel Output check File
sdcscl Output check File
sdcscm Ouptut cross section file
sdcsfcm Ouptut cross section file
sdcsflb Ouptut cross section file
sdcstotlb Ouptut cross section file
sdlbcl Ouptut cross section file
SHELL.TBL Input shell corrections File
sigs Ouptut check file
temp File
tmadland Input file with fission barriers
man3 pdf Manual
hms.pdf pdf Monte Carlo capabilities
hms.ps ps Monte Carlo capabilities
clusterhms.pdf pdf Precompound model explained
clusterhms.ps ps Precompound model explained
Keywords: compound nuclei, evaporation model, nuclear models, precompound-nucleus emission.