Keyword | Short explanation |
---|---|
MassTable | Path to the mass tables |
GDRParams | Path to the file with gdr parameters |
LevelDir | Path to the directory which contains the level files |
SpinFile | Path to the file which contains the spin information |
ProtonModel | Sets the model for proton transmission function. |
pNorm | Multiplication factor for the proton transmission coefficient |
NeutronModel | Sets the model for neutron transmission function. |
nNorm | Multiplication factor for the neutron transmission coefficient |
AlphaModel | Sets the model for neutron transmission function. |
aNorm | Multiplication factor for the alpha transmission coefficient |
E1Model | Sets the model for E1 gamma transmission function. |
M1Model | Sets the model for M1 gamma transmission function. |
E2Model | Sets the model for E2 gamma transmission function. |
gNorm | Multiplication factor for the gamma transmission coefficient |
PorterThomasParticle | Toggle the Porter-Thomas Fluctuations for particle transmission |
PorterThomasGamma | Toggle the Porter-Thomas Fluctuations for gamma transmission |
GammaChannel | Toggle the gamma channel |
NeutronChannel | Toggle the neutron channel |
ProtonChannel | Toggle the proton channel |
AlphaChannel | Toggle the alpha channel |
LevelDensity | Sets the model for the Nuclear Level Density. |
cTable | Value to normalize the level spacing at the neutron separation energy. |
eBinning | Number of continuum bins during the continuum calculations. |
Keyword | Short explanation |
---|---|
Reaction | Reaction string,e.g., 25Mg+a |
EnergyFile | Path to the file containing a list of energies |
ReactionFile | Path to the file containing a list of reactions |
CalcRates | Turn calculation of rates on or off (if neutron) |
CalcAverageWidth | Calculates the average s-wave radiative width at threshold and exits. |
ResidualGamma | Toggles if residual or total capture cross section is calculated. |
ResidualNeutron | Toggles if neutron residual or total capture cross section is calculated. |
ResidualProton | Toggles if proton residual or total capture cross section is calculated. |
ResidualAlpha | Toggles if alpha residual or total capture cross section is calculated. |
CalculateGammaCutoff | Toggles if Gamma-Cutoff energy should be calculated or not. |
EntranceState | Give the number of the initial state, e.g. 0 for groundstate |
g_ExitStates | Define how many partial cross section should be calculated. |
n_ExitStates | Define how many partial cross section should be calculated. |
p_ExitStates | Define how many partial cross section should be calculated. |
a_ExitStates | Define how many partial cross section should be calculated. |
PrintXS | Toggle if calculated cross sections should be written to a file |
PrintTRANS | Toggle if calculated transmission coefficients should be written to a file |
PrintRATE | Toggle if calculated reaction rates should be written to a file |
Keyword | Short explanation |
---|---|
Suffix | Suffix which can be given to the output files. |
Isotope | Isotope of interest. Format example: 94Mo |
Spin | Spin of the initial state as a double. |
Parity | Parity of the initial state: 1 = + , -1 = - |
EnergyLow | Lower limit of the excitation energy window in MeV |
EnergyHigh | Upper limit of the excitation energy window in MeV |
Events | Number of simulated decays |
ChunkSize | Size of the chunks which are calculated at the same time |
Preequillibrium | Toggle if the prequillibrium decayer should be used |
PreEqConf | Sets the initial exciton configuration. |
Keyword | Short explanation |
---|---|
Z | Charge of the isotope |
A | Mass of the isotope |
Mode | create or extend |
OutputFile | OutputFile of the level scheme |
Emin | Starting energy for the creation of the level scheme |
Emax | Energy limit for the creation of the level scheme |
The default mass tables can be found in /tables/masses/
. Currently, Sapphire uses the mass excesses from the Reference Input Parameter Library (RIPL-3) to calculate atomic masses and Q-Values. The experimental mass excesses were evaluated by G. Audi and A.H. Wapstra.
If no experimental mass excesses are available, Sapphire uses the ground state properties of the Finite Range Droplet Model (FRDM) from RIPL-3.
Users who want to use different ground state properties are free to edit the data tables or exchange them with other ones. However, the file structure needs to stay the same as defined by RIPL-3.
This keywords sets the path to the file containing the GDR parameters. Currently the parameters from RIPL-3 are used and stored in /tables/gamma/ripl3_gdr_parameters.dat
. If changed by the user, the new file has to be in the same format as the current file. For more information, see the official RIPL-3 README-file.
Currently available models are:
[0] Brink-Axel Lorentzian
Simple Standard Lorentzian (SLO) with GDR parameters from [RIPL-3]. See GDRParams for details.
[1] Generalized Lorentzian by Kopecky-Uhl
[2] McCullaghGSF
[3] Microscopical E1 strength based on QRPA calculations using the D1M Gogny Force (default)
This model is based on the published tables of the PSF Database. The tables can be found in tables/gamma/D1M/
. The tables are modified by the analytical corrections for the up-bend and nuclear temperature. For details see references:
- S. Goriely et al., The European Physical Journal A 55, 172 (2019)
- S. Goriely, S. Hilaire, S. Péru, K. Sieja, Phys. Rev. C 98, 014327 (2018)
[0] Brink-Axel Lorentzian
Simple Standard Lorentzian (SLO) with GDR parameters from [RIPL-3]. See GDRParams for details.
[2] McCullaghGSF
[3] Microscopical M1 strength based on QRPA calculations using the D1M Gogny Force (default)
This model is based on the published tables of the PSF Database. The tables can be found in tables/gamma/D1M/
. The tables are modified by the analytical corrections for the up-bend and nuclear temperature. For details see references:
- S. Goriely et al., The European Physical Journal A 55, 172 (2019)
- S. Goriely, S. Hilaire, S. Péru, K. Sieja, Phys. Rev. C 98, 014327 (2018)
[0] Brink-Axel Lorentzian Simple Standard Lorentzian (SLO) with GDR parameters from [RIPL-3]. See GDRParams for details.
[2] McCullaghGSF
For a simple normalization of the gamma-decay width, the parameter gNorm
can be used. All gamma-ray transmission coefficients are multiplied with this factor. It's default value is 1.0
.
Currently available models:
-
Rauscher Level Density
-
Microscopical Level Density HFB-BSk14
Quotation from RIPL-3:
"The nuclear level density is coherently obtained on the basis of the single-particle level scheme and pairing energy derived at the ground state deformation based on the BSk14 Skyrme force (S. Goriely, M. Samyn, J.M. Pearson, Phys. Rev. C75 (2007) 064312).
Additionally, the phenomenological level density parameters ctable and ptable are tabulated in files (*.cor) by fitting the HFB calculated curve to the RIPL II recommended spacings of s-wave neutron resonances D0 and to the cumulative number of low-lying levels (S. Goriely, S. Hilaire, A.J. Koning, Phys. Rev. C 78 (2008) 064307)".
Normalization factor
With this parameter the level density can be fitted to level spacing at the neutron separation energy
The known levels are also derived from RIPL-3 and can be found in /tables/levels/
.
In some situations the user might want to exclude specific channels in the calculations, for instance, if the user is only interested in the gamma-ray decay behaviour while neutron decay is also open but much more likely. In these cases the keywords AlphaChannel
, ProtonChannel
, NeutronChannel
, or GammaChannel
can be set to 0
.
In this example the statistical decay of 2- states in 92Mo at excitation energies between 8.0 MeV and 8.5 MeV will be simulated. The input file looks like the code below.
[General]
LevelDensity = 0
E1Model = 0
M1Model = 0
[Decayer]
Isotope = 92Mo
Events = 10000
ChunkSize= 10000
Spin = 2.0
Parity = -1
EnergyLow = 8.0
EnergyHigh = 8.5
This will generate the following gamma-ray spectrum and TSC matrix: