GAM
.
Decay photons, such as the 1.779-MeV photon from the Al-28
$\beta\bar{~~}$ decay mentioned above, can also be added into the
photon source as shown in the next sample problem.
TEST 6 -- HEAT, DAMAGE, PHOTON SOURCE 0 1 0 1 1 1 0 3 0 0 30 2 47 0 0 1 1 1 14 4 AL-27 ALUM/ 1 1 AL27/ HEAT DPA GAM GAM GAM GAM GAM GAM GAM GAM GAM GAM GAM GAM 1 HEAT/ 1 NG 1.125E6/ 2 DAME .02/ 11 NG/ STOPThe 12 occurrences of
GAM
reserve spaces for the 12 photon
groups. Group 9 (1-2 MeV) is in position 11, and the last edit
specification adds the equilibrium 1.779-MeV photon production
rate into that group (one such delayed gamma is produced per
capture event). Note also that damage energy is converted to DPA
in position 2 using 25 eV for the displacement energy ${ 0.02 =
[1/(2*25)] }$. Most SN codes could use these cross
sections and print out steady-state photon source vectors by
region to be used in a subsequent photon transport calculation.
Coupled sets, like the one defined in Sample Problem 3, can also
be prepared including steady-state radioactive decay contributions.
Putting a negative sign on JEDPOS
defines the gamma group
in the coupled set that will receive the contributions defined
by that edit specification. The Problem 3 input would become
TEST 3A -- COUPLED SET WITH STEADY-STATE DECAY 0 3 0 3 1 1 0 3 0 0 42 2 46 0 0 1 1 2 1 2 AL-27 * */ 1 1 AL27/ HEAT 1 HEAT/ NN AND NG PART 1 GHEAT/ GG PART 1 NG 1.125e6 AL27 / DELAYED HEAT AND GAMMAS FOR AL27 -8 NG 1. AL27 1 NP 3.2e5 AL27 -10 NP .72 AL27 -9 NP .28 AL27 STOPDelayed heat and photon production edit specifications for some important materials are given in the
DELAY12
and
DELAY24
files included in the TRANSX distribution. As
an example, the 12-group data for U-238 are repeated below:
1 N2N 0.060E+6 U238 1 NG 0.160E+6 U238 1 NF 8.580E+6 U238 -4 NF 5.995E-4 U238 -5 NF 4.072E-3 U238 -6 NF 2.036E-2 U238 -7 NF 9.226E-2 U238 -8 NF 3.033E-1 U238 -9 NF 1.442E+0 U238 -10 NF 3.384E+0 U238 -11 NF 4.726E+0 U238 -12 NF 1.514E+0 U238The heating part (position 1) includes the beta decay heating for Pu-239 and Np-239; thus, it includes all the heat up to the appearance of the final Pu-239 product. The contributions to heating and photon production from fission come from the decay of the fission products.
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