ORNL-2106 - the Molten Salt Energy Technologies Web Site
ORNL-2106 - the Molten Salt Energy Technologies Web Site
ORNL-2106 - the Molten Salt Energy Technologies Web Site
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ANP PROJECT PROGRESS REPORT<br />
a 2.32-Mev alpha particle is given off and that in<br />
<strong>the</strong> remaining 7% a 2.8-Mev alpha particle is given<br />
off.ll The heating from beta decay resulting from<br />
neutron captures in copper was calculated, and it<br />
was found to be negligible compared with <strong>the</strong><br />
a Ipha-part ic le heating.<br />
The gamma-ray heating resulting from <strong>the</strong><br />
emission of decay gamma radiation in <strong>the</strong> heat<br />
exchanger was calculated on <strong>the</strong> basis of slab<br />
geometry by using Eq. 6 for each energy group.<br />
The spectrum of gamma rays was divided into <strong>the</strong><br />
seven energy groups given in ref. 3, with average<br />
energies of 0.5, 1, 2, 4, 6, 8, and 10 MeV. The<br />
buildup factor for <strong>the</strong> heat exchanger was used<br />
for each energy group. The total heating at<br />
various points was calculated by summing over<br />
<strong>the</strong> contributions of each energy group.<br />
The source strength of <strong>the</strong> gamma rays resulting<br />
from inelastic neutron scattering in <strong>the</strong> beryllium<br />
reflector was also calculated. These sources are<br />
appreciable only in <strong>the</strong> first 9 cm of beryllium.<br />
However, <strong>the</strong>ir contributions to <strong>the</strong> heating in <strong>the</strong><br />
regions around <strong>the</strong> heat exchanger are small<br />
compared with those of <strong>the</strong> beryllium capture<br />
gamma-ray sources. The reason for this is that<br />
<strong>the</strong> gamma rays from inelastic scattering were<br />
taken to be I-Mev gamma rays, which are at-<br />
tenuated much more strongly by <strong>the</strong> beryllium than<br />
are <strong>the</strong> bMev capture gamma rays. In addition<br />
<strong>the</strong> total source strength of <strong>the</strong> gamma rays from<br />
inelastic neutron scattering is much smaller than<br />
that of <strong>the</strong> capture gamma rays because of <strong>the</strong><br />
volumes of beryllium involved in each.<br />
The source strength of <strong>the</strong> capture gamma rays<br />
resulting from delayed neutron captures was<br />
calculated by assuming that 50% of <strong>the</strong> delayed<br />
neutrons were given off in <strong>the</strong> heat exchanger and<br />
that all <strong>the</strong>se neutrons were captured in <strong>the</strong><br />
neighborhood of <strong>the</strong> heat exchanger. By assuming<br />
that an &Mev gamma ray was given off for each<br />
capture, <strong>the</strong> average source strength per unit<br />
volume was found to be small as compared with<br />
<strong>the</strong> o<strong>the</strong>r sources in this region.<br />
The capture gamma-ray sources in <strong>the</strong> copper<br />
were calculated in <strong>the</strong> same general way that <strong>the</strong><br />
alpha-particle heating in <strong>the</strong> copper was calcu-<br />
lated, with <strong>the</strong> source converted to a surface<br />
source of gamma rays. In itself this is not an<br />
insignificant source, but <strong>the</strong> heating resulting<br />
from this source would be only about 2% of <strong>the</strong><br />
total from all <strong>the</strong> sources considered here.<br />
34<br />
The gamma.rays resulting from inelastic neutron<br />
scattering in <strong>the</strong> core shells were calculated by<br />
using <strong>the</strong> Curtiss-Wright multigroup fluxes5 and<br />
an inelastic microscopic cross section of 1.5<br />
barns (ref. 13) for <strong>the</strong> constituents of Inconel.<br />
It was assumed thaf a 2-Mev gamma ray was given<br />
off for each inelastic collision. The results<br />
gave a source strength of about 10% of that<br />
resulting from <strong>the</strong> capture gamma rays in <strong>the</strong>se<br />
shells.<br />
As has already been remarked, <strong>the</strong> capture<br />
gamma rays in <strong>the</strong> island core shell were neglected<br />
because of <strong>the</strong> shielding properties of <strong>the</strong> fuel.<br />
Where it has not been stated o<strong>the</strong>rwise, <strong>the</strong><br />
dimensions used in <strong>the</strong>se calculations were those<br />
from ref. 1 for <strong>the</strong> equatorial plane of <strong>the</strong> reactor.<br />
RADIATION HEATING IN VARIOUS REGIONS<br />
OFTHENORTHHEAD<br />
H. W. Bertini D. L. Platus14<br />
Calculations of <strong>the</strong> radiation heating to be<br />
ex cted in various regions in <strong>the</strong> north head of<br />
<strong>the</strong> ART were undertaken in order to supply<br />
pt numbers from which <strong>the</strong>rmal-stress calculations<br />
could be made. Because of <strong>the</strong> complexity and<br />
<strong>the</strong> time that would be involved in calculating<br />
accurately <strong>the</strong> heating in all <strong>the</strong> regions of <strong>the</strong><br />
north head, it was decided to make preliminary<br />
estimates of <strong>the</strong> deposition rates. More accurate<br />
values calculated for o<strong>the</strong>r regions of <strong>the</strong> reactor<br />
were used as guides. In all cases <strong>the</strong> tendency<br />
was to overestimate <strong>the</strong> heating. These estimates<br />
can be used to identify <strong>the</strong> <strong>the</strong>rmal-stress<br />
problems, and where <strong>the</strong> calculated <strong>the</strong>rmal<br />
stresses are marginal, <strong>the</strong> heating will be recalculated,<br />
Calculations were made of <strong>the</strong> heat-deposition<br />
rate in a slab of lnconel bounded on one side by<br />
an infinite fuel region containing <strong>the</strong> sources of<br />
radiation. This heat-generation rate was used in<br />
all regions in <strong>the</strong> north head which are bounded by<br />
finite fuel volumes,<br />
The heat-deposition rates in a slab of lnconel<br />
bounded on one side by slabs of sodium of various<br />
thicknesses were calculated, and <strong>the</strong> results were<br />
extrapolated and interpolated to obtain <strong>the</strong> heat-<br />
generation rates in <strong>the</strong> lnconel regions of <strong>the</strong> north<br />
13H. Le Taylor, 0. Lonsio, and T. W. Bonner, Pkys.<br />
Rev. 100, 174 (1955).<br />
assignment from USAF.<br />
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