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Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
1
Controlled Fission• Note that is greater than 2 at thermal energies andalmost 3 at high energies.• These “extra” neutrons are Used to convert fertile into fissile fuel.• Plutonium economy.• India and thorium.• Efficiency of this process is determined by neutronenergy spectrum.
Variations in Variations in
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
2
Controlled Fission
• Conversion ratio Conversion ratio CR is defined as the average rate of fissile atom production to the average rate of fissile atom consumption.• For LWR's CR 0.6.• CR is called BR for values > 1.• Fast breeder reactors have BR > 1.• They are called “fast” because primary fissions inducing neutrons are fast not thermal, thus η > 2.5 but σf is only a few barns.• Moderator??
3
Controlled Fission
Time scale for neutron multiplicationTime scale for neutron multiplication• Time constant includes moderation time (~10-6 s) and diffusion time of thermal neutrons (~10-3 s).
Time Average number of thermal neutrons t nt + knt + 2 k2n
• For a short time dt
• Show thatShow that
nkn
dt
dn
tkentn )1(0)(
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
4
• k = 1 n is constant (Desired).• k < 1 n decays exponentially.• k > 1 n grows exponentially with time constant / (k-1).• k = 1.01 (slightly supercritical..!) e(0.01/0.001)t = e10 = 22026 in 1s. in 1s. • Design the reactor to be slightly subcritical for prompt neutrons.• The “few” “delayed” neutrons will be used to achieve criticality, allowing enough time tomanipulate the controlrods (or use shim or …).
Controlled Fission
Dan
gero
us
Dan
gero
us
Cd control rodsCd control rods
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
tkentn )1(0)(
Reactivity.
5
Fission Reactors
Essential elements:Essential elements:• Fuel (fissile material).• Moderator (not in reactors using fast neutrons).• Reflector (to reduce leakage and critical size).• Containment vessel (to prevent leakage of waste).• Shielding (for neutrons and ’s).• Coolant.• Control system.• Emergency systems (to prevent runaway during failure).
Core
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
Chapter 4 in Lamarsh
6
Fission Reactors
Types of reactors:Types of reactors:Used for what?Used for what?• Power reactors: extract kinetic energy of fragments as heat boil water steam drives turbine electricity.• Research reactors: low power (1-10 MW) to generate neutrons (~1013 n.cm-2.s-1 or higher) for research.• Converters and breeders: Convert non-thermally-fissionable material (non-fissile) to a thermally-fissionable material (fissile).• ADS.• Fusion.
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
What are neutron generators?What are neutron generators?
7
Fission Reactors
What neutron energy?What neutron energy?• Thermal, fast reactors.• Large, smaller but more fuel.
What fuel?What fuel?• Natural uranium, enriched uranium, 233U, 239Pu,Mixtures.
From converter or breeder reactor.How???
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
8
Fission ReactorsWhat assembly?What assembly?• Heterogeneous: moderator and fuel are lumped. • Homogeneous: moderator and fuel are mixed together.• In homogeneous systems, it is easier to calculate p and
f for example, but a homogeneous natural uranium-graphite mixture can not go critical. Why?
What coolant?What coolant?• Coolant prevents meltdown of the core.• It transfers heat in power reactors.• Why pressurized-water reactors.• Why liquid sodium?
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
What moderator?What moderator?1. Cheap and abundant.2. Chemically stable.3. Low mass (high logarithmic energy decrement).4. High density.5. High s and very low a.• Graphite (1,2,4,5) increase amount to compensate 3.• Water (1,2,3,4) but n + p d + enriched uranium.• D2O (heavy water) (1!) but has low capture cross
section natural uranium, but if capture occurs, produces tritium (more than a LWR).
• ….. 9
More on Moderators
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
10
More on Moderators
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
Moderating ratio
Calculate both moderating power and ratio for water, heavy water, graphite, polyethylene and boronboron.Tabulate your results and comment.
a
s
Moderating power
HW 12HW 12 LiBnB 7*1110
B-10
1/v region
Good absorber,
Good absorber, bad moderator.
bad moderator.
Never consider this only!
For a compound?
1010BB
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
11
HW 12 HW 12 (continued)(continued)
More on Moderators
Calculate the moderating power and ratio for pure D2O as well as for D2O contaminated with a) 0.25% and b) 1% H2O.Comment on the results.In CANDU systems there is a need for heavy water upgradors.
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
12
More on Moderators
1
1ln
2
)1(1ln
2
\
A
A
A
A
E
Eu
av
nEEn lnln \
)/ln( \
nEEnRecall
After n collisions
)/ln( thf EE
n
Total mean free path = n s
Is it random walk or there is a preferred direction???
creation
absorption
After one collision
f
th
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
13
More on Moderators
Assumptions:Assumptions:1.1.Elastic scattering. Elastic scattering. E2.2.Target nucleus at rest. Target nucleus at rest. E3.3.Spherical symmetry in Spherical symmetry in CM.CM.
Recall (head-on). Then the maximum energy loss is (1-)E, or E E\ E. For an ss-wave-wave collision:
show that
Obviously
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
14
More on ModeratorsHW 13 (or 6HW 13 (or 6\\))
EEA
AE
2
min\
1
1
EEEPdEEEP
E
E )1(
1)(1)( \\\
EE )1(21\
otherwise
EEEE
E
dE
dEE
ss
s
0)1(
)()(
|
|\
After one collision.
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
15
More on Moderators
2
222
2
2\
)1(
sincos
cos)1()1(2
1
)1(
cos21
A
A
A
AA
E
E CMCM
(Re)-verify
For doing so, you need to verify and use
CM
CM
AA
A
cos21
cos1cos
2
HW 13 (or 6HW 13 (or 6\\) ) continued…continued…• Scattering Kernel.Scattering Kernel.• Slowing down density.Slowing down density.• Migration length.Migration length.• Fermi age and continuous fermi model.Fermi age and continuous fermi model.
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
16
More on Moderators
HW 13 (or 6HW 13 (or 6\\) ) continued…continued…
• Forward scattering is preferred for “practical” moderators (small A).• If isotropic neutron scattering (spherically symmetric) in the laboratorylaboratory frame average cosine of the scattering angle is zero.
Show that A3
2)(cos
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
17
More on Moderators
Spherically symmetric in CM
Show that
)(4
1)( E
d
ds
CMsCM
s
CM
CMs
s A
AAE
cos1
)1cos2(
4
)()(
1
2312
Try to sketch.
HW 13 (or 6HW 13 (or 6\\) ) continued…continued…
• Neutron scatteringscattering is isotropic in the laboratory system?! valid for neutron scattering with heavy nuclei, which is not true for usual thermal reactor moderators (corrections are applied).
Distinguish fromDistinguish from
• Angular neutron distribution.distribution.
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
18
More on Moderators
Moderator-to-fuel ratio Moderator-to-fuel ratio Nm/Nu.• Ratio p a of the moderator f (leakage ).• Ratio slowing down time p f (leakage ).
• T ratio (why).• Other factors also change.• Temperature coefficient of reactivity.• Moderator temperature coefficient of reactivity.
Self regulation.
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
19
One-Speed Interactions• Particular general.Recall:• Neutrons don’t have a chance to interact with each other (review test!) Simultaneous beams, different intensities, same energy:
Ft = t (IA + IB + IC + …) = t (nA + nB + nC + …)v• In a reactor, if neutrons are moving in all directions n = nA + nB + nC + …
Rt = t nv = t
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
20
drn ),(
r
d
Neutrons per cm3
at r whose velocity vector lies within d about .
4
),()( drnrn
• Same argument as before vdrnrdI ),(),(
)()()()(),()(),()()(
),()(),(
4
rrrnrvdrnvrrdFrFrR
rdIrrdF
ttt
t
One-Speed Interactions
drnvr ),()(4
where
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
21
Multiple Energy Interactions
dEdErn ),,(
Neutrons per cm3 at r with energy interval (E, E+dE) whose velocity vector lies within d about .
• Generalize to include energy
4
),,(),( dEdErndEErn
0 4
),,()(
dEdErnrn
dEErErdEEvErnErdEErR tt ),(),()(),(),(),(
0
),(),()( dEErErrR t
Thus knowing the material properties t and the neutron flux as a function of space and energy, we can calculate the interaction rate throughout the reactor.
Scalar
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
22
Neutron Current
• Similarly and so on …
• Redefine as
0
),()()( dEErErR SS
Scalar
vdrnrdI ),(),( dvrnrId
),(),(
drnvr ),()(4
drnvJ ),(
4
Neutron current densityNeutron current density
J• From larger flux to smaller flux!
• Neutrons are not pushed!• More scattering in one direction than in the other.
xJxJ ˆ
Nuclear Reactors, BAU, 1st Semester, 2008-2009 (Saed Dababneh).
23
4
cos),(ˆ dvrnJxJ xx
NetNet flow of neutrons per second per unit area normal to the x direction:
In general: nJnJ ˆ
Equation of ContinuityEquation of Continuity
A
a dAntrJdtrrdtrSdtrnt
ˆ),(),()(),(),(
Rate of change in neutron density
Production rate
Absorption rate
“Leakage in/out” rate
Volume Source distribution
function
Surface area
bounding
Normal to A
Equation of Continuity