Video summary
The video centers on a group discussion regarding the OpenFOAM engine form, specifically focusing on solving coupled neutronics and fluid dynamics problems for molten salt reactors. The instructor explains that students have obtained slightly different results depending on whether they recalculated the fluid velocity field or simply used the previous solution from an earlier time step. While both approaches are technically correct, recalculating the fluid dynamics leads to a more converged velocity field, which in turn causes a slight change in the effective delayed neutron fraction (beta-effective). This occurs because precursors born in high-importance regions decay in low-importance areas as they move with the fluid, reducing their contribution to the neutron chain reaction. The discussion highlights that this effect is significant enough to alter beta-effective by hundreds of pcm, which has profound implications for reactor safety margins and control rod design.
To address convergence issues in the simulations, the instructor demonstrates how to adjust numerical schemes within OpenFOAM, specifically switching from a linear discretization scheme to an upwind scheme for the divergence operator in precursor equations. He explains that while linear schemes are more accurate, they can be unstable when dealing with moving fluids; the upwind scheme sacrifices some accuracy for stability by using values from upstream cells rather than interpolating between them. The session also covers practical computational considerations, such as estimating run times based on cell counts and time steps, and managing memory usage when solving for multiple fields like temperature and energy. A key technical point raised is that users must ensure their initial neutron flux guess is non-zero to avoid floating-point exceptions during the power iteration process, a nuance that requires experience to troubleshoot effectively.
The final part of the discussion outlines the setup for Assignment 4, which involves adding an energy solution to achieve a fully coupled multi-physics steady-state simulation including temperature effects. The instructor proposes simplifying the problem by assuming that temperature changes do not significantly alter the fluid velocity field in this specific high-convection scenario, allowing students to focus on implementing a heat exchanger with a fixed secondary side temperature of 900 Kelvin. This setup simulates a realistic reactor system where neutronics, fluid movement, and precursor transport are all interacting simultaneously. The session concludes by addressing power maneuvering strategies, noting that in such reactors, control rods are primarily used for safety shutdowns rather than power regulation due to the small beta-effective value, which necessitates alternative methods like variable speed pumps or boron concentration adjustments for power control.
Read the full video transcript
that well that will be our group
discussion for today because while it's
interactive you can discuss with us
and if you have questions about the
openmc part it's going to be in the
discussion of tomorrow from 4 to 5 30.
so today we stick to open Farm engine
form and we do that till the end so
go ahead to assignment three
and in probably 20 minutes or so I will
maybe half an hour I will give you the
solution
of assignment 3 and give you
uh assignment for
we'll start it and we will probably
finish it tomorrow during the offbeat
presentation because Alessandro told me
it needs just an hour for offbeat
so tomorrow we will finish assignment
four
so assignmentary today we start
assignment for wishing finish assignment
for tomorrow and openmc we discussed it
tomorrow afternoon
have we decided to do it tomorrow
funny
foreign
do you have the key effective
or is group one
okay group two
not yet group three
zero point
nine four one
another digit
another one
group four
foreign
right
this is interesting let's say
so this one so you are grouped two right
one
which kind of Divergence game have you
used
girls upwind
Carla you find the reason why
I think they are both
they are both correct okay
I speak about six PCM difference I think
the difference is that some of you
started from the previous solution did
not solve for fluid mechanics solved
only
for neutronics using the previous
velocity field
some of you started from the previous
velocity but solved for couple
neutronics and fluid dynamics
is that the case so for those of you
with the
that one where is solving also for fluid
dynamics or not
only the neutronics no Fleet Dynamics
for those of you obtained
this in your control deck did you have
solve three mechanics to true or to
false
true so that is the difference so what
happened is some of you use the velocity
field that we had before and solved on
that some of you recalculated it and
simply in 10 additional seconds it
changed a little bit because before we
we found our field after 10 seconds
which was almost a steady state if you
run it for another 10 seconds apparently
changes a little bit
so that's what happened for those of you
who kept solving fluid dynamics
you obtain the solution it is fluid
dynamically a bit more converged
so both are correct the difference is
very small it's just about how accurate
you are
so for those of you who resold free
Dynamics you just sold for additional 10
seconds you got the velocity field that
is slightly different
and that means that you have a slightly
different K effect why
you have different scale effective not
because the velocity field impacts
how you do
how many precastors Decay either outside
of the core or in low important low
nutrients importance regions
all right
shall I do the exercise for everybody
okay let's try to do the exercise for
everybody I will try
I said to start from
assignment to write yeah
too late
which is the Delta activity
stuff so this will be
1 minus
Guided by the
the map probably you will end up with
how much
yeah
get something with
120 PCM which is in the order of
magnitude of your
beta because we are saying that we are
moving the precautions so this has to
deal with the uh your delayed Neutron
and this is well I don't know I don't
know which is the beta here do you
remember Carlo
um
fraction here the effective static yeah
approximately 300 300 so we are more or
less in the same order of management
that which makes totally uh totally
sales
sorry this is minus because we are
we are losing so this means that our
with respect to the previous case our
Neutron delayed neutrons are created in
zones that has low importance so so in
which they contribute the probability to
contribute to the uh Neutron reactions
chain is lower
all right
um check what I do
all right for those one who did it right
check what I'm doing I'm getting tired
and I may forget things so
um
we said we would start from case two so
for the moment I just copy pasted case
two into a case three
and we said we want to start from a good
guess and the good guess was the
solution we had before
so what we can do is we go into zero
and we pretty much remove fluid region
and we take it from time step 10 of the
previous case so we just copy paste
uh not sure why it didn't sorry
huh not specified there are wonderful
something oh I might have it open in
not sure where actually
apologies to interrupt briefly
but we just checked for the posters and
can you raise your hand if you did not
yet put your poster there
one two
if you did not
if you did not one two three because we
are missing still
I think about six but you can just get
it already printed here at the info post
but they will close in 10 minutes so
you should just go ask them to to get it
if you don't have it yet print it if you
have it with you and you just need to
put it up then it's fine
so I'm removing
Brute Force oh yeah no it did disappear
this is what happens when you use WSL
sometimes
it does strange things so it would it
would say in window that I deleted it
that I couldn't delete it and now it's
not there anymore so apparently it
worked
um
WSL sometimes will do that so my
suggestion is always if you can use
directly Linux
um
so we go back to our starting case
stream
zero now we don't have fluid anymore
take another wind off
starting case three if you want inside
10 we still have the results we had
before from fluid region you take it you
copy paste and you have a good starting
point for a fluid Dynamic solution
and now what we want to do is solve the
coupled problem so starting case
system
contradict
and it's a little bit small I'm sorry
about that but 0 10 0.1 everything we
did before is more or less correct it
depends on when you want whether you
want to solve for fluid mechanics again
or not
according to Ali we can avoid that right
let me try so let's imagine we don't
solve for food mechanics so we will try
to get
his number
so we leave the neutronics as it was 0
10 0.1
um
actually anything else no I don't change
anything in contradict let's try it
let's see
I will check
that's the nice thing of simulations we
are not using a real reactor will not
break it
it looks like let's see
I did not so you guys did something
different
it's not yeah please
uh what you mean
no number iteration zero is because we
are
doing a steady state and you are
implicit lighterating for 100 times
so if you iterate even within the time
steps you will be doing the same thing
um
I'm curious because in my own how I
would have done it I would have done
what I did now and solved the three
Dynamics again getting what
people got that did
and some of you managed to get it
without re-running with Dynamics and
curious what you did
comes in
zero
uh
they took the end folder of case one
that makes sense
so it's true that you have two ways to
get huh
started from the end folder of the case
one
uh-huh
you didn't call you didn't copy paste
so you have two options here sorry for
about the confusions you have two
options either
you did what I did now so you start from
zero you copy paste your fluid but then
you solve again for free Dynamics
why because the neutronic solver needs
to go get data from
uh the fluid solver so you need to run
them couples for the neutral region to
realize oh I need to take the
fluid
um velocity if you don't do that it
doesn't know it it doesn't get it so
either you do what I did you start from
velocity
and just also solve for free Dynamics or
I believe
you guys started from
folder 10 of the case one right
this is
where did you place it
at the velocity you took the Velocity in
the fluid of the velocity of the neutral
region
which is exactly what I did and we're
getting we are not getting the same
result so either I did something
different or you did something different
and we have to figure out who did
something different this what I'm
showing you is wrong
so while we figure out what he did
I think I know but we try to understand
I will show you what I would do which is
in this case
we get
we copy pasted the fluid solution into
xero to get a good guess
that my suggestion is solve it again to
make sure that the thing is coupled even
if it takes more time so what I would do
is inside I would enter this the
contradict so system contradict
I will start from zero where we have
our good guess and in 10
and now we are solving fluid dynamics
again so you have to have a good
safe
initial time step
and you will need to
adjust the time step because we are
doing fluid mechanics again so we do
wait a sec
I don't find that just time step I'm a
bit blind In This Moment
oh yeah
I cannot hear you sorry
I'm actually curious to do that I will
try something sorry for the test just
give me a sec
I think we have to do what I'm doing
oh Jen four more thing I will haven't
forgot anything it will run for a while
because we are solving again
hmm
oh you know what you can make it easier
since we are starting from a good guess
we don't need to resolve again for 10
seconds we can solve for one
right because we are essentially having
converged field we don't need to redo it
again so we will just solve for one
second
and you're right I forgot the Phoebe
scheme right
of
I think I have a better time copy
pasting
so this is what I was telling you
um
sometimes you will think get things that
do not converge in open form and in
pretty much any
Library numerical Library out there
sometimes you will have to touch the
numerics
and when things don't converge in fluid
dynamics most of the time you get them
to converge using an upwind scheme
upwind scheme is relatively inaccurate
you need fine meshes
that is bounded
oh you do that you same thing as for the
other fields you tell
the name of the operator that you want
to discretize
and you say instead of Gauss leaner
because the default was Gauss linear you
say chaos
upwind
and I believe it is correct I think I'm
missing the underscore right
give me a sec yeah absolutely
so we are just telling
um
transform
discretize the precars the Divergence in
the precursors equation using an upwind
scheme instead of a linear scheme
those of you doesn't have any idea about
what an upwind scheme is I can
tell you actually so
when we discretize the Divergence
so imagine you have two cells
what is the value of the field
upwind is simply saying okay my value on
the face is equal to the value in the
cell that is happening to me so if you
have a velocity like this you're just
saying okay my value here is equal to
this one
plus that when you do linear you're
saying okay my value here is the linear
interpolation between my value here and
my value here
you can understand how linear is more
accurate
because we are saying okay my value is
actually an integration between the two
versus same well I use the one in the
other cell
but saying I use the one in the other
cell is more stable
um We call we call it a bounded scheme
um
why did I lose it
oh yeah
or Ctrl s
close it
so I think I changed everything I wanted
to change let's see if it works
so what we did we copy pasted our
velocity field into zero to get a good
guess and we are simply resolving from 0
to 10 both free Dynamics and neutronics
to get a solution that couples the three
Dynamics and the neutronics
this is going to be slow so while we
wait for this I would like to ask if you
have any questions and then I will give
you assignment 4 that we will finish
tomorrow
if you have any questions about this
even slower than I hoped for
but it's not that it is correct so when
you discretize things uh you can have we
speak about orders of convergence we
speak about first order second order
and essentially when you are first order
instead of second order you have
said to have the same accuracy you have
to have a finer mesh so you are less
accurate you're not wrong
Your solution will always converge to
the correct mathematical solution as far
as you have a fine enough mesh it's just
that it will require a finer mesh
that you can see how it is less accurate
I mean saying that
the value here
is equal to the value here it's an
approximation saying that it is the
average between here and here is the
better approximation
and the very general rule of thumb in
numerics when it's more accurate most of
the time is less stable
at almost inevitably always happen
and fluid dynamics is the bad guys on
linear is complicated to solve
Divergence is the most unstable operator
to solve
it will happen quite a few times that
you have to have an upwind instead of
linear scheme
and neutronics
we want both
no we want to have a different so what
we did before is we solve nutronics and
we get a case for a static fuel
now we are solving Us for free Dynamics
so our field will be circulating
circulating fluid means that our
precursors will move so we want a couple
solution we want to see how neutronics
is affected by circulating fuel
does that make sense am I not answering
the question probably
you can
sure
we have time you see how slow this thing
is
say again
can you switch on your mic I
I just wanted to like I just wanted to
confirm partially for my sake uh that
when we are bringing in the solutions
from the previous exercises for the
fluids we want to bring in the solution
from exercise one but the neutronic
solution should come from exercise two
actually for the electronic solution you
can take it it will not change much yeah
it's also really cheap right compared to
this it's very cheap so you can start
from a zero flat flat not Zero from one
flat flux okay
um and it will not change much but you
can you can initialize neutronic
starting from exercise two fluid Dynamic
starting from exercise one and use both
The crucial part is fluid dynamics this
is the one that takes long bread yeah I
just want to clarify that where the
solutions yeah yeah
uh actually why I was speaking I said
you could start from zero or one it's
not the same thing if you try to start a
solution with a flux zero
I think you will get a floating Point
exception because we are using power
iteration
and what we are doing is that we are
normalizing our solution based on the
integral in the previous solution and if
your previous solution was Zero it will
give you a miss an error so you have to
start from a flux that is not zero when
you solve for neutronics this
is little something that you have to
keep in mind
unfortunately we do not have a check
like if there is zero tell the user that
it shouldn't be zero is something you
have to figure out but I guess the
moment you get this floating point you
may think that there is some divide by
zero somewhere
um
it requires some experience uh we gave I
mean if you look at my slides this
morning and the slides we gave on Monday
we give rules of thumb some what
resources you need how much it will take
the how much resources you need it's
easy
um
think about the 30 000 cells per core
you know how many sets you have you know
how many Korean needs
memory depends if you're solving for
fluid dynamics very often fields or for
discrete ordinance where you have one
thousand
can be one gigabyte per
um
million cells so you can have several
tenths of gigabytes per million cells it
depends on how many fields you're
solving for
typically discrete ordinance where you
might have 30 directions and 30 energy
groups and all of a sudden you have 900
fields
memory requirements are a lot in free
Dynamics you have 10 Fields much less
so it's it's you can calculate them you
have to keep in mind these numbers
about how much time it requires well it
depends on how many time steps you are
running
if you have a solution that you have to
run for
like I'm working a little bit on nuclear
thermal propulsion you have something
that moves at several hundreds of meters
per seconds you can imagine that the
current number is horribly small you get
down to 10 to the minus 6 and you have
to run it for minutes
so we have a lot of 10 steps you have 10
to the minus 6
time steps that you have to run for
minutes so it's a lot it's going to take
a long time if you do something like we
are doing today we have a quarter number
of
we have a Time step of zero point
something for 10 seconds we don't have
many cells and it's gonna take probably
10 minutes
so depending on the following you can go
from minutes to hours to days there is
no
there are some rules that you can use
but there is no General answer to the
question
the Darcy for shimer I'm not using Darcy
for Shiner actually in these simulations
say again
it should be 2 power to 7
and you should get that by setting
eigenvalue to true and by setting P
Target in the reactor state to two to
the seven
Stefan
is to add on the question with the time
estimates what you can do is you can
look at the log file and you will see
there's a workload time and you can just
take the difference between let's say a
time step and the previous one so you
know how much time the solver takes for
one iteration or one time step and then
you can make some estimates with the
estimated number of time steps so you
get roughly a time of the Run
yeah all right so that's a way to
estimate how long to wait that's true
you can estimate at the beginning yeah
wait you should wait until you
It's tricky because imagine you have a
simulation when you have a loss of flow
your current number is going to change
it should run
seriously then it's okay if you keep
let's say let's say adaptive time
stepping and varying the flow rate of
this won't work yeah
but there are several ways and after a
while it becomes an art to understand
how long it will be your solution
looks like it's going in the right
direction so while we wait for this
thing I would like to
is there any questions otherwise I would
like to at least give you
an assignment that we will complete
tomorrow
and
I want to give it to you so that you can
start thinking about it
um assignment 4 is
the final
steady state multi-physics we are going
to add energy
so the temperature solution
um
let me find it
so the idea is
we add the solution for energy
we as usual we don't start from scratch
we copy paste the previous folder
and we want to solve for temperatures
still the achievement of a steady state
now to make it less computationally
expensive
I will ask you to assume that the fluid
dynamics is not affected by the
temperature which means we keep the
velocity field that we already have
is that always the case do you know if
usually we can say the temperature does
not affect our
velocity field
anyone
how does temperature
affect fluid dynamics which way
if you parameterize viscosity well
buoyancy there is another one
another one
density
is going to change your uh Mass
conservation equation is Gonna Change
now we don't have a guess we have a
liquid
and we have an extremely high convection
we're speaking about the reactor where
the field moves at 2-3 meters per second
so density is Not Gonna Change much
buoyancy is not going to change our
solution much because it is mainly
Force convection
so the reason why I'm telling you you
can forget about
how temperature affects fluid dynamics
is because it's a very good
approximation it's not perfect but it's
a good approximation we have a liquid
and we are enforced convection
now the tricky part
and I think I will need to give you some
help tomorrow about this
you will need a heat exchanger
now in gen form there are numbers of way
to simulate a heat exchanger
which makes things a bit more
complicated
there is one that is easy and that is
the one that we very often use when we
do multiphysics we assume that on the
secondary side there is a fixed
temperature
and what I would like to have is a
secondary side with this
um
fixed temperature of 900 Kelvin
you will need the volumetric area do you
know what a volumetric area is
is an area
of heat transfer divided by volume
all right so if you have I don't know
8x6
yeah
all right so imagine you have a very
strange heat exchanger where you have
primary fluid and the secondary fluid
and you have one tube it's the worst
heat exchanger ever
your volumetric area is the surface of
the tube
divided by the volume of the heat
exchanger is giving you in
um
intensive way instead of extensive way
what is the surface area of your heat
exchanger it's just this area divided by
the volume
is something you need
you can understand this is something you
need I mean heat exchanger is
characterized by a volumetric area so
you will need to give it how you will
find it out
um the tricky part about this exercise
is that if you were learning gen form in
time having a few days you would look
into the options you would read the
documentation and you would find out to
set
a fixed temperature something somewhere
in the frame of an exercise like we're
doing today and tomorrow you don't have
time to you know look into the
documentation so I'm telling you
and I will tell you tomorrow when we do
it the power model that you need to use
is called literally fixed temperature
all together fixed temperature
I'll tell you again this tomorrow
but you can understand that if you want
if ever reactor that now produce power
you need to evacuate the power if you
need to evaluate the power you need a
heat exchanger the easy way to set it up
is okay I assume that there is a
subscale structure that in our case is
the fluid in the secondary circuit that
has a fixed
temperature of 900 Degrees this is our
heat sink
so this is what I would like to do
tomorrow
we will take an hour in the offbeat
presentation
to try to finish exercise four why I
want to finish exercise 4 is because
this will give us a fully multi-physics
solution where we have temperature
neutronics
and movement of delay Neutron precursors
um
and this is a solution of a fairly real
system with the real 2D geometry
starting from there it's gonna be easy
to run a transient
all right so what we will ask you
tomorrow if you can after the course
try to stay here go home go in your room
go with your group somewhere and try to
run a transient but I will show you
tomorrow
that will be assignment five
it's you will see it's a relatively easy
assignment compared to what we did today
but step by step
today I will show you the solution that
we got for assignment 3. tomorrow we'll
do assignment for and we'll give you as
assignment for Friday
to do one transient
now let's hope that our simulation has
converged
hopefully
almost
are we far from that
or one
nine four one nine four one nine four
one nine four one is that the thing
that's for one nine four one seriously
um I clearly had a problem so I will
give you the solution tomorrow
I think I forgot to set the parameter
somewhere huh
again
oh
thank you I'm in the wrong common or
maybe
explain the thing
oh yeah you're right nine four one
nine two
four and four one nine two four man
I'm slightly different likely because I
sold for one second instead of 10
seconds again
depending on how long you do it you
change a little bit the solution
two four
we are two PCM away from that solution
so it probably because I run it for one
second a new guy ran it for 10 I assume
but it's okay
so I didn't do a mistake which is good
and we can look at the solution so first
of all well the key effect you find it
there you find it in many different
places
as Stefano says it's smaller than before
because we are losing some of the
precastors outside of our reactor
we look at the solution
after some time
so we ran to one so we have to go to
time step number one
refresh
let's see if it worked
so we looked at like fluxes let me just
look at the neutral region so otherwise
it gets
funny
um
did you expect the flux to change
with the Newton flux to change with the
movement of the neutrons
no anyone will expect it to change
think about it our neutrons are moving
at
what's the speed of a thermal Neutron
more or less
order of magnitude
2000 we are in a fast Spectrum reactor
what the speed of our neutrons
a lot
doesn't matter a lot even if it was
thermal we have to take about 2000
meters per second
our fluid is moving
at two
so the fact that our nuclei are moving
compared to our reference system by 2
out of 2000 which will probably be two
out of 200 000.
does it change our solution no usually
when we solve for when we study molten
salt reactors we assume that the neutron
field is not affected by the velocity of
the fluid
which is typically a nearly perfect
approximation it's even hard to call it
an approximation
things change when you want to simulate
when you want to
um
stimulate precursors
as gets number seven
so number seven is a relatively fast
decaying precursors
and even though it's fast decaying we
still see the effect of Transport so our
flux was perfectly centered here you
remember
now our precursor for Group of Seven
which is the fastest Decay are slightly
above what's happening is that our
precastors are born in a place
that they Decay somewhere else and their
pick is actually moved somewhere else so
our precursors are moving if you get
something that is moving at this
decaying a bit slower like group five
you'll see that effect even more why
because they are Decay more slowly they
have more time to get away from the
center of the core
and you look at precursor five I think
it's a good example because
sometimes we tend to think that the only
way we lose precastors is that they go
into the
heat exchange or the pumps and they are
outside of the core
but that it's an extreme case what's
also happening is that our precursors
globally are moving to low flux region
now if you're a bit Neutron transport
Savvy you know that flux and a joint
flux they tend to be very similar
so you are also moving to regions of
your core where that joint flux or the
Neutron's importance is smaller
so the value of your precursor decaying
here or here is not the same
so you are we are losing bit effective
also because some of our precursors are
decaying in low importance regions of
the core
so this is something that is extremely
important in molten salt reactors so
let's forget a little bit about genfoam
let's speak about physics
in this reactor if you have a static
field you would have a bit effect if
that is already small because this one
is a thorium-based reactor
the uranium plutonium version of it
let's say the Terra power version of it
is
uh uranium 5 but imagine you want to use
plutonium because you want to do burn so
both for tutorium and for plutonium
already your beta effect if your static
bit effective is
300 PCM more or less do you know how
much it is in a pwr
7 800 so we already have a bit effective
that is small
and all of a sudden we lose part of it
because you lose delay Neutron
precursors outside of your core
and you don't lose a little bit of it in
this half of it your bit effective goes
from 300 to 150.
all of a sudden you ever reactor doesn't
have much margin to prompt criticality
this can have significant impacts
on the design for instance you will not
typical thing that we do when we design
a reactor we say okay we don't want our
control rows to exceed
bit effective why because you don't want
be in a situation where you extract your
control Road and your reactor is super
prompt critical so for instance that
means that in a fast reactor like this
one
your control rod will have to be limited
to maximum 100 and something PCM
you want to achieve a cold shutdown of
this reactor
and you want each of your control row to
be maximum 100 PCM
you're gonna need a lot of control rods
and this is problematic for this reactor
this is one of the reasons why people
think about okay we don't get to a cold
shutdown we get to a hot critical state
or we change the shutdown mode we dump
our soul to in critically safe dump
tanks so we empty our reactor we put the
fuel into tanks
that are critically safe
one of the reason is the small beta and
actually the very high feedback
coefficient this reactors fit the
coefficient on the order of almio
Stefano 7 PCM per Kelvin density plus
temperature
five and seven PCM Perkins a lot on
minus negative which means if you have
to go from 700 Kelvin to
room temperature 300 is 400 kelvins
multiplied by
seven it's too difficult three thousand
more or less almost three thousand PCM
you would need
three thousand hundred and fifty twenty
twenty control rows authentic controls
is a lot in this reactor and also
controls will change your view
other problem is that you don't want to
put controls inside the reactor why
because that will affect your velocity
in the reactor
you don't want to mess with the velocity
so very often when we speak about molten
salt reactor people think about using
control drums
pentecontrol drums that get 250 PCM not
really so it's very complicated again
they're very ineffective so it's the
whole thing of the small bit effective
it makes the old design of the reactor a
bit complicated
I just wanted to conclude the demo day
on a more
nuclear engineering oriented note
um
and you know also to mention you know
you can use how you can use these tools
to get data that are essential to design
that are essential to understanding a
reactor and I'm pretty happy that we got
here in one day
so congratulations thanks for
trying to get there
tomorrow we will try in an hour or so
to add temperature solution to this
all right
um
how are we in the program
okay should we do poster
and just because we have we calculated
nine only positively so I think we can
do
um
to do it today and also into the old all
the posters okay
okay then we can do it today
okay so we have time okay so we can do
the post now straight away or we give 10
minutes right
straight away slowly slowly okay let's
slowly move to the poster please try to
prepare yourself
and again just to remind you because we
are it's just three minutes presentation
and then few minutes answering questions
um wishing you all good luck today
foreign
[Music]
how will power maneuvering be done in
for such reactor this is a very good
question probably Stefano can answer but
I believe the strut there are few
strategies that you can use you can use
variable speed pumps
you can drive
um using the secondary circuit
and you can do control rows you can it's
not forbidden I Am pro controllers but
the thing is you can have controls for
control or for safety shutdown safety
shutdown is more complicated because you
have to compensate for 3000 PCM
yeah but we'll be mailing you with the
power extraction which is actually what
you do in in light Water Reactor control
rod are not used to control your power
controlled in light Water Reactor are
used to control the temperature the
average temperature in the light Water
Reactor here probably we don't need to
control the average temperature even if
because if you just you are just
extracting power the average temperature
will be constant because you are not
adding any other reactivity coefficient
so the for the power maneuvering will be
mainly do just through extraction you
are extracting from the uh intermediate
or the uh Energy commercial system less
power
but control order mainly for safety
reason rather than let's say control
reason
it's called safety rules
[Music]
I'm not sure I understand the question
um
if you mean calculating the bottom
concentration that will make your
reactor critical
we don't we use an external reactivity
which is equivalent to using Boron we
can use Boron concentration as an
external input to the point kinetic
solver to as an additional feed
so if that answers your question
otherwise please ask again
be more specific about what you mean by
calculating Boron concentration
all right then thank you thank you Carl
thank you all and thank you online
participants and we will see you
tomorrow at 9 00 am