fundamentals of nuclear engineering17 point reactor dynamics solutions • most applications of...
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Fundamentals of Nuclear Engineering
Module 8: Low Power Reactor Dynamics
Dr. John H. Bickel
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Objectives:
Previous lectures described origins of neutron diffusion equation and balance required for reactor criticality. This lecture will:
1. Describe time dependent fission neutron source via 6-Delayed Neutron Group Model
2. Develop Point Reactor Dynamics neutron density model 3. Define: reactivity, delayed neutron fraction, neutron
lifetime4. Describe low power (Zero Feedback) reactor dynamics
response to step and ramp changes in reactivity5. Demonstrate simulated startup and low power operation
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Time Dependent Neutron Sources
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Each Fission produces
multiple neutrons:
• Fission yields on average: “ν” total neutrons• Fission yield increases slightlyslightly with neutron energy• For U235: ν(E) ≈ 2.44 • For U233: ν(E) ≈ 2.50 • For Pu239: ν(E) ≈ 2.90• In discussions of steady state criticality: timingtiming of of
neutron emissionneutron emission was not necessary to describe
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Physics of Neutron Emission• Neutron flux promptly emittedpromptly emitted at fission:
• Delayed neutron flux, characterized by β:
• Overall fission neutron source can be described as:
• Delayed neutron emission: combination of: • physical insight (known Isotope decay half-lives)• experimental observation
• β-decay of Br87 and I137 are known to be sources of longest delayed neutrons
• Other β-decay reactions have been lumped togetherlumped together in groups with roughly equivalent decay constantsroughly equivalent decay constants
)]()()1[()( tttS f βχφβν +−Σ=
)()1( tf φβν −Σ
)(tf βχνΣ
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Origin of ~55 sec. Delayed Neutron• 0n1 + 92U235 → fission 35Br87 is a fission product
• 35Br87 → 36Kr87 + 0β-1 +ν β-decay (neutron decays to proton)
• 35Br87 → 35Br86 + 0n1 neutron emission
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Delayed Neutrons Grouped into 6-Groups
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Delayed Neutron Groupsshow slight differences
for U233, U235, Pu239
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6-Delayed Neutron Groups Model:
• Each delayed neutron precursor group “Ci” is modeled via buildup (proportional to: βi) and decay (with rate: λi):
• Overall fission neutron source is expressed as:
),(),(),( trCtrt
trCiifi
i λφνβ −Σ=∂
∂
∑
∑
=
=
=−
+Σ−=
6
1
6
1
:
),(),()1(),(
ii
ii
if
where
trCtrtrS
ββ
λφνβ
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Substituting Neutron Source Term into Time-Dependent Diffusion Equation:
• Recall:
• Substituting 6-Delayed Neutron Group Model yields following system of 7 equations:
),(),(),(),(1),( 2 trDtrtrSt
trVt
trNa φφφ
∇+Σ−=∂
∂=
∂∂
6...1:
),(),(),(
),(),(),(),()1(),(1 26
1
=−
−Σ=∂
∂
∇+Σ−+Σ−=∂
∂ ∑=
iwhere
trCtrt
trC
trDtrtrCtrt
trV
iifii
aii
if
λφνβ
φφλφνβφ
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For Simplification: Separation of Variables
• Assume: Φ(r,t) = φ(r) VN(t) and: Ci(r,t) = φ(r) ci(t)
• Dividing out the spatial flux distribution from all equations, and substitution of the Geometrical Buckling coefficient: B2
yields:
)()()()()()(
)()(])(
)()1)[(()()(6
1
2
tcrtNrdt
tdcr
crtNr
rDVVrdt
tdNr
iifii
iiiaf
λϕνβϕϕ
λϕϕϕνβϕϕ
−Σ=
+∇
+Σ−Σ−= ∑=
)()()(
)()(]1)1(
[)( 6
1
22
tctNdt
tdc
tctVNBLdt
tdN
iifii
ii
iaa
f
λνβ
λνβ
−Σ=
+Σ−−Σ
Σ−= ∑
=
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Further Simplifications:
• Define average neutron lifetime as:
• Recognize full multiplication factor corrected for leakage:
• System of equations becomes:
122 )]1([ −+Σ= BLVl a
)1(/
22BLk af
+
ΣΣ=ν
)()()(
)()(1)1()( 6
1
tctNlk
dttdc
tctNl
kdt
tdN
iiii
ii
i
λβ
λβ
−=
+−−
= ∑=
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Limitations in Point Reactor Dynamics Model• 6-Delayed Neutron Group Model was derived assuming
fission product β-decay as the source• Delayed neutron production via 2.2MeV Deuterium photo-
nuclear (n,γ) reactions would be significant in any D2O moderated reactor such as CANDU. Overall dynamics would be slower than in PWR/BWR.
• 6-Delayed Neutron Group Model is function of assumed fissionable isotopes
• Buildup of Pu239 decreases β from 0.0065 – but never reaches pure Pu239 β value of: 0.0021
• Neutron lifetime is for thermal reactors thermal reactors and is typically on order of 10-4 - 10-5 sec. Neutron lifetime in fast reactor is on order of: 10-6 - 10-7 sec.
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Low Power Reactor Dynamics• Following discussions pertain to scenarios typical of very low very low
power reactor operationpower reactor operation•• NonNon--linear Feedback Effectslinear Feedback Effects on multiplication factor become
significant when usable power (heat) is being generated• Feedback effects will be discussed in subsequent lecture• Previously calculation showed: (1Wt) / (2.0x108eV/fission)(1.6x10-19Wt-sec/eV) = 3.1x1010fissions/sec.
• 4000MWt reactor with core loading of: 1.2x105kg 3.5% enriched Uranium would require an average neutron flux of ~ 1013 - 1014 neutrons/cm2-sec.
•• THUS:THUS: following discussion of low power reactor dynamics will relate to Φ ≤ 1010 neutrons/cm2-sec.
• In start-up range all reactors (PWR, BWR) behave same.
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Steady State Solution
• Steady state solution is obtained by setting:
• Solving for precursor concentrations yields:
• Which is simply: k = 1 - or in a state of criticalitycriticality
0==dtdc
dtdN i
lk
lk
ltkNtN
lk
dtdN
ltkNtc
i i
ii
i
ii
ββλ
βλβλ
β
+−−
=
+−−
==
=
∑=
1)1(0
)()(1)1(0
)()(
6
1
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Point Reactor Dynamics Solutions
• Most applications of Point Reactor Dynamics involve time dependent changestime dependent changes to multiplication factor: k(t)
• This generally implies solution of a messy system of nonnon--linear differential equationslinear differential equations.
• Several “simplifiedsimplified” cases exist which allow hand solution – when k(t) is a step or ramp
• However: Objective is not solving differential equations – but understanding reactor dynamics
• Thus: use MATHCAD
)()()()(
)()(1)()1()( 6
1
tctNl
tkdt
tdc
tctNl
tkdt
tdN
iiii
ii
i
λβ
λβ
−=
+−−
= ∑=
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Transition from Critical to Supercritical• Consider situation where system is initially critical: k = 1.0• Adjustment made at 10 seconds and system becomes
slightly supercritical: k = 1.002• Initial conditions:
• Numerical simulation of this scenario yields following
0==dtdc
dtdN i
0)0(
)0()0(
NNlkNc
i
ii
=
=λ
β
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Transition to Supercritical with k = 1.002
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Transition to Supercritical with k = 1.002• Log N(t) gives different
perspective• Note “prompt jumpprompt jump” with
“exponential tailexponential tail”• This is related to physics of
prompt vs. delayed neutrons
• After prompt neutron transients die out, N(t) can be modeled as:
N(t) = Aoexp(ωt)• Reactor period: T = 1 / ω
depends on magnitude of change in k
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Delayed Neutrons:Delayed Neutrons: Key to Reactor Control
• Neutron life-cycle was previously described as →
• Time constant of one cycle: ℓ = 10-4 - 10-5 sec.
• No mechanical device known could operate to intervene in chain reaction growing this fast
• Removing between 0.0021 – 0.0065 neutrons in each 10-4 - 10-5 sec. cycle dramatically cuts back on neutron in growth of chain reaction.
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Reactor Dynamics With vs. Without Delayed Neutrons
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Transition to Subcritical• Consider situation where system is initially critical: k = 1.0 • Adjustment made at 10 seconds and system becomes
subcritical: k = 0.99• Initial conditions:
• Numerical simulation yields following
0==dtdc
dtdN i
0)0(
)0()0(
NNlkNc
i
ii
=
=λ
β
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Transition to Subcritical Simulation
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Transition to Subcritical Simulation
• Previous calculation was: k = 1.00 to k = 0.99
• Suppose reduction was 3x• Change: k = 1.00 to k = 0.97• Observe shape combination
of “prompt dropprompt drop” and “exponential tailexponential tail”
• Again this is caused by differences between prompt vs. delayed neutrons
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Concept of Reactivity
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Reactivity is Fractional “k” Deviation from 1.0
• Reactivity is defined: ρ(t) = (k(t) – 1) / k• Neutron Lifetime is slightly redefined: Λ = ℓ / k• This formalism works well in vicinity of critical system
conditions – where studying deviations of: ~ +/- 0.03• Substituting these changes into Point Reactor Dynamics
equations yield following system of equations:
)()()(
)()())(()( 6
1
tctNdt
tdc
tctNtdt
tdN
iiii
ii
i
λβ
λβρ
−Λ
=
+Λ−
= ∑=
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Comparison of keff vs. ρ
> 0.0> 1.0Supercritical:
= 0.0= 1.0Critical:
< 0.0< 1.0Subcritical:
Reactivity:ρ
Multiplication Factor: keff
Parameter:
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Expression of Reactivity Units• Reactivity can be expressed directly as: ∆k/k or, as
comparison to: ββ• Old texts such as Glasstone & Sesonske: “Nuclear Reactor
Engineering” (1967) used units of: $, ¢• ρ = 1$ is reactivity change to/from critical conditions
equivalent to ρ = β, or ρ = 0.0065• ρ = 1¢ is 1/100th of this, or: ρ = ~6.5x10-5
• 80’s SARs use: ∆k/k, or %∆k/k• 90’s SARs use: “pcm” (per cent milli-rho) 1pcm = 1x10-5
• In Europe, or former Soviet Countries reactivity is expressed directly in units of β, example: ρ = .12β
• Problem with using units of β: it is not constantit is not constant• Recall that with: U235 burnup/ Pu239 buildup, ββ decreasesdecreases
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Prompt Drop From Control Rod Insertion
• Sudden change in reactivity results in “Prompt Drop”
• Followed by exponential decay
• Magnitude of initial drop can be directly related to reactivity change
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Prompt Drop From Control Rod Insertion• Assume control rod reactivity change: control rod reactivity change: --ρρCRCR is made faster
than shortest delayed neutron precursor response time• Initially precursor populations would be given by:
• Upon substitutions, summing precursor contributions, point reactor dynamics equation becomes:
• Expression is linear differential equation solvable as:
Λ≈
i
ii
Ntcλ
β )0()(
)0()()()( NtNdt
tdN CR
Λ+
Λ−−
=ββρ
)0(])(exp[)0()0()( NtNNtNCR
CR
CR
CR
CR βρββρ
βρρ
βρβ
+≈
Λ+
−+
++
=
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Prompt Drop From Control Rod Insertion• Doing a little rearranging, ratio of before/after flux
immediately after control rod drop would be:
• This is historic method of checking individual control rod reactivity worth during low power startup testing.
• Example: ρCR = 100pcm = 10-3∆k/k = 0.154β = 0.154$• Dropping control rod would result in immediate drop to:
N0/N1 = (ρCR + β)/ β = (1.154 β)/β = 1.154N1 = N0/1.154 = 0.866 N0
βρ
ββρ
⎟⎟⎠
⎞⎜⎜⎝
⎛−≈
+≈
11
0
1
0
NN
NN
CR
CR
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Reactivity Excursions from Low Power• Normal process of reactor startup involves slow, controlled
evolution to increase keff to point of criticality
• Prior to reaching criticality flux increases linearlyflux increases linearly as reactivity increased
• When criticality reached, flux increases exponentiallyflux increases exponentially up to point of power/heat generation
• Heat production results in non-linear feedback that will slow down and halt further power increase until reactivity added
• Sudden spike in neutron flux, with corresponding spike in fuel/coolant temperatures obviously needs to be avoidedobviously needs to be avoided
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Reactivity Excursions from Low Power• Example taken from ANO-1
FSAR• Assumed initial flux: 10-7%• Assumed reactivity insertion
rate: dρ/dt = 1x10-3∆k/k/sec. = 100pcm/sec. = 0.154β/sec
• Note: prompt dropprompt drop followed by exponential decayexponential decay tail
• To avoid startup power excursions, automatic trips provided on: hi flux, hi log power.
• Better to avoid hi dρ/dtadditions !
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Limiting Rates of Reactivity Addition
• Given that operators bring reactor to criticality using control rods (BWRs/PWRs) or dilution of soluble Boron (PWRs)
• Features should exist to: • Alarm to operator if too much reactivity is being added• Terminate adding further reactivity• Initiate automatic shutdown if addition rate is excessive• Measuring reactivity is difficultdifficult• Measuring reactor period is actually straight forwardstraight forward
given ability to measure log N(t)• Desire is to limit/control reactivity addition rates based
upon reactor periodreactor period
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“Reactor Period” is NOTNOT about periodic or cyclic type phenomenon
• Many mechanical and electrical systems involve simple harmonic systems
• Period: T = 1/ ω
•• Reactor PeriodReactor Period is inverse of exponential rate constant
•• Reactor PeriodReactor Period: T = 1/ ω• In reactor physics “period” is
inverse rate of exponential growth:
N(t) ~ N0 exp (t / T)
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Reactor Period and Reactivity• Previous simulations of
supercriticalsupercritical show long term exponential growth
• Exponential growth is expected because of chain multiplication, k > 1.0
• Rate of exponential growth or “inverse of period” is directly related to ∆ρ
• Larger changes from critical (∆ρ) result in shorter periods.
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Reactor Period and Reactivity• Assume overall solution of form: N(t) = ∑Ai exp(ωit)• Assume unique long term relationship between reactivity
change: “∆ρ” and reactor period: “T”• With: ω = 1/T, assume after short term transients die out,
that: N(t) ~ Aoexp(ωt) - all higher order terms gone• After initial transients, precursor concentrations can be
expressed: Ci(t) = Aoexp(ωt)βi / Λ λi
• Substituting into point reactor dynamics equation yields following:
∑
∑∑
∑
=
==
=
+Λ+Λ=
+Λ−=
+−
++
Λ−=Λ
++⎟⎠⎞
⎜⎝⎛
Λ−
=
6
1
6
1
6
1
6
1
)()(
)()(
)()()()(
)()(
i i
i
i i
i
i
ii
i i
ii
i i
ii
λωωβωωρ
λωωβωρ
λωβλ
λωλωβωρω
λωβλβωρω
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Reactor Period and Reactivity Graphical Solution
• Specific reactivity value ρ chosen• Horizontal line drawn to find intersection with roots• Roots identified: 6 always negative, 1 root dependent on
whether ρ is positive/negative
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MATHCAD Plot of Negative/Positive Roots• Six negative valued roots are associated with delayed neutron
precursor group decay processes (ωi is always negative)• Most right-hand root can be positive/negative depending on
whether ∆ρ is positive or negative• General solution is of form: N(t) = ∑Ai exp(ωit)
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How Reactor Period and Reactivity Used to Control Reactor Startup
• Reactivity not measurable • Log power rate is measurable• Log power rate can be
converted to Reactor Period: T• Reactivity can be computed
from:
•• Prompt Critical PeriodPrompt Critical Period ~ 2.993 sec. (for assumed: Λ,β values)
• Operator displays and Control Rod Withdrawal Prohibit features are quite common
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Period Meters on Russian RBMK-1500
Redundant Reactor Period Meters (∞,10sec) shown on Control Rod Panel
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Reactimeter Panel on Russian RBMK-1500
Direct Indication of Startup Reactivity (like shown above) was added on all Russian Reactors following April 1986 Accident at Chornobyl Unit 4
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Summary: Low Power Reactor Dynamics
• Delayed neutron fraction: β - plays key role in ability to control dynamics of nuclear reactors
• Point reactor dynamics model is commonly used as basis for all safety analysis work – subject to assumed limitations
• Low power reactor dynamics not subject to feedback effects found at power operation
• Subcritical: keff < 1.000, ρ < 0.0, T ~ ∞sec.• Critical: keff = 1.000, ρ = 0.0, T ~ ∞sec.• Supercritical: keff > 1.000, ρ > 0.0, 10 sec. < T < ∞ sec.• Prompt Supercritical: keff > β +1.000, ρ ≥ β, T < 2.993 sec.• Reactor startup involves slow controlled evolution from
subcritical to critical operation followed by controlled exponential rise to point where heat is being generated.