Report-Choking flow application in nuclear reactor core

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    Choking flowas a application in nuclear reactor core

    (Report)

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    Choking is term in fluid mechanics represent that the flow is choked. When

    flow is choked, the flow rate attained its maximum value for other parameter

    like stagnation pressure, length, diameter of pipe etc. Choking generally can

    be seen in Nozzles, Orifice. At minimum cross section, the flow attain M=1

    i,e. sonic flow.

    m.= mass flow rate, kg/s | C= discharge coefficient, dimensionless

    A= discharge hole cross-sectional area, m\ | k= cp/cv of the gas

    = real gas density at P and T, kg/m

    P0= absolute upstream pressure of the gas, Pa

    At the choked area we can measure the mass flow rate and amazingly

    further reduction in downstream pressure doesnt affect mass flow rate.

    Hence we called conditions to be choked at critical location.

    Fig(1.1)

    Likewise choking also occur in liquid flow through pipe, but equations

    representing choking water flow or fluid are different than gas choking flow

    as gas is compressible but water is not and there are many other reasons.

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    Choking flow has many applications in our life. Indian nuclear power station

    production is about 3.2% of overall electricity production. Nuclear power

    plant has very basic setup. Nuclear core where fuel rods are mounted

    undergoes nuclear fission and produce extent of heat that heats water and

    heated water allowed to pass through heat exchanger in which it evaporate

    water. The evaporated water allowed to rotated turbine blades whichproduce electric power.

    Inside core Uranium atoms undergoes fission reaction and produce heat.

    To control extent of heat control rods are introduced. Main purpose of

    control rod is to absorb neutrons produced in fission process and break

    /control chain reaction. To cool / rapid cool the fuel rods coolant is use.

    Generally water serves the purpose of coolant in most of nuclear power

    plants.

    But in case if something went wrong and coolant stats escape from the

    core, fuel rods will heat up and results can be devastating. To avoid such

    consequences we need to prepare for backup plants like ECCS

    (Emergency core cooling system) and RELAP. This fill up core will coolant

    through different methods so that fuel rod remain at low temp.

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    Fig 1.3

    Water inside core has tendency to for two phase mixture or superheated

    vapour because of heat of fuel rods but the pressurizer apply pressure on

    water and make it subcooled (Compressed) as shown in above (see fig 1.3)

    Temperature can reach upto 250oc 300 oc. Hence pipe which used to flow

    high pressure high temp. fluid may fail due to metallurgical problem. This

    cause cracks to form or even it can break. At this condition our ECCS canbe used for emergency backup for coolant. But how to design ECCS?

    ECCS need mass flux (mass flow rate per unit area) at break location and

    other parameters like leak rate and depressurization rate. Hence we need

    dedicated calculations for the mass flux and depressurization rate at break

    or leak.

    In this reports we are going to discuss how to form the basic models that

    can predict the mass flow rate (critical) and depressurization rate. Many

    models are proposed for choked flow, we are going to discuss few of them

    and based upon that we are going to form our ECCS and other cooling

    arrangement plans.

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    It is experimentally proved that flow choked at break or leak and hence it is

    useful tool for our calculations of mass flow rate. We have given that our

    inlet conditions are subcooled with known temperature and pressure. Then

    it would be so easy to from direct relation between mass flow rate and inlet

    and exit parameters. But is it?

    No. As we can see from fig 1.3 water is subcooled at inlet but as pressure

    decreases water is losing the temperature. At certain point water will starts

    to convert into steams. Hence our pipe flow is no longer single phase flow.

    Both steam and water at high temp will start to escape from break of leak.

    All calculations that we are going to make must be applicable to both

    vapour/steam and water and we know water and steam have different

    properties. So we need to understand different property of steam and water.

    Little observation can be made like water and steam velocity is same or

    different at critical location or water and steam are in thermodynamic

    equilibrium or not. If it became possible to form relations between water and

    steam then it will be lot easier to formulate relations of mass flow rate.

    Based upon this conditions few models are proposed are given below.

    1. Homogeneous Equilibrium Model(HEM)2. Non-Homogeneous Equilibrium Model (NHEM)

    3. Homogeneous Non-Equilibrium Model (HNEM)

    4. Non-Homogeneous Non-Equilibrium Model(NHNEM)

    Homogeneous means that our two phases has same velocities.

    Non-Homogeneous means two phase velocities are different.

    Equilibrium means that two phases are in thermodynamic equilibrium.

    Non-Equilibrium applied to two phased with thermodynamic instability.

    Based on those models it is very easy to understand choking flow criterion.

    This models may not give exact value but sufficient to design and operate

    ECCS.

    Many researchers worked on this topic and Moody and Henry-Fauske

    Models are most followed. Based on their studies and other paperworks we

    are going to form our models.

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    1. Homogeneous Equilibrium Model(HEM)

    At exit we have two phases; vapour and water. In this model we are going

    to treat the fluid as pseudo mixture that can be described by same

    equations as a single equivalent flow. Hence, our velocities u (l) and u (g)

    are same and two phases are in thermodynamic equilibrium.

    The main criteria to achieve thermodynamic equilibrium are long length. In

    long sections, there is enough time to achieve thermodynamic equilibrium

    and hence HEM is good way to analyse critical flow rate in long pipe flow.

    The basic conditions are (key)

    1. Same Velocity

    2. Phase Equilibrium

    3. Pseudo fluid (considering two phase mixture as a fluid)

    The Bernoulli equation in its general differential form of energy balance per

    unit mass can be written as

    Where;

    P= pressure

    v= specific volume

    V= velocity

    g= gravity

    D= diameter

    F= friction factor

    L= length W

    W= work done

    c = critical & e=external

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    Assuming no work interaction and no elevation changes.

    Our formula become

    As we already mentioned that we are going to assume the two phase

    mixture as pseudo fluid, hence we must not hesitate to take specific volume

    of pseudo fluid as specific volume of mixture and hence velocity of pseudo

    mixture can be written as

    Where;

    m= total mass (mtotal=mwater+ mvapour)

    A= orifice area (break area)

    V= velocity

    v= specific volume (total)

    Replacing Velocity from (3) in equation (2).

    The final equation become

    Substituting = 1/ v and integrate we get

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    Friction factor can be calculated from colebrooks formula or blasius

    correlation for Re< 105

    Based on experimental data and calculations we find value of f can be

    taken approx. 0.003. Later we can compare our calculated data and

    measured data based on different value off.

    To find maximum flow rate, following things are calculated,

    1. Inlet pressure Pb is measured

    2. Exit pressure Pe is measured

    3. Quality at exit is calculated

    Considering isentropic and adiabatic flow, hence no heat interaction to

    surrounding. By enthalpy conservation we can write

    Hb = X Hg + (1-X) Hf

    Where Hb is enthalpy at entrance of pipe

    Hf is enthalpy of water at exit

    Hg is enthalpy of vapour at exit

    X is quality at exit

    Hence X = (Hb Hf ) / Hfg

    To calculate density and specific volume of mixture, we need to consider

    specific volume of each phase and hence

    vm = X vg + (1-X)vf and = 1/ vm

    As we studies in choking flow reduction in back pressure increases mass

    flow rate. Hence for each pressure drop (exit) interval density is obtained

    from (4) and arithmetic mean value is used in (5) to calculate mass flux.

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    From this graph we can see that as exit pressure decreases our flow tends

    towards constant mass flux line. But after some pressure decrease in exit

    pressure will not lead to increase in mass flux (like in graph after 4.0 atmany decrease in pressure does not cause mass flux to change). Each graph

    is drawn for different inlet pressure. As we can see that as pressure

    decreases mass flow flux for same exit pressure decreases. In nuclear

    reactor core, we have depressurization rate hence we can plot series of

    graphs for different inlet pressure.

    But in case of real life problem, we have same exit pressure. Based on

    experiments done so far, it is prove that the pressure inside nuclear reactor

    core is more than sufficient to cause choking in flow for exit pressure equal

    to atmospheric pressure. Hence we need not to worry about exit pressure

    and hence mass flow rate or mass flux is independent of exit conditions and

    it can easily predict.

    Restrictions:

    As we are talking about HEM (Homogeneous Equilibrium Model), for

    phases to be in thermal equilibrium, sufficient time must be allowed for

    thermodynamic stabilization. Hence for HEM, flow must be taken in long

    pipe section where there is sufficient time for phase equilibrium. HEM can

    give best predicted value in long sections and deviate from observed value

    for short pipes and also pipes with short bore.

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    Above diagram is plot between mass flux observed at exit and pipe length

    for testing HEM.

    Looking at Exp. Data graph (with surface tension) and Model (smooth

    entrance) we see huge deviation for pipe length less than 600 mm. Though

    600 mm is very short length but we can see appreciable convergence of

    Experimental data and data tabulated by HEM.

    This table shows that mass flux decreases as time passes due to

    depressurization in core. Total water/coolant blow down can be calculated

    by integrating mass flow arte Vs time equation or simply area under cure

    (shown above) multiplied by orifice area. Using this model we can designECCS and amount of coolant/water needed.

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    2. Homogeneous Non-Equilibrium Model(HNEM)

    The major phenomenon that are ignored in HEM two phase flow are Bubble

    nucleation, interphase heat, mass and momentum transfer. All this

    parameter if taken into account, our model will be more complicated to

    understand and to solve.

    Hence in HNEM we will solve one dimension mass and momentum

    conservation ad transfer equations with bubble nucleation phenomenon and

    phase change. As HNEM is complicated model to solve and different

    approached as been developed which can be categorized as follows:

    1. Empirical Model (based on observation and experiments)

    2. Physically Based model for thermal non-equilibrium

    3. Two.-Fluid models

    In our report we are going to discuss Henry-Fauske Empirical Model, which

    is rather simple to explain and understand.

    They introduce coefficient N which is fraction of equilibrium vapourgenerated. From this value we can calculate non-equilibrium steam

    generation. Also assuming are VL = VG we are going to form our HNEM

    Empirical Model.

    Henry-Fauske assume that non-equilibrium steam X quality is proportional

    to equilibrium steam quality X

    As discussed N is dimensionless constant determined by empirical

    calculations of Henry-Fauske and observed that it depends on geometry of

    break or leak or test section. N can vary from 7-100. Flashing is process of

    rapid conversion of liquid into steam. As we assumed the fluid at inlet is

    subcooled means it is compressed and when it brought isentropically tolower pressure (fig.1.3) it start to flashing into vapour. This phenomenon

    occurs below some pressure called depressurization pressure.

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    First we will discuss the flow under subcooled inlet and next based upon

    that we will determine flashing process and calculate mass flow rate.

    Critical Flow with Subcooled Inlet:

    Fig 2.1

    This fig. is graph between pressure (local pressure) and distance along testsection (Reocreux Test) with subcooled inlet.

    For this test we are taking inlet pressure about 1.8 bar which is very low

    compared to actual nuclear core pressure. As we move from inlet of test

    section toward downstream local pressure P starts decreasing and

    saturation pressure PTi corresponding to inlet water temp. Ti reached. After

    pressure PTi water became superheated and at pressure Pb there is enough

    superheat first bubble to form. See fig2.2 [A]. After that point local pressure

    continue to decreasing and reach Pd where significant amount of steams

    begins to form, See fig 2.2 [D]

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    [A] [B] [C] [D]

    Fig 2.2 we can see bubbles are forming before vaporization.

    From Reocreux test fig 2.1 we can see that Pd is reached at end of pipe

    (constant diameter) or at critical location. Hence Pd=Pc. Where Pc is

    pressure at critical location.

    From fig.2.1 we can see that steam volume fraction is zero (0) upto the

    critical location and starts increasing rapidly beyond that point. At that

    location (here at critical location) one can define critical pressure difference

    Pd which can be defined as pressure below saturated pressure

    corresponding to water temperature required to form significant amount of

    steam.

    In diffuser section local pressure continues to decrease and steam volume

    fraction and steam content increases. From calculated steam volume

    fraction and local pressure P we can calculate non-equilibrium steam

    quality X. For equal water and steam velocity we can write

    Where g is vapour density and l is liquid density. As we are considering all

    process in this model are isentropic, hence from isentropic relations we can

    calculate liquid entropy

    Where So is stagnation entropy and Sg is saturated steam entropy at local

    pressure P. We can find P + Pd from below

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    Fig 2.3

    From this we can calculate Pd along diffuser section and can be seen infig. 2.1. We can see that Pd relatively remain constant along diffuser

    section. This determine strong non-equilibrium between two phases.

    To measure degree of non-equilibrium in pipe and diffuse r section we need

    to calculate equilibrium steam quality from isentropic calculations.

    So is stagnation entropy and Sg and Sf are vapour entropy and liquid

    entropy at saturated pressure Ps taken equal to the local pressure.

    Corresponding calculated from equation 3 called as eq called equivalent

    volume fraction. This is shown in fig 2.1 by dashed line.

    Conclusions: (examining fig 2.1)

    1. Nucleated bubble nucleated at pressure Pb do not get opportunity to

    grow due to limited time for heat transfer between them and superheated

    liquid. As heat transfer rate between steam and water is low due to equal

    velocities.

    After studying other Reocreux test (with less subcooled inlet) we found that

    flashing need not to occur at critical location and bubble can get more time

    to grow but at last there will be non-equilibrium in critical location. We foundthat Pd in both case are same and hence we can find Pd where significant

    amount of steam begins to form. Corresponding non-equilibrium steam

    volume fraction can be plotted and shown in fig 2.4

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    Fig 2.4

    From Alamgir and Lienhard subcooled depressurization model we arrived at

    Where is surface tension, k is Boltzmanns constant, Tc is critical

    temperature, is rate of depressurization, Tr is reduced temp (Ti/Tc)

    For pipe depressurization Alamgir have recommended

    Where KL is liquid thermal conductivity, is liquid viscosity, Hfg is heat of

    vaporization, Pr is prandlt number, T* is difference between stagnation

    temp and temp at critical location.

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    Above equation represent relation between different term including nozzle

    diameter or Critical location diameter D. V* is critical velocity.

    Flashing and Critical Flow Model:

    Proposed flashing model was formulated from result obtained from fig 2.1and fig 2.4. We assumed

    1. The first significant steam form at Pd below saturation temp

    corresponding to liquid temp. Hence liquid temp has to be superheated by

    amount Tdcorresponding to Pd.

    2. Any temp formed will be at saturation conditions corresponding to

    pressure P.

    Assuming isentropic flashing process we can calculate non-equilibrium

    steam quality

    Where so is stagnation entropy, sg is saturated vapour entropy at pressure

    p and sf is superheated liquid entropy at temp T+Td where T is sat. tempcorresponding to P. As explained earlier we can write

    From enthalpy balance over control volume give by equation

    For frictionless isentropic fluid, the local pressure gradient with distance z is

    given by

    After lengthy iteration and approximation in model we arrived at

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    Where is depressurization rate, and Gc is flow rate at critical location and

    Gt is maximum flow rate.

    Using this relation we can find decompression pressure change

    and neglecting any density change at

    critical location we from

    Comarison:

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    Comparison Between observed mass flux with calculated mass flux ofHEM and HNEM

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