Boron Worth

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    Neutron X-section

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    Boron

    Boron used as chemical shim

    Reactivity control due

    Power transients

    Fuel B/U Fission Fragments Poisoning etc

    Shutdown margin during shutdown and

    refueling

    Dissolved in coolant uniformly Constant flux profile

    Avg. power density increase

    Better b/u

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    Boron

    Stable

    Weak acid hence less pH variation

    Remains dissolved if < 5%w/w at room temp

    B is 17.7% of H3BO3,B19.8% B10, 80.2 B11

    B10 Wa=3837 b; forBWa=3837.198=760b

    B10 is 1/v absorber

    eLiBnB 24273*11

    5

    1

    0

    10

    5 pp E

    eHn 42 3142*11

    5

    1

    0

    10

    5 pp E

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    Concentration =

    Concentration measured in ppm

    ppm | parts per million

    Boron

    610vsolventofmass

    soluteofmass

    610vsolventofass

    soluteofass

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    Neutron Moderation

    Collision with Nuclei

    \=2/(A+2/3)

    N = ln(Eh/El)/\

    \ = 0.948 for water

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    Nuclear Stability

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    Nuclear Stability

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    Binding Energy

    Let us analyze Fe-56, Z=26

    Atomic Mass = 55.934930 amu

    26 P, 30 N, 30 e

    ! 26(1.00727647)+30(1.00866501)

    +26(5.485803E-04)

    ! 56.463402

    ! 56.46340255.934930=0.528472 amu

    Interesting!!!!

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    Binding Energy

    1 amu = 1.660566E-27 kg=931.502 Mev/c2

    0.528472 931.502 =492.272725 Mev/c2

    8.79 MeV/neucleon

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    Nuclear Fission

    Splitting of a heavy nucleus to 2 or

    more light nuclei

    Release of Energy

    Fission is initiated by absorption of a

    neutron by fissionable material

    2 to 3 neutrons on the average are

    released in each fission. The fission fragments are radioactive

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    Nuclear Fission

    Nucleus contains P & N

    Electric Coulomb forces of repulsion

    between Ps short range strong nuclear forces which

    bind the particles of a nucleus together

    Normally a certain ratio of N/P is stable

    N/P ~ 1 is stable for smaller values

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    Nuclear Fission

    N/P > 1 is required for largernuclei

    For very large nuclei, (Zaround 90) no completestability Nuclei with large half lives are

    considered almost stable

    Nuclei tend to become stable

    by emitting radiations (E, F, p,n, positron)

    Many isotopes of larger nucleicould be almost stable

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    Nuclear Fission

    Binding energy is to be supplied to break a

    nucleus

    B

    E is eqt. to the mass deficit If energy is supplied to a nucleus by a K,

    the result may emission of any radiation to

    obtain naturally stable form.

    The stable form may be isotope of the same

    element or radioactive nucleus of another

    atom still changing to some stable nucleus.

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    Further Topics of Discussion

    Nuclear chain Reaction

    Uses of Fission

    Non fissionable absorption, escape

    k, criticality, critical mass/size

    Moderator

    Reduction in non fissionable capture by isotope

    separation (enrichment) Purification of materials(Fuel, moderator)

    Control of chain reaction, weapon or power

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