PDF 3.2 Neutrons Are Special

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    Nuclear Reactionsand Radiation

    3.2 Neutrons are special !

    L. R. Foulke

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    Neutron Interactions Fission

    As the fission products de-excite and decay overtime they release

    rays particles, particles, and neutrons from

    radioactive decay

    These emissions are referred to as delayed.

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    Neutron Interactions

    Fission

    Fission fragments (some unstable)

    Pre-Collision

    proton

    neutrons

    Electrons (beta particles)

    ray

    Image Source: See Note 1 for Ionized nucleus

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    Nuclear Reactions Reactions between a subatomic particle (neutron) and

    a nucleus are of particular interest.

    Nuclear reactions are most easily caused by neutrons Charged particles cant reach nucleus due to

    electrostatic forces

    For convenience we use a shorthand notation todescribe nuclear reactions

    Like everything else in nature, nuclear reactionsmust obey balance equations.

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    Nuclear Reactions(n,n)

    (n,n)

    (n,)

    (n,2n)

    (n,f)

    After formation, unstablecompound nuclei may

    stabilize through one of

    several decay mechanisms.

    n Not all neutron interactionshave unique outcomes.

    Image Source: See Note 2

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    Nuclear Reactionsn Neutron Induced Reactionsn Elastic Scattering (n,n)

    n Inelastic Scattering (n,n)

    n (Radiative) Capture (also called n, reactions)

    nH)*D(nH 101

    1

    2

    1

    1

    0

    1

    1 ++

    2656Fe+

    0

    1n (

    26

    57Fe)*

    26

    56*Fe+

    0

    1n+

    0

    0

    ++0

    0

    236

    92

    236

    92

    1

    0

    235

    92 U)*U(nU

    ++0

    0

    24

    11

    24

    11

    1

    0

    23

    11 Na)*Na(nNa

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    Nuclear Reactionsn Neutron Induced Reactionsn Charged Particle (n , ) (n,p) (n,d) (n,2p) . . . .

    n Multiple Neutron (n,2n) (n,3n) . . . .

    n Fission (n,f)

    4

    2

    7

    3

    *11

    5

    1

    0

    10

    5 LiB)(nB ++

    nUUnU1

    0

    232

    92

    *234

    92

    1

    0

    233

    92 2)( ++

    0

    0

    1

    021

    *236

    92

    1

    0

    235

    92 )( ynxFFUnU ++++

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    Nuclear Reactions

    nOther Nuclear Reactions (Neutron as a Product)nAlpha ( ,n)

    n Gamma ( ,n)nCC)*(Be

    1

    0

    12

    6

    13

    6

    4

    2

    9

    4 ++

    nHH)*(D 1011210021 ++

    Neutron source

    Neutron source

    Referred to as a photoneutron reaction

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    Nuclear Fission Of all the nuclear reactions wehave considered, fission is the

    most interesting

    Occurs only in the heaviest,least stable atoms

    Can occur as a natural decaymode (spontaneous fission),

    or due to a nuclear interactionby another particle (a neutron)

    n Only the Actinides (Z 89) are large enough to allow fissionn Only 2 elements are naturally occurring thorium (Th) and Uranium (U)n Only 3 total naturally occurring isotopes 232Th, 235U, and 238Un Other isotopes can be artificially produced by neutron bombardment

    Image Source: See Note 3

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    Energy Released During Fissionn Sensible energy released during fission

    MeV %

    Fission Fragments (Kinetic Energy) 168 84.0

    Neutrons (Kinetic Energy) 5 2.5

    Prompt Gamma Rays 7 3.5

    Delayed Radiations

    Beta Particles* (Kinetic Energy) 8 4.0

    Gamma Rays 7 3.5

    Radiative Capture Gammas 5 2.5

    TOTAL 200 100

    Fissioning one uranium atom providesnearly 100,000,000 times as much energy

    as combusting one carbon atom.

    *Neutrinos account for another

    12 MeV that cannot be detected

    7.5 %Max. Decay

    Heat

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    Energy Released During Fission

    Fission

    Delayed Energy Release

    Prompt

    Energy Release

    Image Source: See note 2

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    Prompt Energy Release Accounts for90% of energy released in fission

    Kinetic energy of fission fragments ( 84%) Kinetic energy of free neutrons (2.5%) Gamma rays emitted during fission (3.5%)

    Random number of free neutrons produced in fission Between 0 and 5 neutrons produced per fission Average (denoted ) between 2-3 produced per fission

    Prompt energy is divided between fission fragmentsand neutrons and gamma rays

    Free neutrons can be produced with a wide range of initialvelocities (kinetic energy).

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    Neutron Energy Spectrum

    Energy Range: 0.1 10 MeV

    Most ProbableEnergy:

    0.7 MeV Average Energy

    2 MeV

    Fission Neutron

    Energy Distribution

    Image Source: See note 2

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    Delayed Energy Release Accounts for10% of energy released in fission

    Radioactive decay of unstable fission products ( 10%) Energy may be released over hundreds of years as harmful

    gamma radiation.

    Explains why spent nuclear fuel is difficult to handle. The type and amount of delayed radiation depends

    heavily on what daughter nuclei are produced during

    fission. Fission splits original nucleus randomly into two pieces Fission fragments are typically not the same size

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    1. Public domain:http://en.wikipedia.org/wiki/File:Alpha_Decay.svg

    2. Reprinted with permission from theAmerican Nuclear Society. NuclearEngineering Theory and Technology ofCommercial Nuclear Powerby Ronald AllenKnief, 2nd Edition. Copyright 2008 by the

    American Nuclear Society, La Grange Park,Illinois. Figure 2-4 (slide 6), 2-7 (slide 13),2-8 (slide 15).

    3. Creative Commons: Adapted fromhttp://en.wikipedia.org/wiki/File:Periodic Table Radioactivity.svg

    Image Source Notes