2.4 just like your checkbook-it all has to balance

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    A Look at NuclearScience and Technology

    Larry Foulke

    Atomic and Nuclear Physics The Einstein Connection

    2.4 Just like your checkbook; it all has to balance andUnstable nuclides eventually go away

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    Nuclear Decay Chart of Nuclides

    2

    Check the web athttp://www-nds.iaea.org/relnsd/vcharthtml/VChartHTML.htmlFor an alternative chart

    Try also

    http://wwwndc.jaea.go.jp/CN10/

    Or

    http://en.wikipedia.org/wiki/Chart_of_nuclides

    These web links are on the Week 2 Overview.

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    Nuclear Data

    NZ

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    Nuclear Decay Balance Eqns. Shorthand notation for writing nuclear decay events

    Similar to chemical balance equations

    Equation must always conserve mass and charge Typically dont list energy or momentum in these

    balance equations5

    92

    235

    U!

    90

    231

    Th+ 24

    "

    Examples

    !" 00

    0

    1

    239

    94

    239

    93 ++#

    $PuNp

    Alpha Decay:

    Beta Decay:

    Positron Emiss.: !" 0

    0

    0

    1

    11

    5

    11

    6 ++#

    +

    BC

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    Nuclear DataN

    Z

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    Nuclear Decay Balance Eqns. Shorthand notation for writing nuclear decay events

    Similar to chemical balance equations

    Equation must always conserve mass and charge Typically dont list energy or momentum in these

    balance equations7

    !

    4

    2

    231

    90

    235

    92 +"

    ThU

    Examples

    HeThU

    4

    2

    231

    90

    235

    92 +!

    or

    93

    239Np!

    94

    239Pu +

    "1

    0#+0

    0$

    Alpha Decay:

    Beta Decay:

    Positron Emiss.: !" 0

    0

    0

    1

    11

    5

    11

    6 ++#

    +

    BC

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    NZ

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    Nuclear DataN

    Z

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    Nuclear Decay

    The decay of an unstable nucleus is a random process. Every unstable nuclide is characterized by a unique

    decay constant,!

    . Decay Constant

    The probability that a single nucleus will decay perunit time.

    Units:10

    !"

    #$%

    &

    secondnuclei

    decay

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    Decay Activity

    IfNis the number of nuclei present in a sample thenthe rate of nuclear decays for the sample is given by:

    Ais referred to as the activityof the sample.Activity has basic units of

    SI Unit: 1 Becquerel [Bq] = 1 decay/sec Old Unit: 1 Curie [Ci] = 3.7!1010decay/sec

    11

    [ ]nucleisecondnuclei

    decay

    second

    decay!"

    #

    $%&

    '="#

    $%&

    '

    A

    (t)= !N

    (t)

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    Decay Activity (Time Dependent)

    Each radioactive decay destroys one of the unstablenuclei, changing the number of nuclei present.

    The number of nuclei,N, and activity,A, are timedependent quantities

    12

    1decay[ ] = !1nucleus[ ]

    ( ) ( )tNtA !=

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    Decay Activity (Time Dependent)

    The original formula can be rewritten in terms of thefractional nuclide population remaining after time t.

    13

    N t( )=N 0( )e!" t

    A t

    ( )= A 0

    ( )e!" t

    N t( )N 0( )

    =A(t)

    A(0)= e!" tFractional population

    at time t

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    Example calculation Presume that we have 1,000,000 nuclei of uranium-235 which

    has a half-life of

    And lets say we want to know the fractional population ofuranium-235 after radioactive decay for one million years

    First, we have to calculate the decay constant from the half-life of7.04x108years

    14

    !1

    2

    = 7.04x108years = 704million years

    != 0.693

    7.04x108yrs( )

    = 9.84x10"10yrs"1

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    Example calculation

    Presume that we have 1,000,000 nuclei of uranium-235 whichhas a radioactive decay constant of:

    And lets say we want to know the fractional population ofuranium-235 after radioactive decay for one-year (or one yearsworth of seconds = 3.15576x107seconds)

    The answer is:

    15

    )( )

    te

    N

    tN !"=

    0

    Fractional population

    at time t

    ! = 9.84x10"10

    yrs"1

    N t( )

    N 0( )= e

    !9.84x10!10yr!1( )(1,000,000yrs)= e!9.84x10

    !10

    = 0.99902

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    Decay in Units of Half-Life

    Knief, Fig 2-2

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    Half-Life Examples

    Uranium 232 70 yr233 160,000 yr234 250,000 yr

    235 704,000,000 yr236 23,000,000 yr238 4,500,000,000 yr

    Fission ProductsStrontium-90 29 yrCesium-137 30 yr

    17

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    Mean Time to Decay

    In addition to the half-life it is also usefulto know the mean lifetime for a nuclide

    Mean Lifetime (")The average (mean) time that it will take for

    a single nuclide to decay.

    Units: [seconds]18

    !"

    1=

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    Nuclear Decay During a nuclear decay much of the excess energy of an

    unstable nuclei is removed with the emitted particle:

    Changes in binding energy of nucleus Kinetic energy given to emitted particle

    However, following the decay event, the productnucleus may be left in an excited state (still too muchenergy)

    In these cases the nucleus can do one of two things: Undergo nuclear decay again Rearrange nucleons in nucleus to achieve a lower overall

    energy state. 19

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    1. Reprinted with permission from Bechtel MarinePropulsion Corporation.

    Image Source Notes

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    Supplemental Exercise Slides

    21

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    Nuclear Decay Balance Eqns.

    Shorthand notation for writing nuclear decay events Similar to chemical balance equations

    Equation must always conserve mass and charge Typically dont list energy or momentum in these

    balance equations 22

    !4

    2

    231

    90

    235

    92 +" ThU

    ExamplesHeThU

    4

    2

    231

    90

    235

    92 +!

    or!" 0

    0

    0

    1

    239

    94

    239

    93 ++#

    $PuNp

    Alpha Decay:

    Beta Decay:

    Positron Emiss.: !" 0

    0

    0

    1

    11

    5

    11

    6 ++#

    +

    BC

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    NZ

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    24

    NZ

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    Example calculation #2

    Presume that we have 1,000,000 nuclei of Tritium (H-3) whichhas a radioactive decay constant of:

    And lets say we want to know how long it will take for thefractional population of Tritium to decay to half of it initial value

    We find the answer by solving for time, t. We solve and find that

    25

    ( )( )

    te

    N

    tN !"=

    0

    Fractional population

    at time t

    ! = 1.78x10"9sec

    "1

    0.5=N t( )N 0( )

    = e! 1.78x10

    !9sec

    !1( ) t( )

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    Explanation of natural log

    calculations

    26

    x = e

    !yStandard equation used

    in this course

    We take the natural

    log of both sides to get !n x( ) = !n e!y( ) =!y

    Which usually looks like thisin our problems:

    ( )( )

    t

    eN

    tN !"=

    0

    !n

    N t( )N 0( )

    !

    "#

    $

    %& = !n e

    '( t( ) ='(tWhich usually looks like this

    in our problems:

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    Decay Half-Life Calculate the amount of time required for 50% of a nuclide

    population to decay:

    This is referred to as the nuclides half-life Conversely, the decay constant is found by

    27

    N t( )N 0( )

    =

    1

    2= 0.5

    0.5 = e!"T1

    2 !n 0.5[ ]=!"T12 T12 = !!n 0.5[ ]

    "

    T12 =!!n 0.5[ ]

    "Units: [seconds]

    ! ="!n 0.5[ ]

    T12

    =

    0.693

    T12

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    Decay Activity (Time Dependent)

    Looking at units we see:

    The decay activity is the rate of decrease of a given nuclidepopulation

    Can be written as a first-order separable ODE (OrdinaryDifferential Equation)

    28

    A t( ) =decays

    second

    !

    "#

    $

    %& =

    -nuclei

    second

    !

    "#

    $

    %& =

    -dN t( )

    dt

    ( ) ( )

    ( )tNdt

    tdNtA !=

    "

    =

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    Decay Activity (Time Dependent)

    From this ODE we can solve for the nuclidepopulation as a function of time,N(t)

    29

    ( )( )tN

    dt

    tdN!=

    "

    ( )( )

    dttN

    tdN!"=

    ( )

    ( ) !! "= dttdNtN

    #1

    ( )[ ] CttNLog +!= "

    ( ) Ct eetN !"=

    Original Equation

    Multiply both sides by dt/N(t)

    Integrate

    Take exponent of both sides

    Evaluate indefinite integral

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    Decay Activity (Time Dependent)

    We need a boundary condition to determine theconstant of integration, C

    LetN(0) be the initial nuclide population (at t=0)

    Final equation:

    ( ) Ct eetN !"=

    ( ) CeeN 00 !"=

    ( )0NeC =

    1

    ( ) ( ) teNtN !"= 0

    Memorize this!