anp np slides l13 v2

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  • 7/23/2019 ANP NP Slides L13 v2

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    Lecture 13Previously

    Seen beta and gamma decay

    Today

    Look at alpha decaySee alpha decay chainsSee large range of alpha decay lifetimes

    Due to quantum tunneling

    See some applications of radiation

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    Alpha decay: changes N and Z

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    Homer at NukePlant

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    Alpha decay chain

    Includes !-decay- preferentially shed ns

    (recall, for large A: N > Zbut for small A: N = Z.So as move to lower A,need to reduce N/Z ratio)

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    Actually, only 4 possibledecay chains.. as a decay

    changes A by 4.i.e. writing A = 4n + mChains for m = 0, 1, 2, 3

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    (R

    1/")

    (EQ)

    Massive range in alpha lifetimes

    Exponential depon Z/!Q

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    Picture alpha emission as:

    Schematic of alpha emission

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    What potential does alpha feel?

    Schematic of alpha emission

    +

    => Vmax

    2(Z 2)e2

    40rn

    2Ze2

    40r0A1/3

    = 2.4 Z

    A1/3 MeV"10s of MeV

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    Massive range in alpha lifetimes

    e2kd

    e2

    k(r) dr =e2G

    G=

    2mQ

    h

    Ze2

    40Q=e2

    2m

    40h

    ZQ

    = 2.0 ZQ

    MeV1/2

    R=1

    =ae

    2G

    logR= log a

    (2log e)G= log a

    1.7

    Z

    Q

    d

    V

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    (R

    1/")

    (EQ)

    Massive range in alpha lifetimes

    Exponential dep= -1.7 x Z/!Q

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    Practicalities

    Problem sheetsPS3 last Friday, soln this wednesdayPS4 this Friday no assessed question

    Past Exams

    ALL PS contain past exam Qs, or equiv material,e.g. PS1 Qs: 1, 3, 4, 5

    PS2 Qs: 1, 2, 3

    PS3 Qs: 1, 2, 3, 4

    Your Exam: 40% A, 60% NPP (~40%PP, 20% NP)

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    Energy loss by charged particlesParticle with charge Z

    i,

    velocity

    !=v/c

    gas of electrons

    Energy lost by charged particle per unit length traversedgiven by dE/dx:

    dEdx ! ""Z

    A

    1

    me

    " Zi2"

    1

    "2

    of medium of incident

    particle

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    Energy loss by charged particlesEnergy lost by charged particle per unit length traversed

    given by dE/dx: dEdx ! ""

    Z

    A

    1

    me

    " Zi

    2"

    1

    "2

    of medium of incident

    particle

    Recall: E ~ !mv2= !mc2!2

    dE/dx #1/!2 #m/Ei.e. for a given E, dE/dx larger for larger m,

    e.g. m#/me~7500.

    Highly relativistic electrons lose most energy viaBremsstralung. This radiation (photons) is emittedwhen charged particles are accelerated or decelerated

    e.g. by the nuclear electric field.

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    Absorption of $rays in matter

    Incomingphoton Outgoing

    electron

    Photoelectric Effect

    Incoming photon outgoing photon

    scatteredelectron

    %

    1

    %

    2

    Compton Scattering

    Pair Production

    Energetic photon (E$> 1.02 MeV) convertd to e+e- pair

    In intense electric field of nucleus.

    Prob. of pair production Z2(E - 1.02)

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    Energy loss by electrons & photons

    Fractio

    nalEnergyLos

    s/UnitLength

    Electron Energy (MeV)

    Ionization

    Bremsstrahlung

    0.5

    1.0

    10 100Photon Energy (MeV)

    Photoelectric

    Pairproduction

    Compton

    K absorption edge

    Abso

    rptionCoefficien

    t/(g/cm2)

    0.1

    1

    10

    0.1 10

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    Interactions of neutrons with matter

    n n

    p

    n-p elastic scattering

    n

    N

    n

    &

    n

    Inelastic scattering

    N

    A

    N

    A-3

    NA+1

    *

    &

    Neutron capture

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    Radiation Units: Activity &Absorbed dose

    Activity

    Measures strength of the ionisingradiation.

    Unit, the becquerel(Bq):1 Bq = 1 disintegration/second

    Absorbed dose

    Measures total energy absorbed per unitmass.

    Unit, the gray(Gy): 1 Gy = 1 J/kg.

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    Radiation Units: Equivalent dose

    Measures biological effect of absorbed dose Obtained by multiplying the latter by thequality factor, Q, which describes how muchbiological damage the specific type of

    radiation causes. Q = 1 for !& $rays, but

    Q = 20 for #-particles.

    Unit sievert(Sv), 1 Sv = = Q x dose[Gy]. Amount of damage also dep on dose rateand part of body exposed.

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    Characteristics of various types ofradiation

    Typical energies ~ MeV

    (=Q)

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    Typical Radiation Dose Rates fromCommon Sources

    Source mSv/year

    Cosmic rays 0.26

    Natural backgrounds (U, Th, Ra) 1.65Within body (

    40K,

    14C) 0.30

    Global fallout

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    Positron Emission Tomography

    crystals + photodetectors

    annihilationphoton trajectories

    object

    Annihilationevent

    coincidenceevents

    Schematic of PETe+e- -> $$

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    Pathway of an Innovation1928: Diracs description of electrons consistent withEinsteins special relativity and quantum mechanicsPredicted the existence of anti-particles (e.g positronbasis of PET) and explained spin (basis of MRI)1932: Operation of first cyclotron , the anti-electron(positron) discovered

    Radionuclides (e.g. fluorine18 (half-life ~110min) usedin PET scanning are produced by cyclotrons in hospitals.PET cameras today use APDs (and Si PMs) and heavyscintillating crystals and starting to be combinedwithMRI scanner.

    The scientific basis for all medical imaging(functional & physiological) are steeped in

    nuclear/particle physics

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    Accelerators developed in labs used inhospitals

    Around 9000 of the

    17000 acceleratorsoperating in the Worldtoday are used formedicine.

    Example: Hadron Therapy

    Courtesy of IBA