Atomic Shell ionization

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    M. Guerra, F. Parente and J. P. Santos

    Departamento de Fsica da Faculdade de Cincias eTecnologia da Universidade Nova de Lisboa, Monte daCaparica 2825-114 Caparica, Portugal

    Centro de Fsica Atmica, Av. Prof. Gama Pinto 2, 1649-003Lisboa, Portugal

    5 th SPARC Workshop and Collaboration MeetingSetember 23 28, Predeal, Romania

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    Outline

    Goals and Motivations

    Historical Overview

    The Binary Encounter Bethe Model

    Results

    Conclusions

    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    Goals

    Adapt the Binary Encounter Bethe (BEB) modelto the ionization of ions with several chargestates

    Compute electron impact L-shell ionizationcross sections, using the BEB/RBEB model

    Comparison with other experimental andtheoretical results

    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    Motivation

    Semiconductor Fabrication

    Plasma Modelling

    Atmosferic Science

    Astrophysics

    Magnetic Fusion (Tokamaks)

    Biomedical Applications Radiation therapy

    Charged particles beams for cancer treatment

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    Rutherford Scattering

    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    2

    22

    0 14,

    WT

    Ra

    dW

    TWd

    e- e-

    e- e-

    dW

    WT

    RaT

    T

    0 222

    0 14

    2

    sin

    1

    2 42

    0

    mv

    c

    d

    d

    T Kinetic energy of the incident electronW Kinetic energy of the ejected electrona0 Bohrs radiusR Rydbergs constant

    T-W Kinetic energy of the scattered electron

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    Motts Scattering

    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    2

    0 22

    22

    0 1114WT

    dWWTWTWWT

    RaT

    22

    22

    0 1114,

    WTWTWWT

    Ra

    dWTWd

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    Motts Scattering

    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    T

    Introducing the binding energyB and changing variables

    BWE

    22

    22

    0 1114,

    WTWTEET

    NRa

    dW

    TWd

    valid only if W>>B

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    Binary Encounter Theory The target electron is described as having a velocity distribution

    The symmetry of the Motts expression is mantained in what

    concerns the exchange of the scattered and ejected electron

    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    3322

    22

    0 11

    3

    41114,

    WTE

    U

    WTWTEEBUT

    NRa

    dW

    TWd

    T

    Binary Encounter Theory

    Modified Mott Expression

    m

    pU

    2

    2

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    Binary Encounter Dipole Model BED

    Combines the binary encounter theory with the dipoleinteraction of the Bethe theory for fast incident electrons

    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    dw

    wdf

    wN

    t

    wtwNN

    wtwt

    NN

    utB

    S

    dW

    TWd

    i

    i

    1

    ln1

    1

    12

    1

    1

    1

    1

    2

    1

    ,

    22

    2204 BRNaS

    BUu

    BWw

    BTt

    dwdw

    wdfNi

    0

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    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    1

    ln11112

    ln

    1 2 t

    t

    tt

    t

    ut

    StBEB

    Differential oscillator strength for H has a simple shape

    ...1

    2

    w

    b

    dw

    wdf

    Binary Encounter Bethe Model BEB

    Good agreement for total ionization cross sections up to 20 KeV

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    Relativistic Version of BEB Model

    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    cv

    cv

    cv

    uu

    bb

    tt

    2

    2

    2

    2

    2

    2

    '1

    11

    '1

    11

    '1

    11

    u

    b

    t

    u

    b

    t

    2

    2

    2

    '

    '

    '

    mcUu

    mcBb

    mcTt

    2

    1

    2'1

    '

    2'1

    '21

    1

    ln11

    11'2ln

    1ln

    2

    1

    '2

    4

    2

    2

    2

    2

    2

    2

    2

    222

    42

    0

    t

    t

    b

    t

    t

    t

    t

    t

    tb

    b

    Nat t

    t

    t

    but

    RBEB

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    K-shell ionization

    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    L-shell ionizationAtomic L-Shell Ionization Cross Sections by Electron Impact

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    Au

    Pb Xe

    Bi

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    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    K-shell ionization

    XePb

    BiAu

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    Conclusions Great versatility of the BEB/RBEB model in

    obtaining electron impact cross sections for a

    great variety of atoms Disagreements between the cross sections

    calculated with BEB/RBEB, and experimentalcross sections are smaller than 10% for energies

    lower than 1 MeV The lack of electron correlation might be the

    cause of poor results for the K-shell of heavyelements

    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    6

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    Future Work

    Calculate binding and kinetic energies of the Kand L-shell electrons taking into account

    electron correlation

    Modification of the BEB/RBEB expression tobetter account for ionization of ions with several

    charge states Derive an analogous expression to theBEB/RBEB for positron impact ionization

    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    Aknowledgments

    Atomic L-Shell Ionization Cross Sections by Electron Impact

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    Fundao para a Cincia e TecnologiaPhD Grant SFRH/BD/38691/2007

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    Atomic L-Shell Ionization Cross Sections by Electron Impact

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