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Charge State Distribution of Recoil 16 O from 4 He( 12 C, 16 O) g in Astrophysical interest 劉劉劉 A 劉劉劉劉 B 劉劉 劉 、西 B 劉劉劉劉 B 劉劉劉劉 B 劉劉劉劉劉 B 劉劉劉劉 B 劉劉劉 B Maria T. Rosary B 劉劉劉 A 劉劉劉劉劉劉劉劉劉 A 劉劉劉劉劉劉劉劉劉劉劉劉 B 2011-12-03

Charge State Distribution of Recoil 16 O from 4 He( 12 C , 16 O) g in Astrophysical interest

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Charge State Distribution of Recoil 16 O from 4 He( 12 C , 16 O) g in Astrophysical interest. 劉盛進 A 、相良建至 B 、寺西高 B 、 藤田訓裕 B 、山口祐幸 B 、  松田沙矢香 B 、三鼓達輝 B 、岩崎諒 B 、 Maria T. Rosary B 、櫻井誠 A 神户大学理学研究科 A 九州大学理学府物理学専攻 B. 2011-12-03. introduction. Astrophysics. - PowerPoint PPT Presentation

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Page 1: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Charge State Distribution of Recoil 16O from 4He(12C, 16O)

g in Astrophysical interest  劉盛進 A 、相良建至 B 、寺西高 B 、 藤田訓裕 B 、山口祐幸 B 、 松田沙矢香 B 、三鼓達輝 B 、岩崎諒 B 、 Maria T. RosaryB 、櫻井誠 A

神户大学理学研究科 A 九州大学理学府物理学専攻 B

2011-12-03

Page 2: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

introduction

Total S-factor of 4He+12C 16O+g

Ruhr U.Kyushu U.

extrapolation

Astrophysics.4He(12C, 16O)g Ecm=2.4 MeV,1.5MeV Succeeded !!  

For the recoils 16Oq+, to determine 4He(12C, 16O)g total cross section, fraction of 16Oq+ should be precisely known.

Investigation: charge exchange processes and charge state distribution of Oxygen though Helium gas.

16O1+,2+,….8+

The fraction of 16Oq+??

16Oq+ detector

Page 3: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Features of ion-atom collision

physical processes:Capture, Ionization, Excitation,…..

q-1q-2

q+1

Chargedistribution

Charge exchange

e- e-(Auger)

Page 4: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Ionization of Projectile, Aq+ A(q+1)+

For a collision, from an initial state i to a final state f, ionization cross section is given:

PWBA: plan wave Born Approximation• Projectile in initial and final states is represented by plane wave,

(~exp(iqr)).• Perturbation of the projectile orbits is neglected.• Screening effect is taken into account.• projectile assumed to linearly without deviation of trajectory.

(initial) (final)

min

2 212 3

0

8 ( , , ) ( )if nlm nlmnlm nlm q

dqd d f q Z qv q

2 2 2( , , ) exp( ) ( ) ( )nlm f nlmf q iRq r r dRdr Scattering amplitudeEffective charge of target(He): 2

1( )Z q Ejection electron energy:

Projectile velocity: n

Minimum momentum transfer: qmin=( Ip+e) /n Ip is binding energy of the projectile electron, e is energy of the ejected electron,

2

2

2 ( 1)2 0dR dR Z l lE Rdr r dr r r

The final state: to solve radial

equation in coulomb field

21 1( )2

n

aa aba ab

ZHr r

nlm nlmH E

For the initial state(nlm) of ionized electron, the Schrodinger equation at multi-electrons system :

,

Page 5: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Capture of Projectile, Aq+ A(q-1)+

Impact parameter treatment 2

0

2 ( )ij ijb d

• electron exchange is neglected.• The corresponding trajectory may be uniquely

distinguished by an impact parameter and a velocity. • Nuclear and nuclear interaction is neglected.

The H-like wave functions of an optical electron in the initial and final states:

1/ 2( ) ( )z Hnl nlP r Z P Zr

( ) exp( ( ) )A Bij i jb i i t dt

*

2 2 1( ) ( ) ( ) exp( )B A Aj i rr V r r ir dv

1( )Ai r : electron initial state

2( )Bj r : electron final state

22

( , ) A B AZ Z ZV r tR r

,A Bi j : corresponding eigen-energies

(initial) (final)

Page 6: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

100 1000 10000

1E-18

1E-17

1E-16

1E-15

1E-14

1E-13

1E-12

Cro

ss s

ectio

n cm

2Energy (keV)

Arsenv Our CalculationCDW

1000 10000

1E-20

1E-19

1E-18

1E-17

1E-16

1E-15

cm

2

E , KeV

Experimental data Theory calculation

16O6+ 16O7+16O5+ 16O4+

Arseny: adiabatic approximation, low energyCDW: Continuum distorted wave approximation, high energy

F.M.Martine et al. PRA,1965(1971)

Possibility>1

Ionization cross section Capture cross section

Page 7: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Equilibrium Charge State Distributions

Variation of the charge state distribution:

Equilibrium distribution:

All fractions reach a certain value and keep constant.

, / 0x dF dx

' ', , '', '

( ) 0q q q q q qq q q

F F

' ', , '', '

( )qq q q q q q

q q q

dFF F

dx

1qq

F Non-equili.

equili.

Cross sections of ionization and capture are required

,Gain Loss

Page 8: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Results

0 300 600 900 1200 1500 1800 2100 24000.0

0.2

0.4

0.6

0.8

1.0

1+5+

4+2+

Frac

tion

Thickness ( x 1014 atom/cm2)

3+

4.5 MeV 16O3+ + He

0 300 600 900 1200 1500 1800 2100 24000.0

0.2

0.4

0.6

0.8

1.0

2+6+

5+

4+

Frac

tion

Thickness x ( 1014 atoms/cm2)

7.2MeV 16O3+ + He

3+

1+,7+,8+

The thickness evolution of fraction at 7.2 MeV and 4.5 MeV

Equilibrium distribution can be obtained

Evolution of fraction against thickness

Equili. Distri.Equili. Distri.

3+, 100% 3+, 100%

HeHe

Page 9: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Charge state distribution

0 2 4 6 8

0.0

0.1

0.2

0.3

0.4

0.5

Frac

tion

Charge state

Theory Experiment

4.5MeV16O1+ + He

0 2 4 6 8

0.0

0.1

0.2

0.3

0.4

0.5

Frac

tion

Chareg state

Theory experiment7.2 MeV

16O1+ + He

The results of calculation deviated from the experimental results and shift to left.Reflecting the shape of experimental data well but mean charge state is smaller.

Theory Experiment

4.5 MeV 2.88 3.507.2 MeV 4.15 4.38

Mean charge state:

Page 10: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

0 2 4 6 8

0

10

20

30

40

50

Frac

tion

Charge state

Theory experiment

2.2 MeV

0 2 4 6 8

0

10

20

30

40

50

Frac

tion

Charge state

theory exp.

3.2MeV

0 2 4 6 8-5

0

5

10

15

20

25

30

35

40

45

Frac

tion

Charge state

Theory Experiment

5.2MeV

Data from TRIUMF Lab. (energy: 2.2MeV --- 14 MeV)

Shift to left.!!

0 2 4 6 8-5

0

5

10

15

20

25

30

35

40

45

50

Frac

tion

Charge state

Theory Exp.

9.4MeV

0 2 4 6 8-5

0

5

10

15

20

25

30

35

40

45

50

Frac

tion

Charge state

Theory Exp.

12 MeV

0 2 4 6 8

0

10

20

30

40

50

60

Frac

tion

Charge state

Theory Exp.

14MeV

Page 11: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

1 2 3 4 5 6 7-5

0

5

10

15

20

25

30

35

40

Frac

tion

Charge state

Theory(Correction) Experiment Theory(Original)

4.5MeV

1 2 3 4 5 6 7

0

10

20

30

40

Frac

tion

Charge state

Theory(modification)Experiment Theory(Original)

7.2MeV

Enhanced ionization cross section

If ionization cross section is enhanced 2 times, calculation agrees with experimental data

• Blue curve: Calculation (σion. ×2)• Red curve: Experiment• Black curve: Calculation (σion. ×1)

Mean Charge state

Theory(σion. ×1)

Experiment

Theory(σion. ×2)

4.5 MeV 2.88 3.50 3.607.2 MeV 4.15 4.38 4.54

Page 12: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Enhanced ionization cross section

Ionization cross section is enhanced 2 times

0 2 4 6 8

0

10

20

30

40

50

Frac

tion

Charge state

Theory(Modification) experiment Theory(original)

2.2 MeV

0 2 4 6 8-5

0

5

10

15

20

25

30

35

40

45

50

Frac

tion

Charge state

Theory(Correction)Experiment Theory(original)

3.2MeV

-1 0 1 2 3 4 5 6 7 8 9

0

10

20

30

40

50

Frac

tion

Charge state

Theory(Correction) Experiment Theory(Original)

5.2MeV

0 2 4 6 8

0

10

20

30

40

50

Frac

tion

Charge state

Theory(correction) Experiment Theory(original)

9.4MeV

-1 0 1 2 3 4 5 6 7 8 9

0

10

20

30

40

50

60

Frac

tion

Charge state

Theory(Correction) Experiment Theor(Original)

12MeV

0 2 4 6 8-10

0

10

20

30

40

50

60

70

Frac

tion

Charge state

Theory (Correction) Experiment Theory(Original)

14MeV

Date from TRIUNF Lab.

• Blue curve: Calculation (σion. ×2)• Red curve: Experiment• Black curve: Calculation (σion. ×1)

Page 13: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Discussion Theory Correction PWBA: Polarization effect• Perturbation of projectile orbits.• Result: a reduction in electron binding energy and increase

the ionization probability

And excited state effects may play an important role in ionization of projectile. (Probability: Pexcited > Pdirect)

Ionization cross section:1s 1s

2s

Ground state 16O5+ Excited state 16O5+

total direct subsequent

Polarization effect

Proj. IonProj. Ion Targ. atom

ground--excited--ionized

Ioni.Ioni.

2s

Page 14: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Conclusion Charge exchange and charge distribution have been calculated

Ionization cross section: PWBA Capture cross section: Impact Parameter Model

Comparison between theory and experiment. Theory reflected experiment data but mean charge state was smaller Try to correct theory (σion. ×2) and almost agreed well with experimental data.

Future: Theory Correction (polarization effect and excited effect) Prediction of non-equilibrium distribution at various energyMeasurement of 4He(12C, 16O) g at low energy :1.15MeV, 1.0MeV,……

Page 15: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

THANK YOU FOR ATTENDANCE

Page 16: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

r2

r’1r’’1

RZ1

Z2

Projectile Target

Hamiltonian:

2 2 2 21 1 1 1 2 2

' '' ' ''1 1 2 1 1

' ' ' 12 2 2 2

M Z Z ZH VM r r r r r

1 2 2 2 1' '' ' '

1 1 2 2 1 2 2

1 1Z Z Z Z ZVR R r R r R r R r r R r r

Interaction potential:

Proj. electron

TargetElectron 1

TargetElectron 2

Page 17: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Projectile as a plane wave: Initial state:exp(-ikR) Final state: exp(-ik’R) q=k’-k (momentum

transfer)

Ionized electron state Initial state: i final state: ff

The state of atom electron j1s1s(r’1, r’’2) , jn’l’(r’1, r’’2)

Page 18: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

According the quantum transition, the cross section2

2

2 2

' ( )4if

M vd f q dv

2 ' ' 1 1 2 1 1 1 1 1 2( ) exp( ) ( ) ( ' '') ( ) ( ' '')f n l i s sf q iRq r r r V r r r dRdr dr

' 'i f

n l

d d

2 1nl nlm

nlm

Nl

M: reduced mass, v initial velocity, v’ the final velocity

Summation of the states of target atom :

Summation of the states of projectile:

'

2

1 4''

iR qiRq irq irqee dR e dR e

R r R q

Page 19: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

2 ' ' 1 1 2 1 1 1 1 1 2( , , ) exp( ) ( ) ( ' '') ( ) ( ' '')f n l i s sf q iRq r r r V r r r dRdr dr 2(1 ) 1 1 1

nl nl

s nl s nl nl s 2 2

1

(1 ) 1 (1 1 )nl

s nl s s

2 sind d 2 2 2' 2 'cosq k k kk 22 sin'

qdqd dkk

min

2 212 3

0

8 ( , , ) ( )2 1 2 1

nl nlnlm

nl nl q

N N dqd d f q Z ql l v q

Minimum momentum transfer: qmin=Ip+e+ E△ T

Ip is binding energy of the projectile electron, e is energy of the ejected electron,△ET is the excitation energy of the target electron

The closure condition:

Page 20: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

222( , , ) exp( )f q f iqr nlm

( ) ( , )nlm nl lmR r Y 21 1( )2

n

aa aba ab

ZHr r

( )! 2 1( 1) (cos )( )! 4

m m imlm l

l m lY P el m

Scattering amplitude: F factor

For the nlm initial state, the Hamiltonian at multi-electorns system :

Spherical function:

2

2

2 ( 1)2 0dR dR Z l lE Rdr r dr r r

The final state: to solve radial equation at the coulomb central field

Page 21: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Capture Impact parameter treatment Assume: 1. electron exchange may be neglected. 2. effects of the identity of the nuclei may be

neglected 3. the relative motion of the nuclei takes place

at such velocities v, that the scattering is confined to negligibly small angles.

4. the corresponding trajectory for the incident nucleus may be uniquely distinguished by an impact parameter and a velocity.

Page 22: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

X

Z

Y

Velocity : n

Rimpact parameter: r

B(ion) A(target)

n

r2

rr1

r2=r-R/2 r1=r+R/2R O (mid-poit)

2

1 1 1 1( , )( ) ( ) / 2

V r tR r R t r R t

R vt

e

:t :t

Page 23: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

For the atom electron:( ) ( , ) 0el nH i r t

t

0 ( , )elH H V r t

20

1

1 1( )2 rH

r

Omit nuclear interaction to get a rectilinear orbits from the equation of motion for the nuclei

2

1( , )V r tr

2

1 1 1 1( , )( ) ( ) / 2

V r tR r R t r R t

Page 24: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Defining initial unperturbed eigen function of the electron on A

0 1 1( ) ( )Ai i iH r r

To make an expansion of y(r,t)in the state f(s) of A

1 1 1( , ) ( , ) ( ) ( )Aii t

i i i itr t r t r e r

1( , ) ( ) ( ) exp( )n nk k pk

r t a t r i t

z r v

21 1

2 8k

Ap vz v

Page 25: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

( ) ( )B Bf k k kH x x

After reaction:

( , )el f fH H V r t

21 1( )2f rH

x

1

1 1fV

R r

1 1 1( , ) ( , ) ( ) ( )Bfi tB B B

i f f ftr t r t r e r

To make an expansion of (r,t)in the state f(s) of B

( , ) ( ) ( )exp( )n nk k qk

r t b t x i t 21 1

2 8k

Bq vz v

Page 26: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

As it is the cross section describing the capture of an electron from state i of A to state jof B is given by

2

0

2 ( )ij jb d

The initial conditions being ( ) 1, ( ) 0( )i pa a p i

jdbi

dt 2

21 1( ) ( , ) exp( ) exp[ ( ) ]2 8

B A Bj r jr V r t ivz d i v t

21

1 1( , ) ( ) exp( ( ) )2 8

A Ai ir t r ivz i v t

*2 1 1

exp( ( ) )

( ) ( ) ( ) exp( )

A Bji i j

B A Aii j i r

g i t

g r V r r ivz d

z r v

*2 1 1( ) exp( ( ) ) ( ) ( ) ( ) exp( )A B B A A

j i j j i rb i i t dt r V r r ivz d

Finally:

Page 27: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

* *( ) ( )exp( ) , ( ) ( ) exp( )i

A A Bi j jp V r ipr dr q r iqr dr

22

1( , ) ( , ) exp( )(2 ) p

b v f q v iq d qv

*( , ) ( ) ( )A B

i jf q v p q 2 2, 2q p v q p w

So the radial part of the exchange amplitude for the n0l0m0-n1l1m1 transition has the form

0 1

0 0 1 1 0 1

0 0 1 1

2 2 2 2

4( , ) (cos )

( ) ( ( / / 2) ) ( ( / / 2) )

m ml m l m l l

n l n l

b v pdpC C P Pv

J p F k w v v F k w v v

Using the Fourier transform

w :The difference between the binding energies of capture electron in the initial and final state

Page 28: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Function F for the initial and final states are defined by the radial integrals

0 0 0 0 0

1 1 1 1 1

2 2

0

( ) ( ) ( ) ,

( ) ( ) ( ) ( ) , 2

n l n l l

n l n l l

F y P r j ry rdr

F x P r j rx V r rdr x y w

The H-like wave functions of an optical electron in the initial and final states:

1/ 2( ) ( )z Hnl nlP r Z P Zr

PnlH is the radial wave function of a hydrogen atom and Coulomb interaction

potential has the form :

1( ) /V r Z r

Page 29: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

min

2 212 3

0

8 ( , , ) ( )if nlm nlmnlm nlm q

dqd d f q Z qv q

2 2 2( , , ) exp( ) ( ) ( )nlm f nlmf q iRq r r dRdr Scattering amplitudeEffective charge of target(He): 2

1( )Z q Ejection electron energy:

Projectile velocity: n

Minimum momentum transfer: qmin=( Ip+e) /n Ip is binding energy of the projectile electron, e is energy of the ejected electron,

2

2

2 ( 1)2 0dR dR Z l lE Rdr r dr r r

The final state: to solve radial equation in coulomb field

21 1( )2

n

aa aba ab

ZHr r

nlm nlmH E

For the initial state(nlm) of ionized electron, the Schrodinger equation at multi-electrons system :

,

Page 30: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Capture cross sectionImpact parameter treatment Assumption: 1. electron exchange may be neglected. 2. the relative motion of the nuclei takes

place at such velocities v, that the scattering is confined to negligibly small angles.

3. the corresponding trajectory for the incident nucleus may be uniquely distinguished by an impact parameter and a velocity.

Page 31: Charge  State Distribution of  Recoil  16 O from  4 He( 12 C ,  16 O) g  in Astrophysical interest

Proj. Ion Targ. atom

Ioni.

Aq+ A(q-1)+