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

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Page 1: 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

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 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

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 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

Features of ion-atom collision

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

q-1

q-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 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

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 2

12 30

8( , , ) ( )if nlm nlm

nlm nlm q

dqd d f q Z q

v 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 0

dR dR Z l lE R

dr r dr r r

The final state: to solve radial

equation in coulomb field

21 1( )

2

n

aa aba ab

ZH

r 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 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

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 t

R 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 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

100 1000 10000

1E-18

1E-17

1E-16

1E-15

1E-14

1E-13

1E-12

Cro

ss s

ect

ion

cm

2

Energy (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 sectionCapture cross section

Page 7: 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

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 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

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+

Fra

ctio

n

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+

Fra

ctio

n

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 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

Charge state distribution

0 2 4 6 8

0.0

0.1

0.2

0.3

0.4

0.5

Fra

ctio

n

Charge state

Theory Experiment

4.5MeV16O1+ + He

0 2 4 6 8

0.0

0.1

0.2

0.3

0.4

0.5

Fra

ctio

n

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 3.50

7.2 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 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

0 2 4 6 8

0

10

20

30

40

50

Fra

ctio

n

Charge state

Theory experiment

2.2 MeV

0 2 4 6 8

0

10

20

30

40

50

Fra

ctio

n

Charge state

theory exp.

3.2MeV

0 2 4 6 8-5

0

5

10

15

20

25

30

35

40

45

Fra

ctio

n

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

Fra

ctio

n

Charge state

Theory Exp.

9.4MeV

0 2 4 6 8-5

0

5

10

15

20

25

30

35

40

45

50

Fra

ctio

n

Charge state

Theory Exp.

12 MeV

0 2 4 6 8

0

10

20

30

40

50

60

Fra

ctio

n

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 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

1 2 3 4 5 6 7-5

0

5

10

15

20

25

30

35

40

Fra

ctio

n

Charge state

Theory(Correction) Experiment Theory(Original)

4.5MeV

1 2 3 4 5 6 7

0

10

20

30

40

Fra

ctio

n

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 3.60

7.2 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 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

Enhanced ionization cross section

Ionization cross section is enhanced 2 times

0 2 4 6 8

0

10

20

30

40

50

Fra

ctio

n

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

Fra

ctio

n

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

Fra

ctio

n

Charge state

Theory(Correction) Experiment Theory(Original)

5.2MeV

0 2 4 6 8

0

10

20

30

40

50

Fra

ctio

n

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

Fra

ctio

n

Charge state

Theory(Correction) Experiment Theor(Original)

12MeV

0 2 4 6 8-10

0

10

20

30

40

50

60

70

Fra

ctio

n

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 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

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 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

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 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

THANK YOU FOR ATTENDANCE

Page 16: 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

r2

r’1

r’’1

R

Z1

Z2

Projectile Target

Hamiltonian:

2 2 2 21 1 1 1 2 2

' '' ' ''1 1 2 1 1

' ' ' 1

2 2 2 2M Z Z Z

H VM r r r r r

1 2 2 2 1' '' ' '

1 1 2 2 1 2 2

1 1Z Z Z Z ZV

R 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 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

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

transfer)

Ionized electron state Initial state: fi 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 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

According the quantum transition, the cross section

22

2 2

'( )

4if

M vd f q d

v

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

N

l

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 qi Rq irq irqe

e dR e dR eR r R q

Page 19: 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

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 1nl 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 d

kk

min

2 2

12 30

8( , , ) ( )

2 1 2 1nl nl

nlmnl nl q

N N dqd d f q Z q

l 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 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

22

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

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

2

n

aa aba ab

ZH

r r

( )! 2 1( 1) (cos )

( )! 4m m im

lm l

l m lY P e

l m

Scattering amplitude: F factor

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

Spherical function:

2

2

2 ( 1)2 0

dR dR Z l lE R

dr 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 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

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 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

X

Z

Y

Velocity : n

Rimpact parameter: r

B(ion) A(target)

n

r2

r

r1

r2=r-R/2 r1=r+R/2

R O (mid-poit)

2

1 1 1 1( , )

( ) ( ) / 2V r t

R 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 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

For the atom electron:

( ) ( , ) 0el nH i r tt

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 t

r

2

1 1 1 1( , )

( ) ( ) / 2V r t

R 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 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

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( , ) ( , ) ( ) ( )Ai

i 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 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 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 y(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 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

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

2

1 1( ) ( , ) exp( ) exp[ ( ) ]

2 8B A Bj r jr V r t ivz d i v t

21

1 1( , ) ( ) exp( ( ) )

2 8A A

i 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 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

* *( ) ( ) 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 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

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 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

min

2 2

12 30

8( , , ) ( )if nlm nlm

nlm nlm q

dqd d f q Z q

v q

2 2 2( , , ) exp( ) ( ) ( )nlm f nlmf q iRq r r dRdr Scattering amplitude

Effective 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 0

dR dR Z l lE R

dr r dr r r

The final state: to solve radial equation in coulomb field

21 1( )

2

n

aa aba ab

ZH

r r nlm nlmH E

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

,

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Capture cross section

Impact 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.

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Proj. Ion Targ. atom

Ioni.

Aq+ A(q-1)+