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Studies on alpha-induced astrophysical reactions using the low-energy RI beam separator Studies on alpha-induced astrophysical reactions using the low-energy RI beam separator

Studies on alpha-induced astrophysical reactions using the low-energy RI beam separator - PowerPoint Presentation

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Studies on alpha-induced astrophysical reactions using the low-energy RI beam separator - PPT Presentation

Center for Nuclear Study Univ of Tokyo Hidetoshi Yamaguchi D Kahl T NakaoY Wakabayashi S Kubono T Hashimoto S Hayakawa T Kawabata N Iwasa ID: 935756

jun 2013 beam 7be 2013 jun 7be beam reaction energy inpc 4inpc phys resonant crib target cns cluster univ

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Slide1

Studies on alpha-induced astrophysical reactions using the low-energy RI beam separator CRIB

Center for Nuclear Study, Univ. of TokyoHidetoshi Yamaguchi, D. Kahl, T. Nakao,Y. Wakabayashi, S. Kubono, T. Hashimoto, S. Hayakawa, T. Kawabata, N. Iwasa, T. Teranishi, Y.K. Kwon, D.N. Binh, L.H. Khiem, and N.G. Duy

Slide2

OutlineCRIB…low-energy RI beam facility of the Univ. of Tokyo, located in RIBF of RIKEN Nishina

center.Recent projects…emphasis on a-induced astrophysical reactionsAlpha resonant scattering for (a,g) reaction study [e.g. 7Li/7Be+a]Direct measurement of (a, p) reactions [e.g. 18Ne/30S(a, p)]2013 Jun 4INPC 2013

Slide3

CRIB CNS

Radio-Isotope Beam separator , operated by CNS (Univ. of Tokyo), located at RIBF (RIKEN Nishina Center). Low-energy(<10MeV/u) RI beams by in-flight method.Primary beam from K=70 AVF cyclotron. Momentum (Magnetic rigidity) separation by “double achromatic” system, and velocity separation by a Wien filter. Orbit radius: 90 cm, solid angle: 5.6 msr, momentum resolution: 1/850.INPC 20132013 Jun 4

Slide4

Low-Energy RI beam Productions at CRIB

Direct reactions such as (p,n), (d,p) and (3He,n)

in inverse kinematics are mainly used for the production….large cross sectionMany RI beams

have been produced at CRIB:

typically

10

4

-10

6

pps

7

Be…

2 x 10

8

pps available with a cryogenic target.H. Yamaguchi et al., NIM A (2008)

RI beam at CRIB /Stable nuclei

INPC 2013

2013 Jun 4

Slide5

International collaborations at CRIBCRIB experiments performed in 2007-2011,

by collaborated members of CNS and other institutes: INPC 20132013 Jun 4

Slide6

Recent research projects

Proton/alpha resonant scattering26Si+p (Collaborated with Chung-Ang, Korea) H.S. Jung et al., published at PRC (2012).7Li/7Be+a (CNS) H. Yamaguchi et al., PRC (2011&2013).21Na+p, 22Na+p [18Ne(a,p), Ne-Na cycle] (IMP/CIAE, China)17F+p [Resonances for 14O(a,p)](IMP/CIAE, China) (α,p) reaction measurement, Active target (GEM-MSTPC)18Ne(a,p) (CNS, Hashimoto (now at RCNP))30S(α,p) (CNS, Daid Kahl)22Mg(α,p) (IOP, Vietnam , Nguyen Ngoc Duy

)44Ti(a,p) (KEK,

Ishiyama

)

44

Ti beam test

successful.

(

a,g

)

16

N

16O*⇒12C+a for 12C(a,g) (Catania, Italy, S. Cherubini)Reaction mechanism8B+Pb (Padova, Italy, C. Signorini)β-decay

7Be lifetime in metal (Tohoku Univ, Otsuki)2013 Jun 4INPC 2013

Slide7

7Li+a/ 7Be+a study

7Li(a,g)11B …important at high-T, as a production reaction of 11B (the n-process in core-collapse supernovae).7Be(a,g)11B … one of the reaction in hot p-p chain, relevant at high-T. Contribution of higher-lying resonances unknown. a-cluster structure in 11B/11C :2a+t / 2a+3He cluster states are known to exist (similar to the dilute cluster structure in 12C.)Several “bands” which have

a-cluster structure could be formed. We can study the band and cluster structure more in detail.INPC 2013

2013 Jun 4

Slide8

7

Be(a,g)np-process calculation (T9>1) shows considerable contribution by 10B(a,p)13C and 7Be(a,g)11C as much as the triple-alpha process.S. Wanajo et al., Astrophys. J (2010)2013 Jun 4INPC 2013

Slide9

7Li/7Be+α; method

“Thick target with inverse kinematics” Resonant elastic scatterings can be measured at qcm=180 deg. MCP2013 Jun 4INPC 2013

Slide10

7Be+a Excitation functions4 excitation functions… new information on resonant widths, spin, and parity.

H. Yamaguchi et al., PRC, Published in Mar. 2013.2013 Jun 4INPC 2013

Slide11

Resonant contribution to 7Be(a,g)

Small but not negligible contribution compared to lower-lying states (~10%).2013 Jun 4INPC 2013

Slide12

(Rotational) bands in 11C2

rotational bands (K=3/2+,5/2+) were suggested in Soic. et al. (2004).Jp=9/2+ was assigned for the resonance at 12.4 MeV, and it can be the member of K=3/2+ band. A negative-parity band is proposed. 2a+3He cluster?2013 Jun 4INPC 2013

Slide13

Interpretation of the new negative-parity band (11B case)

2013 Jun 4INPC 2013

Slide14

Study on the ap-processap-process: (a,p),(p,g) reactions occur faster than β-decay at high temperature. Accelerates the rp-process (Wallace and Woosley, 1981).Suitable objective for CRIBNot many direct measurements of (a,p) reactions have been performed in other facilities. Involves A=18-30, proton richunstable nuclei.T=1.5GK, close to the beam energy at CRIB.2013 Jun 4INPC 2013

Slide15

18

Ne(a,p) (T. Hashimoto; RCNP)

11C

12

C

13

C

13

N

14

N

15

N

12

N

16

O

17

O18O

9

C

10

C

11

N

15

O

14

O

19

F

18

F

17

F

20

Ne

21

Ne

22

Ne

19

Ne

18

Ne

stable

unstable

hot-CNO

12

C(p, γ)

13

N(p, γ)

14

O(

b

)

14

N(p,

g

)

15

O(

b

)

15

N(p,

a

)

12

C

second hot CNO cycle

14

O(α, p)

17

F(p, γ)

18

Ne(

b

)

18

F(p, α)

15

O(

b

)

15

O(p, α)

12

C

18

Ne(α, p)

21

Na

22

Na

22

Na

23

Na

21

Na

20

Na

18

Ne(

a

, p)

21

Na is an important breakout reaction from hot-CNO cycle

to the

rp

-process

(B to C in the figure)

A: hot-CNO

B: second hot-CNO

C:

18

Ne(

a

, p)

21

Na

D:

18

Ne(2p,

g

)

20

Mg

E:

15

O(2p,

g

)

17

F

J. Phys. G: Nucl. Part. Phys. 25 (1999)R133

17

Ne

X-ray bursts

2013 Jun 4

INPC 2013

Relevant energy (temperature):

E

cm

= 0.5 - 3.8 MeV (T = 0.6 - 3 GK).

Slide16

Experimental Setup

He (90%) +CO2 (10%) mixture gas(160 torr)

z

x

y

Acts as a He target and a detector (TPC) simultaneously

3-dimentional trajectory and energy loss can be measured

Good event identification.

18

Ne beam

Beam monitor

INPC 2013

2013 Jun 4

Slide17

Typical event of

18Ne(a, p)21Na reaction PreliminarySi telescopes

Total energy (MeV)

p

a

(

Stopped in first layer)

Energy loss in first layer (MeV)

Pad No.

Pad No.

Pad No.

dE/Pad (MeV)

X position (cm)

Y position (cm)

Analysis is in progress …

18

Ne

21

Na

18

Ne

21

Na

18

Ne

18

Ne

18

Ne

21

Na

18

Ne

Preliminary

2013 Jun 4

INPC 2013

Reaction events are observed !

Slide18

CRIB - Recent PublicationsProton resonant scattering13

N+p; Teranishi et al., PLB (2007), 21Na/22Mg+p; J.J. He et al., PRC (2007/2009), Eur. Phys. J (2010), 7Be+p; H. Yamaguchi et al., PLB (2009).26Si+p (Chung-Ang Univ., SNU) H.S. Jung et al., Phys. Rev. C (2012). 25Al+p; Jun Chen et al., Phys. Rev. C(2012): related to galactic gamma-ray from 26Al.Alpha resonant scattering7Li+a; H. Yamaguchi et al., Phys. Rev (2011).7Be+a; H. Yamaguchi et al., Phys. Rev. C (2013).Other reactions21Na(a,p) direct reaction measurement; Dam N. Binh, Dr. thesis of Univ. of Tokyo (2009).11C(a,p) direct reaction measurement; S. Hayakawa, Dr. thesis of Univ. of Tokyo (2012), another paper in preparation.17F+12C; Quasi-elastic scattering G.L. Zhang et al., Eur. Phys. J. A (2012).12N(p,g) by ANC B. Guo et al., Phys. Rev. C (2013).

2013 Jun 4

INPC 2013

Slide19

INPC 2013

2013 Jun 4Summary CRIB is a low-energy RI beam facility operated by CNS, University of Tokyo, providing RI beams of good intensity and purity.Standard experiments: Proton/alpha resonant scattering, direct (a,p) reaction measurement using an active target (GEM-MSTPC) 7Li+a,7Be+aStrong resonances were observed. The “thick target method with inverse kinematics” could be applied to many nuclides. We can study astrophysical reactions and alpha-cluster structures.Active target Has been used in several (a,p) measurements, analysis is in progress.

We welcome new users and new ideas!

Firenze

è come un albero fiorito

che in

piazza

dei Signori ha tronco e fronde

....