The Nuclear Responses for Double Beta Neutrinos and Double Spin Isospin Resonances by Using of Double Charge Exchange Heavey Ion Reaction

K. Takahisa; H. Akimune; H. Ejiri; H. Fujimura; M. Fujiwara; K. Hara; H. Hasimoto; K. Hatanaka; T. Itahasi; T. Kawabata; K. Kawase; Y. Koreeda; N. Maehara; S. Mordechai; Y. Nagai; K. Nakanishi; S. Ninomiya; T. Shima; M. Tanaka; S. Umehara; S. Umisedo; H. P. Yoshida; S. Yoshida; M. Yoshimura; M. Yosoi

doi:10.1142/9789812702739_0062

The Nuclear Responses for Double Beta Neutrinos and Double Spin Isospin Resonances by Using of Double Charge Exchange Heavey Ion Reaction

K. Takahisa, H. Akimune, H. Ejiri, H. Fujimura, M. Fujiwara, K. Hara, H. Hasimoto, K. Hatanaka, T. Itahasi, T. Kawabata, K. Kawase, Y. Koreeda, N. Maehara, S. Mordechai, Y. Nagai, K. Nakanishi, S. Ninomiya, T. Shima, M. Tanaka, S. UmeharaS. Umisedo, H. P. Yoshida, S. Yoshida, M. Yoshimura, M. Yosoi

Department of Physics

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

To study double spin-isospin responses in view of the ββν decays, double charge-exchange nuclear reactions have measured at RCNP. We have succeeded to measure the double charge exchange reaction by means of heavy ion reaction. From these experiments, we conclude that the (11B,11Li) reaction at 70 MeV/nucleon is a good spectroscopic tool. We believe that the reaction can be well applied to the study of pure spin-flip nuclear responses in higher-excited regions including DGT and higher ∆L excitations.

Original language	English
Title of host publication	Origin of Matter and Evolution of Galaxies 2003
Editors	M. Terasawa, S. Kubono (CNS, University of Tokyo, Japan), T. Kishida (RIKEN, Japan), K. Nomoto (University of Tokyo, Japan), T. Kajino (National Astronomical Observatory, Japan, T. Motobayashi (RIKEN, Japan) & K Nomoto (University of Tokyo, Japan)
Publisher	World Scientific
Pages	533-536
ISBN (Electronic)	9789814482837
ISBN (Print)	9789812388247
DOIs	https://doi.org/10.1142/9789812702739_0062
State	Published - 1 Dec 2004

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Takahisa, K., Akimune, H., Ejiri, H., Fujimura, H., Fujiwara, M., Hara, K., Hasimoto, H., Hatanaka, K., Itahasi, T., Kawabata, T., Kawase, K., Koreeda, Y., Maehara, N., Mordechai, S., Nagai, Y., Nakanishi, K., Ninomiya, S., Shima, T., Tanaka, M., ... Yosoi, M. (2004). The Nuclear Responses for Double Beta Neutrinos and Double Spin Isospin Resonances by Using of Double Charge Exchange Heavey Ion Reaction. In M. Terasawa, S. Kubono (CNS, University of Tokyo, Japan), T. Kishida (RIKEN, Japan), K. Nomoto (University of Tokyo, Japan), T. Kajino (National Astronomical Observatory, Japan, & T. Motobayashi (RIKEN, Japan) & K Nomoto (University of Tokyo, Japan) (Eds.), Origin of Matter and Evolution of Galaxies 2003 (pp. 533-536). World Scientific. https://doi.org/10.1142/9789812702739_0062

Takahisa, K. ; Akimune, H. ; Ejiri, H. et al. / The Nuclear Responses for Double Beta Neutrinos and Double Spin Isospin Resonances by Using of Double Charge Exchange Heavey Ion Reaction. Origin of Matter and Evolution of Galaxies 2003. editor / M. Terasawa ; S. Kubono (CNS, University of Tokyo, Japan) ; T. Kishida (RIKEN, Japan) ; K. Nomoto (University of Tokyo, Japan) ; T. Kajino (National Astronomical Observatory, Japan ; T. Motobayashi (RIKEN, Japan) & K Nomoto (University of Tokyo, Japan). World Scientific, 2004. pp. 533-536

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title = "The Nuclear Responses for Double Beta Neutrinos and Double Spin Isospin Resonances by Using of Double Charge Exchange Heavey Ion Reaction",

abstract = "To study double spin-isospin responses in view of the ββν decays, double charge-exchange nuclear reactions have measured at RCNP. We have succeeded to measure the double charge exchange reaction by means of heavy ion reaction. From these experiments, we conclude that the (11B,11Li) reaction at 70 MeV/nucleon is a good spectroscopic tool. We believe that the reaction can be well applied to the study of pure spin-flip nuclear responses in higher-excited regions including DGT and higher ∆L excitations.",

author = "K. Takahisa and H. Akimune and H. Ejiri and H. Fujimura and M. Fujiwara and K. Hara and H. Hasimoto and K. Hatanaka and T. Itahasi and T. Kawabata and K. Kawase and Y. Koreeda and N. Maehara and S. Mordechai and Y. Nagai and K. Nakanishi and S. Ninomiya and T. Shima and M. Tanaka and S. Umehara and S. Umisedo and Yoshida, {H. P.} and S. Yoshida and M. Yoshimura and M. Yosoi",

year = "2004",

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doi = "10.1142/9789812702739_0062",

language = "English",

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pages = "533--536",

editor = "Terasawa, { M. } and {Kubono (CNS, University of Tokyo, Japan)}, { S. } and {Kishida (RIKEN, Japan)}, T. and {Nomoto (University of Tokyo, Japan)}, { K.} and {Kajino (National Astronomical Observatory, Japan}, {T. } and {Motobayashi (RIKEN, Japan) & K Nomoto (University of Tokyo, Japan)}, {T. }",

booktitle = "Origin of Matter and Evolution of Galaxies 2003",

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Takahisa, K, Akimune, H, Ejiri, H, Fujimura, H, Fujiwara, M, Hara, K, Hasimoto, H, Hatanaka, K, Itahasi, T, Kawabata, T, Kawase, K, Koreeda, Y, Maehara, N, Mordechai, S, Nagai, Y, Nakanishi, K, Ninomiya, S, Shima, T, Tanaka, M, Umehara, S, Umisedo, S, Yoshida, HP, Yoshida, S, Yoshimura, M & Yosoi, M 2004, The Nuclear Responses for Double Beta Neutrinos and Double Spin Isospin Resonances by Using of Double Charge Exchange Heavey Ion Reaction. in M Terasawa, S Kubono (CNS, University of Tokyo, Japan), T Kishida (RIKEN, Japan), K Nomoto (University of Tokyo, Japan), T Kajino (National Astronomical Observatory, Japan & T Motobayashi (RIKEN, Japan) & K Nomoto (University of Tokyo, Japan) (eds), Origin of Matter and Evolution of Galaxies 2003. World Scientific, pp. 533-536. https://doi.org/10.1142/9789812702739_0062

The Nuclear Responses for Double Beta Neutrinos and Double Spin Isospin Resonances by Using of Double Charge Exchange Heavey Ion Reaction. / Takahisa, K.; Akimune, H.; Ejiri, H. et al.
Origin of Matter and Evolution of Galaxies 2003. ed. / M. Terasawa; S. Kubono (CNS, University of Tokyo, Japan); T. Kishida (RIKEN, Japan); K. Nomoto (University of Tokyo, Japan); T. Kajino (National Astronomical Observatory, Japan; T. Motobayashi (RIKEN, Japan) & K Nomoto (University of Tokyo, Japan). World Scientific, 2004. p. 533-536.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

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T1 - The Nuclear Responses for Double Beta Neutrinos and Double Spin Isospin Resonances by Using of Double Charge Exchange Heavey Ion Reaction

AU - Takahisa, K.

AU - Akimune, H.

AU - Ejiri, H.

AU - Fujimura, H.

AU - Fujiwara, M.

AU - Hara, K.

AU - Hasimoto, H.

AU - Hatanaka, K.

AU - Itahasi, T.

AU - Kawabata, T.

AU - Kawase, K.

AU - Koreeda, Y.

AU - Maehara, N.

AU - Mordechai, S.

AU - Nagai, Y.

AU - Nakanishi, K.

AU - Ninomiya, S.

AU - Shima, T.

AU - Tanaka, M.

AU - Umehara, S.

AU - Umisedo, S.

AU - Yoshida, H. P.

AU - Yoshida, S.

AU - Yoshimura, M.

AU - Yosoi, M.

PY - 2004/12/1

Y1 - 2004/12/1

N2 - To study double spin-isospin responses in view of the ββν decays, double charge-exchange nuclear reactions have measured at RCNP. We have succeeded to measure the double charge exchange reaction by means of heavy ion reaction. From these experiments, we conclude that the (11B,11Li) reaction at 70 MeV/nucleon is a good spectroscopic tool. We believe that the reaction can be well applied to the study of pure spin-flip nuclear responses in higher-excited regions including DGT and higher ∆L excitations.

AB - To study double spin-isospin responses in view of the ββν decays, double charge-exchange nuclear reactions have measured at RCNP. We have succeeded to measure the double charge exchange reaction by means of heavy ion reaction. From these experiments, we conclude that the (11B,11Li) reaction at 70 MeV/nucleon is a good spectroscopic tool. We believe that the reaction can be well applied to the study of pure spin-flip nuclear responses in higher-excited regions including DGT and higher ∆L excitations.

U2 - 10.1142/9789812702739_0062

DO - 10.1142/9789812702739_0062

M3 - Conference contribution

SN - 9789812388247

SP - 533

EP - 536

BT - Origin of Matter and Evolution of Galaxies 2003

A2 - Terasawa, M.

A2 - Kubono (CNS, University of Tokyo, Japan), S.

A2 - Kishida (RIKEN, Japan), T.

A2 - Nomoto (University of Tokyo, Japan), K.

A2 - Kajino (National Astronomical Observatory, Japan, T.

A2 - Motobayashi (RIKEN, Japan) & K Nomoto (University of Tokyo, Japan), T.

PB - World Scientific

ER -

Takahisa K, Akimune H, Ejiri H, Fujimura H, Fujiwara M, Hara K et al. The Nuclear Responses for Double Beta Neutrinos and Double Spin Isospin Resonances by Using of Double Charge Exchange Heavey Ion Reaction. In Terasawa M, Kubono (CNS, University of Tokyo, Japan) S, Kishida (RIKEN, Japan) T, Nomoto (University of Tokyo, Japan) K, Kajino (National Astronomical Observatory, Japan T, Motobayashi (RIKEN, Japan) & K Nomoto (University of Tokyo, Japan) T, editors, Origin of Matter and Evolution of Galaxies 2003. World Scientific. 2004. p. 533-536 doi: 10.1142/9789812702739_0062

The Nuclear Responses for Double Beta Neutrinos and Double Spin Isospin Resonances by Using of Double Charge Exchange Heavey Ion Reaction

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