Non-resonant triple alpha reaction rate at low temperature

T. Itoh; A. Tamii; N. Aoi; J. Carter; L. Donaldson; H. Fujita; T. Furuno; T. Hashimoto; T. Kawabata; M. Kamimura; K. Miki; F. Nemulodi; R. Neveling; K. Ogata; E. Sideras-Haddad; F. D. Smit; C. Swarts

doi:10.1063/1.4874073

Non-resonant triple alpha reaction rate at low temperature

T. Itoh, A. Tamii, N. Aoi, J. Carter, L. Donaldson, H. Fujita, T. Furuno, T. Hashimoto, T. Kawabata, M. Kamimura, K. Miki, F. Nemulodi, R. Neveling, K. Ogata, E. Sideras-Haddad, F. D. Smit, C. Swarts

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

Abstract

Our experimental goal is to study the non-resonant triple alpha reaction rate at low temperture (T < 10⁸ K). The ¹³C(p,d) reaction at 66 MeV has been used to probe the alpha-unbound continuum state in ¹²C just below the 2^nd 0⁺ state at 7.65 MeV. The transition strength to the continuum state is predicted to be sensitive to the non-resonant triple alpha reaction rate. The experiment has been performed at iThemba LABS. We report the present status of the experiment.

Original language	English
Title of host publication	Origin of Matter and Evolution of Galaxies 2013 - Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013
Publisher	American Institute of Physics Inc.
Pages	226-228
Number of pages	3
ISBN (Print)	9780735412286
DOIs	https://doi.org/10.1063/1.4874073
Publication status	Published - 2014
Externally published	Yes
Event	12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013 - Tsukuba, Japan Duration: Nov 18 2013 → Nov 21 2013

Publication series

Name	AIP Conference Proceedings
Volume	1594
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013
Country/Territory	Japan
City	Tsukuba
Period	11/18/13 → 11/21/13

All Science Journal Classification (ASJC) codes

Physics and Astronomy(all)

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10.1063/1.4874073

Cite this

Itoh, T., Tamii, A., Aoi, N., Carter, J., Donaldson, L., Fujita, H., Furuno, T., Hashimoto, T., Kawabata, T., Kamimura, M., Miki, K., Nemulodi, F., Neveling, R., Ogata, K., Sideras-Haddad, E., Smit, F. D., & Swarts, C. (2014). Non-resonant triple alpha reaction rate at low temperature. In Origin of Matter and Evolution of Galaxies 2013 - Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013 (pp. 226-228). (AIP Conference Proceedings; Vol. 1594). American Institute of Physics Inc.. https://doi.org/10.1063/1.4874073

Non-resonant triple alpha reaction rate at low temperature. / Itoh, T.; Tamii, A.; Aoi, N. et al.

Origin of Matter and Evolution of Galaxies 2013 - Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013. American Institute of Physics Inc., 2014. p. 226-228 (AIP Conference Proceedings; Vol. 1594).

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

Itoh, T, Tamii, A, Aoi, N, Carter, J, Donaldson, L, Fujita, H, Furuno, T, Hashimoto, T, Kawabata, T, Kamimura, M, Miki, K, Nemulodi, F, Neveling, R, Ogata, K, Sideras-Haddad, E, Smit, FD & Swarts, C 2014, Non-resonant triple alpha reaction rate at low temperature. in Origin of Matter and Evolution of Galaxies 2013 - Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013. AIP Conference Proceedings, vol. 1594, American Institute of Physics Inc., pp. 226-228, 12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013, Tsukuba, Japan, 11/18/13. https://doi.org/10.1063/1.4874073

Itoh T, Tamii A, Aoi N, Carter J, Donaldson L, Fujita H et al. Non-resonant triple alpha reaction rate at low temperature. In Origin of Matter and Evolution of Galaxies 2013 - Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013. American Institute of Physics Inc. 2014. p. 226-228. (AIP Conference Proceedings). doi: 10.1063/1.4874073

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title = "Non-resonant triple alpha reaction rate at low temperature",

abstract = "Our experimental goal is to study the non-resonant triple alpha reaction rate at low temperture (T < 108 K). The 13C(p,d) reaction at 66 MeV has been used to probe the alpha-unbound continuum state in 12C just below the 2nd 0+ state at 7.65 MeV. The transition strength to the continuum state is predicted to be sensitive to the non-resonant triple alpha reaction rate. The experiment has been performed at iThemba LABS. We report the present status of the experiment.",

author = "T. Itoh and A. Tamii and N. Aoi and J. Carter and L. Donaldson and H. Fujita and T. Furuno and T. Hashimoto and T. Kawabata and M. Kamimura and K. Miki and F. Nemulodi and R. Neveling and K. Ogata and E. Sideras-Haddad and Smit, {F. D.} and C. Swarts",

year = "2014",

doi = "10.1063/1.4874073",

language = "English",

isbn = "9780735412286",

series = "AIP Conference Proceedings",

publisher = "American Institute of Physics Inc.",

pages = "226--228",

booktitle = "Origin of Matter and Evolution of Galaxies 2013 - Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013",

note = "12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013 ; Conference date: 18-11-2013 Through 21-11-2013",

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T1 - Non-resonant triple alpha reaction rate at low temperature

AU - Itoh, T.

AU - Tamii, A.

AU - Aoi, N.

AU - Carter, J.

AU - Donaldson, L.

AU - Fujita, H.

AU - Furuno, T.

AU - Hashimoto, T.

AU - Kawabata, T.

AU - Kamimura, M.

AU - Miki, K.

AU - Nemulodi, F.

AU - Neveling, R.

AU - Ogata, K.

AU - Sideras-Haddad, E.

AU - Smit, F. D.

AU - Swarts, C.

PY - 2014

Y1 - 2014

N2 - Our experimental goal is to study the non-resonant triple alpha reaction rate at low temperture (T < 108 K). The 13C(p,d) reaction at 66 MeV has been used to probe the alpha-unbound continuum state in 12C just below the 2nd 0+ state at 7.65 MeV. The transition strength to the continuum state is predicted to be sensitive to the non-resonant triple alpha reaction rate. The experiment has been performed at iThemba LABS. We report the present status of the experiment.

AB - Our experimental goal is to study the non-resonant triple alpha reaction rate at low temperture (T < 108 K). The 13C(p,d) reaction at 66 MeV has been used to probe the alpha-unbound continuum state in 12C just below the 2nd 0+ state at 7.65 MeV. The transition strength to the continuum state is predicted to be sensitive to the non-resonant triple alpha reaction rate. The experiment has been performed at iThemba LABS. We report the present status of the experiment.

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T3 - AIP Conference Proceedings

SP - 226

EP - 228

BT - Origin of Matter and Evolution of Galaxies 2013 - Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013

PB - American Institute of Physics Inc.

T2 - 12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013

Y2 - 18 November 2013 through 21 November 2013

ER -

Non-resonant triple alpha reaction rate at low temperature

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