Neutron capture rates on radioactive nuclides - DANCE

R. Reifarth; U. Agvaanluvsan; A. Alpizar-Vicente; T. A. Bredeweg; E. I. Esch; U. Greife; R. C. Haight; R. Hatarik; F. Herwig; J. M. O'Donnell; R. S. Rundberg; J. M. Schwantes; J. L. Ullmann; D. J. Vieira; J. M. Wouters

doi:10.1016/j.newar.2006.06.051

Neutron capture rates on radioactive nuclides - DANCE

R. Reifarth, U. Agvaanluvsan, A. Alpizar-Vicente, T. A. Bredeweg, E. I. Esch, U. Greife, R. C. Haight, R. Hatarik, F. Herwig, J. M. O'Donnell, R. S. Rundberg, J. M. Schwantes, J. L. Ullmann, D. J. Vieira, J. M. Wouters

Mechanical Engineering

Research output: Contribution to journal › Review article › peer-review

3 Scopus citations

Abstract

The nucleosynthesis of the elements including their stellar sites is one of the most interesting nuclear physics challenges. Information on reaction rates for neutron induced reactions have a direct impact on existing stellar models. Except for the stable isotopes, very few neutron-induced reactions in the energy range of interest have been measured to date. DANCE measurements on stable and unstable isotopes can provide many of the missing key reactions that are needed to understand the nucleosynthesis of the heavy elements, which is illustrated at the example of the ¹⁵¹Sm(n,γ) reaction.

Original language	English (US)
Pages (from-to)	644-647
Number of pages	4
Journal	New Astronomy Reviews
Volume	50
Issue number	7-8
DOIs	https://doi.org/10.1016/j.newar.2006.06.051
State	Published - Oct 2006

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1016/j.newar.2006.06.051

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Reifarth, R., Agvaanluvsan, U., Alpizar-Vicente, A., Bredeweg, T. A., Esch, E. I., Greife, U., Haight, R. C., Hatarik, R., Herwig, F., O'Donnell, J. M., Rundberg, R. S., Schwantes, J. M., Ullmann, J. L., Vieira, D. J., & Wouters, J. M. (2006). Neutron capture rates on radioactive nuclides - DANCE. New Astronomy Reviews, 50(7-8), 644-647. https://doi.org/10.1016/j.newar.2006.06.051

@article{fef52afb68b647f6bbf828085bf60f89,

title = "Neutron capture rates on radioactive nuclides - DANCE",

abstract = "The nucleosynthesis of the elements including their stellar sites is one of the most interesting nuclear physics challenges. Information on reaction rates for neutron induced reactions have a direct impact on existing stellar models. Except for the stable isotopes, very few neutron-induced reactions in the energy range of interest have been measured to date. DANCE measurements on stable and unstable isotopes can provide many of the missing key reactions that are needed to understand the nucleosynthesis of the heavy elements, which is illustrated at the example of the 151Sm(n,γ) reaction.",

author = "R. Reifarth and U. Agvaanluvsan and A. Alpizar-Vicente and Bredeweg, {T. A.} and Esch, {E. I.} and U. Greife and Haight, {R. C.} and R. Hatarik and F. Herwig and O'Donnell, {J. M.} and Rundberg, {R. S.} and Schwantes, {J. M.} and Ullmann, {J. L.} and Vieira, {D. J.} and Wouters, {J. M.}",

note = "Funding Information: This work has benefited from the use of the Los Alamos Neutron Science Center at the Los Alamos National Laboratory. This facility is funded by the US Department of Energy and operated by the University of California under Contract W-7405-ENG-36. The Colorado School of Mines group is funded via DOE grant: DE-FG02-93ER40789. ",

year = "2006",

month = oct,

doi = "10.1016/j.newar.2006.06.051",

language = "English (US)",

volume = "50",

pages = "644--647",

journal = "New Astronomy Reviews",

issn = "1387-6473",

publisher = "Elsevier",

number = "7-8",

}

TY - JOUR

T1 - Neutron capture rates on radioactive nuclides - DANCE

AU - Reifarth, R.

AU - Agvaanluvsan, U.

AU - Alpizar-Vicente, A.

AU - Bredeweg, T. A.

AU - Esch, E. I.

AU - Greife, U.

AU - Haight, R. C.

AU - Hatarik, R.

AU - Herwig, F.

AU - O'Donnell, J. M.

AU - Rundberg, R. S.

AU - Schwantes, J. M.

AU - Ullmann, J. L.

AU - Vieira, D. J.

AU - Wouters, J. M.

N1 - Funding Information: This work has benefited from the use of the Los Alamos Neutron Science Center at the Los Alamos National Laboratory. This facility is funded by the US Department of Energy and operated by the University of California under Contract W-7405-ENG-36. The Colorado School of Mines group is funded via DOE grant: DE-FG02-93ER40789.

PY - 2006/10

Y1 - 2006/10

N2 - The nucleosynthesis of the elements including their stellar sites is one of the most interesting nuclear physics challenges. Information on reaction rates for neutron induced reactions have a direct impact on existing stellar models. Except for the stable isotopes, very few neutron-induced reactions in the energy range of interest have been measured to date. DANCE measurements on stable and unstable isotopes can provide many of the missing key reactions that are needed to understand the nucleosynthesis of the heavy elements, which is illustrated at the example of the 151Sm(n,γ) reaction.

AB - The nucleosynthesis of the elements including their stellar sites is one of the most interesting nuclear physics challenges. Information on reaction rates for neutron induced reactions have a direct impact on existing stellar models. Except for the stable isotopes, very few neutron-induced reactions in the energy range of interest have been measured to date. DANCE measurements on stable and unstable isotopes can provide many of the missing key reactions that are needed to understand the nucleosynthesis of the heavy elements, which is illustrated at the example of the 151Sm(n,γ) reaction.

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U2 - 10.1016/j.newar.2006.06.051

DO - 10.1016/j.newar.2006.06.051

M3 - Review article

AN - SCOPUS:33749155010

SN - 1387-6473

VL - 50

SP - 644

EP - 647

JO - New Astronomy Reviews

JF - New Astronomy Reviews

IS - 7-8

ER -

Neutron capture rates on radioactive nuclides - DANCE

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