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Kinoshita N, Paul M, Kashiv Y, Collon P, Deibel CM, DiGiovine B, Greene JP, Jiang CL, Marley ST, Pardo RC, Rehm KE, Robertson D, Scott R, Schmitt C, Tang XD, Vondrasek R, Yokoyama A. Retraction. Science 2023; 379:1307. [PMID: 36996231 DOI: 10.1126/science.adh7739] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 04/01/2023]
Affiliation(s)
- N Kinoshita
- Shimizu Corporation Institute of Technology, Tokyo, Japan
| | - M Paul
- Hebrew University of Jerusalem, Jerusalem, Israel
| | - Y Kashiv
- University of Notre Dame, Notre Dame, IN, USA
| | - P Collon
- University of Notre Dame, Notre Dame, IN, USA
| | - C M Deibel
- Louisiana State University, Baton Rouge, LA, USA
| | - B DiGiovine
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - J P Greene
- Argonne National Laboratory, Argonne, IL, USA
| | - C L Jiang
- Argonne National Laboratory, Argonne, IL, USA
| | - S T Marley
- Louisiana State University, Baton Rouge, LA, USA
| | - R C Pardo
- Argonne National Laboratory, Argonne, IL, USA
| | - K E Rehm
- Argonne National Laboratory, Argonne, IL, USA
| | - D Robertson
- University of Notre Dame, Notre Dame, IN, USA
| | - R Scott
- Argonne National Laboratory, Argonne, IL, USA
| | - C Schmitt
- University of Notre Dame, Notre Dame, IN, USA
| | - X D Tang
- Institute of Modern Physics, Lanzhou, China
| | - R Vondrasek
- Argonne National Laboratory, Argonne, IL, USA
| | - A Yokoyama
- Kanazawa University, Kakumamachi, Kanazawa, Ishikawa, Japan
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Tessler M, Paul M, Halfon S, Meyer BS, Pardo R, Purtschert R, Rehm KE, Scott R, Weigand M, Weissman L, Almaraz-Calderon S, Avila ML, Baggenstos D, Collon P, Hazenshprung N, Kashiv Y, Kijel D, Kreisel A, Reifarth R, Santiago-Gonzalez D, Shor A, Silverman I, Talwar R, Veltum D, Vondrasek R. Stellar ^{36,38}Ar(n,γ)^{37,39}Ar Reactions and Their Effect on Light Neutron-Rich Nuclide Synthesis. Phys Rev Lett 2018; 121:112701. [PMID: 30265109 DOI: 10.1103/physrevlett.121.112701] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/05/2018] [Revised: 07/24/2018] [Indexed: 06/08/2023]
Abstract
The ^{36}Ar(n,γ)^{37}Ar (t_{1/2}=35 d) and ^{38}Ar(n,γ)^{39}Ar (269 yr) reactions were studied for the first time with a quasi-Maxwellian (kT∼47 keV) neutron flux for Maxwellian average cross section (MACS) measurements at stellar energies. Gas samples were irradiated at the high-intensity Soreq applied research accelerator facility-liquid-lithium target neutron source and the ^{37}Ar/^{36}Ar and ^{39}Ar/^{38}Ar ratios in the activated samples were determined by accelerator mass spectrometry at the ATLAS facility (Argonne National Laboratory). The ^{37}Ar activity was also measured by low-level counting at the University of Bern. Experimental MACS of ^{36}Ar and ^{38}Ar, corrected to the standard 30 keV thermal energy, are 1.9(3) and 1.3(2) mb, respectively, differing from the theoretical and evaluated values published to date by up to an order of magnitude. The neutron-capture cross sections of ^{36,38}Ar are relevant to the stellar nucleosynthesis of light neutron-rich nuclides; the two experimental values are shown to affect the calculated mass fraction of nuclides in the region A=36-48 during the weak s process. The new production cross sections have implications also for the use of ^{37}Ar and ^{39}Ar as environmental tracers in the atmosphere and hydrosphere.
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Affiliation(s)
- M Tessler
- Racah Institute of Physics, Hebrew University, Jerusalem 91904, Israel
| | - M Paul
- Racah Institute of Physics, Hebrew University, Jerusalem 91904, Israel
| | | | - B S Meyer
- Department of Physics and Astronomy, Clemson University, Clemson, South Carolina 29634, USA
| | - R Pardo
- Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - R Purtschert
- Physics Institute, University of Bern, 3012 Bern, Switzerland
| | - K E Rehm
- Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - R Scott
- Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - M Weigand
- Goethe University Frankfurt, Frankfurt 60438, Germany
| | | | | | - M L Avila
- Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - D Baggenstos
- Physics Institute, University of Bern, 3012 Bern, Switzerland
| | - P Collon
- Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | | | - Y Kashiv
- Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - D Kijel
- Soreq NRC, Yavne 81800, Israel
| | | | - R Reifarth
- Goethe University Frankfurt, Frankfurt 60438, Germany
| | - D Santiago-Gonzalez
- Argonne National Laboratory, Argonne, Illinois 60439, USA
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A Shor
- Soreq NRC, Yavne 81800, Israel
| | | | - R Talwar
- Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - D Veltum
- Goethe University Frankfurt, Frankfurt 60438, Germany
| | - R Vondrasek
- Argonne National Laboratory, Argonne, Illinois 60439, USA
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Kinoshita N, Paul M, Kashiv Y, Collon P, Deibel CM, DiGiovine B, Greene JP, Henderson DJ, Jiang CL, Marley ST, Nakanishi T, Pardo RC, Rehm KE, Robertson D, Scott R, Schmitt C, Tang XD, Vondrasek R, Yokoyama A. A Shorter
146
Sm Half-Life Measured and Implications for
146
Sm-
142
Nd Chronology in the Solar System. Science 2012; 335:1614-7. [PMID: 22461609 DOI: 10.1126/science.1215510] [Citation(s) in RCA: 139] [Impact Index Per Article: 11.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
The extinct p-process nuclide (146)Sm serves as an astrophysical and geochemical chronometer through measurements of isotopic anomalies of its α-decay daughter (142)Nd. Based on analyses of (146)Sm/(147)Sm α-activity and atom ratios, we determined the half-life of (146)Sm to be 68 ± 7 (1σ) million years, which is shorter than the currently used value of 103 ± 5 million years. This half-life value implies a higher initial (146)Sm abundance in the early solar system, ((146)Sm/(144)Sm)(0) = 0.0094 ± 0.0005 (2σ), than previously estimated. Terrestrial, lunar, and martian planetary silicate mantle differentiation events dated with (146)Sm-(142)Nd converge to a shorter time span and in general to earlier times, due to the combined effect of the new (146)Sm half-life and ((146)Sm/(144)Sm)(0) values.
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Affiliation(s)
- N. Kinoshita
- Research Facility Center for Science and Technology, University of Tsukuba, Japan
| | - M. Paul
- Racah Institute of Physics, Hebrew University, Jerusalem, Israel 91904
| | - Y. Kashiv
- Department of Physics, University of Notre Dame, Notre Dame, IN 46556–5670, USA
| | - P. Collon
- Department of Physics, University of Notre Dame, Notre Dame, IN 46556–5670, USA
| | - C. M. Deibel
- Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
- Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, MI 46624, USA
| | - B. DiGiovine
- Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
| | - J. P. Greene
- Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
| | - D. J. Henderson
- Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
| | - C. L. Jiang
- Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
| | - S. T. Marley
- Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
| | - T. Nakanishi
- Faculty of Chemistry, Institute of Science and Engineering, Kanazawa University, Japan
| | - R. C. Pardo
- Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
| | - K. E. Rehm
- Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
| | - D. Robertson
- Department of Physics, University of Notre Dame, Notre Dame, IN 46556–5670, USA
| | - R. Scott
- Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
| | - C. Schmitt
- Department of Physics, University of Notre Dame, Notre Dame, IN 46556–5670, USA
| | - X. D. Tang
- Department of Physics, University of Notre Dame, Notre Dame, IN 46556–5670, USA
| | - R. Vondrasek
- Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
| | - A. Yokoyama
- Faculty of Chemistry, Institute of Science and Engineering, Kanazawa University, Japan
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Kinoshita N, Hashimoto T, Nakanishi T, Yokoyama A, Amakawa H, Mitsugashira T, Ohtsuki T, Takahashi N, Ahmad I, Greene JP, Henderson DJ, Jiang CL, Notani M, Pardo RC, Patel N, Rehm KE, Scott R, Vondrasek R, Jisonna L, Collon P, Robertson D, Schmitt C, Tang XD, Kashiv Y, Paul M. Technological Development for Half-life Measurement of 146Sm Nuclide. ACTA ACUST UNITED AC 2007. [DOI: 10.14494/jnrs2000.8.109] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/18/2022]
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Nassar H, Paul M, Ahmad I, Ben-Dov Y, Caggiano J, Ghelberg S, Goriely S, Greene JP, Hass M, Heger A, Heinz A, Henderson DJ, Janssens RVF, Jiang CL, Kashiv Y, Nara Singh BS, Ofan A, Pardo RC, Pennington T, Rehm KE, Savard G, Scott R, Vondrasek R. 40Ca(alpha, gamma)44Ti reaction in the energy regime of supernova nucleosynthesis. Phys Rev Lett 2006; 96:041102. [PMID: 16486801 DOI: 10.1103/physrevlett.96.041102] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/31/2005] [Indexed: 05/06/2023]
Abstract
The 44Ti(t1/2=59 yr) nuclide, an important signature of supernova nucleosynthesis, has recently been observed as live radioactivity by gamma-ray astronomy from the Cas A remnant. We investigate in the laboratory the major 44Ti production reaction 40Ca(alpha, gamma)44Ti (Ec.m. approximately 0.6-1.2 MeV/u by direct off-line counting of 44Ti nuclei. The yield, significantly higher than inferred from previous experiments, is analyzed in terms of a statistical model using microscopic nuclear inputs. The associated stellar rate has important astrophysical consequences, increasing the calculated supernova 44Ti yield by a factor approximately 2 over previous estimates and bringing it closer to Cas A observations.
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Affiliation(s)
- H Nassar
- Racah Institute of Physics, Hebrew University, 91904 Jerusalem, Israel
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