1
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Jayatissa H, Avila ML, Rehm KE, Mohr P, Meisel Z, Chen J, Hoffman CR, Liang J, Müller-Gatermann C, Neto D, Ong WJ, Psaltis A, Santiago-Gonzalez D, Tang TL, Ugalde C, Wilson G. Study of the ^{22}Mg Waiting Point Relevant for X-Ray Burst Nucleosynthesis via the ^{22}Mg(α,p)^{25}Al Reaction. Phys Rev Lett 2023; 131:112701. [PMID: 37774292 DOI: 10.1103/physrevlett.131.112701] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/30/2022] [Revised: 02/21/2023] [Accepted: 08/08/2023] [Indexed: 10/01/2023]
Abstract
The ^{22}Mg(α,p)^{25}Al reaction rate has been identified as a major source of uncertainty for understanding the nucleosynthesis flow in Type-I x-ray bursts. We report a direct measurement of the energy- and angle-integrated cross sections of this reaction in a 3.3-6.9 MeV center-of-mass energy range using the MUlti-Sampling Ionization Chamber (MUSIC). The new ^{22}Mg(α,p)^{25}Al reaction rate is a factor of ∼4 higher than the previous direct measurement of this reaction within temperatures relevant for x-ray bursts, resulting in the ^{22}Mg waiting point of x-ray burst nucleosynthesis flow to be significantly bypassed via the (α,p) reaction.
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Affiliation(s)
- H Jayatissa
- Physics Division, Argonne National Laboratory, Lemont, Illinois 60439, USA
| | - M L Avila
- Physics Division, Argonne National Laboratory, Lemont, Illinois 60439, USA
| | - K E Rehm
- Physics Division, Argonne National Laboratory, Lemont, Illinois 60439, USA
| | - P Mohr
- Institute for Nuclear Research (Atomki), P.O. Box 51, Debrecen H-4001, Hungary
| | - Z Meisel
- Institute of Nuclear and Particle Physics, Ohio University, Athens, Ohio 45701, USA
| | - J Chen
- Physics Division, Argonne National Laboratory, Lemont, Illinois 60439, USA
| | - C R Hoffman
- Physics Division, Argonne National Laboratory, Lemont, Illinois 60439, USA
| | - J Liang
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
| | - C Müller-Gatermann
- Physics Division, Argonne National Laboratory, Lemont, Illinois 60439, USA
| | - D Neto
- Department of Physics, University of Illinois Chicago, 845 W. Taylor St., Chicago, Illinois 60607, USA
| | - W J Ong
- Lawrence Livermore National Laboratory, 7000 East Ave, Livermore, California 94550, USA
| | - A Psaltis
- Institut für Kernphysik, Technische Universität Darmstadt, Darmstadt D-64289, Germany
| | | | - T L Tang
- Physics Division, Argonne National Laboratory, Lemont, Illinois 60439, USA
| | - C Ugalde
- Department of Physics, University of Illinois Chicago, 845 W. Taylor St., Chicago, Illinois 60607, USA
| | - G Wilson
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
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2
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Patch S, Santiago-Gonzalez D, Mustapha B. Thermoacoustic Range Verification in the Presence of Acoustic Heterogeneity and Soundspeed Errors– Accuracy and Robustness Relative to Live Ultrasound Images. Int J Radiat Oncol Biol Phys 2019. [DOI: 10.1016/j.ijrobp.2019.06.830] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/26/2022]
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3
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Hall MR, Bardayan DW, Baugher T, Lepailleur A, Pain SD, Ratkiewicz A, Ahn S, Allen JM, Anderson JT, Ayangeakaa AD, Blackmon JC, Burcher S, Carpenter MP, Cha SM, Chae KY, Chipps KA, Cizewski JA, Febbraro M, Hall O, Hu J, Jiang CL, Jones KL, Lee EJ, O'Malley PD, Ota S, Rasco BC, Santiago-Gonzalez D, Seweryniak D, Sims H, Smith K, Tan WP, Thompson P, Thornsberry C, Varner RL, Walter D, Wilson GL, Zhu S. Key ^{19}Ne States Identified Affecting γ-Ray Emission from ^{18}F in Novae. Phys Rev Lett 2019; 122:052701. [PMID: 30822026 DOI: 10.1103/physrevlett.122.052701] [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: 08/17/2018] [Revised: 11/15/2018] [Indexed: 06/09/2023]
Abstract
Detection of nuclear-decay γ rays provides a sensitive thermometer of nova nucleosynthesis. The most intense γ-ray flux is thought to be annihilation radiation from the β^{+} decay of ^{18}F, which is destroyed prior to decay by the ^{18}F(p,α)^{15}O reaction. Estimates of ^{18}F production had been uncertain, however, because key near-threshold levels in the compound nucleus, ^{19}Ne, had yet to be identified. We report the first measurement of the ^{19}F(^{3}He,tγ)^{19}Ne reaction, in which the placement of two long-sought 3/2^{+} levels is suggested via triton-γ-γ coincidences. The precise determination of their resonance energies reduces the upper limit of the rate by a factor of 1.5-17 at nova temperatures and reduces the average uncertainty on the nova detection probability by a factor of 2.1.
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Affiliation(s)
- M R Hall
- Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - D W Bardayan
- Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - T Baugher
- Department of Physics and Astronomy, Rutgers University, New Brunswick, New Jersey 08903, USA
| | - A Lepailleur
- Department of Physics and Astronomy, Rutgers University, New Brunswick, New Jersey 08903, USA
| | - S D Pain
- Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - A Ratkiewicz
- Department of Physics and Astronomy, Rutgers University, New Brunswick, New Jersey 08903, USA
| | - S Ahn
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
| | - J M Allen
- Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - J T Anderson
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - A D Ayangeakaa
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - J C Blackmon
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - S Burcher
- Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
| | - M P Carpenter
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - S M Cha
- Department of Physics, Sungkyunkwan University, Suwon 16419, South Korea
| | - K Y Chae
- Department of Physics, Sungkyunkwan University, Suwon 16419, South Korea
| | - K A Chipps
- Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - J A Cizewski
- Department of Physics and Astronomy, Rutgers University, New Brunswick, New Jersey 08903, USA
| | - M Febbraro
- Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - O Hall
- Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA
- Department of Physics, University of Surrey, Guildford, Surrey GU2 7XH, United Kingdom
| | - J Hu
- Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - C L Jiang
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - K L Jones
- Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
| | - E J Lee
- Department of Physics, Sungkyunkwan University, Suwon 16419, South Korea
| | - P D O'Malley
- Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - S Ota
- Physics Division, Lawrence Livermore National Laboratory, Livermore, California 94551, USA
| | - B C Rasco
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - D Santiago-Gonzalez
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - D Seweryniak
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - H Sims
- Department of Physics and Astronomy, Rutgers University, New Brunswick, New Jersey 08903, USA
- Department of Physics, University of Surrey, Guildford, Surrey GU2 7XH, United Kingdom
| | - K Smith
- Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
| | - W P Tan
- Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - P Thompson
- Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
- Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
| | - C Thornsberry
- Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
| | - R L Varner
- Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - D Walter
- Department of Physics and Astronomy, Rutgers University, New Brunswick, New Jersey 08903, USA
| | - G L Wilson
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
- Department of Physics and Applied Physics, University of Massachusetts Lowell, Lowell, Massachusetts 01854, USA
| | - S Zhu
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
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4
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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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5
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Santiago-Gonzalez D, Auranen K, Avila ML, Ayangeakaa AD, Back BB, Bottoni S, Carpenter MP, Chen J, Deibel CM, Hood AA, Hoffman CR, Janssens RVF, Jiang CL, Kay BP, Kuvin SA, Lauer A, Schiffer JP, Sethi J, Talwar R, Wiedenhöver I, Winkelbauer J, Zhu S. Probing the Single-Particle Character of Rotational States in ^{19}F Using a Short-Lived Isomeric Beam. Phys Rev Lett 2018; 120:122503. [PMID: 29694087 DOI: 10.1103/physrevlett.120.122503] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/09/2018] [Indexed: 06/08/2023]
Abstract
A beam containing a substantial component of both the J^{π}=5^{+}, T_{1/2}=162 ns isomeric state of ^{18}F and its 1^{+}, 109.77-min ground state is utilized to study members of the ground-state rotational band in ^{19}F through the neutron transfer reaction (d,p) in inverse kinematics. The resulting spectroscopic strengths confirm the single-particle nature of the 13/2^{+} band-terminating state. The agreement between shell-model calculations using an interaction constructed within the sd shell, and our experimental results reinforces the idea of a single-particle-collective duality in the descriptions of the structure of atomic nuclei.
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Affiliation(s)
- D Santiago-Gonzalez
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - K Auranen
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - M L Avila
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - A D Ayangeakaa
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - B B Back
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - S Bottoni
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - M P Carpenter
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - J Chen
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - C M Deibel
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A A Hood
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - C R Hoffman
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - R V F Janssens
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - C L Jiang
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - B P Kay
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - S A Kuvin
- Department of Physics, University of Connecticut, Storrs, Connecticut 06269, USA
| | - A Lauer
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - J P Schiffer
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - J Sethi
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
- Department of Chemistry and Biochemistry, University of Maryland, College Park, Maryland 20742, USA
| | - R Talwar
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - I Wiedenhöver
- Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
| | - J Winkelbauer
- Los Alamos National Laboratory, Los Alamos, New Mexico 87544, USA
| | - S Zhu
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
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6
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Courtin S, Jiang C, Fruet G, Heine M, Jenkins D, Adsley P, Morris L, Regan P, Rudigier M, Montanari D, Della Negra S, de Séréville N, Haas F, Hammache F, Kirsebom O, Lesrel J, Meyer A, Montanari D, Auranen K, Avila M, Ayangeakaa A, Back B, Bottoni S, Carpenter M, Dickerson C, DiGiovine B, Greene J, Henderson D, Hoffman C, Janssens R, Kay B, Kuvin S, Lauritsen T, Pardo R, Rehm K, Santiago-Gonzalez D, Sethi J, Seweryniak D, Talwar R, Ugalde C, Zhu S, Deibel C, Marley S, Bourgin D, Stodel C, Lefebvre-Schuhl A, Almaraz-Calderon S, Fang X, Tang X, Alcorta M, Bucher B, Albers M, Bertone P. Cross section measurements in the 12C+12C system. EPJ Web Conf 2017. [DOI: 10.1051/epjconf/201716501015] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
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7
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Almaraz-Calderon S, Rehm KE, Gerken N, Avila ML, Kay BP, Talwar R, Ayangeakaa AD, Bottoni S, Chen AA, Deibel CM, Dickerson C, Hanselman K, Hoffman CR, Jiang CL, Kuvin SA, Nusair O, Pardo RC, Santiago-Gonzalez D, Sethi J, Ugalde C. Study of the ^{26}Al^{m}(d,p)^{27}Al Reaction and the Influence of the ^{26}Al 0^{+} Isomer on the Destruction of ^{26}Al in the Galaxy. Phys Rev Lett 2017; 119:072701. [PMID: 28949677 DOI: 10.1103/physrevlett.119.072701] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/12/2017] [Indexed: 06/07/2023]
Abstract
The existence of ^{26}Al (t_{1/2}=7.17×10^{5} yr) in the interstellar medium provides a direct confirmation of ongoing nucleosynthesis in the Galaxy. The presence of a low-lying 0^{+} isomer (^{26}Al^{m}), however, severely complicates the astrophysical calculations. We present for the first time a study of the ^{26}Al^{m}(d,p)^{27}Al reaction using an isomeric ^{26}Al beam. The selectivity of this reaction allowed the study of ℓ=0 transfers to T=1/2, and T=3/2 states in ^{27}Al. Mirror symmetry arguments were then used to constrain the ^{26}Al^{m}(p,γ)^{27}Si reaction rate and provide an experimentally determined upper limit of the rate for the destruction of isomeric ^{26}Al via radiative proton capture reactions, which is expected to dominate the destruction path of ^{26}Al^{m} in asymptotic giant branch stars, classical novae, and core collapse supernovae.
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Affiliation(s)
- S Almaraz-Calderon
- Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
| | - K E Rehm
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - N Gerken
- Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
| | - M L Avila
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - B P Kay
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - R Talwar
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - A D Ayangeakaa
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - S Bottoni
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - A A Chen
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
| | - C M Deibel
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - C Dickerson
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - K Hanselman
- Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
| | - C R Hoffman
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - C L Jiang
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - S A Kuvin
- Department of Physics, University of Connecticut, Storrs, Connecticut 06269, USA
| | - O Nusair
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - R C Pardo
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - D Santiago-Gonzalez
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - J Sethi
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
| | - C Ugalde
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
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8
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Parker JJ, Wiedenhöver I, Cottle PD, Baker J, McPherson D, Riley MA, Santiago-Gonzalez D, Volya A, Bader VM, Baugher T, Bazin D, Gade A, Ginter T, Iwasaki H, Loelius C, Morse C, Recchia F, Smalley D, Stroberg SR, Whitmore K, Weisshaar D, Lemasson A, Crawford HL, Macchiavelli AO, Wimmer K. Isomeric Character of the Lowest Observed 4^{+} State in ^{44}S. Phys Rev Lett 2017; 118:052501. [PMID: 28211717 DOI: 10.1103/physrevlett.118.052501] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/03/2016] [Indexed: 06/06/2023]
Abstract
Previous experiments observed a 4^{+} state in the N=28 nucleus ^{44}S and suggested that this state may exhibit a hindered E2-decay rate, inconsistent with being a member of the collective ground state band. We populate this state via two-proton knockout from a beam of exotic ^{46}Ar projectiles and measure its lifetime using the recoil distance method with the GRETINA γ-ray spectrometer. The result, 76(14)_{stat}(20)_{syst} ps, implies a hindered transition of B(E2;4^{+}→2_{1}^{+})=0.61(19) single-particle or Weisskopf units strength and supports the interpretation of the 4^{+} state as a K=4 isomer, the first example of a high-K isomer in a nucleus of such low mass.
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Affiliation(s)
- J J Parker
- Department of Physics, Florida State University, Tallahassee, Florida, 32306, USA
| | - I Wiedenhöver
- Department of Physics, Florida State University, Tallahassee, Florida, 32306, USA
| | - P D Cottle
- Department of Physics, Florida State University, Tallahassee, Florida, 32306, USA
| | - J Baker
- Department of Physics, Florida State University, Tallahassee, Florida, 32306, USA
| | - D McPherson
- Department of Physics, Florida State University, Tallahassee, Florida, 32306, USA
| | - M A Riley
- Department of Physics, Florida State University, Tallahassee, Florida, 32306, USA
| | - D Santiago-Gonzalez
- Department of Physics, Florida State University, Tallahassee, Florida, 32306, USA
| | - A Volya
- Department of Physics, Florida State University, Tallahassee, Florida, 32306, USA
| | - V M Bader
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 48824, USA
| | - T Baugher
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 48824, USA
| | - D Bazin
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
| | - A Gade
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 48824, USA
| | - T Ginter
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
| | - H Iwasaki
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 48824, USA
| | - C Loelius
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 48824, USA
| | - C Morse
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 48824, USA
| | - F Recchia
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
| | - D Smalley
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
| | - S R Stroberg
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 48824, USA
| | - K Whitmore
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 48824, USA
| | - D Weisshaar
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
| | - A Lemasson
- Grand Accélérateur National dIons Lourds (GANIL), CEA/DSM-CNRS/IN2P3 Caen, France
| | - H L Crawford
- Lawrence Berkeley National Laboratory, Nuclear Science Division, 1 Cyclotron Road, Berkeley, California 94720-8153, USA
| | - A O Macchiavelli
- Lawrence Berkeley National Laboratory, Nuclear Science Division, 1 Cyclotron Road, Berkeley, California 94720-8153, USA
| | - K Wimmer
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
- Department of Physics, Central Michigan University, Mt. Pleasant, Michigan 48859, USA
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Courtin S, Jiang C, Fruet G, Auranen K, Avila M, Ayangeakaa A, Back B, Bottoni S, Carpenter M, Dickerson C, DiGiovine B, Greene J, Henderson D, Hoffman C, Janssens R, Kay B, Kuvin S, Lauritsen T, Pardo R, Rehm K, Santiago-Gonzalez D, Sethi J, Seweryniak D, Talwar R, Ugalde C, Zhu S, Deibel C, Marley S, Bourgin D, Haas F, Heine M, Montanari D, Jenkins D, Morris L, Lefebvre-Schuhl A, Almaraz-Calderon S, Fang X, Tang X, Alcorta M, Bucher B, Albers M, Bertone P. How well do we understand the reaction rate of C burning? EPJ Web Conf 2017. [DOI: 10.1051/epjconf/201716300011] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022] Open
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Avila ML, Rehm KE, Almaraz-Calderon S, Carnelli PFF, DiGiovine B, Esbensen H, Hoffman CR, Jiang CL, Kay BP, Lai J, Nusair O, Pardo RC, Santiago-Gonzalez D, Talwar R, Ugalde C. Study of the 20,22Ne+ 20,22Ne and 10,12,13,14,15C+ 12C Fusion Reactions with MUSIC. EPJ Web of Conferences 2016. [DOI: 10.1051/epjconf/201611708009] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
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Santiago-Gonzalez D, Jiang C, Rehm K, Alcorta M, Almaraz-Calderon S, Avila M, Ayangeakaa A, Back B, Bourgin D, Bucher B, Carpenter M, Courtin S, David H, Deibel C, Dickerson C, DiGiovine B, Fang X, Greene J, Haas F, Henderson D, Janssens R, Jenkins D, Lai J, Lauritsen T, Lefebvre-Schuhl A, Montanari D, Pardo R, Paul M, Seweryniak D, Tang X, Ugalde C, Zhu S. Fusion measurements of 12C+ 12C at energies of astrophysical interest. EPJ Web of Conferences 2016. [DOI: 10.1051/epjconf/201611709011] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
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Galtarossa F, Jiang C, Stefanini A, Esbensen H, Rehm K, Almaraz Calderon S, Avila M, Back B, Bourgin D, Corradi L, Courtin S, Fioretto E, Goasduff A, Haas F, Mazzocco M, Montanari D, Montagnoli G, Mijiatovic T, Sagaidak R, Santiago-Gonzalez D, Scarlassara F, Strano E, Szilner S. Fusion reactions of 58,64Ni+ 124Sn. EPJ Web of Conferences 2016. [DOI: 10.1051/epjconf/201611708011] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
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Avila ML, Rogachev GV, Koshchiy E, Baby LT, Belarge J, Kemper KW, Kuchera AN, Mukhamedzhanov AM, Santiago-Gonzalez D, Uberseder E. Constraining the 6.05 MeV 0+ and 6.13 MeV 3- cascade transitions in the 12C(α,γ)16O reaction using the asymptotic normalization coefficients. Phys Rev Lett 2015; 114:071101. [PMID: 25763945 DOI: 10.1103/physrevlett.114.071101] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/17/2014] [Indexed: 06/04/2023]
Abstract
The 12C(α,γ)^16O reaction plays a fundamental role in astrophysics and needs to be known with accuracy better than 10%. Cascade γ transitions through the excited states of 16 O are contributing to the uncertainty. We constrained the contribution of the 0+ (6.05 MeV) and 3- (6.13 MeV) cascade transitions by measuring the asymptotic normalization coefficients for these states using the α-transfer reaction 6 Li(12C,d)^16O at sub-Coulomb energy. The contribution of the 0+ and 3- cascade transitions at 300 keV is found to be 1.96 ± 0.3 and 0.12 ± 0.04 keV b for destructive interference of the direct and resonance capture and 4.36 ± 0.45 and 1.44 ± 0.12 keV b for constructive interference, respectively. The combined contribution of the 0+ and 3- cascade transitions to the 12C(α,γ)16O reaction cross section at 300 keV does not exceed 4%. Significant uncertainties have been dramatically reduced.
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Affiliation(s)
- M L Avila
- Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
| | - G V Rogachev
- Department of Physics & Astronomy and Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA
| | - E Koshchiy
- Department of Physics & Astronomy and Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA
| | - L T Baby
- Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
| | - J Belarge
- Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
| | - K W Kemper
- Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
| | - A N Kuchera
- Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
| | - A M Mukhamedzhanov
- Department of Physics & Astronomy and Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA
| | - D Santiago-Gonzalez
- Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
| | - E Uberseder
- Department of Physics & Astronomy and Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA
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