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Skowronski J, Boeltzig A, Ciani GF, Csedreki L, Piatti D, Aliotta M, Ananna C, Barile F, Bemmerer D, Best A, Broggini C, Bruno CG, Caciolli A, Campostrini M, Cavanna F, Colombetti P, Compagnucci A, Corvisiero P, Davinson T, Depalo R, Di Leva A, Elekes Z, Ferraro F, Formicola A, Fülöp Z, Gervino G, Gesuè RM, Guglielmetti A, Gustavino C, Gyürky G, Imbriani G, Junker M, Lugaro M, Marigo P, Masha E, Menegazzo R, Paticchio V, Perrino R, Prati P, Rapagnani D, Rigato V, Schiavulli L, Sidhu RS, Straniero O, Szücs T, Zavatarelli S. Proton-Capture Rates on Carbon Isotopes and Their Impact on the Astrophysical ^{12}C/^{13}C Ratio. Phys Rev Lett 2023; 131:162701. [PMID: 37925687 DOI: 10.1103/physrevlett.131.162701] [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: 01/23/2023] [Revised: 05/03/2023] [Accepted: 07/13/2023] [Indexed: 11/07/2023]
Abstract
The ^{12}C/^{13}C ratio is a significant indicator of nucleosynthesis and mixing processes during hydrogen burning in stars. Its value mainly depends on the relative rates of the ^{12}C(p,γ)^{13}N and ^{13}C(p,γ)^{14}N reactions. Both reactions have been studied at the Laboratory for Underground Nuclear Astrophysics (LUNA) in Italy down to the lowest energies to date (E_{c.m.}=60 keV) reaching for the first time the high energy tail of hydrogen burning in the shell of giant stars. Our cross sections, obtained with both prompt γ-ray detection and activation measurements, are the most precise to date with overall systematic uncertainties of 7%-8%. Compared with most of the literature, our results are systematically lower, by 25% for the ^{12}C(p,γ)^{13}N reaction and by 30% for ^{13}C(p,γ)^{14}N. We provide the most precise value up to now of 3.6±0.4 in the 20-140 MK range for the lowest possible ^{12}C/^{13}C ratio that can be produced during H burning in giant stars.
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Affiliation(s)
- J Skowronski
- Dipartimento di Fisica, Università degli Studi di Padova, 35131 Padova, Italy
- INFN, Sezione di Padova, 35131 Padova, Italy
| | - A Boeltzig
- Helmholtz-Zentrum Dresden-Rossendorf, 01328 Dresden, Germany
- INFN, Laboratori Nazionali del Gran Sasso, 67100 Assergi, Italy
- Dipartimento di Fisica "E. Pancini," Università degli Studi di Napoli "Federico II," 80125 Naples, Italy
| | - G F Ciani
- Dipartimento di Fisica "M. Merlin," Università degli Studi di Bari "A. Moro," 70125 Bari, Italy
- INFN, Sezione di Bari, 70125 Bari, Italy
| | - L Csedreki
- Institute for Nuclear Research (ATOMKI), P.O. Box 51, H-4001 Debrecen, Hungary
| | - D Piatti
- Dipartimento di Fisica, Università degli Studi di Padova, 35131 Padova, Italy
- INFN, Sezione di Padova, 35131 Padova, Italy
| | - M Aliotta
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - C Ananna
- Dipartimento di Fisica "E. Pancini," Università degli Studi di Napoli "Federico II," 80125 Naples, Italy
- INFN, Sezione di Napoli, 80125 Naples, Italy
| | - F Barile
- Dipartimento di Fisica "M. Merlin," Università degli Studi di Bari "A. Moro," 70125 Bari, Italy
- INFN, Sezione di Bari, 70125 Bari, Italy
| | - D Bemmerer
- Helmholtz-Zentrum Dresden-Rossendorf, 01328 Dresden, Germany
| | - A Best
- Dipartimento di Fisica "E. Pancini," Università degli Studi di Napoli "Federico II," 80125 Naples, Italy
- INFN, Sezione di Napoli, 80125 Naples, Italy
| | - C Broggini
- INFN, Sezione di Padova, 35131 Padova, Italy
| | - C G Bruno
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - A Caciolli
- Dipartimento di Fisica, Università degli Studi di Padova, 35131 Padova, Italy
- INFN, Sezione di Padova, 35131 Padova, Italy
| | - M Campostrini
- Laboratori Nazionali di Legnaro, 35020 Legnaro, Italy
| | - F Cavanna
- INFN, Sezione di Torino, 10125 Torino, Italy
| | - P Colombetti
- INFN, Sezione di Torino, 10125 Torino, Italy
- Dipartimento di Fisica, Università degli Studi di Torino, 10125 Torino, Italy
| | - A Compagnucci
- INFN, Laboratori Nazionali del Gran Sasso, 67100 Assergi, Italy
- Gran Sasso Science Institute, 67100 L'Aquila, Italy
| | - P Corvisiero
- Università degli Studi di Genova, 16146 Genova, Italy
- INFN, Sezione di Genova, 16146 Genova, Italy
| | - T Davinson
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - R Depalo
- Università degli Studi di Milano, 20133 Milano, Italy
- INFN, Sezione di Milano, 20133 Milano, Italy
| | - A Di Leva
- Dipartimento di Fisica "E. Pancini," Università degli Studi di Napoli "Federico II," 80125 Naples, Italy
- INFN, Sezione di Napoli, 80125 Naples, Italy
| | - Z Elekes
- Institute for Nuclear Research (ATOMKI), P.O. Box 51, H-4001 Debrecen, Hungary
| | - F Ferraro
- INFN, Laboratori Nazionali del Gran Sasso, 67100 Assergi, Italy
- Università degli Studi di Milano, 20133 Milano, Italy
| | | | - Zs Fülöp
- Institute for Nuclear Research (ATOMKI), P.O. Box 51, H-4001 Debrecen, Hungary
| | - G Gervino
- INFN, Sezione di Torino, 10125 Torino, Italy
- Dipartimento di Fisica, Università degli Studi di Torino, 10125 Torino, Italy
| | - R M Gesuè
- INFN, Laboratori Nazionali del Gran Sasso, 67100 Assergi, Italy
- Gran Sasso Science Institute, 67100 L'Aquila, Italy
| | - A Guglielmetti
- Università degli Studi di Milano, 20133 Milano, Italy
- INFN, Sezione di Milano, 20133 Milano, Italy
| | | | - Gy Gyürky
- Institute for Nuclear Research (ATOMKI), P.O. Box 51, H-4001 Debrecen, Hungary
| | - G Imbriani
- Dipartimento di Fisica "E. Pancini," Università degli Studi di Napoli "Federico II," 80125 Naples, Italy
- INFN, Sezione di Napoli, 80125 Naples, Italy
| | - M Junker
- INFN, Laboratori Nazionali del Gran Sasso, 67100 Assergi, Italy
| | - M Lugaro
- Konkoly Observatory, Research Centre for Astronomy and Earth Sciences (CSFK), MTA Centre for Excellence, 1121 Budapest, Hungary
- ELTE Eötvös Loránd University, Institute of Physics, 1117 Budapest, Hungary
| | - P Marigo
- Dipartimento di Fisica, Università degli Studi di Padova, 35131 Padova, Italy
- INFN, Sezione di Padova, 35131 Padova, Italy
| | - E Masha
- Helmholtz-Zentrum Dresden-Rossendorf, 01328 Dresden, Germany
- Università degli Studi di Milano, 20133 Milano, Italy
| | - R Menegazzo
- INFN, Sezione di Padova, 35131 Padova, Italy
| | | | - R Perrino
- INFN, Sezione di Bari, 70125 Bari, Italy
| | - P Prati
- Università degli Studi di Genova, 16146 Genova, Italy
- INFN, Sezione di Genova, 16146 Genova, Italy
| | - D Rapagnani
- Dipartimento di Fisica "E. Pancini," Università degli Studi di Napoli "Federico II," 80125 Naples, Italy
- INFN, Sezione di Napoli, 80125 Naples, Italy
| | - V Rigato
- Laboratori Nazionali di Legnaro, 35020 Legnaro, Italy
| | - L Schiavulli
- Dipartimento di Fisica "M. Merlin," Università degli Studi di Bari "A. Moro," 70125 Bari, Italy
- INFN, Sezione di Bari, 70125 Bari, Italy
| | - R S Sidhu
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - O Straniero
- INFN, Sezione di Roma, 00185 Roma, Italy
- INAF-Osservatorio Astronomico d'Abruzzo, 64100, Teramo, Italy
| | - T Szücs
- Institute for Nuclear Research (ATOMKI), P.O. Box 51, H-4001 Debrecen, Hungary
| | - S Zavatarelli
- Università degli Studi di Genova, 16146 Genova, Italy
- INFN, Sezione di Genova, 16146 Genova, Italy
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2
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Phong VH, Nishimura S, Lorusso G, Davinson T, Estrade A, Hall O, Kawano T, Liu J, Montes F, Nishimura N, Grzywacz R, Rykaczewski KP, Agramunt J, Ahn DS, Algora A, Allmond JM, Baba H, Bae S, Brewer NT, Bruno CG, Caballero-Folch R, Calviño F, Coleman-Smith PJ, Cortes G, Dillmann I, Domingo-Pardo C, Fijalkowska A, Fukuda N, Go S, Griffin CJ, Ha J, Harkness-Brennan LJ, Isobe T, Kahl D, Khiem LH, Kiss GG, Korgul A, Kubono S, Labiche M, Lazarus I, Liang J, Liu Z, Matsui K, Miernik K, Moon B, Morales AI, Morrall P, Nepal N, Page RD, Piersa-Siłkowska M, Pucknell VFE, Rasco BC, Rubio B, Sakurai H, Shimizu Y, Stracener DW, Sumikama T, Suzuki H, Tain JL, Takeda H, Tarifeño-Saldivia A, Tolosa-Delgado A, Wolińska-Cichocka M, Woods PJ, Yokoyama R. β-Delayed One and Two Neutron Emission Probabilities Southeast of ^{132}Sn and the Odd-Even Systematics in r-Process Nuclide Abundances. Phys Rev Lett 2022; 129:172701. [PMID: 36332266 DOI: 10.1103/physrevlett.129.172701] [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: 06/04/2022] [Revised: 07/30/2022] [Accepted: 08/25/2022] [Indexed: 06/16/2023]
Abstract
The β-delayed one- and two-neutron emission probabilities (P_{1n} and P_{2n}) of 20 neutron-rich nuclei with N≥82 have been measured at the RIBF facility of the RIKEN Nishina Center. P_{1n} of ^{130,131}Ag, ^{133,134}Cd, ^{135,136}In, and ^{138,139}Sn were determined for the first time, and stringent upper limits were placed on P_{2n} for nearly all cases. β-delayed two-neutron emission (β2n) was unambiguously identified in ^{133}Cd and ^{135,136}In, and their P_{2n} were measured. Weak β2n was also detected from ^{137,138}Sn. Our results highlight the effect of the N=82 and Z=50 shell closures on β-delayed neutron emission probability and provide stringent benchmarks for newly developed macroscopic-microscopic and self-consistent global models with the inclusion of a statistical treatment of neutron and γ emission. The impact of our measurements on r-process nucleosynthesis was studied in a neutron star merger scenario. Our P_{1n} and P_{2n} have a direct impact on the odd-even staggering of the final abundance, improving the agreement between calculated and observed Solar System abundances. The odd isotope fraction of Ba in r-process-enhanced (r-II) stars is also better reproduced using our new data.
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Affiliation(s)
- V H Phong
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
- University of Science, Vietnam National University, Hanoi 120062, Vietnam
| | - S Nishimura
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
| | - G Lorusso
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
- National Physical Laboratory, Teddington TW11 0LW, United Kingdom
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - T Davinson
- School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3FD, United Kingdom
| | - A Estrade
- Department of Physics, Central Michigan University, Mount Pleasant, Michigan 48859, USA
| | - O Hall
- School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3FD, United Kingdom
| | - T Kawano
- Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - J Liu
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
- Department of Physics, University of Hong Kong, Pokfulman Road, Hong Kong
| | - F Montes
- National Superconducting Cyclotron Laboratory, East Lansing, Michigan 48824, USA
| | - N Nishimura
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
- Astrophysical Big-Bang Laboratory, Cluster for Pioneering Research, RIKEN, Wako, Saitama 351-0198, Japan
| | - R Grzywacz
- Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
| | - K P Rykaczewski
- Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - J Agramunt
- Instituto de Fsica Corpuscular, CSIC and Universitat de Valencia, E-46980 Paterna, Spain
| | - D S Ahn
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
- Center for Exotic Nuclear Studies, Institute for Basic Science, Daejeon 34126, Republic of Korea
| | - A Algora
- Instituto de Fsica Corpuscular, CSIC and Universitat de Valencia, E-46980 Paterna, Spain
| | - J M Allmond
- Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - H Baba
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
| | - S Bae
- Center for Exotic Nuclear Studies, Institute for Basic Science, Daejeon 34126, Republic of Korea
| | - N T Brewer
- Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
- Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - C G Bruno
- School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3FD, United Kingdom
| | | | - F Calviño
- Universitat Politecnica de Catalunya, E-08028 Barcelona, Spain
| | - P J Coleman-Smith
- STFC Daresbury Laboratory, Daresbury, Warrington WA4 4AD, United Kingdom
| | - G Cortes
- Universitat Politecnica de Catalunya, E-08028 Barcelona, Spain
| | - I Dillmann
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia V8P 5C2, Canada
| | - C Domingo-Pardo
- Instituto de Fsica Corpuscular, CSIC and Universitat de Valencia, E-46980 Paterna, Spain
| | - A Fijalkowska
- Faculty of Physics, University of Warsaw, PL02-093 Warsaw, Poland
| | - N Fukuda
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
| | - S Go
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
| | - C J Griffin
- School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3FD, United Kingdom
| | - J Ha
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
- Seoul National University, Department of Physics and Astronomy, Seoul 08826, Republic of Korea
| | - L J Harkness-Brennan
- Department of Physics, University of Liverpool, Liverpool L69 7ZE, United Kingdom
| | - T Isobe
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
| | - D Kahl
- School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3FD, United Kingdom
- Extreme Light Infrastructure-Nuclear Physics, Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering (IFIN-HH), 077125 Bucharest-Măgurele, Romania
| | - L H Khiem
- Institute of Physics, Vietnam Academy of Science and Technology, Ba Dinh, 118011 Hanoi, Vietnam
- Graduate University of Science and Technology, Vietnam Academy of Science and Technology, Cau Giay, 122102 Hanoi, Vietnam
| | - G G Kiss
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
- Institute for Nuclear Research (Atomki), Debrecen H4032, Hungary
| | - A Korgul
- Faculty of Physics, University of Warsaw, PL02-093 Warsaw, Poland
| | - S Kubono
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
| | - M Labiche
- STFC Daresbury Laboratory, Daresbury, Warrington WA4 4AD, United Kingdom
| | - I Lazarus
- STFC Daresbury Laboratory, Daresbury, Warrington WA4 4AD, United Kingdom
| | - J Liang
- McMaster University, Department of Physics and Astronomy, Hamilton, Ontario L8S 4M1, Canada
| | - Z Liu
- Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China
- School of Nuclear Science and Technology, University of Chinese Academy of Sciences, Beijing 100049, China
| | - K Matsui
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
- University of Tokyo, Department of Physics, Tokyo 113-0033, Japan
| | - K Miernik
- Faculty of Physics, University of Warsaw, PL02-093 Warsaw, Poland
| | - B Moon
- Center for Exotic Nuclear Studies, Institute for Basic Science, Daejeon 34126, Republic of Korea
| | - A I Morales
- Instituto de Fsica Corpuscular, CSIC and Universitat de Valencia, E-46980 Paterna, Spain
| | - P Morrall
- STFC Daresbury Laboratory, Daresbury, Warrington WA4 4AD, United Kingdom
| | - N Nepal
- Department of Physics, Central Michigan University, Mount Pleasant, Michigan 48859, USA
| | - R D Page
- Department of Physics, University of Liverpool, Liverpool L69 7ZE, United Kingdom
| | | | - V F E Pucknell
- STFC Daresbury Laboratory, Daresbury, Warrington WA4 4AD, United Kingdom
| | - B C Rasco
- Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - B Rubio
- Instituto de Fsica Corpuscular, CSIC and Universitat de Valencia, E-46980 Paterna, Spain
| | - H Sakurai
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
- University of Tokyo, Department of Physics, Tokyo 113-0033, Japan
| | - Y Shimizu
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
| | - D W Stracener
- Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - T Sumikama
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
| | - H Suzuki
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
| | - J L Tain
- Instituto de Fsica Corpuscular, CSIC and Universitat de Valencia, E-46980 Paterna, Spain
| | - H Takeda
- RIKEN Nishina Center, Wako, Saitama 351-0198, Japan
| | - A Tarifeño-Saldivia
- Instituto de Fsica Corpuscular, CSIC and Universitat de Valencia, E-46980 Paterna, Spain
- Universitat Politecnica de Catalunya, E-08028 Barcelona, Spain
| | - A Tolosa-Delgado
- Instituto de Fsica Corpuscular, CSIC and Universitat de Valencia, E-46980 Paterna, Spain
| | - M Wolińska-Cichocka
- Heavy Ion Laboratory, University of Warsaw, Pasteura 5A, PL-02-093 Warsaw, Poland
| | - P J Woods
- School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3FD, United Kingdom
| | - R Yokoyama
- Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
- Center for Nuclear Study, University of Tokyo, RIKEN Campus, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
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3
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Ciani GF, Csedreki L, Rapagnani D, Aliotta M, Balibrea-Correa J, Barile F, Bemmerer D, Best A, Boeltzig A, Broggini C, Bruno CG, Caciolli A, Cavanna F, Chillery T, Colombetti P, Corvisiero P, Cristallo S, Davinson T, Depalo R, Di Leva A, Elekes Z, Ferraro F, Fiore E, Formicola A, Fülöp Z, Gervino G, Guglielmetti A, Gustavino C, Gyürky G, Imbriani G, Junker M, Lugaro M, Marigo P, Masha E, Menegazzo R, Mossa V, Pantaleo FR, Paticchio V, Perrino R, Piatti D, Prati P, Schiavulli L, Stöckel K, Straniero O, Szücs T, Takács MP, Terrasi F, Vescovi D, Zavatarelli S. Direct Measurement of the ^{13}C(α,n)^{16}O Cross Section into the s-Process Gamow Peak. Phys Rev Lett 2021; 127:152701. [PMID: 34677992 DOI: 10.1103/physrevlett.127.152701] [Citation(s) in RCA: 9] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/11/2021] [Revised: 06/08/2021] [Accepted: 08/17/2021] [Indexed: 06/13/2023]
Abstract
One of the main neutron sources for the astrophysical s process is the reaction ^{13}C(α,n)^{16}O, taking place in thermally pulsing asymptotic giant branch stars at temperatures around 90 MK. To model the nucleosynthesis during this process the reaction cross section needs to be known in the 150-230 keV energy window (Gamow peak). At these sub-Coulomb energies, cross section direct measurements are severely affected by the low event rate, making us rely on input from indirect methods and extrapolations from higher-energy direct data. This leads to an uncertainty in the cross section at the relevant energies too high to reliably constrain the nuclear physics input to s-process calculations. We present the results from a new deep-underground measurement of ^{13}C(α,n)^{16}O, covering the energy range 230-300 keV, with drastically reduced uncertainties over previous measurements and for the first time providing data directly inside the s-process Gamow peak. Selected stellar models have been computed to estimate the impact of our revised reaction rate. For stars of nearly solar composition, we find sizeable variations of some isotopes, whose production is influenced by the activation of close-by branching points that are sensitive to the neutron density, in particular, the two radioactive nuclei ^{60}Fe and ^{205}Pb, as well as ^{152}Gd.
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Affiliation(s)
- G F Ciani
- Gran Sasso Science Institute, Viale F. Crispi 7, 67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi, Italy
- Institute for Nuclear Research (ATOMKI), P.O. Box 51, HU-4001 Debrecen, Hungary
| | - L Csedreki
- Gran Sasso Science Institute, Viale F. Crispi 7, 67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi, Italy
- Institute for Nuclear Research (ATOMKI), P.O. Box 51, HU-4001 Debrecen, Hungary
| | - D Rapagnani
- Università di Napoli "Federico II," 80126 Napoli, Italy
- INFN, Sezione di Napoli, 80126 Napoli, Italy
| | - M Aliotta
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - J Balibrea-Correa
- Università di Napoli "Federico II," 80126 Napoli, Italy
- INFN, Sezione di Napoli, 80126 Napoli, Italy
| | - F Barile
- Università degli Studi di Bari, 70121 Bari, Italy
- INFN, Sezione di Bari, 70125 Bari, Italy
| | - D Bemmerer
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstrasse 400, 01328 Dresden, Germany
| | - A Best
- Università di Napoli "Federico II," 80126 Napoli, Italy
- INFN, Sezione di Napoli, 80126 Napoli, Italy
| | - A Boeltzig
- Università di Napoli "Federico II," 80126 Napoli, Italy
- INFN, Sezione di Napoli, 80126 Napoli, Italy
| | - C Broggini
- INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - C G Bruno
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - A Caciolli
- INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
- Università degli Studi di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - F Cavanna
- INFN, Sezione di Torino, Via Pietro Giuria, 1, 10125 Torino, Italy
| | - T Chillery
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - P Colombetti
- INFN, Sezione di Torino, Via Pietro Giuria, 1, 10125 Torino, Italy
| | - P Corvisiero
- Università degli Studi di Genova, 16126 Genova, Italy
- INFN, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - S Cristallo
- INAF, Osservatorio Astronomico d'Abruzzo, 64100 Teramo, Italy
- INFN, Sezione of Perugia, Via A. Pascoli snc, 06123 Perugia, Italy
| | - T Davinson
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - R Depalo
- INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
- Università degli Studi di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - A Di Leva
- Università di Napoli "Federico II," 80126 Napoli, Italy
- INFN, Sezione di Napoli, 80126 Napoli, Italy
| | - Z Elekes
- Institute for Nuclear Research (ATOMKI), P.O. Box 51, HU-4001 Debrecen, Hungary
| | - F Ferraro
- Università degli Studi di Genova, 16126 Genova, Italy
- INFN, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - E Fiore
- Università degli Studi di Bari, 70121 Bari, Italy
- INFN, Sezione di Bari, 70125 Bari, Italy
| | - A Formicola
- INFN, Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi, Italy
| | - Zs Fülöp
- Institute for Nuclear Research (ATOMKI), P.O. Box 51, HU-4001 Debrecen, Hungary
| | - G Gervino
- Università degli Studi di Torino, 10125 Torino, Italy
- INFN, Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy
| | - A Guglielmetti
- Università degli Studi di Milano, 20133 Milano, Italy
- INFN, Sezione di Milano, Via G. Celoria 16, 20133 Milano, Italy
| | - C Gustavino
- INFN, Sezione di Roma La Sapienza, Piazzale A. Moro 2, 00185 Roma, Italy
| | - Gy Gyürky
- Institute for Nuclear Research (ATOMKI), P.O. Box 51, HU-4001 Debrecen, Hungary
| | - G Imbriani
- Università di Napoli "Federico II," 80126 Napoli, Italy
- INFN, Sezione di Napoli, 80126 Napoli, Italy
| | - M Junker
- INFN, Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi, Italy
| | - M Lugaro
- Institute of Physics, ELTE Eötvös Loránd University, 1053 Budapest, Hungary
- Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, MTA Centre for Excellence, 1121 Budapest, Hungary
| | - P Marigo
- INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
- Università degli Studi di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - E Masha
- Università degli Studi di Milano, 20133 Milano, Italy
- INFN, Sezione di Milano, Via G. Celoria 16, 20133 Milano, Italy
| | - R Menegazzo
- INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - V Mossa
- INFN, Sezione di Bari, 70125 Bari, Italy
| | - F R Pantaleo
- Università degli Studi di Bari, 70121 Bari, Italy
- INFN, Sezione di Bari, 70125 Bari, Italy
| | | | - R Perrino
- INFN, Sezione di Bari, 70125 Bari, Italy
| | - D Piatti
- INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
- Università degli Studi di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - P Prati
- Università degli Studi di Genova, 16126 Genova, Italy
- INFN, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - L Schiavulli
- Università degli Studi di Bari, 70121 Bari, Italy
- INFN, Sezione di Bari, 70125 Bari, Italy
| | - K Stöckel
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstrasse 400, 01328 Dresden, Germany
- Technische Universität Dresden, Institut für Kern- und Teilchenphysik, Zellescher Weg 19, 01069 Dresden, Germany
| | - O Straniero
- INFN, Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi, Italy
- INAF, Osservatorio Astronomico d'Abruzzo, 64100 Teramo, Italy
| | - T Szücs
- Institute for Nuclear Research (ATOMKI), P.O. Box 51, HU-4001 Debrecen, Hungary
| | - M P Takács
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstrasse 400, 01328 Dresden, Germany
- Technische Universität Dresden, Institut für Kern- und Teilchenphysik, Zellescher Weg 19, 01069 Dresden, Germany
| | - F Terrasi
- INFN, Sezione di Napoli, 80126 Napoli, Italy
- Università degli Studi della Campania "L. Vanvitelli" (Caserta), 81100 Caserta, Italy
| | - D Vescovi
- INFN, Sezione of Perugia, Via A. Pascoli snc, 06123 Perugia, Italy
- Goethe University, Max-von-Laue-Strasse 1, Frankfurt am Main 60438, Germany
| | - S Zavatarelli
- INFN, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
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4
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Mossa V, Stöckel K, Cavanna F, Ferraro F, Aliotta M, Barile F, Bemmerer D, Best A, Boeltzig A, Broggini C, Bruno CG, Caciolli A, Chillery T, Ciani GF, Corvisiero P, Csedreki L, Davinson T, Depalo R, Di Leva A, Elekes Z, Fiore EM, Formicola A, Fülöp Z, Gervino G, Guglielmetti A, Gustavino C, Gyürky G, Imbriani G, Junker M, Kievsky A, Kochanek I, Lugaro M, Marcucci LE, Mangano G, Marigo P, Masha E, Menegazzo R, Pantaleo FR, Paticchio V, Perrino R, Piatti D, Pisanti O, Prati P, Schiavulli L, Straniero O, Szücs T, Takács MP, Trezzi D, Viviani M, Zavatarelli S. The baryon density of the Universe from an improved rate of deuterium burning. Nature 2020; 587:210-213. [PMID: 33177669 DOI: 10.1038/s41586-020-2878-4] [Citation(s) in RCA: 58] [Impact Index Per Article: 14.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/07/2020] [Accepted: 09/16/2020] [Indexed: 11/09/2022]
Abstract
Light elements were produced in the first few minutes of the Universe through a sequence of nuclear reactions known as Big Bang nucleosynthesis (BBN)1,2. Among the light elements produced during BBN1,2, deuterium is an excellent indicator of cosmological parameters because its abundance is highly sensitive to the primordial baryon density and also depends on the number of neutrino species permeating the early Universe. Although astronomical observations of primordial deuterium abundance have reached percent accuracy3, theoretical predictions4-6 based on BBN are hampered by large uncertainties on the cross-section of the deuterium burning D(p,γ)3He reaction. Here we show that our improved cross-sections of this reaction lead to BBN estimates of the baryon density at the 1.6 percent level, in excellent agreement with a recent analysis of the cosmic microwave background7. Improved cross-section data were obtained by exploiting the negligible cosmic-ray background deep underground at the Laboratory for Underground Nuclear Astrophysics (LUNA) of the Laboratori Nazionali del Gran Sasso (Italy)8,9. We bombarded a high-purity deuterium gas target10 with an intense proton beam from the LUNA 400-kilovolt accelerator11 and detected the γ-rays from the nuclear reaction under study with a high-purity germanium detector. Our experimental results settle the most uncertain nuclear physics input to BBN calculations and substantially improve the reliability of using primordial abundances to probe the physics of the early Universe.
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Affiliation(s)
- V Mossa
- INFN, Sezione di Bari, Bari, Italy
| | - K Stöckel
- Helmholtz-Zentrum Dresden-Rossendorf, Dresden, Germany.,Technische Universität Dresden, Dresden, Germany
| | - F Cavanna
- INFN, Sezione di Genova, Genoa, Italy.,INFN, Sezione di Torino, Turin, Italy
| | - F Ferraro
- INFN, Sezione di Genova, Genoa, Italy.,Università degli Studi di Genova, Genoa, Italy
| | - M Aliotta
- School of Physics and Astronomy, SUPA, University of Edinburgh, Edinburgh, UK
| | - F Barile
- INFN, Sezione di Bari, Bari, Italy
| | - D Bemmerer
- Helmholtz-Zentrum Dresden-Rossendorf, Dresden, Germany
| | - A Best
- Università degli Studi di Napoli "Federico II", Naples, Italy.,INFN, Sezione di Napoli, Naples, Italy
| | - A Boeltzig
- Gran Sasso Science Institute, L'Aquila, Italy.,INFN, Laboratori Nazionali del Gran Sasso (LNGS), Assergi, Italy
| | | | - C G Bruno
- School of Physics and Astronomy, SUPA, University of Edinburgh, Edinburgh, UK
| | - A Caciolli
- INFN, Sezione di Padova, Padua, Italy.,Università degli Studi di Padova, Padua, Italy
| | - T Chillery
- School of Physics and Astronomy, SUPA, University of Edinburgh, Edinburgh, UK
| | - G F Ciani
- Gran Sasso Science Institute, L'Aquila, Italy.,INFN, Laboratori Nazionali del Gran Sasso (LNGS), Assergi, Italy
| | - P Corvisiero
- INFN, Sezione di Genova, Genoa, Italy.,Università degli Studi di Genova, Genoa, Italy
| | - L Csedreki
- Gran Sasso Science Institute, L'Aquila, Italy.,INFN, Laboratori Nazionali del Gran Sasso (LNGS), Assergi, Italy
| | - T Davinson
- School of Physics and Astronomy, SUPA, University of Edinburgh, Edinburgh, UK
| | - R Depalo
- INFN, Sezione di Padova, Padua, Italy
| | - A Di Leva
- Università degli Studi di Napoli "Federico II", Naples, Italy.,INFN, Sezione di Napoli, Naples, Italy
| | - Z Elekes
- Institute for Nuclear Research (Atomki), Debrecen, Hungary
| | - E M Fiore
- INFN, Sezione di Bari, Bari, Italy.,Dipartimento Interateneo di Fisica, Università degli Studi di Bari, Bari, Italy
| | - A Formicola
- INFN, Laboratori Nazionali del Gran Sasso (LNGS), Assergi, Italy
| | - Zs Fülöp
- Institute for Nuclear Research (Atomki), Debrecen, Hungary
| | - G Gervino
- Università degli Studi di Torino, Turin, Italy.,INFN, Sezione di Torino, Turin, Italy
| | - A Guglielmetti
- Università degli Studi di Milano, Milan, Italy.,INFN, Sezione di Milano, Milan, Italy
| | | | - G Gyürky
- Institute for Nuclear Research (Atomki), Debrecen, Hungary
| | - G Imbriani
- Università degli Studi di Napoli "Federico II", Naples, Italy.,INFN, Sezione di Napoli, Naples, Italy
| | - M Junker
- INFN, Laboratori Nazionali del Gran Sasso (LNGS), Assergi, Italy
| | | | - I Kochanek
- INFN, Laboratori Nazionali del Gran Sasso (LNGS), Assergi, Italy
| | - M Lugaro
- Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, MTA Centre for Excellence, Budapest, Hungary.,Institute of Physics, ELTE Eötvös Loránd University, Budapest, Hungary
| | - L E Marcucci
- INFN, Sezione di Pisa, Pisa, Italy.,Dipartimento di Fisica "E. Fermi", Università degli Studi di Pisa, Pisa, Italy
| | - G Mangano
- Università degli Studi di Napoli "Federico II", Naples, Italy.,INFN, Sezione di Napoli, Naples, Italy
| | - P Marigo
- INFN, Sezione di Padova, Padua, Italy.,Università degli Studi di Padova, Padua, Italy
| | - E Masha
- Università degli Studi di Milano, Milan, Italy.,INFN, Sezione di Milano, Milan, Italy
| | | | - F R Pantaleo
- INFN, Sezione di Bari, Bari, Italy.,Dipartimento Interateneo di Fisica, Politecnico di Bari, Bari, Italy
| | | | - R Perrino
- INFN, Sezione di Bari, Bari, Italy.,INFN, Sezione di Lecce, Lecce, Italy
| | - D Piatti
- INFN, Sezione di Padova, Padua, Italy
| | - O Pisanti
- Università degli Studi di Napoli "Federico II", Naples, Italy.,INFN, Sezione di Napoli, Naples, Italy
| | - P Prati
- INFN, Sezione di Genova, Genoa, Italy.,Università degli Studi di Genova, Genoa, Italy
| | - L Schiavulli
- INFN, Sezione di Bari, Bari, Italy.,Dipartimento Interateneo di Fisica, Università degli Studi di Bari, Bari, Italy
| | - O Straniero
- INFN, Laboratori Nazionali del Gran Sasso (LNGS), Assergi, Italy.,INAF Osservatorio Astronomico d'Abruzzo, Teramo, Italy
| | - T Szücs
- Helmholtz-Zentrum Dresden-Rossendorf, Dresden, Germany
| | - M P Takács
- Helmholtz-Zentrum Dresden-Rossendorf, Dresden, Germany.,Technische Universität Dresden, Dresden, Germany
| | - D Trezzi
- Università degli Studi di Milano, Milan, Italy.,INFN, Sezione di Milano, Milan, Italy
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5
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Ferraro F, Takács MP, Piatti D, Cavanna F, Depalo R, Aliotta M, Bemmerer D, Best A, Boeltzig A, Broggini C, Bruno CG, Caciolli A, Chillery T, Ciani GF, Corvisiero P, Davinson T, D'Erasmo G, Di Leva A, Elekes Z, Fiore EM, Formicola A, Fülöp Z, Gervino G, Guglielmetti A, Gustavino C, Gyürky G, Imbriani G, Junker M, Karakas A, Kochanek I, Lugaro M, Marigo P, Menegazzo R, Mossa V, Pantaleo FR, Paticchio V, Perrino R, Prati P, Schiavulli L, Stöckel K, Straniero O, Szücs T, Trezzi D, Zavatarelli S. Direct Capture Cross Section and the E_{p}=71 and 105 keV Resonances in the ^{22}Ne(p,γ)^{23}Na Reaction. Phys Rev Lett 2018; 121:172701. [PMID: 30411966 DOI: 10.1103/physrevlett.121.172701] [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: 07/12/2018] [Revised: 09/10/2018] [Indexed: 06/08/2023]
Abstract
The ^{22}Ne(p,γ)^{23}Na reaction, part of the neon-sodium cycle of hydrogen burning, may explain the observed anticorrelation between sodium and oxygen abundances in globular cluster stars. Its rate is controlled by a number of low-energy resonances and a slowly varying nonresonant component. Three new resonances at E_{p}=156.2, 189.5, and 259.7 keV have recently been observed and confirmed. However, significant uncertainty on the reaction rate remains due to the nonresonant process and to two suggested resonances at E_{p}=71 and 105 keV. Here, new ^{22}Ne(p,γ)^{23}Na data with high statistics and low background are reported. Stringent upper limits of 6×10^{-11} and 7×10^{-11} eV (90% confidence level), respectively, are placed on the two suggested resonances. In addition, the off-resonant S factor has been measured at unprecedented low energy, constraining the contributions from a subthreshold resonance and the direct capture process. As a result, at a temperature of 0.1 GK the error bar of the ^{22}Ne(p,γ)^{23}Na rate is now reduced by 3 orders of magnitude.
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Affiliation(s)
- F Ferraro
- Università degli Studi di Genova, Via Dodecaneso 33, 16146 Genova, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - M P Takács
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstr. 400, 01328 Dresden, Germany
- Technische Universität Dresden, Institut für Kern- und Teilchenphysik, Zellescher Weg 19, 01069 Dresden, Germany
| | - D Piatti
- Dipartimento di Fisica e Astronomia, Università degli Studi di Padova, Via F. Marzolo 8, 35131 Padova, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - F Cavanna
- Istituto Nazionale di Fisica Nucleare, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - R Depalo
- Dipartimento di Fisica e Astronomia, Università degli Studi di Padova, Via F. Marzolo 8, 35131 Padova, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - M Aliotta
- School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - D Bemmerer
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstr. 400, 01328 Dresden, Germany
| | - A Best
- Università degli Studi di Napoli "Federico II", Dipartimento di Fisica "E. Pancini", Via Cintia, 80126 Napoli, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Via Cintia, 80126 Napoli, Italy
| | - A Boeltzig
- Gran Sasso Science Institute, 67100 L'Aquila, Italy
| | - C Broggini
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - C G Bruno
- School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - A Caciolli
- Dipartimento di Fisica e Astronomia, Università degli Studi di Padova, Via F. Marzolo 8, 35131 Padova, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - T Chillery
- School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - G F Ciani
- Gran Sasso Science Institute, 67100 L'Aquila, Italy
- Istituto Nazionale di Fisica Nucleare Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi (AQ), Italy
| | - P Corvisiero
- Università degli Studi di Genova, Via Dodecaneso 33, 16146 Genova, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - T Davinson
- School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - G D'Erasmo
- Università degli Studi di Bari, 70125 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70125 Bari, Italy
| | - A Di Leva
- Università degli Studi di Napoli "Federico II", Dipartimento di Fisica "E. Pancini", Via Cintia, 80126 Napoli, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Via Cintia, 80126 Napoli, Italy
| | - Z Elekes
- Institute for Nuclear Research of the Hungarian Academy of Sciences (MTA Atomki), PO Box 51, H-4001 Debrecen, Hungary
| | - E M Fiore
- Università degli Studi di Bari, 70125 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70125 Bari, Italy
| | - A Formicola
- Istituto Nazionale di Fisica Nucleare Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi (AQ), Italy
| | - Zs Fülöp
- Institute for Nuclear Research of the Hungarian Academy of Sciences (MTA Atomki), PO Box 51, H-4001 Debrecen, Hungary
| | - G Gervino
- Istituto Nazionale di Fisica Nucleare, Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy
- Università degli Studi di Torino, Via P. Giuria 1, 10125 Torino, Italy
| | - A Guglielmetti
- Università degli Studi di Milano, Via G. Celoria 16, 20133 Milano, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Milano, Via G. Celoria 16, 20133 Milano, Italy
| | - C Gustavino
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma La Sapienza, Piazzale A. Moro 2, 00185 Roma, Italy
| | - Gy Gyürky
- Institute for Nuclear Research of the Hungarian Academy of Sciences (MTA Atomki), PO Box 51, H-4001 Debrecen, Hungary
| | - G Imbriani
- Università degli Studi di Napoli "Federico II", Dipartimento di Fisica "E. Pancini", Via Cintia, 80126 Napoli, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Via Cintia, 80126 Napoli, Italy
| | - M Junker
- Istituto Nazionale di Fisica Nucleare Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi (AQ), Italy
| | - A Karakas
- Monash Centre for Astrophysics, School of Physics & Astronomy, Monash University, VIC 3800, Australia
| | - I Kochanek
- Istituto Nazionale di Fisica Nucleare Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi (AQ), Italy
| | - M Lugaro
- Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, 1121 Budapest, Hungary
| | - P Marigo
- Dipartimento di Fisica e Astronomia, Università degli Studi di Padova, Via F. Marzolo 8, 35131 Padova, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - R Menegazzo
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - V Mossa
- Università degli Studi di Bari, 70125 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70125 Bari, Italy
| | - F R Pantaleo
- Università degli Studi di Bari, 70125 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70125 Bari, Italy
| | - V Paticchio
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70125 Bari, Italy
| | - R Perrino
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70125 Bari, Italy
| | - P Prati
- Università degli Studi di Genova, Via Dodecaneso 33, 16146 Genova, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - L Schiavulli
- Università degli Studi di Bari, 70125 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70125 Bari, Italy
| | - K Stöckel
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstr. 400, 01328 Dresden, Germany
- Technische Universität Dresden, Institut für Kern- und Teilchenphysik, Zellescher Weg 19, 01069 Dresden, Germany
| | - O Straniero
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Via Cintia, 80126 Napoli, Italy
- Osservatorio Astronomico di Collurania, 64100 Teramo, Italy
| | - T Szücs
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstr. 400, 01328 Dresden, Germany
- Institute for Nuclear Research of the Hungarian Academy of Sciences (MTA Atomki), PO Box 51, H-4001 Debrecen, Hungary
| | - D Trezzi
- Università degli Studi di Milano, Via G. Celoria 16, 20133 Milano, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Milano, Via G. Celoria 16, 20133 Milano, Italy
| | - S Zavatarelli
- Istituto Nazionale di Fisica Nucleare, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
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6
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Cavanna F, Depalo R, Aliotta M, Anders M, Bemmerer D, Best A, Boeltzig A, Broggini C, Bruno CG, Caciolli A, Corvisiero P, Davinson T, di Leva A, Elekes Z, Ferraro F, Formicola A, Fülöp Z, Gervino G, Guglielmetti A, Gustavino C, Gyürky G, Imbriani G, Junker M, Menegazzo R, Mossa V, Pantaleo FR, Prati P, Scott DA, Somorjai E, Straniero O, Strieder F, Szücs T, Takács MP, Trezzi D. Erratum: Three New Low-Energy Resonances in the ^{22}Ne(p,γ)^{23}Na Reaction [Phys. Rev. Lett. 115, 252501 (2015)]. Phys Rev Lett 2018; 120:239901. [PMID: 29932705 DOI: 10.1103/physrevlett.120.239901] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/14/2018] [Indexed: 06/08/2023]
Abstract
This corrects the article DOI: 10.1103/PhysRevLett.115.252501.
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7
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Bruno CG, Scott DA, Aliotta M, Formicola A, Best A, Boeltzig A, Bemmerer D, Broggini C, Caciolli A, Cavanna F, Ciani GF, Corvisiero P, Davinson T, Depalo R, Di Leva A, Elekes Z, Ferraro F, Fülöp Z, Gervino G, Guglielmetti A, Gustavino C, Gyürky G, Imbriani G, Junker M, Menegazzo R, Mossa V, Pantaleo FR, Piatti D, Prati P, Somorjai E, Straniero O, Strieder F, Szücs T, Takács MP, Trezzi D. Improved Direct Measurement of the 64.5 keV Resonance Strength in the ^{17}O(p,α)^{14}N Reaction at LUNA. Phys Rev Lett 2016; 117:142502. [PMID: 27740778 DOI: 10.1103/physrevlett.117.142502] [Citation(s) in RCA: 10] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/29/2016] [Indexed: 06/06/2023]
Abstract
The ^{17}O(p,α)^{14}N reaction plays a key role in various astrophysical scenarios, from asymptotic giant branch stars to classical novae. It affects the synthesis of rare isotopes such as ^{17}O and ^{18}F, which can provide constraints on astrophysical models. A new direct determination of the E_{R}=64.5 keV resonance strength performed at the Laboratory for Underground Nuclear Astrophysics (LUNA) accelerator has led to the most accurate value to date ωγ=10.0±1.4_{stat}±0.7_{syst} neV, thanks to a significant background reduction underground and generally improved experimental conditions. The (bare) proton partial width of the corresponding state at E_{x}=5672 keV in ^{18}F is Γ_{p}=35±5_{stat}±3_{syst} neV. This width is about a factor of 2 higher than previously estimated, thus leading to a factor of 2 increase in the ^{17}O(p, α)^{14}N reaction rate at astrophysical temperatures relevant to shell hydrogen burning in red giant and asymptotic giant branch stars. The new rate implies lower ^{17}O/^{16}O ratios, with important implications on the interpretation of astrophysical observables from these stars.
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Affiliation(s)
- C G Bruno
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - D A Scott
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - M Aliotta
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - A Formicola
- INFN, Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi, Italy
| | - A Best
- Università di Napoli "Federico II" and INFN, Sezione di Napoli, 80126 Napoli, Italy
| | - A Boeltzig
- Gran Sasso Science Institute, INFN, Viale F. Crispi 7, 67100 L'Aquila, Italy
| | - D Bemmerer
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstrasse 400, 01328 Dresden, Germany
| | - C Broggini
- INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - A Caciolli
- Università degli Studi di Padova and INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - F Cavanna
- Università degli Studi di Genova and INFN, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - G F Ciani
- Gran Sasso Science Institute, INFN, Viale F. Crispi 7, 67100 L'Aquila, Italy
| | - P Corvisiero
- Università degli Studi di Genova and INFN, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - T Davinson
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - R Depalo
- Università degli Studi di Padova and INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - A Di Leva
- Università di Napoli "Federico II" and INFN, Sezione di Napoli, 80126 Napoli, Italy
| | - Z Elekes
- Institute for Nuclear Research (MTA ATOMKI), P.O. Box 51, HU-4001 Debrecen, Hungary
| | - F Ferraro
- Università degli Studi di Genova and INFN, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - Zs Fülöp
- Institute for Nuclear Research (MTA ATOMKI), P.O. Box 51, HU-4001 Debrecen, Hungary
| | - G Gervino
- Università degli Studi di Torino and INFN, Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy
| | - A Guglielmetti
- Università degli Studi di Milano and INFN, Sezione di Milano, Via G. Celoria 16, 20133 Milano, Italy
| | - C Gustavino
- INFN, Sezione di Roma La Sapienza, Piazzale A. Moro 2, 00185 Roma, Italy
| | - Gy Gyürky
- Institute for Nuclear Research (MTA ATOMKI), P.O. Box 51, HU-4001 Debrecen, Hungary
| | - G Imbriani
- Università di Napoli "Federico II" and INFN, Sezione di Napoli, 80126 Napoli, Italy
| | - M Junker
- INFN, Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi, Italy
| | - R Menegazzo
- INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - V Mossa
- Università degli Studi di Bari e INFN, Sezione di Bari, 70125 Bari, Italy
| | - F R Pantaleo
- Università degli Studi di Bari e INFN, Sezione di Bari, 70125 Bari, Italy
| | - D Piatti
- Università degli Studi di Padova and INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - P Prati
- Università degli Studi di Genova and INFN, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - E Somorjai
- Institute for Nuclear Research (MTA ATOMKI), P.O. Box 51, HU-4001 Debrecen, Hungary
| | - O Straniero
- Osservatorio Astronomico di Collurania, Teramo, INFN, Sezione di Napoli, 80126 Napoli, Italy
| | - F Strieder
- South Dakota School of Mines, 501 E. Saint Joseph Street, South Dakota 57701, USA
| | - T Szücs
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstrasse 400, 01328 Dresden, Germany
| | - M P Takács
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstrasse 400, 01328 Dresden, Germany
| | - D Trezzi
- Università degli Studi di Milano and INFN, Sezione di Milano, Via G. Celoria 16, 20133 Milano, Italy
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8
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Cavanna F, Depalo R, Aliotta M, Anders M, Bemmerer D, Best A, Boeltzig A, Broggini C, Bruno CG, Caciolli A, Corvisiero P, Davinson T, di Leva A, Elekes Z, Ferraro F, Formicola A, Fülöp Z, Gervino G, Guglielmetti A, Gustavino C, Gyürky G, Imbriani G, Junker M, Menegazzo R, Mossa V, Pantaleo FR, Prati P, Scott DA, Somorjai E, Straniero O, Strieder F, Szücs T, Takács MP, Trezzi D. Three New Low-Energy Resonances in the ^{22}Ne(p,γ)^{23}Na Reaction. Phys Rev Lett 2015; 115:252501. [PMID: 26722918 DOI: 10.1103/physrevlett.115.252501] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/17/2015] [Indexed: 06/05/2023]
Abstract
The ^{22}Ne(p,γ)^{23}Na reaction takes part in the neon-sodium cycle of hydrogen burning. This cycle affects the synthesis of the elements between ^{20}Ne and ^{27}Al in asymptotic giant branch stars and novae. The ^{22}Ne(p,γ)^{23}Na reaction rate is very uncertain because of a large number of unobserved resonances lying in the Gamow window. At proton energies below 400 keV, only upper limits exist in the literature for the resonance strengths. Previous reaction rate evaluations differ by large factors. In the present work, the first direct observations of the ^{22}Ne(p,γ)^{23}Na resonances at 156.2, 189.5, and 259.7 keV are reported. Their resonance strengths are derived with 2%-7% uncertainty. In addition, upper limits for three other resonances are greatly reduced. Data are taken using a windowless ^{22}Ne gas target and high-purity germanium detectors at the Laboratory for Underground Nuclear Astrophysics in the Gran Sasso laboratory of the National Institute for Nuclear Physics, Italy, taking advantage of the ultralow background observed deep underground. The new reaction rate is a factor of 20 higher than the recent evaluation at a temperature of 0.1 GK, relevant to nucleosynthesis in asymptotic giant branch stars.
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Affiliation(s)
- F Cavanna
- Università degli Studi di Genova and INFN, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - R Depalo
- Università degli Studi di Padova and INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - M Aliotta
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - M Anders
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstr. 400, 01328 Dresden, Germany
- Technische Universität Dresden, Institut für Kern- und Teilchenphysik, Zellescher Weg 19, 01069 Dresden, Germany
| | - D Bemmerer
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstr. 400, 01328 Dresden, Germany
| | - A Best
- Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi (AQ), Italy
| | - A Boeltzig
- Gran Sasso Science Institute, 67100 LAquila, Italy
| | - C Broggini
- INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - C G Bruno
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - A Caciolli
- Università degli Studi di Padova and INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - P Corvisiero
- Università degli Studi di Genova and INFN, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - T Davinson
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3JZ Edinburgh, United Kingdom
| | - A di Leva
- Università di Napoli Federico II and INFN, Sezione di Napoli, 80126 Napoli, Italy
| | - Z Elekes
- Institute for Nuclear Research (MTA ATOMKI), PO Box 51, HU-4001 Debrecen, Hungary
| | - F Ferraro
- Università degli Studi di Genova and INFN, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - A Formicola
- Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi (AQ), Italy
| | - Zs Fülöp
- Institute for Nuclear Research (MTA ATOMKI), PO Box 51, HU-4001 Debrecen, Hungary
| | - G Gervino
- Università degli Studi di Torino and INFN, Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy
| | - A Guglielmetti
- Università degli Studi di Milano and INFN, Sezione di Milano, Via G. Celoria 16, 20133 Milano, Italy
| | - C Gustavino
- INFN, Sezione di Roma La Sapienza, Piazzale A. Moro 2, 00185 Roma, Italy
| | - Gy Gyürky
- Institute for Nuclear Research (MTA ATOMKI), PO Box 51, HU-4001 Debrecen, Hungary
| | - G Imbriani
- Università di Napoli Federico II and INFN, Sezione di Napoli, 80126 Napoli, Italy
| | - M Junker
- Laboratori Nazionali del Gran Sasso (LNGS), 67100 Assergi (AQ), Italy
| | - R Menegazzo
- INFN, Sezione di Padova, Via F. Marzolo 8, 35131 Padova, Italy
| | - V Mossa
- Università degli Studi di Bari and INFN, Sezione di Bari, 70125 Bari, Italy
| | - F R Pantaleo
- Università degli Studi di Bari and INFN, Sezione di Bari, 70125 Bari, Italy
| | - P Prati
- Università degli Studi di Genova and INFN, Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - D A Scott
- SUPA, School of Physics and Astronomy, University of Edinburgh, EH9 3JZ Edinburgh, United Kingdom
| | - E Somorjai
- Institute for Nuclear Research (MTA ATOMKI), PO Box 51, HU-4001 Debrecen, Hungary
| | - O Straniero
- Osservatorio Astronomico di Collurania, Teramo, and INFN, Sezione di Napoli, Napoli, Italy
| | - F Strieder
- Institut für Experimentalphysik III, Ruhr-Universität Bochum, 44780 Bochum, Germany
| | - T Szücs
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstr. 400, 01328 Dresden, Germany
| | - M P Takács
- Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstr. 400, 01328 Dresden, Germany
- Technische Universität Dresden, Institut für Kern- und Teilchenphysik, Zellescher Weg 19, 01069 Dresden, Germany
| | - D Trezzi
- Università degli Studi di Milano and INFN, Sezione di Milano, Via G. Celoria 16, 20133 Milano, Italy
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9
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Bruno CG. [Mezlocillin in bronchopneumopathy caused by neoplasm obstruction]. Arch Monaldi Mal Torace 1987; 42:389-96. [PMID: 3509656] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 01/06/2023]
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