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Ti-44, Al-26 and Mn-53 samples for nuclear astrophysics: The needs, the possibilities and the sources

Exploration of the physics involved in the production of cosmogenic radionuclides requires experiments using the same rare, radioactive nuclei in sufficient quantities. For this work, such exotic radionuclides have been extracted from previously proton-irradiated stainless steel samples using wet ch...

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Detalles Bibliográficos
Autores principales: Dressler, R, Ayranov, M, Bemmerer, D, Bunka, M, Dai, Y, Lederer, C, Fallis, J, Murphy, A StJ, Pignatari, M, Schumann, D, Stora, T, Stowasser, T, Thielemann, F K, Woods, P J
Publicado: 2012
Materias:
Acceso en línea:https://dx.doi.org/10.1088/0954-3899/39/10/105201
http://cds.cern.ch/record/1559766
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author Dressler, R
Ayranov, M
Bemmerer, D
Bunka, M
Dai, Y
Lederer, C
Fallis, J
Murphy, A StJ
Pignatari, M
Schumann, D
Stora, T
Stowasser, T
Thielemann, F K
Woods, P J
author_facet Dressler, R
Ayranov, M
Bemmerer, D
Bunka, M
Dai, Y
Lederer, C
Fallis, J
Murphy, A StJ
Pignatari, M
Schumann, D
Stora, T
Stowasser, T
Thielemann, F K
Woods, P J
author_sort Dressler, R
collection CERN
description Exploration of the physics involved in the production of cosmogenic radionuclides requires experiments using the same rare, radioactive nuclei in sufficient quantities. For this work, such exotic radionuclides have been extracted from previously proton-irradiated stainless steel samples using wet chemistry separation techniques. The irradiated construction material has arisen from an extended material research programme at the Paul Scherrer Institute, called STIP (SINQ Target Irradiation Program), where several thousand samples of different materials were irradiated with protons and neutrons of energies up to 570 MeV. In total, 8 Oe 10(17) atoms of (44)Ti, -10(16) atoms of (26)Al and -10(19) atoms of (53)Mn are available from selected samples. These materials may now be used to produce targets or radioactive beams for nuclear reaction studies with protons, neutrons and alpha-particles. The work is part of the ERAWAST initiative (Exotic Radionuclides from Accelerator Waste for Science and Technology), aimed at facilitating new collaborations between the isotope producers and users from different scientific fields including nuclear astrophysics.
id cern-1559766
institution Organización Europea para la Investigación Nuclear
publishDate 2012
record_format invenio
spelling cern-15597662019-09-30T06:29:59Zdoi:10.1088/0954-3899/39/10/105201http://cds.cern.ch/record/1559766Dressler, RAyranov, MBemmerer, DBunka, MDai, YLederer, CFallis, JMurphy, A StJPignatari, MSchumann, DStora, TStowasser, TThielemann, F KWoods, P JTi-44, Al-26 and Mn-53 samples for nuclear astrophysics: The needs, the possibilities and the sourcesAstrophysics and AstronomyNuclear Physics - TheoryExploration of the physics involved in the production of cosmogenic radionuclides requires experiments using the same rare, radioactive nuclei in sufficient quantities. For this work, such exotic radionuclides have been extracted from previously proton-irradiated stainless steel samples using wet chemistry separation techniques. The irradiated construction material has arisen from an extended material research programme at the Paul Scherrer Institute, called STIP (SINQ Target Irradiation Program), where several thousand samples of different materials were irradiated with protons and neutrons of energies up to 570 MeV. In total, 8 Oe 10(17) atoms of (44)Ti, -10(16) atoms of (26)Al and -10(19) atoms of (53)Mn are available from selected samples. These materials may now be used to produce targets or radioactive beams for nuclear reaction studies with protons, neutrons and alpha-particles. The work is part of the ERAWAST initiative (Exotic Radionuclides from Accelerator Waste for Science and Technology), aimed at facilitating new collaborations between the isotope producers and users from different scientific fields including nuclear astrophysics.oai:cds.cern.ch:15597662012
spellingShingle Astrophysics and Astronomy
Nuclear Physics - Theory
Dressler, R
Ayranov, M
Bemmerer, D
Bunka, M
Dai, Y
Lederer, C
Fallis, J
Murphy, A StJ
Pignatari, M
Schumann, D
Stora, T
Stowasser, T
Thielemann, F K
Woods, P J
Ti-44, Al-26 and Mn-53 samples for nuclear astrophysics: The needs, the possibilities and the sources
title Ti-44, Al-26 and Mn-53 samples for nuclear astrophysics: The needs, the possibilities and the sources
title_full Ti-44, Al-26 and Mn-53 samples for nuclear astrophysics: The needs, the possibilities and the sources
title_fullStr Ti-44, Al-26 and Mn-53 samples for nuclear astrophysics: The needs, the possibilities and the sources
title_full_unstemmed Ti-44, Al-26 and Mn-53 samples for nuclear astrophysics: The needs, the possibilities and the sources
title_short Ti-44, Al-26 and Mn-53 samples for nuclear astrophysics: The needs, the possibilities and the sources
title_sort ti-44, al-26 and mn-53 samples for nuclear astrophysics: the needs, the possibilities and the sources
topic Astrophysics and Astronomy
Nuclear Physics - Theory
url https://dx.doi.org/10.1088/0954-3899/39/10/105201
http://cds.cern.ch/record/1559766
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