Underground nuclear astrophysics studies with CASPAR

The drive of low-energy nuclear astrophysics laboratories is to study the reactions of importance to stellar burning processes and elemental production through stellar nucleosynthesis, over the energy range of astrophysical interest. As laboratory measurements approach the stellar burning window, th...

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Main Authors: Robertson Daniel, Couder Manoel, Greife Uwe, Strieder Frank, Wiescher Michael
Format: Article
Language:English
Published: EDP Sciences 2016-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/201610909002
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author Robertson Daniel
Couder Manoel
Greife Uwe
Strieder Frank
Wiescher Michael
author_facet Robertson Daniel
Couder Manoel
Greife Uwe
Strieder Frank
Wiescher Michael
author_sort Robertson Daniel
collection DOAJ
description The drive of low-energy nuclear astrophysics laboratories is to study the reactions of importance to stellar burning processes and elemental production through stellar nucleosynthesis, over the energy range of astrophysical interest. As laboratory measurements approach the stellar burning window, the rapid drop off of cross-sections is a significant barrier and drives the need to lower background interference. The natural background suppression of underground accelerator facilities enables the extension of current experimental data to lower energies. An example of such reactions of interest are those thought to be sources of neutrons for the s-process, the major production mechanism for elements above the iron peak. The reactions 13C(α,n)16O and 22Ne(α,n)25Mg are the proposed initial focus of the new nuclear astrophysics accelerator laboratory (CASPAR) currently under construction at the Sanford Underground Research Facility, Lead, South Dakota
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spelling doaj.art-cb13d296ce1a4f62af9f8d4dde7b12022022-12-21T22:25:20ZengEDP SciencesEPJ Web of Conferences2100-014X2016-01-011090900210.1051/epjconf/201610909002epjconf_omeg2016_09002Underground nuclear astrophysics studies with CASPARRobertson Daniel0Couder Manoel1Greife Uwe2Strieder Frank3Wiescher Michael4Department of Physics, University of Notre DameDepartment of Physics, University of Notre DameDepartment of Physics, Colorado School of MinesDepartment of Physics, South Dakota School of Mines and TechnologyDepartment of Physics, University of Notre DameThe drive of low-energy nuclear astrophysics laboratories is to study the reactions of importance to stellar burning processes and elemental production through stellar nucleosynthesis, over the energy range of astrophysical interest. As laboratory measurements approach the stellar burning window, the rapid drop off of cross-sections is a significant barrier and drives the need to lower background interference. The natural background suppression of underground accelerator facilities enables the extension of current experimental data to lower energies. An example of such reactions of interest are those thought to be sources of neutrons for the s-process, the major production mechanism for elements above the iron peak. The reactions 13C(α,n)16O and 22Ne(α,n)25Mg are the proposed initial focus of the new nuclear astrophysics accelerator laboratory (CASPAR) currently under construction at the Sanford Underground Research Facility, Lead, South Dakotahttp://dx.doi.org/10.1051/epjconf/201610909002
spellingShingle Robertson Daniel
Couder Manoel
Greife Uwe
Strieder Frank
Wiescher Michael
Underground nuclear astrophysics studies with CASPAR
EPJ Web of Conferences
title Underground nuclear astrophysics studies with CASPAR
title_full Underground nuclear astrophysics studies with CASPAR
title_fullStr Underground nuclear astrophysics studies with CASPAR
title_full_unstemmed Underground nuclear astrophysics studies with CASPAR
title_short Underground nuclear astrophysics studies with CASPAR
title_sort underground nuclear astrophysics studies with caspar
url http://dx.doi.org/10.1051/epjconf/201610909002
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AT coudermanoel undergroundnuclearastrophysicsstudieswithcaspar
AT greifeuwe undergroundnuclearastrophysicsstudieswithcaspar
AT striederfrank undergroundnuclearastrophysicsstudieswithcaspar
AT wieschermichael undergroundnuclearastrophysicsstudieswithcaspar