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Recent results from the carbon fusion project at Notre Dame

  • Brian Bucher
  • , Masahiro Notani
  • , Adam Alongi
  • , Justin Browne
  • , Craig Cahillane
  • , Erin Dahlstrom
  • , Paul Davies
  • , Xiao Fang
  • , Larry Lamm
  • , Chi Ma
  • , Alexander Moncion
  • , Wanpeng Tan
  • , Xiao Dong Tang
  • , Spencer Thomas

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

1 Scopus citations

Abstract

The carbon fusion project at Notre Dame is aimed towards measuring the 12C+12C fusion cross section and its decay branches relevant to astrophysics down to the lowest possible energies. To complement this approach, we are also exploring new techniques for providing more reliable extrapolations of the cross sections in the energy ranges where experimental data are unavailable. In this paper, we report two recent results: 1) an upper limit for the 12C+12C fusion cross section, and 2) a new measurement of 12C(12C,n) along with an improved extrapolation technique based on the mirror reaction channel, 12C(12C,p). The outlook for astrophysical heavy-ion fusion studies at Notre Dame is also discussed.

Original languageEnglish
Title of host publicationOrigin of Matter and Evolution of Galaxies 2011
Pages275-280
Number of pages6
DOIs
StatePublished - 2012
Externally publishedYes
EventInternational Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 - Wako, Japan
Duration: Nov 14 2011Nov 17 2011

Publication series

NameAIP Conference Proceedings
Volume1484
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

ConferenceInternational Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
Country/TerritoryJapan
CityWako
Period11/14/1111/17/11

Keywords

  • fusion
  • nuclear reactions
  • nucleosynthesis

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