Difference between revisions of "References and Documents"
Jump to navigation
Jump to search
| Line 3: | Line 3: | ||
** Proposal [[Media:PAC40_proposal.pdf]] | ** Proposal [[Media:PAC40_proposal.pdf]] | ||
| − | = Bubble Chamber | + | = Bubble Chamber = |
* ''First determination of an astrophysical cross section with a bubble chamber: The <sup>15</sup>N(α, γ ) <sup>19</sup>F reaction'' | * ''First determination of an astrophysical cross section with a bubble chamber: The <sup>15</sup>N(α, γ ) <sup>19</sup>F reaction'' | ||
| Line 14: | Line 14: | ||
F. Seitz, Phys. of Fluids '''1''' (1957) 2 [[media:Phys.Fluids.1.2.pdf]] | F. Seitz, Phys. of Fluids '''1''' (1957) 2 [[media:Phys.Fluids.1.2.pdf]] | ||
| − | = Oxygen S-Factor | + | = Oxygen S-Factor = |
Revision as of 11:34, 1 August 2013
Program Advisory Committee (PAC)
- PAC40 Experiment Proposal (June 2013)
- Proposal Media:PAC40_proposal.pdf
Bubble Chamber
- First determination of an astrophysical cross section with a bubble chamber: The 15N(α, γ ) 19F reaction
C. Ugalde et al., Phys. Lett. B 719 (2013) 74 media:Bubble_Chamber_PLB_719_74_2013.pdf
- New insights into particle detection with superheated liquids
S. Archambault et al., New J. Phys. 13 (2011) 043006 media:Bubble_physics.pdf
- On the Theory of the Bubble Chamber
F. Seitz, Phys. of Fluids 1 (1957) 2 media:Phys.Fluids.1.2.pdf
Oxygen S-Factor
Nucleosynthesis
- Nucleosynthesis and remnants in massive stars of solar metallicity
S.E. Woosley and A. Heger, Phys. Reports 442 (2007 269 media:Phys.Reports.442.269.pdf