Astrophysical factors of fusion extracted using the Trojan horse method
Journal Article
·
· Physical Review C
- Texas A & M Univ., College Station, TX (United States); DOE/OSTI
- Beihang Univ., Beijing (China)
- Curtin Univ., Perth, WA (Australia)
Carbon-carbon burning plays an important role in many stellar environments. Recently, Tumino et al. reported a sharp rise of the astrophysical S factor for carbon-carbon fusion determined using the indirect Trojan horse method. We demonstrate that the rise at low energies seen in the aforementioned work is an artifact of using an invalid plane-wave approximation that neglects the Coulomb interactions between charged particles. Our analysis shows that such a rise disappears if the Coulomb (or Coulomb-nuclear) interactions in the initial and final states are included.
- Research Organization:
- Texas A & M Univ., College Station, TX (United States)
- Sponsoring Organization:
- USDOE National Nuclear Security Administration (NNSA); NSF
- Grant/Contract Number:
- FG02-93ER40773; NA0003841
- OSTI ID:
- 1610250
- Alternate ID(s):
- OSTI ID: 1529709
- Journal Information:
- Physical Review C, Journal Name: Physical Review C Journal Issue: 6 Vol. 99; ISSN PRVCAN; ISSN 2469-9985
- Publisher:
- American Physical Society (APS)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
The initial mass-final luminosity relation of type II supernova progenitors. Hints of new physics? | text | January 2019 |
The Initial Mass–Final Luminosity Relation of Type II Supernova Progenitors: Hints of New Physics?
|
journal | August 2019 |
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