𝔖 Bobbio Scriptorium
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Nova reaction rates and experiments

✍ Scribed by S. Bishop; C. Herlitzius; J. Fiehl


Book ID
104089550
Publisher
Elsevier Science
Year
2011
Tongue
English
Weight
521 KB
Volume
66
Category
Article
ISSN
0146-6410

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✦ Synopsis


Oxygen-neon novae form a subset of classical novae events known to freshly synthesize nuclei up to mass number A 40. Because several gamma-ray emitters lie in this mass range, these novae are also interesting candidates for gamma-ray astronomy. The properties of excited states within those nuclei in this mass region play a critical role in determining the resonant (p, Ξ³ ) reaction rates, themselves, largely unknown for the unstable nuclei. We describe herein a new Doppler shift lifetime facility at the Maier-Leibnitz tandem laboratory, Technische UniversitΓ€t MΓΌnchen, with which we will map out important resonant (p, Ξ³ ) nova reaction rates.


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