Tz = −1 nuclei in the rp-process — astrophysical implications and a new experimental approach-Reference-Cited by-同舟云学术

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Tz = −1 nuclei in the rp-process — astrophysical implications and a new experimental approach

Published:1999-07 Issue:1 Volume:654 Page:924c-927c
ISSN:0375-9474
Container-title:Nuclear Physics A
language:en
Short-container-title:Nuclear Physics A

Author:

Schatz H.,Bacher A.,Berg G.P.A.,Black T.C.,Choi S.,Foster C.C.,Görres J.,Jiang K.,Lozowski B.,Stech E.,Stephenson E.J.,Tischhauser P.,Wiescher M.

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference17 articles.

1. Explosive hydrogen burning

2. Reaction rates and reaction sequences in the rp-process

3. rp-process nucleosynthesis at extreme temperature and density conditions

4. Bridging the waiting points: The role of two-proton capture reactions in therpprocess

5. Hydrodynamic Studies of Accretion onto Massive White Dwarfs: ONeMg-enriched Nova Outbursts. I. Dependence on White Dwarf Mass

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1. First Direct Measurement Constraining the Ar34(α,p)K37 Reaction Cross Section for Mixed Hydrogen and Helium Burning in Accreting Neutron Stars;Physical Review Letters;2023-05-22

2. Nuclear Data Sheets for A=24;Nuclear Data Sheets;2022-12

3. Nuclear processes in astrophysics: Recent progress;The European Physical Journal A;2018-12

4. Dependence of X-Ray Burst Models on Nuclear Masses;The Astrophysical Journal;2017-08-01

5. Indirect study of the stellar Ar34(α,p)K37 reaction rate through Ca40(p,t)Ca38 reaction measurements;Physical Review C;2017-05-10

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