What are the astrophysical sites for the r-process and the production of heavy elements?

2011/01/18 by F.‐K. Thielemann, F.-K. Thielemann, A. Arcones +21 · 2 citations
Physics and Astronomy · #Astronomical and nuclear sciences #Astrophysics #Ejecta #Gamma-ray bursts and supernovae #Neutrino #Neutron star #Nuclear physics #Nuclear physics research studies #Nucleosynthesis #Physics #Supernova #r-process

paper · doi:10.1016/j.ppnp.2011.01.032

openalex publication_date 2011/01/18 · crossref created 2011/01/18 · crossref issued 2011/04/01 · crossref published 2011/04/01 · crossref published-print 2011/04/01 · crossref deposited 2021/11/17 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/22 · crossref indexed 2026/08/05

Citations

• Ge<mml:mprescripts/><mml:none/>70(p,γ)As<mml:mprescripts/><mml:none/>71andGe<mml:mprescripts/><mml:none/>76(p,n)As<mml:mprescripts/><mml:none/>76cross sections for the astrophysicalpprocess: Sensitivity of the optical proton potential at low energies
• Branchings in the γ process path revisited
• [CLC][ITAL]r[/ITAL][/CLC]-Process in Neutron Star Mergers
• Nuclear weak-interaction processes in stars
• Nucleosynthesis in Magnetically Driven Jets from Collapsars
• Nucleosynthesis yields of core-collapse supernovae and hypernovae, and galactic chemical evolution
• The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis
• Explosive Nucleosynthesis from Gamma‐Ray Burst and Hypernova Progenitors: Direct Collapse versus Fallback
• Coulomb Suppression of the Stellar Enhancement Factor
• Ther‐Process in Neutrino‐driven Winds from Nascent, “Compact” Neutron Stars of Core‐Collapse Supernovae
• rp-process nucleosynthesis at extreme temperature and density conditions

Cited by

• A Chemical Signature from Fast-rotating Low-metallicity Massive Stars: ROA 276 in ω Centauri*
• R-process [wikipedia]