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Nucleosynthesis
The R-Process Nucleosynthesis and Related Challenges
Electron Capture in Stars
Star Factories: Nuclear Fusion and the Creation of the Elements
Heavy Element Nucleosynthesis
Sensitivity of Type Ia Supernovae to Electron Capture Rates E
Nucleosynthesis
S-Process Nucleosynthesis
Lecture 3: Nucleosynthesis
12.744/12.754 Lecture 2: Cosmic Abundances, Nucleosynthesis and Element Origins
Nucleosynthetic Isotope Variations of Siderophile and Chalcophile
1 Big Bang Nucleosynthesis: Overview
Lecture 7: "Basics of Star Formation and Stellar Nucleosynthesis" Outline
198 4Apj. . .211 . .7 91N the Astrophysical Journal, 277:791-805
Nucleosynthesis •Light Element Processes •Neutron Capture Processes •LEPP and P Nuclei •Explosive C-Burning •Explosive H-Burning •Degenerate Environments
Influence of Pairing and Deformation on Charge Exchange Transitions
Stellar Nucleosynthesis
Nuclear Binding Energy 1 Nuclear Binding Energy
Nucleosynthesis: the S-, R- and P- Processes
Top View
Nucleosynthesis
Nuclear Fusion: How Are Elements Created in Stars?
NUCLEOSYNTHESIS a Reasonable Starting Point for Isotope Geochemistry Is a Determination of the Abundances of the Naturally Occurring Nuclides
Supernova Nucleosynthesis
Stellar Nucleosynthesis
THE R-, S-, and P-PROCESSES in NUCLEOSYNTHESIS
R-Process Nucleosynthesis in Supernovae the Heaviest Elements Are Made Only in Cataclysmic Events
The Nucleosynthesis of Chemical Elements Outline
P-Process Nucleosynthesis Via Proton-Capture Reactions in Thermonuclear Supernovae Explosions
Nucleosynthesis of Heavy Elements in Supernovae and Neutron-Star Mergers
Current Status of R -Process Nucleosynthesis
Double Beta Decay - Physics Beyond the Standard Model Now, and in Future (Genius)
Modern Results for the Cosmic Ray Nucleosynthesis of P-Nuclei
6 Big Bang Nucleosynthesis
Nucleosynthesis and Energy Production in Stars: Bethe's Crowning Achievement
Lecture 15 Explosive Nucleosynthesis and the R-Process
Nucleosynthesis and the Origin of the Elements
Research Article Electron Capture Cross Sections for Stellar Nucleosynthesis
Neutrinoless Double Beta Decay: Theory
R-Process Nucleosynthesis of the Heavy Elements
Nucleosynthesis and Galactic Chemical Evolution of the Isotopes of Oxygen
Neutron Star Mergers and Nucleosynthesis of Heavy Elements
Big Bang Nucleosynthesis
Nuclear Science and the New Standard Model: Fundamental Symmetries and Neutrinos in the Next Decade
High-Precision Penning-Trap Mass Spectrometry at SHIPTRAP and PENTATRAP for Neutrino Physics Research
Lecture 27: Stellar Nucleosynthesis
Big Bang Forgedthe First Elements
Supernova Nucleosynthesis
Nucleosynthesis 69
The Origin of the Elements
The R-Process in Supernovae and Neutron Star Mergers
Nucleosynthesis
Neutrinos and Nucleosynthesis the Effect of Neutrinos on Nucleosynthesis in Core-Collapse Supernovae
Nucleosynthesis at the Termination Point of the S Process
The Production of Proton-Rich Isotopes Beyond Iron: the Γ Process in Stars
Lecture 15 Explosive Nucleosynthesis and the R-Process
10 Nucleosynthesis
Radon Measurement for Neutrinoless Double Beta Decay Xavier Carlos Quintana University of New Mexico
Schatz, H. the Evolution of Elements and Isotopes. Elements
Chapter 7: Nucleosynthesis in Supernovae
Experiments for P-Process Nucleosynthesis with Special Focus on the Most Abundant P Nucleus 92Mo
Exotic Nuclei and Explosive Nucleosynthesis
BIG BANG NUCLEOSYNTHESIS the Binding Energies of the First Four Light Nuclei, 2H, 3H, 3He and 4He Are 2.22 Mev, 6.92 Mev, 7.72 M