Results 41 to 50 of about 3,422,985 (329)

Active-Sterile Neutrino Transformation and r-Process Nucleosynthesis [PDF]

open access: yes, 2000
The type II supernova is considered as a candidate site for the production of heavy elements. Since the supernova produces an intense neutrino flux, neutrino scattering processes will impact element formation.
McLaughlin, G. C.
core   +3 more sources

Estimation of Heat Source Model’s Parameters for GMAW with Non-linear Global Optimization—Part I: Application of Multi-island Genetic Algorithm

open access: yesMetals, 2020
Estimating the thermo-elasto-plastic deformation by arc welding through finite element analysis has been used in various industrial fields. The Goldak heat source model is one of the most important and widely used models in finite element analysis, and ...
Changmin Pyo, Jisun Kim, Jaewoong Kim
doaj   +1 more source

Changes in r-process abundances at late times [PDF]

open access: yes, 2001
We explore changes in abundance patterns that occur late in the r process. As the neutrons available for capture begin to disappear, a quasiequilibrium funnel shifts material into the large peaks at A=130 and A=195, and into the rare-earth "bump" at A ...
B. S. Meyer   +15 more
core   +3 more sources

Kinematic Prediction and Experimental Demonstration of Conditioning Process for Controlling the Profile Shape of a Chemical Mechanical Polishing Pad

open access: yesApplied Sciences, 2021
The uniformity of the wafer in a chemical mechanical polishing (CMP) process is vital to the ultra-fine and high integration of semiconductor structures.
Hanchul Cho   +3 more
doaj   +1 more source

A new r-process star with low abundances of r-process elements

open access: yesJournal of Physics: Conference Series, 2016
Metal-poor stars with measurable r-process element abundances provide key clues to the production site(s) of the r-process and how its products are mixed with the surrounding medium. While the number of stars exhibiting strong enhancements of r-process elements has grown over the years, the lower "floor" of r-process enrichment in metal-poor stars has ...
Frebel, Anna L.   +2 more
openaire   +2 more sources

Probing the Production of Actinides under Different r-process Conditions [PDF]

open access: yes, 2019
Several extremely metal-poor stars are known to have an enhanced thorium abundance. These actinide-boost stars have likely inherited material from an r-process that operated under different conditions than the r-process that is reflected in most other ...
Arcones, A.   +3 more
core   +3 more sources

Efficient co‐production of propionic acid and succinic acid by Propionibacterium acidipropionici using membrane separation coupled technology

open access: yesEngineering in Life Sciences, 2021
To improve the fermentation efficiency of Propionibacterium acidipropionici, a semi‐continuous coupled fermentation process was established to achieve co‐production of propionic acid (PA) and succinic acid (SA).
Xiaolian Li   +4 more
doaj   +1 more source

The End Of Nucleosynthesis: Production Of Lead And Thorium In The Early Galaxy [PDF]

open access: yes, 2009
We examine the Pb and Th abundances in 27 metal-poor stars (-3.1 56) enrichment was produced only by the rapid (r-) nucleosynthesis process. New abundances are derived from Hubble Space Telescope/Space Telescope Imaging Spectrograph, Keck/High ...
Christlieb, Norbert   +6 more
core   +2 more sources

Evaluation of micropillar array columns for chromatographic separation of phosphorothioated oligonucleotides and their diastereomers

open access: yesAnalytical Science Advances, 2021
Chromatographic analysis of therapeutic oligonucleotides is challenging due to the presence of closely related impurities, degradants or metabolites and due to the presence of phosphorothioate bonds, which introduce chiral centers.
Lieve Dillen   +5 more
doaj   +1 more source

Supernova Neutrino-Nucleus Physics and the r-process

open access: yes, 2004
This talk reviews three inputs important to neutrino-induced nucleosynthesis in a supernova: 1) "standard" properties of the supernova neutrino flux, 2) effects of phenomena like neutrino oscillations on that flux, and 3) nuclear structure issues in ...
Haxton, W. C.
core   +1 more source

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