Results 21 to 30 of about 65,258,316 (368)

The s-process branching at $^{186}$Re revised [PDF]

open access: yesProceedings of International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX — PoS(NIC-IX), 2010
info:eu-repo/semantics ...
Mohr, Peter   +3 more
openaire   +3 more sources

Chemical evolution with rotating massive star yields - I. The solar neighbourhood and the s-process elements [PDF]

open access: yes, 2018
We present a comprehensive study of the abundance evolution of the elements from H to U in the Milky Way halo and local disk. We use a consistent chemical evolution model, metallicity dependent isotopic yields from low and intermediate mass stars and ...
N. Prantzos   +5 more
semanticscholar   +1 more source

Discovery of s-process enhanced stars in the LAMOST survey [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2019
Here we present the discovery of 895 s-process-rich candidates from 454 180 giant stars observed by the Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) using a data-driven approach.
Brodie J. Norfolk   +9 more
semanticscholar   +1 more source

New s-process Mechanism in Rapidly Rotating Massive Population II Stars [PDF]

open access: yesAstrophysical Journal, 2019
We report a new mechanism for the s-process in rotating massive metal-poor stars. Our models show that above a critical rotation speed, such stars evolve in a quasi-chemically homogeneous fashion, which gives rise to a prolific s-process.
P. Banerjee, A. Heger, Y. Qian
semanticscholar   +1 more source

Application of Neutron Capture Reaction Rate from Kernel Ridge Regression Prediction in s-process Simulation

open access: yesYuanzineng kexue jishu, 2023
The origin of elements in the universe is a basic scientific problem. The slow neutron capture process (s-process) is believed to be responsible for the nucleosynthesis of about half of the elements heavier than iron.
HUANG Tianxing;WU Xinhui
doaj   +1 more source

Non-standard s-process in massive rotating stars [PDF]

open access: yesAstronomy & Astrophysics, 2018
Context. Recent studies show that rotation significantly affects the s-process in massive stars. Aims. We provide tables of yields for non-rotating and rotating massive stars between 10 and 150 M⊙ at Z = 10−3 ([Fe/H] = −1.8).
A. Choplin   +5 more
semanticscholar   +1 more source

Study of the Briquetting Process of Walnut Shells for Pyrolysis and Combustion

open access: yesApplied Sciences, 2023
Walnut shells can be used as fuels in power plants directly or as biochars obtained by pyrolysis or torrefaction. They are an example of clean waste biomass which shows a low ash content and a high Net Calorific Value, making them excellent for energy ...
Rafael Font   +5 more
doaj   +1 more source

Advances in s-process models [PDF]

open access: yesNuclear Physics A, 2001
8 pages, 4 figures, submitted for "Nuclei in the Cosmos 2000 ...
Lugaro, Maria, Herwig, Falk
openaire   +2 more sources

The s process in AGB stars as constrained by a large sample of barium stars [PDF]

open access: yesAstronomy & Astrophysics, 2018
Context. Barium (Ba) stars are dwarf and giant stars enriched in elements heavier than iron produced by the slow neutron-capture process (s process).
B. Cseh   +10 more
semanticscholar   +1 more source

Assessment of Two Materials as Adsorbents for the Effective Removal and Further Pre-Concentration of Gallium from Aqueous Solutions: Mesoporous Carbon vs. Clinoptilolite

open access: yesSeparations, 2023
In this research, the adsorption of gallium onto natural zeolite (clinoptilolite) and two mesoporous-activated carbons were compared and evaluated. The clinoptilolite was treated with HCl (HCPL), while mesoporous-activated carbons (MCSG60A and MCO1) were
Patricia Sáez   +6 more
doaj   +1 more source

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