Results 1 to 10 of about 52,014 (259)

Nucleosynthesis in Supernovae [PDF]

open access: greenPhysical Review Letters, 1999
Core collapse supernovae are dominated by energy transport from neutrinos. Therefore, some supernova properties could depend on symetries and features of the standard model weak interactions. The cross section for neutrino capture is larger than that for
Horowitz, C. J., Li, Gang
core   +7 more sources

Explosive Nucleosynthesis: Prospects [PDF]

open access: yesPhysics Reports, 1999
Explosive nucleosynthesis is a combination of the nuclear physics of thermonuclear reactions, and the hydrodynamics of the plasma in which the reactions occur. It depends upon the initial conditions---the stellar evolution up to the explosive instability,
A. van Riper   +49 more
core   +7 more sources

Leptonic Photons and Nucleosynthesis [PDF]

open access: yesPhysics Letters B, 1996
Should $U(1)$ long-range forces be associated to electron, muon and/or tau quantum number then their ''fine structure constants" are seen to be bound by nucleosynthesis data to be less than about $1.7 \times 10^{-11}$.
Grifols, J. A., Masso, E.
core   +6 more sources

Neutrinos and Primordial Nucleosynthesis [PDF]

open access: yesNuclear Physics B - Proceedings Supplements, 2004
The importance of the Big Bang Nucleosynthesis (BBN) as a unique tool for studying neutrino properties is discussed, and the recent steps towards a self-consistent and robust handling of the weak reaction decoupling from the thermal bath as well as of ...
Cuoco   +13 more
core   +5 more sources

Neutrino Effects in Nucleosynthesis [PDF]

open access: yesNeutrino Physics, 2000
The nucleosynthesis within a Type II supernova occurs in an intense neutrino flux. I discuss some of the effects associated with neutrino interactions, including direct synthesis in the neutrino process, the role of neutrinos in controlling the r-process
Haxton, W. C.
core   +7 more sources

Primordial Nucleosynthesis [PDF]

open access: yesJournal of Physics: Conference Series, 2013
Invited Plenary Talk given at the 11th International Conference on Nucleus-Nucleus Collisions (NN2012), San Antonio, Texas, USA, May 27-June 1, 2012. To appear in the NN2012 Proceedings in Journal of Physics: Conference Series (JPCS)
Coc, Alain, Vangioni, Elisabeth
openaire   +18 more sources

Neutrino nucleosynthesis [PDF]

open access: yesPhysics Letters B, 2005
We study neutrino process nucleosynthesis in massive stars using newly calculated cross sections, an expanded reaction network, and complete and self-consistent models of the progenitor star. We reevaluate the production of light isotopes from abundant progenitors as well as that of rare, heavy, proton-rich isotopes.
Heger, A.   +5 more
openaire   +4 more sources

Hypernovae and their nucleosynthesis [PDF]

open access: yesSymposium - International Astronomical Union, 2003
We review the characteristics of nucleosynthesis in ‘hypernovae’, i.e., core-collapse supernovae with very large explosion energies (≳ 1052 ergs). The hypernova yields show the following characteristics: (i) the mass ratio between the complete and incomplete Si burning regions is larger in hypernovae than normal supernovae.
Ken'ichi Nomoto   +5 more
openaire   +3 more sources

Hydrogen Tunneling in Stoichiometric and Catalytic Reactions involving Transition Metals

open access: yesChemCatChem, Volume 15, Issue 24, December 19, 2023., 2023
An overview on the importance of the participation of hydrogen tunneling in E−H bond activation reactions (E=C, O, Si…) mediated by transition metals is presented. Understanding when hydrogen tunneling occurs can be a powerful tool for designing new catalysts to perform challenging reactions.
Jon M. Matxain, Miguel A. Huertos
wiley   +1 more source

A Proposal for a Low‐Frequency Axion Search in the 1–2 μ$\umu$ eV Range and Below with the BabyIAXO Magnet

open access: yesAnnalen der Physik, Volume 535, Issue 12, December 2023., 2023
This article describes the implementation of low‐frequency axion haloscope setups inside the future BabyIAXO magnet. The RADES proposal has a potential sensitivity to the axion‐photon coupling down to values corresponding to the KSVZ model, in the mass range between 1 and 2 μ$\umu$eV.
Saiyd Ahyoune   +29 more
wiley   +1 more source

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