Results 61 to 70 of about 13,537 (199)
Kilonova Emission and Heavy Element Nucleosynthesis
The binary neutron star merger observed and localized on 17 August 2017 by the LIGO and Virgo gravitational interferometers and by numerous telescopes on the ground and in orbit linked in an unambiguous way the coalescence of double neutron stars with ...
Elena Pian
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Nucleosynthesis in Thermonuclear Supernovae [PDF]
The explosion energy of thermonuclear (Type Ia) supernovae is derived from the difference in nuclear binding energy liberated in the explosive fusion of light 'fuel' nuclei, predominantly carbon and oxygen, into more tightly bound nuclear 'ash' dominated by iron and silicon group elements.
Seitenzahl, Ivo R., Townsley, Dean M.
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Properties and Composition of Magnetized Nuclei
The properties and mass distribution of the ultramagnetized atomic nuclei which arise in heavy-ion collisions and magnetar crusts, during Type II supernova explosions and neutron star mergers are analyzed.
V.N. Kondratyev
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Explosive nucleosynthesis: prospects [PDF]
15 pages, no figures, Elsevier Science volume honoring David N ...
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International audiencePrimordial nucleosynthesis, or big bang nucleosynthesis (BBN), is one of the three evidences for the big bang model, together with the expansion of the universe and the cosmic microwave background.
Alain Coc +3 more
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13 pages, including 4 figures, to appear in the Proceedings of the Workshop on ``Theoretical and Phenomenological Aspects of Underground Physics" (TAUP'95), Suppl. Nucl. Phys. B (M. Fatas, ed.)
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Precise Calculations of Nucleosynthesis Parameters and Electron Self-mass [PDF]
We study the effect of temperature on beta decay rate during primordial nucleosynthesis. Using thermal contributions to the renormalized mass of electron, we re-compute thermal effects to the nucleosynthesis parameters in the early universe in relation ...
Singh, Jaskeerat, Masood, Samina
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Structure effects of 20N in elemental abundance estimations during explosive nucleosynthesis [PDF]
Most nuclei far from the valley of stability, and typically near the drip lines, exhibit exotic features that have challenged our current understanding of nuclear structure.
Barman Jinti, Chatterjee Rajdeep
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To appear in the proceedings of the May 2003 STScI Symposium, ``The Local Group as an Astrophysical Laboratory''; 17 pages, 11 figures.
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15 pages, 1 (new) figure; mini-review in the Review of Particle Physics 2014 by the Particle Data Group (http://pdg.lbl.gov/)
Fields, B, Molaro, P, Sarkar, S
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