Results 171 to 180 of about 112,099 (203)
Solar abundance of osmium. [PDF]
Proc Natl Acad Sci U S A, 1976 Jacoby G, Aller LH.
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Explosive Processes in Nucleosynthesis
European Physical Journal A, 2002 There are many explosive processes in nucleosynthesis: big bang nucleosynthesis, the rp-process, the $\gamma$-process, the $\nu$-process, and the r-process.
R N Boyd
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Explosive Nucleosynthesis: Prospects [PDF]
Physics Reports, 2000 15 pages, no figures, Elsevier Science volume honoring David N ...
David Arnett
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Neutrinos and Explosive Nucleosynthesis
Progress in Particle and Nuclear Physics, 2010Abstract Core-collapse supernovae produce a hot protoneutron star that cools emitting huge amounts of neutrinos of all flavors. The interaction of these neutrinos with the outer layers of the protoneutron star produces an outflow of matter whose composition is determined by the luminosities and energies of the emitted neutrinos and antineutrinos. The
Gabriel MartÃnez-Pinedo +1 more
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Explosive Nucleosynthesis in Hypernovae [PDF]
Astrophysical Journal, 2001 Accepted for publication in the Astrophysical Journal (13 March 2001) Tables 6 - 9 are available at http://www.astron.s.u-tokyo.ac.jp/~nakamura/research/papers/nakamuratab.ps ...
UMEDA Hideyuki +2 more
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Explosive Nucleosynthesis in Stars
Nature, 1970Recent calculations provide convincing evidence that the naturally occurring nuclei were produced in explosions. The required temperature, density and expansion rate strongly suggest that before the explosion the objects were ordinary evolved massive stars.
W D, Arnett, D D, Clayton
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Explosive Nucleosynthesis in Massive Stars
AIP Conference Proceedings, 2010In this short paper we will review the basic properties of the explosive nucleosynthesis in massive stars. In particular we will describe how the the basic properties of an expanding adiabatic shock wave, coupled to the behavior of the matter at various high temperatures to the presupernova evolution of a massive star, contribute to produce its final ...
Tatsushi Shima +2 more
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Gamma-Ray Observations of Explosive Nucleosynthesis Products [PDF]
Advances in Space Research, 2005 Invited review given at the 35th COSPAR Scientific Assembly, Paris, July 18-25 2004, session E1.4 (joint session with E1.5) 'Young Neutron Stars and Supernova Remnants' edited by C. Rakowski and S. Chatterjee.
Jacco Vink
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Explosive Nucleosynthesis in Stars
1980As seen from Chapter II, the evolution of the stars depends essentially on their masses: low mass stars evolve into white dwarfs at the very end of the planetary nebulae phase (Figure V.1) while high mass ones become neutron stars after having exploded at their supernovae stage (Figure V.2), or black holes.
Jean Audouze, Sylvie Vauclair
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