Results 181 to 190 of about 767 (211)
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
G Martínez-Pinedo, A Arcones
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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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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 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 ...
Marco Limongi +2 more
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Explosive nucleosynthesis in ONeMg novae
Nuclear Physics A, 1997Abstract A quasi-analytic study on ONeMg novae is performed to examine explosive nucleosynthesis in wide range of white dwarf and envelope masses. Comparing our results with recent observations enables us to constrain those two parameters. About a half of observed ONeMg novae may have attained high envelope masses such as ∼10−4 M⊙, then obtained high
S. Wanajo +4 more
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Explosive Nucleosynthesis in Supernovae and Hypernovae
AIP Conference Proceedings, 2010We review the properties of supernovae (SNe) as a function of the progenitor’s mass M. (1) 8–10 M⊙ stars are super‐AGB stars and resultant electron capture SNe may be Faint supernovae like Type IIn SN 2008S. (2) 10–13 M⊙ stars undergo Fe‐core collapse to form neutron stars (NSs) and Faint supernovae. (3) 13 M⊙–MBN stars undergo Fe‐core collapse to form
Ken’ichi Nomoto +8 more
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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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Explosive Nucleosynthesis in the Galaxy
Nature Physical Science, 1971The hypothesis that most of the naturally occurring nuclei in the mass range 20≤A≤62 were produced by nuclear detonation in supernova explosions is examined in the context of different galactic histories.
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Supernova neutrinos and explosive nucleosynthesis
AIP Conference Proceedings, 2014Core-collapse supernovae eject huge amount of flux of energetic neutrinos. We studied the explosive nucleosyn-thesis in supernovae and found that several isotopes 7Li, 11B, 92Nb, 138La and 180Ta as well as r-process nuclei are affected by the neutrino interactions.
T. Kajino +9 more
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