The evolution and explosion of massive stars

@article{Woosley1978TheEA,
  title={The evolution and explosion of massive stars},
  author={S. E. Woosley and Alexander Heger and Thomas A. Weaver},
  journal={Reviews of Modern Physics},
  year={1978},
  volume={74(4)},
  pages={1015-1071}
}
Like all true stars, massive stars are gravitationally confined thermonuclear reactors whose composition evolves as energy is lost to radiation and neutrinos. Unlike lower-mass stars (M≲8M⊙), however, no point is ever reached at which a massive star can be fully supported by electron degeneracy. Instead, the center evolves to ever higher temperatures, fusing ever heavier elements until a core of iron is produced. The collapse of this iron core to a neutron star releases an enormous amount of… 
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References

SHOWING 1-10 OF 76 REFERENCES
EVOLUTION AND EXPLOSION OF MASSIVE STARS *
amount of energy, a tiny fraction of which is sufficient to explode the star as a supernova. The authors examine our current understanding of the lives and deaths of massive stars, with special
The tidal disruption of neutron stars by black holes in close binaries.
The formation of close, doubly compact binary systems from close massive binaries is considered. Massive X-ray binaries are shown to be possible progenitors of these systems. The recent observation
Neutrino processes and pair formation in massive stars and supernovae.
Abstract : The paper traces the physical properties of matter inside highly evolved stars, on the assumption that the whole material of the star is non-degenerate and that the star is in
The hydrodynamics of type II supernovae.
Observations of Type II supernovae indicate the presence of a moderately cool expanding photosphere. This situation can result from an explosion in a star with an extended envelope. The evolutionary
Neutron-capture nucleosynthesis in the helium-burning cores of massive stars
We investigate the consequences for nucleosynthsis of the neutron release from the nuclear reaction /sup 22/Ne(..cap alpha..,n)/sup 25/ Mg when it occurs in the convective helium-burning cores of
Presupernova evolution of massive stars.
Population I stars of 15 M/sub sun/ and 25 M/sub sun/ have been evolved from the zero-age main sequence through iron core collapse utilizing a numerical model that incorporates both implicit
Neutrino-induced production of isotope11B in the carbon layer of a star
Neutrinos emitted by a collapsing stellar core are shown to interact effectively with the carbon layer of the stellar envelope, thereby producing a sufficiently large amount of isotope11B to account
Advanced evolution of massive stars. VII. Silicon burning
In this investigation the stages of ignition, flash, and consumption of silicon are studied for helium cores of mass M/sub b/6, 8, 12, 16, 24, and 32M/sub sun/Both hydrostatic and hydrodynamic
On the theory of the light curves of supernovae
An account of the theory of the light curves of supernovae is presented, based on certain assumptions concerning the passage through the stellar atmosphere of powerful shock waves. The investigation
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