At the end of the life of a massive star, its iron core collapses under the unopposed attraction of gravity and initiates the supernova process. A violent explosion ensues and blows off the surface layers of the star, leaving behind a neutron star or a black hole. Both the nature of the collapse and
Supernovae as Nuclear and Particle Physics Laboratories
✍ Scribed by M. Liebendörfer; T. Fischer; M. Hempel; A. Mezzacappa; G. Pagliara; I. Sagert; J. Schaffner-Bielich; S. Scheidegger; F.-K. Thielemann; S.C. Whitehouse
- Publisher
- Elsevier Science
- Year
- 2009
- Tongue
- English
- Weight
- 185 KB
- Volume
- 827
- Category
- Article
- ISSN
- 0375-9474
No coin nor oath required. For personal study only.
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