Abstract
We investigate the final fate of spherical dust collapse by using the orthonormal frame formalism with the Hubble normalized variables and the separable volume gauge, which is usually used for analyzing cosmological dynamics. As a result, we find that the final fate of spherical dust collapse is characterized by the quantity concerned with the energy density in this formalism. We discuss the final fate of spherical perfect fluid collapse with a barotropic equation of state and conjecture a criterion for the final fate of spherical gravitational collapse.
Original language | English |
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Pages | 353-356 |
Number of pages | 4 |
Publication status | Published - 2007 |
Externally published | Yes |
Event | 17th Workshop on General Relativity and Gravitation in Japan, JGRG 2007 - Nagoya, Japan Duration: Dec 3 2007 → Dec 7 2007 |
Other
Other | 17th Workshop on General Relativity and Gravitation in Japan, JGRG 2007 |
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Country/Territory | Japan |
City | Nagoya |
Period | 12/3/07 → 12/7/07 |
All Science Journal Classification (ASJC) codes
- Atomic and Molecular Physics, and Optics