Published March 22, 1984
| Version v1
Journal article
Thermodynamics and the end of a closed Universe
Description
If the Universe is closed and began with low entropy, it began without an initial singularity in an unstable de Sitter phase. Because of the irreversible nature of the processes, when the closed Universe ultimately contracts it will not bounce, but will go into a 'final crunch'. In the final reheating, symmetry will be restored, but the contraction will never become deflationary. A closed Universe therefore lives only once, and can start with a whimper, but goes out with a bang. (author)
Additional details
Publishing Information
- Journal Title
- Nature (London)
- Journal Volume
- 308
- Journal Issue
- 5957
- Series
- Nature (London).
- Journal Page Range
- 319-322
- ISSN
- 0028-0836
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 15054750
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANALYTICAL SOLUTION; CONTRACTION; COSMIC RADIATION; COSMOLOGICAL MODELS; DE SITTER GROUP; ENTROPY; EXPANSION; GALACTIC EVOLUTION; SYMMETRY; THERMODYNAMICS; UNIVERSE
- Descriptors DEC
- IONIZING RADIATIONS; LIE GROUPS; MATHEMATICAL MODELS; PHYSICAL PROPERTIES; RADIATIONS; SYMMETRY GROUPS; THERMODYNAMIC PROPERTIES