We discuss the role of strangeness in dense matter and especially in neutron stars. The early (in density) introduction of hyperons found in many calculations is probably delayed by the decrease in vector mean field acting on the neutron. This decrease results from both conventional many-body rescat
Quartetting in fermionic matter and -particle condensation in nuclear systems
✍ Scribed by P. Schuck; Y. Funaki; H. Horiuchi; G. Röpke; A. Tohsaki; T. Yamada
- Publisher
- Elsevier Science
- Year
- 2007
- Tongue
- English
- Weight
- 852 KB
- Volume
- 59
- Category
- Article
- ISSN
- 0146-6410
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✦ Synopsis
The onset of quartetting, i.e. α-particle condensation, in symmetric nuclear matter is studied with the help of an in-medium modified four nucleon equation. It is found that at very low density, quartetting wins over pairing because of the strong binding of the α particles. The critical temperature can reach values up to around 6 MeV. Also, the disappearance of α particles with increasing density, i.e. the Mott transition, is investigated. In finite nuclei the Hoyle state, that is, the 0 + 2 of 12 C is identified as an 'α-particle condensate' state. It is conjectured that such states also exist in heavier nα nuclei, such as 16 O, 20 Ne, etc. Exploratory calculations are performed for the density dependence of the α-condensate fraction at zero temperature to address the suppression of the four-particle condensate below nuclear-matter density. Possible quartet condensation in other systems is discussed briefly.
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