Properties of strange-matter stars
Conference
·
OSTI ID:10192550
- Univ., of Munich, Theresienstr. (Germany). Institute of Theoretical Physics
- Lawrence Berkeley Lab., CA (United States)
This paper deals with an investigation of the properties of hypothetical strange-matter stars, which are composed of u, d, s quark matter whose energy per baryon number lies below the one of {sup 56}Fe (Witten`s strange matter hypothesis). Observable quantities which allow to distinguish such objects from their ``conventional`` counterparts, neutron stars and white dwarfs, are pointed out.
- Research Organization:
- Lawrence Berkeley Lab., CA (United States)
- Sponsoring Organization:
- USDOE, Washington, DC (United States)
- DOE Contract Number:
- AC03-76SF00098
- OSTI ID:
- 10192550
- Report Number(s):
- LBL-35929; CONF-9407143-1; ON: DE95002329
- Resource Relation:
- Conference: International conference nuclei in the cosmos,Gran Sasso (Italy),8-13 Jul 1994; Other Information: PBD: Jul 1994
- Country of Publication:
- United States
- Language:
- English
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