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https://doi.org/10.1063/1.4732...
Article . 1995 . Peer-reviewed
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Article . 1994
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Properties of strange-matter stars

descriptionPublicationkeyboard_double_arrow_right Article , Other literature type 01 Jan 1995Publisher:AIPJournal:AIP Conference Proceedings, volume 327, pages 485-488 (issn: 0094-243X, Copyright policy )
Authors: Weber, F.; Kettner, Ch.; Glendenning, N. K.;

doi: 10.1063/1.47327

Properties of strange-matter stars

Abstract

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 56Fe (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.

Related Organizations
Keywords

General Physics, White Dwarf Stars 661300, Quark Matter, Strangeness, Neutron Stars, 71 Classical And Quantum Mechanics, Strange Particles, Stars, Pulsars, Other Aspects Of Physical Science

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
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Average
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