White dwarf stars as strange quark matter detectors

Autor:	O G Benvenuto
Rok vydání:	2005
Předmět:	Physics Nuclear and High Energy Physics Gravity (chemistry) Strange quark Range (particle radiation) White dwarf Astronomy Observable Astrophysics Core (optical fiber) Strange matter Quark star Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics
Zdroj:	Journal of Physics G: Nuclear and Particle Physics. 31:L13-L17
ISSN:	1361-6471 0954-3899
Popis:	We show that the presence of a strange matter core inside a white dwarf (WD) star produces a drastic change in the spectrum of non-radial oscillations in the range of periods corresponding to gravity modes. The distinctive, observable signal for such a core is a very short period spacing between consecutive modes, far shorter than in the case of pulsating WDs without any compact core.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::a5b44dc336cca00d85927d773185433a https://doi.org/10.1088/0954-3899/31/11/l01 Zobrazit plný text záznamu