Skip navigation

Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12128/7207
Title: White dwarf constraints on dark matter particles
Authors: Malec, Beata
Biesiada, Marek
Keywords: ciemna materia; widma gwiazd; astrofizyka; Biały karzeł
Issue Date: 2009
Citation: Acta Physica Polonica B, Vol. 40, no. 11 (2009), s. 3165-3169
Abstract: Matter budget in the Universe together with primordial nucleosynthesis bounds on baryonic density suggests that dark matter in galaxies should have non-baryonic nature. On the other hand, considerable agreement of a variety of astrophysical observations with standard physics can serve as a source of constraints on non-standard ideas. In this context we consider G117-B15A pulsating white dwarf for which the rate of period change of its fundamental mode has been accurately measured. This star has been claimed the most stable oscillator ever recorded in the optical band. Here we use this object to derive a bound on theories with large extra dimensions as well as to constrain supersymmetric dark matter.
URI: http://hdl.handle.net/20.500.12128/7207
ISSN: 0587-4254
Appears in Collections:Artykuły (WNŚiT)

Files in This Item:
File Description SizeFormat 
Malec_White_dwarf_constraints.pdf477,92 kBAdobe PDFView/Open
Show full item record


Uznanie Autorstwa 3.0 Polska Creative Commons License Creative Commons