DC pole | Wartość | Język |
dc.contributor.author | Malec, Beata | - |
dc.contributor.author | Biesiada, Marek | - |
dc.date.accessioned | 2018-11-20T12:40:45Z | - |
dc.date.available | 2018-11-20T12:40:45Z | - |
dc.date.issued | 2001 | - |
dc.identifier.citation | Acta Physica Polonica. B, 2001, no. 11, s. 3683-3693 | pl_PL |
dc.identifier.issn | 0587-4254 | - |
dc.identifier.uri | http://hdl.handle.net/20.500.12128/7156 | - |
dc.description.abstract | In this paper we briefly review main ideas underlying the constraints
on exotic physics coming from Astrophysics already used by the others.
Next we present a new bound coming from the White Dwarf cooling. Such
stringent bound is possible due to accurate measurements offered by astroseismology.
Specifically we consider the G117-B15A pulsating white dwarf
(ZZ Ceti star) for which the speed of the period increase has been accurately
measured for its fundamental oscillation mode. It has been claimed
that this mode detected in G117-B15A is perhaps the most stable oscillation
ever recorded in the optical band. Then we review our result concerning the
bounds on compactification scale in the theory with large extra dimensions
according to Arkani-Hamed, Dimopoulos and Dvali. Because an additional
channel of energy loss (Kaluza-Klein gravitons) would speed up the cooling
rate, one is able to use the aforementioned stability to derive a bound on
compactification scale. We find the lower bound on compactification scale
to be Ms > 14.3 TeV/c2 which is more stringent than solar or red-giant
bounds, as well as the bound coming from LEP. In final section we point out
that pulsating hot “pre-White Dwarf” PG 1159-035 (GW Virginis) whose
oscillation period increases at the rate of the order of magnitude larger than
predicted could be a promising object for further investigations. | pl_PL |
dc.language.iso | en | pl_PL |
dc.rights | Uznanie autorstwa 3.0 Polska | * |
dc.rights.uri | http://creativecommons.org/licenses/by/3.0/pl/ | * |
dc.subject | exotic physics | pl_PL |
dc.subject | astrophysics | pl_PL |
dc.title | White dwarfs as a source of constraints on exotic physics | pl_PL |
dc.type | info:eu-repo/semantics/article | pl_PL |
dc.relation.journal | Acta Physica Polonica. B | pl_PL |
Pojawia się w kolekcji: | Artykuły (WNŚiT)
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