Cosmic tachyon background radiation

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3961

Full metadata record

DC Field	Value	Language
dc.contributor.author	Tomaschitz, R	-
dc.date.accessioned	2008-10-24T14:27:30Z	-
dc.date.available	2008-10-24T14:27:30Z	-
dc.date.issued	1999-10	-
dc.identifier.citation	International Journal of Modern Physics A, Vol. 14, No. 27, pp. 4275 - 4285	en
dc.identifier.issn	0217-75IX	-
dc.identifier.uri	http://hdl.handle.net/2248/3961	-
dc.description	Restricted Access	-
dc.description.abstract	The equilibrium statistical mechanics of a background radiation of superluminal particles is investigated, based on a vectorial wave equation for tachyons of the Proca type. The partition function, the spectral energy density, and the various thermodynamic variables of an ideal Bose gas of tachyons in an open Robertson-Walker cosmology are derived. The negative mass square in the wave equation changes the frequency scaling in the Rayleigh-Jeans law, and there are also significant changes in the low temperature regime as compared to the microwave background, in particular in the caloric and thermal equations of state.	en
dc.language.iso	en	en
dc.publisher	World Scientific Publishing	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1999IJMPA..14.4275T	en
dc.subject	Background Radiation: Cosmic	en
dc.title	Cosmic tachyon background radiation	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

Files in This Item:

File	Description	Size	Format
Cosmic tachyon background radiation.pdf	Restricted Access	346.93 kB	Adobe PDF	View/Open

DSpace JSPUI