Ultra high energy cosmic rays above 1011 GeV: Hints to new physics beyond Standard Model

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3320

Full metadata record

DC Field	Value	Language
dc.contributor.author	Bhattacharjee, P	-
dc.date.accessioned	2008-09-02T10:45:05Z	-
dc.date.available	2008-09-02T10:45:05Z	-
dc.date.issued	2000-08	-
dc.identifier.citation	Pramana Journal of Physics, Vol. 55, No. 1 – 2, pp. 297 - 305	en
dc.identifier.issn	0304-4289	-
dc.identifier.uri	http://hdl.handle.net/2248/3320	-
dc.description.abstract	The observed cosmic ray events above 10/Sup11 GeV are difficult to explain within the context of known physics of propagation of known particles in the Universe and within the standard acceleration mechanisms that are likely to operate in powerful astrophysical objects. Several ideas of possible new physics beyond the Standard Model have been suggested in order to explain these events. The major suggestions are summarized here.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://www.ias.ac.in/pramana/v55/p297/abs.htm	en
dc.subject	Ultra High Energy Cosmic Rays	en
dc.subject	Physics beyond Standard Model	en
dc.title	Ultra high energy cosmic rays above 1011 GeV: Hints to new physics beyond Standard Model	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

Files in This Item:

File	Description	Size	Format
Ultra high energy cosmic rays above 1011 GeV: Hints to new physics beyond Standard Model		89.16 kB	Adobe PDF	View/Open

DSpace JSPUI