Planetary heat flow limits on monopole and axion fluxes

dc.contributor.author	Sivaram, C
dc.date.accessioned	2008-12-29T14:43:00Z
dc.date.available	2008-12-29T14:43:00Z
dc.date.issued	1987-02
dc.identifier.citation	Earth, Moon, and Planets, Vol. 37, No. 2, pp. 155 - 159	en
dc.identifier.issn	0167-9295
dc.identifier.uri	http://hdl.handle.net/2248/4205
dc.description.abstract	Recent improvements in the quantitative estimates of the observed heat flow from planetary objects of the solar system may be used to put rather stringent limits on any background monopole flux. The axion flux from the giant planets is also estimated.	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Co.	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1987EM%26P...37..155S	en
dc.relation.uri	http://www.springerlink.com/content/4707188157n0h121/	en
dc.subject	Gas Giant Planets	en
dc.subject	Heat Flux	en
dc.subject	Magnetic Monopoles	en
dc.subject	Planetary Radiation	en
dc.subject	Grand Unified Theory	en
dc.subject	Nucleons	en
dc.subject	Radioactive Decay	en
dc.title	Planetary heat flow limits on monopole and axion fluxes	en
dc.type	Article	en