Planetary heat flow limits on monopole and axion fluxes

Details Planetary heat flow limits on monopole and axion fluxes Planetary heat flow limits on monopole and axion fluxes

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987em%26p...37..155s&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 37, Feb. 1987, p. 155-159.

Physics

4

Gas Giant Planets, Heat Flux, Magnetic Monopoles, Planetary Radiation, Grand Unified Theory, Nucleons, Radioactive Decay

Scientific paper

Recent improved quantitative estimates of the observed heat flow from planetary objects in the solar system are used to set a limit on the background monopole flux (less than 10 to the -19th/sq cm per s per sr) which is two orders more stringent than the Parker bound. Axion flux estimations from the giant planets are also given. A solar axion flux on earth of 10 to the 14th/s per sq cm (10 to the 8th GeV/V) squared, with solar axion energies in the soft X-ray range, and an axion flux on earth from Jupiter of 10 to the 6th/s per sq cm (10 to the 8th GeV/V) squared, with axion energies centered about 10 eV, are derived.

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