Negative exotic particles as low-temperature fusion catalysts and geochemical distribution

Details Negative exotic particles as low-temperature fusion catalysts and geochemical distribution Negative exotic particles as low-temperature fusion catalysts and geochemical distribution

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981natur.292...41j&link_type=abstract

Nature, Volume 292, Issue 5818, pp. 41-43 (1981).

Physics

5

Scientific paper

Minute concentrations of unfamiliar particles (X+ or X-) with atomic weights M between 102 and 106 (1011 and 1015 eV) may be remnants1-4 of the Big Bang or may originate in recent events (their expected properties are discussed elsewhere5). The adduct of X- with a Z-nucleus acts as a superheavy isotope of (Z-1). It is shown here that although their geochemical separation would be less obvious than that of fractionally charged species containing unsaturated quarks6,7 it should still be possible to concentrate these exotic isotopes. Exceptional cases are the neutral adducts pX and 2DX, which may form tiny molecules with a second proton, or a polymer with a density M × 1010 g cm-3 which could act as a low-temperature fusion catalyst and explain the excess heat irradiated by Jupiter.

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