Abstract
According to a number of suggestions, stable strange matter could exist in the form of supermassive nuclei (or 'strange nuggets')1,2. In contrast to ordinary nuclei, which contain only 'up' and 'down' quarks, a piece of strange matter should comprise a mixture of 'up', 'down' and 'strange' quarks in roughly equal proportions. Small amounts of strange matter could have survived from the early stages of the Universe1. Alternatively, strange matter might reach the Earth as a flux of strange nuggets produced in collisions of neutron stars3. Limits to the cosmic flux of strange nuggets with masses in the range from 10−4 to 250 g have been obtained in a search for light produced by the nuggets in the upper atmosphere4. Here we report the results of a search for supermassive nuclei by using Rutherford backscattering of heavy ions. The method is sensitive to a broad range of masses extending to those that exceed the projectile mass by several orders of magnitude. Upper limits for the abundance of strange nuggets with masses A ≈ 4 × 102 to 107 AMU relative to the number of nucleons were found to be in the range 10−10 to 10−14.
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Brügger, M., Lützenkirchen, K., Polikanov, S. et al. Search for strange matter by Rutherford backscattering. Nature 337, 434–436 (1989). https://doi.org/10.1038/337434a0
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DOI: https://doi.org/10.1038/337434a0
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