Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2000-09-18
Risk Anal. 24 (2004) 157-168
Physics
High Energy Physics
High Energy Physics - Phenomenology
Final version; to appear in "Risk Analysis"
Scientific paper
Recent papers by Busza et al. (BJSW) and Dar et al. (DDH) argue that astrophysical data can be used to establish small bounds on the risk of a ``killer strangelet'' catastrophe scenario in the RHIC and ALICE collider experiments. DDH and other commentators (initially including BJSW) suggested that these empirical bounds alone do give sufficient reassurance. This seems unsupportable when the bounds are expressed in terms of expected cost -- a good measure, according to standard risk analysis arguments. For example, DDH's main bound, $p_{\rm catastrophe} < 2 \times 10^{-8}$, implies only that the expectation value of the number of deaths is bounded by 120. This paper reappraises the DDH and BJSW risk bounds by comparing risk policy in other areas. For example, it is noted that, even if highly risk tolerant assumptions are made and no value is placed on the lives of future generations, a catastrophe risk no higher than $\approx 10^{-15}$ per year would be required for consistency with established policy for radiation hazard risk minimization. It is concluded that the costs of small risks of catastrophe have been significantly underestimated by BJSW (initially), by DDH and by other commentators. Lessons for future policy are proposed.
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