Hafnium controversy

The hafnium controversy is a debate over the possibility of 'triggering' rapid energy releases, via gamma ray emission, from a nuclear isomer of hafnium, 178m2Hf. The energy release is potentially 5 orders of magnitude (105 times) more energetic than a chemical reaction, but 3 orders of magnitude less than a nuclear reaction. In 1998, a group led by Carl Collins of the University of Texas at Dallas reported[1][2] having successfully initiated such a trigger. Signal-to-noise ratios were small in those first experiments, and to date no other group has been able to duplicate these results. Peter Zimmerman described claims of weaponization potential as having been based on "very bad science".[3]

Background

178m2Hf is a particularly attractive candidate for induced gamma emission (IGE) experiments, because of its high density of stored energy, 2.5 MeV per nucleus, and long 31-year half life for storing that energy. If radiation from some agent could "trigger" a release of that stored energy, the resulting cascade of gamma photons would have the best chance of finding a pair of excited states with the inverted lifetimes needed for stimulated emission. While induced emission adds only power to a radiation field, stimulated emission adds coherence. The possibility to manipulate gamma ray coherence, even to a small degree, would be interesting.[4] The lifetime of the hafnium isomer is long enough for tractable amounts of material to be collected into experimental targets. Such samples would hold no hazards for personnel working with the material; 1 microgram of 178m2Hf has an activity of 1.5 megabecquerels (41 microcuries).

A proposal to test the efficacy for "triggering" 178m2Hf was approved by a NATO-Advanced Research Workshop (NATO-ARW) held in Predeal in 1995.[5] Although the proposal was to use incident protons to bombard the target, α-particles were available when the first experiment was scheduled. It was done by a French, Russian, Romanian and American team. Results were said [6] to be extraordinary, but the results were not published. Nevertheless, 178m2Hf was implied to be of special importance to potential applications of IGE. A controversy quickly erupted.

Importance

Chronology of notable events

Experiment producing IGE from a sample of the nuclear isomer 178m2Hf. (left to right) Students on duty; (w/ladder) the world's most stable beamline for monochromatic X-rays, BL01B1; (rt.) main ring of the SPring-8 synchrotron at Hyogo.

References

  1. Collins, C.B., Davanloo, F., Iosif, M.; et al. (1999). "Accelerated Emission of Gamma Rays from the 31-yr Isomer of 178Hf Induced by X-Ray Irradiation". Physical Review Letters. 82 (4): 695–698. Bibcode:1999PhRvL..82..695C. doi:10.1103/PhysRevLett.82.695.
  2. Collins, C.B., Davanloo, F., Rusu, A.C.; et al. (2000). "Gamma emission from the 31-yr isomer of 178Hf induced by x-ray irradiation". Physical Review C. 61: 054305–054305–7. Bibcode:2000PhRvC..61e4305C. doi:10.1103/PhysRevC.61.054305.
  3. Peter Zimmerman (June 2007). "The Strange Tale of the Hafnium Bomb: A Personal Narrative". American Physical Society. Retrieved 5 March 2016.
  4. Dietrick E. Thomsen Pumping up hope for gamma ray laser, Science News, Nov 1, 1986
  5. Proceedings of the NATO-ARW are collected in Hyperfine Interactions, 107, pp 3–492 (1997).
  6. Link to review of "Isomer Triggering history from one participant.
  7. N. Lewis; R. Garwin; D. Hammer; W. Happer; R. Jeanloz. J. Katz; S. Koonin; P. Weinberger; E. Williams (October 1997). High Energy Density Explosives (PDF). JSR-97-110. Sect. 4, p. 13.
  8. S. Weinberger (28 March 2004). "Scary things come in small packages". Sunday Supplement Magazine. Washington Post. Retrieved 2009-05-03.
  9. Bertram Schwarzschild (May 2004). "Conflicting Results on a Long-Lived Nuclear Isomer of Hafnium Have Wider Implications". Physics Today. 57: 21–24. Bibcode:2004PhT....57e..21S. doi:10.1063/1.1768663.
  10. San Jose newspaper article., October, 2003.
  11. C. Rusu (PhD Dissertation, U of Texas at Dallas, 2002)Available from: Proquest (Order Number: 3087127).
  12. 1 2 Publications by Center for Quantum Electronics, University of Texas at Dallas Retrieved on 2010-12-12.
  13. C.B. Collins, N.C. Zoita, F. Davanloo, Y. Yoda, T. Uruga, J.M.Pouvesle, and I.I. Popescu (2005). "Nuclear resonance spectroscopy of the 31-yr isomer of Hf-178". Laser Physics Letters. 2 (3): 162–167. Bibcode:2005LaPhL...2..162C. doi:10.1002/lapl.200410154.
  14. Ahmad, I.; et al. (2001). "Search for X-Ray Induced Acceleration of the Decay of the 31-Yr Isomer of 178Hf Using Synchrotron Radiation". Physical Review Letters. 87 (7): 072503. Bibcode:2001PhRvL..87g2503A. doi:10.1103/PhysRevLett.87.072503. PMID 11497887.
  15. Ahmad, I.; et al. (2003). "Search for x-ray induced decay of the 31-yr isomer of 178Hf at low x-ray energies". Physical Review C. 67 (4): 041305R. Bibcode:2003PhRvC..67d1305A. doi:10.1103/PhysRevC.67.041305.
  16. Tkalya, Eugene V. (2003). "Probability of L-shell nuclear excitation by electronic transitions in 178Hfm2". Physical Review C. 68 (6): 064611. Bibcode:2003PhRvC..68f4611T. doi:10.1103/PhysRevC.68.064611.
  17. Tkalya, Eugene V. (2005). "Induced decay of 178Hfm2: Theoretical analysis of experimental results". Physical Review C. 71 (2): 024606. Bibcode:2005PhRvC..71b4606T. doi:10.1103/PhysRevC.71.024606.
  18. Tkalya, Evgenii V (2005). "Induced decay of the nuclear isomer 178m2Hf and the 'isomeric bomb'". Physics-Uspekhi. 48 (5): 525–531. Bibcode:2005PhyU...48..525T. doi:10.1070/PU2005v048n05ABEH002190. [Uspekhi Fiz. Nauk 175, 555 (2005)].
  19. Pereira; et al. (2007). "Economics of isomeric energy". Laser Physics. 17: 874–879. Bibcode:2007LaPhy..17..874P. doi:10.1134/S1054660X0706014X.
  20. Hartouni, E.P, et al., "Theoretical Assessment of 178Hfm2 De-excitation, LLNL Report TR-407631, October 9, 2008, p.33. https://e-reports-ext.llnl.gov/pdf/366265.pdf
  21. Karamian, S. E.; et al. (2009). "Spallation and fission products in the (p+179Hf) and (p+natHf) reactions". Nuclear Instruments and Methods in Physics Research A. 600: 488–497. Bibcode:2009NIMPA.600..488K. doi:10.1016/j.nima.2008.12.001.

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