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Neutrino and Dark‐Matter Detection at Low Temperature

AUG 01, 1991
The use of low‐temperature techniques to see tiny energies in massive detectors may be opening a ‘low energy’ frontier of particle physics.
Leo Stodolsky

It is with shock, and with new respect for the subtleties of condensed matter physics, that the noninitiate (such as I was) first realizes that at low temperatures a microscopic energy—like that associated with a single atom—can be enough to seriously affect the state of a macroscopic body.

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References

  1. 1. The theme of this article was the topic of three workshops, whose proceedings contain extensive discussions and references: K. Pretzl, N. Schmitz, L. Stodolsky, eds., Proc. Wksp. On Low Temperature Detectors for Neutrinos and Dark Matter, Springer‐Verlag, New York (1987);
    L. Gonzalez‐Mestres, D. Perret‐Gallix, Proc. Wksp. on Low Temperature Detectors for Neutrinos and Dark Matter II, Editions Frontières, Gif‐sur‐Yvette, France (1988);
    L. Brogiato, D. V. Camin, E. Fiorini, eds., Proc. Wksp. on Low Temperature Detectors for Neutrinos and Dark Matter III, Editions Frontières, Gif‐sur‐Yvette, France (1990).

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  7. 7. For some references on dark matter, see V. Trimble, Annu. Rev. Astron. Astrophys. 25, 425 (1987); https://doi.org/ARAAAJ
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    M. Turner, “Dark Matter in the Universe,” Proc. Nobel Symp. 79, Nobel Committee, Stockholm.

  8. 8. See the review by J. Primack, D. Seckel, B. Sadoulet, Annu. Rev. Nucl. Part. Sci. 38, 751 (1989).https://doi.org/ARPSDF

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  11. 11. S. P. Ahlen, F. T. AvignoneIII, R. L. Brodzinski, A. K. Drukier, G. Gelmini, D. N. Spergel, Phys. Lett. B 195, 603 (1987). https://doi.org/PYLBAJ
    For silicon detectors, see D. O. Caldwell et al., Phys. Rev. Lett. 65, 1305 (1990).https://doi.org/PRLTAO

  12. 12. For early work on superconducting grains, see A. K. Drukier, C. Valette, Nucl. Instrum. Methods 105, 285 (1972); https://doi.org/NUIMAL
    D. Hueber, C. Valette, G. Waysand, Nucl. Instrum. Methods 167, 201 (1979). https://doi.org/NUIMAL
    For recent work see the workshops in ref. 1. For studies of single grains, see M. Frank, P. Freund, J. Gebauer, K. Pretzl, A. Singsaas, L.. Stodolsky, Nucl. Instrum. Methods A 287, 583 (1990); https://doi.org/NIMAER
    M. Frank, P. Freund, J. Gebauer, K. Pretzl, A. Singsaas, L.. Stodolsky, Phys. Lett. B 230, 159 (1989).https://doi.org/PYLBAJ

  13. 13. W. Seidel, G. Forster, W. Christen, F. von Feilitzsch, H. Göbel, F. Pröbst, R. L. Mössbauer, Phys. Lett. B 236, 483 (1990).https://doi.org/PYLBAJ

  14. 14. D. McCammon, in workshop III of ref. 1, p. 213, and private communication.

  15. 15. A. Alessandrello, D. V. Camin, E. Fiorini, A. Giuliani, Phys. Lett. B 202, 611 (1988).https://doi.org/PYLBAJ

  16. 16. For He 3, see G. R. Pickett, in workshop II of ref. 1, p. 377B.

  17. 17. D. J. Goldie, N. E. Booth, C. Patel, G. L. Salmon, Phys. Rev. Lett. 64, 954 (1990). https://doi.org/PRLTAO
    T. Peterreins, F. Pröbst, F. von Feilitzsch, R. L. Mössbauer, H. Kraus, Phys. Lett. B 202, 161 (1988). https://doi.org/PYLBAJ
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  18. 18. B. A. Young, B. Cabrera, A. T. Lee, Phys. Rev. Lett. 64, 2795 (1990).https://doi.org/PRLTAO

  19. 19. R. E. Lanou, H. J. Maris, G. M. Seidel, Phys. Rev. Lett. 58, 2498 (1987). https://doi.org/PRLTAO
    H. Kinder, in workshop III of ref. 1, p. 305.

  20. 20. A. Cummings et al., “Performance of a 60 Gram Cryogenic Detector,” Center for Particle Astrophysics, U. Calif., Berkeley (1990).

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  23. 23. For a survey of these issues, see L. Stodolsky, A. Bottino, P. Monacelli, eds., TAUP ‘89, Editions Frontières, Gif‐sur‐Yvette, France (1989), p. 2.

More about the Authors

Leo Stodolsky. Max Planck Institute for Physics, Munich, Germany.

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Volume 44, Number 8

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