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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.

DOI: 10.1063/1.881266

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.

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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    A. De Rüjula, D. Nanopoulous, P. Shaver, eds., A Unified View of the Micro‐ and Macro‐Cosmos, World Scientific, Singapore (1987);
    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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  10. 10. B. Cabrera, L. Krauss, F. Wilczek, Phys. Rev. Lett. 55, 25 (1984).https://doi.org/PRLTAO

  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
    D. Twerenbold, A. Zehnder, J. Appl. Phys. 61, 1 (1987).https://doi.org/JAPIAU

  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).

  21. 21. F. T. AvignoneIII et al., Phys. Lett. B 256, 559 (1991).https://doi.org/PYLBAJ

  22. 22. M. Bühler, E. Umlauf, Europhys. Lett. 5, 297 (1988).https://doi.org/EULEEJ

  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.

This Content Appeared In
pt-cover_1991_08.jpeg

Volume 44, Number 8

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