Searching for the cosmion by scattering in Si detectors

D. O. Caldwell, B. Magnusson, M. S. Witherell, A. Da Silva, B. Sadoulet, C. Cork, F. S. Goulding, D. A. Landis, N. W. Madden, R. H. Pehl, A. R. Smith, G. Gerbier, E. Lesquoy, J. Rich, M. Spiro, C. Tao, D. Yvon, and S. Zylberajch
Phys. Rev. Lett. 65, 1305 – Published 10 September 1990
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Abstract

A new particle, the cosmion, has been proposed to be the dark matter of the Universe and to explain the solar ν deficit by cooling the solar core to reduce B8 ν production. Such cosmions in the galactic halo would scatter from nuclei in terrestrial detectors. Measurements were made in Si ionization detectors in a very-low-background environment down to energies of 1.1 keV. These results exclude nearly all of the mass range possible for cosmions with coherent nuclear interactions.

  • Received 5 June 1990

DOI:https://doi.org/10.1103/PhysRevLett.65.1305

©1990 American Physical Society

Authors & Affiliations

D. O. Caldwell, B. Magnusson, and M. S. Witherell

  • Department of Physics, University of California, Santa Barbara, Santa Barbara, California 93106

A. Da Silva and B. Sadoulet

  • Department of Physics, University of California, Berkeley, Berkeley, California 94720

C. Cork, F. S. Goulding, D. A. Landis, N. W. Madden, R. H. Pehl, and A. R. Smith

  • Lawrence Berkeley Laboratory, Berkeley, California 94720

G. Gerbier, E. Lesquoy, J. Rich, M. Spiro, C. Tao, D. Yvon, and S. Zylberajch

  • Département de Physique des Particules Elémentaires, Centre d’Etudes Nucléaires de Saclay, F-91191 Gif-sur-Yvette CEDEX, France

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Vol. 65, Iss. 11 — 10 September 1990

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