- Access by Xinjiang University
and as dark matter
Phys. Rev. D 40, 3187 – Published 15 November, 1989
DOI: https://doi.org/10.1103/PhysRevD.40.3187
Abstract
The singlet-Majoron model, with broken spontaneously at the GeV scale, allows in or with masses in the range of 1 keV to 35 MeV. Neutrino-Majoron scattering leads to an unusual processing of the density perturbation spectrum; the resulting large-scale structure will be very similar to warm or cold dark matter. The Higgs boson may decay predominantly into invisible channels giving signatures with a missing-mass peak.
References (21)
- J. Kormendy and G. R. Knapp, in Dark Matter in the Universe, proceedings of IAU Symposium No. 117, Princeton, New Jersey, 1985, edited by J. Kormendy and G. R. Knapp (Reidel, Boston, 1987)
- A. Guth, Phys. Rev. D 23, 347 (1981)
- A. GuthProceedings of the Workshop on Particle Astrophysics, Berkeley, 1988, edited by E. Norman (World Scientific, Singapore, 1989)
- R. V. Wagoner, W. A. Fowler, and F. Hoyle, Astrophys. J. 148, 3 (1967) J. Yang, M. Turner, G. Steigman, D. Schramm, and K. Olive, ibid. 281, 493 (1984)
- J. Applegate and C. Hogan, Phys. Rev. D 31, 3037 (1985)
- S. Dimopoulos, R. Esmailzadeh, L. Hall, and G. Starkman, Phys. Rev. Lett. 60, 7 (1988)
- R. Cowsik and J. McClelland, Phys. Rev. Lett. 29, 669 (1972)
- C. Frenk, S. White, and M. Davis, Astrophys. J. 271, 417 (1983) J. Centrella and A. Melott, Nature (London) 305, 196 (1983)
- S. Tremaine and J. E. Gunn, Phys. Rev. Lett. 42, 407 (1979)
- H. Georgi, S. L. Glashow, and S. Nussinov, Nucl. Phys. B193, 297 (1981)
- E. Kolb and M. Turner, Phys. Lett. 159B, 102 (1985)
- P. Pal, Phys. Rev. D 30, 2100 (1984)
- T. Yanagida, in Proceedings of the Workshop on Unified Theory and Baryon Number in the Universe, edited by O. Sawada and A. Sugamota (National Laboratory for High Energy Physics KEK, Tsukuba, Japan, 1979) M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity, proceedings of the Workshop, Stony Brook, 1979, edited by P. van Nieuwenhuizen and D. Z. Freedman (North-Holland, Amsterdam, 1980)
- G. Gelmini and R. Roncadelli, Phys. Lett. 99B, 411 (1981)
- Y. Chikashige, R. Mohapatra, and R. Peccei, Phys. Lett. 98B, 265 (1981)
- S. L. Glashow, Phys. Lett. B 187, 367 (1987)
- B. W. Lee and S. Weinberg, Phys. Rev. Lett. 39, 165 (1977)
- D. Dearborn, D. Schramm, and G. Steigman, Phys. Rev. Lett. 56, 26 (1986)
- A. Melott et al., Phys. Rev. Lett. 51, 935 (1983)
- Kamiokande II Collaboration, K. Hirota et al., Phys. Rev. Lett. 58, 1490 (1987) IMB III Collaboration, R. M. Bionta et al., ibid. 58, 1494 (1987)
- S. Burrows and J. M. Lattimer, Astrophys. J. 307, 178 (1986)