Supersymmetric Relics from the Big Bang
John R. Ellis, J.S. Hagelin (SLAC), Dimitri V. Nanopoulos, Keith A. Olive, M. Srednicki (CERN)

Jul 1983 - 24 pages

  • Nucl.Phys. B238 (1984) 453-476
    IN *BATAVIA 1984, PROCEEDINGS, INNER SPACE/OUTER SPACE*, 458-459.
    In *Srednicki, M.A. (ed.): Particle physics and cosmology* 223-246
  • (1984)
  • DOI: 10.1016/0550-3213(84)90461-9
  • SLAC-PUB-3171

Abstract (Elsevier)
We consider the cosmological constraints on supersymmetric theories with a new, stable particle. Circumstantial evidence points to a neutral gauge/Higgs fermion as the best candidate for this particle, and we derive bounds on the parameters in the lagrangian which govern its mass and couplings. One favored possibility is that the lightest neutral supersymmetric particle is predominantly a photino ∼ γ with mass above 1 2 GeV, while another is that the lightest neutral supersymmetric particle is a Higgs fermion with mass above 5 GeV or less than O(100) eV. We also point out that a gravitino mass of 10 to 100 GeV implies that the temperature after completion of an inflationary phase cannot be above 10 14 GeV, and probably not above 3 × 10 12 GeV. This imposes constraints on mechanisms for generating the baryon number of the universe.


PDG: Other bounds on chitilde(1)0 from astrophysics and cosmology
Keyword(s): INSPIRE: astrophysics | sparticle: mass | mass: sparticle | supergravity | fermion: Higgs particle | numerical calculations
 Record added 1983-07-01, last modified 2018-03-27