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Title: Gravitinos as the cold dark matter in an. cap omega. = 1 universe

Technical Report ·
DOI:https://doi.org/10.2172/6259994· OSTI ID:6259994

In attempts to simultaneously have galaxy formation with adiabatic fluctuations, dark galactic halos and a critical ..cap omega.. = 1, recent models have been proposed with a heavy (cold) species which decays and a lighten (hot or warm) one which is stable. Surprisingly enough, these models are very constraining. Independent of the particle physics model, the decay width of the heavy particle must be 0(10/sup -40/) GeV. Such a scale is only natural in theories involving gravity where one expects GAMMA - M/sub H//sup 3//M/sub p//sup 2/, where M/sub H/ is the mass of the heavy particle and M/sub p/ is the planck mass. In this paper, we suggest that the heavy particle might be the gravitino which is present in all supergravity theories. This model would then require that the gravitino decay products not include photons, indicating that the lightest supersymmetric particle (LSP) must be something other than the photino. An acceptable candidate for the LSP might be the axino, the supersymmetric partner of the axion.

Research Organization:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
DOE Contract Number:
AC02-76CH03000
OSTI ID:
6259994
Report Number(s):
FNAL/Pub-84/120-A; ON: DE85003953
Resource Relation:
Other Information: Portions are illegible in microfiche products
Country of Publication:
United States
Language:
English

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