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U.S. Department of Energy
Office of Scientific and Technical Information

Natural inflation

Conference ·
OSTI ID:6046856
A pseduo-Nambu-Goldstone boson, with a potential of the form V({phi}) = {Lambda}{sup 4}(1 {plus minus} cos({phi}/f)), can naturally give rise to an epoch of inflation in the early universe. Successful inflation can be achieved if f {approximately} m{sub pl} and {Lambda} {approximately} m{sub GUT}. Such mass scales arise in particle physics models with a gauge group that becomes strongly interacting a the GUT scale, e.g., as is expected to happen in the hidden sector of superstring theories. The density fluctuation spectrum is a non-scale-invariant power law, with extra power on large scales. 12 refs., 3 figs.
Research Organization:
Fermi National Accelerator Lab., Batavia, IL (USA)
Sponsoring Organization:
DOE; USDOE, Washington, DC (USA)
DOE Contract Number:
AC02-76CH03000
OSTI ID:
6046856
Report Number(s):
FNAL/C-91/51-A; CONF-901141--2; ON: DE91009459
Country of Publication:
United States
Language:
English