PT Journal
AU Barenboim, G
   Park, WI
TI New- vs. chaotic- inflations
SO Journal of Cosmology and Astroparticle Physics
JI J. Cosmol. Astropart. Phys.
PY 2016
BP 061
EP 20pp
VL 02
IS 2
DI 10.1088/1475-7516/2016/02/061
LA English
DE inflation; physics of the early universe; cosmology of theories beyond the SM
AB We show that "spiralized" models of new-inflation can be experimentally identified mostly by their positive spectral running in direct contrast with most chaotic-inflation models which have negative runnings typically in the range of O(10(-4)-10(-3)).
ER