TY  - JOUR
AU  - Barenboim, G.
AU  - Park, W. I.
PY  - 2016
DA  - 2016//
TI  - New- vs. chaotic- inflations
T2  - J. Cosmol. Astropart. Phys.
JO  - Journal of Cosmology and Astroparticle Physics
SP  - 061
EP  - 20pp
VL  - 02
IS  - 2
PB  - Iop Publishing Ltd
KW  - inflation
KW  - physics of the early universe
KW  - 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)).
SN  - 1475-7516
UR  - https://arxiv.org/abs/1504.02080
UR  - https://doi.org/10.1088/1475-7516/2016/02/061
DO  - 10.1088/1475-7516/2016/02/061
LA  - English
N1  - WOS:000372467600062
ID  - Barenboim+Park2016
ER  -