TY - JOUR
T1 - Reheating in small-field inflation on the brane
T2 - the swampland criteria and observational constraints in light of the PLANCK 2018 results
AU - Osses, Constanza
AU - VIDELA MENARES, NELSON MANUEL
AU - Panotopoulos, Grigoris
N1 - Funding Information:
We are grateful to the anonymous reviewer for a careful reading of the manuscript as well as for numerous useful comments and suggestions. C. O. is supported by CONICYT Chile, scholarship ANID-PFCHA/Doctorado Nacional/2018-21181476 and N. V. is supported by FONDECYT Grant 11170162. G. P. thanks the Fundação para a Ciência e Tecnologia (FCT), Portugal, for the financial support to the Center for Astrophysics and Gravitation-CENTRA, Instituto Superior Técnico, Universidade de Lisboa, through the Project No. UIDB/00099/2020.
Funding Information:
We are grateful to the anonymous reviewer for a careful reading of the manuscript as well as for numerous useful comments and suggestions. C. O. is supported by CONICYT Chile, scholarship ANID-PFCHA/Doctorado Nacional/2018-21181476 and N. V. is supported by FONDECYT Grant No 11170162. G. P. thanks the Funda??o para a Ci?ncia e Tecnologia (FCT), Portugal, for the financial support to the Center for Astrophysics and Gravitation-CENTRA, Instituto Superior T?cnico, Universidade de Lisboa, through the Project No. UIDB/00099/2020.
Publisher Copyright:
© 2021, The Author(s).
PY - 2021/6
Y1 - 2021/6
N2 - We study cosmological inflation and its dynamics in the framework of the Randall–Sundrum II brane model. In particular, we analyze in detail four representative small-field inflationary potentials, namely Natural inflation, Hilltop inflation, Higgs-like inflation, and Exponential SUSY inflation, each characterized by two mass scales. We constrain the parameters for which a viable inflationary Universe emerges using the latest PLANCK results. Furthermore, we investigate whether or not those models in brane cosmology are consistent with the recently proposed Swampland Criteria, and give predictions for the duration of reheating as well as for the reheating temperature after inflation. Our results show that (i) the distance conjecture is satisfied, (ii) the de Sitter conjecture and its refined version may be avoided, and (iii) the allowed range for the five-dimensional Planck mass, M5, is found to be 105TeV≲M5≲1012TeV. Our main findings indicate that non-thermal leptogenesis cannot work within the framework of RS-II brane cosmology, at least for the inflationary potentials considered here.
AB - We study cosmological inflation and its dynamics in the framework of the Randall–Sundrum II brane model. In particular, we analyze in detail four representative small-field inflationary potentials, namely Natural inflation, Hilltop inflation, Higgs-like inflation, and Exponential SUSY inflation, each characterized by two mass scales. We constrain the parameters for which a viable inflationary Universe emerges using the latest PLANCK results. Furthermore, we investigate whether or not those models in brane cosmology are consistent with the recently proposed Swampland Criteria, and give predictions for the duration of reheating as well as for the reheating temperature after inflation. Our results show that (i) the distance conjecture is satisfied, (ii) the de Sitter conjecture and its refined version may be avoided, and (iii) the allowed range for the five-dimensional Planck mass, M5, is found to be 105TeV≲M5≲1012TeV. Our main findings indicate that non-thermal leptogenesis cannot work within the framework of RS-II brane cosmology, at least for the inflationary potentials considered here.
UR - http://www.scopus.com/inward/record.url?scp=85107114122&partnerID=8YFLogxK
U2 - 10.1140/epjc/s10052-021-09283-6
DO - 10.1140/epjc/s10052-021-09283-6
M3 - Article
AN - SCOPUS:85107114122
VL - 81
JO - European Physical Journal C
JF - European Physical Journal C
SN - 1434-6044
IS - 6
M1 - 485
ER -