Final published version, 327 KB, PDF document
Available under license: CC BY
Final published version, 156 KB, PDF document
Available under license: CC BY
Final published version
Licence: CC BY: Creative Commons Attribution 4.0 International License
Research output: Contribution to Journal/Magazine › Journal article › peer-review
Research output: Contribution to Journal/Magazine › Journal article › peer-review
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TY - JOUR
T1 - Warm quintessential inflation
AU - Dimopoulos, Konstantinos
AU - Donaldson Wood, Leonora
PY - 2019/9/10
Y1 - 2019/9/10
N2 - We introduce warm quintessential inflation and study it in the weak dissipative regime. We consider the original quintessential inflation model, which approximates quartic chaotic inflation at early times and thawing quartic inverse-power-law quintessence at present. We find that the model successfully accounts for both inflation and dark energy observations, while it naturally reheats the Universe, thereby overcoming a major problem of quintessential inflation model-building.
AB - We introduce warm quintessential inflation and study it in the weak dissipative regime. We consider the original quintessential inflation model, which approximates quartic chaotic inflation at early times and thawing quartic inverse-power-law quintessence at present. We find that the model successfully accounts for both inflation and dark energy observations, while it naturally reheats the Universe, thereby overcoming a major problem of quintessential inflation model-building.
KW - cosmic inflation
KW - Quintessential Inflation
KW - Quintessence
KW - warm inflation
KW - cosmology
U2 - 10.1016/j.physletb.2019.07.017
DO - 10.1016/j.physletb.2019.07.017
M3 - Journal article
VL - 796
SP - 26
EP - 31
JO - Physics Letters B
JF - Physics Letters B
SN - 0370-2693
ER -