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Warm quintessential inflation

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Warm quintessential inflation. / Dimopoulos, Konstantinos; Donaldson Wood, Leonora.

In: Physics Letters B, Vol. 796, 10.09.2019, p. 26-31.

Research output: Contribution to journalJournal articlepeer-review

Harvard

Dimopoulos, K & Donaldson Wood, L 2019, 'Warm quintessential inflation', Physics Letters B, vol. 796, pp. 26-31. https://doi.org/10.1016/j.physletb.2019.07.017

APA

Dimopoulos, K., & Donaldson Wood, L. (2019). Warm quintessential inflation. Physics Letters B, 796, 26-31. https://doi.org/10.1016/j.physletb.2019.07.017

Vancouver

Dimopoulos K, Donaldson Wood L. Warm quintessential inflation. Physics Letters B. 2019 Sep 10;796:26-31. https://doi.org/10.1016/j.physletb.2019.07.017

Author

Dimopoulos, Konstantinos ; Donaldson Wood, Leonora. / Warm quintessential inflation. In: Physics Letters B. 2019 ; Vol. 796. pp. 26-31.

Bibtex

@article{c97db34f4d074670bb558b5dc6983359,
title = "Warm quintessential inflation",
abstract = "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.",
keywords = "cosmic inflation, Quintessential Inflation, Quintessence, warm inflation, cosmology",
author = "Konstantinos Dimopoulos and {Donaldson Wood}, Leonora",
year = "2019",
month = sep,
day = "10",
doi = "10.1016/j.physletb.2019.07.017",
language = "English",
volume = "796",
pages = "26--31",
journal = "Physics Letters B",
issn = "0370-2693",
publisher = "ELSEVIER SCIENCE BV",

}

RIS

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 -