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Jointly modelling Cosmic Inflation and Dark Energy

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Jointly modelling Cosmic Inflation and Dark Energy. / Dimopoulos, Konstantinos.
In: Journal of Physics: Conference Series, Vol. 2105, 012001, 26.11.2021.

Research output: Contribution to Journal/Magazine › Conference article › peer-review

Harvard

Dimopoulos, K 2021, 'Jointly modelling Cosmic Inflation and Dark Energy', Journal of Physics: Conference Series, vol. 2105, 012001. https://doi.org/10.1088/1742-6596/2105/1/012001

APA

Dimopoulos, K. (2021). Jointly modelling Cosmic Inflation and Dark Energy. Journal of Physics: Conference Series, 2105, Article 012001. https://doi.org/10.1088/1742-6596/2105/1/012001

Vancouver

Dimopoulos K. Jointly modelling Cosmic Inflation and Dark Energy. Journal of Physics: Conference Series. 2021 Nov 26;2105:012001. doi: 10.1088/1742-6596/2105/1/012001

Author

Dimopoulos, Konstantinos. / Jointly modelling Cosmic Inflation and Dark Energy. In: Journal of Physics: Conference Series. 2021 ; Vol. 2105.

Bibtex

@article{deddac6cd2074506816cd8b7c9db2623,
title = "Jointly modelling Cosmic Inflation and Dark Energy",
abstract = "Quintessential inflation utilises a single scalar field to account for the observations of both cosmic inflation and dark energy. The requirements for modelling quintessential inflation are described and two explicit successful models are presented in the context of α-attractors and Palatini modified gravity. ",
keywords = "cosmic inflation, Quintessential Inflation, modified gravity, dark energy, Cosmology",
author = "Konstantinos Dimopoulos",
year = "2021",
month = nov,
day = "26",
doi = "10.1088/1742-6596/2105/1/012001",
language = "English",
volume = "2105",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",

}

RIS

TY - JOUR

T1 - Jointly modelling Cosmic Inflation and Dark Energy

AU - Dimopoulos, Konstantinos

PY - 2021/11/26

Y1 - 2021/11/26

N2 - Quintessential inflation utilises a single scalar field to account for the observations of both cosmic inflation and dark energy. The requirements for modelling quintessential inflation are described and two explicit successful models are presented in the context of α-attractors and Palatini modified gravity.

AB - Quintessential inflation utilises a single scalar field to account for the observations of both cosmic inflation and dark energy. The requirements for modelling quintessential inflation are described and two explicit successful models are presented in the context of α-attractors and Palatini modified gravity.

KW - cosmic inflation

KW - Quintessential Inflation

KW - modified gravity

KW - dark energy

KW - Cosmology

U2 - 10.1088/1742-6596/2105/1/012001

DO - 10.1088/1742-6596/2105/1/012001

M3 - Conference article

VL - 2105

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

M1 - 012001

ER -