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Models of quintessential inflation.

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Models of quintessential inflation. / Dimopoulos, Konstantinos.
International Workshop On Particle Physics And The Early Universe (COSMO-01). ed. / K. Enqvist. 2001.

Research output: Contribution in Book/Report/Proceedings - With ISBN/ISSN › Chapter

Harvard

Dimopoulos, K 2001, Models of quintessential inflation. in K Enqvist (ed.), International Workshop On Particle Physics And The Early Universe (COSMO-01).

APA

Dimopoulos, K. (2001). Models of quintessential inflation. In K. Enqvist (Ed.), International Workshop On Particle Physics And The Early Universe (COSMO-01)

Vancouver

Dimopoulos K. Models of quintessential inflation. In Enqvist K, editor, International Workshop On Particle Physics And The Early Universe (COSMO-01). 2001

Author

Dimopoulos, Konstantinos. / Models of quintessential inflation. International Workshop On Particle Physics And The Early Universe (COSMO-01). editor / K. Enqvist. 2001.

Bibtex

@inbook{b782851b0cc04bdbbaf36fc8c8a489de,
title = "Models of quintessential inflation.",
abstract = "A unified approach to quintessence and inflation is investigated with the use of a single scalar field. It is argued that successful potentials have to approximate a combination of exponential and inverse power-law decline in the limit of large values of the scalar field. A class of such potentials is studied analytically and it is found that quintessential inflation is indeed possible. Successful models, not involving more than two natural mass scales, are obtained, which do not require fine-tuning of initial conditions and do not result in eternal acceleration.",
author = "Konstantinos Dimopoulos",
note = "astro-ph/0111500",
year = "2001",
language = "English",
editor = "K. Enqvist",
booktitle = "International Workshop On Particle Physics And The Early Universe (COSMO-01)",

}

RIS

TY - CHAP

T1 - Models of quintessential inflation.

AU - Dimopoulos, Konstantinos

N1 - astro-ph/0111500

PY - 2001

Y1 - 2001

N2 - A unified approach to quintessence and inflation is investigated with the use of a single scalar field. It is argued that successful potentials have to approximate a combination of exponential and inverse power-law decline in the limit of large values of the scalar field. A class of such potentials is studied analytically and it is found that quintessential inflation is indeed possible. Successful models, not involving more than two natural mass scales, are obtained, which do not require fine-tuning of initial conditions and do not result in eternal acceleration.

AB - A unified approach to quintessence and inflation is investigated with the use of a single scalar field. It is argued that successful potentials have to approximate a combination of exponential and inverse power-law decline in the limit of large values of the scalar field. A class of such potentials is studied analytically and it is found that quintessential inflation is indeed possible. Successful models, not involving more than two natural mass scales, are obtained, which do not require fine-tuning of initial conditions and do not result in eternal acceleration.

M3 - Chapter

BT - International Workshop On Particle Physics And The Early Universe (COSMO-01)

A2 - Enqvist, K.

ER -