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Cosmological consequences of dilatons in the electroweak model

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Cosmological consequences of dilatons in the electroweak model. / McDonald, John.
In: Physics Letters B, Vol. 274, No. 1, 02.01.1992, p. 72-78.

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

Harvard

McDonald, J 1992, 'Cosmological consequences of dilatons in the electroweak model', Physics Letters B, vol. 274, no. 1, pp. 72-78. https://doi.org/10.1016/0370-2693(92)90306-O

APA

McDonald, J. (1992). Cosmological consequences of dilatons in the electroweak model. Physics Letters B, 274(1), 72-78. https://doi.org/10.1016/0370-2693(92)90306-O

Vancouver

McDonald J. Cosmological consequences of dilatons in the electroweak model. Physics Letters B. 1992 Jan 2;274(1):72-78. doi: 10.1016/0370-2693(92)90306-O

Author

McDonald, John. / Cosmological consequences of dilatons in the electroweak model. In: Physics Letters B. 1992 ; Vol. 274, No. 1. pp. 72-78.

Bibtex

@article{97f78214a24d470496d83764cca1d3e7,
title = "Cosmological consequences of dilatons in the electroweak model",
abstract = "We consider the cosmological evolution of an electroweak model with a Jordan-Brans-Dicke dilaton, as would result from spontaneously breaking scale-invariance in a complete theory. For the case where the Friedman-Robertson-Walker (FRW) metric is introduced in the Einstein frame, it is shown that the phase transition is first-order, in agreement with previous treatments of this question. It is however argued that the treatment given here is more physically correct than previous treatments. It is also shown that at the electroweak phase transition, which occurs at the temperature of chiral symmetry breaking, most of the vacuum energy goes into oscillations of the dilaton field, with essentially no reheating or increase in entropy. As a result, the universe becomes effectively matter dominated before nucleosynthesis, ruling out the model. The only way to avoid this problem is to have scale-invariance broken at less than O(10(7)) GeV. For the case where the FRW metric is introduced in the Jordan frame, the electroweak phase transition is of second-order as for the minimal standard model. The question of the energy density in dilatons is dependent upon the assumed form of the dilaton potential.",
keywords = "INFLATION",
author = "John McDonald",
year = "1992",
month = jan,
day = "2",
doi = "10.1016/0370-2693(92)90306-O",
language = "English",
volume = "274",
pages = "72--78",
journal = "Physics Letters B",
issn = "0370-2693",
publisher = "ELSEVIER SCIENCE BV",
number = "1",

}

RIS

TY - JOUR

T1 - Cosmological consequences of dilatons in the electroweak model

AU - McDonald, John

PY - 1992/1/2

Y1 - 1992/1/2

N2 - We consider the cosmological evolution of an electroweak model with a Jordan-Brans-Dicke dilaton, as would result from spontaneously breaking scale-invariance in a complete theory. For the case where the Friedman-Robertson-Walker (FRW) metric is introduced in the Einstein frame, it is shown that the phase transition is first-order, in agreement with previous treatments of this question. It is however argued that the treatment given here is more physically correct than previous treatments. It is also shown that at the electroweak phase transition, which occurs at the temperature of chiral symmetry breaking, most of the vacuum energy goes into oscillations of the dilaton field, with essentially no reheating or increase in entropy. As a result, the universe becomes effectively matter dominated before nucleosynthesis, ruling out the model. The only way to avoid this problem is to have scale-invariance broken at less than O(10(7)) GeV. For the case where the FRW metric is introduced in the Jordan frame, the electroweak phase transition is of second-order as for the minimal standard model. The question of the energy density in dilatons is dependent upon the assumed form of the dilaton potential.

AB - We consider the cosmological evolution of an electroweak model with a Jordan-Brans-Dicke dilaton, as would result from spontaneously breaking scale-invariance in a complete theory. For the case where the Friedman-Robertson-Walker (FRW) metric is introduced in the Einstein frame, it is shown that the phase transition is first-order, in agreement with previous treatments of this question. It is however argued that the treatment given here is more physically correct than previous treatments. It is also shown that at the electroweak phase transition, which occurs at the temperature of chiral symmetry breaking, most of the vacuum energy goes into oscillations of the dilaton field, with essentially no reheating or increase in entropy. As a result, the universe becomes effectively matter dominated before nucleosynthesis, ruling out the model. The only way to avoid this problem is to have scale-invariance broken at less than O(10(7)) GeV. For the case where the FRW metric is introduced in the Jordan frame, the electroweak phase transition is of second-order as for the minimal standard model. The question of the energy density in dilatons is dependent upon the assumed form of the dilaton potential.

KW - INFLATION

U2 - 10.1016/0370-2693(92)90306-O

DO - 10.1016/0370-2693(92)90306-O

M3 - Journal article

VL - 274

SP - 72

EP - 78

JO - Physics Letters B

JF - Physics Letters B

SN - 0370-2693

IS - 1

ER -