### 抄録

We analyze the observational constraints on brane-world cosmology whereby the universe is described as a three-brane embedded in a five-dimensional anti–de Sitter space. In this brane-universe cosmology, the Friedmann equation is modified by the appearance of extra terms which derive from the existence of the extra dimensions. In the present work we concentrate on the “dark radiation” term which diminishes with the cosmic scale factor as (Formula presented) We show that, although the observational constraints from primordial abundances allow only a small contribution when this term is positive, a much wider range of negative values is allowed. Furthermore, such a negative contribution can reconcile the tension between the observed primordial (Formula presented) and D abundances. We also discuss the possible constraints on this term from the power spectrum of CMB anisotropies in the limit of negligible cosmological perturbation on the brane world. We show that BBN limits the possible contribution from dark radiation just before the (Formula presented) annihilation epoch to lie between -123% and +11% of the background photon energy density. Combining this with the CMB constraint reduces this range to between -41% and +10.5% at the (Formula presented) confidence level.

元の言語 | 英語 |
---|---|

ページ数 | 1 |

ジャーナル | Physical Review D - Particles, Fields, Gravitation and Cosmology |

巻 | 66 |

発行部数 | 4 |

DOI | |

出版物ステータス | 出版済み - 1 1 2002 |

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### All Science Journal Classification (ASJC) codes

- Nuclear and High Energy Physics
- Physics and Astronomy (miscellaneous)

### これを引用

*Physical Review D - Particles, Fields, Gravitation and Cosmology*,

*66*(4). https://doi.org/10.1103/PhysRevD.66.043521

**Observational constraints on dark radiation in brane cosmology.** / Ichiki, K.; Yahiro, M.; Kajino, T.; Orito, M.; Mathews, G. J.

研究成果: ジャーナルへの寄稿 › 記事

*Physical Review D - Particles, Fields, Gravitation and Cosmology*, 巻. 66, 番号 4. https://doi.org/10.1103/PhysRevD.66.043521

}

TY - JOUR

T1 - Observational constraints on dark radiation in brane cosmology

AU - Ichiki, K.

AU - Yahiro, M.

AU - Kajino, T.

AU - Orito, M.

AU - Mathews, G. J.

PY - 2002/1/1

Y1 - 2002/1/1

N2 - We analyze the observational constraints on brane-world cosmology whereby the universe is described as a three-brane embedded in a five-dimensional anti–de Sitter space. In this brane-universe cosmology, the Friedmann equation is modified by the appearance of extra terms which derive from the existence of the extra dimensions. In the present work we concentrate on the “dark radiation” term which diminishes with the cosmic scale factor as (Formula presented) We show that, although the observational constraints from primordial abundances allow only a small contribution when this term is positive, a much wider range of negative values is allowed. Furthermore, such a negative contribution can reconcile the tension between the observed primordial (Formula presented) and D abundances. We also discuss the possible constraints on this term from the power spectrum of CMB anisotropies in the limit of negligible cosmological perturbation on the brane world. We show that BBN limits the possible contribution from dark radiation just before the (Formula presented) annihilation epoch to lie between -123% and +11% of the background photon energy density. Combining this with the CMB constraint reduces this range to between -41% and +10.5% at the (Formula presented) confidence level.

AB - We analyze the observational constraints on brane-world cosmology whereby the universe is described as a three-brane embedded in a five-dimensional anti–de Sitter space. In this brane-universe cosmology, the Friedmann equation is modified by the appearance of extra terms which derive from the existence of the extra dimensions. In the present work we concentrate on the “dark radiation” term which diminishes with the cosmic scale factor as (Formula presented) We show that, although the observational constraints from primordial abundances allow only a small contribution when this term is positive, a much wider range of negative values is allowed. Furthermore, such a negative contribution can reconcile the tension between the observed primordial (Formula presented) and D abundances. We also discuss the possible constraints on this term from the power spectrum of CMB anisotropies in the limit of negligible cosmological perturbation on the brane world. We show that BBN limits the possible contribution from dark radiation just before the (Formula presented) annihilation epoch to lie between -123% and +11% of the background photon energy density. Combining this with the CMB constraint reduces this range to between -41% and +10.5% at the (Formula presented) confidence level.

UR - http://www.scopus.com/inward/record.url?scp=85038335253&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85038335253&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.66.043521

DO - 10.1103/PhysRevD.66.043521

M3 - Article

AN - SCOPUS:85038335253

VL - 66

JO - Physical Review D - Particles, Fields, Gravitation and Cosmology

JF - Physical Review D - Particles, Fields, Gravitation and Cosmology

SN - 1550-7998

IS - 4

ER -