Cosmological constraints on bulk neutrinos

被引：18

作者：

Abazajian, KN ^{[1
]}

Fuller, GM

Patel, M

机构：

[1] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA

[2] Fermilab Natl Accelerator Lab, NASA Fermilab Astrophys Ctr, Batavia, IL 60510 USA

来源：

PHYSICAL REVIEW LETTERS | 2003年 / 90卷 / 06期

关键词：

D O I：

10.1103/PhysRevLett.90.061301

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Recent models invoking extra spacelike dimensions inhabited by (bulk) neutrinos are shown to have significant cosmological effects if the size of the largest extra dimension is R greater than or similar to 1 fm. We consider effects on cosmic microwave background anisotropies, big bang nucleosynthesis, deuterium and Li-6 photoproduction, diffuse photon backgrounds, and structure formation. The resulting constraints can be stronger than either bulk graviton overproduction constraints or laboratory constraints.

引用

页码：4 / 061301

页数：4

共 50 条

[41] NEUTRINO MASS AND SPONTANEOUS PARITY NON-CONSERVATION [J].

MOHAPATRA, RN ;

SENJANOVIC, G .

PHYSICAL REVIEW LETTERS, 1980, 44 (14) :912-915

[42] Three flavour neutrino oscillations in models with large extra dimensions [J].

Mohapatra, RN ;

Pérez-Lorenzana, A .

NUCLEAR PHYSICS B, 2001, 593 (03) :451-470

[43] Inflation in models with large extra dimension driven by a bulk scaler field -: art. no. 105030 [J].

Mohapatra, RN ;

Pérez-Lorenzana, A ;

Pires, CAD .

PHYSICAL REVIEW D, 2000, 62 (10) :1-6

[44] NEUTRINO DISPERSION AT FINITE TEMPERATURE AND DENSITY [J].

NOTZOLD, D ;

RAFFELT, G .

NUCLEAR PHYSICS B, 1988, 307 (04) :924-936

[45]

Primack J.R., ASTROPH0007165

[46]

Ressell M.T., 1990, Comments on Astrophysics, V14, P323

[47] TREATMENT OF NEUTRINO OSCILLATIONS IN A THERMAL ENVIRONMENT [J].

STODOLSKY, L .

PHYSICAL REVIEW D, 1987, 36 (08) :2273-2277

[48] Is cosmology consistent? [J].

Wang, XM ;

Tegmark, M ;

Zaldarriaga, M .

PHYSICAL REVIEW D, 2002, 65 (12)

[49]

WITTEN E, HEPPH0002297

[50]

YANAGIDA T, 1979, P WORKSH UN THEOR BA

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