BBN and CMB constraints on universal lepton asymmetry, quintessential inflation, and brane world cosmology

M. Orito; T. Kajino; K. Ichiki; M. Yahiro; G. J. Mathews; Y. Wang

doi:10.1016/S0375-9474(03)00950-3

BBN and CMB constraints on universal lepton asymmetry, quintessential inflation, and brane world cosmology

M. Orito, T. Kajino, K. Ichiki, M. Yahiro, G. J. Mathews, Y. Wang

Experimental Particle Physics

Research output: Contribution to journal › Article › peer-review

1 Citation (Scopus)

Abstract

Recent progress in cosmological deep survey has clarified progressively the origin and distribution of matter and evolution of Galaxies in the Universe. The origin of the light elements in the Big-Bang nucleosynthesis (BBN) has been a topic of broad interest for its significance in constraining the dark matter component in the Universe, and also in seeking for the cosmological model which best fits the recent data of cosmic microwave background (CMB) fluctuations.

Original language	English
Pages (from-to)	C1-C8
Journal	Nuclear Physics A
Volume	719
Issue number	1-4
DOIs	https://doi.org/10.1016/S0375-9474(03)00950-3
Publication status	Published - May 19 2003

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics

Access to Document

10.1016/S0375-9474(03)00950-3

Cite this

@article{fa368fdaf9df4e098dbf7d45f8aed7eb,

title = "BBN and CMB constraints on universal lepton asymmetry, quintessential inflation, and brane world cosmology",

abstract = "Recent progress in cosmological deep survey has clarified progressively the origin and distribution of matter and evolution of Galaxies in the Universe. The origin of the light elements in the Big-Bang nucleosynthesis (BBN) has been a topic of broad interest for its significance in constraining the dark matter component in the Universe, and also in seeking for the cosmological model which best fits the recent data of cosmic microwave background (CMB) fluctuations.",

author = "M. Orito and T. Kajino and K. Ichiki and M. Yahiro and Mathews, {G. J.} and Y. Wang",

year = "2003",

month = may,

day = "19",

doi = "10.1016/S0375-9474(03)00950-3",

language = "English",

volume = "719",

pages = "C1--C8",

journal = "Nuclear Physics A",

issn = "0375-9474",

publisher = "Elsevier",

number = "1-4",

}

TY - JOUR

T1 - BBN and CMB constraints on universal lepton asymmetry, quintessential inflation, and brane world cosmology

AU - Orito, M.

AU - Kajino, T.

AU - Ichiki, K.

AU - Yahiro, M.

AU - Mathews, G. J.

AU - Wang, Y.

PY - 2003/5/19

Y1 - 2003/5/19

N2 - Recent progress in cosmological deep survey has clarified progressively the origin and distribution of matter and evolution of Galaxies in the Universe. The origin of the light elements in the Big-Bang nucleosynthesis (BBN) has been a topic of broad interest for its significance in constraining the dark matter component in the Universe, and also in seeking for the cosmological model which best fits the recent data of cosmic microwave background (CMB) fluctuations.

AB - Recent progress in cosmological deep survey has clarified progressively the origin and distribution of matter and evolution of Galaxies in the Universe. The origin of the light elements in the Big-Bang nucleosynthesis (BBN) has been a topic of broad interest for its significance in constraining the dark matter component in the Universe, and also in seeking for the cosmological model which best fits the recent data of cosmic microwave background (CMB) fluctuations.

UR - http://www.scopus.com/inward/record.url?scp=0038119670&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0038119670&partnerID=8YFLogxK

U2 - 10.1016/S0375-9474(03)00950-3

DO - 10.1016/S0375-9474(03)00950-3

M3 - Article

AN - SCOPUS:0038119670

VL - 719

SP - C1-C8

JO - Nuclear Physics A

JF - Nuclear Physics A

SN - 0375-9474

IS - 1-4

ER -

BBN and CMB constraints on universal lepton asymmetry, quintessential inflation, and brane world cosmology

Abstract

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this