Scalar field in the anisotropic universe - Wikidata - awgldk - TriplyDB

Scalar field in the anisotropic universe

Scalar field in the anisotropic universe

http://www.wikidata.org/entity/Q57656099

about

Solutions in the scalar-tensor theory with nonminimal derivative coupling Higher order spectra from an initially anisotropic universe Erratum: Scalar field in the anisotropic universe [Phys. Rev. D81, 083517 (2010)]

P2860

Erratum: Scalar field in the anisotropic universe [Phys. Rev. D81, 083517 (2010)]

P921

Q57656021-5170C184-986F-410A-ADE1-ACE1960AC1B5 Q57656046-52774C69-0551-4D09-ADE4-FFC66D88BFAD Q57656096-D78854CD-8977-488B-9891-C959BBD8177E

P2860

Q57656096-421AD1FD-51BE-4A72-B6A6-E95206E37DCA

P921

Scalar field in the anisotropic universe

http://www.wikidata.org/entity/Q57656099

description

im April 2010 veröffentlichter wissenschaftlicher Artikel

@de

wetenschappelijk artikel

@nl

наукова стаття, опублікована у квітні 2010

@uk

name

Scalar field in the anisotropic universe

@en

Scalar field in the anisotropic universe

@nl

type

label

Scalar field in the anisotropic universe

@en

Scalar field in the anisotropic universe

@nl

prefLabel

Scalar field in the anisotropic universe

@en

Scalar field in the anisotropic universe

@nl

P1433

Q57656099-1E2E46EF-6688-4BAE-A5D1-E8C6786FDA98

P1476

Q57656099-2654B728-FD84-496E-BE8E-1074F06E219E

P2093

Q57656099-9989E655-C7A1-4CA7-A1C3-0B0F40D099D4

Q57656099-F585539A-E69D-4246-918F-7BF6F78B66B6

P2507

Q57656099-14b81dfc-42f3-6e36-eae7-5a2e9574cfeb

P2860

Q57656099-01CF570C-79D6-4A10-B229-880046B7DBAC

Q57656099-0F7345DD-F8A8-4487-807A-CB4253E46014

Q57656099-0FE03EBD-B348-4B78-AA10-69953FEBEDD8

Q57656099-30EB05B0-A764-43BA-BF21-E2BE981592A1

Q57656099-396F13B2-8419-445E-AEB0-4B9015379D75

Q57656099-49E57F30-1738-4D56-A8EB-F8DCA47FE60B

Q57656099-6418CF6C-B78B-4DE0-B6E1-11A607494839

Q57656099-7AE624A0-FA38-489A-BF1A-8B61ECDF0765

Q57656099-9192492B-643C-4A7F-920E-C795B6A175B1

Q57656099-983297DD-16F3-4F7A-B249-6785ACE993C3

P31

Q57656099-C2A9A2AC-4860-4D2E-A147-CE72777F50E0

P356

Q57656099-5E47A2DE-2E05-4B08-8A05-D5A858C1B530

P407

Q57656099-E853A63F-EBC2-48AE-A8D5-E6BDD3E0E32E

P433

Q57656099-9A376CA9-749C-42A4-A721-B63BAEFB53D9

P478

Q57656099-F7A7FCBD-ED5D-4429-9D31-283652ECEC99

P577

Q57656099-BA0DBF32-4883-4DD2-A24E-B4CB1614927C

P356

PHYSREVD.81.083517

P1433

Physical Review D

P1476

Scalar field in the anisotropic universe

@en

P2093

Hyeong-Chan Kim

http://www.w3.org/2001/XMLSchema#string

Masato Minamitsuji

http://www.w3.org/2001/XMLSchema#string

P2507

Erratum: Scalar field in the anisotropic universe [Phys. Rev. D81, 083517 (2010)]

P2860

Significance of the largest scale CMB fluctuations in WMAP

Is the low-l microwave background cosmic?

Dodecahedral space topology as an explanation for weak wide-angle temperature correlations in the cosmic microwave background

Oscillatory approach to a singular point in the relativistic cosmology

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data

Inflationary universe with anisotropic hair.

First‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Preliminary Maps and Basic Results

Five-year Wilkinson Microwave Anisotropy Probe observations: cosmological interpretation

Asymmetries in the Cosmic Microwave Background Anisotropy Field

Evidence of Vorticity and Shear at Large Angular Scales in theWMAPData: A Violation of Cosmological Isotropy?

P31

scholarly article

P356

10.1103/PHYSREVD.81.083517

http://www.w3.org/2001/XMLSchema#string

P407

P433

8

http://www.w3.org/2001/XMLSchema#string

P478

81

http://www.w3.org/2001/XMLSchema#string

P577

2010-04-15T00:00:00Z

http://www.w3.org/2001/XMLSchema#dateTime