The DOI matches its Crossref record; 24 of the 24 references it cites were found in a registry or an index.
Cosmological Parameter Extraction from the First Season of Observations with the Degree Angular Scale Interferometer
Open accessAbstract
The Degree Angular Scale Interferometer (DASI) has measured the power spectrum of the cosmic microwave background anisotropy over the range of spherical harmonic multipoles 100 < l < 900. We compare these data, in combination with the COBE DMR results, to a seven-dimensional grid of adiabatic cold dark matter (CDM) models. Adopting the priors h > 0.45 and 0.0 ≤ τ c ≤ 0.4, we find that the total density of the universe Ω tot = 1.04 ± 0.06 and the spectral index of the initial scalar fluctuations n s = 1.01 in accordance with the predictions of inflationary theory. In addition, we find that the physical density of baryons Ω b h 2 = 0.022 , and the physical density of cold dark matter Ω cdm h 2 = 0.14 ± 0.04. This value of Ω b h 2 is consistent with that derived from measurements of the primeval deuterium abundance combined with big bang nucleosynthesis theory. Using the result of the Hubble Space Telescope ( HST ) Key Project, h = 0.72 ± 0.08, we find that Ω tot = 1.00 ± 0.04, the matter density Ω m = 0.40 ± 0.15, and the vacuum energy density Ω Λ = 0.60 ± 0.15. (All 68% confidence limits.)
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A flat Universe from high-resolution maps of the cosmic microwave background radiation
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Fluctuations in the New Inflationary Universe
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Spontaneous creation of almost scale-free density perturbations in an inflationary universe
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The development of irregularities in a single bubble inflationary universe
Hawking, S. W. (1982) · Physics Letters B · doi:10.1016/0370-2693(82)90373-2 · Cited by 1,985
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Cited by
Cosmological parameters from CMB and other data: A Monte Carlo approach
Lewis, A., & Bridle, S. (2002) · Physical Review D · doi:10.1103/physrevd.66.103511 · Cited by 3,495
Beyond the cosmological standard model
Joyce, A., Jain, B., Khoury, J., & Trodden, M. (2015) · Physics Reports · doi:10.1016/j.physrep.2014.12.002 · Cited by 1,231
The inflationary brane-antibrane universe
Burgess, C. P., Majumdar, M., Nolte, D., Quevedo, F., Rajesh, G., & Zhang, R.-J. (2001) · Journal of High Energy Physics · doi:10.1088/1126-6708/2001/07/047 · Cited by 549
The Evolution of X-Ray Clusters of Galaxies
Rosati, P., Borgani, S., & Norman, C. (2002) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.40.120401.150547 · Cited by 482
Supersymmetric dark matter in light of WMAP
Ellis, J., Olive, K. A., Santoso, Y., & Spanos, V. C. (2003) · Physics Letters B · doi:10.1016/s0370-2693(03)00765-2 · Cited by 398
Metadata
- Authors
- Pryke, C., Halverson, N. W., Leitch, E. M., Kovac, J., Carlstrom, J. E., Holzapfel, W. L., & Dragovan, M.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2002-03-20
- Volume
- 568
- Issue
- 1
- Pages
- 46-51
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2949473086
- Cited by
- 312
- References
- 24
- FWCI
- 50.14
- Type
- journal article
- Language
- en
- Open access
- bronze
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