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Cosmic Microwave Background Anisotropies
Open accessAbstract
▪ Abstract Cosmic microwave background (CMB) temperature anisotropies have and will continue to revolutionize our understanding of cosmology. The recent discovery of the previously predicted acoustic peaks in the power spectrum has established a working cosmological model: a critical density universe consisting of mainly dark matter and dark energy, which formed its structure through gravitational instability from quantum fluctuations during an inflationary epoch. Future observations should test this model and measure its key cosmological parameters with unprecedented precision. The phenomenology and cosmological implications of the acoustic peaks are developed in detail. Beyond the peaks, the yet to be detected secondary anisotropies and polarization present opportunities to study the physics of inflation and the dark energy. The analysis techniques devised to extract cosmological information from voluminous CMB data sets are outlined, given their increasing importance in experimental cosmology as a whole.
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“Analysis of the WMAP data puts very strongly pressure on the simple monomial w ( χ ) = G 4 χ 4 at the 3 σ level[18, 40]”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [40]
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“, it is curl-free), and is referred to as the E-mode polarization.(14) The CMB E modes originate from the same primary anisotropies seen in the intensity, therefore, they provide a semi-independent probe of the base cosmological model, known as ΛCDM .”
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“(40) should be modified and rewritten as (Doran & Lilley 2002; Doran et al. 2002; Hu & Dodelson 2002; Hu et al. 2001) ln = lA(n − ζn), (41) where ζn = ζ + ∆ζ, here ∆ζ is a general phase shift, whose form for the first three peaks is given in (Doran & Lilley 2002), and ζ = a1(rrec)a2 + Ωrecφ ,…”
BackgroundCMB anisotropies in the presence of extra dimensions
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“…therein), several balloon-borne and ground-based operating experiments were successful in detecting CMB anisotropies on degree and subdegree angular scales (Lee et al. 2001; Padin et al. 2001; De Bernardis et al. 2002; Halverson et al. 2002; see also Hu & Dodelson 2002, and references therein).”
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Regis, M., & Clarkson, C. (2012) · General Relativity and Gravitation · doi:10.1007/s10714-011-1322-3 · Cited by 36
COSMOS-e’-GTachyon from string theory
Choudhury, S., & Panda, S. (2016) · The European Physical Journal C · doi:10.1140/epjc/s10052-016-4072-2 · Cited by 43
Homogeneous scalar field and the wet dark sides of the universe
Díez-Tejedor, A., & Feinstein, A. (2006) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.74.023530 · Cited by 35
Bose–Einstein condensation, dark matter and acoustic peaks
Ferrer, F., & Grifols, J. A. (2004) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2004/12/012 · Cited by 36
Reduction of cosmological data for the detection of time-varying dark energy density
Dick, J., Knox, L., & Chu, M. (2006) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2006/07/001 · Cited by 36
Dark matter component in hadronic models with short-range correlations
Lourenço, O., Frederico, T., & Dutra, M. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.105.023008 · Cited by 35
Power spectra to 1 per cent accuracy between dynamical dark energy cosmologies★
Francis, M. J., Lewis, G. F., & Linder, E. V. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12139.x · Cited by 35
Amblard, A., Cooray, A. R., & Kaplinghat, M. (2007) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.75.083508 · Cited by 34
Clarifying inflation models: Slow roll as an expansion in 1/Nefolds
Boyanovsky, D., de Vega, H. J., & Sanchez, N. G. (2006) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.73.023008 · Cited by 38
Sharp, M. K., Marrone, D. P., Carlstrom, J. E., Culverhouse, T. L., Greer, C. H., Hawkins, D., Hennessy, R., Joy, M. K., Lamb, J. W., Leitch, E. M., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/713/1/82 · Cited by 34
Model-independent constraints on Ωm and H(z) from the link between geometry and growth
Ruiz-Zapatero, J., García-García, C., Alonso, D., Ferreira, P. G., & Grumitt, R. D. P. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac431 · Cited by 34
Symons, T., Zemcov, M. B., Cooray, A. R., Lisse, C. M., & Poppe, A. R. (2023) · The Astrophysical Journal · doi:10.3847/1538-4357/acaa37 · Cited by 34
“EBL sources include faint residual radiation from the universe’s early evolution, such as the cosmic microwave background (Hu & Dodelson 2002), as well as later emission from stellar and galactic evolution through cosmic time (Hauser & Dwek 2001; Cooray 2016), and as a result is a powerful probe of…”
BackgroundAdshead, P. J., & Easther, R. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/10/047 · Cited by 35
A review of modeling interacting transient phenomena with non-equilibrium Green functions
Hirsbrunner, M. R., Philip, T. M., Basa, B., Kim, Y., Park, M. J., & Gilbert, M. J. (2019) · Reports on Progress in Physics · doi:10.1088/1361-6633/aafe5f · Cited by 36
Herranz, D., Kuruoğlu, E. E., & Toffolatti, L. (2004) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20035858 · Cited by 33
“For a recent review on the study of CMB anisotropies, see Hu & Dodelson (2002).”
BackgroundDistinguishing among scalar field models of dark energy
Maor, I., & Brustein, R. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.67.103508 · Cited by 33
“The position of the first peak is already measured rather well, to about 3% at the 1σ level (see, for example, [23]).”
BackgroundDependence of the cosmic microwave background lensing power spectrum on the matter density
Pan, Z., Knox, L., & White, M. J. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu1971 · Cited by 29
“Fortunately, the anisotropies arise from relatively simple physical processes so such an understanding is possible (Hu & Dodelson 2002).”
BackgroundBarman, B., & Ghoshal, A. (2022) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2022/03/003 · Cited by 32
Nonparametric Inference for the Cosmic Microwave Background
Genovese, C. R., Miller, C. J., Nichol, R. C., Arjunwadkar, M., & Wasserman, L. (2004) · Statistical Science · doi:10.1214/088342304000000161 · Cited by 32
“Mathematical techniques for studying fluid dynamics apply well in this scenario and have been investigated by many authors (see for instance Hu and Sugiyama 1995; Hu 1999, 2001, 2003; Hu and Dodelson 2002).”
MethodDiffuse Source Separation in CMB Observations
Delabrouille, J., & Cardoso, J.-F. (2008) · Lecture notes in physics · doi:10.1007/978-3-540-44767-2_6 · Cited by 32
“Eriksen and collaborators have developed a method based on a refined modelling of the astrophysical components and fitted this model to the data to obtain estimates of foreground parameters (Eriksen et al. [ 21 ]).”
BackgroundMethodBose, S., & Грищук, Л. П. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.66.043529 · Cited by 30
“For the latest statement that the initial spectrum of gravitational waves is “constrained to be small compared with the initial density spectrum” see the latest article praising inflationary predictions (for instance, [ 28 ]).”
BackgroundInfluentialStraumann, N. (2007) · Lecture notes in physics · doi:10.1007/978-3-540-71117-9_13 · Cited by 31
LEPTOGENESIS FROM SOFT SUPERSYMMETRY BREAKING: SOFT LEPTOGENESIS
FONG, C. S., GONZALEZ-GARCIA, M. C., & NARDI, E. (2011) · International Journal of Modern Physics A · doi:10.1142/s0217751x1105405x · Cited by 31
“All the parameters appearing in the superpotential (10) and in the Lagrangian (12) (or equivalently in the first three lines of Eq.”
BackgroundInfluentialCosmic microwave background acoustic peak locations
Pan, Z., Knox, L., Mulroe, B., & Narimani, A. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw833 · Cited by 31
“For simplicity we drop, for now, the Ψ̈ term on the left side of the above equation and we have (Hu & Dodelson 2002){ d2 dη2 + k2c2s } [Θ0 + Φ] = 0, (7) where we have used the facts that Φ = Ψ in the absence of photon anisotropic stress, c2s ' 1/3, and Ψ̈ term is small after potentials decay.”
MethodTwo-phase reheating: CMB constraints on inflation and dark matter phenomenology
Haque, M. R., Maity, D., & Saha, P. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.102.083534 · Cited by 37
SPECTRAL DISTORTIONS OF THE CMB DIPOLE
Balashev, S. A., Kholupenko, E. E., Chluba, J., Ivanchik, A. V., & Varshalovich, D. A. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/810/2/131 · Cited by 31
Early Dark Energy in Type IIB String Theory
Cicoli, M., Licheri, M., Mahanta, R., McDonough, E., Pedro, F. G., & Scalisi, M. (2023) · Journal of High Energy Physics · doi:10.1007/jhep06(2023)052 · Cited by 31
“For a review of CMB physics and terminology, see [63].”
Background
Metadata
- Authors
- Hu, W., & Dodelson, S.
- Affiliations
- Fermi National Accelerator Laboratory (US)
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 2002-09
- Volume
- 40
- Issue
- 1
- Pages
- 171-216
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2123864481
- Cited by
- 745
- References
- 208
- Citations by year
- 2026: 35 · 2025: 38 · 2024: 38 · 2023: 28 · 2022: 34 · 2021: 27 · 2020: 37 · 2019: 58 · 2018: 25 · 2017: 25 · 2016: 24 · 2015: 29 · 2014: 26 · 2013: 29 · 2012: 18
- FWCI
- 3.64
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Annual Review of Astronomy and Astrophysics (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- cosmic microwave background, temperature anisotropy, acoustic peaks, power spectrum, inflation (cosmology), dark energy, dark matter, gravitational instability, quantum fluctuations, secondary anisotropies, CMB polarization, cosmological parameters, structure formation
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