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Cosmic Microwave Background Anisotropies
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▪ 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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“Measurements of the cosmic microwave background (CMB), the oldest light in the universe, contain a wealth of cosmological information, informing our understanding of physical processes across nearly all of cosmic time (see Hu & Dodelson 2002 for a review).”
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“are sufficient to characterise the key features of the first three peaks of the CMB [131, 132] (see also [133]).”
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Supernova Cosmology: Legacy and Future
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Cosmic microwave background anisotropies at second order: I
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“These anisotropies can be divided into two categories: scattering secondaries, when the CMB photons scatter with electrons along the line of sight, and gravitational secondaries when effects are mediated by gravity [21].”
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“ces, once theoretical uncertainties as well as statistical and systematic errors are accounted for [6]. The second way is from measurements of the CMB anisotropies (for pedagogical reviews, see Refs. [10, 11]). The crucial time for CMB is that of recombination, when the temperature dropped down to T <˘1eV and neutr…”
BackgroundIntegrated Sachs-Wolfe effect in cross-correlation: The observer's manual
Afshordi, N. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.70.083536 · Cited by 116
The 21-cm emission from the reionization epoch: extended and point source foregrounds
Matteo, T. D., Ciardi, B., & Miniati, F. (2004) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.08443.x · Cited by 115
Mukherjee, P., & Wang, Y. (2003) · The Astrophysical Journal · doi:10.1086/379161 · Cited by 113
“W ith W M AP,CM B data continues to be fully consistent with in ation (Guth 1981; Kolb & Turner 1990;Hu & Dodelson 2002;Peebles & Ratra 2003).”
BackgroundSmall-angle CMB temperature anisotropies induced by cosmic strings
Fraisse, A. A., Ringeval, C., Spergel, D. N., & Bouchet, F. R. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.043535 · Cited by 116
Secondary anisotropies of the CMB
Aghanim, N., Majumdar, S., & Silk, J. I. (2008) · Reports on Progress in Physics · doi:10.1088/0034-4885/71/6/066902 · Cited by 108
Cosmological Constraints from Multiple Probes in the Dark Energy Survey
Abbott, T. M. C., Alarcon, A., Allam, S., Andersen, P., Andrade-Oliveira, F., Annis, J. T., Asorey, J., Avila, S., Bacon, D., Banik, N., et al. (2019) · Physical Review Letters · doi:10.1103/physrevlett.122.171301 · Cited by 108
Self-citationJackson, N. J. (2007) · Living Reviews in Relativity · doi:10.12942/lrr-2007-4 · Cited by 105
“The process is reviewed in much more detail in [60].”
The Beginning and Evolution of the Universe
Ratra, B., & Vogeley, M. S. (2008) · Publications of the Astronomical Society of the Pacific · doi:10.1086/529495 · Cited by 118
“It has been the subject of recent reviews; see White & Cohn (2002), Hu & Dodelson (2002), Peebles & Ratra (2003, § IV.”
BackgroundThe Methodology of Scientific Research Programs
Merritt, D. R. (2020) · Cambridge University Press eBooks · doi:10.1017/9781108610926.003 · Cited by 97
Model of dark matter and dark energy based on gravitational polarization
Luc Blanchet, A., & Tiec, A. L. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.024031 · Cited by 98
Liang, Z.-C., Hu, Y.-M., Jiang, Y., Cheng, J., Zhang, J.-D., & Mei, J. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.105.022001 · Cited by 95
Planck pre-launch status: Expected LFI polarisation capability
Leahy, J. P., Bersanelli, M., D’Arcangelo, O., Ganga, K. M., Leach, S. M., Moss, A., Keihänen, E., Keskitalo, R., Kurki-Suonio, H., Poutanen, T. J., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200912855 · Cited by 93
“The importance of CMB polarimetry is now widely appreciated (e.g. Hu & Dodelson 2002).”
BackgroundBaumann, D. (2018) · doi:10.22323/1.305.0009 · Cited by 90
Analogue cosmological particle creation in an ultracold quantum fluid of light
Steinhauer, J., Abuzarli, M., Aladjidi, T., Bienaimé, T., Piekarski, C., Liu, W., Giacobino, E., Bramati, A., & Glorieux, Q. (2022) · Nature Communications · doi:10.1038/s41467-022-30603-1 · Cited by 105
Tests and Problems of the Standard Model in Cosmology
López-Corredoira, M. (2017) · Foundations of Physics · doi:10.1007/s10701-017-0073-8 · Cited by 87
“[202] and references therein for further comments).”
Dipolar dark matter and dark energy
Luc Blanchet, A., & Tiec, A. L. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.023524 · Cited by 87
Baryon acoustic oscillations from the SDSS DR10 galaxies angular correlation function
Carvalho, G. C., Bernui, A., Benetti, M., Carvalho, J., & Alcaniz, J. S. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.93.023530 · Cited by 87
Comparing early dark energy and extra radiation solutions to the Hubble tension with BBN
Seto, O., & Toda, Y. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.103.123501 · Cited by 86
Cosmic Acceleration, Dark Energy, and Fundamental Physics
Turner, M. S., & Dragan Huterer, A. (2007) · Journal of the Physical Society of Japan · doi:10.1143/jpsj.76.111015 · Cited by 86
Structure formation constraints on the Jordan-Brans-Dicke theory
Acquaviva, V., Baccigalupi, C., Leach, S. M., Liddle, A. R., & Perrotta, F. (2005) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.71.104025 · Cited by 91
The cosmic microwave background in an inhomogeneous universe
Clarkson, C., & Regis, M. (2011) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2011/02/013 · Cited by 84
“are sufficient to characterize the key features of the first three peaks of the CMB [63, 64] (see also [65–68] who use different but analogous parameters).”
Jackson, N. J. (2015) · Living Reviews in Relativity · doi:10.1007/lrr-2015-2 · Cited by 83
“The process is reviewed in much more detail in [92].”
BackgroundPhysics of the cosmic microwave background anisotropy
Bucher, M. (2015) · International Journal of Modern Physics D · doi:10.1142/s0218271815300049 · Cited by 92
“rving to probe the big bang. In this review, we have tried to sketch the most important aspects of the physics of the CMB in a self-contained way. Other reviews with a dierent emphasis include Refs. [92], [153] and [201]. We have seen how the CMB provides a snapshot of the state of the universe at around zˇ1100;when t…”
BackgroundSPTpol: an instrument for CMB polarization measurements with the South Pole Telescope
Austermann, J. E., Lueker, M., Shirokoff, E. D., & Vieira, J. D. (2012) · CaltechAUTHORS (California Institute of Technology) · Cited by 81
Delensing CMB Polarization with External DatasetsPreprint
Smith, K. M., Hanson, D., Loverde, M., Hirata, C. M., & Zahn, O. (2016) · Cited by 81
CMB and matter power spectra of early f(R) cosmology in the Palatini formulation
Li, B., & Chu, M. C. (2006) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.74.104010 · Cited by 79
Theoretical uncertainty in baryon oscillations
Eisenstein, D. J., & White, M. J. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.70.103523 · Cited by 78
Zahn, O., & Zaldarriaga, M. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.67.063002 · Cited by 77
Full-sky map of the ISW and Rees-Sciama effect from Gpc simulations
Cai, Y.-C., Cole, S., Jenkins, A. R., & Frenk, C. S. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16946.x · Cited by 75
“The power spectrum of the thermal effect is about one order of magnitude greater than the kSZ effect at arc minute and degree scales (e.g. Cooray 2001; Hu & Dodelson 2002).”
BackgroundCMB 3-point functions generated by nonlinearities at recombination
Creminelli, P., & Zaldarriaga, M. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.70.083532 · Cited by 77
“These anisotropies can be divided into scattering secondaries, when the CMB photons scatter with electrons along the line of sight, and gravitational secondaries when effects are mediated by gravity (for a review of all the different secondary effects see [8]).”
BackgroundNon‐Gaussianity and the Cosmic Microwave Background Anisotropies
Bartolo, N., Matarrese, S., & Riotto, A. W. (2010) · Advances in Astronomy · doi:10.1155/2010/157079 · Cited by 77
“These anisotropies can be divided into two categories: scattering secondaries, when the CMB photons scatter with electrons along the line of sight, and gravitational secondaries when effects are mediated by gravity [39].”
BackgroundFong, C. S., Nardi, E., & Riotto, A. W. (2012) · Archive ouverte UNIGE (University of Geneva) · Cited by 75
An Introduction to Radio Astronomy
Burke, B. F., Smith, F. G., & Wilkinson, P. N. (2019) · Cambridge University Press eBooks · doi:10.1017/9781316987506 · Cited by 78
FIRI—A far-infrared interferometer
Helmich, F. P., & Ivison, R. J. (2008) · Experimental Astronomy · doi:10.1007/s10686-008-9100-2 · Cited by 73
Padin, S., Staniszewski, Z. K., Keisler, R., Joy, M., Stark, A. A., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., et al. (2008) · Applied Optics · doi:10.1364/ao.47.004418 · Cited by 73
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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