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These lecture notes comprise an informal but pedagogical introduction to the well established physics and phenomenology of the cosmic microwave background (CMB) between big bang nucleosynthesis and recombination.
Bardeen, J.M. (1980). Gauge invariant cosmological perturbations, Phys. Rev. , D22
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Alpher, R.A. and Herman, R.C. (1948). On the relative abundance of the elements, Phys. Rev. , 74
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Gamow, G. (1948). The origin of elements and the separation of galaxies, Phys. Rev. , 74
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Dicke, R.H., Peebles, P.J.E., Roll, P.G. and Wilkinson, D.T. (1965). Cosmic Black-Body Radiation., ApJ , 142
1965
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Sachs, R.K. and Wolfe, A.M. (1967). Perturbations of a Cosmological Model and Angular Variations of the Microwave Background, ApJ , 147
1967
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Peebles, P.J.E. (1968). Recombination of the Primeval Plasma, ApJ , 153
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Silk, J. (1968). Cosmic Black-Body Radiation and Galaxy Formation, ApJ , 151
1968
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Zeldovich, Y.B. and Sunyaev, R.A. (1969). The Interaction of Matter and Radiation in a Hot-Model Universe, Ap&SS , 4
1969
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Peebles, P.J.E. and Yu, J.T. (1970). Primeval Adiabatic Perturbation in an Expanding Universe, ApJ , 162
1970
Earlier work this paper cites.
Danese, L. and de Zotti, G. (1982). Double Compton process and the spectrum of the microwave background, A&A , 107
1982
Earlier work this paper cites.
Kaiser, N. (1983). Small-angle anisotropy of the microwave background radiation in the adiabatic theory, MNRAS , 202
1983
Earlier work this paper cites.
Bond, J.R. and Efstathiou, G. (1984). Cosmic background radiation anisotropies in universes dominated by nonbaryonic dark matter, ApJ , 285
1984
Earlier work this paper cites.
Vittorio, N. and Silk, J. (1984). Fine-scale anisotropy of the cosmic microwave background in a universe dominated by cold dark matter, ApJ , 285
1984
Earlier work this paper cites.
Polnarev, A.G. (1985). Polarization and Anisotropy Induced in the Microwave Background by Cosmological Gravitational Waves, Soviet Astronomy , 29
1985
Earlier work this paper cites.
Bond, J.R. and Efstathiou, G. (1987). The statistics of cosmic background radiation fluctuations, MNRAS , 226
1987
Earlier work this paper cites.
Smoot, G.F. et al. (1992). Structure in the COBE differential microwave radiometer first-year maps, ApJ , 396
1992
Cited alongside, same era.
Hu, W. and Silk, J. (1993). Thermalization and spectral distortions of the cosmic background radiation, Phys. Rev. , D48
1993
Cited alongside, same era.
Hu, W. and Sugiyama, N. (1995). Anisotropies in the Cosmic Microwave Background: An Analytic Approach, Astrophys. J. , 444
1995
Cited alongside, same era.
Fixsen, D.J. et al. (1996). The Cosmic Microwave Background Spectrum from the Full COBE FIRAS Data Set, ApJ , 473
1996
Cited alongside, same era.
Hu, W. and Sugiyama, N. (1996). Small scale cosmological perturbations: An Analytic approach, Astrophys. J. , 471
1996
Cited alongside, same era.
Hanany, S. et al. (2000). MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of 10’-5°, ApJ , 545
2000
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Lewis, A., Challinor, A. and Lasenby, A. (2000). Efficient Computation of Cosmic Microwave Background Anisotropies in Closed Friedmann-Robertson-Walker Models, ApJ , 538
2000
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Seager, S., Sasselov, D.D. and Scott, D. (2000). How exactly did the Universe become neutral?, Astrophys. J. Suppl. , 128
2000
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Tytler, D. et al. (2000). Review of Big Bang nucleosynthesis and primordial abundances., Physica Scripta Volume T , 85
2000
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Hu, W., Fukugita, M., Zaldarriaga, M. and Tegmark, M. (2001). CMB Observables and Their Cosmological Implications, Astrophys. J. , 549
2001
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Hu, W. and White, M.J. (1996). A New Test of Inflation, Phys. Rev. Lett. , 77
1996
Cited alongside, same era.
Seljak, U. and Zaldarriaga, M. (1996). A Line-of-Sight Integration Approach to Cosmic Microwave Background Anisotropies, ApJ , 469
1996
Cited alongside, same era.
Hu, W. and White, M.J. (1997). CMB Anisotropies: Total Angular Momentum Method, Phys. Rev. , D56
1997
Cited alongside, same era.
Kamionkowski, M., Kosowsky, A. and Stebbins, A. (1997). Statistics of cosmic microwave background polarization, Phys. Rev. , D55
1997
Cited alongside, same era.
White, M.J. and Hu, W. (1997). The Sachs-Wolfe effect, Astron. Astrophys. , 321
1997
Cited alongside, same era.
Zaldarriaga, M. and Seljak, U. (1997). An all-sky analysis of polarization in the microwave background, Phys. Rev. D , 55
1997
Cited alongside, same era.
Eisenstein, D., Hu, W. and Tegmark, M. (1998). Cosmic Complementarity: H 0 H_{0} and Ω m \Omega_{m} from Combining CMB Experiments and Redshift Surveys, ApJ , 504
1998
Cited alongside, same era.
Padin, S. et al. (2001). First Intrinsic Anisotropy Observations with the Cosmic Background Imager, ApJ , 549
2001
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Pryke, C. et al. (2001). Cosmological Parameter Extraction from the First Season of Observations with DASI, ApJ , In Press
2001
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Hu, W. and Dodelson, S. (2002). Cosmic Microwave Background Anisotropies, Ann. Rev. Astron. Astrophys. , 40
2002
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Kovac, J. et al. (2002). Detection of polarization in the cosmic microwave background using DASI, Nature , 420
2002
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Hu, W. (2003). Covariant Linear Perturbation Formalism, ICTP , 14
2003
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Hu, W. and White, M.J. (2004). The cosmic symphony, Sci. Am. , 290N2
2004
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Hu, W. and Okamoto, T. (2004). Principal Power of the CMB, Phys. Rev. , D69
2004
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Eisenstein, D.J. et al. (2005). Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies, Astrophys. J. , 633
2005
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Hu, W. (2005). Dark Energy Probes in Light of the CMB, ASPC , 339
2005
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Spergel, D.N. et al. (2007). Wilkinson Microwave Anisotropy Probe (WMAP) three year results: Implications for cosmology, Astrophys. J. Suppl. , 170
2007
Later among the works it cites.