The Cosmic microwave background radiation

@article{Gawiser2000TheCM,
  title={The Cosmic microwave background radiation},
  author={Eric Gawiser and Joseph I. Silk},
  journal={Physics Reports},
  year={2000},
  volume={333},
  pages={245-267}
}

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References

SHOWING 1-10 OF 138 REFERENCES
The physics of microwave background anisotropies
The residual radiation from the Big Bang is observable as the cosmic microwave background–a near-uniform sea of photons with an average temperature of 2.7 K. Small variations in the temperature of
Gravitational Lensing and the Cosmic Microwave Background
We present calculations of the effect of the gravitational lensing of the cosmic microwave photons, produced by linear density perturbations, on the anisotropies of the cosmic microwave background
Extracting primordial density fluctuations
The combination of detections of anisotropy in cosmic microwave background radiation and observations of the large-scale distribution of galaxies probes the primordial density fluctuations of the
Measurements of Structure in the Cosmic Background Radiation with the Cambridge Cosmic Anisotropy Telescope
We have observed a 2° × 2° area of sky at frequencies of 15.5 and 16.5 GHz with the Cambridge Cosmic Anisotropy Telescope (CAT). Comparison with earlier measurements at 13.5 GHz shows that the
Looking for a cosmological constant with the Rees-Sciama effect.
TLDR
The prospects for using an x-ray/COBE comparison to detect a cosmological constant are discussed and a correlation between the CMB anisotropy and the potential reflects the matter density is examined.
Ionization by early quasars and Cosmic Microwave Background anisotropies. (Erratum)
We discuss the photoionization of the intergalactic medium by early formed quasars and propose a mechanism which could generate measurable temperature fluctuations $\delta_{T }~=~\Delta T/T$ of the
Small-Scale Anisotropy of the Cosmic Background Radiation and Scattering by Cloudy Plasma
If the first stars formed soon after decoupling of baryons from the thermal cosmic background radiation (CBR), the radiation may have been last scattered in a cloudy plasma. We discuss the resulting
Small scale cosmic microwave background anisotropies as a probe of the geometry of the universe
We perform detailed calculations of cosmic microwave background (CMB) anisotropies in a cold dark matter (CDM)-dominated open universe with primordial adiabatic density perturbations for a variety of
Impact of Inhomogeneous Reionization on Cosmic Microwave Background Anisotropy
It is likely that the reionization of the Universe did not occur homogeneously. Using a model that associates ionized patches with overdense regions, we find that the resulting cosmic microwave
Contribution of Extragalactic Infrared Sources to Cosmic Microwave Background Foreground Anisotropy
We estimate the level of confusion to cosmic microwave background (CMB) anisotropy measurements caused by extragalactic infrared sources. CMB anisotropy observations at high resolution and high
...
...