Cosmic Microwave Background Anisotropies

By Wayne Hu, Scott Dodelson. 2001

681 citations recorded by the source corpus.

▪ Abstract Cosmic microwave background (CMB) temperature anisotropies have and will continue to revolutionize our understanding of cosmology. The recent discovery of the previously predicted acoust...

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Citations in the corpus

Does the Hubble constant tension call for new physics? (2018, background): “, the matter density ωM, the baryon density ωB, the angular distance to recombination dA(z∗) and the overall spectral tilt of primordial fluctuations, n [44].”
On the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Matter (2006, background): “…Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85121 2Departments of Physics and Astronomy, University of California, Berkeley, CA 94720 3Alfred P. Sloan Fellow the CMB acoustic peaks (Bennett, Turner, & White 1997; Hu et al. 1997; Hu & Dodelson 2002; White & Cohn 2002).”
The Hubble Constant (2010, background): “A recent detailed review of the cosmic microwave background is given in Hu & Dodelson (2002).”
Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies (2005, background): “…are generated early (z ≫ 1000) and are dominantly adiabatic (Hu & White 1996a,b; Hu et al. 1997; Peiris et al. 2003; Moodley et al. 2004), and by their mere existence largely validate the simple theory used to support their interpretation (for reviews, see Hu et al. 1997; Hu & Dodelson 2002).”
Primordial nucleosynthesis for the new cosmology: Determining uncertainties and examining concordance (2004, background): “…of CMB theory see White, Scott and Silk (1994) [27], Tegmark (1995) [28], Van der Veen (1998) [29], Kamionkowski and Kosowsky (1999) [30] and Hu and Dodelson (2002) [31] and of CMB observations see Wang et al (2002) [32] for a pre-WMAP evaluation and the individual group papers mentioned…”
Delensing CMB polarization with external datasets (2010, methodology): “Lens reconstruction from temperature has been applied to detect CMB lensing in WMAP, in crosscorrelation with large-scale structure [46, 47] and is expected to be a powerful source of cosmological information in the near future [48, 49, 50, 51, 52, 53, 54, 55, 56, 57, 58, 59].”
Astrobiology: The Study of the Living Universe (2005, background): “In this context there is some irony in the recent determination that matter like that we know on Earth in fact comprises only some four percent of the massenergy of the universe (Hu & Dodelson 2002).”
Multiscale cluster lens mass mapping - I. Strong lensing modelling (2009, background): “…2003) or the velocity dispersion of the galaxies in galaxy clusters (e.g. Czoske et al. 2002) but also to reproduce the large scale galaxy distribution (e.g. Guzzo et al. 2008; Seljak et al. 2005) and thecosmological microwave background (CMB) fluctuations (e.g. the review by Hu & Dodelson 2002).”
CONSTRAINTS ON COSMOLOGY FROM THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM OF THE 2500 deg2 SPT-SZ SURVEY (2012, methodology): “For each case, we begin by briefly reviewing the origins of the WMAP7 constraints (see, e.g., Hu & Dodelson 2002) and then discuss the origins of the SPT constraints.”
Leptogenesis (2008, unknown): “The second way to determine ΩB is from measurements of the cosmic microwave background (CMB) anisotropies (for a pedagogical review, see [5]).”
The fundamental constants and their variation: observational and theoretical status (2002, background): “The Cosmic Microwave Background Radiation (CMBR) is composed of the photons emitted at the time of the recombination of hydrogen and helium when the universe was about 300,000 years old [see e.g. Hu and Dodelson (2002) or Durrer (2002) for recent reviews on CMBR physics].”