4.2 Article

New horizons in cosmology with spectral distortions of the cosmic microwave background

Journal

EXPERIMENTAL ASTRONOMY
Volume 51, Issue 3, Pages 1515-1554

Publisher

SPRINGER
DOI: 10.1007/s10686-021-09729-5

Keywords

Cosmology; Early universe; Cosmic microwave background; CMB spectral distortions; Particle physics

Funding

  1. European Research Council under the European Union [725456]
  2. Royal Society [UF130435, RG140523]
  3. Spanish Ministry of Science and Innovation (MICINN) [AYA2017-84185-P]
  4. European Union [687312]
  5. Spanish Ministry of Science [PGC2018-097585B-C21]
  6. ASI/Physics Department of the University of Roma-Tor Vergata [2016-24-H.0]
  7. Royal Society [UF130435] Funding Source: Royal Society

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This paper discusses the unique scientific opportunities presented by studying spectral distortions of the cosmic microwave background, emphasizing the importance of precision spectroscopy using existing technology. It highlights the potential for new discoveries in physics and challenges to our current understanding of the laws of nature, offering valuable insights into the early Universe.
This Voyage 2050 paper highlights the unique science opportunities using spectral distortions of the cosmic microwave background (CMB). CMB spectral distortions probe many processes throughout the history of the Universe, delivering novel information that complements past, present and future efforts with CMB anisotropy and large-scale structure studies. Precision spectroscopy, possible with existing technology, would not only provide key tests for processes expected within the cosmological standard model but also open an enormous discovery space to new physics. This offers unique scientific opportunities for furthering our understanding of inflation, recombination, reionization and structure formation as well as dark matter and particle physics. A dedicated experimental approach could open this new window to the early Universe in the decades to come, allowing us to turn the long-standing upper distortion limits obtained with COBE/FIRAS some 25 years ago into clear detections of the expected standard distortion signals and also challenge our current understanding of the laws of nature.

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