The cosmic 21-cm revolution :charting the first billion years of our universe /

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"Version: 20191201"--Title page verso.Includes bibliographical references.1. Theoretical framework : the fundamentals of the 21 cm line -- 1.1. Radiative transfer of the 21 cm line -- 1.2. The spin temperature -- 1.3. Heating of the intergalactic medium2. Astrophysics from the 21 cm background -- 2.1. Properties of the high-z intergalactic medium -- 2.2. Sources of the UV and x-ray background -- 2.3. Predictions for the 21 cm background -- 2.4. Summary3. Physical cosmology from the 21 cm line -- 3.1. Introduction -- 3.2. Cosmology in the dark ages -- 3.3. Cosmology during the era of astrophysics -- 3.4. 21 cm cosmology in a larger context4. Inference from the 21 cm signal -- 4.1. What do we actually measure? -- 4.2. Optimal methods for characterizing the 21 cm signal -- 4.3. Modeling the 21 cm signal -- 4.4. Inference methods for the 21 cm signal5. 21 cm observations : calibration, strategies, observables -- 5.1. Interferometry overview -- 5.2. 21 cm observables : power spectra and images -- 5.3. Interferometric calibration and 21 cm observations -- 5.4. Array design and observing strategies -- 5.5. Conclusions -- 5.6. Acknowledgments6. Foregrounds and their mitigation -- 6.1. What are the foregrounds? -- 6.2. Foreground mitigation -- 6.3. Conclusions7. Global signal instrumentation -- 7.1. Introduction -- 7.2. Radiometer basics -- 7.3. Challenges facing experiments -- 7.4. Pr?ecis of design requirements -- 7.5. Outside the box architectures8. Status of 21 cm interferometric experiments -- 8.1. Introduction -- 8.2. Early work -- 8.3. Experimental methodologies and current experiments -- 8.4. Published results -- 8.5. Current challenges -- 8.6. Prospects for the future9. Future prospects -- 9.1. What drives future 21 cm signal experiment? -- 9.2. Ground-based interferometers -- 9.3. Global signal experiments -- 9.4. Space-based instruments -- 9.5. The far future of 21 cm cosmology.The redshifted 21-cm signal is set to transform astrophysical cosmology, bringing a historically data-starved field into the era of Big Data. Corresponding to the spin-flip transition of neutral hydrogen, the 21-cm line is sensitive to the temperature and ionization state of the cosmic gas, as well as to cosmological parameters. Crucially, with the development of new interferometers it will allow us to map out the first billion years of our universe, enabling us to learn about the properties of the unseen first generations of galaxies. Rapid progress is being made on both the observational and theoretical fronts, and important decisions on techniques and future direction are being made. The Cosmic 21-cm Revolution gathers contributions from current leaders in this fast-moving field, providing both an overview for graduate students and a reference point for current researchers.Graduate students and researchers in cosmology.Also available in print.Mode of access: World Wide Web.System requirements: Adobe Acrobat Reader, EPUB reader, or Kindle reader.Andrei Mesinger obtained his PhD from Columbia University in 2006. After a postdoc at Yale University, and a Hubble fellowship at Princeton University, he moved to Scuola Normale Superiore in Pisa in 2011 as junior faculty. He has authored over 100 publications on early structure formation and the epoch of reionization, as well as creating the widely-used public simulation code, 21cmFAST. In 2015, his research was recognized with a prestigious 1.5 million euro Starting Grant award from the European Research Council.Title from PDF title page (viewed on January 6, 2020).

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: .,

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1 online resource (various pagings) :illustrations (some color).

Language

English

ISBN/ISSN

9780750322362

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523.1

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Subject(s)

Nuclear astrophysics.
SCIENCE / Astronomy.
Cosmology.
Cosmology & the universe.
Red shift.

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edited by Andrei Mesinger.

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