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Titlebook: Understanding the Epoch of Cosmic Reionization; Challenges and Progr Andrei Mesinger Book 2016 Springer International Publishing Switzerlan

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發(fā)表于 2025-3-21 16:12:58 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Understanding the Epoch of Cosmic Reionization
副標題Challenges and Progr
編輯Andrei Mesinger
視頻videohttp://file.papertrans.cn/942/941797/941797.mp4
概述Brings together experts from diverse fields to create a comprehensive picture of reionization and the cosmic dawn of the Universe.Forms a timely guide for robustly interpreting the wave of recent and
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Understanding the Epoch of Cosmic Reionization; Challenges and Progr Andrei Mesinger Book 2016 Springer International Publishing Switzerlan
描述The dawn of the first stars, galaxies and black holes signaled a fundamental milestone in our Universe’s evolution: the Epoch of Reionization. The light from these galactic ancestors began spreading out, ionizing virtually every atom in existence. Our Universe transitioned from darkness to light, from cold to hot, from simple and boring to the wondrous cosmic zoo we see around us today.Despite its importance, observations of reionization have been few, and their interpretation has been highly controversial. Fortunately, this is rapidly changing. We will soon enter the "Big Data” era of this mysterious epoch, driven by an upcoming wave of observations with state-of-the-art telescopes as well as new sophisticated analysis tools.?.The aim of this volume is to summarize the current status and future outlook of the reionization field. We bring together leading experts in many sub-disciplines, highlighting the measurements that will illuminate our understanding of reionization and the cosmic dawn: (i) 21cm interferometry; (ii) high-redshift quasar spectra; (iii) high-redshift galaxy surveys; (iv) primary and secondary anisotropies of the Cosmic Microwave Background; (v) high-resolution s
出版日期Book 2016
關鍵詞Cosmic Background Radiation; Cosmic Dawn; Early Universe Astrophysics; First Light Cosmology; Future Obs
版次1
doihttps://doi.org/10.1007/978-3-319-21957-8
isbn_softcover978-3-319-79372-6
isbn_ebook978-3-319-21957-8Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer International Publishing Switzerland 2016
The information of publication is updating

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Cosmic Reionization and the First Nonlinear Structures in the Universe,on the earliest, least well understood stages, and emphasize the most important open questions. We include a historical summary, and highlight the role of reionization as one of the few milestones in the evolution of the universe since the Big Bang, and its status as a unique probe of the beginning
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Constraining Reionization with Ly, Emitting Galaxies,ter I summarise the increasing observational support for the claim that Ly. photons emitted by galaxies at .?>?6 are suppressed by intervening HI gas. I describe key physical processes that affect Ly. transfer during the EoR. I argue that in spite of the uncertainties associated with this complex mu
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Metal Enrichment in the Reionization Epoch,dered to be primary sources of the ionizing radiation required to power cosmic reionization. Therefore, an intimate link between metal and ionizing photon production must exist. In this chapter, I elaborate on this concept, outlining the basic ingredients necessary to model metal enrichment and inte
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Quasars as Probes of Cosmological Reionization,onding to a redshift of .???5), and are powerful probes of the inter-galactic medium at that time. This review covers current efforts to identify high-redshift quasars and how they have been used to constrain the reionization history. This includes a full description of the various processes by whic
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