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相关论文: Physical Processes at Cosmic Dawn

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The search for the first illuminated astronomical sources in the universe is at the edge of the cosmic frontier. Promising techniques for discovering the first objects and their effects span the electromagnetic spectrum and include…

天体物理学 · 物理学 2009-11-13 E. J. Barton , J. S. Bullock , A. Cooray , M. Kaplinghat

The cosmic dawn and epoch of reionization mark the time period in the universe when stars, galaxies, and blackhole seeds first formed and the intergalactic medium changed from neutral to an ionized one. Despite substantial progress with…

I review recent progress and challenges in studies of the earliest galaxies, seen when the Universe was less than 1 billion years old. Can they be used as reliable tracers of the physics of cosmic reionization thereby complementing other,…

宇宙学与河外天体物理 · 物理学 2014-11-14 Richard S. Ellis

After recombination the cosmic gas was left in a cold and neutral state. However, as the first stars and black holes formed within early galactic systems, their UV and X-ray radiation induced a gradual phase transition of the intergalactic…

宇宙学与河外天体物理 · 物理学 2014-09-18 Andrea Ferrara , Stefania Pandolfi

The intergalactic medium - the cosmic gas that fills the great spaces between the galaxies - is affected by processes ranging from quantum fluctuations in the very early universe to radiative emission from newly-formed stars. This gives the…

天体物理学 · 物理学 2008-11-26 Rennan Barkana , Abraham Loeb

The study of cosmic reionization has acquired increasing significance over the last few years because of various reasons. On the observational front, we now have good quality data of different types at high redshifts (quasar absorption…

天体物理学 · 物理学 2007-05-23 T. Roy Choudhury , A. Ferrara

Reionization represents an important phase in the history of our Universe when ultraviolet radiation from the first luminous sources, primarily stars and accreting black holes, ionized the neutral hydrogen atoms in the intergalactic medium…

宇宙学与河外天体物理 · 物理学 2025-02-18 Anirban Chakraborty , Tirthankar Roy Choudhury

The universe goes through several phase transitions during its formative stages. Cosmic reionization is the last of them, where ultraviolet and X-ray radiation escape from the first generations of galaxies heating and ionizing their…

宇宙学与河外天体物理 · 物理学 2019-07-17 John H. Wise

This is the report of the {\em Working Group on Early Universe Cosmology and Tests of Fundamental Physics}, group P4.8 of the of the Snowmass 2001 conference. Here we summarize the impressive array of advances that have taken place in this…

高能物理 - 唯象学 · 物理学 2010-04-08 Andreas Albrecht , Joshua A. Frieman , Mark Trodden

In these notes we present a selection of topics, each section approximately amounting to one lecture. We begin with a brief recapitulation of General Relativity, and the Standard Model of Cosmology. This is followed by lectures on important…

高能物理 - 唯象学 · 物理学 2014-11-14 U. A. Yajnik

In these lecture notes we review the current knowledge about the formation of the first luminous objects. We start from the cosmological context of hierarchical models of structure formation, and discuss the main physical processes which…

天体物理学 · 物理学 2015-06-24 Emanuele Ripamonti , Tom Abel

Wasn't this a fun meeting? Yes, except for the rain. This summary highlights scientific themes of the 13th IAP conference: (1) The History of Baryons; (2) The History of Metals; (3) Reionization of the IGM; (4) The Assembly of Galaxies,…

天体物理学 · 物理学 2007-05-23 J. Michael Shull

Understanding the formation of the first stars and galaxies is a key problem in modern cosmology. In these lecture notes, we will derive some of the basic physical principles underlying this emerging field. We will consider the basic…

宇宙学与河外天体物理 · 物理学 2012-03-20 Volker Bromm

These lectures summarize our basic understanding of the emergence of cosmic structures, the epoch of first light, the survival of early substructure in present-day galaxy halos.

天体物理学 · 物理学 2007-06-04 Piero Madau

The formation of the first stars and quasars marks the transformation of the universe from its smooth initial state to its clumpy current state. In popular cosmological models, the first sources of light began to form at redshift 30 and…

天体物理学 · 物理学 2011-08-23 Rennan Barkana , Abraham Loeb

The development of primordial inhomogeneities into the non-linear regime and the formation of the first bound objects mark the transition from a simple cooling universe -- described by just a few parameters -- to a very messy hot one -- the…

天体物理学 · 物理学 2009-11-07 Piero Madau

I give a brief overview of cosmic ray physics, highlighting some key questions and how they will be addressed by new experiments.

天体物理学 · 物理学 2011-05-12 Thomas K. Gaisser

Galaxy formation is at the forefront of observation and theory in cosmology. An improved understanding is essential for improving our knowledge both of the cosmological parameters, of the contents of the universe, and of our origins. In…

宇宙学与河外天体物理 · 物理学 2018-10-17 Joseph Silk , Arianna Di Cintio , Irina Dvorkin

Cosmology is passing through a golden phase of rapid advance. The cosmology workshop at ICGC-2004 attracted a large number of research contributions from diverse topics of cosmology. I attempt to classify and summarize the research work and…

天体物理学 · 物理学 2015-06-24 Tarun Souradeep

This paper summarizes highlights of the OG3.1, 3.2 and 3.3 sessions of the XXVIth International Cosmic Ray Conference in Salt Lake City, which were devoted to issues of origin/composition, acceleration and propagation.

天体物理学 · 物理学 2009-10-31 Matthew G. Baring
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