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相关论文: A smoother end to the dark ages

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Paramount among the processes that ended the cosmic `dark ages' must have been the formation of the first generation of stars (the so-called Population III). We summarize recent progress in constraining its nature, and we discuss the basic…

天体物理学 · 物理学 2009-11-07 Volker Bromm , Paolo S. Coppi , Richard B. Larson

The very first stars to form in the Universe heralded an end to the cosmic dark ages and introduced new physical processes that shaped early cosmic evolution. Until now, it was thought that these stars lived short, solitary lives, with only…

宇宙学与河外天体物理 · 物理学 2015-05-27 Paul C. Clark , Simon C. O. Glover , Rowan J. Smith , Thomas H. Greif , Ralf S. Klessen , Volker Bromm

The universe would have been completely dark between the epoch of recombination and the development of the first non-linear structure. But at redshifts beyond 5 -- perhaps even beyond 20 -- stars formed within `subgalaxies' and created the…

天体物理学 · 物理学 2009-10-31 Martin J. Rees

The emergence of the first black holes during the first billion years of cosmic history marks a key event in cosmology. Their formation is part of the overall process of ending the cosmic dark ages, when the first stars appeared in low-mass…

星系天体物理 · 物理学 2019-07-26 Aaron Smith , Volker Bromm

The first light from stars and quasars ended the ``dark ages'' of the universe and led to the reionization of hydrogen by redshift 7. Current observations are at the threshold of probing this epoch. The study of high-redshift sources is…

天体物理学 · 物理学 2009-10-31 Abraham Loeb , Rennan Barkana

The Dark Age is the period between the time when the cosmic microwave background was emitted and the time when the evolution of structure in the universe led to the gravitational collapse of objects in which the first stars were formed. The…

天体物理学 · 物理学 2009-11-10 Jordi Miralda-Escude

One of the milestones in the cosmic history is the formation of the first luminous objects and Hydrogen reionization. The standard theory of cosmic structure formation predicts that the first generation of stars were born about a few…

宇宙学与河外天体物理 · 物理学 2014-07-02 Aravind Natarajan , Naoki Yoshida

The first phase of stellar evolution in the history of the universe may be Dark Stars, powered by dark matter heating rather than by fusion. Weakly interacting massive particles, which are their own antiparticles, can annihilate and provide…

宇宙学与河外天体物理 · 物理学 2010-02-17 Douglas Spolyar , Katherine Freese , Paolo Gondolo , Anthony Aguirre , Peter Bodenheimer , Jeremy A. Sellwood , Naoki Yoshida

Over the past decade, a consensus picture has emerged in which roughly a quarter of the universe consists of dark matter. The observational evidence for the existence of dark matter is reviewed: rotation curves of galaxies, weak lensing…

天体物理学 · 物理学 2015-05-13 Katherine Freese

The emergence of the first sources of light at redshifts of z ~ 10-30 signaled the transition from the simple initial state of the Universe to one of increasing complexity. We review recent progress in our understanding of the formation of…

宇宙学与河外天体物理 · 物理学 2015-05-27 Torgny Karlsson , Volker Bromm , Joss Bland-Hawthorn

The Cosmic Dark Ages mark a pivotal era of the universe's evolution, transitioning from a neutral, opaque medium to the emergence of the first stars and galaxies that initiated cosmic reionization. This study examines the thermodynamics of…

星系天体物理 · 物理学 2024-12-24 K. El Bourakadi , G. Otalora

Recent observations of hydrogen absorption that occurred when the first stars turned on may give insights into the nature of dark matter.

宇宙学与河外天体物理 · 物理学 2018-08-01 Abraham Loeb , Julian B. Munoz

The first phase of stellar evolution in the history of the universe may be Dark Stars, powered by dark matter heating rather than by fusion. Weakly interacting massive particles, which are their own antiparticles, can annihilate and provide…

The first star clusters and quasars resulted directly from the growth of linear density fluctuations in the early Universe. Since they emerged from a well-defined set of initial conditions, the interplay between observational data from the…

天体物理学 · 物理学 2007-05-23 Abraham Loeb

We have proposed that the first phase of stellar evolution in the history of the Universe may be Dark Stars (DS), powered by dark matter heating rather than by nuclear fusion. Weakly Interacting Massive Particles, which may be their own…

宇宙学与河外天体物理 · 物理学 2014-11-18 Katherine Freese , Douglas Spolyar , Peter Bodenheimer , Paolo Gondolo

A new line of research on Dark Stars is reviewed, which suggests that the first stars to exist in the universe were powered by dark matter heating rather than by fusion. Weakly Interacting Massive Particles, which may be there own…

天体物理学 · 物理学 2015-05-13 Katherine Freese , Peter Bodenheimer , Paolo Gondolo , Douglas Spolyar

The first phase of stellar evolution in the history of the universe may be Dark Stars, powered by dark matter heating rather than by fusion. Weakly interacting massive particles, which are their own antiparticles, can annihilate and provide…

宇宙学与河外天体物理 · 物理学 2010-02-17 Paolo Gondolo , Katherine Freese , Douglas Spolyar , Anthony Aguirre , Peter Bodenheimer , Jeremy A. Sellwood , Naoki Yoshida

One of the next decade's most exciting prospects is to explore the cosmic "dark ages," during which the first stars in the Universe formed, with the 21 cm line of neutral hydrogen. At z>6, this light redshifts into the low-frequency radio…

The earliest generation of stars, far from being a mere novelty, transformed the universe from darkness to light. The first atoms to form after the Big Bang filled the universe with atomic hydrogen and a few light elements. As gravity…

天体物理学 · 物理学 2009-11-11 Rennan Barkana

Observations made using large ground-based and space-borne telescopes have probed cosmic history all the way from the present-day to a time when the Universe was less than a tenth of its present age. Earlier on lies the remaining frontier,…

宇宙学与河外天体物理 · 物理学 2015-05-13 Volker Bromm , Naoki Yoshida , Lars Hernquist , Christopher F. McKee
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