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相关论文: From Darkness To Light: The First Stars in the Uni…

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The first stars to form in the Universe -- the so-called Population III stars -- bring an end to the cosmological Dark Ages, and exert an important influence on the formation of subsequent generations of stars and on the assembly of the…

宇宙学与河外天体物理 · 物理学 2015-06-11 Simon C. O. Glover

The cosmic dark ages are the mysterious epoch during which the pristine gas began to condense and ultimately form the first stars. Although these beginnings have long been a topic of theoretical interest, technology has only recently…

How and when did the first generation of stars form at the end of the cosmic dark ages? Quite generically, within variants of the cold dark matter model of cosmological structure formation, the first sources of light are expected to form in…

天体物理学 · 物理学 2009-11-11 Volker Bromm

The first stars in the universe are thought to be massive, forming in dark matter halos with masses around 10^6 solar masses. Recent simulations suggest that these metal-free (Population III) stars may form in binary or multiple systems.…

宇宙学与河外天体物理 · 物理学 2012-06-21 John H. Wise

We review recent theoretical results on the formation of the first stars in the universe, and emphasize related open questions. In particular, we discuss the initial conditions for Population III star formation, as given by variants of the…

天体物理学 · 物理学 2008-11-26 Volker Bromm , Richard B. Larson

From studying the cosmic microwave background, we know our Universe started out very simple. It was by and large homogeneous and isotropic, with small fluctuations that can be described by linear perturbation theory. In stark contrast, the…

星系天体物理 · 物理学 2020-01-22 Ralf S. Klessen

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…

Population III (or Pop. III) stars, the first stellar generation built up from metal-free primordial gas, first started to form at redshifts z ~ 30. They formed primarily in small dark matter halos with masses of a few million solar masses.…

太阳与恒星天体物理 · 物理学 2025-09-19 Simon C. O. Glover , Ralf S. Klessen

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

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

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

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

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

The first generation of stars, often called Population III (or Pop III), form from metal-free primordial gas at redshifts 30 and below. They dominate the cosmic star formation history until redshifts 15 to 20, at which point the formation…

宇宙学与河外天体物理 · 物理学 2023-04-06 Ralf S. Klessen , Simon C. O. Glover

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

Modern cosmological simulations predict that the first generation of stars formed with a mass scale around 100 solar masses about 300-400 million years after the Big Bang. When the first stars reached the end of their lives, many of them…

高能天体物理现象 · 物理学 2014-07-30 Ke-Jung Chen

The formation of the first generations of stars at redshifts z > 15-20 signaled the transition from the simple initial state of the universe to one of increasing complexity. We here review recent progress in understanding the assembly…

天体物理学 · 物理学 2009-11-13 Jarrett L. Johnson , Thomas H. Greif , Volker Bromm

The first stars ended the cosmic Dark Ages and created the first heavy elements necessary for the formation of planets and life. The properties of these stars remain uncertain, and it may be decades before individual Pop III stars are…

宇宙学与河外天体物理 · 物理学 2015-06-11 Daniel J. Whalen , Chris L. Fryer , Daniel E. Holz , Alexander Heger , S. E. Woosley , Massimo Stiavelli , Wesley Even , Lucille L. Frey

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 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
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