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In popular cold dark matter cosmological scenarios, stars may have first appeared in significant numbers around a redshift of 10 or so, as the gas within protogalactic halos with virial temperatures in excess of 20,000 K (corresponding to…

天体物理学 · 物理学 2007-05-23 Piero Madau

The first stars in the history of the Universe are likely to form in the dense central regions of 10^5-10^6 Msolar cold dark matter halos at z=10-50. The annihilation of dark matter particles in these environments may lead to the formation…

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

A mechanism of creation of stellar-like objects in the very early universe, from the QCD phase transition till BBN and somewhat later, is studied. It is argued that in the considered process primordial black holes with masses above a few…

宇宙学与河外天体物理 · 物理学 2014-01-15 A. D. Dolgov , S. I. Blinnikov

Massive stars are able to pursue their evolution through the whole sequence of burning phases. They are born hot and luminous, and live a short life before exploding as a supernova or collapsing directly into a black hole. They have a…

太阳与恒星天体物理 · 物理学 2025-02-11 Sylvia Ekström

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

The first stars fundamentally transformed the early universe by emitting the first light and by producing the first heavy elements. These effects were predetermined by the mass distribution of the first stars, which is thought to have been…

宇宙学与河外天体物理 · 物理学 2015-06-03 Takashi Hosokawa , Kazuyuki Omukai , Naoki Yoshida , Harold W. Yorke

If Dark Matter (DM) is composed by Weakly Interacting Massive Particles, its annihilation in the halos harboring the earliest star formation episode may strongly influence the first generation of stars (Population III). Whereas DM…

宇宙学与河外天体物理 · 物理学 2011-03-24 Fabio Iocco

The first generation of stars in the Universe is yet to be observed. There are two leading theories for those objects that mark the beginning of the cosmic dawn: hydrogen burning Population~III stars and Dark Stars, made of hydrogen and…

宇宙学与河外天体物理 · 物理学 2023-08-16 Cosmin Ilie , Jillian Paulin , Katherine Freese

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 earliest stars to form in the Universe were the first sources of light, heat and metals after the Big Bang. The products of their evolution will have had a profound impact on subsequent generations of stars. Recent studies of primordial…

天体物理学 · 物理学 2015-06-24 R. Schneider , A. Ferrara , R. Salvaterra , K. Omukai , V. Bromm

Dark matter in the form of weakly interacting massive particles is predicted to become gravitationally captured and accumulate in stars. While the subsequent annihilations of such particles lead to the injection of energy into stellar…

高能物理 - 唯象学 · 物理学 2014-11-20 Dan Hooper , Douglas Spolyar , Alberto Vallinotto , Nickolay Y. Gnedin

The astronomical dark matter is an essential component of the Universe and yet its nature is still unresolved. It could be made of neutral and massive elementary particles which are their own antimatter partners. These dark matter species…

高能天体物理现象 · 物理学 2015-06-19 Pierre Salati

The first stars are expected to form through molecular-hydrogen (H$_2$) cooling, a channel that is especially sensitive to the thermal and ionization state of gas, and can thus act as a probe of exotic energy injection from decaying or…

宇宙学与河外天体物理 · 物理学 2023-08-28 Wenzer Qin , Julian B. Munoz , Hongwan Liu , Tracy R. Slatyer

If the cosmological dark matter has a component made of small primordial black holes, they may have a significant impact on the physics of the first stars and on the subsequent formation of massive black holes. Primordial black holes would…

天体物理学 · 物理学 2009-10-28 Cosimo Bambi , Douglas Spolyar , Alexander D. Dolgov , Katherine Freese , Marta Volonteri

The first bright objects to form in the Universe might not have been "ordinary" fusion-powered stars, but "Dark Stars" (DSs) powered by the annihilation of dark matter (DM) in the form of Weakly Interacting Massive Particles (WIMPs). If…

宇宙学与河外天体物理 · 物理学 2021-04-07 Tanja Rindler-Daller , Katherine Freese , Richard H. D. Townsend , Luca Visinelli

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 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 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

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