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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

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, and in this paper we examine the history of these DS. The power…

宇宙学与河外天体物理 · 物理学 2011-02-11 Douglas Spolyar , Peter Bodenheimer , Katherine Freese , Palo Gondolo

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 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…

Dark Stars (DS) may constitute the first phase of stellar evolution, powered by dark matter (DM) annihilation. We will investigate here the properties of DS assuming the DM particle has the required properties to explain the excess positron…

宇宙学与河外天体物理 · 物理学 2011-06-02 Cosmin Ilie , Katherine Freese , 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 nuclear fusion. Weakly Interacting Massive Particles, which may be their own antipartners, collect inside…

宇宙学与河外天体物理 · 物理学 2014-11-20 Katherine Freese , Cosmin Ilie , Douglas Spolyar , Monica Valluri , Peter Bodenheimer

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

Dark Stars are the very first phase of stellar evolution in the history of the universe: the first stars to form (typically at redshifts $z \sim 10-50$) are powered by heating from dark matter (DM) annihilation instead of fusion (if the DM…

天体物理学 · 物理学 2011-02-11 Katherine Freese , Peter Bodenheimer , Douglas Spolyar , Paolo Gondolo

Dark Stars are stellar objects made (almost entirely) of hydrogen and helium, but powered by the heat from Dark Matter annihilation, rather than by fusion. They are in hydrostatic and thermal equilibrium, but with an unusual power source.…

宇宙学与河外天体物理 · 物理学 2016-08-24 Katherine Freese , Tanja Rindler-Daller , Douglas Spolyar , Monica Valluri

Dark stars (DSs) -- first stars powered by dark-matter (DM) heating rather than fusion -- could form in the early Universe. They can grow to $\gtrsim 10^5 M_{\odot}$ masses and collapse into seeds of supermassive black holes (SMBHs). We…

高能物理 - 唯象学 · 物理学 2025-05-23 Thomas Schwemberger , Volodymyr Takhistov

The first stars in the universe form inside $\sim 10^6 M_\odot$ dark matter (DM) haloes whose initial density profiles are laid down by gravitational collapse in hierarchical structure formation scenarios. During the formation of the first…

天体物理学 · 物理学 2011-02-11 Katherine Freese , Paolo Gondolo , J. A. Sellwood , Douglas Spolyar

The first stars to form in the Universe may be powered by the annihilation of weakly interacting dark matter particles. These so-called dark stars, if observed, may give us a clue about the nature of dark matter. Here we examine which…

宇宙学与河外天体物理 · 物理学 2014-11-20 P. Gondolo , Ji-Haeng Huh , Hyung Do Kim , S. Scopel

Primordial stars formed in the early universe are thought to be hosted by compact dark matter (DM) halos. If DM consists of Weakly Interacting Massive Particles (WIMPs), such stars may be powered by DM annihilation during the early phases…

宇宙学与河外天体物理 · 物理学 2014-02-20 Shingo Hirano , Hideyuki Umeda , 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 Paolo Gondolo , Katherine Freese , Douglas Spolyar , Anthony Aguirre , Peter Bodenheimer , Jeremy A. Sellwood , Naoki Yoshida

The first stars to form in the history of the universe may have been powered by dark matter annihilation rather than by fusion. This new phase of stellar evolution may have lasted millions to billions of years. These dark stars can grow to…

宇宙学与河外天体物理 · 物理学 2010-11-23 K. Freese , E. Ruiz , M. Valluri , C. Ilie , D. Spolyar , P. Bodenheimer

Dark matter (DM) in protostellar halos can dramatically alter the current theoretical framework for the formation of the first stars. Heat from supersymmetric DM annihilation can overwhelm any cooling mechanism, consequently impeding the…

天体物理学 · 物理学 2008-11-26 Katherine Freese , Paolo Gondolo , Douglas Spolyar

Dark matter annihilation might power the first luminous stars in the Universe. These types of stars, known as dark stars, could form in $(10^6\mathrm{-}10^8)\,M_\odot$ protohalos at redshifts $z \sim 20$, and they could be much more…

高能物理 - 唯象学 · 物理学 2022-08-30 Youjia Wu , Sebastian Baum , Katherine Freese , Luca Visinelli , Hai-Bo Yu

(abridged) This comment is intended to show that simulations by Smith et al. (S12) support the Dark Star (DS) scenario and even remove some potential obstacles. Our previous work illustrated that the initial hydrogen densities of the first…

宇宙学与河外天体物理 · 物理学 2013-04-30 Paolo Gondolo , Katherine Freese , Douglas Spolyar , Peter Bodenheimer

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 annihilation of weakly interacting massive particles can provide an important heat source for the first (Pop. III) stars, potentially leading to a new phase of stellar evolution known as a "Dark Star". When dark matter (DM) capture via…

天体物理学 · 物理学 2009-06-23 Katherine Freese , Douglas Spolyar , Anthony Aguirre
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