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We study the effects of WIMP dark matter (DM) on the collapse and evolution of the first stars in the Universe. Using a stellar evolution code, we follow the pre-Main Sequence (MS) phase of a grid of metal-free stars with masses in the…

天体物理学 · 物理学 2011-02-11 F. Iocco , A. Bressan , E. Ripamonti , R. Schneider , A. Ferrara , P. Marigo

The first stars to form in the universe may have been dark stars, powered by dark matter annihilation instead of nuclear fusion. The initial amount of dark matter gathered by the star gravitationally can sustain it only for a limited period…

宇宙学与河外天体物理 · 物理学 2011-03-18 Sofia Sivertsson , Paolo Gondolo

Assuming that Dark Matter is dominated by WIMPs, it accretes by gravitational attraction and scattering over baryonic material and annihilates inside celestial objects, giving rise to a "Dark Luminosity" which may potentially affect the…

天体物理学 · 物理学 2010-11-11 Fabio Iocco

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 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

A mechanism is identified whereby dark matter (DM) in protostellar halos dramatically alters the current theoretical framework for the formation of the first stars. Heat from neutralino DM annihilation is shown to overwhelm any cooling…

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

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

Recent theoretical studies have revealed the possibly important role of the capture and annihilation process of weakly interacting massive particles (WIMPs) for the first stars. Using new evolutionary models of metal-free massive stars, we…

天体物理学 · 物理学 2011-02-11 Sung-Chul Yoon , Fabio Iocco , Shizuka Akiyama

We present the first 3D simulations to include the effects of dark matter annihilation feedback during the collapse of primordial mini-halos. We begin our simulations from cosmological initial conditions and account for dark matter…

宇宙学与河外天体物理 · 物理学 2015-06-11 Rowan J. Smith , Fabio Iocco , Simon C. O. Glover , Dominik R. G. Schleicher , Ralf S. Klessen , Shingo Hirano , Naoki Yoshida

The presence of large amounts of WIMP dark matter in stellar cores has been shown to have significant effects upon models of stellar evolution. We present a series of detailed grids of WIMP-influenced stellar models for main sequence stars,…

天体物理学 · 物理学 2010-02-16 Pat Scott , Malcolm Fairbairn , Joakim Edsjö

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

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

We study the effects of WIMP dark matter (DM) annihilations on the thermal and chemical evolution of the gaseous clouds where the first generation of stars in the Universe is formed. We follow the collapse of the gas inside a typical halo…

宇宙学与河外天体物理 · 物理学 2010-02-16 E. Ripamonti , F. Iocco , A. Bressan , R. Schneider , A. Ferrara , P. Marigo

We include an energy term based on Dark Matter (DM) self-annihilation during the cooling and subsequent collapse of the metal-free gas, in halos hosting the formation of the first stars in the Universe. We have found that the feedback…

宇宙学与河外天体物理 · 物理学 2015-05-18 E. Ripamonti , F. Iocco , A. Ferrara , R. Schneider , A. Bressan , P. Marigo

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 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

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

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 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
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