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Related papers: Dark Matter capture and annihilation on the First …

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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…

Cosmology and Nongalactic Astrophysics · Physics 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…

Astrophysics · Physics 2009-06-23 Katherine Freese , Douglas Spolyar , Anthony Aguirre

We study the evolution of the first stars in the universe (Population III) from the early pre-Main Sequence until the end of helium burning in the presence of WIMP dark matter annihilation inside the stellar structure. The two different…

Astrophysics · Physics 2009-11-13 F. Iocco , A. Bressan , E. Ripamonti , R. Schneider , A. Ferrara , P. Marigo

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…

Astrophysics · Physics 2011-02-11 F. Iocco , A. Bressan , E. Ripamonti , R. Schneider , A. Ferrara , P. Marigo

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…

Astrophysics · Physics 2008-11-26 Katherine Freese , Paolo Gondolo , Douglas Spolyar

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…

Astrophysics · Physics 2009-06-23 Douglas Spolyar , Katherine Freese , Paolo Gondolo

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…

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…

Cosmology and Nongalactic Astrophysics · Physics 2014-02-20 Shingo Hirano , Hideyuki Umeda , 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…

Astrophysics · Physics 2011-02-11 Katherine Freese , Paolo Gondolo , J. A. Sellwood , 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, and in this paper we examine the history of these DS. The power…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-11 Douglas Spolyar , Peter Bodenheimer , Katherine Freese , Palo Gondolo

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…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Rowan J. Smith , Fabio Iocco , Simon C. O. Glover , Dominik R. G. Schleicher , Ralf S. Klessen , Shingo Hirano , Naoki Yoshida

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…

Cosmology and Nongalactic Astrophysics · Physics 2011-03-18 Sofia Sivertsson , Paolo Gondolo

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…

Astrophysics · Physics 2011-02-11 Sung-Chul Yoon , Fabio Iocco , Shizuka Akiyama

We calculate the limits on the fraction of viable dark matter minihalos in the early universe to host Population III.1 stars, surviving today as dark matter spikes in our Milky Way halo. Motivated by potential hints of light dark matter…

Cosmology and Nongalactic Astrophysics · Physics 2013-05-30 Pearl Sandick , Juerg Diemand , Katherine Freese , Douglas Spolyar

Dark Matter (DM) can be trapped by the gravitational field of any star, since collisions with nuclei in dense environments can slow down the DM particle below the escape velocity ($v_{esc}$) at the surface of the star. If captured, the DM…

Cosmology and Nongalactic Astrophysics · Physics 2022-02-16 Cosmin Ilie , Caleb Levy , Jacob Pilawa , Saiyang Zhang

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…

Cosmology and Nongalactic Astrophysics · Physics 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…

Cosmology and Nongalactic Astrophysics · Physics 2010-02-17 Paolo Gondolo , Katherine Freese , Douglas Spolyar , Anthony Aguirre , Peter Bodenheimer , Jeremy A. Sellwood , Naoki Yoshida

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…

Astrophysics · Physics 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…

Cosmology and Nongalactic Astrophysics · Physics 2010-02-17 Douglas Spolyar , Katherine Freese , Paolo Gondolo , Anthony Aguirre , Peter Bodenheimer , Jeremy A. Sellwood , Naoki Yoshida

We show that a star orbiting close enough to an adiabatically grown supermassive black hole can capture a large number of weakly interacting massive particles (WIMPs) during its lifetime. WIMP annihilation energy release in low- to…

Astrophysics · Physics 2007-05-23 I. V. Moskalenko , L. L. Wai
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