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Related papers: Impacts of WIMP dark matter upon stellar evolution…

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In regions of very high dark matter density such as the Galactic centre, the capture and annihilation of WIMP dark matter by stars has the potential to significantly alter their evolution. We describe the dark stellar evolution code…

Astrophysics · Physics 2011-07-19 Pat Scott , Malcolm Fairbairn , Joakim Edsjö

Recent work has indicated that WIMP annihilation in stellar cores has the potential to contribute significantly to a star's total energy production. We report on progress in simulating the effects of WIMP capture and annihilation upon…

Astrophysics · Physics 2017-08-23 Pat Scott , Joakim Edsjö , Malcolm Fairbairn

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

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 modify a stellar structure code to estimate the effect upon the main sequence of the accretion of weakly interacting dark matter onto stars and its subsequent annihilation. The effect upon the stars depends upon whether the energy…

Astrophysics · Physics 2008-11-26 Malcolm Fairbairn , Pat Scott , Joakim Edsjo

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…

Cosmology and Nongalactic Astrophysics · Physics 2010-02-16 E. Ripamonti , F. Iocco , A. Bressan , R. Schneider , A. Ferrara , P. Marigo

The rapid appearance of supermassive black holes (SMBHs) at $z\gtrsim7$ requires efficient pathways to form massive black hole seeds. We investigate whether annihilation of weakly interacting massive particles (WIMPs) can alter primordial…

Astrophysics of Galaxies · Physics 2025-10-02 Konstantinos Topalakis , Devesh Nandal , Jonathan C. Tan

We study the impact of the capture and annihilation of Weakly Interacting Massive Particles (WIMPs) on the evolution of Pop III stars. With a suitable modification of the Geneva stellar evolution code, we study the evolution of 20 and 200…

Astrophysics · Physics 2010-04-15 Marco Taoso , Gianfranco Bertone , Georges Meynet , Sylvia Ekstrom

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 most compelling and popular models for dark matter predict that it should congregate and annihilate in stellar cores. Stars where annihilation contributes substantially to the total energy budget look very different to those with which…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 Pat Scott

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

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

Context: While stars have often been used as laboratories to study dark matter (DM), red giant branch (RGB) stars and all the rich phenomenology they encompass have frequently been overlooked by such endeavors. Aims: We study the capture,…

Solar and Stellar Astrophysics · Physics 2021-07-30 José Lopes , Ilídio Lopes

We announce the public release of the 'dark' stellar evolution code DarkStars. The code simultaneously solves the equations of WIMP capture and annihilation in a star with those of stellar evolution assuming approximate hydrostatic…

Cosmology and Nongalactic Astrophysics · Physics 2016-11-15 Pat Scott , Joakim Edsjö , Malcolm Fairbairn

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

Although dark matter makes up 80% of the gravitational mass of our Galaxy, its composition is not known. One hypothesis is that dark matter consists of massive particles called WIMPs. WIMPs are expected to accumulate and coannihilate in the…

Astrophysics · Physics 2007-11-16 Benjamin Monreal , Lorne A. Nelson , Joseph A. Formaggio

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…

Astrophysics · Physics 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…

Cosmology and Nongalactic Astrophysics · Physics 2011-03-24 Fabio Iocco

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
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