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Dark stars: a review
Stockholms universitet, Nordiska institutet för teoretisk fysik (Nordita). Stockholms universitet, Naturvetenskapliga fakulteten, Fysikum. Stockholms universitet, Naturvetenskapliga fakulteten, Oskar Klein-centrum för kosmopartikelfysik (OKC). University of Michigan, USA.
Stockholms universitet, Naturvetenskapliga fakulteten, Fysikum. Stockholms universitet, Naturvetenskapliga fakulteten, Oskar Klein-centrum för kosmopartikelfysik (OKC).
Antal upphovsmän: 42016 (Engelska)Ingår i: Reports on progress in physics (Print), ISSN 0034-4885, E-ISSN 1361-6633, Vol. 79, nr 6, artikel-id 066902Artikel i tidskrift (Refereegranskat) Published
Abstract [en]

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. Weakly interacting massive particles (WIMPs), among the best candidates for dark matter, can be their own antimatter and can annihilate inside the star, thereby providing a heat source. Although dark matter constitutes only <= 0.1% of the stellar mass, this amount is sufficient to power the star for millions to billions of years. Thus, the first phase of stellar evolution in the history of the Universe may have been dark stars. We review how dark stars come into existence, how they grow as long as dark matter fuel persists, and their stellar structure and evolution. The studies were done in two different ways, first assuming polytropic interiors and more recently using the MESA stellar evolution code; the basic results are the same. Dark stars are giant, puffy (similar to 10 AU) and cool (surface temperatures similar to 10 000 K) objects. We follow the evolution of dark stars from their inception at similar to 1M(circle dot) as they accrete mass from their surroundings to become supermassive stars, some even reaching masses >10(6)M(circle dot) and luminosities >10(10)L(circle dot), making them detectable with the upcoming James Webb Space Telescope. Once the dark matter runs out and the dark star dies, it may collapse to a black hole; thus dark stars may provide seeds for the supermassive black holes observed throughout the Universe and at early times. Other sites for dark star formation may exist in the Universe today in regions of high dark matter density such as the centers of galaxies. The current review briefly discusses dark stars existing today, but focuses on the early generation of dark stars.

Ort, förlag, år, upplaga, sidor
2016. Vol. 79, nr 6, artikel-id 066902
Nyckelord [en]
astroparticle physics, dark matter, first stars, cosmology
Nationell ämneskategori
Fysik
Identifikatorer
URN: urn:nbn:se:su:diva-135072DOI: 10.1088/0034-4885/79/6/066902ISI: 000383955500010PubMedID: 27214049OAI: oai:DiVA.org:su-135072DiVA, id: diva2:1050340
Tillgänglig från: 2016-11-28 Skapad: 2016-10-31 Senast uppdaterad: 2018-08-07Bibliografiskt granskad

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Freese, KatherineSpolyar, Douglas
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Nordiska institutet för teoretisk fysik (Nordita)FysikumOskar Klein-centrum för kosmopartikelfysik (OKC)
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