The formation of boson stars by gravitational collapse in the early universe is considered. It is demonstrated that while the simplest models are unfavourable for boson star formation, the inclusion of a boson self-interaction and consideration of a boson-antiboson asymmetry allow substantial possibilities for the cosmological formation of boson stars.
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Amer Museum Nat Hist, Dept Astrophys, Cent Pk West & 79th St, New York, NY 10024 USA
CUNY, Lehman Coll, Dept Phys & Astron, Bronx, NY 10468 USA
Ecole Polytech Fed Lausanne EPFL, Inst Phys, Lab Astrophys, Observ Sauverny, CH-1290 Versoix, SwitzerlandAmer Museum Nat Hist, Dept Astrophys, Cent Pk West & 79th St, New York, NY 10024 USA
Chan, James Hung-Hsu
Sibiryakov, Sergey
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McMaster Univ, Dept Phys & Astron, Hamilton, ON L8S 4M1, Canada
Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, CanadaAmer Museum Nat Hist, Dept Astrophys, Cent Pk West & 79th St, New York, NY 10024 USA
Sibiryakov, Sergey
Xue, Wei
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Univ Florida, Dept Phys, Gainesville, FL 32611 USAAmer Museum Nat Hist, Dept Astrophys, Cent Pk West & 79th St, New York, NY 10024 USA
机构:Lanzhou University,Lanzhou Center for Theoretical Physics, Key Laboratory of Theoretical Physics of Gansu Province, School of Physical Science and Technology
Chen Liang
Ji-Rong Ren
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机构:Lanzhou University,Lanzhou Center for Theoretical Physics, Key Laboratory of Theoretical Physics of Gansu Province, School of Physical Science and Technology
Ji-Rong Ren
Shi-Xian Sun
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机构:Lanzhou University,Lanzhou Center for Theoretical Physics, Key Laboratory of Theoretical Physics of Gansu Province, School of Physical Science and Technology
Shi-Xian Sun
Yong-Qiang Wang
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机构:Lanzhou University,Lanzhou Center for Theoretical Physics, Key Laboratory of Theoretical Physics of Gansu Province, School of Physical Science and Technology