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Gravitational Bose-Einstein Condensation in the Kinetic Regime. / Levkov, D. G.; Panin, A. G.; Tkachev, I. I.

In: Physical Review Letters, Vol. 121, No. 15, 151301, 12.10.2018.

Research output: Contribution to journalArticlepeer-review

Harvard

Levkov, DG, Panin, AG & Tkachev, II 2018, 'Gravitational Bose-Einstein Condensation in the Kinetic Regime', Physical Review Letters, vol. 121, no. 15, 151301. https://doi.org/10.1103/PhysRevLett.121.151301

APA

Vancouver

Levkov DG, Panin AG, Tkachev II. Gravitational Bose-Einstein Condensation in the Kinetic Regime. Physical Review Letters. 2018 Oct 12;121(15):151301. doi: 10.1103/PhysRevLett.121.151301

Author

Levkov, D. G. ; Panin, A. G. ; Tkachev, I. I. / Gravitational Bose-Einstein Condensation in the Kinetic Regime. In: Physical Review Letters. 2018 ; Vol. 121, No. 15.

BibTeX

@article{8692e2fe9ab94024a5b22e380cb803b3,
title = "Gravitational Bose-Einstein Condensation in the Kinetic Regime",
abstract = "We study Bose-Einstein condensation and the formation of Bose stars in virialized dark matter halos and miniclusters by universal gravitational interactions. We prove that this phenomenon does occur and it is described by a kinetic equation. We give an expression for the condensation time. Our results suggest that Bose stars may form kinetically in mainstream dark matter models such as invisible QCD axions and fuzzy dark matter.",
keywords = "AXION MINICLUSTERS, STARS",
author = "Levkov, {D. G.} and Panin, {A. G.} and Tkachev, {I. I.}",
year = "2018",
month = oct,
day = "12",
doi = "10.1103/PhysRevLett.121.151301",
language = "English",
volume = "121",
journal = "Physical Review Letters",
issn = "0031-9007",
publisher = "American Physical Society",
number = "15",

}

RIS

TY - JOUR

T1 - Gravitational Bose-Einstein Condensation in the Kinetic Regime

AU - Levkov, D. G.

AU - Panin, A. G.

AU - Tkachev, I. I.

PY - 2018/10/12

Y1 - 2018/10/12

N2 - We study Bose-Einstein condensation and the formation of Bose stars in virialized dark matter halos and miniclusters by universal gravitational interactions. We prove that this phenomenon does occur and it is described by a kinetic equation. We give an expression for the condensation time. Our results suggest that Bose stars may form kinetically in mainstream dark matter models such as invisible QCD axions and fuzzy dark matter.

AB - We study Bose-Einstein condensation and the formation of Bose stars in virialized dark matter halos and miniclusters by universal gravitational interactions. We prove that this phenomenon does occur and it is described by a kinetic equation. We give an expression for the condensation time. Our results suggest that Bose stars may form kinetically in mainstream dark matter models such as invisible QCD axions and fuzzy dark matter.

KW - AXION MINICLUSTERS

KW - STARS

UR - http://www.scopus.com/inward/record.url?scp=85054850811&partnerID=8YFLogxK

U2 - 10.1103/PhysRevLett.121.151301

DO - 10.1103/PhysRevLett.121.151301

M3 - Article

C2 - 30362790

AN - SCOPUS:85054850811

VL - 121

JO - Physical Review Letters

JF - Physical Review Letters

SN - 0031-9007

IS - 15

M1 - 151301

ER -

ID: 17118745