Do dark matter axions form a condensate with long-range correlation?
By A. Guth, M. Hertzberg, C. Prescod-Weinstein. 2014
243 citations recorded by the source corpus.
The authors investigate the formation of Bose-Einstein condensates from axion dark matter, and it is shown that a homogeneous condensate with long range correlations is unstable when $a\phantom{\rule{0}{0ex}}t\phantom{\rule{0}{0ex}}t\phantom{\rule{0}{0ex}}r\phantom{\rule{0}{0ex}}a\phantom{\rule{0}{0ex}}c\phantom{\rule{0}{0ex}}t\phantom{\rule{0}{0ex}}i\phantom{\rule{0}{0ex}}v\phantom{\rule{0}{0ex}}e$ interactions like gravity are taken into account. Instead many Bose-Einstein condensates in form of Bose stars with correlation lengths much below galactic scales are created.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/9c875fc744e12a0c940e6260814c129eb27b94ec
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In Astronomy and Astrophysics
- Paolo Pani
- V. Cardoso
- Jeremiah P. Ostriker
- S. Tremaine
- A. Peter
- L. Hui
- Matthew R. Buckley
- T. Broadhurst
In Nuclear and High Energy Physics
In Statistical and Nonlinear Physics
- Paolo Pani
- S. Tremaine
- T. Broadhurst
- Hsi-Yu Schive
- Tzihong Chiueh
- Kuan-Wei Huang
- V. Cardoso
- A. Peter
Citations in the corpus
- Ultralight scalars as cosmological dark matter (2016, methodology): “The situation is analogous to using the Maxwell equations to describe configurations involving a large number of photons (see [36] for a discussion; see also [37, 38] for the use of the Schrödinger equation in modeling large scale structure).”
- Gravitational probes of dark matter physics (2017, background): “The lack of an axion signal would imply that QCD axions are excluded as dark matter unless the vacuum misalignment angle θ 1 or most axions cluster in Bose stars [184].”
- Theory of dark matter superfluidity (2015, background): “, (5)In the context of QCD axion, it has been argued that Bose-Einstein condensation can occur in galaxies [126, 127], though this has been disputed recently [128].”
- Testing the nature of dark compact objects: a status report (2019, background): “Self-gravitating solutions for the theory above are broadly referred to as boson stars, and can be generalized through the inclusion of nonlinear self-interactions (Kaup 1968; Ruffini and Bonazzola 1969; Khlopov et al. 1985; Seidel and Suen 1991; Guth et al. 2015; Brito et al. 2016a; Minamitsuji 201”
- CONTRASTING GALAXY FORMATION FROM QUANTUM WAVE DARK MATTER, ψDM, WITH ΛCDM, USING PLANCK AND HUBBLE DATA (2015, background): “They are non-thermally generated and can be described by a single coherent wave function (Turner 1983; Goodman 2000; Böhmer & Harko 2007; Sikivie & Yang 2009; Davidson 2015; Guth et al. 2015).”