The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
Nonlinear axion dynamics and the formation of cosmological pseudosolitons
Open accessAbstract
The (3+1)-dimensional evolution of an inhomogeneous axion field configuration around the QCD epoch is studied numerically, including important nonlinear effects due to the attractive self-interaction. It is found that axion perturbations on scales corresponding to causally disconnected regions at $T\ensuremath{\sim}1$ GeV can lead to very dense pseudosoliton configurations we call axitons. These configurations evolve to axion miniclusters with a present density ${\ensuremath{\rho}}_{a}\ensuremath{\gtrsim}{10}^{\ensuremath{-}8}$ g ${\mathrm{cm}}^{\ensuremath{-}3}$. This is high enough for the collisional $2a\ensuremath{\rightarrow}2a$ process to lead to Bose-Einstein relaxation in the gravitationally bound clumps of axions, forming Bose stars.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Dynamics of bubbles in general relativity
Berezin, V. A., Kuzmin, V. A., & Tkachev, I. I. (1987) · Physical Review D · doi:10.1103/physrevd.36.2919 · Cited by 283
Self-citation
Cited by
New experimental approaches in the search for axion-like particles
Irastorza, I. G., & Redondo, J. (2018) · Progress in Particle and Nuclear Physics · doi:10.1016/j.ppnp.2018.05.003 · Cited by 745
The landscape of QCD axion models
Di Luzio, L., Giannotti, M., Nardi, E., & Visinelli, L. (2020) · Physics Reports · doi:10.1016/j.physrep.2020.06.002 · Cited by 657
Raffelt, G. G. (2008) · Lecture Notes in Physics · doi:10.1007/978-3-540-73518-2_3 · Cited by 566
Do dark matter axions form a condensate with long-range correlation?
Guth, A. H., Hertzberg, M. P., & Prescod-Weinstein, C. (2015) · Physical Review D · doi:10.1103/physrevd.92.103513 · Cited by 279
Femtolensing by dark matter revisited
Katz, A., Kopp, J., Sibiryakov, S., & Xue, W. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/12/005 · Cited by 253
Metadata
- Authors
- Kolb, E. W., & Tkachev, I. I.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1994-05-15
- Volume
- 49
- Issue
- 10
- Pages
- 5040-5051
- ISSN
- 0556-2821 (ISSN-L)
- OpenAlex
- W1413354382
- Cited by
- 273
- References
- 1
- FWCI
- 2.55
- Type
- journal article
- Language
- en
- Open access
- green
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
