Testing Statistical Isotropy on the Sphere with Minkowski Tensors
Stephen Appleby, Changbom Park
astro-ph.CO
Submitted: 2026-07-27
Comments: Comments welcome!
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Is the Observable Universe Consistent with the Cosmological Principle?
- Planck 2018 results. VII. Isotropy and Statistics of the CMB
- A Test of the Cosmological Principle with Quasars
- Power Asymmetry in Cosmic Microwave Background Fluctuations from Full Sky to Sub-degree Scales: Is the Universe Isotropic?
- Cosmic radio dipole from NVSS and WENSS
- Strong Evidence Against a Statistically Isotropic Universe
- How isotropic is dark energy?
- Planck 2018 results. VI. Cosmological parameters
- A large disparity in cosmic reference frames determined from the sky distributions of radio sources and the microwave background radiation
- Integrated perturbation theory for cosmological tensor fields. I. Basic formulation
- Integrated perturbation theory for cosmological tensor fields. II. Loop corrections
- Integrated perturbation theory for cosmological tensor fields. III. Projection effects
- Integrated perturbation theory for cosmological tensor fields. IV. Full-sky formulation
- Information content in anisotropic cosmological fields: Impact of different multipole expansion scheme for galaxy density and ellipticity correlations
- Limits on Primordial Non-Gaussianity from Minkowski Functionals of the WMAP Temperature Anisotropies
- Local analyses of Planck maps with Minkowski Functionals
- On Minkowski Functionals of CMB polarization
- Minkowski Functionals of SDSS-III BOSS : Hints of Possible Anisotropy in the Density Field?
- Betti numbers of Gaussian fields
- Alpha, Betti and the Megaparsec Universe: on the Topology of the Cosmic Web
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