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Related Experiment Video

Updated: Jul 19, 2026

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
06:14

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

Ellipsoidal universe can solve the cosmic microwave background quadrupole problem.

L Campanelli1, P Cea, L Tedesco

  • 1INFN-Sezione di Ferrara, and Dipartimento di Fisica, Università di Ferrara, I-44100 Ferrara, Italy. campanelli@fe.infn.it

Physical Review Letters
|October 10, 2006
PubMed
Summary

The Wilkinson Microwave Anisotropy Probe (WMAP) data reveals a low quadrupole anomaly. A plane-symmetric universe geometry can significantly reduce this anomaly without impacting other cosmic microwave background measurements.

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Area of Science:

  • Cosmology
  • Astrophysics
  • Cosmic Microwave Background Radiation

Background:

  • The Lambda-cold dark matter (ΛCDM) model is the standard cosmological model.
  • Recent Wilkinson Microwave Anisotropy Probe (WMAP) data show a discrepancy in the quadrupole amplitude.
  • This anomaly challenges the predictions of the standard ΛCDM model.

Purpose of the Study:

  • To investigate explanations for the low quadrupole anomaly observed in WMAP data.
  • To explore the impact of non-standard universe geometries on cosmological observables.
  • To reconcile observational data with theoretical predictions.

Main Methods:

  • Analysis of Wilkinson Microwave Anisotropy Probe (WMAP) data.
  • Theoretical modeling of a plane-symmetric universe geometry.
  • Comparison of model predictions with observed angular power spectrum of temperature anisotropy.

Main Results:

  • A plane-symmetric spatial geometry with an eccentricity of approximately 10⁻² at decoupling can significantly reduce the quadrupole amplitude.
  • This modification does not adversely affect higher multipoles in the angular power spectrum.
  • The proposed geometry offers a potential solution to the observed quadrupole anomaly.

Conclusions:

  • The observed low quadrupole anomaly may be explained by a universe with a plane-symmetric geometry.
  • This finding suggests that the large-scale structure of the universe might deviate from perfect isotropy.
  • Further investigation into non-standard cosmological models is warranted.