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Maxwell's Multipole Vectors and the CMB

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arxiv astro-ph/0412231 v2 pith:DEEE4FUR submitted 2004-12-09 astro-ph

classification astro-ph
keywords vectorsalgorithmalignmentmaxwellmultipoleapproacharticlebetter
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The recently re-discovered multipole vector approach to understanding the harmonic decomposition of the cosmic microwave background traces its roots to Maxwell's Treatise on Electricity and Magnetism. Taking Maxwell's directional derivative approach as a starting point, the present article develops a fast algorithm for computing multipole vectors, with an exposition that is both simpler and better motivated than in the author's previous work. Tests show the resulting algorithm, coded up as a Mathematica notebook, to be both fast and robust. This article serves to announce the free availability of the code. The algorithm is then applied to the much discussed anomalies in the low-ell CMB modes, with sobering results. Simulations show the quadrupole-octopole alignment to be unusual at the 98.7% level, corroborating earlier estimates of a 1-in-60 alignment while showing recent reports of 1-in-1000 (using non-unit-length normal vectors) to have unintentionally relied on the near orthogonality of the quadrupole vectors in one particular data set. The alignment of the quadrupole and octopole vectors with the ecliptic plane is confirmed at better than the 2sigma level.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Cosmic Multipoles in Galaxy Surveys Part I: How Inferences Depend on Source Counts and Masks

    astro-ph.CO 2024-12 conditional novelty 5.0 of 10

    A simulation study shows that a traceless tensor, Bayesian fitting approach recovers galaxy-count dipole, quadrupole, and octupole signals on masked skies once source counts exceed about 500,000.

  2. Fr\'echet Vectors as sensitive tools for blind tests of CMB anomalies

    astro-ph.CO 2024-11 conditional novelty 5.0 of 10

    Fréchet Vectors, built from Multipole Vectors, are more sensitive to CMB anisotropies, and Planck 2018 temperature maps show small tensions with a Gaussian and statistically isotropic sky.

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