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Long Range Forces from the Cosmological Neutrino Background

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arxiv hep-ph/9306222 v1 pith:IVSMVAGW submitted 1993-06-03 hep-ph astro-ph

classification hep-phastro-ph
keywords backgroundforcesneutrinolongrangecosmologicalcomponentsdecreases
verification ladder T0 review T1 audit T2 compute T3 formal

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The cosmological neutrino background will mediate long range forces between objects. For a background of temperature T, the potential decreases as 1/r^5 for r >> 1/T and as 1/r for r << 1/T. These forces have large spin-dependent components. If the neutrino background is nonrelativistic, the long range forces are enhanced by a factor of the inverse neutrino velocity. These long range forces may provide a method for observing the cosmological neutrino background.

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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. Effect of Cosmic Neutrino Background on the Dark Matter Self-interaction via Neutrino force

    hep-ph 2025-09 conditional novelty 5.0 of 10

    The cosmic neutrino background screens the neutrino-pair force between scalar dark matter particles for m_chi below the CnuB temperature, reshaping SIDM parameter space and eliminating Sommerfeld enhancement.

  2. Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials

    gr-qc 2025-05 reject novelty 4.0 of 10

    A heuristic model claims neutrino- and boson-mediated forces would shift black hole photon spheres and shadows, with attractive forces enlarging and repulsive forces shrinking them.

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