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Fermion absorption cross section of a Schwarzschild black hole

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arxiv gr-qc/0503019 v1 pith:BPDEMGQG submitted 2005-03-04 gr-qc astro-ph

Fermion absorption cross section of a Schwarzschild black hole

classification gr-qc astro-ph
keywords crosssectionparticleabsorptioncouplingsenergiesfindhole
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study the absorption of massive spin-half particles by a small Schwarzschild black hole by numerically solving the single-particle Dirac equation in Painleve-Gullstrand coordinates. We calculate the absorption cross section for a range of gravitational couplings Mm/m_P^2 and incident particle energies E. At high couplings, where the Schwarzschild radius R_S is much greater than the wavelength lambda, we find that the cross section approaches the classical result for a point particle. At intermediate couplings we find oscillations around the classical limit whose precise form depends on the particle mass. These oscillations give quantum violations of the equivalence principle. At high energies the cross section converges on the geometric-optics value of 27 \pi R_S^2/4, and at low energies we find agreement with an approximation derived by Unruh. When the hole is much smaller than the particle wavelength we confirm that the minimum possible cross section approaches \pi R_S^2/2.

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Cited by 3 Pith papers

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

  1. Primordial Black Hole mass growth from neutrinos during the radiation era

    astro-ph.CO 2026-07 conditional novelty 6.0

    PBHs of ~1e3–1e7 solar masses can significantly grow by absorbing neutrinos before matter-radiation equality.

  2. Absorption cross section of a Schwarzschild black hole for a massive vector field

    gr-qc 2026-06 unverdicted novelty 6.0

    Numerical computation of absorption cross sections for massive Proca fields on Schwarzschild black holes, revealing mass-induced longitudinal modes and breaking of even-odd parity degeneracy in transmission spectra.

  3. Primordial Black Hole mass growth from neutrinos during the radiation era

    astro-ph.CO 2026-07 conditional novelty 5.5

    Neutrino absorption lets intermediate-mass and supermassive primordial black holes grow during the radiation era, shifting thermal-history peaks and raising f_PBH.