Post-Newtonian effective theory breaks down in generic many-body relativistic dynamics despite small local potentials and velocities, due to sensitivity from absent conserved charges and non-integrability, supplying a criterion for reliable weak-field mass inference relevant to the dark matter
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Greybody lower bounds and absorption cross sections for massless fields of spins 0, 1, and 1/2 are computed in the Euler-Heisenberg black hole with perfect fluid dark matter, revealing monotonic increases with frequency and parameter-dependent deformations of the spectra.
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When Weak Fields Arent Weak: Post-Newtonian effective theory and the Dark Matter Puzzle
Post-Newtonian effective theory breaks down in generic many-body relativistic dynamics despite small local potentials and velocities, due to sensitivity from absent conserved charges and non-integrability, supplying a criterion for reliable weak-field mass inference relevant to the dark matter
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Perturbations and greybody bounds of Euler-Heisenberg black holes surrounded by perfect fluid dark matter
Greybody lower bounds and absorption cross sections for massless fields of spins 0, 1, and 1/2 are computed in the Euler-Heisenberg black hole with perfect fluid dark matter, revealing monotonic increases with frequency and parameter-dependent deformations of the spectra.