Greybody factors for Proca fields in Schwarzschild spacetime are computed via decoupled master equations, revealing a low-mass regime in even-parity vector mode where transmission exceeds the massless case and lower transmission than massive scalars in the even-parity scalar mode.
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Instabilities in quasinormal modes for noncommutative black holes are methodological artifacts of the WKB approximation rather than physical features.
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Greybody factors of Proca fields in Schwarzschild spacetime: A supplemental analysis based on decoupled master equations related to the Frolov-Krtou\v{s}-Kubiz\v{n}\'ak-Santos separation
Greybody factors for Proca fields in Schwarzschild spacetime are computed via decoupled master equations, revealing a low-mass regime in even-parity vector mode where transmission exceeds the massless case and lower transmission than massive scalars in the even-parity scalar mode.
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Perturbing microscopic black holes inspired by noncommutativity
Instabilities in quasinormal modes for noncommutative black holes are methodological artifacts of the WKB approximation rather than physical features.