Introduces Floquet-Bloch theory in azimuth combined with BiGlobal eigenvalue formulation to analyze linear stability of non-axisymmetric convective flows in a rotating baroclinic annulus, identifying cross-modal baroclinic and shear instabilities.
Mayerson, Bart Rip- perda, and Seppe Staelens.A Beginner’s Guide to Black Hole Imaging and Associated Tests of General Rela- tivity, pages 183–237
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A variational latent bottleneck with KL regularization and a dynamic binary mask based on saliency produces model-specific features that keep high accuracy for one classifier but drop others below 2% on CIFAR-100 with over 45x suppression.
Visibility modulations from additional photon rings appear only in spherical boson stars at restricted inclinations, while rotating cases show incomplete rings.
A weighted similarity ensemble unifies user-item and item-item collaborative filtering using shared embeddings to deliver competitive top-N recommendations without extra fine-tuning.
WKB analysis of the Teukolsky equation establishes a quasinormal-mode to greybody-factor correspondence for Kerr black holes that holds in the eikonal limit for gravitational perturbations and matches numerics at high angular momentum.
Longitudinal evaluation over yearly Android app slices shows temporal drift reduces adversarial robustness of malware detectors, with expanding-window retraining providing partial mitigation but not full recovery.
An integrated IoT and CNN system detects cracks in additive manufacturing with 99.54% accuracy and supports predictive maintenance via digital twins.
This conceptual paper identifies shared structures between digital humanism and evolutionary design while highlighting differences in autonomy, subjectivity, and the effects of market-driven specialization.
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Ray tracing ultracompact boson stars: visibility modulations and incomplete photon rings
Visibility modulations from additional photon rings appear only in spherical boson stars at restricted inclinations, while rotating cases show incomplete rings.
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Quasinormal mode/grey-body factor correspondence for Kerr black holes
WKB analysis of the Teukolsky equation establishes a quasinormal-mode to greybody-factor correspondence for Kerr black holes that holds in the eikonal limit for gravitational perturbations and matches numerics at high angular momentum.