Related work: continuation of GPGPU
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@ -456,7 +456,7 @@ Publisher: Multidisciplinary Digital Publishing Institute},
urldate = {2025-03-01},
date = {2008-12},
note = {{ISSN}: 2379-5352},
keywords = {Application software, Central Processing Unit, Computer architecture, Computer graphics, Distributed computing, Grid computing, Multicore processing, Pipelines, Programming profession, Rendering (computer graphics)},
keywords = {Computer architecture, Application software, Central Processing Unit, Computer graphics, Distributed computing, Grid computing, Multicore processing, Pipelines, Programming profession, Rendering (computer graphics)},
file = {IEEE Xplore Abstract Record:C\:\\Users\\danwi\\Zotero\\storage\\2FJP9K25\\references.html:text/html},
}
@ -475,3 +475,34 @@ Publisher: Multidisciplinary Digital Publishing Institute},
note = {Conference Name: {IEEE} Transactions on Parallel and Distributed Systems},
file = {IEEE Xplore Abstract Record:C\:\\Users\\danwi\\Zotero\\storage\\5K63T7RB\\5445082.html:text/html},
}
@article{verbraeck_interactive_2021,
title = {Interactive Black-Hole Visualization},
volume = {27},
issn = {1941-0506},
url = {https://ieeexplore.ieee.org/abstract/document/9226126},
doi = {10.1109/TVCG.2020.3030452},
abstract = {We present an efficient algorithm for visualizing the effect of black holes on its distant surroundings as seen from an observer nearby in orbit. Our solution is {GPU}-based and builds upon a two-step approach, where we first derive an adaptive grid to map the 360-view around the observer to the distorted celestial sky, which can be directly reused for different camera orientations. Using a grid, we can rapidly trace rays back to the observer through the distorted spacetime, avoiding the heavy workload of standard tracing solutions at real-time rates. By using a novel interpolation technique we can also simulate an observer path by smoothly transitioning between multiple grids. Our approach accepts real star catalogues and environment maps of the celestial sky and generates the resulting black-hole deformations in real time.},
pages = {796--805},
number = {2},
journaltitle = {{IEEE} Transactions on Visualization and Computer Graphics},
author = {Verbraeck, Annemieke and Eisemann, Elmar},
urldate = {2025-03-02},
date = {2021-02},
note = {Conference Name: {IEEE} Transactions on Visualization and Computer Graphics},
keywords = {Algorithms, Cameras, Computer Graphics Techniques, Distortion, Engineering, Mathematics, Observers, Physical \& Environmental Sciences, Ray tracing, Real-time systems, Rendering (computer graphics), Visualization},
file = {PDF:C\:\\Users\\danwi\\Zotero\\storage\\HDASRGYN\\Verbraeck und Eisemann - 2021 - Interactive Black-Hole Visualization.pdf:application/pdf},
}
@book{hissbach_overview_2022,
title = {An Overview of Techniques for Egocentric Black Hole Visualization and Their Suitability for Planetarium Applications},
isbn = {978-3-03868-189-2},
url = {https://doi.org/10.2312/vmv.20221207},
abstract = {The visualization of black holes is used in science communication to educate people about our universe and concepts of general relativity. Recent visualizations aim to depict black holes in realtime, overcoming the challenge of efficient general relativistic ray tracing. In this state-of-the-art report, we provide the first overview of existing works about egocentric black hole visualization that generate images targeted at general audiences. We focus on Schwarzschild and Kerr black holes and discuss current methods to depict the distortion of background panoramas, point-shaped stars, nearby objects, and accretion disks. Approaches to realtime visualizations are highlighted. Furthermore, we present the implementation of a state-of-the-art black hole visualization in the planetarium software Uniview.},
publisher = {The Eurographics Association},
author = {Hissbach, Anny-Marleen and Dick, Christian and Lawonn, Kai},
urldate = {2025-03-02},
date = {2022},
langid = {english},
file = {Full Text PDF:C\:\\Users\\danwi\\Zotero\\storage\\TBBLEZ5N\\Hissbach et al. - 2022 - An Overview of Techniques for Egocentric Black Hole Visualization and Their Suitability for Planetar.pdf:application/pdf},
}