Auswahl der wissenschaftlichen Literatur zum Thema „Hole dynamics“
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Zeitschriftenartikel zum Thema "Hole dynamics"
Hu, Xinyu, Yingjie Wei, Cong Wang, Guilin Wang und Yulin Wang. „Cavity dynamics of the projectile passing through the ice hole“. Journal of Applied Physics 133, Nr. 11 (21.03.2023): 114702. http://dx.doi.org/10.1063/5.0142204.
Der volle Inhalt der QuelleEliasson, B., und P. K. Shukla. „The dynamics of electron and ion holes in a collisionless plasma“. Nonlinear Processes in Geophysics 12, Nr. 2 (11.02.2005): 269–89. http://dx.doi.org/10.5194/npg-12-269-2005.
Der volle Inhalt der QuelleAntil, Pearl, und Amita Malik. „Hole Detection for Quantifying Connectivity in Wireless Sensor Networks: A Survey“. Journal of Computer Networks and Communications 2014 (2014): 1–11. http://dx.doi.org/10.1155/2014/969501.
Der volle Inhalt der QuelleKhan, Muhammad Atif, Farhad Ali, Nahid Fatima und Mohamed Abd El-Moneam. „Particles Dynamics in Schwarzschild like Black Hole with Time Contracting Horizon“. Axioms 12, Nr. 1 (27.12.2022): 34. http://dx.doi.org/10.3390/axioms12010034.
Der volle Inhalt der QuelleHutchinson, I. H. „Ion hole equilibrium and dynamics in one dimension“. Physics of Plasmas 30, Nr. 3 (März 2023): 032107. http://dx.doi.org/10.1063/5.0142790.
Der volle Inhalt der QuelleXu, J. H., C. S. Ting und T. K. Lee. „Hole dynamics and effective hole-hole interaction in a quantum antiferromagnet“. Physical Review B 43, Nr. 10 (01.04.1991): 8733–36. http://dx.doi.org/10.1103/physrevb.43.8733.
Der volle Inhalt der QuelleZhang, Baocheng. „Thermodynamics of Acoustic Black Holes in Two Dimensions“. Advances in High Energy Physics 2016 (2016): 1–8. http://dx.doi.org/10.1155/2016/5710625.
Der volle Inhalt der QuelleCorman, Maxence, William E. East und Justin L. Ripley. „Evolution of black holes through a nonsingular cosmological bounce“. Journal of Cosmology and Astroparticle Physics 2022, Nr. 09 (01.09.2022): 063. http://dx.doi.org/10.1088/1475-7516/2022/09/063.
Der volle Inhalt der QuelleRayimbaev, Javlon, Nozima Juraeva, Malika Khudoyberdiyeva, Ahmadjon Abdujabbarov und Mardon Abdullaev. „Quasiperiodic Oscillations and Dynamics of Test Particles around Regular-Kiselev Black Holes“. Galaxies 11, Nr. 6 (16.11.2023): 113. http://dx.doi.org/10.3390/galaxies11060113.
Der volle Inhalt der QuelleAKHMEDOV, E. T. „BLACK HOLE THERMODYNAMICS FROM THE POINT OF VIEW OF SUPERSTRING THEORY“. International Journal of Modern Physics A 15, Nr. 01 (10.01.2000): 1–44. http://dx.doi.org/10.1142/s0217751x00000021.
Der volle Inhalt der QuelleDissertationen zum Thema "Hole dynamics"
Chung, Hyeyoun. „Exploring Black Hole Dynamics“. Thesis, Harvard University, 2014. http://nrs.harvard.edu/urn-3:HUL.InstRepos:14226081.
Der volle Inhalt der QuelleVaziri, Goudarzi Hamed. „Hole Dynamics in Films“. Electronic Thesis or Diss., Sorbonne université, 2023. http://www.theses.fr/2023SORUS640.
Der volle Inhalt der QuelleOceanic film bursting is a phenomenon in which a thin liquid film representing the cap of the bubble bursts at the surface of the ocean, producing film drops. The film bursting phenomenon is critical in ocean-atmosphere exchanges, particularly in transferring heat, mass, and momentum between the ocean and the atmosphere. The film bursting phenomenon comprises a series of complex dynamics, such as drainage, puncture, film retraction, and film disintegration into film drops. The hole healing (i.e., when a hole is too small and is closed after its nucleation) is a critical parameter that could impact the film bursting dynamics, particularly the film thickness at bursting and, thus, the liquid budget for the film drop production. The present work investigates the dynamics of holes in free liquid films, presenting a comprehensive understanding of the hole-healing phenomenon while focusing on the film bursting in the oceanic context. This was achieved through a combination of numerical simulations and analytical approaches. The numerical simulations were carried out using Basilisk. This robust and efficient two-phase flow solver is based on a Volume-of-Fluid (VoF) method and written using the C-programming language. The underlying mechanism for the hole-healing phenomenon was studied in detail. The dichotomy simulations for the determination of the healing threshold carried out in this work have used high-resolution mesh refinement. This was possible by using an adaptive mesh scheme provided by Basilisk. The analytical approaches were used to develop hypotheses to predict the healing threshold of a hole on a film, which were tested against numerical results. The critical dynamics of the hole are examined, and distinct power laws were identified for the tip curvature to illustrate the driving mechanism. The variations in the hole healing threshold with other problem parameters were examined. This study was first carried out for a flat film, discovering that the healing threshold is increased by increasing the film Laplace number. This effect was pronounced for values ranging from 1 to 10000, coinciding with the customary range of film Laplace numbers observed for oceanic bursting bubbles. The observed effects were also elaborated upon, along with physical explanations. Since the exact initial shape of the hole was shown to influence the healing threshold, an examination was carried out to study this effect on the consistency of the results from changing the film Laplace number, taken as an example for the other. It was shown that despite variations in the threshold for different shapes, the effect of changing the film Laplace number was independent of the hole shape. Therefore, the dichotomy results were shown to be independent of the arbitrary choice of the hole shape throughout the study. A similar study was carried out for a hole in a bubble cap after a detailed study of the bubble and gas outflow dynamics. It was discovered that the gas outflow undergoes a Venturi effect, where a stronger outflow, resulting from smaller bubble sizes or higher gas Laplace numbers, was shown to increase the healing threshold. A hypothesis was developed to predict the Venturi effect on the healing threshold, resulting in a Venturi correction term that predicted a power law dependency on the bubble diameter, which agreed with the numerical results. The Venturi effect was significant for high values of the gas Laplace number, where the healing threshold was doubled by increasing the film mean curvature from a flat film to a bubble cap with a size 20 times the bubble cap thickness. These findings provide a comprehensive understanding of the hole-healing phenomenon, particularly in oceanic film bursting. The present work also offers a foundation for future studies on the film-bursting phenomenon involving complex dynamics, including hole healing
Licht, David. „Effective Dynamics of Black Hole Horizons“. Doctoral thesis, Universitat de Barcelona, 2021. http://hdl.handle.net/10803/671802.
Der volle Inhalt der QuelleEn esta tesis hemos presentado un nuevo aspecto perteneciente a la teoría efectiva de la relatividad general en el límite de un gran número de dimensiones. Hemos demostrado que la teoría desarrollada inicialmente para capturar la física de las branas asintóticamente planas también contiene una nueva familia de soluciones localizadas que pueden ser identificadas con agujeros negros de dimensiones más altas como los agujeros negros de Schwarzschild- Thangerlini o de Myers-Perry en el límite de gran D. Usando esta técnica hemos explorado varios aspectos nuevos de dichos agujeros negros. Encontramos una nueva clase de soluciones de barras negras giratorias, que aparecen como objetos estacionarios en la teoría efectiva Describimos un método que permite construir soluciones cargadas a partir de cada solución no cargada. Usando este método construimos agujeros negros cargados y giratorios en la teoría de Einstein-Maxwell. Estudiamos la evolución de las colisiones de agujeros negros en dimensiones superiores usando las ecuaciones efectivas. Demostramos que en estas colisiones es posible formar agujeros negros con horizontes alargados como barras negras o con forma de mancuernas. Con un momento angular lo suficientemente alto, las barras negras pueden ser tan alargadas que son susceptibles a una inestabilidad tipo Greggory-Laflamme, que lleva a una rotura del horizonte y a una singularidad desnuda. Por consiguiente, esto demuestra un ejemplo novedoso de una violación de la hipótesis de 'cosmic censorship' (censura cósmica). Además estudiamos la evolución y el decaimiento de los agujeros negros MP ultraspinning, y observamos una estructura notablemente rica en los estados intermedios del decaimiento.
Pacilio, Costantino. „Classical and quantum aspects of black hole dynamics“. Master's thesis, Alma Mater Studiorum - Università di Bologna, 2014. http://amslaurea.unibo.it/7532/.
Der volle Inhalt der QuelleWang, Xiaoya. „Theory of heavy-hole spin-echo dynamics“. Thesis, McGill University, 2014. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=123115.
Der volle Inhalt der QuelleDans ce mémoire, nous étudions les effets de l'interaction hyperfine sur l'écho de spin d'un trou lourd localisé dans une boîte quantique. Nous considérons l'application d'un champ magnétique perpendiculaire aux fluctuations causéespar l'interaction hyperfine, qui entraîne le système dans un régime de moyenne motionnelle lorsque l'énergie Zeeman pertinente (du trou ou des noyaux nucléaires) dépasse l'amplitude des fluctuations dans le champ de Overhauser. Avec les paramètres utilisés dans la Réf. [1], le régime de moyenne motionnelle est atteint pour un champ magnétique de l'ordre de 1 T. Dans ce régime, la précession rapide du spin autour du champ magnétique externe a l'effet d'une moyenne sur les fluctuations hyperfines, ce qui permet la suppression complète de la décroissance de l'enveloppe du signal de l'écho de spin. Nous prédisons aussi une anisotropie présente dans la dynamique de cohérence qui serait pertinente à la discussion des fluctuations du champ électrique, fluctuations qui limitent les temps de cohérence dans des expériences actuelles[2, 3]. Plus précisément, nous trouvons des directions d'initialisation et de rotation qui repoussent les effets des fluctuations électriques jusqu'à des échelles de temps de l'ordre de plusieurs secondes pour des paramètres expérimentaux typiques[2]. L'anisotropie du système est également responsable d'un comportement inattendu de la pureté du spin, qui quantifie la polarisation restante du qubit de spin suivant l'enchevêtrement avec un environnement pendant un temps t. Nous montrons que la pureté du spin est préservée au maximum pour une initialisation parallèle aux fluctuations hyperfines, dans une superposition d'états propres Zeeman. Ces résultats fournissent une preuve supplémentaire du potentiel des qubits de spin de trou lourd, et permettent de prolonger leur cohérence en optimisant la géométrie du système.
Cáceres, Alejandro. „Electron dynamics in a black hole background“. Thesis, University of Cambridge, 2005. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.614691.
Der volle Inhalt der QuelleBrunner und Michael. „Single hole dynamics in the t-J model“. Phd thesis, Universitaet Stuttgart, 2000. http://elib.uni-stuttgart.de/opus/volltexte/2000/597/index.html.
Der volle Inhalt der QuelleDe, Villiers Jean-Pierre. „Dynamics of cosmic strings in black hole spacetimes“. Thesis, National Library of Canada = Bibliothèque nationale du Canada, 1998. http://www.collectionscanada.ca/obj/s4/f2/dsk2/tape15/PQDD_0012/NQ34754.pdf.
Der volle Inhalt der QuelleZiogas, Vaios. „Transport at strong coupling and black hole dynamics“. Thesis, Durham University, 2018. http://etheses.dur.ac.uk/12683/.
Der volle Inhalt der QuelleBrunner, Michael. „Single hole dynamics in the t-J model“. [S.l.] : Universität Stuttgart , Fakultät Physik, 2000. http://www.bsz-bw.de/cgi-bin/xvms.cgi?SWB8473264.
Der volle Inhalt der QuelleBücher zum Thema "Hole dynamics"
Winter Workshop on Nuclear Dynamics (8th 1992 Jackson Hole, Wyo.). Advances in nuclear dynamics: Proceedings of the 8th Winter Workshop on Nuclear Dynamics, Jackson Hole, Wyoming, USA, 18-25 January 1992. Herausgegeben von Bauer W. 1959- und Back B. Singapore: World Scientific, 1992.
Den vollen Inhalt der Quelle findenUnited States. National Aeronautics and Space Administration., Hrsg. Numerical simulation of receptivity and transition in a boundary layer on a flat plate with a suction hole. Tucson, Ariz: Engineering Experiment Station College of Engineering and Mines, University of Arizona, 1994.
Den vollen Inhalt der Quelle findenUnited States. National Aeronautics and Space Administration., Hrsg. Numerical simulation of receptivity and transition in a boundary layer on a flat plate with a suction hole. Tucson, Ariz: Engineering Experiment Station College of Engineering and Mines, University of Arizona, 1994.
Den vollen Inhalt der Quelle findenTexas A & M University. Turbomachinery Laboratories. und United States. National Aeronautics and Space Administration., Hrsg. SSME seal test program: Test results for hole-pattern damper seals : interim progress report. College Station, Texas: Turbomachinery Laboratories, Mechanical Engineering Department, Texas A&M University, 1985.
Den vollen Inhalt der Quelle findenChilds, Dara W. SSME seal test program: Test results for smooth, hole-pattern, and helically grooved stators : interim progress report. College Station, Tex: Texas A&M, Turbomachinery Laboratories, Mechanical Engineering Dept., 1987.
Den vollen Inhalt der Quelle findenSerebryakov, Andrey, und Gennadiy Zhuravlev. Exploitation of oil and gas fields by horizontal wells. ru: INFRA-M Academic Publishing LLC., 2021. http://dx.doi.org/10.12737/971768.
Der volle Inhalt der QuelleAretakis, Stefanos. Dynamics of Extremal Black Holes. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-95183-6.
Der volle Inhalt der QuelleHemsendorf, Marc. Dynamics of black holes in galactic centres. Aachen: Shaker, 2000.
Den vollen Inhalt der Quelle finden1951-, McConnell C. Douglas, Hrsg. The Holy Spirit and mission dynamics. Pasadena, Calif: William Carey Library, 1997.
Den vollen Inhalt der Quelle findenBallhaus, W. F. Advances in Fluid Dynamics: Proceedings of the Symposium in Honor of Maurice Holt on His 70th Birthday. New York, NY: Springer New York, 1989.
Den vollen Inhalt der Quelle findenBuchteile zum Thema "Hole dynamics"
Aarseth, Sverre J. „Black Hole Binary Dynamics“. In Fred Hoyle’s Universe, 87–92. Dordrecht: Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-1605-5_12.
Der volle Inhalt der QuelleLaguna, Pablo, und Deirdre M. Shoemaker. „9 Computational Black Hole Dynamics“. In The Physics of the Early Universe, 277–98. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-31535-3_9.
Der volle Inhalt der QuelleIsrael, Werner. „Thermodynamics and Internal Dynamics of Black Holes: Some Recent Developments“. In Black Hole Physics, 147–83. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2420-1_4.
Der volle Inhalt der QuelleLarson, Richard B. „Black-Hole Remnants in Globular Clusters“. In Dynamics of Star Clusters, 421–22. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_48.
Der volle Inhalt der QuelleBrunner, Michael, Catia Lavalle, Sylvain Capponi, Martin Feldbacher, Fakher F. Assaad und Alejandro Muramatsu. „Single Hole Dynamics in Correlated Insulators“. In High Performance Computing in Science and Engineering ’01, 145–56. Berlin, Heidelberg: Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-642-56034-7_13.
Der volle Inhalt der QuelleDuncan, Martin J. „Can a Moderately Massive Black Hole Reverse Core Collapse?“ In Dynamics of Star Clusters, 415–17. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_46.
Der volle Inhalt der QuelleAretakis, Stefanos. „Introduction to General Relativity and Black Hole Dynamics“. In Dynamics of Extremal Black Holes, 3–36. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-95183-6_1.
Der volle Inhalt der QuelleAli Alpar, M. „Superfluid Dynamics and Energy Dissipation in Neutron Stars“. In The Neutron Star—Black Hole Connection, 57–70. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0548-7_4.
Der volle Inhalt der QuelleNewman, Paul A. „Chemistry and dynamics of the Antarctic Ozone Hole“. In The Stratosphere: Dynamics, Transport, and Chemistry, 157–71. Washington, D. C.: American Geophysical Union, 2010. http://dx.doi.org/10.1029/2009gm000873.
Der volle Inhalt der QuelleBrügmann, Bernd, Ulrich Sperhake, Doreen Müller, Roman Gold, Pablo Galaviz, Nobert Lages und Marcus Thierfelder. „Project h1021: Dynamics of Binary Black Hole Systems“. In High Performance Computing in Science and Engineering, Garching/Munich 2009, 395–407. Berlin, Heidelberg: Springer Berlin Heidelberg, 2010. http://dx.doi.org/10.1007/978-3-642-13872-0_33.
Der volle Inhalt der QuelleKonferenzberichte zum Thema "Hole dynamics"
KOLOMEITSEV, E. E., und D. N. VOSKRESENSKY. „PARTICLE–HOLE DYNAMICS“. In Proceedings of the Conference “Kadanoff-Baym Equations: Progress and Perspectives for Many-Body Physics”. WORLD SCIENTIFIC, 2000. http://dx.doi.org/10.1142/9789812793812_0025.
Der volle Inhalt der QuelleCornean, Horia, Sergey Sorokin und Benjamin Støttrup. „ACOUSTIC BLACK HOLE PROFILE OPTIMIZATION“. In XI International Conference on Structural Dynamics. Athens: EASD, 2020. http://dx.doi.org/10.47964/1120.9202.20000.
Der volle Inhalt der QuellePrüll, Alexander. „Hole burning: A discrete kinetic approach“. In RAREFIED GAS DYNAMICS: 22nd International Symposium. AIP, 2001. http://dx.doi.org/10.1063/1.1407543.
Der volle Inhalt der QuelleKawamura, J. „NMR Hole-Burning Experiments on Superionic Conductor Glasses“. In SLOW DYNAMICS IN COMPLEX SYSTEMS: 3rd International Symposium on Slow Dynamics in Complex Systems. AIP, 2004. http://dx.doi.org/10.1063/1.1764268.
Der volle Inhalt der QuelleOhno, M., und W. von Niessen. „Dynamics of valence hole excitations in adsorbates“. In Synchrotron radiation and dynamic phenomena. AIP, 1992. http://dx.doi.org/10.1063/1.42530.
Der volle Inhalt der QuelleOhno, M., und P. Decleva. „Dynamics of core hole excitations in adsorbates“. In Synchrotron radiation and dynamic phenomena. AIP, 1992. http://dx.doi.org/10.1063/1.42534.
Der volle Inhalt der QuelleNoack, Ralph. „A Direct Cut Approach for Overset Hole Cutting“. In 18th AIAA Computational Fluid Dynamics Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2007. http://dx.doi.org/10.2514/6.2007-3835.
Der volle Inhalt der QuelleKugler, M., T. Korn, M. Hirmer, D. Schuh, W. Wegscheider, C. Schüller, Jisoon Ihm und Hyeonsik Cheong. „Controlling hole spin dynamics in two-dimensional hole systems at low temperatures“. In PHYSICS OF SEMICONDUCTORS: 30th International Conference on the Physics of Semiconductors. AIP, 2011. http://dx.doi.org/10.1063/1.3666584.
Der volle Inhalt der QuelleAttenberger, T., und U. Bogner. „Crystalline Model Systems Probing Dynamics and Electric-Field Effects“. In Persistent Spectral Hole Burning: Science and Applications. Washington, D.C.: Optica Publishing Group, 1991. http://dx.doi.org/10.1364/pshb.1991.fe9.
Der volle Inhalt der QuelleWang, Xiao-jun, und W. M. Dennis. „Spectral and Temporal Dynamics of Nonequilibrium Phonons in YAG:Pr3+“. In Persistent Spectral Hole Burning: Science and Applications. Washington, D.C.: Optica Publishing Group, 1991. http://dx.doi.org/10.1364/pshb.1991.fc3.
Der volle Inhalt der QuelleBerichte der Organisationen zum Thema "Hole dynamics"
Matsuzaki, Satoshi. Nonphotochemical Hole-Burning Studies of Energy Transfer Dynamics in Antenna Complexes of Photosynthetic Bacteria. Office of Scientific and Technical Information (OSTI), Januar 2001. http://dx.doi.org/10.2172/804159.
Der volle Inhalt der QuelleElliott, J. Hydra modeling of experiments to study ICF capsule fill hole dynamics using surrogate targets. Office of Scientific and Technical Information (OSTI), August 2007. http://dx.doi.org/10.2172/925990.
Der volle Inhalt der QuelleMatsuzaki, Satoshi. Nonphotochemical Hole-Burning Studies of Energy Transfer Dynamics in Antenna Complexes of Photosynthetic Bacteria. Office of Scientific and Technical Information (OSTI), Januar 2001. http://dx.doi.org/10.2172/797635.
Der volle Inhalt der QuelleTang, De-Ming. Excited state structure, energy and electron transfer dynamics of photosynthetic reaction centers: A hole burning study. Office of Scientific and Technical Information (OSTI), März 1991. http://dx.doi.org/10.2172/6120575.
Der volle Inhalt der QuelleMoerner, W. E. Photochemical and Photophysical Dynamics of Persistent Spectral Hole-Burning, Photorefractivity and Single Molecular Absorbers in Condensed Matter. Fort Belvoir, VA: Defense Technical Information Center, August 1992. http://dx.doi.org/10.21236/ada255333.
Der volle Inhalt der QuelleRiley, Kerry Joseph. Probing the Energy Transfer Dynamics of Photosynthetic Reaction Center Complexes Through Hole-Burning and Single-Complex Spectroscopy. Office of Scientific and Technical Information (OSTI), Januar 2007. http://dx.doi.org/10.2172/933127.
Der volle Inhalt der QuelleWu, H. M. Hole burning with pressure and electric field: A window on the electronic structure and energy transfer dynamics of bacterial antenna complexes. Office of Scientific and Technical Information (OSTI), Februar 1999. http://dx.doi.org/10.2172/348905.
Der volle Inhalt der QuelleHane, Jennifer Kazuko. The picosecond dynamics of electron-hole pairs in graded and homogeneous CdSxSe1-x semiconductors. Office of Scientific and Technical Information (OSTI), Mai 1995. http://dx.doi.org/10.2172/88836.
Der volle Inhalt der QuelleKulkarni, M., A. Patel und K. Leung. Mobile IPv4 Dynamic Home Agent (HA) Assignment. RFC Editor, März 2006. http://dx.doi.org/10.17487/rfc4433.
Der volle Inhalt der QuelleLafreniere, Robert A., und Roger Tryon. Dynamic Measurements of Three Urethane Hose Materials. Fort Belvoir, VA: Defense Technical Information Center, Mai 1995. http://dx.doi.org/10.21236/ada640492.
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