Relevant bibliographies by topics / Instabilities

Academic literature on the topic 'Instabilities'

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Published: 4 June 2021
Last updated: 31 August 2024

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Journal articles on the topic "Instabilities"

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Cruz, Akaxia, and Matthew McQuinn. "Astrophysical plasma instabilities induced by long-range interacting dark matter." Journal of Cosmology and Astroparticle Physics 2023, no. 04 (April 1, 2023): 028. http://dx.doi.org/10.1088/1475-7516/2023/04/028.

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Abstract If dark matter is millicharged or darkly charged, collective plasma processes may dominate momentum exchange over direct particle collisions. In particular, plasma streaming instabilities can couple the momentum of the dark matter to counter-streaming baryons or other dark matter and result in the counter-streaming fluids coming to rest with each other, just as happens for baryonic collisionless shocks in astrophysical systems. While electrostatic plasma instabilites (such as the two-stream) are highly suppressed by Landau damping when dark matter is millicharged, in the cosmological situations of interest, electromagnetic instabilities such as the Weibel can couple the momenta, assuming that the linear instability saturates in the manner typically found for baryonic plasmas. We find that the streaming of dark matter in the pre-Recombination universe is affected more strongly by direct collisions than collective processes, validating previous constraints. However, when considering unmagnetized instabilities the properties of the Bullet Cluster merger and other merging cluster systems (which show dark matter streaming through itself) are likely to be substantially altered if [qχ /mχ ] ≳ 10-4, where [qχ /mχ ] is the charge-to-mass ratio of the dark matter relative to that of the proton. When a magnetic field is added consistent with cluster observations, the Weibel and Firehose instabilities result in sufficiently fast growth to reach saturation for [qχ /mχ ] ≳ 10-12–10-11. The Weibel growth rates are even faster in the case of a dark-U(1) charge (because “hot” electrons do not damp the instability), potentially ruling out [qχ /mχ ] ≳ 10-14 in the Bullet Cluster system, in agreement with [1]. The strongest previous limits on millicharged dark matter (mDM) arise from considering the spin-down of galactic disks [2]. We show that plasma instabilities or tangled background magnetic fields could lead to diffusive propagation of the dark matter, weakening these spin-down limits. Thus, plasma instabilities may place some of the most stringent constraints over much of the millicharged, and our results corroborate previous extremely stringent potential constraints on the dark-charged parameter space.
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Pier, John. "Narrative instabilities." Frontiers of Narrative Studies 6, no. 2 (January 12, 2020): 148–56. http://dx.doi.org/10.1515/fns-2020-0011.

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Abstract Taking Nabokov’s Pale Fire as its tutor text, this chapter seeks to demonstrate that narrative functions as a complex or dynamic system. Due to the novel’s nonlinear and multiply configured format, a series of dissipative structures is provoked whereby states near equilibrium, on reaching states far from equilibrium under the weight of multiple causality, putting the system “beyond the threshold of stability” and “at the edge of chaos,” perpetually self-organize. Taking a cue from nonequilibrium thermodynamics, instabilities, it is argued, are inherent to narrative discourse. This calls into question the pertinence of the logic of linearity (“event A causes event B”) as well as the scope of such postulates as the isomorphic relation between sequence and narrative as a whole, a postulate that frames narrative as a closed system following the principle of conservation of energy in classical mechanics. As the poem “Pale Fire” in Nabokov’s novel advances linearly, it is constantly disrupted by the “Commentary” which is related to the poem only tangentially, each text fragmenting the other and self-organizing into new meanings. The effect is to render salient in narrative discourse the complexity science principles (in addition to those mentioned above) of irreversibility (the “arrow of time”) vs. reversibility, sensitivity to initial conditions, negative vs. positive feedback and the symmetry-breaking effects of bifurcation. The manifestation of these principles in Nabokov’s novel raises fundamental questions about the structuring of narrative, but also about the conceptual framework through which narrative at large might be approached.
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Mikhailov, Anatolii L., Nikolai V. Nevmerzhitskii, and Viktor A. Raevskii. "Hydrodynamic instabilities." Physics-Uspekhi 54, no. 4 (April 30, 2011): 392–97. http://dx.doi.org/10.3367/ufne.0181.201104i.0410.

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Heavens, O. S. "Optical Instabilities." Optica Acta: International Journal of Optics 33, no. 9 (September 1986): 1095. http://dx.doi.org/10.1080/716099711.

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Soderholm, Sidney Case. "Aerosol Instabilities." Applied Industrial Hygiene 3, no. 2 (February 1988): 35–40. http://dx.doi.org/10.1080/08828032.1988.10388506.

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Mikhailov, Anatolii L., Nikolai V. Nevmerzhitskii, and Viktor A. Raevskii. "Hydrodynamic instabilities." Uspekhi Fizicheskih Nauk 181, no. 4 (2011): 410. http://dx.doi.org/10.3367/ufnr.0181.201104i.0410.

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Scharfman, Barry E., and Alexandra H. Techet. "Bag instabilities." Physics of Fluids 24, no. 9 (September 2012): 091112. http://dx.doi.org/10.1063/1.4748933.

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Aukrust, T., and E. H. Hauge. "Wetting instabilities." Physical Review A 36, no. 8 (October 1, 1987): 4097–98. http://dx.doi.org/10.1103/physreva.36.4097.

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Furman, A. S. "Photovoltaic instabilities." Ferroelectrics 83, no. 1 (January 1988): 41–53. http://dx.doi.org/10.1080/00150198808235448.

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Einaudi, G. "CORONAL INSTABILITIES." Highlights of Astronomy 8 (1989): 529–33. http://dx.doi.org/10.1017/s1539299600008236.

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AbstractThe interest in the stability of coronal structures derives from their observed lifetime (much longer than the relevant hydromagnetic timescale) coupled with their active behavior. This fact implies that these structures must be globally stable with respect to fast and destructive instabilities and, at the same time, must allow some local, non-disrupting, dissipative process to take place. In highly magnetized media as solar and stellar coronae a large number of plasma instabilities can occur. The present review will concentrate on those governed by the magnetohydrodynamic (MHD) equations with the inclusion of the effects of finite resistivity and viscosity and the use of an energy equation where radiation, mechanical heating and thermal conduction are considered.
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Dissertations / Theses on the topic "Instabilities"

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Barnaby, Neil. "Cosmological instabilities." Thesis, McGill University, 2007. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=103365.

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Though historically the word "tachyon" has been used to describe hypothetical particles which propagate faster than the speed of light, in a more modern context the term has been recycled to refer to certain unstable states in field theory. This thesis explores the role of tachyonic instabilities in cosmology considering tachyons which arise in string theory and also more conventional, field theoretic instabilities. Our study of such instabilities is, in part, motivated by attempts to embed inflation into string theory. We will argue that the study of string theory models of inflation is well-motivated and may provide a rare potential observational window into string physics.
After reviewing the necessary background material concerning inflation, cosmological perturbation theory and tachyonic instabilities we study in detail the dynamics of the tachyonic instability which marks the end of a particular string theory model of inflation, focusing on the processes of reheating and cosmic string production. We show that the peculiar dynamics of the open string tachyon leads to various novelties in these processes and consider also potential observational consequences.
We consider tachyonic preheating at the end of hybrid inflation in a conventional field theory setting and show that the preheating process can leave an observable imprint on the Cosmic Microwave Background, either through n = 4 contamination of the power spectrum or else through large nongaussian signatures. The possibility of large nongaussianity is particularly interesting since it demonstrates that hybrid inflation provides one of the few well-motivated models which can generate an observable nongaussian signature.
Finally, we study a novel string theoretic model of inflation, p-adic inflation. This model is nonlocal, however, it is free of the usual problems (such as ghosts) which plague nonlocal theories. Furthermore, the nonlocal structure of the theory leads to a variety of unexpected dynamics including the possiblity of a slowly rolling inflaton, despite an extremely steep potential.
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Yu, Rui. "Faraday Instabilities." Digital WPI, 2017. https://digitalcommons.wpi.edu/etd-theses/347.

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The shape of a liquid's surface is determined by both the body force and surface force of the liquid. In this report, the body force is solely from the gravitational force. The surface force is generated from the movement of an elastic interface between the solid and liquid. To obtain the shape of the surface, both asymptotic analysis and numerical approaches are used in this report. The asymptotic analysis is applied on the potential flow. The initial conditions are chosen to be the function of the shape of the interface between the solid and liquid and the free stream velocity far away from the interface. The time dependent contributions from the fluid system are also considered. The initial condition changes according to the function of the calculated velocity potential. The numerical approach includes two parts: calculation the velocity potential and a formalism of the change of the system as time evolves. For the first part, two idealized vertical boundaries are utilized to give a unique solution of the Laplace equation. The boundary conditions are determined as the flow under linear viscosity. For the second part, the flow is first assumed to be a potential flow, and a boundary layer is considered to make the no-slip condition valid and to give a more precise approximation for the shear stress.
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Hasan, Haider. "Nearshore hydrodynamical instabilities." Thesis, University of Nottingham, 2006. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.438557.

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Arshad, S. A. "Control of disruptive instabilities." Thesis, University of Oxford, 1991. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.291069.

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Potter, Mark. "Non-Return Valve Instabilities." Thesis, University of Oxford, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.504453.

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Barclay, Graeme James. "Instabilities in liquid crystals." Thesis, University of Strathclyde, 1998. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.366797.

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Zahniser, Russell 1982. "Instabilities of rotating jets." Thesis, Massachusetts Institute of Technology, 2004. http://hdl.handle.net/1721.1/32752.

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Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.
Includes bibliographical references (p. 33-34).
When a jet of water is in free fall, it rapidly breaks up into drops, since a cylinder of water is unstable. This and other problems involving the form of a volume of water bound by surface tension have yielded a wealth of theoretical and experimental results, and given insight into such phenomena as the shape of the Earth. Particularly interesting behaviors tend to emerge when the fluid in question is rotating; a drop may, for example, form a toroidal or ellipsoidal shape or even stretch out into some multi-lobed, non-axisymmetric form. In this paper, we investigate the properties of a rotating jet of water, and determine what regime of the parameter space are dominated by the various forms of instability. This is both predicted theoretically and demonstrated to be accurate experimentally. If we watch a jet of water as the rotation rate is gradually increased from zero, the drop size will start shrinking gradually, and then suddenly, rather than a single row of drops, we will see the jet breaking up into two-lobed, bar shaped forms, like the rung of a ladder. The point at which this transition occurs is characterized in terms of the rotational Bond number, B₀ = ... . The critical B₀ may be as low as 6, if there is a strong bias imparted by vibration of the table at an appropriate frequency, but for a perfectly quiescent rotating jet the second mode does not become dominant until a higher B₀. As the rotation rate is increased above this, the instability grows gradually more dramatic, and eventually the two lobes of each drop are breaking apart and flying outward. Then a transition to a third mode will occur, with three lobes in each drop; this is possible from a B₀ of 12, and dominant above a B₀ slightly higher than that. In general, mode m may occur whenever
(cont.) B₀ > m(m + 1).
by Russell Zahniser.
S.B.
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Latter, Henrik. "Instabilities in planetary rings." Thesis, University of Cambridge, 2007. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.612787.

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Sobral, Yuri Dumaresq. "Instabilities in fluidised beds." Thesis, University of Cambridge, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.612185.

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Santos, German R. "Studies on secondary instabilities." Diss., Virginia Polytechnic Institute and State University, 1987. http://hdl.handle.net/10919/49885.

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Significant advances in understanding early stages of transitional flows have been achieved by studying secondary instabilities in selected prototype flows. These secondary instabilities can be modeled as parametric instabilities of the nearly periodic flow that consists of the prototype velocity profile and a superposed finite-amplitude TS-wave (wavelength λ). The generally three dimensional secondary instabilities are governed by a linearized system of partial differential equations with periodic coefficients which are reduced to an algebraic eigenvalue problem through the application of a spectral collocation method Following Floquet theory, previous analysis looked for subharmonic (wavelength 2 λ) and fundamental (wavelength λ) types of solutions. We extend the Floquet theory to solutions having arbitrary wavelengths, hence including the previous solutions as special cases. Modes with wavelength in between the subharmonic and fundamental values are called detuned modes. Detuned modes lead to combination resonance which has been observed in controlled transition experiments. Knowledge of the bandwidth of amplified detuned or (combination) modes is very important for clarification of the selectivity of the early stages of transition with respect to initial disturbances. We have selected two flows: the Blasius boundary layer flow and the hyperbolic-tangent free-shear flow as prototypes of wall bounded Hows and unbounded Hows, respectively. In the Blasius flow we have concentrated on studying detuned modes. We found the growth rates of modes slightly detuned from the subharmonic wavelength to be almost as large as the growth rate of the subharmonic itself. This result is consistent with both the broadband spectra centered at subharmonic frequency observed in the "biased" experiment of Kachanov & Levchenko, wherein only the TS frequency was introduced, and with the large band-width of resonance in the "controlled" experiments, wherein a TS wave and the detuned modes were introduced simultaneously. In the free-shear flow, our goals were three-fold. The first was to investigate whether the Floquet analysis based on the shape assumption for TS waves would provide results consistent with results for the stability of Stuart vortices. Second, we aimed at revealing the effect of viscosity on these results. Finally, we wanted to evaluate a group of spectral methods for the numerical treatment of the flow in an unbounded domain. We have made a detailed analysis of subharmonic, fundamental, and detuned modes. Results display the basically inviscid, convective character of the secondary instabilities, and their broadband nature in the streamwise and spanwise directions. In the inviscid limit, and for neutral TS waves, a detailed comparison is made with the closely related study on stability of Stuart vortices by Pierrehumbert & Widnall. Good quantitative agreement is obtained. For a wide range of Reynolds numbers and amplitudes of the 2-D primary wave, results reveal that the most unstable subharmonic modes are two-dimensional (vortex pairing). On the other hand, the most unstable fundamental modes are three-dimensional, with short spanwise wavelengths. Detuned modes have characteristics in between, being most unstable in the two-dimensional or three-dimensional form depending on the detuning value. Comparisons of our results for a superposed TS wave of constant amplitude with results obtained by numerical simulations suggested that the growth of the TS wave may have a significant effect on the secondary disturbance growth. To check this hypothesis, we have developed a numerical method that accounts for small variations in the TS amplitude. However, the results indicate that the discrepancies are due to other yet concealed effects.
Ph. D.
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Books on the topic "Instabilities"

1

Charru, François. Hydrodynamic instabilities. Cambridge: Cambridge University Press, 2011.

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Ahrens, Chandler, and Aaron Sprecher, eds. Instabilities and Potentialities. New York : Routledge, 2019.: Routledge, 2019. http://dx.doi.org/10.4324/9780429506338.

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Martinis, J. A. C., and M. Raous, eds. Friction and Instabilities. Vienna: Springer Vienna, 2002. http://dx.doi.org/10.1007/978-3-7091-2534-2.

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Enrique, Tirapegui, Villarroel D, Universidad de Chile. Facultad de Ciencias Físicas y Matemáticas., Universidad Técnica Federico Santa María., and International Workshop on Instabilities and Nonequilibrium Structures (2nd : 1987 : Valparaíso, Chile), eds. Instabilities and nonequilibrium structures II: Dynamical systems and instabilities. Dordrecht: Kluwer Academic Publishers, 1989.

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Tirapegui, Enrique. Instabilities and Nonequilibrium Structures II: Dynamical Systems and Instabilities. Dordrecht: Springer Netherlands, 1989.

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Tirapegui, Enrique. Instabilities and Nonequilibrium Structures. Dordrecht: Springer Netherlands, 1987.

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Tirapegui, Enrique, and Danilo Villarroel, eds. Instabilities and Nonequilibrium Structures. Dordrecht: Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3783-3.

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Gouesbet, G., and A. Berlemont, eds. Instabilities in Multiphase Flows. Boston, MA: Springer US, 1993. http://dx.doi.org/10.1007/978-1-4899-1594-8.

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Straughan, Brian. Explosive Instabilities in Mechanics. Berlin, Heidelberg: Springer Berlin Heidelberg, 1998. http://dx.doi.org/10.1007/978-3-642-58807-5.

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Knopoff, L., V. I. Keilis-Borok, and G. Puppi, eds. Instabilities in Continuous Media. Basel: Birkhäuser Basel, 1985. http://dx.doi.org/10.1007/978-3-0348-6608-8.

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Book chapters on the topic "Instabilities"

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Virga, Epifanio G. "Instabilities." In Variational Theories for Liquid Crystals, 173–243. Boston, MA: Springer US, 1994. http://dx.doi.org/10.1007/978-1-4899-2867-2_4.

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Piel, Alexander. "Instabilities." In Plasma Physics, 197–218. Berlin, Heidelberg: Springer Berlin Heidelberg, 2010. http://dx.doi.org/10.1007/978-3-642-10491-6_8.

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Narayanan, A. Satya. "Instabilities." In Astronomy and Astrophysics Library, 135–54. New York, NY: Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4614-4400-8_6.

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Chiuderi, Claudio, and Marco Velli. "Instabilities." In UNITEXT for Physics, 99–148. Milano: Springer Milan, 2014. http://dx.doi.org/10.1007/978-88-470-5280-2_6.

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Needham, Charles E. "Instabilities." In Blast Waves, 127–37. Berlin, Heidelberg: Springer Berlin Heidelberg, 2010. http://dx.doi.org/10.1007/978-3-642-05288-0_10.

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Visconti, Guido, and Paolo Ruggieri. "Instabilities." In Fluid Dynamics, 163–204. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-49562-6_6.

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Piel, Alexander. "Instabilities." In Graduate Texts in Physics, 211–33. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-63427-2_8.

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Lilly, Douglas K. "Instabilities." In Mesoscale Meteorology and Forecasting, 259–71. Boston, MA: American Meteorological Society, 1986. http://dx.doi.org/10.1007/978-1-935704-20-1_11.

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Needham, Charles E. "Instabilities." In Blast Waves, 151–62. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-65382-2_10.

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Freund, H. P., and T. M. Antonsen. "Sideband Instabilities." In Principles of Free-Electron Lasers, 245–55. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2316-7_6.

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Conference papers on the topic "Instabilities"

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Coullet, P. "Interaction between instabilities, phase instabilities, phase turbulence." In Instabilities and Dynamics of Lasers and Nonlinear Optical Systems. Washington, D.C.: Optica Publishing Group, 1985. http://dx.doi.org/10.1364/idlnos.1985.wb4.

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Pestrikov, D. V. "Transverse instabilities." In HIGH QUALITY BEAMS: Joint US-CERN-JAPAN-RUSSIA Accelerator School. AIP, 2001. http://dx.doi.org/10.1063/1.1420422.

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CHAO, ALEX. "BEAM INSTABILITIES." In Proceedings of the Asian Accelerator School. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812778413_0012.

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Falqués, Albert, Amadeu Montoto, and Vicente Iranzo. "Coastal Morphodynamic Instabilities." In 25th International Conference on Coastal Engineering. New York, NY: American Society of Civil Engineers, 1997. http://dx.doi.org/10.1061/9780784402429.275.

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Haug, Hartmut. "Instabilities In Semiconductors." In 1986 Quebec Symposium, edited by Neal B. Abraham and Jacek Chrostowski. SPIE, 1986. http://dx.doi.org/10.1117/12.938851.

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Pestrikov, D. V. "Head-tail instabilities." In HIGH QUALITY BEAMS: Joint US-CERN-JAPAN-RUSSIA Accelerator School. AIP, 2001. http://dx.doi.org/10.1063/1.1420423.

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Quinlan, John M. "Parametric Combustion Instabilities." In AIAA SCITECH 2022 Forum. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2022. http://dx.doi.org/10.2514/6.2022-1857.

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Kulwicki, B. M. "Instabilities in PTC Resistors." In Sixth IEEE International Symposium on Applications of Ferroelectrics. IEEE, 1986. http://dx.doi.org/10.1109/isaf.1986.201228.

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Hyde, T. W., B. Smith, K. Qiao, and J. Kong. "Instabilities Within Complex Plasmas." In IEEE Conference Record - Abstracts. 2005 IEEE International Conference on Plasma Science. IEEE, 2005. http://dx.doi.org/10.1109/plasma.2005.359386.

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Uddin, M. Nasim, and Daniel F. Watt. "Highspeed laser weld instabilities." In ICALEO® ‘94: Proceedings of the Laser Materials Processing Conference. Laser Institute of America, 1994. http://dx.doi.org/10.2351/1.5058822.

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Reports on the topic "Instabilities"

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K.Y. Ng. Collective instabilities. Office of Scientific and Technical Information (OSTI), August 2003. http://dx.doi.org/10.2172/813535.

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Bloch, Anthony, P. S. Krishnaprasad, Jerrold E. Marsden, and Tudor S. Ratiu. Dissipation Induced Instabilities. Fort Belvoir, VA: Defense Technical Information Center, March 1993. http://dx.doi.org/10.21236/ada454960.

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Blaskiewicz, M., D. P. Deng, W. W. MacKay, V. Mane, S. Peggs, A. Ratti., J. Rose, T. Shea, and J. Wei. Collective Instabilities in RHIC. Office of Scientific and Technical Information (OSTI), September 1994. http://dx.doi.org/10.2172/1119432.

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Rutherford, P. H. Resistive instabilities in tokamaks. Office of Scientific and Technical Information (OSTI), October 1985. http://dx.doi.org/10.2172/5086595.

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Spector, Scott J. Material Instabilities in Solids. Fort Belvoir, VA: Defense Technical Information Center, January 1988. http://dx.doi.org/10.21236/ada189525.

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Desjardins, Tiffany, Rachel Glade, Denis Aslangil, and Elizabeth Merritt. Fluids, instabilities and turbulence. Office of Scientific and Technical Information (OSTI), June 2020. http://dx.doi.org/10.2172/1631568.

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Ya.I. Kolesnichenko, V.V. Lutsenko, V.S. Marchenko, and R.B. White. Non-conventional Fishbone Instabilities. Office of Scientific and Technical Information (OSTI), November 2004. http://dx.doi.org/10.2172/836155.

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Zhang S. Y. and W. Weng. NSNS Transverse Microwave Instabilities. Office of Scientific and Technical Information (OSTI), June 1997. http://dx.doi.org/10.2172/1157212.

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Fox, John D. Multibunch Instabilities and Cures. Office of Scientific and Technical Information (OSTI), May 2003. http://dx.doi.org/10.2172/813144.

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Spector, Scott J. Material Instabilities in Solids. Fort Belvoir, VA: Defense Technical Information Center, October 1989. http://dx.doi.org/10.21236/ada218451.

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