Relevant bibliographies by topics / SPH - Coalescence

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  4. Conference papers

Academic literature on the topic 'SPH - Coalescence'

Author: Grafiati
Published: 4 June 2021
Last updated: 3 February 2022

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Journal articles on the topic "SPH - Coalescence"

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Wang, Dudou, Hongfu Qiang, and Chao Shi. "A multiphase SPH framework for solving the evaporation and combustion process of droplets." International Journal of Numerical Methods for Heat & Fluid Flow 30, no. 3 (December 12, 2019): 1547–75. http://dx.doi.org/10.1108/hff-08-2019-0666.

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Purpose This paper aims to introduce a two-dimensional smoothed particle hydrodynamics (SPH) framework for simulating the evaporation and combustion process of fuel droplets. Design/methodology/approach To solve the gas–liquid two-phase flow problem, a multiphase SPH method capable of handling high density-ratio problems is established. Based on the Fourier heat conduction equation and Fick’s law of diffusion, the SPH discrete equations are derived. To effectively characterize the phase transition problem, inspired by volume of fluid method, the concept of liquid phase mass fraction of the SPH particles is proposed. The one-step global reaction model of n-hexane is used for the vapor combustion. Findings The evaporation and combustion process of single droplet conforms to the law. The framework works out well when the evaporation of multiple droplets involves coalescence process. Three different kinds of flames are observed in succession in the combustion process of a single droplet at different inflow velocity, which agree well with the results of the experiment. Originality/value To the best of the authors’ knowledge, this is the first computational framework that has the capability to simulate evaporation and combustion with SPH method. Based on the particle nature of SPH method, the framework has natural advantages in interface tracking.
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Xu, Xiaoyang, Tingting Tang, and Peng Yu. "A modified SPH method to model the coalescence of colliding non‐Newtonian liquid droplets." International Journal for Numerical Methods in Fluids 92, no. 5 (May 2020): 372–90. http://dx.doi.org/10.1002/fld.4787.

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Wu, Jun, Xuemei Liu, Haihua Xu, and Hongjian Du. "Simulation on the Self-Compacting Concrete by an Enhanced Lagrangian Particle Method." Advances in Materials Science and Engineering 2016 (2016): 1–11. http://dx.doi.org/10.1155/2016/8070748.

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The industry has embraced self-compacting concrete (SCC) to overcome deficiencies related to consolidation, improve productivity, and enhance safety and quality. Due to the large deformation at the flowing process of SCC, an enhanced Lagrangian particle-based method, Smoothed Particles Hydrodynamics (SPH) method, though first developed to study astrophysics problems, with its exceptional advantages in solving problems involving fragmentation, coalescence, and violent free surface deformation, is developed in this study to simulate the flow of SCC as a non-Newtonian fluid to achieve stable results with satisfactory convergence properties. Navier-Stokes equations and incompressible mass conservation equations are solved as basics. Cross rheological model is used to simulate the shear stress and strain relationship of SCC. Mirror particle method is used for wall boundaries. The improved SPH method is tested by a typical 2D slump flow problem and also applied to L-box test. The capability and results obtained from this method are discussed.
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ESCALA, ANDRES, and LUCIANO DEL VALLE. "GAS-INDUCED MERGER OF MASSIVE BLACK HOLE BINARIES." International Journal of Modern Physics E 20, supp01 (December 2011): 79–84. http://dx.doi.org/10.1142/s0218301311040104.

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We use SPH simulations to investigate the effects of gas on the inspiral and merger of massive black hole binary. This scenario is motivated by the very massive nuclear gas disk observed in the central regions of merging galaxies. We run a variety of models, ranging from simulations with relaty smooth gas to cases in which the gas has a more clumpy spatial distribution. We also vary the Mgas / Mbin ratio identifying the case M bin /M gas = 1 as an important limiting test-case for the analytic formulation of the dynamical process that dominates the binary-disk interaction in the late evolution of the system. We find that gas has an important effect in the evolution of interacting massive black hole binary on merging galaxies and that this interaction can be separate in two principal stages. The coalescence timescale that we find for the MBH binary varies between 5 · 106 yr and 2.5 · 107 yr for typical parameters of ULIRGs galaxies. This results supports scenarios of massive black hole evolution and growth in which hierarchical merging plays an important role. The final coalescence of the black hole leads to gravitational radiation emission that would be detected out to high redshift by LISA.
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Li, S. L., C. Agnor, and D. N. C. Lin. "Giant impact, planetary merger, and diversity of planetary-core mass." Proceedings of the International Astronomical Union 3, S249 (October 2007): 301–3. http://dx.doi.org/10.1017/s1743921308016736.

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AbstractTransit observations indicate a large dispersion in the internal structure among the known gas giants. This is a big challenge to the conventional sequential planetary formation scenario because the diversity is inconsistent with the expectation of some well defined critical condition for the onset of gas accretion in this scenario. We suggest that giant impacts may lead to the merger of planets or the accretion of planetary embryos and cause the diversity of the core mass. By using an SPH scheme, we show that direct parabolic collisions generally lead to the total coalescence of impinging gas giants whereas, during glancing collisions, the efficiency of core retention is much larger than that of the envelope. We also examine the adjustment of the gaseous envelope with a 1D Lagrangian hydrodynamic scheme. In the proximity of their host stars, the expansion of the planets' envelopes, shortly after sufficiently catastrophic impacts, can lead to a substantial loss of gas through Roche-lobe overflow. We are going to examine the possibility that the accretion of several Earth-mass objects can significantly enlarge the planets' photosphere and elevate the tidal dissipation rate over the time scale of 100 Myr.
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Filloux, Charline, J. A. de Freitas Pacheco, Fabrice Durier, and Joseph Silk. "Evolution of Supermassive Black Holes." Proceedings of the International Astronomical Union 5, S267 (August 2009): 202. http://dx.doi.org/10.1017/s1743921310006228.

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Cosmological simulations describing both the evolution of supermassive black holes and their host galaxies were performed by using the tree PM-SPH code GADGET-2 (Springel 2005). Physical mechanisms affecting the dynamics and the physical conditions of the gas (ionization and cooling processes, local heating by stars, injection of mechanical energy by supernovae, chemical enrichment) were introduced in the present version of the code (Filloux 2009). Black holes in a state of accretion (AGNs) also inject mechanical energy in the surrounding medium, contributing for quenching the star formation activity. In all simulations a ΛCDM cosmology was adopted (h = 0.7, ΩΛ=0.7, Ωm=0.3, Ωb=0.046 and σ8=0.9). Simulations were performed in a volume with a side of 50h−1 Mpc, starting at z = 50 and through the present time (z = 0). For low and intermediate resolution runs, the initial gas mass particles are respectively 5.35× 108M⊙ and 3.09×108M⊙. Black holes (BHs) are represented by collisionless particles and seeds of 100 M⊙ were introduced in density peaks at z = 15, growing either by accretion or coalescence. The accretion rate from the “disk mode” is based on a turbulent viscous thin disk model whereas in the “spherical mode” the rate is given by the Bondi–Hoyle formula. When accreting matter, jets, modeled by conical regions perpendicular to the disk plane, inject kinetic energy into the surrounding medium. Two models were tested: in the first, the injected energy rate is about 10% of the gravitational energy rate released in the accretion process while in the second, the injected energy rate is based on the Blandford & Znajek (1977) mechanism. All simulations give, at z = 0, similar black hole mass function but they overestimate slightly the BH density for masses above ~ 108M⊙. The resulting BH density in this mass range is affected by feedback processes since they control the amount of gas available for accretion. The present simulations are not able to produce very massive BHs (~109M⊙) at z ~ 6. However the evolution of the BH mass density derived from our simulations are in quite good agreement with that derived from the QSO luminosity function. This indicates that our simulations reproduce quite well the average accretion rate history of BHs. Correlations between the BH mass and properties of the host galaxy (velocity dispersion for bulge systems or the stellar mass or the dark halo mass) are also well reproduced. In conclusion, these exploratory simulations reproduce the data at z = 0 quite well. However, the present adopted recipe for the accretion rate in the “disk mode” seems to be inefficient to produce massive BHs as early as z ~ 6. Higher resolution simulations including a new approach for modeling the “disk mode” are presently under way and that particular difficulty is expected to be solved.
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Fu, Ming, Vincent Chi Hang Lui, Mai Har Sham, Vassilis Pachnis, and Paul Kwong Hang Tam. "Sonic hedgehog regulates the proliferation, differentiation, and migration of enteric neural crest cells in gut." Journal of Cell Biology 166, no. 5 (August 30, 2004): 673–84. http://dx.doi.org/10.1083/jcb.200401077.

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Enteric neural crest cells (NCCs) migrate and colonize the entire gut and proliferate and differentiate into neurons and glia of the enteric nervous system in vertebrate embryos. We have investigated the mitogenic and morphogenic functions of Sonic hedgehog (Shh) on enteric NCCs in cell and organ culture. Enteric NCCs expressed Shh receptor Patched and transcripts encoding the Shh signal transducer (Gli1). Shh promoted the proliferation and inhibited the differentiation of NCCs. The pro-neurogenic effect of glial cell line–derived neurotrophic factor (GDNF) on NCCs was abolished by Shh. In gut explants, NCCs migrated from the explants onto the adjacent substratum if GDNF was added, whereas addition of Shh abolished this migration. Neuronal differentiation and coalescence of neural crest–derived cells into myenteric plexuses in explants was repressed by the addition of Shh. Our data suggest that Shh controls the proliferation and differentiation of NCCs and modulates the responsiveness of NCCs toward GDNF inductions.
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Petzke, Martin. "The Global “Bookkeeping” of Souls: Quantification and Nineteenth-Century Evangelical Missions." Social Science History 42, no. 2 (2018): 183–211. http://dx.doi.org/10.1017/ssh.2017.50.

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This article combines perspectives of the sociology of quantification and field theory in analyzing the emergence of a field of global evangelical missions. Drawing analogies to Werner Sombart's thesis on the relationship of double-entry bookkeeping and the genesis of capitalism, it shows how the introduction of statistical methods and accounting techniques into the realm of missions in the nineteenth century constructed a visibility of a global distribution of religious adherents that spurred, oriented, and perpetuated an interorganizational sphere geared toward the conversion of the world to Christianity. The article identifies the soteriological and eschatological prerequisites that led to the coalescence of demographic notions and missionary perspectives and draws attention to the extensive reporting system of missionary societies that further consolidated logics of “bookkeeping” in missions. It argues that this ongoing evangelical missionary enterprise is an instance of a more general mechanism of quantification spawning a social field dedicated to the maintenance or alteration of particular “quantities.”
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Ma, Tian-Bao, Yuan-Zhong Hu, and Hui Wang. "Formation and coalescence of linear chains in growth of nanostructured sp–sp2 amorphous carbon films." Chemical Physics Letters 462, no. 1-3 (September 2008): 104–8. http://dx.doi.org/10.1016/j.cplett.2008.07.088.

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Mahulikar, Shripad P., and Pallavi Rastogi. "Study of black hole as dissipative structure using negentropy." Canadian Journal of Physics 94, no. 10 (October 2016): 960–66. http://dx.doi.org/10.1139/cjp-2016-0388.

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The area of the event horizon of a black hole (Aeh) is so far linked only with its entropy (SBH). In this theoretical investigation, it is shown that relating Aeh only to SBH is inadequate, because Aeh is linked to the black hole’s negentropy, which encompasses its entropy. Increasing Aeh of black holes that grow now follows from the negentropy theorem (NET) and also from the well-known area theorem. The decreasing Aeh of black holes that decay follows from the converse to NET and is not a violation of the area theorem. The corollary to NET is proved for the case when two dissipative structures merge, which is the basis for the coalescence of black holes. The converse of corollary to NET explains negentropy loss due to splitting of a dissipative structure. When applied to black hole explosion (i.e., splitting into an infinite number of parts), converse of corollary to NET reduces to converse of NET. The entropy/energy ratio of the exported Hawking radiance from black holes contributes to the entropy increase of the universe. These aspects justify the consideration of black holes as thermodynamic dissipative structures.
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Dissertations / Theses on the topic "SPH - Coalescence"

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Renvoizé, Vincent. "Hydrodynamique et évolution d'objets compacts : binaires serrées et naines blanches." Lyon, École normale supérieure (sciences), 2002. http://www.theses.fr/2002ENSL0221.

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Le travail présenté est constitué de trois parties indépendantes. Dans la première partie, on étudie à l'aide de la technique SPH (Smoothed Particle Hydrodynamics) la déformation du secondaire au contact de Roche dans les variables cataclysmiques (CV). Ces déformations conduisent à une période orbitable plus grande que celle prévue par la troisième loi de Képler. La prise en compte de cette modification dans des modèles dévolution de CV explique partiellement pourquoi la période des CV observées a un minimum vers 80 minutes. La deuxième partie traite des binaires serrées de naines blanches. On présente un modèle analytique simple du transfert de masse dans ces systèmes lorsque le secondaire remplit son lobe de Roche. L'étude montre que si le rapport des masses est petit (secondaire légerà, alors de transfert de masse est stable et dure typiquement cent millions d'années. Dans le cas contraire, il est instable et la coalescence complète se produit en quelques minutes. Une modélisation SPH montre le déroulement de cette coalescence. La troisième partir concerne le refroidissement des naines blanches isolées pour donner une relation âge-luminosité de ces objets. Le refroidissement est étudié à l'aide d'une code d'évolution stellaire qui calcule complètement la structure de l'étoile (équation d'état, de transfert d'énergie, du mouvement)̀. Ce code est adapté pour traiter la cristallisation du plasma dans le cas d'une composition pure (C ou O) ou d'une mélange (C+O). L'allongement du temps de refroidissement à cause de la cristallisation est étudié. Les courbes de luminosité correspondant à différentes masses sont présentées.
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Salazar, Valenzuela Christian David. "Diversification in the Neotropics: Insights from Demographic and Phylogenetic Patternsof Lancehead Pitvipers (Bothrops spp.)." The Ohio State University, 2016. http://rave.ohiolink.edu/etdc/view?acc_num=osu1462545845.

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Fansi, Joseph. "PREDICTION PAR ELEMENTS FINIS DE LA RUPTURE DES ACIERS DUAL_PHASE EN UTILISANT UN MODELE DE GURSON AVANCE." Phd thesis, Ecole nationale supérieure d'arts et métiers - ENSAM, 2013. http://tel.archives-ouvertes.fr/tel-00869032.

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L'actuelle investigation numérique du Gurson-Tvergaard-Needleman (GTN) modèle avancé est une extension du travail de Ben Bettaieb et al. (2011). Le modèle a été implémenté à l'aide d'une sous routine (VUMAT) contenu dans le code commerciale d'éléments finis Abaqus/explicit. Le modèle d'endommagement améliore l'original en intégrant les trois mécanismes d'endommagement, la nucléation, la croissance, et la coalescence des cavités. Le modèle d'endommagement intègre les lois de nucléation et de croissance basés sur les phénomènes purement physiques. Ces nouvelles contributions incluant l'influence de l'écrouissage cinématique, ont été validées par les résultats de mesures expérimentales de tomographie à rayon X à haute résolution. Aussi, l'implémentation numérique de l'écrouissage cinématique dans le modèle modifié a contraint de proposer et de réarranger la définition de la triaxialité que l'on trouve habituellement dans la littérature. A coté de cela, un second critère d'initiation à la rupture basé sur l'ultime distance inter-cavités a été inclue afin de localiser et de quantifier avec plus de précision la distribution des déformations peu avant que le matériau ne casse complètement. L'actuel modèle d'endommagement a été appliqué dans des conditions industrielles pour prédire l'évolution de l'endommagement, l'état de contraintes, et l'initiation à la rupture pour différentes géométries de tôles et sur des essais d'emboutissage de tôles minces.
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Tseng, Shu-Ping, and 曾書萍. "Inferring the speciation model with coalescent-based multi-locus approach: A case of Takydromus spp." Thesis, 2011. http://ndltd.ncl.edu.tw/handle/pvf7b5.

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碩士
國立臺灣師範大學
生命科學研究所
100
Allopatric speciation is the dominant view of speciation among evolutionists. It is the process, where an ancestral population splits into two populations because of a geographic barrier. Genetic divergence gradually accumulates between the two descendant populations and ultimately results in two reproductively isolated entities. Under this scenario, speciation seems unlikely to proceed with the existence of gene flow. However, alternative geographic speciation modes allowing certain amount of gene flow (i.e. parapatic and sympatric modes) during speciation have gained more attention and related studies been published in recent years. In this study, we aim to test the existence of historical gene flow to evaluate the predominance of allopatric isolation during the speciation process across three reciprocally monophyletic species: Takydromus viridipunctatus, T. luyeanus and T. hsuehshanensis. The EST database of Takydromus spp. was constructed by using 454 sequencing, and 20 nuclear loci were successfully identified and amplified from the lizards for genetic investigations. IMA2 analyses revealed significant gene flows among the three species disfavouring a strictly allopatric speciation model. An approximate Bayesian computation (ABC) model choice procedure further indicated that an “early gene flow model” but not an “secondary contact model” fits better with the empirical data (T. viridipunctatus and T. luyeanus). Hence, historical but contemporary gene flow has occurred between T. viridipunctatus and T. luyeanus. We concluded that “parapatric” rather than “allopatric” is the predominant mode of speciation across Takydromus species.
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Book chapters on the topic "SPH - Coalescence"

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Acevedo-Malavé, Alejandro. "Hydrodynamics of Multiple Coalescence Collisions of Liquid Drops: From the Modelling of the Coalescence Phenomenon to Flocculation of Drops in 3D Using the SPH Formalism." In Computational and Experimental Fluid Mechanics with Applications to Physics, Engineering and the Environment, 315–23. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-00191-3_18.

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Conference papers on the topic "SPH - Coalescence"

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Hafskjold, Bjorn, Thomas B. Morrow, Harald K. B. Celius, and David R. Johnson. "Drop-Drop Coalescence In Oil/Water Separation." In SPE Annual Technical Conference and Exhibition. Society of Petroleum Engineers, 1994. http://dx.doi.org/10.2118/28536-ms.

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Chase, George G., and Abdulwahab S. Aljuhani. "Electro-coalescence of Water Droplets in Air Medium by Electrowetting." In SPE Eastern Regional Meeting. Society of Petroleum Engineers, 2013. http://dx.doi.org/10.2118/165674-ms.

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Woerpel, Craig, Shawn C. Maxwell, Bill Underhill, and James E. Wolfe. "Automated Monitoring of a Hydraulic Fracture by Coalescence Microseismic Mapping." In SPE Eastern Regional Meeting. Society of Petroleum Engineers, 2010. http://dx.doi.org/10.2118/139043-ms.

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Ortega, P., G. McGrath, G. Nunez, and D. Joseph. "Device for Testing the Dynamic Stability of Highly Concentrated Emulsions against Coalescence." In SPE International Thermal Operations and Heavy Oil Symposium. Society of Petroleum Engineers, 2001. http://dx.doi.org/10.2118/69729-ms.

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Amarzguioui, Morad, and Per Christian Jacobsen. "Novel use of Electro Coalescence to Enhance, Optimize and Debottleneck Oil Separation Trains." In SPE Annual Technical Conference and Exhibition. Society of Petroleum Engineers, 2015. http://dx.doi.org/10.2118/174763-ms.

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Hatchell, Daniel, Wen Song, and Hugh Daigle. "Effect of Inter-Particle Van Der Waals Attraction on the Stability of Pickering Emulsions in Brine." In SPE Annual Technical Conference and Exhibition. SPE, 2021. http://dx.doi.org/10.2118/206112-ms.

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Abstract Pickering emulsions are stabilized by solid particles that occupy the fluid-fluid interface, physically preventing coalescence. Their stability in brine, where interparticle electrostatic repulsion is negligible and van der Waals (vdW) attraction dominates, makes them attractive for applications in porous media. Recent studies postulate that inter-droplet particle networks assemble in brine and aid Pickering emulsion stability to coalescence. This work experimentally assesses the effect of increasing interparticle vdW attraction on particle network strength and emulsion stability. We grafted 6 nm, 12 nm, and 20 nm silica nanoparticles with varying densities of polyethylene glycol (PEG) to prevent aggregation and dispersed them in either brine or deionized water (DI). We characterized the PEG-coated nanoparticles with thermogravimetric analysis and dynamic light scattering to determine PEG grafting density, diameter, and zeta potential. To generate oil-in-water emulsions, we sonicated dispersions of variable nanoparticle concentration and decane in equal volumes. We imaged the emulsions with microscopy and centrifuged them for 15 minutes at 5000 g of acceleration, using the volume of decane released after centrifugation as a measurement of emulsion coalescence to the applied force. Nanoparticle characterization confirmed successful grafting of PEG to the silica surface. We compared trends in emulsion stability as a function of salinity and particle diameter to changes in the relevant interparticle forces described by extended Derjaguin-Landau-Verwey-Overbeek (DLVO) theory. Analysis of microscopy images showed an increase in emulsion droplet diameter with decreasing nanoparticle concentration, salinity, and increasing nanoparticle diameter. Through centrifugation we observed that lower PEG grafting densities tended to produce more stable emulsions, suggesting that particles with high grafting densities and consequently high steric repulsion tended to repel and prevent formation of strong particle networks. Emulsions generated in DI coalesced more easily, indicating that electrostatic repulsion dominated relative to vdW attraction and that particle networks did not form. In brine, where electrostatic forces were screened out by counterions, the emulsions better resisted coalescence, consistent with the formation of a particle network. The strength of the network was inferred from the difference in emulsion stability to coalescence in DI and in brine. We measured a greater brine-DI stability difference of 3.7× for the larger 20 nm PEG-coated nanoparticles, compared with 3.3× and 2.2× for the 12 nm and 6 nm PEG-coated particles, respectively, further supporting the role of particle networks on emulsion stability.
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Bradford, I., T. Probert, D. Raymer, A. Ozbek, P. Primiero, E. Kragh, J. Drew, and C. Woerpel. "Application of Coalescence Microseismic Mapping to Hydraulic Fracture Monitoring Conducted Using a Surface Array." In 75th EAGE Conference and Exhibition incorporating SPE EUROPEC 2013. Netherlands: EAGE Publications BV, 2013. http://dx.doi.org/10.3997/2214-4609.20131028.

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Lu, Yaojun, John J. Greene, and Madhusuden Agrawal. "CFD Characterization of Liquid Carryover in Gas/Liquid Separator with Droplet Coalescence due to Vessel Internals." In SPE Annual Technical Conference and Exhibition. Society of Petroleum Engineers, 2009. http://dx.doi.org/10.2118/124205-ms.

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Drozdov, A. N., N. A. Drozdov, N. F. Bunkin, and V. A. Kozlov. "Study of Suppression of Gas Bubbles Coalescence in the Liquid for Use in Technologies of Oil Production and Associated Gas Utilization." In SPE Russian Petroleum Technology Conference. Society of Petroleum Engineers, 2017. http://dx.doi.org/10.2118/187741-ms.

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Drozdov, A. N., N. A. Drozdov, N. F. Bunkin, and V. A. Kozlov. "Study of Suppression of Gas Bubbles Coalescence in the Liquid for Use in Technologies of Oil Production and Associated Gas Utilization (Russian)." In SPE Russian Petroleum Technology Conference. Society of Petroleum Engineers, 2017. http://dx.doi.org/10.2118/187741-ru.

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