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Relevant bibliographies by topics / Properties and evolution

Academic literature on the topic 'Properties and evolution'

Author: Grafiati

Published: 10 March 2023

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Journal articles on the topic "Properties and evolution"

1

Dzugan, Jan, and Pavel Konopik. "OS15F059 SMALL PUNCH TEST APPLICATION TO MATERIAL PROPERTIES EVOLUTION DETERMINATION." Abstracts of ATEM : International Conference on Advanced Technology in Experimental Mechanics : Asian Conference on Experimental Mechanics 2011.10 (2011): _OS15F059——_OS15F059—. http://dx.doi.org/10.1299/jsmeatem.2011.10._os15f059-.

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Dzugan, Jan, and Pavel Konopik. "OS15-3-1 SMALL PUNCH TEST APPLICATION TO MATERIAL PROPERTIES EVOLUTION DETERMINATION." Abstracts of ATEM : International Conference on Advanced Technology in Experimental Mechanics : Asian Conference on Experimental Mechanics 2011.10 (2011): _OS15–3–1—. http://dx.doi.org/10.1299/jsmeatem.2011.10._os15-3-1-.

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Camacho, L. M., J. R. Gomez, B. A. Omirov, and R. M. Turdibaev. "SOME PROPERTIES OF EVOLUTION ALGEBRAS." Bulletin of the Korean Mathematical Society 50, no. 5 (September 30, 2013): 1481–94. http://dx.doi.org/10.4134/bkms.2013.50.5.1481.

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Pantleon, Wolfgang, and Andy Horsewell. "Deformation structures: evolution and properties." Materials Science and Technology 21, no. 12 (December 2005): 1363. http://dx.doi.org/10.1179/174328405x74186.

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Dean, M. N., B. O. Swanson, and A. P. Summers. "Biomaterials: Properties, variation and evolution." Integrative and Comparative Biology 49, no. 1 (May 4, 2009): 15–20. http://dx.doi.org/10.1093/icb/icp012.

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Petrounia, Ioanna P., and Frances H. Arnold. "Designed evolution of enzymatic properties." Current Opinion in Biotechnology 11, no. 4 (August 2000): 325–30. http://dx.doi.org/10.1016/s0958-1669(00)00107-5.

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Bressan, A. "Properties of massive star evolution." Space Science Reviews 66, no. 1-4 (1994): 373–82. http://dx.doi.org/10.1007/bf00771086.

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Mereghetti, Sandro, José A. Pons, and Andrew Melatos. "Magnetars: Properties, Origin and Evolution." Space Science Reviews 191, no. 1-4 (March 25, 2015): 315–38. http://dx.doi.org/10.1007/s11214-015-0146-y.

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Latushkin, Yuri, and Yuri Tomilov. "Fredholm properties of evolution semigroups." Illinois Journal of Mathematics 48, no. 3 (July 2004): 999–1020. http://dx.doi.org/10.1215/ijm/1258131066.

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Bastolla, Ugo, Markus Porto, H. Eduardo Roman, and Michele Vendruscolo. "Statistical Properties of Neutral Evolution." Journal of Molecular Evolution 57 (August 1, 2003): S103—S119. http://dx.doi.org/10.1007/s00239-003-0013-4.

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Dissertations / Theses on the topic "Properties and evolution"

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Tabera, Martin Luis. "Evolution and properties of planetary systems." Thesis, Uppsala universitet, Observationell astrofysik, 2020. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-438128.

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Thelwall, Simon. "The properties of 4.1G : localisation, interactions and evolution." Thesis, University of Kent, 2006. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.429656.

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Groenewegen, Martin Arnold Theodoor. "On the evolution and properties of AGB stars." Amsterdam : Amsterdam : Sterrenkundig Instituut 'Anton Pannekoek' ; Universiteit van Amsterdam [Host], 1993. http://dare.uva.nl/document/91969.

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Pascut, Aurelia. "Evolution of X-ray properties of galaxy groups." Thesis, University of Birmingham, 2015. http://etheses.bham.ac.uk//id/eprint/6235/.

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This thesis presents the results from the Chandra Deep Group Survey, a survey dedicated to find high redshift groups of galaxies in deepest observations available in the Chandra archive. The catalogue compiled from this survey contains 26 groups and 36 clusters with available redshifts, with largest redshift being 1.3. This sample has been used to investigate the evolution of the thermal state of the gas at the centre of groups and compare this evolution to that of clusters. Different parameters have been used to quantify the strength of cool cores and it has been showed that groups and clusters have similar evolution of their cool core properties. Both classes of systems have a wide spread in the cool core strength at low redshifts, which then narrows at high redshifts showing a lack of strong cool core systems.

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Pascut, Aurelia. "Evolution of X-ray Properties of Galaxy Groups." Thesis, University of Birmingham (United Kingdom), 2017. http://pqdtopen.proquest.com/#viewpdf?dispub=10591255.

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Studies of scaling relations in groups and clusters of galaxies have shown that the X-ray properties of groups deviate the most from the self-similar prediction. This is because groups are more affected by non-gravitational processes due to their shallower potential well, a behaviour which makes groups an ideal class of systems for the study of the impact of feedback. From the observational point of view, the study of the X-ray properties of groups, especially at high redshifts is hindered by their lower surface brightness compared to their more massive counterparts. We present the result from the Chandra Deep Group Survey, a survey dedicated to find high redshift groups in the deepest observations available in the Chandra archive. We found 26 groups and 36 clusters with available redshifts, with largest redshift being 1.3. We have used this sample to investigate the evolution of cool cores in these two classes of systems using cooling time divided by the age of the cluster as a parameter to describe the cooling state. We have found that groups and clusters have similar evolution in their cool core properties. Both classes of systems have a wide spread in the cool core parameter at low redshifts, which then narrows at high redshifts showing a lack of strong cool core systems.

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Durkalec, Anna. "Properties and evolution of galaxy clustering at 2." Thesis, Aix-Marseille, 2014. http://www.theses.fr/2014AIXM4758/document.

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Cette thèse porte sur l'étude des propriétés et l'évolution de regroupement de galaxies pour les galaxies de la gamme de 22. Je ai pu mesurer la distribution spatiale d'une population générale de galaxie à redshift z~3 pour la première fois avec une grande précision. Je ai quantifié le regroupement de galaxie en estimation et la modélisation de la fonction de corrélation projetée (espace réel) à deux points, pour une population générale de 3022 galaxies. Je ai prolongé les mesures de regroupement à la luminosité et des sous-échantillons de masse sélectionné stellaires. Mes résultats montrent que la force de regroupement de la population générale de la galaxie ne change pas de redshift z~3,5 à z~2,5, mais dans les deux redshift va plus lumineux et des galaxies plus massives sont plus regroupées que les moins lumineux (massives). En utilisant la distribution d'occupation de halo (HOD) formalisme je mesuré une masse moyenne de halo hôte au redshift z~3 significativement plus faible que les masses halo moyens observés à faible redshift. Je ai conclu que la population de formation d'étoiles observé des galaxies à z~3 aurait évolué dans le massif et lumineux la population de galaxies au z=0. Aussi, je interpréter les mesures de regroupement en termes de biais de galaxies à grande échelle linéaire. Je trouve que ce est nettement plus élevé que le biais des galaxies redshift intermédiaire et faible. Enfin, je ai calculé le ratio-stellaire Halo masse (SHMR) et l'efficacité intégrée de formation d'étoiles (ISFE) pour étudier l'efficacité de la formation des étoiles et l'assemblage masse stellaire
This thesis focuses on the study of the properties and evolution of galaxy clustering for galaxies in the redshift range 22. I was able to measure the spatial distribution of a general galaxy population at redshift z~3 for the first time with a high accuracy. I quantified the galaxy clustering by estimating and modelling the projected (real-space) two-point correlation function, for a general population of 3022 galaxies. I extended the clustering measurements to the luminosity and stellar mass-selected sub-samples. My results show that the clustering strength of the general galaxy population does not change significantly from redshift z~3.5 to z~2.5, but in both redshift ranges more luminous and more massive galaxies are more clustered than less luminous (massive) ones. Using the halo occupation distribution (HOD) formalism I measured an average host halo mass at redshift z~3 significantly lower than the observed average halo masses at low redshift. I concluded that the observed star-forming population of galaxies at z~3 might have evolved into the massive and bright (Mr<-21.5) galaxy population at redshift z=0. Also, I interpret clustering measurements in terms of a linear large-scale galaxy bias. I find it to be significantly higher than the bias of intermediate and low redshift galaxies. Finally, I computed the stellar-to-halo mass ratio (SHMR) and the integrated star formation efficiency (ISFE) to study the efficiency of star formation and stellar mass assembly. I find that the integrated star formation efficiency is quite high at ~16% for the average galaxies at z~3

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Dighe, Manish D. "Quantitative characterization of damage evolution in an Al-Si-Mg base cast alloy." Thesis, Georgia Institute of Technology, 1998. http://hdl.handle.net/1853/20219.

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Han, Jixiong. "Processing microstructure evolution and properties of nanoscale aluminum alloy." Cincinnati, Ohio : University of Cincinnati, 2005. http://www.ohiolink.edu/etd/view.cgi?acc%5Fnum=ucin1121701078.

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Thesis (Ph. D.)--University of Cincinnati, 2005.
Title from electronic thesis title page (viewed Apr. 11, 2006). Includes abstract. Keywords: Al-Cu nanoparticle; Al nanoparticle; Al-Al2O3 composite; 2024Al-Al2O3 composite; nanocomposite; nanoparticle; phase transformation; precipitate; plasma ablation; inert gas condensation; exploding wire; consolidation; sinter; cold roll; hot roll; aging; thermal-soaking; mechanical properties; strengthening mechanism. Includes bibliographical references.

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Slijkhuis, Sander. "On the properties and evolution of proto-planetary nebulae." Amsterdam : Amsterdam : Sterrenkundig Instituut 'Anton Pannekoek' ; Universiteit van Amsterdam [Host], 1991. http://dare.uva.nl/document/92056.

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Grigoriou, Georgios. "Structure evolving systems : model structure evolution and system properties." Thesis, City University London, 2012. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.576948.

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This thesis deals with a new paradigm for Complex Systems of an evolving structure which is referred to as Structure Evolving Systems (SES). A wide range of challenging issues are concerned involving the evolution of structure and associated system properties through different forms of complexity and these are closely related to integrated system design. The thesis deals specifically with issues related to the representation of t.he different forms of structural evolut.ion. A number of new forms of evolution are introduced expressing differ- ent design problems, such as Design Time Evolution, Dimensional Graph Evolution, Life Cycle Structural Evolution, Cascade Design Evolution. The main objective is to develop a representation framework for the different types of structural evolution which will offer the proper set up for the study of evolution of structural characteristics and system prop- erties. The main part of the study is concerned with the development of representation of the System Structure Evolution in terms of a chain of models as a way to represent the different stages of Design Time Evolution which involves the modelling of a system from the very early stages up to the late stages when detailed descriptions are used for design. The development of nested representations for the case of Single-Input, Single-Output Systems is presented here based on the theory of continuous fraction expansion of rational functions and then examine property evolution within the naturally generated nests. A " natural" way for generating chains of models of variable complexity is introduced based on a frequency domain approach using the infinite Laurent expansion. This approach provides a natural link to the problem of partial realization, which in turn provides a useful set up for tpe study of evolution of system structure and properties. Within the framework of Cascade Design Evolution, we develop a generic representation describing the evolution from the aggregate system to the composite system. This involves the development of the new concept of COTY1- pleteness of composition. We also clarify the notion of deviations from completeness ,; , develop a representation of the noncomplete composite system in terms of standard control concepts and tools. This provides the fundamentals for the development of a control theory based approach for designing composite systems with desirable structural characteristics. Within this framework, completeness is expressed as output feedback and deviations from completeness as input and output decentralized squaring down. This representation pro- vides control concepts and tools which allow the structuring of linear composite systems to be addressed as a problem of generalised control design. The present work contributes to the development of the theory of the new system paradigm and studies the evolution of a number of system properties under different types of system structure evolution.

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Books on the topic "Properties and evolution"

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J, Kemp S., Merriman R. J, British Geological Survey, and Mineralogical Society (Great Britain). Clay Minerals Group. Meeting, eds. Clay mineral evolution, basin maturity and mudrock properties. Keyworth, Nottingham, UK: British Geological Survey, 1998.

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Informational biopolymers of genes and gene expression: Properties and evolution. United States: University Science Bks, 2005.

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R, Mackinnon Ian D., and United States. National Aeronautics and Space Administration., eds. Cometary evolution: Clues on physical properties from chondritic interplanetary dust particles. [Washington, DC: National Aeronautics and Space Administration, 1989.

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R, Mackinnon Ian D., and United States. National Aeronautics and Space Administration., eds. Cometary evolution: Clues on physical properties from chondritic interplanetary dust particles. [Washington, DC: National Aeronautics and Space Administration, 1989.

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R, Mackinnon Ian D., and United States. National Aeronautics and Space Administration., eds. Cometary evolution: Clues on physical properties from chondritic interplanetary dust particles. [Washington, DC: National Aeronautics and Space Administration, 1989.

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Kuznet︠s︡ov, A. N. Plany stroenii︠a︡ konechnosteĭ i ėvoli︠u︡t︠s︡ii︠a︡ tekhniki bega u tetrapod. Moskva: Izd-vo Moskovskogo gos. universiteta, 1999.

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Space Telescope Science Institute (U.S.) and United States. National Aeronautics and Space Administration., eds. Radio and infrared properties of young stars. Baltimore, MD: Space Telescope Science Institute, 1987.

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D, Kerr Arnold, Santare Michael H. 1959-, and Chajes Michael J, eds. The mechanics of solids: History and evolution : a festschrift in honor of Arnold D. Kerr. Newark, N.J: University of Delaware Press, 2008.

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Green, David W. Evolution of standardized procedures for adjusting lumber properties for change in moisture content. Madison, WI: U.S. Dept. of Agriculture, Forest Service, Forest Products Laboratory, 2001.

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The mammalian jaw: A mechanical analysis. Cambridge: Cambridge University Press, 2012.

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Book chapters on the topic "Properties and evolution"

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Bürger, Reinhard. "Mathematical properties of mutation-selection models." In Mutation and Evolution, 279–98. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5210-5_23.

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Ratner, Vadim A., Andrey A. Zharkikh, Nikolay Kolchanov, Sergey N. Rodin, Viktor V. Solovyov, and Andrey S. Antonov. "Dynamic Properties of Self-Reproducing Molecular Systems: Theoretical Analysis." In Molecular Evolution, 11–37. Berlin, Heidelberg: Springer Berlin Heidelberg, 1996. http://dx.doi.org/10.1007/978-3-662-12530-4_2.

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Bressan, A. "Properties of Massive Star Evolution." In Evolution of Massive Stars, 373–82. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1080-8_45.

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Tanvuia, L., W. W. Zeilinger, P. Focardi, B. Kelm, and R. Rampazzo. "Environmental Effects on Galaxy Properties." In The Evolution of Galaxies, 165–68. Dordrecht: Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-3315-1_29.

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Lewin, L. "The evolution of the ladder concept." In Structural Properties of Polylogarithms, 1–10. Providence, Rhode Island: American Mathematical Society, 1991. http://dx.doi.org/10.1090/surv/037/01.

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Holt, John A., and Michel Lepage. "Termites and Soil Properties." In Termites: Evolution, Sociality, Symbioses, Ecology, 389–407. Dordrecht: Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-017-3223-9_18.

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Kruszewski, A. "Evolution in Quasar Clustering Properties." In High Energy Astrophysics, 255–62. Berlin, Heidelberg: Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-73560-8_29.

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Bothun, G. "Greenhouse Gases: Properties and Evolution." In Encyclopedia of the UN Sustainable Development Goals, 1–17. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-319-71057-0_61-1.

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Mereghetti, Sandro, José A. Pons, and Andrew Melatos. "Magnetars: Properties, Origin and Evolution." In The Strongest Magnetic Fields in the Universe, 321–44. New York, NY: Springer New York, 2016. http://dx.doi.org/10.1007/978-1-4939-3550-5_10.

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Gerrard, A. J. "Landscape evolution and rock properties." In Rocks and Landforms, 55–84. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-011-5983-8_3.

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Conference papers on the topic "Properties and evolution"

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Parmar, Arvind. "The properties of accreting x-ray pulsars." In The evolution of X-ray binaries. AIP, 1994. http://dx.doi.org/10.1063/1.45982.

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Wachter, Stefanie. "Chandra Localizations of LMXBs: IR Counterparts and their Properties." In INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP, 2005. http://dx.doi.org/10.1063/1.2130304.

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Woo, Jonathan W., George W. Clark, and Fumiaki Nagase. "Properties of interstellar grains derived from x-ray eclipse observation." In The evolution of X-ray binaries. AIP, 1994. http://dx.doi.org/10.1063/1.45943.

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Raimundo, Sandra I., Andrew C. Fabian, A. Comastri, L. Angelini, and M. Cappi. "AGN properties in a cosmological evolution scenario." In X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Conference. AIP, 2010. http://dx.doi.org/10.1063/1.3475318.

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Balitsky, Ian, and Giovanni A. Chirilli. "Conformal Properties of Rapidity Evolution of TMDs." In INT Program INT-18-3. WORLD SCIENTIFIC, 2020. http://dx.doi.org/10.1142/9789811214950_0054.

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Matt, G. "The Properties of the Absorbing and Line Emitting Matter in IGR J16318-4848." In INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP, 2005. http://dx.doi.org/10.1063/1.2130275.

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Yoshida, T., N. Itagaki, and K. Katō. "Symplectic structure and transition properties of [sup 12]C." In ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2011. AIP, 2012. http://dx.doi.org/10.1063/1.4763441.

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Rud, A. D., A. M. Lakhnik, and I. M. Kirian. "Phase evolution in the Al-Mg system during mechanical alloying." In 2017 IEEE 7th International Conference "Nanomaterials: Application & Properties" (NAP). IEEE, 2017. http://dx.doi.org/10.1109/nap.2017.8190208.

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Olatunji, Obafemi, Stephen Akinlabi, Nkosinathi Madushele, Paul Adedeji, and Samuel Fatoba. "Evolution Algorithms and Biomass Properties Prediction: A Review." In ASME 2019 Power Conference. American Society of Mechanical Engineers, 2019. http://dx.doi.org/10.1115/power2019-1826.

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Abstract The complexity of real-world applications of biomass energy has increased substantially due to so many competing factors. There is an ongoing discussion on biomass as a renewable energy source and its cumulative impact on the environment vis-a-vis water competition, environmental pollution and so on. This discussion is coming at a time when evolutionary algorithms and its hybrid forms are gaining traction in several applications. In the last decade, evolution algorithms and its hybrid forms have evolved as a significant optimization and prediction technique due to its flexible characteristics and robust behaviour. It is very efficient means of solving complex global optimization problems. This article presents the state-of-the-art review of different types of evolutionary algorithms, which have been applied in the prediction of major properties of biomass such as elemental compositions and heating values. The governing principles, applications, merits, and challenges associated with this technique are elaborated. The future directions of the research on biomass properties prediction are discussed.

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Knobloch, Roman, Jaroslav Mlynek, and Radek Srb. "Improving convergence properties of a differential evolution algorithm." In APPLICATIONS OF MATHEMATICS IN ENGINEERING AND ECONOMICS (AMEE’16): Proceedings of the 42nd International Conference on Applications of Mathematics in Engineering and Economics. Author(s), 2016. http://dx.doi.org/10.1063/1.4968451.

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Reports on the topic "Properties and evolution"

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A. D. Rollett, D. J. Srolovitz, and A. Karma. Microstructural Evolution Based on Fundamental Interfacial Properties. Office of Scientific and Technical Information (OSTI), July 2003. http://dx.doi.org/10.2172/883040.

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Arraki, Kenza Sigrid. Evolution of dwarf galaxy properties in local group environments. Office of Scientific and Technical Information (OSTI), May 2016. http://dx.doi.org/10.2172/1491856.

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Fryer, Gerard J., Jill L. Karsten, and Roy H. Wilkens. Evolution of Porosity and Seismic Properties of Shallow Oceanic Crust. Fort Belvoir, VA: Defense Technical Information Center, November 1996. http://dx.doi.org/10.21236/ada319149.

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Osterkamp, T. E., and J. P. Gosink. An Investigation of Frazil and Anchor Ice: Formation, Properties, Evolution and Dynamics. Fort Belvoir, VA: Defense Technical Information Center, February 1985. http://dx.doi.org/10.21236/ada153041.

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Graber, Hans C., and Brian K. Haus. Evolution of the Directional Properties of Surface Waves Propagating across the Shelf. Fort Belvoir, VA: Defense Technical Information Center, September 2001. http://dx.doi.org/10.21236/ada626208.

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Green, David W., and James W. Evans. Evolution of standardized procedures for adjusting lumber properties for change in moisture content. Madison, WI: U.S. Department of Agriculture, Forest Service, Forest Products Laboratory, 2001. http://dx.doi.org/10.2737/fpl-gtr-127.

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Elena V. Belova, Ronald C. Davidson, Hantao Ji, and Masaaki Yamada. Kinetic Effects on the Stability Properties of Field-reversed Configurations: II. Nonlinear Evolution. Office of Scientific and Technical Information (OSTI), November 2003. http://dx.doi.org/10.2172/820209.

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Chen, Qian. Evolution, Interaction, and Intrinsic Properties of Dislocations in Intermetallics: Anisotropic 3D Dislocation Dynamics Approach. Office of Scientific and Technical Information (OSTI), January 2008. http://dx.doi.org/10.2172/939374.

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Zhang, Yida, Pania Newell, Yunping Xi, Andrea Tyrrell, Mitul Sisodiya, Xiang Zhou, Yao Wang, Yanbo Wang, and Bozo Vazic. Time-dependent THMC properties and microstructural evolution of damaged rocks in excavation damage zone. Office of Scientific and Technical Information (OSTI), November 2022. http://dx.doi.org/10.2172/1897054.

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Stubbins, James, Brent Heuser, Peter Hosemann, and Xiang Liu. Fundamental Studies of Irradiation-Induced Modifications in Microstructural Evolution and Mechanical Properties of Advanced Alloys. Office of Scientific and Technical Information (OSTI), April 2018. http://dx.doi.org/10.2172/1434640.

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