Fractal nature of cluster systems

The article analyzes the correlation between the screen reality and the first-order reality in the digital culture. Specific concepts of the scientific paradigm of the late 20th century are considered as constituent principles of the on-screen reality of the digital epoch. The study proves that the post-non-classical cultural world view, emerging from the dynamic “chaos” of informational and semantic rows of TV programs and cinematographic narrations, is of a fractal nature. The article investigates different types of fractality of the TV content and film plots, their inner and outer “strange loops” and artistic interpretations of the “butterfly effect”.

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Cross-polarization kinetics and fractal nature of thermal equilibration in spin systems: From low-dimensional proton conductors to tripeptides

Journal of Physics and Chemistry of Solids ◽

10.1016/j.jpcs.2021.109946 ◽

2021 ◽

Vol 152 ◽

pp. 109946

Author(s):

Laurynas Dagys ◽

Vytautas Klimavicius ◽

Martin Brodrecht ◽

Gerd Buntkowsky ◽

Vytautas Balevicius

Keyword(s):

Spin Systems ◽

Proton Conductors ◽

Cross Polarization ◽

Fractal Nature ◽

Thermal Equilibration ◽

Low Dimensional

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ChemInform Abstract: HETERONUCLEAR CLUSTER SYSTEMS, XI. PREPARATION, PROPERTIES, AND MOLECULAR STRUCTURES OF TITANIUM-, ZIRCONIUM-, AND HAFNIUM-SUBSTITUTED OXYMETHYLIDYNE-TRICOBALTNONCARBONYL CLUSTER COMPOUNDS

Chemischer Informationsdienst ◽

10.1002/chin.197826284 ◽

1978 ◽

Vol 9 (26) ◽

Author(s):

B. STUTTE ◽

V. BAETZEL ◽

R. BOESE ◽

G. SCHMID

Keyword(s):

Molecular Structures ◽

Cluster Compounds ◽

Cluster Systems ◽

Titanium Zirconium ◽

Heteronuclear Cluster

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Ages of Galactic and Extragalactic Star Clusters of Various Abundances

Highlights of Astronomy ◽

10.1017/s1539299600005025 ◽

1983 ◽

Vol 6 ◽

pp. 109-117 ◽

Cited By ~ 3

Author(s):

R.D. Cannon

Keyword(s):

Star Clusters ◽

Magellanic Clouds ◽

Open Clusters ◽

Simultaneous Solution ◽

Low Mass Stars ◽

Cluster Systems ◽

Distant Cluster ◽

Low Mass

In this review I shall concentrate mainly on globular star clusters in our Galaxy since these are the objects for which most work has been done recently, both observationally and theoretically. However, I shall also discuss briefly the oldest open clusters and clusters in the Magellanic Clouds. Little can be said about more distant cluster systems, since the only observations available are of integrated colours or spectra and these seem to be rather unreliable indicators of age. It is perhaps worth pointing out that the title may be slightly misleading; the problem is not so much to determine the ages of clusters of known abundances, as to obtain the best simultaneous solution for both age and composition, since some of the most important abundances (notably helium and oxygen) are virtually unobservable in little-evolved low mass stars.

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