Standard

Geometry of the pore space and dynamic pore and cracked media deforming. / Sibiryakov, B.

в: Journal of Physics: Conference Series, Том 1141, № 1, 012075, 21.12.2018.

Результаты исследований: Научные публикации в периодических изданиях › статья по материалам конференции › Рецензирование

Harvard

Sibiryakov, B 2018, 'Geometry of the pore space and dynamic pore and cracked media deforming', Journal of Physics: Conference Series, Том. 1141, № 1, 012075. https://doi.org/10.1088/1742-6596/1141/1/012075

APA

Sibiryakov, B. (2018). Geometry of the pore space and dynamic pore and cracked media deforming. Journal of Physics: Conference Series, 1141(1), [012075]. https://doi.org/10.1088/1742-6596/1141/1/012075

Vancouver

Sibiryakov B. Geometry of the pore space and dynamic pore and cracked media deforming. Journal of Physics: Conference Series. 2018 дек. 21;1141(1):012075. doi: 10.1088/1742-6596/1141/1/012075

Author

Sibiryakov, B. / Geometry of the pore space and dynamic pore and cracked media deforming. в: Journal of Physics: Conference Series. 2018 ; Том 1141, № 1.

BibTeX

@article{0c63020b36fc47aebd2b5757f2e43a57,
title = "Geometry of the pore space and dynamic pore and cracked media deforming",
abstract = "In this paper presents the elements of blocked media deforming theory. It means that these media have a specific surface and (related with it) average distance from one crack (pore) to another one. This way requires the creation a new model of continuum, which is contains the integral geometry of pore space. The equations of motion and equilibrium are equations of the infinite order due to infinite numbers of freedom degrees. Along the usual seismic waves, these equations describe very slow waves, not bounded below and, besides of it, they predict the instable solutions, due to parametric resonances in structures bodies. The number of instable solutions corresponds to seismological Gutenberg-Richter law. The dispersion of an average size of structure produces both the fast catastrophes (small dispersion) and slow catastrophes (high dispersion).",
author = "B. Sibiryakov",
note = "Publisher Copyright: {\textcopyright} 2018 Institute of Physics Publishing. All rights reserved.; 7th International Conference on Mathematical Modeling in Physical Sciences, IC-MSQUARE 2018 ; Conference date: 27-08-2018 Through 31-08-2018",
year = "2018",
month = dec,
day = "21",
doi = "10.1088/1742-6596/1141/1/012075",
language = "English",
volume = "1141",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",

}

RIS

TY - JOUR

T1 - Geometry of the pore space and dynamic pore and cracked media deforming

AU - Sibiryakov, B.

N1 - Publisher Copyright: © 2018 Institute of Physics Publishing. All rights reserved.

PY - 2018/12/21

Y1 - 2018/12/21

N2 - In this paper presents the elements of blocked media deforming theory. It means that these media have a specific surface and (related with it) average distance from one crack (pore) to another one. This way requires the creation a new model of continuum, which is contains the integral geometry of pore space. The equations of motion and equilibrium are equations of the infinite order due to infinite numbers of freedom degrees. Along the usual seismic waves, these equations describe very slow waves, not bounded below and, besides of it, they predict the instable solutions, due to parametric resonances in structures bodies. The number of instable solutions corresponds to seismological Gutenberg-Richter law. The dispersion of an average size of structure produces both the fast catastrophes (small dispersion) and slow catastrophes (high dispersion).

AB - In this paper presents the elements of blocked media deforming theory. It means that these media have a specific surface and (related with it) average distance from one crack (pore) to another one. This way requires the creation a new model of continuum, which is contains the integral geometry of pore space. The equations of motion and equilibrium are equations of the infinite order due to infinite numbers of freedom degrees. Along the usual seismic waves, these equations describe very slow waves, not bounded below and, besides of it, they predict the instable solutions, due to parametric resonances in structures bodies. The number of instable solutions corresponds to seismological Gutenberg-Richter law. The dispersion of an average size of structure produces both the fast catastrophes (small dispersion) and slow catastrophes (high dispersion).

UR - http://www.scopus.com/inward/record.url?scp=85059424825&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/1141/1/012075

DO - 10.1088/1742-6596/1141/1/012075

M3 - Conference article

AN - SCOPUS:85059424825

VL - 1141

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012075

T2 - 7th International Conference on Mathematical Modeling in Physical Sciences, IC-MSQUARE 2018

Y2 - 27 August 2018 through 31 August 2018

ER -

ID: 18071865