scholarly journals On the role of density inhomogeneity and local anisotropy in the fate of spherical collapse

1998 ◽  
Vol 237 (3) ◽  
pp. 113-118 ◽  
Author(s):  
L Herrera ◽  
A Di Prisco ◽  
J.L Hernández-Pastora ◽  
N.O Santos
2019 ◽  
Vol 34 (02) ◽  
pp. 1950012 ◽  
Author(s):  
M. Z. Bhatti ◽  
Z. Yousaf ◽  
A. Yousaf

Assuming a system with spherical symmetry in f(R) gravity filled with dissipative charged and anisotropic matter, we study the impact of density inhomogeneity and local anisotropy on the gravitational collapse in the presence of charge. For this purpose, we evaluated the modified Maxwell field equations, Weyl curvature tensor, and the mass function. Using Misner–Sharp mass formalism, we construct a relation between the Weyl tensor, density inhomogeneity, and local anisotropy. Specifically, we obtain the expression of modified Tolman mass which helps to analyze the influence of charge and dark source terms on different physical factors, also it helps to study the role of these factors on gravitational collapse.


2019 ◽  
Vol 99 (8) ◽  
Author(s):  
Vladislav D. Kurilovich ◽  
Pavel D. Kurilovich ◽  
Igor S. Burmistrov ◽  
Moshe Goldstein

1996 ◽  
Vol 152 (1-2) ◽  
pp. 17-21 ◽  
Author(s):  
J.F. Calleja ◽  
M.C. Contreras ◽  
M. Rivas ◽  
J.A. Corrales ◽  
G. Suran ◽  
...  

2021 ◽  
Author(s):  
Ganapati Sahoo ◽  
Soumak Bhattacharjee ◽  
Andrey Debolsky ◽  
Evgeny Kadanstev ◽  
Evgeny Mortikov ◽  
...  

<p>Turbulent flows within and above urban and vegetative canopies in the atmospheric boundary layer have profound implications for a variety of important problems in  agricultural  and urban meteorology, such as the spreading of pollens and pollutants. We study such turbulence via Direct Numerical Simulations (DNSs), by using the code developed in (2019 Mortikov),  in which there is a closed channel between two parallel walls and a canopy of constant areal density profile on the lower wall. We impose periodic boundary conditions in the horizontal directions and a no-slip impenetrable boundary condition in the wall-normal direction. For the canopy, we use different formulations of the Forchheimer drag. We assess the role of the canopy on the turbulent flow. In particular, we show the influence of added drag on the mean profiles, balance equations of the second-order moments, and the local anisotropy of the flow.</p><p>We observe that the turbulence transport profile undergoes an abrupt transition at the canopy top and transfer of energy from the roughness sublayer above the canopy to inside the canopy.  <br>The pressure-strain correlation removes energy from the wall-normal fluctuations, which has the least share of the turbulent kinetic energy and distributes it among the other components in the bulk of the canopy. In the inertial range, within and above the canopy, the energy spectra for the streamwise component is steeper than the spanwise and the wall-normal components and is closer to the Kolmogorov -5/3 spectrum as observed in the eddy covariance measurements in the roughness sublayer (2020 Bhattacharjee).</p><p>We thank the DST, CSIR (India), SERC (IISc) for computational resources, the AtMath Collaboration at the University of Helsinki, and ICOS by University of Helsinki for their support. This study was also partially funded by RFBR project number 20-05-00776.</p><p>Reference</p><p>2019, Mortikov, E. V., Glazunov, A. V., & Lykosov, V. N. Numerical study of plane Couette flow: turbulence statistics and the structure of pressure–strain correlations, Russian Journal of Numerical Analysis and Mathematical Modelling, 34(2), 119-132. doi: https://doi.org/10.1515/rnam-2019-0010.</p><p>2020, Bhattacharjee S., Pandit R., Vesala T., Mammarella I., Katul G., and Sahoo G. Anisotropy and multifractal analysis of turbulent velocity and temperature in the roughness sublayer of a forested canopy, arXiv:2010.04194.</p>


2004 ◽  
Vol 69 (6) ◽  
Author(s):  
Pankaj S. Joshi ◽  
Rituparno Goswami

2011 ◽  
Vol 20 (09) ◽  
pp. 1689-1703 ◽  
Author(s):  
L. HERRERA

We identify the factors responsible for the appearance of energy density inhomogeneities in a self-gravitating fluid, and describe the evolution of those factors from an initially homogeneous distribution. It is shown that a specific combination of the Weyl tensor and/or local anisotropy of pressure and/or dissipative fluxes entails the formation of energy density inhomogeneities. Different cases are analyzed in detail and in the particular case of dissipative fluids, the role of relaxational processes as well as nonlocal effects are brought out.


2010 ◽  
Vol 97 (23) ◽  
pp. 232511 ◽  
Author(s):  
Gino Hrkac ◽  
Thomas G. Woodcock ◽  
Colin Freeman ◽  
Alexander Goncharov ◽  
Julian Dean ◽  
...  

JAMA ◽  
1966 ◽  
Vol 195 (12) ◽  
pp. 1005-1009 ◽  
Author(s):  
D. J. Fernbach
Keyword(s):  

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