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pro vyhledávání: '"Chang, Eonho"'
Autor:
Chang, Eonho, Youdin, Andrew N.
The Rossby wave instability (RWI) is the fundamental non-axisymmetric radial shear instability in disks. The RWI can facilitate disk accretion, set the shape of planetary gaps and produce large vortices. It arises from density and/or temperature feat
Externí odkaz:
http://arxiv.org/abs/2407.12722
High resolution sub-mm observations of protoplanetary disks with ALMA have revealed that dust rings are common in large, bright disks. The leading explanation for these structures is dust-trapping in a local gas pressure maximum, caused by an embedde
Externí odkaz:
http://arxiv.org/abs/2303.03469
Autor:
Chang, Eonho, Garaud, Pascale
Zahn's widely-used model for turbulent mixing induced by rotational shear has recently been validated (with some caveats) in non-rotating shear flows. It is not clear, however, whether his model remains valid in the presence of rotation, even though
Externí odkaz:
http://arxiv.org/abs/2107.03978
Autor:
Choi, Jinwoo, Chang, EonHo, Anstine, Dylan M., Madjet, Mohamed El-Amine, Chakraborty, Himadri S.
Publikováno v:
Phys. Rev. A 95, 023404 (2017)
We study the photoionization properties of the C_60 versus C_240 molecule in a spherical jellium frame of density functional method. Two different approximations to the exchange-correlation (xc) functional are used: (i) The Gunnerson-Lundqvist parame
Externí odkaz:
http://arxiv.org/abs/1610.00346
Akademický článek
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Autor:
Jinwoo Choi1, Chang, EonHo1, Anstine, Dylan M.1, Madjet, Mohamed El-Amine2, Chakraborty, Himadri S.1 himadri@nwmissouri.edu
Publikováno v:
Physical Review A: Atomic, Molecular & Optical Physics. Feb2017, Vol. 95 Issue 2, p1-1. 1p.
