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Chameleon Halo Modeling in f(R) Gravity     Chameleon  Halo Modeling  Gravity       font style='font-size:12px;'> 2011/10/21
We model the chameleon effect on cosmological statistics for the modified gravity f(R) model of cosmic acceleration. The chameleon effect, required to make the model compatible with local tests of gra...
To investigate the structure and composition of the dusty interstellar medium (ISM) of low surface brightness (LSB) disk galaxies, we have used multiwavelength photometry to construct spectral energy ...
We model the evolution of IR galaxies using a phenomenological approach to match the observed source counts at different IR wavelengths. We introduce a new algorithm for reproducing source counts base...
Morpho-Kinematic Modeling of Gaseous Nebulae with SHAPE     Morpho-Kinematic Modeling  Gaseous Nebulae       font style='font-size:12px;'> 2009/6/30
Morpho-Kinematic Modeling of Gaseous Nebulae with SHAPE。
Modeling the radial velocities and proper motions of herbig-haro objects。
The Trapezium Stars. Preliminary Results on Detailed Atmosphere Modeling
We study the temporal changes of the power law rigidity spectrum of the Forbush decrease (Fd) of the galactic cosmic ray (GCR) intensity. We show that the power law rigidity spectrum of Fd for the pe...
Modeling Repulsive Gravity with Creation      Cosmology  theory  observation  creation  negative energy fields  SNe Ia       font style='font-size:12px;'> 2009/5/12
There is a growing interest among cosmologists for theories with negative energy scalar fields and creation, in order to model a repulsive gravity. The classical steady state cosmology proposed by B...
Modeling Repulsive Gravity with Creation      Cosmology  theory  observation  creation  negative energy fields  SNe Ia       font style='font-size:12px;'> 2010/9/16
There is a growing interest among cosmologists for theories with negative energy scalar fields and creation, in order to model a repulsive gravity. The classical steady state cosmology proposed by Bon...

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