Outline Introduction Why nuclear force(baryon-baryon interaction) Current status Our aim—a relativistic baryon-baryon force Advantages of a covariant formulati
Status of BOUT++code neutral transport Radial neutral propagation during SMBI 3D SMBI Simulations in HL-2A Validations with HL-2A experiment,consisting well wit
Present status of the inflationary scenario Physical scales related to inflation Visualizing small differences in the duration of inflation Model reconstruction
Outline Cosmological Implications:Why do we need the interaction between DE&DM?Perturbation theory when DE&DM are in interaction Observational Signatures:Is the