Chao-Jun Feng

Towards realisticf(T)models with nonminimal torsion-matter coupling extension

Using the observation data of SNeIa, CMB and BAO, we establish two concrete

THE CASIMIR FORCE OF QUANTUM SPRING IN THE (D+1)-DIMENSIONAL SPACETIME

f(T)

CASIMIR EFFECT WITH A HELIX TORUS BOUNDARY CONDITION

models with nonminimal torsion-matter coupling extension. We study in detail the cosmological implication of our models and find they are successful in describing the observation of the Universe, its large scale structure and evolution. In other words, these models do not change the successful aspects of

Fermionic Casimir effect with helix boundary condition

\Lambda

Action functional of the Cardassian universe

CDM scenario under the error band of fitting values as describing the evolution history of the Universe including radiation-dominated era, matter-dominated era and the present accelerating expansion. Meanwhile, the significant advantage of these models is that they could avoid the cosmological constant problem of

k-Inflation in noncommutative space–time

\Lambda

Some developments of the Casimir effect in p-cavity of (D + 1)-dimensional space–time

CDM. A joint analysis is performed by using the data of CMB+BAO+JLA, which leads to

Note on Power-Law Inflation in Noncommutative Space-Time

\Omega_{m0}=0.255\pm 0.010, \Omega_{b0}h^2=0.0221\pm 0.0003

CASIMIR EFFECT UNDER QUASI-PERIODIC BOUNDARY CONDITION INSPIRED BY NANOTUBES

and

Can be OPERA neutrino as tachyonic chameleon

H_0=68.54\pm 1.27