supported by the National Natural Science Foundation of China(Grant Nos.11405024 and 11175042);the Fundamental Research Fundsfor the Central Universities(Grant Nos.N130305007 and N120505003)
Previous studies have shown that for the Supernova Legacy Survey three-year (SNLS3) data there is strong evidence for the redshifl- evolution of color-luminosity parameter β of type Ia supernovae (SN Ia). In this...
supported by the National Natural Science Foundation of China (Grant No. 11175042);the National Ministry of Education of China (Grant No. N120505003)
In this work, we constrain the spectral index nt of the primordial gravitational wave power spectrum in a universe with sterile neutrinos by using the Planck temperature data, the WMAP 9-year polarization data, the ba...
supported by the National Natural Science Foundation of China(Grant Nos.10975032 and 11175042);the National Ministry of Education of China(Grants Nos.NCET-09-0276,N110405011 and N120505003);the Provincial Department of Education of Liaoning(Grant No.L2012087)
In this paper, a new version of the interacting model of new agegraphic dark energy (INADE) is proposed and analyzed in detail. The interaction between dark energy and dark matter is reconsidered. The interaction te...
Project supported by the National Natural Science Foundation of China (Grant Nos. 10705041,10975032,11047112,and 11175042);the Program for New Century Excellent Talents at the University of Ministry of Education of China (Grant No. NCET-09-0276);the National Ministry of Education of China(Grant Nos. N100505001 and N110405011)
The initial condition Ωde(zini)=n^2(1+zini)^-2/4 at zini = 2000,widely used to solve the differential equation of the density of the new agegraphic dark energy(NADE) Ωde,makes the NADE model a single-paramete...