supported by the National Natural Science Foundation of China(Grant Nos.11275035,11675032,11322545,11335012,and11575271);"the Fundamental Research Funds for the Central Universities"(Grant No.DUT16LK31);the Top-Notch Young Talents Program of China;the Key Research Program of Frontier Sciences,Chinese Academy of Sciences
The neutrino oscillations imply that at least two neutrinos have non-zero masses[1].However,up to now,we only measure the differences of neutrino mass squares in a standard scenario with three massive eigenstates[2],i.e.
supported in part by the National Natural Science Foundation of China(11690021,11690022,11690023,11622546,11575272,11375260 and 11335012);the Strategic Priority Research Program of CAS(XDB23030100);the Key Research Program of Frontier Sciences of CAS(QYZDJ-SSWSYS006)
The direct detection of gravitational wave by Laser Interferometer Gravitational-Wave Observatory indicates the coming of the era of gravitational-wave astronomy and gravitational-wave cosmology. It is expected that m...
supported by the National Natural Science Foundation of China(Grant Nos.11405024,11275247,and 11335012);the Fundamental Research Funds for the Central Universities(Grant No.16lgpy50);a985 grant at Sun Yat-Sen University
In this work, we explore the cosmological implications of different baryon acoustic oscillation (BAO) data, including the BAO data extracted by using the spherically averaged one-dimensional galaxy clustering (GC)...
Supported by National Natural Science Foundation of China(11305181,11322545,11335012);Open Project Program of State Key Laboratory of Theoretical Physics,Institute of Theoretical Physics,Chinese Academy of Sciences,China(Y5KF181CJ1)
The power spectrum of primordial tensor perturbations Pt increases rapidly in the high frequency region if the spectral index nt 〉 0. It is shown that the amplitude of relic gravitational waves ht (5×109 Hz) varie...
Supported by National Natural Science Foundation of China(11375203,11305181,11322545,11335012);Knowledge Innovation Program of The Chinese Academy of Sciences
In some quantum gravity theories, a foamy structure of space-time may lead to Lorentz invariance violation(LIV). As the most energetic explosions in the Universe, gamma-ray bursts(GRBs) provide an effect way to pr...
supported by the project of Knowledge Innovation Program of Chinese Academy of Sciences,and the National Natural Science Foundation of China(Grant Nos.10821504,11322545 and 11335012)
In this paper we propose a new inflation model named( p, q) inflation model in which the inflaton potential contains both positive and negative powers of inflaton field in the polynomial form. We derive the accurate p...
supported by the Project of Knowledge Innovation Program of Chinese Academy of Science,National Natural Science Foundation of China(Grant Nos.11322545 and 11335012)
Even though the Hubble constant cannot be significantly determined just by the low-redshift Baryon Acoustic Oscillation(BAO)data, it can be tightly constrained once the high-redshift BAO data are combined. We combined...
supported by the National Natural Science Foundation of China (Grant Nos. 10821504, 11322545, 11335012, 11173021 and 11322324);the Project of KIP of the Chinese Academy of Sciences and the National Basic Research Program of China (Grant No. 2012CB821804)
Recently Background Imaging of Cosmic Extragalactic Polarization (B2) discovered the relic gravitational waves at 7.00- confi- dence level. However, the other cosmic microwave background (CMB) data, for example Pl...
supported by the National Natural Science Foundation of China (Grant Nos. 11275247 and 11335012);XDL acknowledges suport from the KDES program
We investigate a second order parabolic parametrization, w(a) = wt + wa(at - a)2, which is a direct characterization of a possible turning in w. The cosmological consequence of this parametrization is explored by...