supported by the National Key R&D Program of China(2023YFA1607800,2023YFA1607803);the National Natural Science Foundation of China (NSFC,Grant Nos.11925303 and11890691);supported by the National Natural Science Foundation of China (NSFC,Grant No.12203062);by a CAS Project for Young Scientists in Basic Research (No.YSBR-092);supported by science research grants from the China Manned Space Project with No.CMS-CSST-2021-B01;supported by the New Cornerstone Science Foundation through the XPLORER prize。
We develop methods to extract key dark energy information from cosmic distance measurements including the BAO scales and supernova(SN) luminosity distances.Demonstrated using simulated data sets of the complete DESI,L...
supported by the National Key R&D Program of China(2023YFA1607800 and 2023YFA1607803);National Natural Science Foundation of China (NSFC,Grant Nos.11925303 and 11890691);supported by the National Natural Science Foundation of China (NSFC,Grant No.12203062);by a CAS Project for Young Scientists in Basic Research (No.YSBR-092);supported by science research grants from the China Manned Space Project with No.CMS-CSST-2021-B01;supported by the New Cornerstone Science Foundation through the XPLORER prize。
We extract key information on dark energy from current observations of BAO,OHD and H_(0),and find hints of dynamical behavior of dark energy.In particular,a dynamical dark energy model whose equation of state crosses-...
In the ΛCDM cosmological model, based on observations of supernovae Ia, the cosmic dark energy density is assumed to be Ω_(Λ)~ 0.70 and the gravitational mass density is assumed to be Ω_(m)~ 0.30. Based on the ass...
supported by the National Key Research and Development Program of China(No.2021YFA0718404);the National Natural Science Foundation of China(No.12220101003);the Project for Young Scientists in Basic Research of Chinese Academy of Sciences(No.YSBR-061)。
Precise measurements of the spectra of secondary and primary cosmic rays are crucial for understanding the origin and propagation of those energetic particles.The High Energy Cosmic-radiation Detection(HERD)facility o...
the National Natural Science Foundation of China(Grant Nos.12105032,11873001,12047564,12075041 and 12147102);the Fundamental Research Funds for the Central Universities of China(Grant Nos.2021CDJQY-011 and 2020CDJQY-Z003);the Science Foundation of Chongqing(Grant No.D63012022005);Chongqing Science and Technology research project(Grant No.KJ111206);the Natural Science Foundation of Chongqing(Grant No.cstc2021jcyj-msxm X0481);the Scientific Research and Innovation Project of Graduate Students in Chongqing(Grant No.CYS20272)。
Although the spatial curvature has been measured with very high precision,it still suffers from the well-known cosmic curvature tension.In this paper,we use an improved method to determine the cosmic curvature,by usin...
the National Key R&D Program of China(Grant No.2018YFE0202900);the National Natural Science Foundation of China(Grant No.11573030)。
Fast Fourier transform based estimators are formulated for measuring momentum power spectra,including the auto power spectra of the momentum,the momentum divergence,and the cross spectrum of density fluctuation and mo...
the National Natural Science Foundation of China(Nos.11633001,11920101003,11703034,11773032 and 11573031);the Strategic Priority Research Program of the Chinese Academy of Sciences(No.XDB23000000);the Interdiscipline Research Funds of Beijing Normal University;the NAOC Nebula Talents Program。
We investigate the relationship between cosmic curvature and model of dark energy(hereafter DE)with recent TypeⅠa supernovae(hereafter SNeⅠa)data,i.e.,the Pantheon sample including 1048 SNeⅠa with 0.01
With an initial requirement to make observations a minimum of 5–10 years,Hubble Space Telescope(HST)has continued to operate well for 30 years.It has relied upon five servicing missions to repair and replace essentia...
funded by the National Key Research and Development Program of China (2016YFA0400201);supported by the National Natural Science Foundation of China (11673047,11673075, 11303107, U1738127 and U1738205)
The DArk Matter Particle Explorer(DAMPE) is a space-borne apparatus for detecting the highenergy cosmic-ray-like electrons, γ-rays, protons and heavy ions. The Plastic Scintillator Detector(PSD)is the top-most sub-de...
The origin of the highest-energy particles in nature, ultra-high-energy(UHE) cosmic rays, is still unknown. In order to resolve this mystery, very large detectors are required to probe the low flux of these particles ...