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In this paper, we show that massive envelopes made of highly compressed normal matter surrounding dark objects (DEOs) can curve the surrounding spacetime and make the systems observationally indistinguishable from the...
Recently, it was argued that the energy density of the supranuclear dense matter inside the cores of massive neutron stars must have reached the , beyond which supranuclear dense matter becomes incompressible entropy-...
In view of the growing difficulties of ΛCDM-cosmologies to compete with recent highly accurate cosmological observations, I propose the alternative model: the Unicentric Model of the Observable UNiverse (UNIMOUN). Th...
It was argued that old and massive neutron stars end up as black objects that are made of purely incompressible superconducting gluon-quark superfluid matter (henceforth SuSu-objects). Based on theoretical investigati...
Recently, a unicentric model of our observable universe was proposed. Accordingly, the big bang was neither a singular event nor invoked by external forces, but rather a frequent event in cosmic life cycles that occur...
supported by the National Key R&D Program of China(Grant Nos.2020YFC2201400,2020SKA0120102,and 2016YFA0400704);the National Natural Science Foundation of China(Grant Nos.11690024,11873056,and 11991052);the Strategic Priority Program of the Chinese Academy of Sciences(Grant No.XDB 23040100);the Beijing Municipal Natural Science Foundation(Grant No.1204038)。
Quasars with periodic light curves are considered as candidates of supermassive binary black hole(BBH)systems.One way for further confirmations may be searching for other characteristic signatures,such as those in the...
support of a grant from the John Templeton Foundation and the National Astronomical Observatories, Chinese Academy of Sciences;the Subaru team and the National Natural Science Foundation of China (Grant No. 11890694);the National Natural Science Foundation of China (Grant Nos. 10173025, 10673013, 10778709, 11073031 and 11653005);the National Basic Research Program of China (973 Program, TG 2000077602)
High resolution deep imaging from space and adaptive optics techniques with large ground-based facilities have enabled studies examining faint host galaxies of high redshift quasi-stellar objects (QSOs). However, the ...
makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration;provided by the National Development and Reform Commission;supported by grants from the National Natural Science Foundation of China (Grant Nos. 11703065 and 11573054)
Quasars are essential for astrometry in the sense that they are spatially stationary because of their large distance from the Sun. The European Space Agency(ESA) astrometric satellite Gaia is scanning the whole sky wi...
the National Key Program for Science and Technology Research and Development(Grant No.2016YFA0400704);the National Natural Science Foundation of China(Grant Nos.11373031,and11390372);the Strategic Priority Program of the Chinese Academy of Sciences(Grant No.XDB 23040100)
Radiative efficiency is an important physical parameter that describes the fraction of accretion material converted to radiative energy for accretion onto massive black holes (MBHs). With the simplest Sottan argumen...
We have determined the Optical Luminosity Function (OLF) of a sample of 80946 Quasi Stellar Objects (QSOs) taken from the Sloan Digital Sky Survey Data Release Seven (SDSS DR7) with redshift range??0.3 z Mi < -22.5. T...