Qiu-he Peng graduated from Department of Astronomy, Nanjing University at 1960 firstly taught at Peking University for 18 years and then is teaching at Nanjing University. He is mainly engaged in nuclear astrophysics, particle astrophysics, and galactic astronomy research. In the field of nuclear astrophysics, his researches involve neutron stars (pulsars), the supernova explosion mechanism and the thermonuclear reaction inside the star, the synthesis of heavy elements and an interstellar radioactive element such as the origin of celestial 26Al. 225 papers of him have been published.

An anomaly strong radial magnetic field near the Galactic Center (GC) is detected . The lower limit of the radial magnetic field at r=0.12 pc from the GC.

 

Its Possible scientific significances are following:

 

The black hole model at the GC is incorrect. The reason is that  radiations observed from the region neighbor of the GC are hardly emitted by the gas of accretion disk due to it being prevented from approaching to the GC by the abnormally strong radial magnetic field.

 

This is an anticipated signals for existence of magnetic monopoles(MM). The lower limit of the detected radial magnetic field is quantitatively in agreement with the prediction of our paper “An AGN model with MM".

 

Magnetic monopoles may play a key role in some very important  astrophysical problems using the Robakov-Callen effect that nucleons may decay catalyzed by MM.

 

Taking the RC effect as an energy source, we have proposed a unified model for various supernova explosion, including to solve the question of the energy source both in the Earth core and in the white dwarfs.