After graduated from Department of Astronomy, Nanjing University at 1960, Qiu-he Peng teached at Peking University for 18 years and then is teaching at Nanjing University.

Q. Peng is mainly engaged in nuclear astrophysics , particle astrophysics and galactic astronomy research. In the field of nuclear astrophysics, Peng’s researches involve neutron stars (pulsars), the supernova explosion mechanism and the thermonuclear reaction inside the star, the synthesis of heavy elements and interstellar radioactive element such as the origin of celestial 26Al. 226 papers of him have be published.

In recent 10 years, his works are mainly on the astrophysics with both particle physics and condensed matter physics.

Papers in recent years

1. Q. Peng et al., 2014,
   “Error Analysis of Ia Supernova and Query on Cosmic Dark Energy”
   J. Astrophys. Astr. (2014)35, 253-256 (Indian Academy of Sciences)

2. Q. Peng et al., 2016,
   “Query on Accelerating Expansion of the Universe by Error Analysis of Ia Supernova”
   Nuclear Physics in Astrophysics VI (NPA6), IOP Publishing, Journal of Physics: Conference Series 665 (2016)
   012073

3. Q. Peng et al., 2016,
   “Origin of Strong Magnetic Fields of Magnetars“
   Universal Journal of Physics and Application 10(3): 68-71, 2016

4. Q. Peng et al., 2016,
   “The Physics of Magnetars II - The Electron Fermi Energy of and the Origin of High X-ray Luminosity of Magnetars“
   Universal Journal of Physics and Application 10(3): 72-79, 2016

5. Q. Peng et al., 2016,
   “A possible influence on standard model of quasars and active galactic nuclei in strong magnetic field“
   Astrophys Space Sci (2016) 361:388

6. Q. Peng et al., 2017,
   “Some new possible anticipated signals for existence of magnetic monopoles“
   New Astronomy, 57 (2017)59-62

7. Q. Peng et al., 2017,
   “A unified model of supernova driven by magnetic monopoles“
   Astrophys Space Sci (2017) 362:222

For a complete list of papers, please click here.