activity
20002026
most citedThe physics of strong magnetic fields in neutron stars

57 citations · 213 across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.GA2026

A new model of quasar mass evolution

Z. Li, M. Zhang, Q. -H. Peng +1

Magnetic monopoles have been a trending topic among physicists and astronomers since the 1930s. Researchers have been working hard to find evidence of magnetic monopoles in laborat…

astro-ph.HE2022★ 4 cited

Neutrino Rocket Jet Model: An Explanation of High-velocity Pulsars and their Spin-down Evolution

Zheng Li, Qiu-He Peng, Miao Kang +4

The fact that the spatial velocity of pulsars is generally higher than that of their progenitor stars has bothered astronomers for nearly 50 years. It has been extensively argued t…

physics.gen-ph2020★ 9 cited

A Magnetic-Monopole-Based Mechanism to the formation of the Hot Big Bang Modeled Universe

Qiu-He Peng, Jing-Jing Liu, Chi-Kang Chou

There are some particle physics theories that go beyond the so-called "standard cosmological model" to predict the existence of magnetic monopoles\,(MMs). The discovery of magnetic…

astro-ph.HE2018

The Physical Essence of Pulsar Glitch

Qiu-He Peng, Jing-Jing Liu, Chih-Kang Chou

Based on the magnetic dipole radiation from the 3P2 neutron superfluid vortices (3P2NSFV) in neutron stars, we propose a model of glitch for young pulsars by oscillation between B…

astro-ph.HE2017★ 7 cited

A unified model of supernova driven by magnetic monopoles

Qiu-He Peng, Jing-Jing Liu, Chih-Kang Chou

In this paper, we first discuss a series of important but puzzling physical mechanisms concerning the energy source, various kinds of core collapsed supernovae explosion mechanisms…

nucl-th2017★ 13 cited

Strongly screening electron capture rates of chromium isotopes in presupernova

Jing-Jing Liu, Qiu-He Peng, Liang-Huan Hao +2

Taking into account the effect of electron screening on the electron energy and electron capture threshold energy, by using the method of Shell-Model Monte Carlo and Random Phase A…