activity
19992025
most citedCommon Envelope Evolution: Where we stand and how we can move forward

1k citations · 1.4k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.HE2025★ 16 cited

A pulsar-helium star compact binary system formed by common envelope evolution

Z. L. Yang, J. L. Han, D. J. Zhou +33

A stellar common envelope occurs in a binary system when the atmosphere of an evolving star expands to encompass an orbiting companion object. Such systems are predicted to evolve…

astro-ph.CO2020

The cosmic web through the lens of graph entropy

María Valentina García-Alvarado, Jaime E. Forero-Romero, Xiao-Dong Li

We explore the information theory entropy of a graph as a scalar to quantify the cosmic web. We find entropy values in the range between 1.5 and 3.2 bits. We argue that this entrop…

math.DG2020★ 6 cited

On the Shannon entropy power on Riemannian manifolds and Ricci flow

S. Li, X. -D. Li

In this paper, we prove the concavity of the Shannon entropy power for the heat equation associated with the Laplacian or the Witten Laplacian on complete Riemannian manifolds with…

astro-ph.HE2017★ 20 cited

Could the low braking index pulsar PSR J1734-3333 evolve into a magnetar?

Z. -F. Gao, D. -L. Song, Y. -L. Liu +3

The low braking-index pulsar PSR J17343333 could be born with superhigh internal magnetic fields G, and undergo a supercritical accretion soon af…

hep-ph2015

The Effects of Superhigh Magnetic Fields on Equations of States of Neutron Stars

Z. F. Gao, N. Wang, Y. Xu +2

By introducing Dirac ?-function in superhigh magnetic field, we deduce a general formula for pressure of degenerate and relativistic electrons, Pe, which is suitable for superhigh…

astro-ph.HE2015★ 108 cited

Constraining the Braking Indices of Magnetars

Z. F. Gao, X. D. Li, N. Wang +3

Due to the lack of long term pulsed emission in quiescence and the strong timing noise, it is impossible to directly measure the braking index of a magnetar. Based on the estim…