◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

Wei-Hua Wang

3 papers hereh-index 344 citations9 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • hep-ph1
same name
  • Wei-Hua Wang — 5 papers, h 19
  • Wei-Hua Wang — 3 papers
  • Wei-Hua Wang — 2 papers, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedConstraining mechanism associated with fast radio burst and glitch from SGR J1935

13 citations · 16 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2022★ 1 cited

On torque reversal during delayed spin up glitch of SGR 1935+2154

Wei-Hua Wang, Ming-Yu Ge, Xi Huang +1

Ge et al. reported a peculiar large glitch observed from SGR 1935 recently~\citep{2022arXiv221103246G}. % Interestingly, this glitch occurred about 3.1±2.5 days before FR…

astro-ph.HE2021★ 13 cited

Constraining mechanism associated with fast radio burst and glitch from SGR J1935

Wei-Hua Wang, Heng Xu, Wei-Yang Wang +4

The discovery of fast radio burst (FRB) 200428 from galactic SGR J1935+2154 makes it possible to measure rotational changes accompanied by FRBs and to test several FRB models which…

astro-ph.HE2017★ 2 cited

Net reaction rate and neutrino emissivity for the Urca process in departure from chemical equilibrium

Wei-Hua Wang, Xi Huang, Xiao-Ping Zheng

We discuss the effect of compression on Urca shells in the ocean and crust of accreting neutron stars, especially in superbursting sources. We find that Urca shells may be deviated…

hep-ph2017★ 1 cited

Bondi accretion of dark matter by neutron stars

Xi Huang, Jian-Feng Liu, Wei-Hua Wang +2

In this paper, we have compared two different accretion mechanisms of dark matter particles by a canonical neutron star with M=1.4 M⊙​ and R=10 km, and shown the ef…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.