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Xiaoxuan Liu

6 papers hereh-index 328 citations8 works total

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

author position
  • first author1
  • middle author5

Across the 6 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE6
same name
  • Xiaoxuan Liu — 7 papers, h 7
  • Xiaoxuan Liu — 6 papers, h 4
  • Xiaoxuan Liu — 5 papers, h 6
  • Xiaoxuan Liu — 4 papers, h 3
  • Xiaoxuan Liu — 3 papers, h 2
  • Xiaoxuan Liu — 2 papers, h 3

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

activity
20242026
collaborators
Showing 2025Show all

3 papers · 1 filter

astro-ph.HE2025

The color evolution of magnetar-powered kilonova emission in merging neutron star-neutron star systems

Suo-Ning Wang, Hou-Jun Lü, Xiao-Xuan Liu +3

The first direct detection of the gravitational wave (GW) event GW170817 and its electromagnetic (EM) counterpart open a new window for studying of multi-messenger astronomy. Howev…

astro-ph.HE2025

Neutron Star-White Dwarf Merger as One Possible Optional Source of Kilonova-like Emission: Implications for GRB 211211A

Xiao-Xuan Liu, Hou-Jun Lü, Qiu-Hong Chen +2

Long-duration GRB 211211A, which lacked an associated supernova at such a low redshift z=0.076, but was associated with a possible kilonova emission, has attracted great attentio…

astro-ph.HE2025

How to identify the object with mass range of (2.2−3)M⊙​ in the merger of compact star systems

ZhaoWei Du, HouJun Lü, Xiaoxuan Liu +2

High-frequency gravitational-wave (GW) radiation has been detected by LIGO-Virgo-KAGRA in the merger of compact stars. However, two GW events, GW190814 and GW200210, the mass of on…

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