X. D. Sheng

ORCID: 0009-0007-2375-2327
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About
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Research Areas
  • Gamma-ray bursts and supernovae
  • Astrophysics and Cosmic Phenomena
  • Dark Matter and Cosmic Phenomena
  • Astrophysical Phenomena and Observations
  • Neutrino Physics Research
  • Particle physics theoretical and experimental studies
  • High-pressure geophysics and materials
  • Cosmology and Gravitation Theories
  • Solar and Space Plasma Dynamics
  • Pulsars and Gravitational Waves Research
  • Geophysics and Gravity Measurements
  • Noncommutative and Quantum Gravity Theories
  • Astronomical Observations and Instrumentation

University of California, Santa Barbara
2023

Institute of High Energy Physics
2009

We report on the search for gamma ray bursts (GRBs) in energy range 1–100 GeV coincidence with prompt emission detected by satellites using Astrophysical Radiation Ground-based Observatory at YangBaJing (ARGO-YBJ) air shower detector. Thanks to its mountain location (Yangbajing, Tibet, People's Republic of China, 4300 m above sea level), active surface (∼6700 m2 Resistive Plate Chambers), and large field view (∼2 sr, limited only atmospheric absorption), ARGO-YBJ detector is particularly...

10.1088/0004-637x/699/2/1281 article EN The Astrophysical Journal 2009-06-19

We present relativistic, radiation magnetohydrodynamic simulations of supercritical neutron star accretion columns in Cartesian geometry, including temperature-dependent, polarization-averaged Rosseland mean opacities accounting for classical electron scattering a magnetic field. Just as our previous pure Thomson simulations, vertical oscillations the shock and horizontally propagating entropy waves (photon bubbles) are all simulations. However, at high fields $\gtrsim10^{12}$~G, produce...

10.1093/mnras/stad2043 article EN Monthly Notices of the Royal Astronomical Society 2023-07-07
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