Results 51 to 60 of about 1,721,894 (339)
Preface: High energy astrophysics [PDF]
High energy astrophysics is one of the most active branches in the contemporary astrophysics. It studies astrophysical objects that emit X-ray and γ-ray photons, such as accreting super-massive and stellar-size black holes, and various species of neutron stars.
Bing Zhang, Peter Mésáros
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Chat computational fluid dynamics (CFD) introduces an large language model (LLM)‐driven agent that automates OpenFOAM simulations end‐to‐end, attaining 82.1% execution success and 68.12% physical fidelity across 315 benchmarks—far surpassing prior systems.
E Fan +8 more
wiley +1 more source
HARPO - TPC for High Energy Astrophysics and Polarimetry from the MeV to the GeV
Observation of high-energy sources requires gamma-ray telescopes aboard balloons or satellites to study non thermal phenomena (black holes, neutron stars, active galactic nuclei, supernovae, supernova remnants, and gamma-ray bursts). In recent years, R&D
P. Gros
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ABSTRACT The objective of the current research is to characterize the thermal performance in micropolar fluid flows on a vertically elongated porous sheet in the presence of buoyancy forces. Thus, the motivation of this study is to improve the understanding of buoyancy‐driven micropolar fluid flows through porous media, which are relevant to advanced ...
T. Venu, MD. Shamshuddin, S. O. Salawu
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The development of the atmospheric Cherenkov imaging technique has led to significant advances in gamma-ray detection sensitivity in the energy range from 200 GeV to 50 TeV. The Whipple Observatory 10m reflector has detected the first galactic and extragalactic sources in the Northern Hemisphere; the Crab Nebula has been established as the standard ...
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Very-high-energy gamma-ray emission from GRB 201216C detected by MAGIC
Institute for Cosmic Ray Research, The University of Tokyo, Kashiwanoha 5-1-5, Kashiwa, Japan Max Planck Institut for Physics,Föhringer Ring 6, Munich, Germany INFN MAGIC Group: INFN Sezione di Bari and Dipartimento Interateneo di Fisica dell’Università ...
S. Fukami +194 more
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ABSTRACT Planetary nebulae represent a late evolutionary phase of low‐ to intermediate‐mass stars. In this article, we present the serendipitous discovery of a previously unknown, faint potential Galactic planetary nebula (PN) in the constellation Camelopardalis, identified during a survey‐inspection, aiming at the detection of dwarf companions of the ...
W. E. Celnik +12 more
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Preface for Special Issue of Frontiers of Physics dedicated to High Energy Astrophysics, 3 ...
Zhang, Bing, Meszaros, Peter
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High-energy astrophysics and cosmology [PDF]
12 pages, 16 eps figures, uses espcrc2.sty. Talk presented at the XIIth International Symposium on Very-High-Energy Cosmic-Ray Interactions, CERN, July ...
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Filter transmittance calibration of the follow-up x-ray telescope on board the EP satellite
The Einstein Probe satellite is equipped with two payloads, one of which is the Follow-up X-ray Telescope (FXT). The FXT comprises two completely independent optical and detector systems: FXT-A and FXT-B.
Jingjing Xu +20 more
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