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Merging and Strip** Regimes in Close Pairs of Relativistic Stars: Prospects for Models of Short Gamma-Ray Bursts
We consider the current status of the binary neutron star strip** model to explain short gamma-ray bursts. After the historical joint detection of...
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X- and Gamma-Ray Astrophysics in the Era of Multi-messenger Astronomy
Multi-messenger astronomy is becoming a major avenue to explore the Universe. Several well-known astrophysical sources are also expected to emit...
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Compton Telescopes for Gamma-Ray Astrophysics
Compton telescopes rely on the dominant interaction mechanism in the MeV gamma-ray energy range: Compton scattering. By precisely recording the...
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Observational Consequences of $e^\pm$ Pair Creation in $\gamma$ -Ray Bursts
Physical models for $\gamma$ -ray emission from a relativistic...
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The technology for detection of gamma-ray burst with GECAM satellite
IntroductionThe main physical objective of the GECAM satellite is to detect gamma-ray bursts, which is related to gravitational waves of double...
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The INTEGRAL Burst Alert System
We describe the INTEGRAL Burst Alert System (IBAS): the automatic software developed at the INTEGRAL Science Data Center to allow the rapid...
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The Unique Signature of Shell Curvature in Gamma-Ray Bursts
As a result of sphericalkinematics, temporalev olution of received gammaray emission should demonstrate signatures of curvature from the emitting...
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Gammaless gamma-ray bursts?
One of the possible resolutions of the compactness problem in gamma-ray bursts (GRBs) is by invoking the Lorentz factors associated with the...
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Scintillation Detectors in Gamma-Ray Astronomy
Inorganic Scintillators and Organic Plastic Scintillators are widely used for many applications in modern-day observational astronomy and cosmic-ray...
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Coded Mask Instruments for Gamma-Ray Astronomy
Coded mask instruments have been used in high-energy astronomy for the last 40 years now, and designs for future hard X-ray/low gamma-ray telescopes...
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Gamma ray burst studies with THESEUS
Gamma-ray Bursts (GRBs) are the most powerful transients in the Universe, over–shining for a few seconds all other γ -ray sky sources. Their emission...
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A compact instrument for gamma-ray burst detection on a CubeSat platform II
The Gamma-ray Module, GMOD, is a miniaturised novel gamma-ray detector which will be the primary scientific payload on the Educational Irish Research...
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The Major Gamma-Ray Imaging Cherenkov Telescopes (MAGIC)
The MAGIC telescopes, located at Observatorio El Roque de los Muchachos (La Palma, Spain), are two Imaging Air Cherenkov Telescopes observing the...
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Time Domain Methods for X-Ray and Gamma-Ray Astronomy
A variety of statistical methods for understanding variability in the time domain for low count rate X-ray and gamma-ray sources are explored....
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Gamma-Ray Bursts
Gamma-ray bursts (GRBs) are short and intense bursts of ∼100 keV−1 MeV photons, usually followed by long-lasting decaying afterglow emission in a...
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Gamma-Ray Bursts as Probes for Quantum Gravity
Gamma ray bursts (GRBs) are short and intense pulses of γ-rays arriving from random directions in the sky. Several years ago Amelino-Camelia et al....
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Gamma-Ray Burst from Binary Star: Neutron Star and Carbon–Oxygen Core
AbstractWe investigate the scenario of a binary system composed by a neutron star (NS) and a main sequence star which has been stripped to be a naked...
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Pair Production Detectors for Gamma-Ray Astrophysics
Electron-positron pair production is the essential process for high-energy γ-ray astrophysical observations. Following the pioneering OSO-3 counter...
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Introduction to Ground-Based Gamma-Ray Astrophysics
The origin of cosmic rays, specifically the questions of how and where charged nuclei are accelerated to extreme energies, remain open. The spectral...
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A peculiarly short-duration gamma-ray burst from massive star core collapse
Gamma-ray bursts (GRBs) have been phenomenologically classified into long and short populations based on the observed bimodal distribution of duration
