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The massive X-ray binary Cen X-3 was observed over approximately one quarter of the system's 2.08 day orbit, beginning before eclipse and ending slightly after eclipse center with the Chandra X-ray Observatory using its High-Energy…

Bright AGN frequently show ultra-fast outflows (UFOs) with outflow velocities vout ~0.1c. These outflows may be the source of AGN feedback on their host galaxies sought by galaxy formation modellers. The exact effect of the outflows on the…

Astrophysics of Galaxies · Physics 2015-06-16 Martin A. Bourne , Sergei Nayakshin

While most scintillation-based dark matter experiments search for Weakly Interacting Massive Particles (WIMPs), a sub-GeV WIMP-like particle may also be detectable in these experiments. While dark matter of this type and scale would not…

High Energy Physics - Phenomenology · Physics 2023-10-30 A. R. Caddell , V. V. Flambaum , B. M. Roberts

Charge amplification in liquids could provide single-phase xenon time projection chambers with background discrimination and fiducialisation capabilities similar to those found in dual-phase detectors. Although efforts to achieve the high…

Instrumentation and Detectors · Physics 2024-01-05 P. Knights , H. Sekiya , I. Katsioulas , K. Nikolopoulos , K. Kanzawa , I. Giomataris

Understanding the transition from atomic gas to molecular gas is critical to explain the formation and evolution of molecular clouds. However, the gas phases involved, cold HI and CO-dark molecular gas, are challenging to directly observe…

AXEL is a high pressure xenon gas TPC detector being developed for neutrinoless double-beta decay search. We use the proportional scintillation mode with a new electroluminescence light detection system to achieve high energy resolution in…

Instrumentation and Detectors · Physics 2017-11-27 S. Ban , K. D. Nakamura , S. Akiyama , M. Hirose , A. K. Ichikawa , Y. Ishiyama , A. Minamino , K. Miuchi , T. Nakaya , H. Sekiya , S. Tanaka , K. Ueshima , S. Yanagita

We investigate the production of circularly polarised X and gamma-ray signals in cosmic accelerators such as supernova remnants and AGN jets. Proton-proton and proton-photon collisions within these sites produce a charge asymmetry in the…

High Energy Astrophysical Phenomena · Physics 2021-01-04 Céline Boehm , Céline Degrande , Jakub Scholtz , Aaron C. Vincent

We present a sub-100 pc-scale analysis of the CO molecular gas emission and kinematics of the gravitational lens system SDP.81 at redshift 3.042 using Atacama Large Millimetre/submillimetre Array (ALMA) science verification data and a…

Astrophysics of Galaxies · Physics 2015-08-19 M. Rybak , S. Vegetti , J. P. McKean , P. Andreani , S. D. M. White

We have observed the signatures of valence electron rearrangement in photoexcited ammonia using ultrafast hard X-ray scattering. Time-resolved X-ray scattering is a powerful tool for imaging structural dynamics in molecules because of the…

We have measured the properties of scintillation light in liquid argon doped with xenon concentrations from 165 ppm to 10,010 ppm using a $^{22}$Na source. The energy transfer processes in the xenon-doped liquid argon are discussed in…

Instrumentation and Detectors · Physics 2021-02-03 Y. Y. Gan , M. Y. Guan , Y. P. Zhang , P. Zhang , C. G. Yang , Q. Zhao , Y. T. Wei , W. X. Xiong

During the spin-down phase of the life of a higher-dimensional black hole, the emission of particles on the brane exhibits a strong angular variation with respect to the rotation axis of the black hole. It has been suggested that this…

High Energy Physics - Theory · Physics 2015-06-11 Panagiota Kanti , Nikolaos Pappas

Conceiving the possibility of using plastic scintillator bars as robust detectors for antineutrino detection for the remote reactor monitoring and nuclear safeguard application we study expected basic performance by Monte Carlo simulation.…

Instrumentation and Detectors · Physics 2016-10-20 A. Sh. Georgadze , V. M. Pavlovych , O. A. Ponkratenko , D. A. Litvinov

Many atomic processes result in the emission of photons. Analysis of the properties of emitted photons, such as energy and angular distribution as well as polarization, is regarded as a powerful tool for gaining more insight into the…

Atomic Physics · Physics 2018-04-18 V. A. Zaytsev , A. S. Surzhykov , V. M. Shabaev , Th. Stöhlker

We perform a theoretical study of the scintillation efficiency in the low-energy region crucial for liquid-xenon dark-matter detectors. We develop a computer program to simulate the cascading process of the recoiling xenon nucleus in liquid…

Instrumentation and Detectors · Physics 2013-10-10 Wei Mu , Xiaonu Xiong , Xiangdong Ji

The characteristics of a single-photon emitter based on a semiconductor quantum dot, such as their indistinguishability and brightness, depend on the stability of the recombination channel, which can switch spontaneously between exciton and…

We probe charge photogeneration and subsequent recombination dynamics in neat regioregular poly(3-hexylthiophene) films over six decades in time by means of time-resolved photoluminescence spectroscopy. Exciton dissociation at 10K occurs…

We present models for the X-ray spectrum of the Seyfert 2 galaxy NGC 1068. These are fitted to data obtained using the High Energy Transmission Grating (HETG) on the Chandra X-ray observatory. The data show line and radiative recombination…

High Energy Astrophysical Phenomena · Physics 2015-06-17 T. Kallman , D. A. Evans , H. Marshall , C. Canizares , A. Longinotti , M. Nowak , N. Schulz

Detectors based upon the noble elements, especially liquid xenon as well as liquid argon, as both single- and dual-phase types, require reconstruction of the energies of interacting particles, both in the field of direct detection of dark…

Fast neutron detection is often based on the neutron-proton elastic scattering reaction: the ionization caused by recoil protons in a hydrogenous material constitutes the basic information for the design and development of a class of…

Instrumentation and Detectors · Physics 2023-02-08 P. Console Camprini , F. Leone , C. Massimi , A. Musumarra , M. G. Pellegriti , C. Pisanti , F. Romano , R. Spighi , N. Terranova , M. Villa