A5031949240- Particle physics theoretical and experimental studies
- High-Energy Particle Collisions Research
- Particle Detector Development and Performance
- Quantum Chromodynamics and Particle Interactions
- Dark Matter and Cosmic Phenomena
- Cosmology and Gravitation Theories
- Neutrino Physics Research
- Computational Physics and Python Applications
- Radiation Detection and Scintillator Technologies
- Digital Radiography and Breast Imaging
- Distributed and Parallel Computing Systems
- Atomic and Subatomic Physics Research
- Astrophysics and Cosmic Phenomena
- Medical Imaging Techniques and Applications
- Particle Accelerators and Free-Electron Lasers
- Black Holes and Theoretical Physics
- Galaxies: Formation, Evolution, Phenomena
- Stellar, planetary, and galactic studies
- Advanced Semiconductor Detectors and Materials
- Gamma-ray bursts and supernovae
- Astronomical Observations and Instrumentation
Boğaziçi University
2014-2024
The University of Adelaide
2022-2023
Istanbul Bilgi University
2019
We report on a first measurement with sensitive opto-mechanical force sensor designed for the direct detection of coupling real chameleons to matter. These dark energy candidates could be produced in Sun and stream unimpeded Earth. The KWISP detector installed CAST axion search experiment at CERN looks tiny displacements thin membrane caused by mechanical effect solar chameleons. are detected Michelson interferometer homodyne readout scheme. benefits from focusing action ABRIXAS X-ray...
A group of middle-aged mixed-morphology (MM) supernova remnants (SNRs) interacting with molecular clouds (MC) has been discovered as strong GeV gamma-ray emitters by Large Area Telescope on board Fermi Gamma Ray Space (Fermi-LAT). The recent observations the Suzaku X-ray satellite have revealed that some these emitting SNRs, such IC443, W49B, W44, and G359.1-0.5, overionized plasmas. 3C 391 (G31.9+0.0) is another Galactic MM SNR MC. It was observed in gamma rays Fermi-LAT well 0.3 $-$ 10.0...
We report on a first measurement with sensitive opto-mechanical force sensor designed for the direct detection of coupling real chameleons to matter. These dark energy candidates could be produced in Sun and stream unimpeded Earth. The KWISP detector installed CAST axion search experiment at CERN looks tiny displacements thin membrane caused by mechanical effect solar chameleons. are detected Michelson interferometer homodyne readout scheme. benefits from focusing action ABRIXAS X-ray...