A5013706902- Particle physics theoretical and experimental studies
- High-Energy Particle Collisions Research
- Quantum Chromodynamics and Particle Interactions
- Particle Detector Development and Performance
- Dark Matter and Cosmic Phenomena
- Nuclear Physics and Applications
- Gamma-ray bursts and supernovae
- Cosmology and Gravitation Theories
- Astronomical Observations and Instrumentation
- Computational Physics and Python Applications
- Planetary Science and Exploration
- Astro and Planetary Science
- Neutrino Physics Research
- Astrophysics and Cosmic Phenomena
- Infrared Target Detection Methodologies
- Stochastic processes and statistical mechanics
- Astrophysical Phenomena and Observations
- Statistical Methods and Bayesian Inference
- Historical Studies on Reproduction, Gender, Health, and Societal Changes
- Radioactivity and Radon Measurements
- Calibration and Measurement Techniques
- Radiation Detection and Scintillator Technologies
- Historical Psychiatry and Medical Practices
- Seaweed-derived Bioactive Compounds
- Markov Chains and Monte Carlo Methods
University of Jammu
2018-2025
Guru Nanak Dev University
2023
Chandigarh University
2023
Institute of Nuclear Physics, Polish Academy of Sciences
2020-2022
Indian Space Research Organisation
1993-2017
Vanderbilt University
2012-2015
Institute of High Energy Physics
2015
Fermi National Accelerator Laboratory
2014
European Organization for Nuclear Research
2013
Wayne State University
2009
ASTROSAT is India's first astronomy satellite that will carry an array of instruments capable simultaneous observations in a broad range wavelengths: from the visible, near ultraviolet (NUV), far-UV (FUV), soft X-rays to hard X-rays. There be five principal scientific payloads aboard satellite: (i) Soft X-ray Telescope (SXT), (ii) three Large Area Xenon Proportional Counters (LAXPCs), (iii) Cadmium-Zinc-Telluride Imager (CZTI), (iv) two Ultra-Violet Imaging Telescopes (UVITs) one for visible...
Views Icon Article contents Figures & tables Video Audio Supplementary Data Peer Review Share Twitter Facebook Reddit LinkedIn Tools Reprints and Permissions Cite Search Site Citation Monika Sharma, CMS Collaboration; Measurement of the azimuthal anisotropy neutral pions in PbPb collisions at SNN = 2.76 TeV. AIP Conference Proceedings 21 October 2013; 1560 (1): 663–665. https://doi.org/10.1063/1.4826865 Download citation file: Ris (Zotero) Reference Manager EasyBib Bookends Mendeley Papers...
The agreement of hydrodynamic predictions elliptic flow with data from Au+Au collisions at 200 GeV suggests the strongly coupled Quark Gluon Plasma, sQGP, produced RHIC [1, 2, 3] is a perfect liquid. Shear viscosity to entropy density (η/s) ratio provides measure fluidity Small value η/s may indicate that system more coupled. We present estimations based on measurements in GeV. show how initial conditions affect transport coefficients such as viscosity. In this paper we also an alternative...
The purpose of this study was to compare efficacy kinesio taping (K-taping) and joint mobilization as immediate interventions for treating athletes with glenohumeral internal rotation deficit (GIRD). Thirty-two asymptomatic players were recruited from basketball, volleyball handball who had a loss shoulder range motion (IR ROM) 10 degrees or more on their dominant compared non-dominant side. They randomly assigned 1 2 groups: K-taping (n = 16) 16). Participants in group treated K-tape...
Indian Remote Sensing Satellite-P3 (IRS-P3: 1996-017A) was launched into a near-Earth, polar, Sun-synchronous orbit by India's Polar Satellite Launch Vehicle (PSLV-D3) on March 21, 1996. The X-ray Astronomy Experiment (IXAE) is one of the prime payloads onboard IRS-P3. IXAE has two sets detectors: three pointed-mode proportional counters (PPCs) and Sky Monitor (XSM). IRS-P3 configured to operate in modes, namely, Earth-pointing mode stellar-pointing mode. In remote sensing are operation;...
The Stretched Rohini Satellite Series-C (SROSS-C) was launched into a near-Earth orbit by the Indian Augmented Launch Vehicle (ASLV-D3) on May 20, 1992. A gamma ray burst (GRB) experimental package for detecting and measuring temporal spectral characteristics of celestial GRBs one two main payloads onboard SROSS-C. microprocessor-based electronics unit designed developed payload data handling, control operation in different modes, telemetering to ground stations. electronic instrumentation...