Astronomy and Astrophysics, Nuclear and High Energy Physics, Physics and Astronomy, General Physics and Astronomy
21
Scopus Publications
Scopus Publications
Bridging the gap between virtual and physical laboratories: a web-based interactive platform for undergraduate physics practicals Ashadul Halder, Shibaji Banerjee Physics Education, 2026 The COVID-19 pandemic highlighted the challenges of maintaining hands-on laboratory instruction in undergraduate physics education. In response, we developed and deployed an interactive online physics laboratory platform designed to closely replicate the experimental setups available and curriculum of St. Xavier’s College (Autonomous), Kolkata. The platform is designed to closely replicate real experimental arrangements and is aligned with the curriculum, allowing students to prepare effectively before performing physical experiments. Student feedback revealed that 100% of the respondents rated the platform as beneficial (rating 4 or 5 on a 5-point scale) to improve conceptual understanding and increase confidence in conducting physical experiments. Furthermore, all students agreed that having access to the online prelab simulations is advantageous and recommended its regular use. These findings highlight the effectiveness of web-based simulations as a complementary and sustainable resource for physics education.
Addressing the self-interaction for ELDER dark matter from the 21-cm signal Rupa Basu, Debasish Majumdar, Ashadul Halder, Shibaji Banerjee International Journal of Modern Physics A, 2025 The self-interacting dark matter can affect various cosmological processes. Such interactions can be number conserving (e.g. [Formula: see text]) or number violating (e.g. [Formula: see text]). The latter processes where three (or more) dark matter particles undergo self-annihilation/scattering to produce less number of dark matter is termed as Cannibalism process. In this work, the self-interaction of dark matter and the strength of such interactions are investigated in the light of experimental results of the global 21-cm spectrum of neutral hydrogen from the era of cosmic dawn. From the present work, it appears that [Formula: see text] process is much more dominant over the [Formula: see text] process. It is also found that such interactions affect the dark matter-baryon elastic scattering cross-section. The study also indicates the presence of multi-component dark matter of different mass ranges in the Universe.
Analyzing the 21-cm signal brightness temperature in the Universe with inhomogeneities Shashank Shekhar Pandey, Ashadul Halder, A. S. Majumdar Physical Review D, 2024 We explore the 21-cm signal in our Universe containing inhomogeneous matter distribution at considerably large scales. Employing Buchert's averaging procedure in the context of a model of spacetime with multiple inhomogeneous domains, we evaluate the effect of our model parameters on the observable 21-cm signal brightness temperature. Our model parameters are constrained through the Markov Chain Monte Carlo method using the Union 2.1 supernova Ia observational data. We find that a significant dip in the brightness temperature compared to the $\\Lambda$CDM prediction could arise as an effect of the inhomogeneities present in the Universe.
Future deceleration due to backreaction in a Universe with multiple inhomogeneous domains Ashadul Halder, Shashank Shekhar Pandey, A.S. Majumdar Journal of Cosmology and Astroparticle Physics, 2023 We formulate a model of spacetime with inhomogeneous matter distribution in multiple domains. In the context of the backreaction framework using Buchert's averaging procedure, we evaluate the effect of backreaction due to the inhomogeneities on the late time global evolution of the Universe. Examining the future evolution of this universe, we find that it can transit from the presently accelerating phase to undergo future deceleration. The future deceleration is governed by our model parameters. We constrain the model parameters using observational analysis of the Union 2.1 supernova Ia data employing the Markov Chain Monte Carlo method.
KM3NeT upper bounds of detection rates of solar neutrinos from annihilations of dark matter at the solar core Aman Gupta, Debasish Majumdar, Ashadul Halder Modern Physics Letters A, 2022 The Weakly Interacting Massive Particles (WIMPs) so far remain one of the most popular candidates for dark matter. If captured gravitationally inside the core of the Sun, these WIMPs may produce high-energy neutrinos as the end product in case they undergo self-annihilations at the solar core. In this work, we address the detectability of such neutrinos at the proposed KM3NeT detector. Upper bounds of the detection rate for such neutrinos at KM3NeT are computed for the case of a generic dark matter scenario and also when specific models for particle dark matter are chosen. In this work, upper bounds of muon event rates for different annihilating dark matter masses are computed for each of the cases of dark matter annihilation channels (e.g. [Formula: see text], [Formula: see text], [Formula: see text], etc.). These upper bounds are also computed by considering the dark matter scattering cross-section using upper bounds obtained from PandaX-4T direct dark matter search experiment.