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Kavita Lalwani

Publications and source records attributed to Kavita Lalwani.

6 recordsLinked to original sources

Quantum Simulation of SPAD in the Space Radiation Environment

Single-Photon Avalanche Diodes (SPADs) are critical components of emerging quantum communication networks that detect single photons. They are placed in satellites for long-distance communication and are susceptible to radiation-induced displacement damage in space. This degrades SPAD performance parameters, including reduced efficiency, increased thermal dark counts, damage to the Si crystal, and increased afterpulsing rate. This paper simulates SPAD in a space radiation environment by introducing a quantum simulation framework, modeling the SPAD detector as a three-level quantum system, ground state ($|g\rangle$), excited state ($|e\rangle$) and a trap state ($|t\rangle$). Furthermore, to model the photon as a quantum system, second quantization and Fock-space truncation are used. The interaction between the photon-SPAD closed system is simulated using the Jaynes-Cummings model, and the open-system dynamics is governed by the Lindblad master equation and Qiskit's gate-based noise channels. The key characteristics, such as the efficiency, timing jitter, thermal dark counts, and afterpulsing \& radiation effects, are obtained using quantum simulation of SPAD. This approach differs significantly from conventional TCAD simulations, which rely on semiclassical approximations that do not capture the discrete quantum statistics of single-photon interactions and the dynamics of trap states.

quant-ph↗

A comprehensive study of $Λ_c^- \to Λ(\to p π) μ^- \bar ν_μ$ incorporating SMEFT implications and right-handed neutrino

We present a comprehensive analysis of the decay $Λ_c^- \to Λ(\to pπ)\,μ^- \barν_μ$ within a model-independent effective field theory framework. Previous studies have been restricted to the three-body decay $Λ_c^+ \to Λμ^+ ν_μ$ and considered only left-handed neutrinos within the Low-Energy Effective Theory (LEFT). In this work, we extend the analysis to the complete four-body angular distribution for the first time, incorporating the indirect constraints implied by the Standard Model Effective Field Theory (SMEFT) on the LEFT Wilson coefficients. We also include the effects of right-handed neutrino (RHN) operators, enabling a unified treatment of both left- and right-handed neutrino interactions in the $c \to s μν_μ$ transition. Using the global bounds derived from LEFT observables and their SMEFT correlations, we study the impact of allowed new-physics scenarios on a variety of observables, including differential decay rates, forward-backward asymmetries, polarization asymmetries of the final-state hadron and lepton, and the angular coefficients (${\cal M}_0$ to ${\cal M}_9$) in the 4-body angular distribution. Our analysis reveals significant deviations from the Standard Model in the observables $\mathcal{P}^Λ_L$ and ${\cal M}_1$ for $C^V_{RL}$ and $C^V_{RR}$, and striking $T$-odd effects in ${\cal M}_7$ for complex $C^V_{RL}$. These features provide sensitive probes of vector-type new physics, such as leptoquark or right-handed current models. The predicted patterns can be tested in forthcoming measurements at BESIII, LHCb, and Belle II, where polarization-sensitive observables in $Λ_c$ decays are becoming experimentally accessible.

hep-ph↗

Impact of Solar Particle Events on Space Radiation Shielding: OLTARIS Simulation and Quantum Optimization of Material Selection using QAOA and VQE Algorithms

Space radiation poses a significant challenge for long duration human space missions, with sources including Galactic Cosmic Rays, Solar Particle Events, and trapped particles in the Van Allen belts. These high-energy radiations cause severe biological effects on astronauts and degrade spacecraft systems, making effective shielding critical. Traditionally, passive shielding materials like aluminum have been used, but their limitations, particularly in generating secondary radiation, necessitate better alternatives. In this study, the performance of shielding materials such as lithium hydride, polyethylene, lithium borohydride, beryllium borohydride, and ammonia borane are evaluated in GCR and SPE environments using OLTARIS, a NASA developed tool. The October 1989 SPE is used to study particle flux and dose distributions. Shielding effectiveness varies by environment. Beryllium borohydride performs best in SPE, while lithium hydride gives the lowest dose in GCR. In SPE, performance is linked to hydrogen content. Effect of Solar modulation on GCR dose is also studied. Higher modulation lowers GCR intensity and dose. The complex nature of high energy space radiation and material combinations creates computational challenges. To address this, the material selection problem is modeled as a Quadratic Unconstrained Binary Optimization and solved using the Variational Quantum Eigensolver and Quantum Approximate Optimization Algorithm. Mapping OLTARIS data to the Ising model and applying these quantum classical methods helped identify shielding setups that minimize radiation dose. Results show agreement between OLTARIS and quantum optimization for both environments.

physics.med-ph↗

New Physics effects with right-handed neutrinos in semileptonic decay $B_c^+ \to B_s μ^+ ν_μ$

We extend the Standard Model with the general effective Hamiltonian for the quark level transition $c \to s \ell ν$ with a complete set of four fermion operators including right-handed neutrinos. The current experimental measurements in charm decays are compatible with the Standard Model predictions and are used to constrain the new physics. With the available experimental data, we fit a $χ^2$ function to get the best-fit values of the NP WCs. We investigate the impact of allowed new physics in the observables such as differential branching fraction, forward-backward asymmetry, lepton polarization asymmetry, and convexity parameter in the semileptonic decay $B_c^+ \to B_s μ^+ ν_μ$. The different types of new physics scenarios have significant effects on these considered observables. The future experimental information of these observables can help to disentangle the structure of new physics.

hep-ph↗

Effectiveness of Multi-Layered Radiation Shields Constructed from Polyethylene and Metal Hydrides Using HZETRN and OLTARIS for space applications

A major challenge for extended human spaceflights in deep space is the dangerous exposure to space radiation. In previous studies aluminium has been used as a multilayer shielding material in GCR space radiation environment with high dose equivalent. To further reduce the dose equivalent, shielding effectiveness of various metal hydrides in GCR free space environment is investigated using HZETRN2015 (High charge (Z) & Energy TRaNsport) and OLTARIS (On-Line Tool for the Assessment of Radiation In Space) in this work. Metal hydride materials are chosen because of their capacity to store hydrogen. Among these materials, lithium hydride has demonstrated superior effectiveness as a radiation shield. Given this, the potential of a multilayer shield composed of polyethylene and lithium hydride is also being explored considering the tensile strength certain varieties of polyethylene like UHMWPE (Ultra High Molecular Weight Poly-Ethylene) can provide. The results from HZETRN2015 and OLTARIS transport codes are compared and found in agreement.

physics.space-ph↗

A Method to Simulate the Observed Surface Properties of Proton Irradiated Silicon Strip Sensors

During the scheduled high luminosity upgrade of LHC, the world's largest particle physics accelerator at CERN, the position sensitive silicon detectors installed in the vertex and tracking part of the CMS experiment will face more intense radiation environment than the present system was designed for. To upgrade the tracker to required performance level, extensive measurements and simulations studies have already been carried out. A defect model of Synopsys Sentaurus TCAD simulation package for the bulk properties of proton irradiated devices has been producing simulations closely matching with measurements of silicon strip detectors. However, the model does not provide expected behavior due to the fluence increased surface damage. The solution requires an approach that does not affect the accurate bulk properties produced by the proton model, but only adds to it the required radiation induced properties close to the surface. These include the observed position dependency of the strip detector's charge collection efficiency (CCE). In this paper a procedure to find a defect model that reproduces the correct CCE loss, along with other surface properties of a strip detector up to a fluence $1.5\times10^{15}$ 1 MeV n$_{\textrm{eq}}$ cm$^{-2}$, will be presented. When applied with CCE loss measurements at different fluences, this method may provide means for the parametrization of the accumulation of oxide charge at the SiO2/Si interface as a function of dose.

physics.ins-det↗