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1. Design and evaluation of a multimodal physics simulation

   Tomlinson, Brianna; Kaini, Prakrit; Harden, E. Lynn; Walker, Bruce; Moore, Emily B. (January 2019, Journal on technology and persons with disabilities)

   We present a multimodal physics simulation, including visual and auditory (description, sound effects, and sonification) modalities to support the diverse needs of learners. We describe design challenges and solutions, and findings from final simulation evaluations with learners with and without visual impairments. We also share insights from completing research with members of diverse learner groups (N = 52). This work presents approaches for designing and evaluating accessible interactive simulations for learners with diverse needs. 

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2. A Case Study in Line Balancing and Simulation

   https://doi.org/10.1016/j.promfg.2020.05.076  

   Yilmazlar, I. Ozan; Jeyes, Adarsh; Fiore, Alexis; Patel, Apurva; Spence, Chelsea; Wentzky, Chase; Zero, Nicole; Kurz, Mary E.; Summers, Joshua D.; Taaffe, Kevin M. (January 2020, Procedia Manufacturing)
3. A quantum hamiltonian simulation benchmark

   https://doi.org/10.1038/s41534-022-00636-x  

   Dong, Yulong; Whaley, K. Birgitta; Lin, Lin (December 2022, npj Quantum Information)

   Abstract Hamiltonian simulation is one of the most important problems in quantum computation, and quantum singular value transformation (QSVT) is an efficient way to simulate a general class of Hamiltonians. However, the QSVT circuit typically involves multiple ancilla qubits and multi-qubit control gates. In order to simulate a certain class of n -qubit random Hamiltonians, we propose a drastically simplified quantum circuit that we refer to as the minimal QSVT circuit, which uses only one ancilla qubit and no multi-qubit controlled gates. We formulate a simple metric called the quantum unitary evolution score (QUES), which is a scalable quantum benchmark and can be verified without any need for classical computation. Under the globally depolarized noise model, we demonstrate that QUES is directly related to the circuit fidelity, and the potential classical hardness of an associated quantum circuit sampling problem. Under the same assumption, theoretical analysis suggests there exists an ‘optimal’ simulation time t opt  ≈ 4.81, at which even a noisy quantum device may be sufficient to demonstrate the potential classical hardness. 

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4. Design and simulation of a uniform irradiance photochemical platform

   https://doi.org/10.1039/D2RE00329E  

   Walsh, Dylan J.; Schneider, Timo N.; Olsen, Bradley D.; Jensen, Klavs F. (January 2023, Reaction Chemistry & Engineering)

   The growth of photochemistry and high throughput experimentation in well plates and flow drives interest in photochemical platforms that provide spatially uniform irradiation of reactions. Here, we present a design of a versatile, uniform light platform for photochemistry to enable increased performance and reproducibility for high throughput experimentation in shallow well plates, in-plane flow reactors, and droplets. The design of the platform is driven by the development of an open-source ray tracing light simulation package. Radiometry provides experimental validation of the system's irradiance and irradiance uniformity. The usefulness of the approach is demonstrated by application to the photoinduced electron transfer–reversible addition–fragmentation chain transfer polymerization of methyl acrylate. 

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5. Simulation and sensitivities for a phased IceCube-Gen2 deployment

   https://doi.org/10.22323/1.395.1186  

   Abbasi, Rasha; Ackermann, Markus; Adams, Jenni; Aguilar, Juanan; Ahlers, M.; Ahrens, Maryon; Alispach, Cyril Martin; Allison, Patrick; Alves Junior, Antonio Augusto; Amin, Najia Moureen; et al (March 2022, 37th International Cosmic Ray Conference (ICRC2021))

   The IceCube Neutrino Observatory opened the window on high-energy neutrino astronomy by confirming the existence of PeV astrophysical neutrinos and identifying the first compelling astrophysical neutrino source in the blazar TXS0506+056. Planning is underway to build an enlarged detector, IceCube-Gen2, which will extend measurements to higher energies, increase the rate of observed cosmic neutrinos and provide improved prospects for detecting fainter sources. IceCube-Gen2 is planned to have an extended in-ice optical array, a radio array at shallower depths for detecting ultra-high-energy (>100 PeV) neutrinos, and a surface component studying cosmic rays. In this contribution, we will discuss the simulation of the in-ice optical component of the baseline design of the IceCube-Gen2 detector, which foresees the deployment of an additional ~120 new detection strings to the existing 86 in IceCube over ~7 Antarctic summer seasons. Motivated by the phased construction plan for IceCube-Gen2, we discuss how the reconstruction capabilities and sensitivities of the instrument are expected to progress throughout its deployment. 

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