Scholarly Works, Physics

Permanent URI for this collection

https://hdl.handle.net/10919/24287

Research articles, presentations, and other scholarship

Browse

Now showing 1 - 20 of 1108

Measurements of Electronic Band Structure in CeCoGe₃ by Angle-Resolved Photoemission Spectroscopy
Prater, Robert; Chen, Mingkun; Staab, Matthew; Sreedhar, Sudheer; Byland, Journey; Shen, Zihao; Savrasov, Sergey Y.; Taufour, Valentin; Ivanov, Vsevolod; Vishik, Inna (MDPI, 2026-02-25)
In this paper, we present a comprehensive study of the electronic structure of CeCoGe₃ throughout the entire Brillouin zone in the non-magnetic regime using angle-resolved photoemission spectroscopy (ARPES). The electronic structure agrees in large part with first principles calculations, including predicted topological nodal lines. Two new features in the band structure are also observed, namely a surface state and folded bands, the latter of which is argued to originate from a unit cell reconstruction.
Sensitivity of the Hyper-Kamiokande experiment to neutrino oscillation parameters using accelerator neutrinos
Hyper-Kamiokande Collaboration; Vogelaar, R. Bruce (2026-02-23)
This paper presents the expected sensitivity to the neutrino oscillation parameters of the Hyper-Kamiokande long-baseline program. The Hyper-Kamiokande experiment, currently under construction in Japan, will measure the oscillations of accelerator-produced neutrinos with thousands of selected events per sample: this corresponds to an increase of statistics of a factor 25–100 with respect to recent results from the currently-running long-baseline neutrino oscillation experiment in Japan, T2K. In the most favorable scenario we will achieve the discovery of Charge-Parity (CP) violation in neutrino oscillation at 5 σ C.L. in less than 3 years. With 10 years of data-taking, and assuming a neutrino : antineutrino beam running ratio of 1:3, a CP violation discovery at 5 σ C.L. is possible for more than 60% of the actual values of the CP-violating phase, δ CP . Moreover, we will measure δ CP with a precision ranging from 20 ∘ , in the case of maximal CP violation, to 6 ∘ , in the case of CP conservation. We aim to achieve a 0.5% resolution on the Δ m 32 2 parameter, and a resolution between 3% and 0.5% on the sin 2 θ 23 parameter, depending on its true value. These results are obtained by extending the analysis methods of T2K with dedicated tuning to take into account the Hyper-Kamiokande design: the larger far detector, the more powerful beam, the upgraded near detector ND280, and the planned additional Intermediate Water Cherenkov Detector.
Probing and modeling of photoexcited carrier dynamics in Ge-based heterostructures
Magill, Brenden A.; Mudiyanselage, Rathsara R. H. H.; Paleologu, Thalya; McKinney, Christopher E.; Pleimling, Yannick; Smith, Nicholas W. G.; Hudait, Mantu K.; Stanton, Christopher J.; Khodaparast, Giti A. (American Physical Society, 2025-08-29)
While germanium (Ge) has long been an important player in microelectronics, strain-engineered Ge heterostructures have recently gained increased attention owing to the intriguing possibility of using strain to change the relative positions of the conduction band valleys and, as a result, go from an indirect to a direct gap material. Time-resolved pump-probe spectroscopy is an excellent tool to provide insight into the fundamental interactions and microscopic dynamics of electrons, holes, phonons, and impurities. In this study, using complementary techniques of single-color time-resolved differential reflectivity and two-color time-resolved differential transmission, we gained insights into the effects of interfacial strain on carrier dynamics in several different Ge-based heterostructures. Our structures include high-quality Ge films interfaced with InGaAs and AlAs grown on semi-insulating GaAs as the substrate. In contrast to traditional microwave photoconductivity decay (μ − PCD) measurements, which typically have a time resolution on the ns scale, we probe samples on a 100 fs scale and can measure decay times approximately three orders of magnitude faster than previous μ − PCD measurements. Therefore, our results are sensitive to the effects of both carrier recombination as well as electron intervalley and hole interband scattering.
Impact of Arsenic- and Indium-Terminated InGaAs Stressors on Carrier Confinement, Strain, Defects, and Transport Properties of Tensile-Strained Ge
Karthikeyan, Sengunthar; Khatiwada, Rishav; Heremans, Jean J.; Johnston, Steven W.; Zong, Ze; Zhou, Wei; Hudait, Mantu K. (American Chemical Society, 2025-11-25)
Device-quality tensile-strained Ge (ε-Ge) grown on a large bandgap semiconductor with superior electrical and optical carrier confinement is essential for group-IV-based optoelectronics. Properties of ε-Ge active layers synthesized on In0.24Ga0.76As buffers with two different surface terminations─arsenic-rich and indium-rich─were experimentally demonstrated, highlighting the factors not considered in theoretical calculations. High-resolution X-ray diffraction and Raman spectroscopy analyses of these ε-Ge/In0.24Ga0.76As heterostructures confirmed the fully strained (1.6%) and partially relaxed (0.82%) nature of the ε-Ge bonded with arsenic-terminated (GeAs-terminated) and indium-terminated (GeIn-terminated) In0.24Ga0.76As stressors, respectively. High-resolution cross-sectional transmission electron microscopy showed a coherent, sharp, and fully strained ε-Ge/In0.24Ga0.76As heterointerface in the GeAs-terminatedheterostructure, whereas microtwin defects were present in the GeIn-terminatedheterostructure. These heterostructures were further characterized by evaluating the minority carrier lifetimes, high for GeAs-terminated(525 ns) and low for GeIn-terminated(69 ns), using the photoconductive decay technique. Moreover, band alignment was constructed using X-ray photoelectron spectroscopy, where the GeAs-terminatedheterostructure revealed that both holes and electrons were confined within the ε-Ge active layer as a type-I band alignment with ΔEV, As-terminated= 0.22 eV and ΔEC,As-terminated= 0.38 eV. On the other hand, the GeIn-terminatedheterostructure exhibited a type-II band alignment with ΔEV,In-terminated= – 0.02 eV and ΔEC,In-terminated= 0.53 eV. Furthermore, the magnetotransport properties revealed high mobility (321 cm²/(V s)) with single-electron transport in GeAs-terminatedheterostructure and low mobility (3.34 cm²/(V s)) with multihole transport in the GeIn-terminatedheterostructure. Therefore, preferring the ε-Ge on the arsenic-rich surface of In0.24Ga0.76As stressor over the indium-rich surface during material synthesis offers device-quality materials with high carrier lifetime and superior carrier confinement, which can provide an opportunity to fabricate efficient group-IV-based optoelectronic devices.
AMSB in Sp(N_c) gauge theories
Varier, Digvijay R.; Gu, Zijian; Noether, Bea; Murayama, Hitoshi (2026-02-10)
We present a careful study of the chiral symmetry breaking minima and other potential minima in supersymmetric symplectic QCD (Sp(Nc) with Nf flavors) perturbed by Anomaly Mediated Supersymmetry Breaking (AMSB). Although the case of Nf = Nc + 1 requires particular care due to the inherently strongly coupled nature of the quantum modified moduli space, we are able to show that all Sp(Nc) theories to which AMSB can be applied (Nf < 3(Nc + 1)) possess stable chiral symmetry breaking minima, which are plausibly continuously connected to the vacua of QCD-like Sp(Nc) theories for large SUSY breaking, and are protected from runaways to incalculable minima.
Analytical interaction potential for Lennard-Jones rods
Wang, Junwen; Seidel, Gary D.; Cheng, Shengfeng (American Physical Society, 2025-01-03)
An analytical form has been derived using Ostrogradsky's integration method for the interaction between two thin rods of finite lengths in arbitrary relative configurations in a three-dimensional space, each treated as a line of point particles interacting through the Lennard-Jones 12-6 potential. Simplified analytical forms for coplanar, parallel, and collinear rods are also derived. Exact expressions for the force and torque between the rods are obtained. Similar results for a point particle interacting with a thin rod are provided. These interaction potentials can be widely used for analytical descriptions and computational modeling of systems involving rodlike objects such as liquid crystals, colloids, polymers, elongated viruses and bacteria, and filamentous materials including carbon nanotubes, nanowires, biological filaments, and their bundles.
Analytical sphere-thin rod interaction potential
Wang, Junwen; Cheng, Shengfeng (Springer, 2025-05)
A compact analytical form is derived through an integration approach for the interaction between a sphere and a thin rod of finite and infinite lengths, with each object treated as a continuous medium of material points interacting by the Lennard-Jones 12-6 potential and the total interaction potential as a summation of the pairwise potential between material points on the two objects. Expressions for the resultant force and torque are obtained. Various asymptotic limits of the analytical sphere–rod potential are discussed. The integrated potential is applied to investigate the adhesion between a sphere and a thin rod. When the rod is sufficiently long and the sphere sufficiently large, the equilibrium separation between the two (defined as the distance from the center of the sphere to the axis of the rod) is found to be well approximated as a+0.787σ, where a is the radius of the sphere and σ is the unit of length of the Lennard–Jones potential. Furthermore, the adhesion between the two is found to scale with a √a.
Effect of particle shape on stratification in drying films of binary colloidal mixtures
Liu, Binghan; Grest, Gary S.; Cheng, Shengfeng (AIP Publishing, 2025-07-21)
The role of particle shape in evaporation-induced auto-stratification in polydisperse colloidal suspensions is explored with molecular dynamics simulations of mixtures of spheres and aspherical particles. A unified framework based on the competition between diffusion and diffusiophoresis is proposed to understand the effects of shape and size dispersity. In general, particles diffusing more slowly (e.g., larger particles) tend to accumulate more strongly at the evaporation front. However, larger particles have larger surface areas and therefore greater diffusiophoretic mobility. Hence, they are more likely to be driven away from the evaporation front via diffusiophoresis. For a rapidly dried bidisperse suspension containing small and large spheres, the competition leads to “small-on-top” stratification. Here, we employ a computational model in which the diffusion coefficient is inversely proportional to particle mass. For a mixture of spheres and aspherical particles with similar mass, the diffusion contrast is reduced, and the spheres are always enriched at the evaporation front as they have the smallest surface area for a given mass and, therefore, the lowest diffusiophoretic mobility. For a mixture of solid and hollow spheres that have the same outer radius and thus the same surface area, the diffusiophoretic contrast is suppressed, and the system is dominated by diffusion. Consequently, the solid spheres, which have a larger mass and diffuse more slowly, accumulate on top of the hollow spheres. Finally, for a mixture of thin disks and long rods that differ significantly in shape but have similar mass and surface area, both diffusion and diffusiophoresis contrasts are suppressed, and the mixture does not stratify.
Analytical Interaction Potentials for Disks in Two Dimensions
Liu, Binghan; Wang, Junwen; Grest, Gary S.; Cheng, Shengfeng (2025-11-25)
Compact analytical forms are derived for the interactions involving thin disks in two dimensions using an integration approach. These include interactions between a disk and a material point, between two disks, and between a disk and a wall. Each object is treated as a continuous medium of materials points interacting by the Lennard-Jones 12-6 potential. By integrating this potential in a pairwise manner, expressions for the potentials and resultant forces between extended objects are obtained. All the results are validated with numerical integrations. The analytical potentials are implemented in LAMMPS and used to simulate two-dimensional suspension of disks with an explicit solvent modeled as a Lennard-Jones liquid. In monodisperse disk suspensions, a disorderto- order transition of disk packing is observed as the area fraction of disks is increased or as the solvent evaporates. In bidisperse disk suspensions being rapidly dried, stratification is found with the smaller disks enriched at the evaporation front. Such “small-on-top” stratification echoes the similar phenomenon occurring in three-dimensional polydisperse colloidal suspensions that undergo fast drying. These potentials can be applied to a wide range of two-dimensional systems involving disk-like objects.
Monte Carlo ray-tracing simulations for diffractive optics
Ellepola, Kalani H.; Rajapaksha, Tharindu D.; Remley, Emma E.; Nguyen, Minh L. P.; Macdonnell, Dave G.; Leckey, John P.; Nguyen, Vinh Q. (Optica Publishing Group, 2026-02-09)
Diffractive optic elements offer significant advantages in optical system design, enabling lightweight and compact architectures compared with conventional refractive and reflective components. However, accurately modeling wave-optical effects in such systems remains challenging because characteristic wavelengths of light are much smaller than the overall dimensions of typical optical assemblies. Conventional ray-tracing methods generally neglect these effects, while full-wave simulations become computationally prohibitive for large-scale systems. To overcome these limitations, we introduce a numerical implementation of the Monte Carlo ray-tracing approach based on the Huygens–Fresnel principle to predict key optical parameters, including focusing efficiency, focal spot size, and diffraction patterns with high fidelity. This approach is validated through systematic comparisons of dedicated experimental, theoretical, and numerical results, demonstrating accurate performance over a broad range of optical configurations. We further demonstrate that photon sieves incorporating large numbers of pinholes distributed across Fresnel zones can focus light into spots smaller than the smallest pinhole diameter while strongly suppressing higher diffractive orders and sidelobes. These results highlight the potential of the ray-tracing approach as a practical tool for both the design and optimization of next-generation diffractive optical elements.
Dynamical dark energy, dual spacetime, and DESI
Hur, Sunhaeng; Jejjala, Vishnu; Kavic, Michael J.; Minic, Djordje; Takeuchi, Tatsu (IOP Publishing, 2025-11)
In this paper we discuss possible consequences of a manifestly non-commutative and T-duality covariant formulation of string theory on dark energy, when the correspondence between short distance (UV) and long distance (IR) physics is taken into account. We demonstrate that the dark energy is dynamical, i.e., time-dependent, and we compute the allowed values of w0 and wa, given by w(a) = w0 + wa(1 − a), which compare favorably to the most recent observations by DESI. From this point of view, the latest results from DESI might point to a fundamentally new understanding of quantum spacetime in the context of quantum gravity.
Microsphere Autolithography—A Scalable Approach for Arbitrary Patterning of Dielectric Spheres
Kunkel, Elliott D.; Burnett, Alec G.; Scheiber, Katherine E.; Robinson, Hans D. (Wiley-VCH, 2025-11-28)
Patchy particles, i.e., colloidal particles whose surface properties have been modified in predetermined patterns, can serve as building blocks for efficient self-assembly of well-defined, ordered structures. This paper introduces MicroSphere AutoLithography (µSAL), a scalable lithographic method for production of patchy particles with arbitrary patch motifs. This technique leverages dielectric microspheres as both a lithographic substrate and the illuminating optic, using the fact that when a plane wave of light is refracted through a sphere, it produces a circular patch of high-intensity illumination on the back hemisphere. Exposing a collection of microspheres to multiple plane waves, every sphere simultaneously projects identical patterns of illuminated patches onto its own surface. Here, µSAL is demonstrated in barium titanate glass (BTG) microspheres that are coated with a thin (≈40 nm) conformal film of poly(dopamine) acting as the photoresist, fixating the optical pattern into a permanent metal structure through light-induced reduction of silver ions from the liquid suspension. Varying the index of refraction of the BTG spheres and the suspension produces a range of patch sizes and geometries in good agreement with theoretical modeling.
Characterization and Modeling of Interfacial Photogating Effect in Graphene Field-Effect Transistor Photodetectors on Silicon
Howe, Leslie; Ellepola, Kalani H.; Jahan, Nusrat; Talbert, Brady; Li, James; Cooney, Michael P.; Nguyen, Vinh Q. (ACS, 2025-01)
Infrared photodetection of silicon is prevented by the bandgap energy at wavelengths longer than approximately 1100 nm (∼1.12 eV) at room temperature, while silicon is the most used in modern electronics. Of particular interest is the performance of silicon for photodetectors in the infrared region beyond the silicon bandgap. Here, we demonstrate graphene field-effect transistor photodetectors on silicon with high photoconductive gain and photodetection capability extending to the infrared region. These devices have a photoresponsivity of >106 A/W for excitation above the silicon bandgap energy and yield a value of 35 A/W for infrared detection at a wavelength of 1530 nm. The high photosensitivity of the devices originates from the photogating effect in the nanostructures and a long Urbach tail extending into the infrared region. A model to explain the mechanism of the photoconductive gain is proposed, which shows that the gain results from modulation of the surface charge region under illumination. The gain strongly depends on the excitation power, due to carrier capture processes occurring over the barriers associated with the surface charge region, in agreement with the experimental data. This model properly explains the photoresponse behavior of graphene field-effect transistors on silicon.
Second harmonic generation and ferromagnetic resonance of BaTiO₃-BiFeO₃ films and nanorod arrays
Smith, Nicholas W. G.; Mudiyanselage, Rathsara R. H. H.; Wu, Shuang; Emori, Satoru; Magill, Brenden A.; Priya, Shashank; Khodaparast, Giti A. (IOP Publishing, 2025-07-01)
The solid solution of BaTiO3-BiFeO3 (BTO-BFO) exhibits enhanced magneto-electric coupling compared to the widely explored BiFeO3. In this study, we examined BTO-BFO nanorod arrays (and films) ranging from 200 to 600 nm in height (and thickness) by employing second harmonic emission (SHE) and ferromagnetic resonance (FMR) measurements. We demonstrated a large enhancement in SHE in nanorod arrays compared to the films, which can be attributed to the high surface-to-volume ratio in the nanorod arrays. Our FMR measurements showed low effective damping parameters of (4-8) × 10⁻³ in both nanorods and film structures. These observations are promising for future nonlinear optoelectronics and spintronics applications.
Absence of detectable spin and orbital pumping from Ni to Nb by out-of-plane ferromagnetic resonance
Bakare, Omolara A.; Street, Galen T.; Abdizadeh, Sachli; Maizel, Rachel E.; Klewe, Christoph; Emori, Satoru (AIP Publishing, 2026-02-02)
Excited ferromagnets can pump spin angular momentum, along with possibly orbital angular momentum. Among elemental ferromagnets, Ni has been proposed to exhibit substantial orbital pumping relative to spin pumping. Here, we search for a signature of orbital pumping by Ni, specifically by comparing out-of-plane ferromagnetic resonance in heterostructures without Ni (FeV/Nb) and with Ni (FeV-Ni/Nb). The FeV/Nb series shows a clear increase in Gilbert damping with the Nb sink thickness, attributed to spin pumping from FeV to Nb. Surprisingly, the FeV-Ni/Nb series exhibits no such damping increase, revealing no significant spin or orbital pumping from Ni to Nb. Our results offer a fresh perspective on angular-momentum transfer in Ni/Nb heterostructures.
New Constraints on the Evolution of the M_{H i}-M_☆ Scaling Relation Combining CHILES and MIGHTEE-H i Data
Bianchetti, Alessandro; Sinigaglia, Francesco; Rodighiero, Giulia; Elson, Ed; Vaccari, Mattia; Pisano, D. J.; Luber, Nicholas; Prandoni, Isabella; Hess, Kelley; Baes, Maarten; Adams, Elizabeth A. K.; Maccagni, Filippo M.; Renzini, Alvio; Bisigello, Laura; Yun, Min; Momjian, Emmanuel; Gim, Hansung B.; Pan, Hengxing; Oosterloo, Thomas A.; Dodson, Richard; Lucero, Danielle M.; Frank, Bradley S.; Ilbert, Olivier; Davies, Luke J. M.; Khostovan, Ali A.; Salvato, Mara (IOP Publishing, 2025-04-01)
The improved sensitivity of interferometric facilities to the 21 cm line of atomic hydrogen (H i) enables studies of its properties in galaxies beyond the local Universe. In this work, we perform a 21 cm line spectral stacking analysis combining the MeerKAT International GigaHertz Tiered Extragalactic Exploration and COSMOS H i Large Extra-galactic Survey surveys in the COSMOS field to derive a robust H i-stellar mass relation at z ≈ 0.36. In particular, by stacking thousands of star-forming galaxies subdivided into stellar mass bins, we optimize the signal-to-noise ratio of targets and derive mean H i masses in the different stellar mass intervals for the investigated galaxy population. We combine spectra from the two surveys, estimate H i masses, and derive the scaling relation log 10 M H I = ( 0.32 ± 0.04 ) log 10 M ⋆ + ( 6.65 ± 0.36 ) . Our findings indicate that galaxies at z ≈ 0.36 are H i richer than those at z ≈ 0 but H i poorer than those at z ≈ 1, with a slope consistent across redshift, suggesting that stellar mass does not significantly affect H i exchange mechanisms. We also observe a slower growth rate H i relative to the molecular gas, supporting the idea that the accretion of cold gas is slower than the rate of consumption of molecular gas to form stars. This study contributes to understanding the role of atomic gas in galaxy evolution and sets the stage for future development of the field in the upcoming Square Kilometre Array era.
Gas-rich dwarf galaxy multiples in the Apertif H_I survey
Siljeg, B.; Adams, E. A. K.; Fraternali, F.; Hess, K. M.; Marasco, A.; Denes, H.; Garrido, J.; Lucero, Danielle M.; Morganti, R.; Sanchez-Exposito, S.; van der Hulst, J. M. (EDP Sciences, 2025-11-26)
Context. Dwarf-dwarf galaxy encounters are a key aspect of galaxy evolution as they can ignite or temporarily suppress star formation in dwarfs and can lead to dwarf mergers. However, the frequency and impact of dwarf encounters remain poorly constrained due to limitations in spectroscopic studies, such as surface-brightness incompleteness in optical studies and poor spatial resolution in single-dish neutral hydrogen (H I) surveys. Aims. We aim to quantify the frequency of isolated gas-rich dwarf galaxy multiples using the untargeted, interferometric Apertif H I survey and study the impact of the interaction on star formation rates of galaxies as a function of the on-sky separation. Methods. Our parent dwarf sample consists of 2481 gas-rich galaxies with stellar masses in the range ∼10⁶ < M ⋆/M ⊙ ≲ 5 × 10⁹, for which we identified close companions based on projected separation (r p) and systemic velocity difference (|ΔV sys|). We explored both constant thresholds for r p and |ΔV sys| corresponding to 150 kpc and 150 km s⁻¹ on all galaxies in our sample as well as mass-dependent thresholds based on a stellar-to-halo mass relation. Results. We find the average number of companions per dwarf in our sample to be 13% (20%) when considering mass-dependent (constant) thresholds. We find that the frequency (∼11.6%) of dwarf companions in the stellar mass regime of 2 × 10⁸ < M ⋆/M ⊙ < 5 × 10⁹ is three times higher than previously determined from optical spectroscopic studies, highlighting the power of H I for finding dwarf multiples. Furthermore, we find evidence for an increase in star formation rates (SFRs) of close dwarf galaxy pairs of galaxies with similar stellar masses.
Interfacial Photogating of Graphene Field-Effect Transistor for Photosensory Biomolecular Detection
Howe, Leslie; Wang, Yifei; Ellepola, Kalani H.; Ho, Vinh X.; Dohmen, Rosalie L.; Pinto, Marlo M.; Hoff, Wouter D.; Cooney, Michael P.; Vinh, Nguyen Q. (Wiley-VCH, 2025-05)
The photogating effect, induced by a light-driven gate voltage, modulates the potential energy of the active channel in field-effect transistors, leading to a high photoconductive gain of these devices. The effect is particularly pronounced in low-dimensional structures, especially in graphene field-effect transistors. Along with unusual optical and electrical properties, graphene with ultra-high carrier mobility and a highly sensitive surface generates a strong photogating effect in the structure, making it an excellent element for detecting light-sensitive biomolecules. In this work, graphene field-effect transistor biosensors is demonstrated for the rapid detection of photoactive yellow protein in an aqueous solution under optical illumination. The devices exhibit millisecond-scale response times and achieve a detection limit below 5.8 fM under blue-light excitation, consistent with the absorption characteristics of the protein. The photogating effect in graphene field-effect transistors provides a promising approach for developing high-performance, light-sensitive biosensors for biomolecular detection applications.
Octopamine and tyramine dynamics predict learning rate phenotypes during associative conditioning in honey bees
Sands, Lester P.; Lei, Hong; Batten, Seth R.; Hartle, Alec; Lohrenz, Terry; Barbosa, Leonardo; Bang, Dan; Dayan, Peter; Howe, W. Matt; Smith, Brian H.; Montague, P. Read (American Association for the Advancement of Science, 2026-02-13)
Biogenic amines are fundamental for physiological homeostasis and behavioral control in both vertebrates and invertebrates. Monoamine neurotransmitters released in target brain regions conjointly regulate adaptive learning and plasticity. However, our understanding of these multianalyte mechanisms remains nascent, in part due to limitations in measurement technology. Here, during associative conditioning in honey bees, we concurrently tracked subsecond fluctuations in octopamine, tyramine, dopamine, and serotonin in the antennal lobe, where plasticity influences odorant representations. By repeatedly pairing an odorant with subsequent sucrose delivery, we observed individual differences in the conditioned response to odor, which occurred after a variable number of pairings (learners) or not at all (non-learners). The distinction between learners and non-learners was reflected in neurotransmitter responses across experimental conditions. The speed of learning, the number of pairings prior to a proboscis extension reflex, could be predicted from monoamine opponent signaling (octopamine-tyramine), from both the first presentation of the odorant alone, prior to any pairing with sucrose, and the first conditioned response to the odorant, coming after a number of sucrose pairings. These results suggest that monoamine signaling phenotypes may relate directly to the now widely reported socially relevant genetic differences in honey bee learning.
Performance of a Modular Ton-Scale Pixel-Readout Liquid Argon Time Projection Chamber
Abud, A. Abed; Abi, B.; Acciarri, R.; Acero, M. A.; Adames, M. R.; Adamov, G.; Adamowski, M.; Adams, D.; Adinolfi, M.; Adriano, C.; Aduszkiewicz, A.; Aguilar, J.; Aimard, B.; Akbar, F.; Allison, K.; Monsalve, S. Alonso; Alrashed, M.; Alton, A.; Alvarez, R.; Alves, T.; Amar, H.; Amedo, P.; Anderson, J.; Andrade, D. A.; Andreopoulos, C.; Andreotti, M.; Andrews, M. P.; Andrianala, F.; Andringa, S.; Anfimov, N.; Ankowski, A.; Antoniassi, M.; Antonova, M.; Antoshkin, A.; Aranda-Fernandez, A.; Arellano, L.; Arrieta Diaz, E.; Arroyave, M. A.; Asaadi, J.; Ashkenazi, A.; Asner, D.; Asquith, L.; Atkin, E.; Auguste, D.; Aurisano, A.; Aushev, V.; Autiero, D.; Azfar, F.; Back, A.; Back, H.; Back, J. J.; Bagaturia, I.; Bagby, L.; Balashov, N.; Balasubramanian, S.; Baldi, P.; Baldini, W.; Baldonedo, J.; Baller, B.; Bambah, B.; Banerjee, R.; Barao, F.; Barenboim, G.; Alzas, PB Arham B. A.; Barker, G. J.; Barkhouse, W.; Barr, G.; Barranco Monarca, J.; Barros, A.; Barros, N.; Barrow, D.; Barrow, J. L.; Basharina-Freshville, A.; Bashyal, A.; Basque, V.; Batchelor, C.; Bathe-Peters, L.; Battat, J. B. R.; Battisti, F.; Bay, F.; Bazetto, M. C. Q.; Bazo Alba, J. L. L.; Beacom, J. F.; Bechetoille, E.; Behera, B.; Belchior, E.; Bell, G.; Bellantoni, L.; Bellettini, G.; Bellini, V.; Beltramello, O.; Benekos, N.; Benitez Montiel, C.; Benjamin, D.; Bento Neves, F.; Berger, J.; Berkman, S.; Bernal, J.; Bernardini, P.; Bersani, A.; Bertolucci, S.; Betancourt, M.; Betancur Rodriguez, A.; Bevan, A.; Bezawada, Y.; Bezerra, A. T.; Bezerra, T. J.; Bhat, A.; Bhatnagar, V.; Bhatt, J.; Bhattacharjee, M.; Bhattacharya, M.; Bhuller, S.; Bhuyan, B.; Biagi, S.; Bian, J.; Biery, K.; Bilki, B.; Bishai, M.; Bitadze, A.; Blake, A.; Blaszczyk, F. D.; Blazey, G. C.; Blucher, E.; Bogenschuetz, J.; Boissevain, J.; Bolognesi, S.; Bolton, T.; Bomben, L.; Bonesini, M.; Bonilla-Diaz, C.; Bonini, F.; Booth, A.; Boran, F.; Bordoni, S.; Borges Merlo, R.; Borkum, A.; Bostan, N.; Bracinik, J.; Braga, D.; Brahma, B.; Brailsford, D.; Bramati, F.; Branca, A.; Brandt, A.; Bremer, J.; Brew, C.; Brice, S. J.; Brio, V.; Brizzolari, C.; Bromberg, C.; Brooke, J.; Bross, A.; Brunetti, G.; Brunetti, M.; Buchanan, N.; Budd, H.; Buergi, J.; Burgardt, D.; Butchart, S.; Caceres, G.; Cagnoli, I.; Cai, T.; Calabrese, R.; Calcutt, J.; Calin, M.; Calivers, L.; Calvo, E.; Caminata, A.; Camino, A. F.; Campanelli, W.; Campani, A.; Benitez, A. Campos; Canci, N.; Capo, J.; Caracas, I.; Caratelli, D.; Carber, D.; Carceller, J. M.; Carini, G.; Carlus, B.; Carneiro, M. F.; Carniti, P.; Terrazas, I. Caro; Carranza, H.; Carrara, N.; Carroll, L.; Carroll, T.; Carter, A.; Casarejos, E.; Casazza, D.; Castano Forero, J. F.; Castano, F. A.; Castillo, A.; Castromonte, C.; Catano-Mur, E.; Cattadori, C.; Cavalier, F.; Cavanna, F.; Centro, S.; Cerati, G.; Cerna, C.; Cervelli, A.; Cervera Villanueva, A.; Chakraborty, K.; Chakraborty, S.; Chalifour, M.; Chappell, A.; Charitonidis, N.; Chatterjee, A.; Chen, H.; Chen, M.; Chen, W. C.; Chen, Y.; Chen-Wishart, Z.; Cherdack, D.; Chi, C.; Chirco, R.; Chitirasreemadam, N.; Cho, K.; Choate, S.; Chokheli, D.; Chong, P. S.; Chowdhury, B.; Christian, D.; Chukanov, A.; Chung, M.; Church, E.; Cicala, M. F.; Cicerchia, M.; Cicero, V.; Ciolini, R.; Clarke, P.; Cline, G.; Coan, T. E.; Cocco, A. G.; Coelho, J. A. B.; Cohen, A.; Collazo, J.; Collot, J.; Conley, E.; Conrad, J. M.; Convery, M.; Copello, S.; Cova, P.; Cox, C.; Cremaldi, L.; Cremonesi, L.; Crespo-Anadon, J. I.; Crisler, M.; Cristaldo, E.; Crnkovic, J.; Crone, G.; Cross, R.; Cudd, A.; Cuesta, C.; Cui, Y.; Curciarello, F.; Cussans, D.; Dai, J.; Dalager, O.; Dallavalle, R.; Dallaway, W.; da Motta, H.; Dar, Z. A.; Darby, R.; Da Silva Peres, L.; David, Q.; Davies, G. S.; Davini, S.; Dawson, J.; De Aguiar, R.; De Almeida, P.; Debbins, P.; De Bonis, I.; Decowski, M. P.; de Gouvea, A.; De Holanda, P. C.; Astiz, IL De Icaza L. D. I.; De Jong, P.; Sanchez, P. Del Amo; De la Torre, A.; De Lauretis, G.; Delbart, A.; Delepine, D.; Delgado, M.; Dell'Acqua, A.; Delle Monache, G.; Delmonte, N.; De Lurgio, P.; Demario, R.; De Matteis, G.; de Mello Neto, J. R. T.; DeMuth, D. M.; Dennis, S.; Densham, C.; Denton, P.; Deptuch, G. W.; De Roeck, A.; De Romeri, V.; Detje, J. P.; Devine, J.; Dharmapalan, R.; Dias, M.; Diaz, A.; Diaz, J. S.; Diaz, F.; Di Capua, F.; Di Domenico, A.; Di Domizio, S.; Di Falco, S.; Di Giulio, L.; Ding, P.; Di Noto, L.; Diociaiuti, E.; Distefano, C.; Diurba, R.; Diwan, M.; Djurcic, Z.; Doering, D.; Dolan, S.; Dolek, F.; Dolinski, M. J.; Domenici, D.; Domine, L.; Donati, S.; Donon, Y.; Doran, S.; Douglas, D.; Doyle, T. A.; Dragone, A.; Drielsma, F.; Duarte, L.; Duchesneau, D.; Duffy, K.; Dugas, K.; Dunne, P.; Dutta, B.; Duyang, H.; Dwyer, D. A.; Dyshkant, A. S.; Dytman, S.; Eads, M.; Earle, A.; Edayath, S.; Edmunds, D.; Eisch, J.; Englezos, P.; Ereditato, A.; Erjavec, T.; Escobar, C. O.; Evans, J. J.; Ewart, E.; Ezeribe, A. C.; Fahey, K.; Fajt, L.; Falcone, A.; Fani', M.; Farnese, C.; Farrell, S.; Farzan, Y.; Fedoseev, D.; Felix, J.; Feng, Y.; Fernandez-Martinez, E.; Ferry, G.; Fields, L.; Filip, P.; Filkins, A.; Filthaut, F.; Fine, R.; Fiorillo, G.; Fiorini, M.; Fogarty, S.; Foreman, W.; Fowler, J.; Franc, J.; Francis, K.; Franco, D.; Franklin, J.; Freeman, J.; Fried, J.; Friedland, A.; Fuess, S.; Furic, I. K.; Furman, K.; Furmanski, A. P.; Gaba, R.; Gabrielli, A.; Gago, A. M.; Galizzi, F.; Gallagher, H.; Gallas, A.; Gallice, N.; Galymov, V.; Gamberini, E.; Gamble, T.; Ganacim, F.; Gandhi, R.; Ganguly, S.; Gao, F.; Gao, S.; Garcia-Gamez, D.; Garcia-Peris, M. A.; Gardim, F.; Gardiner, S.; Gastler, D.; Gauch, A.; Gauvreau, J.; Gauzzi, P.; Gazzana, S.; Ge, G.; Geffroy, N.; Gelli, B.; Gent, S.; Gerlach, L.; Ghorbani-Moghaddam, Z.; Giammaria, T.; Gibin, D.; Gil-Botella, I.; Gilligan, S.; Gioiosa, A.; Giovannella, S.; Girerd, C.; Giri, A. K.; Giugliano, C.; Giusti, V.; Gnani, D.; Gogota, O.; Gollapinni, S.; Gollwitzer, K.; Gomes, R. A.; Gomez Bermeo, L. V.; Gomez Fajardo, L. S.; Gonnella, F.; Gonzalez-Diaz, D.; Gonzalez-Lopez, M.; Goodman, M. C.; Goswami, S.; Gotti, C.; Goudeau, J.; Goudzovski, E.; Grace, C.; Gramellini, E.; Gran, R.; Granados, E.; Granger, P.; Grant, C.; Gratieri, D. R.; Grauso, G.; Green, P.; Greenberg, S.; Greer, J.; Griffith, W. C.; Groetschla, F. T.; Grzelak, K.; Gu, L.; Gu, W.; Guarino, V.; Guarise, M.; Guenette, R.; Guerard, E.; Guerzoni, M.; Guffanti, D.; Guglielmi, A.; Guo, B.; Guo, Y.; Gupta, A.; Gupta, V.; Gurung, G.; Gutierrez, D.; Guzowski, P.; Guzzo, M. M.; Gwon, S.; Habig, A.; Hadavand, H.; Haegel, L.; Haenni, R.; Hagaman, L.; Hahn, A.; Haiston, J.; Hakenmueller, J.; Hamernik, T.; Hamilton, P.; Hancock, J.; Happacher, F.; Harris, D. A.; Hartnell, J.; Hartnett, T.; Harton, J.; Hasegawa, T.; Hasnip, C.; Hatcher, R.; Hayrapetyan, K.; Hays, J.; Hazen, E.; He, M.; Heavey, A.; Heeger, K. M.; Heise, J.; Henry, S.; Morquecho, MA Hernandez A. H.; Herner, K.; Hewes, V.; Higuera, A.; Hilgenberg, C.; Hillier, S. J.; Himmel, A.; Hinkle, E.; Hirsch, L. R.; Ho, J.; Hoff, J.; Holin, A.; Holvey, T.; Hoppe, E.; Horiuchi, S.; Horton-Smith, G. A.; Hostert, M.; Houdy, T.; Howard, B.; Howell, R.; Hristova, I.; Hronek, M. S.; Huang, J.; Huang, R. G.; Hulcher, Z.; Ibrahim, M.; Iles, G.; Ilic, N.; Iliescu, A. M.; Illingworth, R.; Ingratta, G.; Ioannisian, A.; Irwin, B.; Isenhower, L.; Ismerio Oliveira, M.; Itay, R.; Jackson, C. M.; Jain, V.; James, E.; Jang, W.; Jargowsky, B.; Jena, D.; Jentz, I.; Ji, X.; Jiang, C.; Jiang, J.; Jiang, L.; Jipa, A.; Joaquim, F. R.; Johnson, W.; Jollet, C.; Jones, B.; Jones, R.; Jose Fernandez, D.; Jovancevic, N.; Judah, M.; Jung, C. K.; Junk, T.; Jwa, Y.; Kabirnezhad, M.; Kaboth, A. C.; Kadenko, I.; Kakorin, I.; Kalitkina, A.; Kalra, D.; Kandemir, M.; Kaplan, D. M.; Karagiorgi, G.; Karaman, G.; Karcher, A.; Karyotakis, Y.; Kasai, S.; Kasetti, S. P.; Kashur, L.; Katsioulas, I.; Kauther, A.; Kazaryan, N.; Ke, L.; Kearns, E.; Keener, P. T.; Kelly, K. J.; Kemp, E.; Kemularia, O.; Kermaidic, Y.; Ketchum, W.; Kettell, S. H.; Khabibullin, M.; Khan, N.; Khvedelidze, A.; Kim, D.; Kim, J.; Kim, M.; King, B.; Kirby, B.; Kirby, M.; Kish, A.; Klein, J.; Kleykamp, J.; Klustova, A.; Kobilarcik, T.; Koch, L.; Koehler, K.; Koerner, L. W.; Koh, D. H.; Kolupaeva, L.; Korablev, D.; Kordosky, M.; Kosc, T.; Kose, U.; Kostelecky, V. A.; Kothekar, K.; Kotler, I.; Kovalcuk, M.; Kozhukalov, V.; Krah, W.; Kralik, R.; Kramer, M.; Kreczko, L.; Krennrich, F.; Kreslo, I.; Kroupova, T.; Kubota, S.; Kubu, M.; Kudenko, Y.; Kudryavtsev, V. A.; Kufatty, G.; Kuhlmann, S.; Kumar, J.; Kumar, P.; Kumaran, S.; Kunze, P.; Kunzmann, J.; Kuravi, R.; Kurita, N.; Kuruppu, C.; Kus, V.; Kutter, T.; Kvasnicka, J.; Labree, T.; Lackey, T.; Lambert, A.; Land, B. J.; Lane, C. E.; Lane, N.; Lang, K.; Langford, T.; Langstaff, M.; Lanni, F.; Lantwin, O.; Larkin, J.; Lasorak, P.; Last, D.; Laudrain, A.; Laundrie, A.; Laurenti, G.; Lavaut, E.; Lawrence, A.; Laycock, P.; Lazanu, I.; Lazzaroni, M.; Le, T.; Leardini, S.; Learned, J.; LeCompte, T.; Lee, C.; Legin, V.; Miotto, G. Lehmann; Lehnert, R.; Leigui de Oliveira, M. A.; Leitner, M.; Silverio, D. Leon; Lepin, L. M.; Li, J. -Y.; Li, S. W.; Li, Y.; Liao, H.; Lin, C. S.; Lindebaum, D.; Linden, S.; Lineros, R. A.; Ling, J.; Lister, A.; Littlejohn, B. R.; Liu, H.; Liu, J.; Liu, Y.; Lockwitz, S.; Lokajicek, M.; Lomidze, I.; Long, K.; Lopes, T. V.; Lopez, J.; Lopez de Rego, I.; Lopez-March, N.; Lord, T.; LoSecco, J. M.; Louis, W. C.; Sanchez, A. Lozano; Lu, X. -G.; Luk, K. B.; Lunday, B.; Luo, X.; Luppi, E.; Maalmi, J.; MacFarlane, D.; Machado, A. A.; Machado, P.; Macias, C. T.; Macier, J. R.; MacMahon, M.; Maddalena, A.; Madera, A.; Madigan, P.; Magill, S.; Magueur, C.; Mahn, K.; Maio, A.; Major, A.; Majumdar, K.; Man, M.; Mandujano, R. C.; Maneira, J.; Manly, S.; Mann, A.; Manolopoulos, K.; Plata, M. Manrique; Manthey Corchado, S.; Manyam, V. N.; Marchan, M.; Marchionni, A.; Marciano, W.; Marfatia, D.; Mariani, Camillo; Maricic, J.; Marinho, F.; Marino, A. D.; Markiewicz, T.; Das Chagas Marques, F.; Marquet, C.; Marsden, D.; Marshak, M.; Marshall, C. M.; Marshall, J.; Martina, L.; Martin-Albo, J.; Martinez, N.; Caicedo, DA Martinez A. M.; Lopez, F. Martinez; Martinez Mirave, P.; Martynenko, S.; Mascagna, V.; Massari, C.; Mastbaum, A.; Matichard, F.; Matsuno, S.; Matteucci, G.; Matthews, J.; Mauger, C.; Mauri, N.; Mavrokoridis, K.; Mawby, I.; Mazza, R.; Mazzacane, A.; McAskill, T.; McConkey, N.; McFarland, K. S.; McGrew, C.; Mcnab, A.; Meazza, L.; Meddage, V. C. N.; Mehta, B.; Mehta, P.; Melas, P.; Mena, O.; Mendez, H.; Mendez, P.; Mendez, D. P.; Menegolli, A.; Meng, G.; Mercuri, A. C. E. A.; Meregaglia, A.; Messier, M. D.; Metallo, S.; Metcalf, J.; Metcalf, W.; Mewes, M.; Meyer, H.; Miao, T.; Miccoli, A.; Michna, G.; Mikola, V.; Milincic, R.; Miller, F.; Miller, G.; Miller, W.; Mineev, O.; Minotti, A.; Miralles, L.; Miranda, O. G.; Mironov, C.; Miryala, S.; Miscetti, S.; Mishra, C. S.; Mishra, S. R.; Mislivec, A.; Mitchell, M.; Mladenov, D.; Mocioiu, I.; Mogan, A.; Moggi, N.; Mohanta, R.; Mohayai, T. A.; Mokhov, N.; Molina, J.; Bueno, L. Molina; Montagna, E.; Montanari, A.; Montanari, C.; Montanari, D.; Montanino, D.; Montano Zetina, L. M.; Mooney, M.; Moor, A. F.; Moore, Z.; Moreno, D.; Moreno-Palacios, O.; Morescalchi, L.; Moretti, D.; Moretti, R.; Morris, C.; Mossey, C.; Mote, M.; Moura, C. A.; Mouster, G.; Mu, W.; Mualem, L.; Mueller, J.; Muether, M.; Muheim, F.; Muir, A.; Mulhearn, M.; Munford, D.; Munteanu, L. J.; Muramatsu, H.; Muraz, J.; Murphy, M.; Murphy, T.; Muse, J.; Mytilinaki, A.; Nachtman, J.; Nagai, Y.; Nagu, S.; Nandakumar, R.; Naples, D.; Narita, S.; Nath, A.; Navrer-Agasson, A.; Nayak, N.; Nebot-Guinot, M.; Nehm, A.; Nelson, J. K.; Neogi, O.; Nesbit, J.; Nessi, M.; Newbold, D.; Newcomer, M.; Nichol, R.; Nicolas-Arnaldos, F.; Nikolica, A.; Nikolov, J.; Niner, E.; Nishimura, K.; Norman, A.; Norrick, A.; Novella, P.; Nowak, J. A.; Oberling, M.; Ochoa-Ricoux, J. P.; Oh, S.; Oh, S. B.; Olivier, A.; Olshevskiy, A.; Olson, T.; Onel, Y.; Onishchuk, Y.; Oranday, A.; Osbiston, M.; Osorio Velez, J. A.; Otiniano Ormachea, L.; Ott, J.; Pagani, L.; Palacio, G.; Palamara, O.; Palestini, S.; Paley, J. M.; Pallavicini, M.; Palomares, C.; Pan, S.; Panda, P.; Vazquez, W. Panduro; Pantic, E.; Paolone, V.; Papadimitriou, V.; Papaleo, R.; Papanestis, A.; Papoulias, D.; Paramesvaran, S.; Paris, A.; Parke, S.; Parozzi, E.; Parsa, S.; Parsa, Z.; Parveen, S.; Parvu, M.; Pasciuto, D.; Pascoli, S.; Pasqualini, L.; Pasternak, J.; Patrick, C.; Patrizii, L.; Patterson, R. B.; Patzak, T.; Paudel, A.; Paulucci, L.; Pavlovic, Z.; Pawloski, G.; Payne, D.; Pec, V.; Pedreschi, E.; Peeters, S. J. M.; Pellico, W.; Perez, A. Pena; Pennacchio, E.; Penzo, A.; Peres, O. L. G.; Gonzalez, YF Perez F. P.; Perez-Molina, L.; Pernas, C.; Perry, J.; Pershey, D.; Pessina, G.; Petrillo, G.; Petta, C.; Petti, R.; Pfaff, M.; Pia, V.; Pickering, L.; Pietropaolo, F.; Pimentel, V. L.; Pinaroli, G.; Pinchault, J.; Pitts, K.; Plows, K.; Plunkett, R.; Pollack, C.; Pollman, T.; Polo-Toledo, D.; Pompa, F.; Pons, X.; Poonthottathil, N.; Popov, V.; Poppi, F.; Porter, J.; Potekhin, M.; Potenza, R.; Pozimski, J.; Pozzato, M.; Prakash, T.; Pratt, C.; Prest, M.; Psihas, F.; Pugnere, D.; Qian, X.; Raaf, J. L.; Radeka, V.; Rademacker, J.; Radics, B.; Rafique, A.; Raguzin, E.; Rai, M.; Rajagopalan, S.; Rajaoalisoa, M.; Rakhno, I.; Rakotondravohitra, L.; Ralte, L.; Delgado, MA Ramirez A. R.; Ramson, B.; Rappoldi, A.; Raselli, G.; Ratoff, P.; Ray, R.; Razafinime, H.; Rea, E. M.; Real, J. S.; Rebel, B.; Rechenmacher, R.; Reggiani-Guzzo, M.; Reichenbacher, J.; Reitzner, S. D.; Sfar, H. Rejeb; Renner, E.; Renshaw, A.; Rescia, S.; Resnati, F.; Restrepo, D.; Reynolds, C.; Ribas, M.; Riboldi, S.; Riccio, C.; Riccobene, G.; Ricol, J. S.; Rigan, M.; Rincon, E. V.; Ritchie-Yates, A.; Ritter, S.; Rivera, D.; Rivera, R.; Robert, A.; Rocabado Rocha, J. L.; Rochester, L.; Roda, M.; Rodrigues, P.; Alonso, MJ Rodriguez J. R.; Rondon, J. Rodriguez; Rosauro-Alcaraz, S.; Rosier, P.; Ross, D.; Rossella, M.; Rossi, M.; Ross-Lonergan, M.; Roy, N.; Roy, P.; Rubbia, C.; Ruggeri, A.; Ferreira, G. Ruiz; Russell, B.; Ruterbories, D.; Rybnikov, A.; Saa-Hernandez, A.; Saakyan, R.; Sacerdoti, S.; Sahoo, S. K.; Sahu, N.; Sala, P.; Samios, N.; Samoylov, O.; Sanchez, M. C.; Sanchez Bravo, A.; Sanchez-Lucas, P.; Sandberg, V.; Sanders, D. A.; Sanfilippo, S.; Sankey, D.; Santoro, D.; Saoulidou, N.; Sapienza, P.; Sarasty, C.; Sarcevic, I.; Sarra, I.; Savage, G.; Savinov, V.; Scanavini, G.; Scaramelli, A.; Scarff, A.; Schefke, T.; Schellman, H.; Schifano, S.; Schlabach, P.; Schmitz, D.; Schneider, A. W.; Scholberg, K.; Schukraft, A.; Schuld, B.; Segade, A.; Segreto, E.; Selyunin, A.; Senise, C. R.; Sensenig, J.; Shaevitz, M. H.; Shanahan, P.; Sharma, P.; Kumar, R.; Shaw, K.; Shaw, T.; Shchablo, K.; Shen, J.; Shepherd-Themistocleous, C.; Sheshukov, A.; Shi, W.; Shin, S.; Shivakoti, S.; Shoemaker, Ian; Shooltz, D.; Shrock, R.; Siddi, B.; Siden, M.; Silber, J.; Simard, L.; Sinclair, J.; Sinev, G.; Singh, Jaydip; Singh, J.; Singh, L.; Singh, P.; Singh, V.; Chauhan, S. Singh; Sipos, R.; Sironneau, C.; Sirri, G.; Siyeon, K.; Skarpaas, K.; Smedley, J.; Smith, E.; Smith, J.; Smith, P.; Smolik, J.; Smy, M.; Snape, M.; Snider, E. L.; Snopok, P.; Snowden-Ifft, D.; Nunes, M. Soares; Sobel, H.; Soderberg, M.; Sokolov, S.; Solano Salinas, C. J.; Soldner-Rembold, S.; Soleti, S. R.; Solomey, N.; Solovov, V.; Sondheim, W. E.; Sorel, M.; Sotnikov, A.; Soto-Oton, J.; Sousa, A.; Soustruznik, K.; Spinella, F.; Spitz, J.; Spooner, N. J. C.; Spurgeon, K.; Stalder, D.; Stancari, M.; Stanco, L.; Steenis, J.; Stein, R.; Steiner, H. M.; Steklain Lisboa, A. F.; Stepanova, A.; Stewart, J.; Stillwell, B.; Stock, J.; Stocker, F.; Stokes, T.; Strait, M.; Strauss, T.; Strigari, L.; Stuart, A.; Suarez, J. G.; Subash, J.; Surdo, A.; Suter, L.; Sutera, C. M.; Sutton, K.; Suvorov, Y.; Svoboda, R.; Swain, S. K.; Szczerbinska, B.; Szelc, A. M.; Sztuc, A.; Taffara, A.; Talukdar, N.; Tamara, J.; Tanaka, H. A.; Tang, S.; Taniuchi, N.; Tapia Casanova, A. M.; Oregui, B. Tapia; Tapper, A.; Tariq, S.; Tarpara, E.; Tatar, E.; Tayloe, R.; Tedeschi, D.; Teklu, A. M.; Vidal, J. Tena; Tennessen, P.; Tenti, M.; Terao, K.; Terranova, F.; Testera, G.; Thakore, T.; Thea, A.; Thiebault, A.; Thomas, S.; Thompson, A.; Thorn, C.; Timm, S. C.; Tiras, E.; Tishchenko, V.; Todorovic, N.; Tomassetti, L.; Tonazzo, A.; Torbunov, D.; Torti, M.; Tortola, M.; Tortorici, F.; Tosi, N.; Totani, D.; Toups, M.; Touramanis, C.; Tran, D.; Travaglini, R.; Trevor, J.; Triller, E.; Trilov, S.; Truchon, J.; Truncali, D.; Trzaska, W. H.; Tsai, Y.; Tsai, Y. -T.; Tsamalaidze, Z.; Tsang, K. V.; Tsverava, N.; Tu, S. Z.; Tufanli, S.; Tunnell, C.; Turner, J.; Tuzi, M.; Tyler, J.; Tyley, E.; Tzanov, M.; Uchida, M. A.; Urena Gonzalez, J.; Urheim, J.; Usher, T.; Utaegbulam, H.; Uzunyan, S.; Vagins, M. R.; Vahle, P.; Valder, S.; Valdiviesso, G. A.; Valencia, E.; Valentim, R.; Vallari, Z.; Vallazza, E.; Valle, J. W. F.; Van Berg, R.; Van de Water, R. G.; Forero, D. V.; Vannozzi, A.; Van Nuland-Troost, M.; Varanini, F.; Oliva, D. Vargas; Vasina, S.; Vaughan, N.; Vaziri, K.; Vazquez-Ramos, A.; Vega, J.; Ventura, S.; Verdugo, A.; Vergani, S.; Verzocchi, M.; Vetter, K.; Vicenzi, M.; Vieira De Souza, H.; Vignoli, C.; Vilela, C.; Villa, E.; Viola, S.; Viren, B.; Vizcaya-Hernandez, A.; Vrba, T.; Vuong, Q.; Waldron, A. V.; Wallbank, M.; Walsh, J.; Walton, T.; Wang, H.; Wang, J.; Wang, L.; Wang, M. H. L. S.; Wang, X.; Wang, Y.; Warburton, K.; Warner, D.; Warsame, L.; Wascko, M. O.; Waters, D.; Watson, A.; Wawrowska, K.; Weber, A.; Weber, C. M.; Weber, M.; Wei, H.; Weinstein, A.; Wenzel, H.; Westerdale, S.; Wetstein, M.; Whalen, K.; Whilhelmi, J.; White, A.; Whitehead, L. H.; Whittington, D.; Wilking, M. J.; Wilkinson, A.; Wilkinson, C.; Wilson, F.; Wilson, R. J.; Winter, P.; Wisniewski, W.; Wolcott, J.; Wolfs, J.; Wongjirad, T.; Wood, A.; Wood, K.; Worcester, E.; Worcester, M.; Wospakrik, M.; Wresilo, K.; Wret, C.; Wu, S.; Wu, W.; Wurm, M.; Wyenberg, J.; Xiao, Y.; Xiotidis, I.; Yaeggy, B.; Yahlali, N.; Yandel, E.; Yang, K.; Yang, T.; Yankelevich, A.; Yershov, N.; Yonehara, K.; Young, T.; Yu, B.; Yu, H.; Yu, J.; Yu, Y.; Yuan, W.; Zaki, R.; Zalesak, J.; Zambelli, L.; Zamorano, B.; Zani, A.; Zapata, O.; Zazueta, L.; Zeller, G. P.; Zennamo, J.; Zeug, K.; Zhang, C.; Zhang, S.; Zhao, M.; Zhivun, E.; Zimmerman, E. D.; Zucchelli, S.; Zuklin, J.; Zutshi, V.; Zwaska, R. (MDPI, 2025-09-11)
The Module-0 Demonstrator is a single-phase 600 kg liquid argon time projection chamber operated as a prototype for the DUNE liquid argon near detector. Based on the ArgonCube design concept, Module-0 features a novel 80k-channel pixelated charge readout and advanced high-coverage photon detection system. In this paper, we present an analysis of an eight-day data set consisting of 25 million cosmic ray events collected in the spring of 2021. We use this sample to demonstrate the imaging performance of the charge and light readout systems as well as the signal correlations between the two. We also report argon purity and detector uniformity measurements and provide comparisons to detector simulations.

Browse

Recent Submissions