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Viegas, R., Roser, J., Barrientos, L., Borja-Lloret, M., Brzezinski, K., Casaña, J. V., et al. (2027). Experimental tests of proton range verification with Compton cameras at proton therapy centers. Radiat. Phys. Chem., 251, 114447–14pp.
Abstract: Proton therapy is a precise cancer treatment that requires meticulous planning to deliver the prescribed dose to the target volume, while sparing healthy tissues. Compton cameras have emerged as a promising technology for in-vivo proton range verification through prompt-gamma detection, given their compactness and compatibility with the treatment gantry. This study evaluates the performance of the MACACOp Compton camera prototype, developed by the IRIS group at IFIC-Valencia, under progressively challenging conditions across several proton therapy facilities. The MACACOp camera, featuring monolithic LaBr3:Ce crystals and SiPM arrays, was tested at the Centro Nacional de Aceleradores, Cyclotron Center Bronowice, and Centro de Protonterapia Quir & oacute;nsalud. Under controlled conditions, the prototype was able to detect changes in photon emission distribution with high precision, resolving 1 mm displacements of a graphite target irradiated with a 8 nA proton beam, with the camera at 200 mm from the target. Additionally, the camera's enhanced timing resolution of 1.5 ns facilitates background rejection, an essential feature for proton therapy monitoring. Building on these results, the FALCON prototype was evaluated, demonstrating improved efficiency and the ability to reconstruct spots even under more challenging accelerator conditions. These findings underscore the potential of Compton cameras for real-time proton range verification, advancing their integration into clinical proton therapy systems.
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Xu, Y. H., Froustey, J., Fuller, G. M., Graf, L., & Patwardhan, A. V. (2026). Neutrino helicity oscillations in astrophysical environments: A many-body approach. Phys. Rev. D, 114(6), 063016–23pp.
Abstract: Neutrino rest mass enables left-handed states to “flip” to right-handed states and vice versa. In-medium effects can enhance the probability for such spin flip. We demonstrate that a full many-body calculation of this process in neutrino-dense environments can lead to spin-flip probabilities that exceed by orders of magnitude those calculated with mean-field treatments. We study simple configurations with a few neutrinos in well-defined momentum states, for which we show that the helicity conversion enhancement is connected to many-body momentum exchange. Such an effect would therefore be missed in a calculation that considers only forward processes. We speculate on the potential astrophysical implications of these results and the range of applicability of our calculation and its limitations.
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Catala, H., Valero, E., & Rodrigo, G. (2026). Quantum computing demonstration of the polaron-molecule transition on a noisy intermediate-scale quantum device. Phys. Rev. A, 114(3), 032609–11pp.
Abstract: The simulation of strongly correlated fermionic systems remains a significant challenge in computational physics due to the exponential growth of the Hilbert space and the fermionic sign problem. In this work, we report a quantum computing demonstration exploring the unified physics of the Fermi polaron and the Bose-Einstein condensate to Bardeen-Cooper-Schrieffer crossover. We develop an effective Hamiltonian formalism that bridges pairing superfluidity and impurity physics, mapping the system onto a gate-based quantum processor via the Jordan-Wigner transformation. By utilizing a first-order Trotter-Suzuki decomposition, we implement an ancilla-controlled Ramsey interferometry protocol to resolve the system's spectral response. Our implementation captures the smooth transition from a dressed quasiparticle (polaron) regime to a stable molecular bound state, characterized by a linear energy renormalization in the strong-coupling limit. We benchmark the quantum protocol against exact diagonalization and demonstrate its execution on the Barcelona Supercomputing Center quantum hardware. To ensure reproducibility, we provide comprehensive device calibration metrics, including qubit coherence times and gate fidelities at the time of execution. Despite inherent hardware noise, the hybrid variational approach qualitatively observes the bifurcation of the spectral density.
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HAWC Collaboration(Alfaro, R. et al), & Coutiño de Leon, S. (2026). HAWC Study on the Ultra-high-energy Gamma-Ray Emissions from the Pulsar Wind Nebula G32.64+0.53. Astrophys. J., 1009(1), 47–11pp.
Abstract: Multi-TeV gamma-ray emission around eHWC J1850+001 (a source from the first HAWC catalog of gamma-ray sources emitting above 56 TeV) is spatially coincident with the pulsar wind nebula (PWN) G32.64+0.53, powered by PSR J1849-0001. The absence of counterparts in radio, optical, and GeV energy ranges, contrasted with clear detections in X-rays and very-high-energy (VHE) gamma rays, is indicative of a nonthermal leptonic origin for the nebula. We apply a systematic analysis pipeline, including a sophisticated model for the Galactic diffuse emission, to 2860 days of data from the HAWC Observatory. Our detailed analysis confirms that the ultra-high-energy (UHE) emission originates from G32.64+0.53, and we measure its spectrum up to 270 TeV with significant emission well beyond 100 TeV. We fit the multiwavelength observations with a time-dependent leptonic model powered by the pulsar's rotational energy, and the results establish the nebula as a leptonic PeV accelerator, capable of accelerating electrons to a maximum energy of Ecut >= 2.9 PeV (95% one-sided lower bound). The model also constrains the nebular magnetic field to 4.28 μG, supporting a leptonic PWN origin for the observed UHE emission.
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Bonatto, A. et al, & Martin-Luna, P. (2026). Laser wakefield acceleration in nanostructured plasmas. Eur. Phys. J. Plus, 141(9), 1043–10pp.
Abstract: Solid-state plasma wakefield acceleration has recently attracted attention as a novel method for achieving unprecedented ultrahigh acceleration gradients on the order of 1 TeV/m or beyond. In this context, recent advancements in nanofabrication techniques have opened up the possibility of creating structured plasmas with tailored properties. For instance, the utilization of carbon nanotube (CNT) bundles holds great potential for generating stable plasmas with electron densities reaching as high as 1022 cm-3 , i.e., orders of magnitude higher than conventional gaseous plasmas. As part of a new collaborative effort called NanoAc, we have conducted particle-in-cell (PIC) simulations to investigate laser wakefield acceleration in nanostructured solid-state plasmas based on CNT arrays. Our results confirm the attainment of wakefields at the TV/m scale. Additionally, we observed self-injection, sub-femtosecond bunch formation, and electron acceleration in micrometer-scale targets, yielding kinetic energies on the order of a few tens of MeV. These findings open up promising possibilities to design novel ultracompact accelerators and radiation sources. In this paper, we report recent simulation results from the NanoAc collaboration and describe ongoing efforts toward future experimental tests at available laser facilities.
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