Probing Scalar Non-Standard Neutrino Interactions using High-Energy Astrophysical NeutrinosScalar non-standard interaction (SNSI) of neutrinos contributes as modifications to the neutrino mass matrix in the oscillation Hamiltonian and can induce a small active-sterile mass splitting due to…Ankur Verma, Carlos A. Argüelles, P. S. Bhupal Dev et al.·Aug 7, 2026SaveLearn
Domain Structures and Static Potentials in \(G2\) Gauge TheoryWe investigate the domain structures of the \(G2\) vacuum and the associated static potentials within the domain model, considering both zero and non-zero aggregate flux vacuum domains. Potentials…Seyed Mohsen Hosseini Nejad·Aug 7, 2026SaveLearn
Spiral structure and logarithmic evolution of deuteron form factors: evidence for a transitional regime in QCDWe present a consistent analysis of elastic electron--deuteron scattering combining perturbative quantum chromodynamics (pQCD) scaling, helicity amplitudes, and phenomenological parameterizations of…Yaroslav D. Krivenko-Emetov, Iryna Myroshnykova·Aug 7, 2026SaveLearn
Loop-Induced Higgs Boson Decays into Gauge Bosons in Radiative Natural SupersymmetryIn this article, we study loop-induced Higgs decays into gauge bosons within the framework of Radiative Natural Supersymmetry. We reproduce the one-loop MSSM calculations for the Higgs partial decay…Edilson A. Reyes R·Aug 7, 2026SaveLearn
Compressed Stop-Neutralino Spectra from Yukawa Unified Non-Holomorphic Pati-Salam Model: Prospects for the FCCWe explore the weak-scale phenomenology of SUSY models with the SU(4)C× SU(2)L× SU(2)R gauge symmetry. We include non-holomorphic soft supersymmetry breaking terms arising from…Ali Cici, Busra Nis, Cem Salih Un·Aug 7, 2026SaveLearn
Magnetic-monopole resummation justifies perturbatively calculated collider production cross sectionsA one-loop resummation scheme, inspired by Dyson-Schwinger (DS) formalism of strongly coupled quantum field theories, is applied to spin-1/2 magnetic monopoles (MMs), in the context of an effective…Jean Alexandre, Nick E. Mavromatos, Vasiliki A. Mitsou et al.·Aug 7, 2026SaveLearn
Decoding the Amplitude Pair with Distinct CPV Phases in Charmed Baryon DecaysIn this Letter, we propose a strategy to extract information on the hierarchical amplitude pair in singly Cabibbo-suppressed (SCS) charmed baryon two-body decays, with a dominant amplitude…Zhi-Peng Xing, Jin Sun, Xiao-Gang He·Aug 7, 2026SaveLearn
Baryons and baryoniums in the perspective of QCD sum rulesFollowing the experimental confirmation of tetraquark and pentaquark states, the search for hexaquark states has emerged as a new frontier in hadron physics. The recent observation of X(1840) and…Sheng-Qi Zhang, Cong-Feng Qiao·Aug 7, 2026SaveLearn
Symmetry-Protected α-Attractor Hybrid Inflation in Supergravity and Constraints from ACT DR6 and DESI DR2We present a symmetry-protected supergravity effective realization of hybrid α-attractor inflation with a sequestered Stückelberg uplift. The model contains four chiral multiplets, an inflaton…Swapnil Kumar Singh·Aug 7, 2026SaveLearn
Axion Production and Detection Using a Dual NMR-type ExperimentAxions that couple to nuclear spins via the axial current interaction can be both produced and detected using nuclear magnetic resonance (NMR) techniques. In this scheme, nuclei driven by a real…Jeff A. Dror, Qiushi Wei, Fengwei Yang·Aug 7, 2026SaveLearn
Small Progenitors, Large Couplings: Type Ic Supernova Constraints on Radiatively Decaying ParticlesSupernova (SN) 1987A provides classic bounds on gamma-ray flashes from the radiative decay of sub-GeV particles, but the latter may decay so rapidly as to be shielded by the stellar envelope. Using…Francisco R. Candón, Damiano F. G. Fiorillo, Hans-Thomas Janka et al.·Aug 7, 2026SaveLearn
Unbinning global LHC analysesNeural simulation-based inference has been shown to outperform traditional, histogram-based inference in numerous phenomenological and experimental studies at the LHC. So far, these analyses have…Henning Bahl, Tilman Plehn, Nikita Schmal·Aug 7, 2026SaveLearn
Rotational susceptibility of a hot and dense hadronic matterWe study the effect of global rotation on rotational susceptibilities (χ(1) ω, χ2 ω, etc.), which quantify how much the system responds to small angular velocities, in a hadron…Bhagyarathi Sahoo, Kshitish Kumar Pradhan, Dushmanta Sahu et al.·Aug 7, 2026SaveLearn
Darkonia at CollidersDark matter may form bound states in a dark sector with an attractive force between two dark matter particles. Searches for dark matter at colliders can differ dramatically from routine searches if…Yang Bai, Susanne Westhoff·Aug 7, 2026SaveLearn
Ultraviolet Flavor Transmission to T-Violating Neutrino Oscillation Observables in a Seesaw Framework with Sterile Mixing and Planck-Suppressed CorrectionsWe construct, numerically validate, and phenomenologically constrain a pipeline connecting a spontaneously CP-violating ultraviolet Type-I seesaw boundary condition to Planck-suppressed corrections…Poulastya Kar, Bipin Singh Koranga, Vivek Nautiyal·Aug 6, 2026SaveLearn
Quantum Computers will constrain the Equation of State of Neutron StarsThe Equation of State (EoS) of Nuclear Matter at high densities, and particularly that of neutron stars, resists ab initio Quantum Chromodynamics (QCD) computations due to the…Adrián Castaño-García, Nahia J. Dios-Bilbao, J. J. Gálvez-Viruet et al.·Aug 6, 2026SaveLearn
Oscillating Neutrinos vs. Oscillating Scalars: Constraining Scalar Dark Matter-Induced Neutrino MassWe consider the hypothesis that neutrino masses are generated by a coupling to an ultra-light (pseudo-)scalar field, which provides the dark matter in the universe. This leads to time-varying…Kierthika Chathirathas, Sabya Sachi Chatterjee, Thomas Schwetz·Aug 6, 2026SaveLearn
Logarithmic Wavelets for Dark Matter--Phonon ScatteringPhonon excitations in crystals are a promising detection channel for sub-GeV dark matter (DM), and anisotropic targets add directional sensitivity through the daily modulation of the rate. Exploiting…Xu-Xiang Li, Zhengkang Zhang·Aug 6, 2026SaveLearn
Generative Amplification with Surrogate Monte CarloAmplitude surrogates for LHC simulations build on generative amplification, the fact that a surrogate trained on an expensive and small training dataset describes the smooth amplitude more precisely…Henning Bahl, Tilman Plehn, Rebecca Revelli·Aug 6, 2026SaveLearn
Infrared singularities and the collinear limits of multi-leg scattering amplitudesScattering amplitudes admit a factorised structure in special kinematic limits, such as the soft and collinear limits. In this work, we investigate the multi-particle collinear limits of massless…Sebastian Jaskiewicz·Aug 6, 2026SaveLearn
Impact of dimension-8 SMEFT operators on baryogenesis via sphaleron decouplingWe investigate whether a baryogenesis mechanism known as sphalerogenesis can account for the observed baryon asymmetry of the Universe within the Standard Model effective field theory. In this…Kiyoto Ogawa, Masanori Tanaka·Aug 6, 2026SaveLearn
QCD analytic couplingA brief overview of QCD analytic coupling is presented, mainly following the results obtained in [1]. An application to the pion-photon transition form factor is demonstrated.I. A. Zemlyakov, I. L. Chuev, A. V. Kotikov·Aug 6, 2026SaveLearn
Descoped and Upscoped FCC-ee Running Scenarios in the SMEFTWe present projections for the sensitivity to new physics of descoped and upscoped FCC-ee scenarios in the framework of the Standard Model Effective Field Theory (SMEFT). Starting from the baseline…Eugenia Celada, Elie Hammou, Jaco ter Hoeve et al.·Aug 6, 2026SaveLearn
Machine Learning is Good for Physics - and Vice VersaScientific AI is rapidly transforming fundamental physics research and challenging defining aspects of the fundamental physics methodology. We discuss opportunities and dangers of this transformation…Michael Krämer, Tilman Plehn·Aug 6, 2026SaveLearn
Net electron spin rotation in a plane-wave pulse: Holonomy set by the anomalous magnetic momentWe compute the spin rotation that survives after a relativistic electron has crossed a plane-wave laser pulse of finite duration. In the interaction picture built on the exact g=2 evolution, the…N. S. Akintsov, A. P. Nevecheria, S. N. Andreev et al.·Aug 6, 2026SaveLearn