Kitasato University
We report the first detection of gamma-ray emission from the Galactic center in the 150-600 keV band using a linear, imaging-spectroscopy approach used in common telescopes with an electron-tracking Compton camera (ETCC) aboard the SMILE-2+ balloon experiment. A one-day flight over Australia resulted in a significant gamma-ray detection in the light curve and revealed a 7.9σ7.9\sigma excess in the image map from the Galactic center region. These results, obtained through a simple and unambiguous analysis, demonstrate the high reliability and sensitivity of the ETCC and establish its potential for future high-precision MeV gamma-ray observations. The measured intensity and spatial distribution were tested against three emission models: a single point-like source, a multi-component structure, and a symmetric two-dimensional Gaussian. All models were found to be statistically consistent with the data. The positronium-related flux in the multi-component model is (3.2 ± 1.4) × 102(3.2~\pm~1.4)~\times~10^{-2} photons cm2^{-2}s1^{-1}, which is approximately a factor of two higher than the value reported by INTEGRAL, with a discrepancy at the 2σ2\sigma level. This difference may arise from unresolved sources or truly diffuse emission, such as exotic processes involving light dark matter or primordial black holes.
We study electric-magnetic duality in Lorentz invariant symmetric tensor gauge theories, where immobile charged particles - fractons - arise due to the generalized current conservation μνJμν=0\partial_{\mu} \partial_{\nu} J^{\mu \nu} = 0 and the fracton gauge principle. We show that the duality in the symmetric gauge theories holds only in four-dimensional spacetime. In higher dimensions, the duality does not hold with only the symmetric gauge fields but tensor fields with more complex symmetries come into play. Furthermore, we show that a hierarchy for the symmetric gauge field theories of higher ranks is interpreted by the bi-form calculus. We also discuss the restricted immobility of pp-branes in the mixed symmetric gauge theories. As a byproduct, we find that novel self-duality conditions are defined as BPS equations in the four-dimensional Euclidean space.
We investigate doubled (generalized) complex structures in 2D2D-dimensional Born geometries where T-duality symmetry is manifestly realized. We show that Kähler, hyperkähler, bi-hermitian and bi-hypercomplex structures of spacetime are implemented in Born geometries as doubled structures. We find that the Born structures and the generalized Kähler (hyperkähler) structures appear as subalgebras of bi-quaternions and split-tetra-quaternions. We find parts of these structures are classified by Clifford algebras. We then study the T-duality nature of the worldsheet instantons in Born sigma models. We show that the instantons in Kähler geometries are related to those in bi-hermitian geometries in a non-trivial way.
We study an analogue of the Drinfel'd double for algebroids associated with the O(D,D+n)O(D,D+n) gauged double field theory (DFT). We show that algebroids defined by the twisted C-bracket in the gauged DFT are built out of a direct sum of three (twisted) Lie algebroids. They exhibit a "tripled", which we call the extended double, rather than the "doubled" structure appeared in (ungauged) DFT. We find that the compatibilities of the extended doubled structure result not only in the strong constraint but also the additional condition in the gauged DFT. We establish a geometrical implementation of these structures in a (2D+n)(2D+n)-dimensional product manifold and examine the relations to the generalized geometry for heterotic string theories and non-Abelian gauge symmetries in DFT.
Large Language Models (LLMs) have demonstrated impressive performance. To understand their behaviors, we need to consider the fact that LLMs sometimes show qualitative changes. The natural world also presents such changes called phase transitions, which are defined by singular, divergent statistical quantities. Therefore, an intriguing question is whether qualitative changes in LLMs are phase transitions. In this work, we have conducted extensive analysis on texts generated by LLMs and suggested that a phase transition occurs in LLMs when varying the temperature parameter. Specifically, statistical quantities have divergent properties just at the point between the low-temperature regime, where LLMs generate sentences with clear repetitive structures, and the high-temperature regime, where generated sentences are often incomprehensible. In addition, critical behaviors near the phase transition point, such as a power-law decay of correlation and slow convergence toward the stationary state, are similar to those in natural languages. Our results suggest a meaningful analogy between LLMs and natural phenomena.
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We investigate the chiral soliton lattice (CSL) in the framework of holographic QCD in magnetic field. Under appropriate boundary conditions for the gauge field and the quark mass deformation, we demonstrate that the ground state in the gravitational dual of QCD is given by the CSL in the background magnetic field and the baryon number density. In the presence of the background magnetic field, we show that the CSL is interpreted as a uniformly distributed D4-branes in the holographic setup, where the chiral soliton is identified with a non-self-dual instanton vortex or a center vortex in the five dimensional bulk gauge theory. While the baryon numbers are given to chiral solitons as well as Skyrmions due to the different terms in the Wess-Zumino-Witten (WZW) term in the chiral perturbation theory, these baryon numbers with different origins are unified in terms of the instanton charge density in five dimensions. With bulk analysis of the WZW term, we find that the pion decay constant becomes dependent on the magnetic field. For the massless pion case, we obtain an analytical form that is in qualitative agreement with lattice QCD results for strong magnetic fields.
We study the O(D,D+n)O(D,D+n) generalized metric and the gauge symmetries in the gauged double field theory (DFT) in view of current algebras and sigma models. We show that the O(D,D+n)O(D,D+n) generalized metric in the gauged DFT is consistent with the heterotic sigma models at the leading order in the α\alpha'-corrections. We then study the non-Abelian gauge symmetries and current algebras of heterotic string theories. We show that the algebras exhibit the correct diffeomorphism, the BB-field gauge transformations of the background fields together with the non-Abelian gauge transformations possibly with the appropriate local Lorentz transformations.
Tohoku University logoTohoku UniversityUniversity of MississippiUniversity of CincinnatiNational United UniversityKyungpook National UniversityHiroshima Institute of TechnologyINFN Sezione di NapoliCharles UniversityNational Central UniversityChinese Academy of Sciences logoChinese Academy of SciencesBudker Institute of Nuclear Physics SB RASGyeongsang National UniversityTel Aviv University logoTel Aviv UniversityKorea UniversityUniversity of Science and Technology of China logoUniversity of Science and Technology of ChinaChonnam National UniversityIndiana UniversitySungkyunkwan UniversityNational Taiwan UniversityUniversity of BonnPanjab UniversityNagoya University logoNagoya UniversityUniversity of TabukUniversity of MelbourneIndian Institute of Technology BhubaneswarUniversity of LjubljanaYonsei UniversityPeking University logoPeking UniversityUniversity of Florida logoUniversity of FloridaPacific Northwest National LaboratoryUniversity of Tokyo logoUniversity of TokyoUniversité Paris-Saclay logoUniversité Paris-SaclayTechnionShandong University logoShandong UniversityÉcole Polytechnique Fédérale de Lausanne (EPFL)University of Sydney logoUniversity of SydneyNovosibirsk State UniversityHanyang UniversityWayne State UniversityHigh Energy Accelerator Research Organization (KEK)Indian Institute of Technology MadrasKitasato UniversityKarlsruhe Institute of Technology logoKarlsruhe Institute of TechnologyUniversity of LouisvilleMoscow Institute of Physics and TechnologyUniversity of MariborUniversity of South CarolinaTokyo Metropolitan UniversitySOKENDAI (The Graduate University for Advanced Studies)University of Eastern FinlandJozef Stefan InstituteDongguk UniversityINFN, Sezione di TorinoNihon UniversityIndian Institute of Technology GuwahatiIndian Institute of Technology HyderabadUniversità di Napoli Federico IIInha UniversityUniversity of Hawai’iKanagawa UniversityMax-Planck-Institut für PhysikCNRS/IN2P3Yamagata UniversityInstitute of high-energy PhysicsLudwig-Maximilian-UniversityJustus Liebig University GiessenKumamoto UniversityKonkuk UniversityDeutsches Elektronen SynchrotronUniversity of ToyamaChristopher Newport UniversityMalaviya National Institute of Technology JaipurUniversity of MiyazakiUniversity of South AlabamaUniversity of Southern MississippiLiaoning Normal UniversityUniversity of California at Santa BarbaraToho UniversityUniversity of GiessenNara University of EducationNara Women’s UniversityP.N. Lebedev Physical Institute of the Russian Academy of SciencesH. Niewodniczanski Institute of Nuclear PhysicsKobayashi-Maskawa Institute for the Origin of Particles and the Universe,Kinki UniversityNihon Dental CollegeNippon Dental UniversityNational Institute of Science Education and Research, HBNIJ-PARCNational Museum of Nature and ScienceKawasaki Medical SchoolOsaka-city UniversityIndian Institute of Science Education and Research −KolkataUniversit Clermont Auvergne
Charged lepton flavor violation is forbidden in the Standard Model but possible in several new physics scenarios. In many of these models, the radiative decays τ±±γ\tau^{\pm}\rightarrow\ell^{\pm}\gamma (=e,μ\ell=e,\mu) are predicted to have a sizeable probability, making them particularly interesting channels to search at various experiments. An updated search via τ±±γ\tau^{\pm}\rightarrow\ell^{\pm}\gamma using full data of the Belle experiment, corresponding to an integrated luminosity of 988 fb1^{-1}, is reported for charged lepton flavor violation. No significant excess over background predictions from the Standard Model is observed, and the upper limits on the branching fractions, B(τ±μ±γ)\mathcal{B}(\tau^{\pm}\rightarrow \mu^{\pm}\gamma) \leq 4.2×1084.2\times10^{-8} and B(τ±e±γ)\mathcal{B}(\tau^{\pm}\rightarrow e^{\pm}\gamma) \leq 5.6×1085.6\times10^{-8}, are set at 90\% confidence level.
In this document, the technical details of the JSNS2^2 (J-PARC Sterile Neutrino Search at J-PARC Spallation Neutron Source) experiment are described. The search for sterile neutrinos is currently one of the hottest topics in neutrino physics. The JSNS2^2 experiment aims to search for the existence of neutrino oscillations with Δm2\Delta m^2 near 1 eV2^2 at the J-PARC Materials and Life Science Experimental Facility (MLF). A 1 MW beam of 3 GeV protons incident on a spallation neutron target produces an intense neutrino beam from muon decay at rest. Neutrinos come predominantly from μ+\mu^+ decay: μ+e++νˉμ+νe\mu^{+} \to e^{+} + \bar{\nu}_{\mu} + \nu_{e}. The experiment will search for νˉμ\bar{\nu}_{\mu} to νˉe\bar{\nu}_{e} oscillations which are detected by the inverse beta decay interaction νˉe+pe++n\bar{\nu}_{e} + p \to e^{+} + n, followed by gammas from neutron capture on Gd. The detector has a fiducial volume of 17 tons and is located 24 meters away from the mercury target. JSNS2^2 offers the ultimate direct test of the LSND anomaly. In addition to the sterile neutrino search, the physics program includes cross section measurements with neutrinos with a few 10's of MeV from muon decay at rest and with monochromatic 236 MeV neutrinos from kaon decay at rest. These cross sections are relevant for our understanding of supernova explosions and nuclear physics.
We investigate T-duality transformation on an almost bi-hermitian space with torsion. By virtue of the Buscher rule, we completely describe not only the covariant derivative of geometrical objects but also the Nijenhuis tensor. We apply this description to an almost bi-hermitian space with isometry and investigate integrability on its T-dualized one. We find that hermiticity is not a sufficient condition to preserve integrability under T-duality transformations. However, in the presence of the K\"{a}hler condition, the T-dualized space still admits integrability of the almost complex structures. We also observe that the form of H-flux is suitable for string compactification scenarios.
ETH Zurich logoETH ZurichCalifornia Institute of Technology logoCalifornia Institute of TechnologyUniversity of ZurichNagoya University logoNagoya UniversityUniversität HeidelbergUniversity of Tokyo logoUniversity of TokyoUniversity of Arizona logoUniversity of ArizonaAalto University logoAalto UniversityUniversity of TurkuDeutsches Elektronen-Synchrotron DESYUniversity of GenevaLiverpool John Moores UniversityUniversitat de BarcelonaUniversidade Federal do ABCUniversität WürzburgKitasato UniversityIlia State UniversityUniversity of OuluTokai UniversityINAF - Osservatorio Astrofisico di TorinoHiroshima UniversityUniversità di TriesteJet Propulsion LaboratoryInstituto de Astrofísica de CanariasUniversidad de ChileUniversitat Autònoma de BarcelonaICRANetINFN, Sezione di TorinoSofia UniversityUniversität InnsbruckUniversity of RijekaTechnische Universität DortmundUniversidad de La LagunaJosip Juraj Strossmayer University of OsijekCrimean Astrophysical ObservatoryKonan UniversityKazan Federal UniversityInstituto de Astrofísica de Andalucía-CSICUlugh Beg Astronomical InstituteMax-Planck-Institut für PhysikAryabhatta Research Institute of Observational Sciences (ARIES)The Barcelona Institute of Science and TechnologyINFN Sezione di PerugiaCIEMATInstitut de Física d’Altes Energies (IFAE)INFN - Sezione di PadovaUniversidad ComplutenseUniversità di UdineUniversità di PerugiaSteward ObservatoryPulkovo ObservatoryINFN PisaUniversitá dell’InsubriaAstronomical Observatory BelgradeKavli Institute for the Physics and Mathematics of the Universe (WPI),Università di SienaUniversità e del Politecnico di BariInstitute for Nuclear Research and Nuclear Energy, Bulgarian Academy of SciencesUniversity of ŁódźShumen UniversityCaltech Optical ObservatoriesLandessternwarteINFN RomaAbastumani ObservatoryInstitute of Astronomy and National Astronomical Observatory, Bulgarian Academy of SciencesSaha Institute of Nuclear Physics, HBNIISDCINFN (Sezione di Bari)Astronomical Institute, St. Petersburg State UniversityPort d'Informació Científica (PIC)INAF – National Institute for AstrophysicsInstitute for Astrophysical Research, Boston UniversitySweetwater Union High School DistrictOsservatorio Astrofisico di AsiagoAstronomical Institute, Uzbek Academy of SciencesEngelhardt Astronomical ObservatoryUniversit di CataniaUniversit di Roma La SapienzaCalifornia State University-SacramentoUniversit di PisaUniversit di PadovaUniversit degli Studi di TorinoINFN Sezione di TriesteINAF ` Osservatorio Astronomico di Trieste
PG 1553+113 is one of the few blazars with a convincing quasi-periodic emission in the gamma-ray band. The source is also a very high-energy (VHE; >100 GeV) gamma-ray emitter. To better understand its properties and identify the underlying physical processes driving its variability, the MAGIC Collaboration initiated a multiyear, multiwavelength monitoring campaign in 2015 involving the OVRO 40-m and Medicina radio telescopes, REM, KVA, and the MAGIC telescopes, Swift and Fermi satellites, and the WEBT network. The analysis presented in this paper uses data until 2017 and focuses on the characterization of the variability. The gamma-ray data show a (hint of a) periodic signal compatible with literature, but the X-ray and VHE gamma-ray data do not show statistical evidence for a periodic signal. In other bands, the data are compatible with the gamma-ray period, but with a relatively high p-value. The complex connection between the low and high-energy emission and the non-monochromatic modulation and changes in flux suggests that a simple one-zone model is unable to explain all the variability. Instead, a model including a periodic component along with multiple emission zones is required.
We present the first measurement of the missing energy due to nuclear effects in monoenergetic, muon neutrino charged-current interactions on carbon, originating from K+μ+νμK^+ \rightarrow \mu^+ \nu_\mu decay at rest (Eνμ=235.5E_{\nu_\mu}=235.5 MeV), performed with the J-PARC Sterile Neutrino Search at the J-PARC Spallation Neutron Source liquid scintillator based experiment. Toward characterizing the neutrino interaction, ostensibly $\nu_\mu n \rightarrow \mu^- por or \nu_\mu^{12}\mathrm{C} \rightarrow \mu^-^{12}\mathrm{N}$, we define the missing energy as the energy transferred to the nucleus (ω\omega) minus the kinetic energy of the outgoing proton(s), EmωTpE_{m} \equiv\omega-\sum T_p, and relate this to visible energy in the detector, $E_{m}=E_{\nu_\mu} (235.5 \mathrm{MeV})-m_\mu (105.7 \mathrm{MeV}) + [m_n-m_p (1.3 \mathrm{MeV})] - E_{\mathrm{vis}}$. The missing energy, which is naively expected to be zero in the absence of nuclear effects (e.g. nucleon separation energy, Fermi momenta, and final-state interactions), is uniquely sensitive to many aspects of the interaction, and has previously been inaccessible with neutrinos. The shape-only, differential cross section measurement reported, based on a (77±3)(77\pm3)% pure double-coincidence kaon decay-at-rest signal (621 total events), provides detailed insight into neutrino-nucleus interactions, allowing even the nuclear orbital shell of the struck nucleon to be inferred. The measurement provides an important benchmark for models and event generators at hundreds of MeV neutrino energies, characterized by the difficult-to-model transition region between neutrino-nucleus and neutrino-nucleon scattering, and relevant for applications in nuclear physics, neutrino oscillation measurements,and Type-II supernova studies.
Neutrino emission from nuclear reactors provides real-time insights into reactor power and fuel evolution, with potential applications in monitoring and nuclear safeguards. Following reactor shutdown, a low-intensity flux of ``residual neutrinos'' persists due to the decay of long-lived fission isotopes in the partially burnt fuel remaining within the reactor cores and in spent nuclear fuel stored in nearby cooling pools. The Double Chooz experiment at the Chooz B nuclear power plant in France achieved the first quantitative measurement of this residual flux based on 17.2 days of reactor-off data. In the energy range where the residual signal is most pronounced, the neutrino detector located 400\,m from the cores recorded 106±18106 \pm 18 neutrino candidate events (5.9σ\sigma significance). This measurement is in excellent agreement with the predicted value of 88±788 \pm 7 events derived from detailed reactor simulations modeling the decay activities of fission products and incorporating the best-available models of neutrino spectra.
Anharmonic decay of coherent optical phonons in semimetal Sb has been investigated by using a femtosecond pump-probe technique. The coherent A1gA_{1g} mode is observed in time domain in a wide temperature range of 7 - 290 K. The decay rate (the inverse of the dephasing time) systematically increases as the lattice temperature increases, which is well explained by anharmonic phonon-phonon coupling, causing decay of the optical phonon into two acoustic phonon modes. The frequency of the A1gA_{1g} mode decreases with the temperature, which is interpreted to the results of both thermal expansion and anharmonic phonon-phonon coupling. The temperature dependence of the amplitude of the coherent A1gA_{1g} mode exhibits a decrease with the lattice temperature, which is well reproduced by considering the peaked intensity of spontaneous Raman scattering assuming a Lorentzian line shape with the linewidth controlled by the anharmonic decay, and this model can be applicable to other metallic system, like Zn.
Molecular dynamics (MD) simulations were conducted using the generalized replica exchange method (gREM) on the 4-cyano-4^{\prime}-nn-alkylbiphenyl (nnCB) system with n=5n=5, 6, 7, and 8, which exhibits a nematic-isotropic (NI) phase transition. Sampling near the phase transition temperature in systems undergoing first-order phase transitions, such as the NI phase transition, is demanding due to the substantial energy gap between the two phases. To address this, gREM, specifically designed for first-order phase transitions, was utilized to enhance sampling near the NI phase transition temperature. Free-energy calculations based on the energy representation (ER) theory were employed to characterize the NI phase transition. ER evaluates the insertion free energy of nnCB molecule for both nematic and isotropic phases, revealing a change in the temperature dependence across the NI phase transition. Further decomposition into intermolecular interaction energetic and entropic terms shows quantitatively the balance between these contributions at the NI phase transition temperature.
We make a comprehensive study on the string winding corrections to supergravity solutions in double field theory (DFT). We find five-brane and wave solutions of diverse codimensions in which the winding coordinates are naturally included. We discuss a physical interpretation of the winding coordinate dependence. The analysis based on the geometric structures behind the solutions leads to an interpretation of the winding dependence as string worldsheet instanton corrections. We also give a brief discussion on the origins of these winding corrections in gauged linear sigma model. Our analysis reveals that for every supergravity solution, one has DFT solutions that include string winding corrections.
Social learning is learning through the observation of or interaction with other individuals; it is critical in the understanding of the collective behaviors of humans in social physics. We study the learning process of agents in a restless multiarmed bandit (rMAB). The binary payoff of each arm changes randomly and agents maximize their payoffs by exploiting an arm with payoff 1, searching the arm at random (individual learning), or copying an arm exploited by other agents (social learning). The system has Pareto and Nash equilibria in the mixed strategy space of social and individual learning. We study several models in which agents maximize their expected payoffs in the strategy space, and demonstrate analytically and numerically that the system converges to the equilibria. We also conducted an experiment and investigated whether human participants adopt the optimal strategy. In this experiment, three participants play the game. If the reward of each group is proportional to the sum of the payoffs, the median of the social learning rate almost coincides with that of the Pareto equilibrium.
Hydrogen-release by photoexcitation, excited-state- hydrogen-transfer (ESHT), is one of the important photo- chemical processes that occur in aromatic acids and is responsible for photoprotection of biomolecules. The mecha- nism is described by conversion of the initial state to a charge- separated state along the O(N)-H bond elongation, leading to dissociation. Thus ESHT is not a simple H-atom transfer in which a proton and a 1s electron move together. Here we show that the electron-transfer and the proton-motion are decoupled in gas-phase ESHT. We monitor electron and proton transfer independently by picosecond time-resolved near-infrared and infrared spectroscopy for isolated phenol--(ammonia)5, a benchmark molecular cluster. Electron transfer from phenol to ammonia occurred in less than 3 picoseconds, while the overall H-atom transfer took 15 picoseconds. The observed electron-proton decoupling will allow for a deeper understanding and control of of photochemistry in biomolecules
DESYKyoto Sangyo UniversityKyoto University logoKyoto UniversityETH Zürich logoETH ZürichOkayama UniversityUniversidad de GranadaThe University of Hong Kong logoThe University of Hong KongUniversity of Tokyo logoUniversity of TokyoGran Sasso Science InstituteFriedrich-Alexander-Universität Erlangen-NürnbergUniversity of ZagrebUniversité de GenèveChiba UniversityUniversität WürzburgUniversidad Complutense de MadridKitasato UniversityINAF - Osservatorio Astrofisico di TorinoHiroshima UniversityUniversidade Federal do Rio de JaneiroUniversità di TriesteUniversity of TsukubaKanazawa UniversityInstituto de Astrofísica de CanariasUniversität HamburgShibaura Institute of TechnologyTokyo Institute of TechnologyMoscow State UniversityUniversity of MontenegroShinshu UniversitySofia UniversityAstronomical Institute of the Czech Academy of SciencesNicolaus Copernicus Astronomical CenterUniversity of LodzUniversity of RijekaTechnische Universität DortmundLaboratoire d’Annecy de physique des particulesUniversity of StavangerUniversità di Napoli Federico IIKonan UniversityAoyama Gakuin UniversityInstituto de Astrofísica de Andalucía-CSICUniversität TübingenMax-Planck-Institut für PhysikINAF-Istituto di RadioastronomiaYamagata UniversityUniversità di BariUniversidad de JaénINAF – Osservatorio Astronomico di RomaInstitut de Física d’Altes Energies (IFAE)University of SplitAGH University of Science and TechnologyINAF - Osservatorio Astrofisico di CataniaUniversidad de GuadalajaraUniversità di UdineINFN, Sezione di CataniaIRFU, CEA, Université Paris-SaclayINFN Sezione di Roma Tor VergataUniversité de Paris, CNRS, Astroparticule et Cosmologie,National Astronomical Observatory of Japan (NAOJ)Università di SienaUniversity of the RyukyusUniversità di Tor VergataUniversité Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, ArtemisInstitut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and TechnologyUniversité Paris Cité, CNRS, Astroparticule et CosmologieLIP - Laboratório de Instrumentação e Física Experimental de PartículasLaboratoire Leprince-Ringuet, École Polytechnique, Institut Polytechnique de ParisNational Institute of Technology, Okinawa CollegeUniversité de Bordeaux, CNRS, LP2IClermont Auvergne University, CNRS, IN2P3, LPCThe Institute of Space and Astronautical Science (JAXA)Universit di FerraraUniversit di Roma La SapienzaUniversit di PisaUniversit di PadovaUniversit degli Studi di TorinoINAF Osservatorio di Astrofisica e Scienza dello Spazio di Bologna
The recurrent nova RS Ophiuchi (RS Oph) underwent a thermonuclear eruption in August 2021. In this event, RS Oph was detected by the High Energy Stereoscopic System (H.E.S.S.), the Major Atmospheric Gamma Imaging Cherenkov (MAGIC), and the first Large-Sized Telescope (LST-1) of the future Cherenkov Telescope Array Observatory (CTAO) at very-high gamma-ray energies above 100 GeV. This means that novae are a new class of very-high-energy (VHE) gamma-ray emitters. We report the analysis of the RS Oph observations with LST-1. We constrain the particle population that causes the observed emission in hadronic and leptonic scenarios. Additionally, we study the prospects of detecting further novae using LST-1 and the upcoming LST array of CTAO-North. We conducted target-of-opportunity observations with LST-1 from the first day of this nova event. The data were analysed in the framework of cta-lstchain and Gammapy, the official CTAO-LST reconstruction and analysis packages. One-zone hadronic and leptonic models were considered to model the gamma-ray emission of RS Oph using the spectral information from Fermi-LAT and LST-1, together with public data from the MAGIC and H.E.S.S. telescopes. RS Oph was detected at 6.6σ6.6\sigma with LST-1 in the first 6.35 hours of observations following the eruption. The hadronic scenario is preferred over the leptonic scenario considering a proton energy spectrum with a power-law model with an exponential cutoff whose position increases from (0.26±0.08)(0.26\pm 0.08) TeV on day 1 up to (1.6±0.6)(1.6\pm 0.6) TeV on day 4 after the eruption. The deep sensitivity and low energy threshold of the LST-1/LST array will allow us to detect faint novae and increase their discovery rate.
We propose a method of detecting non-self-correcting information cascades in experiments in which subjects choose an option sequentially by observing the choices of previous subjects. The method uses the correlation function C(t)C(t) between the first and the t+1t+1-th subject's choices. C(t)C(t) measures the strength of the domino effect, and the limit value $c\equiv \lim_{t\to \infty}C(t)determineswhetherthedominoeffectlastsforever determines whether the domino effect lasts forever (c>0)$ or not (c=0)(c=0). The condition c>0c>0 is an adequate condition for a non-self-correcting system, and the probability that the majority's choice remains wrong in the limit tt\to \infty is positive. We apply the method to data from two experiments in which TT subjects answered two-choice questions: (i) general knowledge questions (Tavg=60T_{avg}=60) and (ii) urn-choice questions (T=63T=63). We find c>0c>0 for difficult questions in (i) and all cases in (ii), and the systems are not self-correcting.
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