PaperPanorama

HEP Phenomenology·hep-ph

Thu·Oct 31, 2024

32 papers16 primary·16 cross-listed·reconstructed*

  1. 01*

    Point cloud-based diffusion models for the Electron-Ion Collider

    Jack Y. Araz🇺🇸 · Vinicius Mikuni🇺🇸 · Felix Ringer🇺🇸 · Nobuo Sato🇺🇸 · Fernando Torales Acosta🇺🇸 · Richard Whitehill🇺🇸

    At high-energy collider experiments, generative models can be used for a wide range of tasks, including fast detector simulations, unfolding, searches of physics beyond the Standard Model, and inference tasks. In particular, it has been demonstrated that score-based diffusion models can generate high-fidelity and accurate samples of jets or collider events. This work expands on previous generative models in three distinct ways. First, our model is trained to generate entire collider events, including all particle species with complete kinematic information. We quantify how well the model learns event-wide constraints such as the conservation of momentum and discrete quantum numbers. We focus on the events at the future Electron-Ion Collider, but we expect that our results can be extended to proton-proton and heavy-ion collisions. Second, previous generative models often relied on image-based techniques. The sparsity of the data can negatively affect the fidelity and sampling time of the model. We address these issues using point clouds and a novel architecture combining edge creation with transformer modules called Point Edge Transformers. Third, we adapt the foundation model OmniLearn, to generate full collider events. This approach may indicate a transition toward adapting and fine-tuning foundation models for downstream tasks instead of training new models from scratch.

    hep-phhep-exPLB(2025)·13 citations
  2. 02*

    Properties of the tensor state

    S. S. Agaev🇦🇿 · K. Azizi🇮🇷 · H. Sundu🇹🇷

    Spectroscopic parameters and decays of the exotic tensor meson with content are explored in the context of the diquark-antidiquark model. We treat it as a state built of axial-vector diquark and antidiquark , where is the charge conjugation matrix. The mass and current coupling of this tetraquark are extracted from two-point sum rules. Our result for proves that is unstable against strong dissociations to two-meson final states. Its dominant decay channels are processes , , and . Kinematically allowed transformations of include also decays and , which are generated by annihilation inside of . The full width of is estimated by considering all of these channels. Their partial widths are calculated by invoking methods of three-point sum rule approach which are required to evaluate strong couplings at corresponding tetraquark-meson-meson vertices. Our predictions for the mass and width of the tensor state provide useful information for experimental studies of fully heavy four-quark exotic structures.

    hep-phhep-exhep-latPRD(2025)·12 citations
  3. 03*

    Thermal effects on warm chromoinflation

    Vahid Kamali🇨🇦 · Rudnei O. Ramos🇧🇷

    We explore a model of a pseudo-Nambu-Goldstone boson inflaton field coupled to a non-Abelian gauge field. This model naturally leads to a warm inflation scenario, where the inflationary dynamics is dominated by thermal dissipation. In this work, we consider a scenario where the inflaton, an axion-like field, is coupled to the gauge field, similar to chromoinflation models. Both the inflaton and the gauge field with a non-vanishing vacuum expectation value are coupled to a thermal radiation bath. We demonstrate that the presence of the thermal bath during warm chromoinflation induces a thermal plasma mass for the background gauge field. This thermal mass can significantly disrupt the dynamics of the background gauge field, thereby driving it to its trivial null solution.

    hep-phastro-ph.COgr-qchep-thJCAP(2025)·4 citations
  4. 04*

    Investigating the Electroweak Phase Transition with a Real Scalar Singlet at a Muon Collider

    Mohamed Aboudonia🇦🇺 · Csaba Balazs🇦🇺 · Andreas Papaefstathiou🇺🇸 · Graham White🇬🇧

    A strong first-order electroweak phase transition (SFOEWPT) is essential for explaining baryogenesis and for potentially generating observable gravitational waves. This study investigates the potential of a high-energy muon collider to examine the occurrence of SFOEWPT within the context of a Standard Model extended by a real scalar singlet (xSM). We analyzed all possible decay modes of the singlet to constrain the valid parameter space of SFOEWPT, which was extracted numerically at different renormalization scales to account for theoretical uncertainties, thereby determining the sensitivity of a muon collider to the production and decay channels of novel heavy scalar particles that emerge in the xSM. The findings demonstrate that a 3 TeV muon collider can directly examine the nature of electroweak symmetry breaking by efficiently detecting novel scalar particles associated with a first-order electroweak phase transition through jet-rich final states, thus complementing the indirect constraints from gravitational wave experiments.

    hep-phastro-ph.COJHEP(2025)·10 citations
  5. 05*

    Beyond Hawking evaporation of black holes formed by dark matter in compact stars

    Ujjwal Basumatary🇮🇳 · Nirmal Raj🇮🇳 · Anupam Ray🇺🇸

    The memory burden effect is an explicit resolution to the information paradox by which an evaporating black hole acquires quantum hair, which then suppresses its rate of mass loss with respect to the semi-classical Hawking rate. We show that this has significant implications for particle dark matter that captures in neutron stars and forms black holes that go on to consume the host star. In particular, we show that constraints on the nucleon scattering cross section and mass of spin-0 and spin-1/2 dark matter would be extended by several orders of magnitude.

    hep-phastro-ph.HEhep-exhep-thPRD(2025)·31 citations
  6. 06*

    Revisiting the model for radiative neutrino masses with dark matter in the gauge theory

    Shinya Kanemura🇯🇵 · Yushi Mura🇯🇵 · Guohao Ying🇯🇵

    The radiative seesaw model with gauged extension is a well-motivated scenario which gives consistent predictions of active neutrino masses and the abundance of dark matter. Majorana masses of right-handed neutrinos, the lightest of which can be identified as dark matter, are given by the spontaneous breaking of the gauge symmetry. We revisit this model with the latest constraints from dark matter searches, neutrino oscillations, flavor experiments and collider experiments. We explore the feasible parameter space of this model, and find that there are still allowed regions under the latest experimental constraints. We present new viable benchmark scenarios for this model, i.e., the right-handed neutrino dark matter scenario and the scalar dark matter scenario. We also mention the testability of these benchmark scenarios at future experiments.

    hep-phPRD(2025)·2 citations
  7. 07*

    Searching for the toponium with the decay

    Yueling Yang🇨🇳 · Bingbing Yang🇨🇳 · Jiazhi Li🇨🇳 · Zhaojie Lu🇨🇳 · Junfeng Sun🇨🇳

    Inspired by the observation of the meson at the LHC and the promising prospect of the meson available at the approaching HL-LHC, branching ratios for the , , , , , and decays are roughly estimated. It is found that tens of opposite-charge dilepton events from the decay and hundreds of events from the decay using the single boson tagging method are expected to be accessible. This estimation provides a reference for future experimental study on the meson.

    hep-phhep-exCPC(2026)·6 citations
  8. 08*

    Radiative corrections and Monte Carlo tools for low-energy hadronic cross sections in collisions

    Riccardo Aliberti🇩🇪 · Paolo Beltrame🇬🇧 · Ettore Budassi🇮🇹 · Carlo M. Carloni Calame🇮🇹 · Gilberto Colangelo🇨🇭 · Lorenzo Cotrozzi🇬🇧 · Achim Denig🇩🇪 · Anna Driutti🇮🇹 · Tim Engel🇩🇪 · Lois Flower🇬🇧 · Andrea Gurgone🇮🇹 · Martin Hoferichter🇨🇭 and 23 other authors

    We present the results of Phase I of an ongoing review of Monte Carlo tools relevant for low-energy hadronic cross sections. This includes a detailed comparison of Monte Carlo codes for electron-positron scattering into a muon pair, pion pair, and electron pair, for scan and radiative-return experiments. After discussing the various approaches that are used and effects that are included, we show differential cross sections obtained with AfkQed, BabaYaga@NLO, KKMC, MCGPJ, McMule, Phokhara, and Sherpa, for scenarios that are inspired by experiments providing input for the dispersive evaluation of the hadronic vacuum polarisation.

    hep-phhep-exSciPost Phys.Comm.Rep.(2025)·54 citations
  9. 09*

    Spin Polarized Quasi-particle in Off-equilibrium Medium

    Shu Lin🇨🇳 · Jiayuan Tian🇨🇳

    It is usually believed that physics in off-equilibrium state characterized by hydrodynamic gradient can be equivalently studied using equilibrium state with suitable metric perturbation. We scrutinize this assumption using chiral kinetic theory in curved space, focusing on spin response to hydrodynamic gradient. Two effects of metric perturbation have been identified: one is to change particle motion by scattering it off the metric fields, which does capture spin response to hydrodynamic gradient, but is limited by kinematic condition in the scattering picture. The other is the genuine effect of off-equilibrium state, which is realizable by mapping the equilibrium state in curved space to flat space through a suitable frame choice. It lifts the kinematic condition in the spin response to hydrodynamic gradient. We classify off-equilibrium effect on spin polarization into modifications of (i) spectral function; (ii) distribution function; (iii) KMS relation. While the last two have been studied using chiral kinetic theory, the first one is usually ignored in kinetic description. We perform a detailed analysis on the first one, finding the radiative correction to spectral function leads to a polarized quasi-particle. The degeneracy of spin responses to different hydrodynamic sources at tree-level is also lifted by radiative correction.

    hep-phhep-thnucl-thPRD(2025)·9 citations
  10. 10*

    Impact of scalar NSI with off-diagonal parameters at DUNE and P2SO

    Sambit Kumar Pusty🇮🇳 · Rudra Majhi🇮🇳 · Dinesh Kumar Singha🇮🇳 · Monojit Ghosh🇭🇷 · Rukmani Mohanta🇮🇳

    In this paper, we studied the impact of the off-diagonal SNSI parameters in the future long-baseline neutrino oscillation experiments DUNE and P2SO. In our analysis, we found that the sensitivities of these experiments altered in a very non-trivial way due to the presence of these parameters. Depending on the values of these parameters, they can either completely mimic the standard scenario or can wash out their CP sensitivity. For large values of parameters and , we obtained larger mass ordering and octant sensitivities as compared to the standard three flavour scenario. For the parameter , the mass ordering sensitivity and the precision of deteriorated compared to the standard scenario. Our results also showed that the sensitivities were significantly influenced by the phases of the off-diagonal parameters.

    hep-phEPJC(2025)·4 citations
  11. 11*

    Probing optimal measurements of the electromagnetic dipole moments of the lepton

    Kartik Bhide🇩🇪 · Valerie Lang🇩🇪

    Precise measurements of the electromagnetic dipole moments of charged leptons are powerful probes of physics beyond the Standard Model of particle physics. It is essential to study avenues for optimizing the measurement strategies for the anomalous magnetic dipole moment (AMDM) and the electric dipole moment (EDM) of the -lepton which have recently become accessible at the Large Hadron Collider (LHC). In this work, we study the prospects of employing optimal observables for measuring the AMDM of the -lepton in PbPb collisions at the LHC. The performance of optimal observables is investigated in a statistical analysis, assuming an integrated luminosity of 2.0 nb, approximately corresponding to the amount of data collected during PbPb collisions in Run 2 of the LHC. Improvements of sensitivity to the AMDM with optimal observables are obtained only for a larger phase space than studied so far, more integrated luminosity or including the determination of the helicities of the -leptons. Both, chances and limitations, of optimal observables for the AMDM determination will be important to consider in future experiments.

    hep-phhep-ex5 citations
  12. 12*

    Testing the molecular nature of the with the and reactions

    Jing Song🇨🇳 · Wei-Hong Liang🇨🇳 · Chu-Wen Xiao🇨🇳 · Jorgivan Morais Dias🇨🇳 · Eulogio Oset🇪🇸

    We report on the reactions and ), and calculate the mass distributions and , respectively. We obtain clear peaks corresponding to the . From the decay of , we also get a second, broader, peak around , which comes from the decay to . This second peak is closely tied to the molecular picture of the with the and components. Its observation would provide a boost to the molecular picture of the .

    hep-phEPJC(2024)·5 citations
  13. 13*

    A Catalog of First-Order Electroweak Phase Transitions in the Standard Model Effective Field Theory

    Eliel Camargo-Molina🇸🇪 · Rikard Enberg🇸🇪 · Johan Löfgren🇸🇪

    We use modern dimensionally-reduced effective field theory methods, with careful attention to scale hierarchies, to analyze and catalog the types of first-order electroweak phase transitions that are possible in the Standard Model Effective Field Theory (SMEFT). Our calculations lay the necessary groundwork to perform gauge invariant, properly resummed perturbative expansions, and therefore address many of the theoretical problems with phase transition calculations. We find three types of configurations of the scalar potential that allow for a first-order phase transition, namely tree-level barriers, radiative barriers, or radiative symmetry breaking through the Coleman-Weinberg mechanism. We also find versions of these with significant supercooling. We perform a global likelihood scan over the Wilson coefficients of SMEFT operators involving only the Higgs field, to identify parameter regions that exhibit these first-order phase transitions and are consistent with experimental and theoretical constraints. We comment on the possibilities for electroweak baryogenesis within the SMEFT, and roughly estimate if the gravitational wave spectra generated by the phase transitions are detectable.

    hep-phastro-ph.COJHEP(2025)·28 citations
  14. 14*

    Right-handed interactions in puzzling -decays

    Damir Bečirević🇫🇷 · Svjetlana Fajfer🇸🇮 · Nejc Košnik🇸🇮 · Lovre Pavičić🇸🇮

    We explain the difference between the measured decay widths of processes and of and their values predicted in the Standard Model by introducing the right-handed interactions both to quarks and to leptons. At low energy scales, in addition to the Standard Model particles, we assume the presence of an additional neutral lepton (right-handed neutrino). We then show a specific realization of such a scenario in a model with a single scalar leptoquark (), and discuss the corresponding phenomenology.

    hep-phPLB(2025)·19 citations
  15. 15*

    Flavor Patterns of Fundamental Particles from Quantum Entanglement?

    Jesse Thaler🇺🇸 · Sokratis Trifinopoulos🇺🇸

    The Cabibbo-Kobayashi-Maskawa (CKM) matrix, which controls flavor mixing between the three generations of quark fermions, is a key input to the Standard Model of particle physics. In this paper, we identify a surprising connection between quantum entanglement and the degree of quark mixing. Focusing on a specific limit of quark scattering mediated by electroweak bosons, we find that the quantum entanglement generated by scattering is minimized when the CKM matrix is almost (but not exactly) diagonal, in qualitative agreement with observation. With the discovery of neutrino masses and mixings, additional angles are needed to parametrize the Pontecorvo-Maki-Nakagawa-Sakata (PMNS) matrix in the lepton sector. Applying the same logic, we find that quantum entanglement is minimized when the PMNS matrix features two large angles and a smaller one, again in qualitative agreement with observation, plus a hint for suppressed CP violation. We speculate on the (unlikely but tantalizing) possibility that minimization of quantum entanglement might be a fundamental principle that determines particle physics input parameters.

    hep-phhep-thquant-phPRD(2025)·44 citations
  16. 16*

    On the time-dependent density of quadratically coupled dark matter around ordinary matter objects

    Clare Burrage🇬🇧 · Benjamin Elder🇬🇧 · Yeray Garcia del Castillo🇦🇺 · Joerg Jaeckel🇩🇪

    Wave-like dark matter may feature quadratic couplings to ordinary matter. This carries profound consequences for the phenomenologies of such models. It changes the dark matter density around dense objects made from ordinary matter such as planets and stars, thereby changing the sensitivity of direct detection experiments on Earth as well as implying forces on other ordinary matter objects in the vicinity. In this note we study the time dependence of the dark matter field around spherical objects of ordinary matter. This work indicates the time-scale on which accelerating objects settle into a stationary state and delineates the applicability of stationary solutions for experimental dark matter tests. We also use this to understand (and effectively eliminate) the infinities in energies, forces, and pressures that appear when naively comparing the total energy around objects with different size but the same total number of ordinary matter particles.

    hep-phastro-ph.COgr-qcPRD(2025)·9 citations
  17. 17*

    Early Dark Energy Effects on the 21cm Signal

    Tal Adi🇮🇱 · Jordan Flitter🇮🇱 · Ely D. Kovetz🇮🇱

    Early dark energy (EDE) is one of the leading models proposed to resolve the perplexing Hubble tension. Despite extensive scrutiny and testing against various observables, conclusive constraints remain elusive as we await new data. In this paper, we study the impact of EDE on the 21cm signal, a powerful probe of cosmic dawn, and the epoch of reionization. First, we examine the signatures of the shift in cosmological parameters and the new EDE parameters on the evolution of the 21cm signal compared to CDM. We then focus on the implications of these signatures for upcoming radio interferometer telescopes, such as the Hydrogen Epoch of Reionization Array (HERA), and their ability to differentiate between EDE and CDM. Finally, we forecast HERA's sensitivity to the fractional energy density of EDE, , assuming a fiducial EDE model. We find significant modifications to the 21cm signal due to the presence of EDE. Furthermore, our analysis suggests that HERA, operating in its designed configuration, is poised to differentiate between the models and be sensitive to within after days of observation and after 2 years.

    astro-ph.COhep-phPRD(2025)·10 citations
  18. 18*

    Analytic evaluation of the three-loop three-point form factor of in sYM

    Johannes M. Henn🇩🇪 · Jungwon Lim🇩🇪 · William J. Torres Bobadilla🇬🇧

    We compute analytically the three-loop correlation function of the local operator inserted into three on-shell states, in maximally supersymmetric Yang-Mills theory. The result is expressed in terms of Chen iterated integrals. We also present our result using generalised polylogarithms, and evaluate them numerically, finding agreement with a previous numerical result in the literature. We observe that the result depends on fewer kinematic singularities compared to individual Feynman integrals. Furthermore, upon choosing a suitable definition of the finite part, we find that the latter satisfies powerful symbol adjacency relations similar to those previously observed for the case.

    hep-thhep-phJHEP(2025)·16 citations
  19. 19*

    Cosmological perturbations in a generalised axion-like dark energy model

    Carlos G. Boiza🇪🇸 · Mariam Bouhmadi-López🇪🇸

    We analyse the cosmological evolution of a generalised axion-like field that drives the late-time acceleration of the Universe. This model can exhibit tracking behaviour, which alleviates the coincidence problem. The cosmological perturbations are carried within a multi-fluid approach where the scalar field is described by a non-adiabatic fluid, i.e., one whose speed of sound in the rest frame differs from the adiabatic one. The cosmological perturbations are solved since the radiation-dominated epoch, imposing initial adiabatic conditions for matter, radiation and the dark energy component, for modes well outside the Hubble horizon in the past. We analyse the homogeneous curvature perturbation, gravitational potential and dark energy perturbations in this model, as well as the matter power spectrum and f{\sigma}8. We discuss which parameters of the model are more favoured observationally.

    astro-ph.COgr-qchep-phhep-thPhys.Dark Univ.(2025)·8 citations
  20. 20*

    Azimuthal Anisotropy Scaling Functions for Identified Particle and Anti-Particle Species across Beam Energies: Insights into Baryon Junction Effects

    Roy A. Lacey (Department of Chemistry, Stony Brook University, Stony Brook, NY)🇺🇸

    Azimuthal anisotropy scaling functions are constructed from species-resolved anisotropy measurements in Pb+Pb (=2.76, 5.02~TeV) and Au+Au (=7.7--200~GeV) collisions to probe baryon transport and medium response at finite baryon chemical potential (). Within this data-driven framework, meson and baryon anisotropies spanning the collective-flow and quenching regimes collapse onto common scaling curves, enabling quantitative separation of viscous attenuation, radial flow, and hadronic re-scattering. The attenuation scale exhibits a non-monotonic beam-energy dependence, coincident with the low-energy rise of hadronic re-scattering, consistent with a temperature-dependent specific shear viscosity featuring a near-minimum near the QCD critical region. A charge-odd baryon--antibaryon separation in the effective radial-flow response is negligible at LHC energies but grows toward lower . This species-uniform, baryon-number-scaling separation across , and disfavors a purely hadronic origin and supports junction-driven net-baryon transport at finite , enhancing the experimental visibility of critical dynamics in finite, rapidly evolving systems. Together, these results establish species-resolved scaling functions as a compact and robust tool for constraining baryon stopping, medium opacity, and QGP transport properties.

    nucl-exhep-exhep-phnucl-thPLB(2026)·3 citations
  21. 21*

    Nucleon-charmonium interactions from lattice QCD

    Yan Lyu🇯🇵 · Takumi Doi🇯🇵 · Tetsuo Hatsuda🇯🇵 · Takuya Sugiura🇯🇵

    We present a realistic lattice QCD study on low-energy - and - interactions based on (2+1) flavor configurations with nearly physical pion mass MeV. The interactions, extracted from the spacetime correlations of nucleon and charmonium system by using the HAL QCD method, are found to be attractive in all distances and possess a characteristic long-range tail consistent with the two-pion exchange potential. The resulting -wave scattering lengths are fm, fm, and fm for spin- -, spin- -, and spin- -, respectively. Our results are orders of magnitude larger than those from the photoproduction experiments assuming the vector meson dominance. Our findings may provide deeper understanding of the nonperturbative QCD phenomena ranging from the origin of nucleon mass to the in-medium mass modification as well as the properties of hidden-charm pentaquark states.

    hep-lathep-phnucl-thPLB(2025)·38 citations
  22. 22*

    Exploring the interaction via femtoscopic study

    Faisal Etminan🇮🇷

    Very recently the Wood-Saxon (WS) type interaction in the single-folding potential approach are constructed to simulate the potentials. One set of the potentials are based on the first principle HAL QCD interactions in channel, and in another set, the -meson-nucleus potentials were calculated by employing the quark-meson coupling (QMC) model. By utilizing these two set of potentials, the two-particle momentum correlation of in high-energy heavy ion collisions is explored. The numerical results show that the correlation functions at small source size (high density nuclear medium) depends on the employed potential model. Also, the correlation functions are obtained within the Lednicky-Lyuboshits (LL) formalism. For small source size, it is found that, the LL formula returns significantly different values due to the large interaction range of the potential.

    nucl-thhep-phPLB(2025)·11 citations
  23. 23*

    Evolution of strangeness and hyperons in quarkyonic matter

    Yuki Fujimoto🇺🇸 · Toru Kojo🇯🇵 · Larry McLerran🇺🇸

    We study the evolution of matter composition from nuclear to quark densities in the confining regime, by extending an ideal model of Quarkyonic matter, IdylliQ model, to multi-flavor systems including strangeness. The model provides a dual description of quark and baryon occupation probabilities which are determined by minimizing the energy of the system. Saturation of low-momentum quark states drives the formation of quark matter and constrains baryon distributions, inducing statistical repulsion among baryon species. Applying the model to charge-neutral matter composed of neutrons, , and hyperons, we find that, for typical size of baryons, -quark saturation occurs before hyperons appear, delaying their onset and shifting the threshold density from -- to -- (: nuclear saturation density). After hyperons emerge, low-momentum hyperon states remain only sparsely occupied due to the quark saturation. These features mitigate the hyperon puzzle, in which the appearance of hyperons softens neutron star equations of state significantly by increasing energy density with little pressure increase. Our results highlight the key role of quark saturation in dense baryonic matter and provide new insights into the interplay between quark dynamics and hyperon physics in neutron stars.

    nucl-thastro-ph.HEhep-phPRC(2026)·30 citations
  24. 24*

    Conditioned quantum-assisted deep generative surrogate for particle-calorimeter interactions

    J. Quetzalcoatl Toledo-Marin🇨🇦 · Sebastian Gonzalez🇨🇦 · Hao Jia🇨🇳 · Ian Lu🇨🇦 · Deniz Sogutlu🇨🇦 · Abhishek Abhishek🇨🇦 · Colin Gay🇨🇦 · Eric Paquet🇨🇦 · Roger Melko🇨🇦 · Geoffrey C. Fox🇺🇸 · Maximilian Swiatlowski🇨🇦 · Wojciech Fedorko🇨🇦

    Particle collisions at accelerators such as the Large Hadron Collider, recorded and analyzed by experiments such as ATLAS and CMS, enable exquisite measurements of the Standard Model and searches for new phenomena. Simulations of collision events at these detectors have played a pivotal role in shaping the design of future experiments and analyzing ongoing ones. However, the quest for accuracy in Large Hadron Collider (LHC) collisions comes at an imposing computational cost, with projections estimating the need for millions of CPU-years annually during the High Luminosity LHC (HL-LHC) run \cite{collaboration2022atlas}. Simulating a single LHC event with \textsc{Geant4} currently devours around 1000 CPU seconds, with simulations of the calorimeter subdetectors in particular imposing substantial computational demands \cite{rousseau2023experimental}. To address this challenge, we propose a conditioned quantum-assisted deep generative model. Our model integrates a conditioned variational autoencoder (VAE) on the exterior with a conditioned Restricted Boltzmann Machine (RBM) in the latent space, providing enhanced expressiveness compared to conventional VAEs. The RBM nodes and connections are meticulously engineered to enable the use of qubits and couplers on D-Wave's Pegasus-structured \textit{Advantage} quantum annealer (QA) for sampling. We introduce a novel method for conditioning the quantum-assisted RBM using \textit{flux biases}. We further propose a novel adaptive mapping to estimate the effective inverse temperature in quantum annealers. The effectiveness of our framework is illustrated using Dataset 2 of the CaloChallenge \cite{calochallenge}.

    cs.LGcs.AIhep-phphysics.comp-ph+1npj Quantum Inf.(2025)·11 citations
  25. 25*

    Possibility of quantum Hall effect in dense quark matter environments: A chiral model approach

    Dani Rose J Marattukalam🇮🇳 · Ashutosh Dwibedi🇮🇳 · Sourodeep De🇮🇳 · Sabyasachi Ghosh🇮🇳

    A high baryon density and strong magnetic fields are expected in peripheral collisions in heavy ion collision experiments, such as the upcoming CBM experiment at FAIR in Germany and NICA in Russia. Such densities are also likely in the core of massive neutron stars, possibly with mixed quark-hadron phases. We employed the chiral effective model to obtain the constituent quark mass in this non-perturbative QCD regime. A quantized version of conductivity and resistivity is found reliable in the quantum domain of low density and high magnetic fields. Landau quantization gives rise to phenomena similar to SdH oscillations and quantum Hall effect in this regime. We have used a density-dependent magnetic field to observe SdH-type oscillations and the possibility of the quantum Hall effect in the interior of neutron stars where the magnetic field varies as a function of the baryon density. Our results indicate the possibility of observing the quantum Hall effect in a neutron star environment.

    nucl-thastro-ph.HEhep-phhep-thPRD(2025)·3 citations
  26. 26*

    The Excess of JWST Bright Galaxies: a Possible Origin in the Ground State of Dynamical Dark Energy in the light of DESI 2024 Data

    Nicola Menci🇮🇹 · Anjan Ananda Sen🇮🇳 · Marco Castellano

    Recent observations by JWST yield a large abundance of luminous galaxies at compared to that expected in the CDM scenario based on extrapolations of the star formation efficiency measured at lower redshifts. While several astrophysical processes can be responsible for such observations, here we explore to what extent such an effect can be rooted in the assumed Dark Energy (DE) sector of the current cosmological model. This is motivated by recent results from different cosmological probes combined with the last data release of the Dark Energy Spectroscopic Instrument (DESI), which indicate a tension in the DE sector of the concordance CDM model. We have considered the effect of assuming a DE characterized by a negative {\Lambda} as the ground state of a quintessence field on the galaxy luminosity function (LF) at high redshifts. We find that such models naturally affect the galaxy UV luminosities in the redshift range needed to match the JWST observations, and with the value of =[-0.6,-0.3] remarkably consistent with that required by independent cosmological probes. A sharp prediction of such models is the steep decline of the abundance of bright galaxies in the redshift range .

    astro-ph.COastro-ph.GAgr-qchep-ph+1ApJ(2024)·39 citations
  27. 27*

    Description of electromagnetic fields in inhomogeneous accelerating sections. II Fields in the regular part

    M. I. Ayzatsky🇺🇦

    In this work we present the results of calculation of the electric field distribution in the inhomogeneous accelerating section on the base of generalized coupled modes theory. It was shown that the proposed coupled differential equations correctly describe electromagnetic field distribution in the regular part of the section under consideration, which is an analogue of the one being developed at CERN.

    physics.acc-phhep-phphysics.class-phphysics.comp-ph5 citations
  28. 28*

    Further support for increasing with effective redshift

    Özgür Akarsu🇹🇷 · Eoin Ó Colgáin🇮🇪 · Anjan A. Sen🇮🇳 · M. M. Sheikh-Jabbari🇮🇷

    In Adil et al. 2023, we reported an increasing trend in with effective redshift based on constraints over the redshift range , and predicted that this trend would be observable in independent datasets. Recently, the studies by Artis et al. and the ACT+DESI collaboration appeared, presenting data that aligns with the expected trends. In this letter, we quantify the statistical significance of the increasing trends in recent studies by fitting a linear model to estimate the slope , and comparing the results to mock simulations. We find probabilities of and , corresponding to approximately for each dataset. Using Fisher's method to combine the independent probabilities, we obtained (). When we incorporate our earlier findings, the combined statistical significance reaches between and . Finally, we discuss how ``scatter" in / constraints from recent DESI full-shape galaxy clustering fits this picture at low statistical significance. This letter continues a series of studies initiated in 2020 that explore redshift-dependent CDM parameters as an indication of a breakdown in the standard cosmological model.

    astro-ph.COhep-phhep-thMNRAS(2025)·23 citations
  29. 29*

    Interferometric Differential High-Frequency Lock-In Probe for Laser-Induced Vacuum Birefringence

    R. G. Bullis · U. D. Jentschura🇺🇸 · D. C. Yost

    We propose a measurement of laser-induced vacuum birefringence through the use of pulsed lasers coupled to femtosecond optical enhancement cavities. This measurement technique features cavity-enhanced pump and probe pulses, as well as an independent control pulse. The control pulse allows for a differential measurement where the final signal is obtained using high-frequency lock-in detection, greatly mitigating time-dependent cavity birefringence as an important and possibly prohibitive systematic effect. In addition, the method features the economical use of laser power, and results in a relatively simple experimental setup.

    physics.opticshep-phquant-phPRResearch(2025)·0 citations
  30. 30*

    From data to the analytic S-matrix: A Bootstrap fit of the pion scattering amplitude

    Andrea Guerrieri🇨🇭 · Kelian Häring🇨🇭 · Ning Su🇺🇸

    We propose a novel strategy to fit experimental data using a UV complete amplitude ansatz satisfying the constraints of Analyticity, Crossing, and Unitarity. We focus on scattering combining both experimental and lattice data. The fit strategy requires using S-matrix Bootstrap methods and non-convex Particle Swarm Optimization techniques. Using this procedure, we numerically construct a full-fledged scattering amplitude that fits the data and contains the known QCD spectrum that couples to states below GeV. The amplitude constructed agrees below the two-particle threshold with the two-loop PT prediction. Moreover, we correctly predict the phase shift, the appearance of a spin three state, and the behavior of the high-energy total cross-section. Finally, we find a genuine tetraquark resonance around 2 GeV, which we argue might be detected by looking into the decays of B mesons.

    hep-thhep-lathep-phSciPost Phys.(2026)·33 citations
  31. 31*

    Can black holes be formed by focussing radiation?

    Diego Blas🇪🇸 · Vitor Cardoso🇩🇰 · Jose María Ezquiaga🇩🇰

    Black holes are extreme outcomes of General Relativity, and can form through a variety of ways, including gravitational collapse of massive stars, or quantum fluctuations in the early universe. Here, we ask the question of whether they can form via focusing of radiation by compact binaries or intense lasers, or via trapping at the light ring of black holes. We provide evidence that gravitational lensing of radiation from a small, finite number of sources is not a viable mechanism to form black holes.

    gr-qchep-phphysics.pop-phPRD(2025)·3 citations
  32. 32*

    Observable CMB B-modes from Cosmological Phase Transitions

    Kylar Greene🇺🇸 · Aurora Ireland🇺🇸 · Gordan Krnjaic🇺🇸 · Yuhsin Tsai🇺🇸

    A B-mode polarization signal in the cosmic microwave background (CMB) is widely regarded as smoking gun evidence for gravitational waves produced during inflation. Here, we demonstrate that tensor perturbations sourced during non-inflationary epochs can yield non-negligible B-mode signals, which can in principle complicate the interpretation of future observational data. As a case study, we consider tensor perturbations sourced in the bubble collision stage of a first-order cosmological phase transition occurring in a secluded dark sector. Although phase transitions arise from causal sub-horizon physics, they nevertheless exhibit a white noise power spectrum on super-horizon scales. Power is suppressed on the large scales relevant for CMB B-mode polarization, but it is not necessarily negligible. We show that for appropriately chosen phase transition parameters, the maximal B-mode amplitude can compete with inflationary predictions that can be tested with current and future experiments. These scenarios can be differentiated by performing measurements on multiple angular scales, since the phase transition signal predicts peak power on smaller scales.

    astro-ph.COgr-qchep-exhep-ph+1PRD(2026)·12 citations

* Reconstructed cohort: no mailing for this day survives in the archive. Papers are grouped by their submission times and arXiv's announcement cut-off, assuming announcement without delay; positions follow identifier order. Validated at ~91% exact-day agreement against the archived era.