PaperPanorama

HEP Phenomenology·hep-ph

Wed·May 27, 2026

28 papers18 primary·10 cross-listed·reconstructed*

  1. 01*

    Muon-Catalyzed Nuclear Fusion: Physical Mechanism, Bottleneck Breakthroughs, and an Engineering Pathway

    Xiong Yin🇨🇳 · Wei Kou🇨🇳 · Xurong Chen🇨🇳

    Muon-catalyzed nuclear fusion (\mucf) replaces atomic electrons with negative muons, compressing atomic orbitals by about two orders of magnitude and enabling deuterium--tritium (D--T) fusion under near-room-temperature conditions. This paper reviews the physical principles of \mucf{} and formulates its essential dynamics as a four-step cycle: muonic-atom formation, muon transfer, resonant \dtmu{} molecular formation, and D--T fusion with muon release and recycling. A kinetic model is used to quantify the number of catalysis cycles per muon and the corresponding energy gain. We focus on the central limitation of catalytic efficiency, namely the alpha-sticking effect, and discuss possible breakthrough routes including nuclear-spin and muon dual polarization, in-flight muon-catalyzed fusion, and heavy-ion-driven magneto-inertial fusion. Within the idealized assumptions of the present model, a four-dimensional synergistic scheme combining dual polarization, high-density confinement, electric-field-assisted muon recovery, and resonant enhancement may increase the number of catalysis cycles per muon from the present experimental record of about 150 to more than 500, potentially enabling an energy gain \(Q>2\). On this basis, we propose a conceptual fusion--fission fuel-breeding hybrid reactor, denoted as \mucf-FBR, which exploits the 14.1-MeV neutron yield of \mucf{} to breed \({}^{239}\mathrm{Pu}\) from a \({}^{238}\mathrm{U}\) blanket in a decoupled fusion--fission operating mode. This concept may offer advantages in engineering robustness, radiation-damage tolerance, and natural-uranium utilization.

    hep-phnucl-exnucl-thphysics.acc-ph0 citations
  2. 02*

    Contributions of interference and non-interference components to CP asymmetries in heavy meson decays

    Jing-Juan Qi🇨🇳 · Yi-Fan Zhao🇨🇳 · Jin-Xia Liu🇨🇳 · Zhen-Hua Zhang🇨🇳 · Xin-Heng Guo🇨🇳 · Zhen-Yang Wang🇨🇳

    In multi-body decays of heavy mesons, conventional CP asymmetry observables obtained by integrating over the full phase space are insensitive to the higher-order wave expansion contributions in the decay amplitude squared, and consequently fail to retain information on interference effects among different resonances. To overcome this limitation, one can introduce a phase-space partitioning scheme based on the zeros of Legendre polynomials, supplemented by a sign-function weighting procedure. On such a basis, two observables are defined, namely an asymmetry observable , and the corresponding CP asymmetry . We further separate the observables into interference and non-interference parts and analyze their respective roles. As an application, the decay channel are analyzed in the region near the resonance. Using the LHCb data, the results show that odd- schemes are particularly effective in isolating interference contributions, while even- schemes are more sensitive to non-interference terms. This new assignment scheme has the potential to be extended to other decay processes, thus enriching the available physical observables.

    hep-phPRD(2026)·0 citations
  3. 03*

    Testing lepton-flavor-violating decay of doubly charged Higgs bosons in type-II seesaw via photon fusion at the high-energy LHC

    Hang Zhou🇨🇳 · Ning Liu🇨🇳

    Tiny neutrino masses can be explained by the type-II seesaw mechanism, where a triplet scalar under is predicted. Collider searches for this exotic scalar have been extensively conducted, especially for its doubly charged component . Utilizing the forward detectors at the Large Hadron Collider (LHC), we study the probing sensitivity for the elastic photon fusion production of the scalars followed by the lepton-flavor-violating (LFV) decay channels . With a high center-of-mass energy of 100 TeV and several luminosity scenarios, we can extensively broaden the exclusion bounds in the parametric space of Br versus the triplet scalar mass . Specifically, at the 100 TeV LHC with an integrated luminosity of 3 ab, the mass exclusion limit at 95\% C.L. can reach around 1150 GeV with the assumption of inverted neutrino mass hierarchy.

    hep-phNPB(2026)·2 citations
  4. 04*

    Isospin-breaking effects on the threshold cusp structures in - scattering

    Katsuyoshi Sone🇯🇵 · Tetsuo Hyodo🇯🇵

    We discuss the isospin-breaking effects on threshold cusp structures in multichannel scattering near two-body thresholds. In hadronic systems with isospin symmetry, two or more nearly degenerate thresholds can appear, and their small splitting due to isospin breaking can generate multiple cusp structures in a narrow energy region. In this paper, using the -matrix representation, we derive a general expression for the scattering amplitude near the thresholds and show that the cusp structures can be classified by the signs of the slopes of the cross section above and below threshold. We also show that additional restrictions appear in two- or three-channel systems and in the Flatté amplitude. For three-channel scattering with two nearby thresholds, we clarify how the two cusp structures are related when the threshold splitting is small and how they merge into a single cusp in the degenerate limit. Finally, we discuss the cusp structures in the elastic cross section in the coupled - system with charge . We show that, when isospin breaking is small, the two cusp structures are constrained by isospin symmetry. We also perform quantitative calculations using both simplified examples and realistic input based on NLO chiral effective field theory, and find that isospin breaking can significantly modify the relative sharpness of the cusps and may even change the cusp type itself.

    hep-phnucl-th0 citations
  5. 05*

    Revealing the Two-Fold Ambiguity: Tau Momentum Reconstruction and Its Impact on Entanglement Observables

    Xiang Zhou🇨🇳 · Jianyong Zhang🇨🇳 · Xia Wan🇨🇳 · Youkai Wang🇨🇳 · Xiaohu Mo🇨🇳

    The neutrinos produced in decays cannot be directly detected, making the reconstruction of kinematics challenging and affecting measurements of quantum correlations such as spin entanglement. For the process , the kinematic constraints allow the momenta to be reconstructed up to a well-known two-fold ambiguity, regardless of the presence of an intermediate resonance state. In this paper, we present a geometric interpretation of this ambiguity and propose a numerical reconstruction method based on singular value decomposition (SVD). Using only the information from visible final-state particles and decay kinematics, the method reconstructs the two possible solutions for the pair. The reconstruction performance is validated with Monte Carlo simulations in typical collider environments. We further investigate the impact of the spurious solution on spin-entanglement measurements and show that reliable entanglement signals can still be extracted even when the true and spurious solutions cannot be experimentally distinguished. This work provides a practical approach for -lepton kinematic reconstruction and spin-entanglement measurements in collider experiments.

    hep-ph3 citations
  6. 06*

    Attractors in a Generalized Relativistic Second Order Spin Hydrodynamics

    Qi Zhou🇨🇳 · Duan She🇨🇳 · Ben-Wei Zhang🇨🇳 · Enke Wang🇨🇳

    We investigate the attractor of spin density in relativistic spin hydrodynamics using Zubarev's non-equilibrium statistical operator formalism in the spin probe limit. We derive the (0+1)D Bjorken flow equations and the associated attractor equation while retaining second order gradient corrections in the relevant relaxation constitutive equations including couplings associated with nonlinear response and nonlocal memory effects. We analyze the early time fixed point structure and analytically determine the early time attractor solution, thereby clarifying branch selection and the role of different dynamical corrections. We find that source-like driving terms modify the leading correction to the attractor solution without changing the fixed point structure, whereas self feedback terms involving the rotational stress tensor modify the dominant balance and modify the early time fixed point structure. We further study the late time asymptotic behavior in the conformal limit and show that the newly added terms affect the first subleading asymptotics without changing the leading late time branches. These results provide a unified picture of early and late time attractor dynamics in the conformal limit.

    hep-ph0 citations
  7. 07*

    Particle-Lund Multimodality in Jet Taggers

    Loukas Gouskos🇺🇸 · Benedikt Maier🇬🇧

    The Lund plane offers a physics-motivated, hierarchical representation of QCD radiation within jets, while transformer-based taggers have reached state-of-the-art performance by learning directly from raw particle constituents and their pairwise relations. We investigate whether transformers implicitly capture hierarchical QCD structure from constituent-level inputs, or whether explicit physics representations remain complementary. To test this, we introduce PLuM, a multimodal architecture that projects particle constituents and Lund plane splittings into a shared latent space, processing both jointly with a unified transformer. Cross-attention allows the model to probe whether structured QCD information provides discriminating power beyond what particles alone encode. We observe systematic gains for top-quark and tagging, while finding no comparable improvement for or topologies. This selective enhancement suggests that explicit hierarchical information about b-jet formation remains complementary to raw particle representations even in highly expressive architectures, while other topologies are already well-captured at constituent level. For high-impact LHC analyses such as Lorentz-boosted di-Higgs searches in the four quark final state (), the gains are substantial: at a di-Higgs efficiency working point, PLuM achieves higher background rejection than the baseline. Our results indicate that physically structured representations of QCD radiation retain discriminating value in the transformer era, motivating further study into how different aspects of jet dynamics are encoded by deep learning algorithms.

    hep-phcs.LGhep-ex0 citations
  8. 08*

    Improved Big Bang Nucleosynthesis constraints on decaying massive relics

    Sara Bianco🇩🇪 · Jonas Frerick🇮🇹 · Marco Hufnagel🇧🇪 · Kai Schmidt-Hoberg🇩🇪

    We present updated and improved Big Bang Nucleosynthesis (BBN) constraints on heavy, long-lived beyond the Standard Model (BSM) relics decaying into pairs of Standard Model particles, covering a comprehensive set of two-body decay channels. We treat the leading effects of these injections in detail, discussing the modification of the neutron-to-proton ratio from hadronic interconversions, as well as hadro- and photodisintegration of the light elements. Our analysis incorporates several important refinements with respect to earlier work. We adopt up-to-date primordial abundance measurements, including the new He determination and the latest nuclear reaction rates. The hadronic and electromagnetic injection spectra are computed using PYTHIA 8, providing a proper treatment of final-state radiation and hadronisation. We further implement an improved treatment of interconversions, accounting for dynamical equilibrium, kaon-induced processes, and updated rates. Additionally, we make use of a refined hadrodisintegration formalism which allows us to also consider disintegration processes while BBN is still active. Together, these improvements yield updated exclusion contours on lifetime, mass, and abundance of the relic for each decay channel considered. Furthermore, we discuss the irreducible freeze-in contribution from inverse decays.

    hep-phastro-ph.CO2 citations
  9. 09*

    Exotic Hadron Spectroscopy in Heavy-Flavor Systems

    Mikhail Mikhasenko🇩🇪

    Recent years have brought a dense sequence of experimental discoveries in heavy-flavor hadron spectroscopy. Heavy-flavor spectroscopy has entered a period in which new hadronic structures are no longer isolated surprises but recurring features across several flavor sectors, seen by multiple experiments in several decay environments. For systems with charm and bottom quarks, smaller widths and cleaner signatures expose regularities that would be harder to isolate in the light-quark sector. This contribution focuses on the classes of states that now define the modern ``exotic'' landscape: hidden-charm pentaquarks, charged charmonium-like structures, resonances in onia-onia systems, doubly-heavy tetraquarks, and open-flavor tetraquarks.

    hep-phPoS(2026)·0 citations
  10. 10*

    Looking for Condensed Gluons: A Cross-Scale Journey from the Deep Structure of Protons to High-Energy Cosmic Rays -- A Mini-Review

    Wei Zhu🇨🇳 · Yu-Chen Tang🇨🇳 · Ye-Yin Zhao🇨🇳 · Bo Yang🇨🇳 · Yu-Chen Xiong🇨🇳

    Quark-gluon dynamics within protons and high-energy radiation phenomena in the universe are typically regarded as two entirely distinct fields. This paper aims to demonstrate that gluon condensation (GC) may serve as a direct bridge between these two fields. We review three key aspects of GC research: first, the Zhu-Shen-Ruan (ZSR) equation, as a nonlinear evolution equation based on structural symmetry, exhibits self-consistent connections with the DGLAP, BFKL and GLR-MQ-ZRS equations, providing a theoretical foundation for the generation of GC; second, the chaotic solutions and the shadowing-antishadowing synergy inherent in this equation can drive gluons to aggregate near the critical momentum, thereby forming a novel type of high-density, strongly interacting matter; third, these changes in microstructure manifest themselves as a broken-power-law feature in high-energy cosmic gamma-ray spectra, thereby offering new insights into the hadronic scenarios underlying certain astrophysical sources. Consequently, GC not only concerns the novel behaviour of quantum chromodynamics under extreme conditions but may also serve as a vital window for probing the deep structure of protons using cosmic-ray signals. With the advancement of higher-precision gamma-ray observations, hadron collision experiments and related theoretical research, the physical picture of GC and its observational criteria are expected to undergo more rigorous testing. Should this picture be confirmed, certain features in the high-energy gamma-ray spectrum will need to be re-examined within the deeper context of hadronic dynamics; simultaneously, GC may also provide a new entry point for research into pion condensation in nuclear physics and even condensed matter physics. Consequently, the significance of the search for GC extends beyond the model itself, reaching into multiple fields of natural science.

    hep-phastro-ph.HEcond-mat.otherhep-thSymmetry(2026)·0 citations
  11. 11*

    Family-separated seesaw relations of Majorana neutrinos

    Zhi-zhong Xing🇨🇳

    Given the canonical seesaw mechanism as a most natural extension of the standard model in its neutrino sector, we find out a special but brand new solution to the exact seesaw equation: for the masses and flavor mixing matrix elements of light and heavy Majorana neutrinos of the -th family (for and ). This family-separated seesaw scenario allows us to establish simple relations between the original seesaw parameters and the active degrees of freedom, and thus offers a number of testable predictions in neutrino phenomenology.

    hep-phhep-exhep-th1 citation
  12. 12*

    Refined extraction of electroweak and nuclear parameters from germanium CENS data

    Valentina De Romeri🇪🇸 · Laura Duque🇲🇽 · Dimitrios K. Papoulias🇩🇪 · G. Sanchez Garcia🇲🇽 · Christoph A. Ternes🇮🇹

    We present a combined analysis of recent CENS data on germanium from two complementary experiments: COHERENT, which uses neutrinos from pion decay at rest, and CONUS+, which detects reactor antineutrinos. Exploiting the complementarity of these two datasets in a joint statistical analysis, we extract the germanium root-mean-square neutron radius and neutron skin with improved precision, disentangling spectral shape distortions from overall normalizations and reducing systematic uncertainties. We also determine the weak mixing angle at low momentum transfer, providing a test of the Standard Model in a less-explored kinematic regime. A key systematic uncertainty in CENS ionization measurements is the nuclear quenching factor; we therefore present our results as a function of variations of the Lindhard model. For the nuclear form factor, we adopt the analytical Klein-Nystrand parametrization and benchmark it against predictions from the large-scale nuclear Shell Model, assessing the impact of nuclear structure uncertainties on our results. Our analysis demonstrates the power of combining datasets across different neutrino sources to maximize sensitivity to both nuclear and electroweak physics.

    hep-phJHEP(2026)·2 citations
  13. 13*

    Polarization dependence of the meson from finite-temperature QCD sum rules

    Hidefumi Matsuda🇨🇳 · Philipp Gubler🇯🇵 · Koichi Hattori🇨🇳

    We study the meson at finite temperature and finite momentum using QCD sum rules. The presence of medium breaks the Lorentz invariance, and induces distinct in-medium modifications of the transverse and longitudinal modes at finite momentum. We find that, with increasing momentum, the masses of both modes increase and a clear transverse--longitudinal splitting develops. The splitting is found to grow with temperature and to be mainly generated by the dimension-four spin-dependent thermal condensates.

    hep-phhep-ex1 citation
  14. 14*

    Influence of the QCD Analogue of the Inverse Compton Effect on the Transverse Momentum and Pseudorapidity Distributions of Secondary Particles in pp Collisions at sqrt (s)= 30 GeV, 510 GeV, and 14 TeV

    M. Alizada🇦🇿 · M. Suleymanov🇦🇿

    Within the framework of numerical simulations, this work investigates the influence of the QCD analogue of the inverse Compton effect (ICE) in the quark--gluon scattering process qg \rightarrow qg on the transverse momentum p_T and pseudorapidity eta distributions of secondary particles produced in proton--proton collisions at energies sqrt{s}=30 GeV, 510 GeV, 14 TeV. In the present context, ICE refers to a class of parton-level kinematic configurations in which the incoming quark carries a larger fraction of energy than the gluon, in contrast to the complementary DCE regime. The simulations were performed using the PYTHIA~8.316 event generator. It is shown that the relative contributions of ICE and DCE strongly depend on the collision energy. As the energy increases from sqrt{s}=30 GeV to sqrt{s}=14 TeV, the ICE contribution becomes comparable to or exceeds the DCE contribution over a broad p_T range. The analysis of pseudorapidity distributions demonstrates that deviations of the ICE/DCE ratio from unity appear predominantly in the central region |eta| simeq 0, corresponding to symmetric partonic configurations x_1 sim x_2, whereas in peripheral regions the ratio approaches unity. The obtained results indicate that, with increasing collision energy, the contribution of ICE-like processes grows due to the enhanced role of gluon collisions in the small-x region.

    hep-phhep-ex0 citations
  15. 15*

    Neutrino-antineutrino superfluidity

    Damiano F. G. Fiorillo🇮🇹 · Georg G. Raffelt🇩🇪 · Günter Sigl🇩🇪

    Despite their feeble interactions, dense astrophysical neutrinos can behave collectively, exchanging flavor through waves of the neutrino plasma. Can collective interactions also induce pairing instabilities and reorganize the neutrino momentum distribution, in analogy to the superfluid instability of fermions? We show that, for standard weak interactions, pairing instabilities can arise only in the presence of discontinuities in the occupation number, such as the sharp Fermi surface responsible for superconductivity in metals. However, discretized energy spectra can mimic such discontinuities and artificially generate superfluid instabilities. These spurious instabilities disappear in the continuum limit.

    hep-phastro-ph.COastro-ph.HE1 citation
  16. 16*

    Constraints on a Light Leptophilic Scalar from Dark-Sector Couplings

    Marco Graziani🇮🇹 · Giacomo Landini🇮🇹 · Federico Mescia🇮🇹 · Claudio Toni🇫🇷 · Ludovico Vittorio🇮🇹

    We study a minimal framework where a Majorana fermion dark matter particle interacts with a light scalar mediator coupled mainly to electrons. We examine both freeze-out and freeze-in production to determine the regions of parameter space that yield the correct relic abundance with particular emphasis on a detailed comparison with results in the recent literature. The analysis includes cosmological and astrophysical constraints as well as laboratory bounds from electron-recoil experiments, fixed target searches, and precision measurements. The combined results identify a narrow but viable parameter region, favoring sub-GeV dark matter, and define clear targets for future experimental tests. This highlights the strong complementarity between direct-detection experiments and collider searches. We additionally investigate the mediator-mass region around 17 MeV, motivated by the hints reported by the ATOMKI experiment and the PADME collaboration, including couplings between the mediator and light quarks. Direct searches already constrain a large region of the parameter space, even when dark matter is produced via freeze-in, pointing again to sub-GeV dark matter.

    hep-ph1 citation
  17. 17*

    Probing Dynamical Inverse Seesaw with Low-frequency Gravitational Waves

    Debasish Borah🇮🇳 · Sounak Dutta🇮🇳 · Partha Kumar Paul🇮🇳 · Indrajit Saha🇮🇳 · Narendra Sahu🇮🇳

    We study the possibility of probing the dynamical inverse seesaw mechanism for the origin of light neutrino masses via the detection of stochastic gravitational waves (GW) in the low-frequency regime currently being probed by pulsar timing arrays. As the lepton number-violating term in inverse seesaw typically remains in the sub-MeV ballpark, its dynamical origin naturally brings the possibility of a low-scale first-order phase transition, which can be probed at low-frequency GW experiments. We also find interesting complementarity with heavy neutral lepton searches, as GW experiments remain sensitive to parameter space with small active-sterile mixing, which is out of reach for most particle physics experiments.

    hep-phastro-ph.COhep-exhep-th1 citation
  18. 18*

    From WIMP to FIMP during reheating: collider vs non-collider probes for p-wave annihilation

    Dipankar Pradhan🇮🇳 · Niloy Mondal🇮🇳 · Abhik Sarkar🇮🇳 · Anupam Ghosh🇮🇳 · Shashwat Sharma🇮🇳 · Mathew Thomas Arun🇮🇳 · Basabendu Barman🇮🇳

    By examining the transition from freeze-out to freeze-in dark matter (DM) production within the framework of perturbative reheating, where DM interacts with the visible sector through effective operators of dimension six, we have investigated how a broad range of new physics probes can reveal the nature of the pre-BBN Universe. Incorporating constraints from direct and indirect DM searches, invisible decay measurements, collider experiments, and gravitational wave observations, our analysis demonstrates that both current and forthcoming experimental sensitivities can serve as powerful tools for probing as well as constraining the post-inflationary era, together with new physics beyond the SM. Our analysis demonstrates that collider experiments at both the intensity and energy frontiers can impose strong bounds on derivative operators whose interactions are typically {\it p-wave suppressed}, and therefore only weakly constrained by astrophysical observations. In particular, these complementary searches can significantly restrict the allowed reheating temperature, DM mass and effective interaction scale required to reproduce the observed DM abundance for DM produced during the epoch of reheating.

    hep-phastro-ph.COhep-exhep-th2 citations
  19. 19*

    NuSTAR as an Axion Helioscope: probing axion-nucleon and axion-electron couplings

    Tiziano Zanzarella🇮🇹 · Francisco R. Candón🇩🇪 · Maurizio Giannotti🇪🇸 · Marco Regis🇮🇹 · Jaime Ruz🇩🇪 · Marco Taoso🇮🇹 · Elisa Todarello🇮🇹 · Julia K. Vogel🇩🇪

    We investigate solar X-ray observations as a probe of axions and axion-like particles. These particles can be produced in the interior of the Sun via the conversion of thermal photons, as well as through processes involving axion-electron and axion-nucleon interactions. The resulting axions can then reconvert into photons in the Sun's atmospheric magnetic field, generating a signal in the X-ray energy range. In this work, we derive new limits on axions using X-ray observations with the Nuclear Spectroscopic Telescope Array (NuSTAR) during the 2020 solar minimum. In the regime where ALP production is dominated by couplings to electrons or nucleons, we obtain bounds on the product of couplings and at 95% CL, for axion masses . These constraints strongly improve current ground-based experimental limits, establishing solar X-ray observations as a powerful and robust method for axion searches.

    astro-ph.COastro-ph.HEhep-ph0 citations
  20. 20*

    Experiments in Agentic AI for Science

    Judy Fox🇺🇸 · Geoffrey Fox🇺🇸

    This paper details two novel frameworks for developing autonomous, agentic AI in scientific workflows. Both systems leverage a hybrid Local Body, Remote Brain architecture via Google Colab, utilizing Python-based local orchestrators to invoke large language model (LLM) cloud backends. The first agent, DeepTS/DeepCollector, automates the large-scale curation, extraction, and deduplication of time-series datasets. The second, DeepScribe, is an autonomous presentation analyzer that converts visually dense, mathematically complex physics lectures into structured scientific reports. Through practical systems engineering-such as granular attribute extraction (Cellular RAG), remote data inspection, and distributed concurrency controls-we demonstrate how agentic AI can overcome the context and reasoning limitations of current state-of-the-art systems to rigorously support scientific workflows. Finally, we outline a generalization of DeepTS to support deep knowledge graphs and discuss the application of this conceptual approach to high-energy physics (DeepQCD).

    cs.AIcs.SYeess.SYhep-ph0 citations
  21. 21*

    Cumulants of mean transverse momentum and elliptic flow in the hydrodynamic model of heavy-ion collisions

    Tribhuban Parida🇵🇱 · Piotr Bożek🇵🇱

    Higher order cumulants between the mean transverse momentum and elliptic flow are calculated in a relativistic viscous hydrodynamic model of relativistic heavy-ion collisions. The results of the hydrodynamic simulations are compared with calculations using event-by-event predictors of the final collective observables constructed from the initial state entropy distribution. The predictors describes quantitatively centrality dependence of the higher cumulants considered in the paper. We derive a quantitative relations between the cumulants of the mean transverse momentum and different moments of the harmonic flow. The hydrodynamic simulations satisfy those relation very well. Those relations could be used to test experimentally the collective origin of the observed correlations between the mean transverse momentum and harmonic flow.

    nucl-thhep-exhep-phnucl-ex2 citations
  22. 22*

    Sensitivity of Heavy-Quark Dipolar Flow to its Initial Spatial Distributions in Cu+Au Collisions

    Ankit Kumar Panda🇨🇳 · Tribhuban Parida🇮🇳

    We investigate charm-quark dynamics in asymmetric Cu+Au collisions at top RHIC energy using a Langevin approach embedded in a realistic hydrodynamic background. The intrinsic asymmetry of the colliding nuclei leads to a spatially lopsided initial energy-density profile, which generates a dipolar flow structure in the transverse plane even at midrapidity. As charm quarks propagate through this medium, they acquire a finite directed flow, . We find that the -integrated heavy-quark is approximately an order of magnitude larger than that of charged hadrons. In addition, the -differential exhibits strong sensitivity to the initial spatial distribution of heavy quarks, emphasizing the importance of pre-equilibrium dynamics in determining final-state anisotropies. Beyond geometric effects, also provides direct sensitivity to medium interactions through the temperature-dependent drag coefficient. Its pronounced dependence on this transport input indicates that precision measurements of heavy-flavor directed flow could place meaningful constraints on heavy-quark transport coefficients, thereby improving Langevin-based descriptions and predictive power for heavy-flavor observables in heavy-ion collisions.

    nucl-thhep-exhep-phnucl-ex0 citations
  23. 23*

    Azimuthal asymmetry in exclusive quasi-elastic neutrino-nucleus interactions

    Marco Vanderpoorten🇧🇪 · Ashish Kumar Jha🇧🇪 · Mathias El Baz🇨🇭 · Kajetan Niewczas🇧🇪 · Federico Sanchez🇨🇭 · Natalie Jachowicz🇧🇪

    In neutrino oscillation experiments, exclusive measurements of neutrino-nucleus interactions play a critical role, by providing the theoretical and experimental input needed for a reliable estimation of the neutrino energy. In this paper, we derive the general form of the azimuthal angle distribution for quasi-elastic scattering, focusing on a dependency that has been routinely overlooked. We demonstrate that the outgoing nucleon exhibits a preference for emission outside the lepton scattering plane, with an asymmetric azimuthal distribution. In the context of neutrino-nucleus scattering, we argue that this asymmetry is caused by parity violation in the weak interaction. Furthermore, we show that in cross section calculations the asymmetry is sensitive to nuclear modeling choices and to the shell structure of the initial nucleus, thus providing a novel source of information for energy reconstruction in neutrino experiments. We study the experimental feasibility of observing this effect by applying a realistic momentum detection threshold and an intranuclear cascade. We estimate that the asymmetry is observable with () events at the 99% confidence level for neutrino interactions on C, suggesting that the effect is within reach of the current generation of neutrino detectors.

    nucl-thhep-ph0 citations
  24. 24*

    Flow-Based Global Proposals for Monte Carlo Sampling in SU(2) Lattice Gauge Theory

    Seung-il Nam🇰🇷

    We propose a formally valid machine-learning-assisted global proposal mechanism for Monte Carlo sampling in lattice gauge theory. The construction is based on a coupling-flow update on the SU(2) lattice-link manifold, in which active links are transformed conditionally on a frozen-link background. For fixed frozen links, the proposal is explicitly invertible and preserves the product Haar measure, so it can be embedded into a Metropolis-Hastings correction without requiring an explicit model of the full proposal density. We implement the method in two-dimensional pure SU(2) lattice gauge theory and benchmark it against a baseline local Metropolis algorithm used as a controlled reference kernel. In the present testbed, the learned proposal reproduces the target ensemble within statistical resolution across the tested configurations. In matched local-step comparisons, the learned proposal reproduces the target ensemble at a quality comparable to the baseline, but does not outperform the pure local baseline in the conservative matched-step case examined with seed-level statistics within this proof-of-principle setup. At the same time, a favorable mixed-step hybrid configuration yields a modest improvement in effective sample size per unit runtime. Because the learned transformation remains in a near-identity regime, the present results should be interpreted as a proof-of-principle demonstration of formal correctness and limited, configuration-dependent efficiency gain within a controlled comparison, rather than as evidence of superiority over optimized conventional update schemes. This work provides a concrete foundation for extending machine-learned nonlocal updates to larger lattices and non-Abelian gauge theories relevant to lattice QCD.

    hep-lathep-ph0 citations
  25. 25*

    For modified gravity, it's the LITTLE THINGS that matter

    Geoff Beck🇿🇦

    Dwarf galaxies have long been recognised as important testing grounds for models of dark matter. For instance, it is here where the cusp-core problem is most apparent. In this work we select two dwarf galaxy samples: LITTLE THINGS and dwarf galaxies in SPARC. We use these to examine whether there are preferences for MOND or dark matter halos in these objects. Notably, our analysis employs the latest developments in Hamiltonian Monte Carlo sampling methodology and robust model comparison via ELPD differences. Our findings suggest a preference for cored halo models over MOND. However, this relies on significant preferences from 7 out of 19 SPARC galaxies and 11 of 18 from LITTLE THINGS (few of which are overwhelming). It is notable that only a single galaxy prefers MOND over a cored halo. Thus, this evidence is suggestive, but does not conclusively decide against MOND. We also test for evidence of a MOND external field effect, and find weak evidence against its presence. Despite these statistical preferences, most SPARC galaxies remain compatible with a universal MOND scale. In LITTLE THINGS, a free MOND model is preferred to a universal value at , but this is of doubtful physical significance. For MOG, the story is different, here we find preferences for all halos (or MOND) against universal MOG models with significant exclusions in individual galaxies across both samples. Thus, a proposed universal rotation curve model derived from MOG is quite strongly disfavoured.

    astro-ph.GAgr-qchep-ph1 citation
  26. 26*

    Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply

    Swagat S. Mishra🇰🇷

    In observational cosmology, the dark energy density and equation of state are effective quantities reconstructed at the background level under a set of assumptions. These include the FLRW framework, the standard Friedmann equation of General Relativity, and separately conserved non-relativistic matter at late times. Recent analyses involving DESI BAO measurements combined with CMB and supernova data have shown mild preference for dynamical dark energy featuring phantom or phantom-crossing behaviour. While the statistical significance of these trends remains limited, and unresolved systematics or modelling uncertainties may still be important, the resulting discussions have highlighted the need for a clearer interpretation of effective dark energy reconstruction. In particular, effective phantom behaviour does not necessarily imply the existence of a fundamental phantom field, microscopic ghost instabilities, violation of the null energy condition by the fundamental stress tensor, or a catastrophic cosmic future. The purpose of this work is to clarify these distinctions, independently of whether the current observational preference for dynamical dark energy survives future data. We discuss the definition of effective dark energy in cosmology, the interpretation of phantom and phantom-crossing behaviour, introduce a simple kinematic criterion for identifying effective phantom evolution directly from the expansion history, and review physical mechanisms through which effective phantom behaviour may arise without fundamental pathologies. While familiar within the dark energy reconstruction community, these distinctions are often left implicit in broader discussions of dynamical dark energy. We hope that this work will remain useful beyond the present observational situation as a clarification of what observationally reconstructed dark energy does and does not imply.

    astro-ph.COgr-qchep-phhep-thPhys.Dark Univ.(2026)·7 citations
  27. 27*

    Gaussian Process Reconstruction of Cosmological Parameters with Gravitational Wave Sirens using Machine Learning

    Gourab Nandi🇮🇳 · Anish Ghoshal🇮🇹 · David F. Mota🇳🇴

    Future gravitational wave (GW) standard siren catalogues will probe the late-time expansion history of the Universe across redshift ranges largely inaccessible to traditional electromagnetic observations. To determine how effectively this background distance information can distinguish between viable cosmological models, we introduce a model-independent reconstruction framework utilizing Gaussian Process Regression (GPR). Analyzing mock LISA and Einstein Telescope (ET) catalogues across six fiducial cosmological backgrounds-CDM, CPL, CPL+, interacting dark matter, interacting dark energy and axion inspired early dark energy. We reconstruct the comoving distance and its derivatives. Crucially, we propagated the full GP covariance, including derivative cross-covariances, to robustly evaluate the Hubble parameter and other diagnostics such as , and . While our analysis demonstrates that GW bright standard sirens faithfully recover fiducial expansion histories, applying pointwise marginal Hellinger distance reveals that background measurements alone do not provide decisive statistical separation among models. Instead, derivative sensitive diagnostics pinpoint specific redshift windows (e.g., for ET and for LISA) where future catalogues will maximize their discriminatory power. As machine learning methodologies become increasingly integral to astrophysics and cosmology, this Bayesian GPR pipeline offers a principled, nonparametric approach to precisely identifying where the most valuable cosmological information lies.

    astro-ph.COgr-qchep-phhep-th0 citations
  28. 28*

    On the Validity of the Effective Theory of (Multi-)Field Inflation

    Andrea Ambrosi de Magistris🇮🇹 · Alberto Salvio🇮🇹

    Motivated by trans-Planckian issues in inflation, we determine the Hilbert space and amplitudes of quantum perturbations in the general low-energy effective theory of (multi-)field inflation without relying on the sub-horizon limit. The scalar sector is the most intricate, featuring field mixings and second-class constraints, which we handle using Dirac brackets. These results enable us to estimate the magnitude of higher-derivative corrections. In the specific case of slow-roll inflation, such estimate can be expressed in terms of the first slow-roll parameter for a given cutoff . We apply our results to several inflationary models with finite : Higgs inflation, the Starobinsky model, natural inflation and hilltop inflation.

    hep-thastro-ph.COhep-ph0 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.