PaperPanorama

HEP Phenomenology·hep-ph

Wed·Dec 31, 2025

26 papers17 primary·9 cross-listed·reconstructed*

  1. 01*

    BSFfast: Rapid computation of bound-state effects on annihilation in the early Universe

    Tobias Binder🇩🇪 · Mathias Garny🇩🇪 · Jan Heisig🇩🇪 · Stefan Lederer🇵🇱

    Bound-state formation (BSF) can have a large impact on annihilation of new physics particles with long-range interactions in the early Universe. In particular, the inclusion of excited bound states has been found to strongly reduce the dark matter abundance and qualitatively modify the associated freeze-out dynamics. While these effects can be captured by an effective annihilation cross section, its explicit computation is numerically expensive and therefore impractical for repeated use in Boltzmann solvers or parameter scans. In this work we present BSFfast, a lightweight numerical tool that provides precomputed, tabulated effective BSF cross sections for a wide class of phenomenologically relevant models, including highly excited bound states and, where applicable, the full network of radiative bound-to-bound transitions. We exploit rescaling relations of the cross section to efficiently cover models with additional free parameters and provide fast interpolation routines in Mathematica, python and C for use in Boltzmann solvers. As an illustration, we apply BSFfast to a superWIMP scenario with a colored mediator, demonstrating that the tool enables phenomenological studies that would otherwise be computationally prohibitive. The code is publicly available on GitHub.

    hep-phEPJC(2026)·5 citations
  2. 02*

    Charm Quark Kinetics in Heavy Ion Collisions

    Valeriya Mykhaylova🇵🇱 · Krzysztof Redlich🇵🇱 · Chihiro Sasaki🇵🇱

    We study the evolution of charm quarks in hot QCD matter with quark flavors by analyzing the charm production rate and the time dependence of their abundance. Microscopically, the system is described within a quasiparticle model, in which interactions among dynamical quarks and gluons are encoded in their effective masses with the running coupling constrained by lattice QCD data. We investigate -quark kinetics in a longitudinally propagating perfect fluid as well as in a viscous medium undergoing (2+1)D expansion, and find that the charm production rate decreases monotonically across all medium formulations. In the scenario, charm production is systematically suppressed due to the effective mass of heavy quasiparticles. Assuming an initial charm yield given by the Statistical Hadronization Model, we solve the rate equation and compute the total charm abundance in hot QCD medium. For all descriptions considered, the charm quark number remains approximately conserved, consistent with existing experimental evidence.

    hep-ph0 citations
  3. 03*

    Gedanken Experiments of Entanglement in Particle Physics: Interactions, Operators and Bell Inequalities in Flavor Space

    Corbin Pacheco (Wayne State University)🇺🇸 · Nausheen R. Shah (Wayne State University)🇺🇸

    In this article we explore ideas from quantum entanglement which can be meaningfully formulated and tested in the collider environment. We propose Bell-type inequalities as operator-level diagnostics of quantum incompatibility in particle-physics systems. We construct flavor operators associated with mass identification, flavor change, and charged-current weak mixing which arise from fundamental interactions in the Standard Model. We treat these interactions as alternative measurement settings in a Gendanken experiment. For entangled two-particle states, these operators generate nontrivial correlations that violate Bell-type bounds, excluding non-contextual local descriptions under the stated assumptions. These violations arise from the algebraic structure of the operators rather than from kinematic correlations or exotic dynamics. We discuss how the predicted correlation patterns may be probed with experimental data, clarifying the scope and limitations of Bell-type reasoning in particle physics.

    hep-phhep-exhep-thquant-phPRD(2026)·2 citations
  4. 04*

    Progress in Lorentz and CPT Violation

    Alan Kostelecky🇺🇸

    This talk at the CPT'25 meeting presents an overview of some recent results in Lorentz and CPT violation. Topics covered include the geometry of Finsler spaces associated with Lorentz violation, the resolution of the concordance problem in Lorentz-violating effective field theories, the relativistic evolution of a spin in background fields, and the phenomenology of searches for flavor-changing Lorentz and CPT violation in charged leptons.

    hep-ph1 citation
  5. 05*

    Origin of hadron mass from gravitational D-form factor and neutron star measurements

    Mamiya Kawaguchi🇨🇳 · Masayasu Harada🇯🇵 · Yong-Liang Ma🇨🇳

    Clarifying the origin of hadron mass is one of the fundamental problems in particle physics, relevant from hadronic scales to astrophysical observations. At low energies, this issue is reflected in the decomposition of the hadron mass into chiral-variant and -invariant components. In this letter, we propose a method to extract the chiral invariant mass from the gravitational -form factor under the assumption of the lightest-sigma meson dominance. Focusing on the nucleon, we show that a sizable chiral invariant mass is required to reproduce lattice QCD data, consistent with neutron star constraints.

    hep-phhep-latnucl-thPLB(2026)·5 citations
  6. 06*

    Inflationary QCD phase diagram

    Kohei Fujikura🇯🇵 · Toshifumi Noumi🇯🇵

    Motivated by the cosmological collider program, which aims to probe high-energy physics through inflation, we investigate the phase diagram of multi-flavor QCD in de Sitter spacetime with a flavor-universal axial chemical potential induced by a rolling inflaton coupled to fermions. We determine the first-order critical line and a critical point as functions of the Hubble parameter and the axial chemical potential, employing an effective description of chiral symmetry breaking within the framework of the Nambu--Jona-Lasinio model. We find that a first-order chiral phase transition may occur during inflation or at its end when the axial chemical potential is sufficiently large and crosses the critical line. This provides a cosmological collider analogue of the QCD phase diagram explored in heavy-ion colliders.

    hep-phastro-ph.COhep-thPRD(2026)·4 citations
  7. 07*

    Dark Matter-Driven Low-Scale Leptogenesis via Neutrino Portal

    Suresh Chand🇮🇳 · Avnish🇮🇳 · Poulose Poulose🇮🇳

    We propose a novel framework for low-scale leptogenesis within an extension of the Standard Model (SM) that includes three SU(2) singlet right-handed neutrinos, a singlet charged neutral fermion, and a real scalar field. In this setup, the CP asymmetry arises through a rich interplay of mechanisms, including two-body decays of the lightest right-handed neutrino into leptons and Higgs or into dark-sector particles, as well as multiple 2 -> 2 scattering processes involving visible and dark states. Crucially, the CP-violating phases originate not only from conventional vertex and self-energy corrections but also from novel interference effects mediated by the dark sector, which significantly enrich the sources of asymmetry. A distinctive feature of our model is the direct connection between the dark sector and leptogenesis, providing a unified explanation for both the matter-antimatter asymmetry and DM abundance. This connection leads to enhanced CP violation in neutrino interactions and predicts new dark-sector particles accessible at the LHC.

    hep-phPRD(2026)·1 citation
  8. 08*

    Landau-Zener-Stückelberg-Majorana dynamics of magnetized quarkonia

    Ahmad Jafar Arifi🇯🇵 · Kei Suzuki🇯🇵

    The mass spectrum of hadrons in magnetic fields features avoided level-crossing structures arising from the mixing of spin eigenstates. In this work, we investigate the impact of level-crossing dynamics of charmonia subjected to time-dependent magnetic fields, where we particularly focus on the occupation probabilities of two or more states as they undergo transitions at avoided crossings. Using a static spectrum of charmonia in magnetic fields, we construct a multi-channel Landau-Zener Hamiltonian. Within this framework, we analyze the time evolution under several representative magnetic-field profiles, including linear ramps and Gaussian decays corresponding to single-passage dynamics, as well as Gaussian pulses realizing double-passage dynamics, and compute the occupation probabilities over a wide range of sweep rates and initial conditions. Our results show that nonadiabatic dynamics, including Landau-Zener transitions and Stückelberg interference, strongly influences the occupation probabilities of charmonia. These findings provide new insights into the real-time dynamics of magnetized hadrons and offer useful guidance for future lattice simulation studies.

    hep-phnucl-thPRD(2026)·2 citations
  9. 09*

    Quantitative Understanding of PDF Fits and their Uncertainties

    Amedeo Chiefa🇬🇧 · Luigi Del Debbio🇬🇧 · Richard Kenway🇬🇧

    Parton Distribution Functions (PDFs) play a central role in describing experimental data at colliders and provide insight into the structure of nucleons. As the LHC enters an era of high-precision measurements, a robust PDF determination with a reliable uncertainty quantification has become mandatory in order to match the experimental precision. The NNPDF collaboration has pioneered the use of Machine Learning (ML) techniques for PDF determinations, using Neural Networks (NNs) to parametrise the unknown PDFs in a flexible and unbiased way. The NNs are then trained on experimental data by means of stochastic gradient descent algorithms. The statistical robustness of the results is validated by extensive closure tests using synthetic data. In this work, we develop a theoretical framework based on the Neural Tangent Kernel (NTK) to analyse the training dynamics of neural networks. This approach allows us to derive, under precise assumptions, an analytical description of the neural network evolution during training, enabling a quantitative understanding of the training process. Having an analytical handle on the training dynamics allows us to clarify the role of the NN architecture and the impact of the experimental data in a transparent way. Similarly, we are able to describe the evolution of the covariance of the NN output during training, providing a quantitative description of how uncertainties are propagated from the data to the fitted function. While our results are not a substitute for PDF fitting, they do provide a powerful diagnostic tool to assess the robustness of current fitting methodologies. Beyond its relevance for particle physics phenomenology, our analysis of PDF determinations provides a testbed to apply theoretical ideas about the learning process developed in the ML community.

    hep-phcs.LGEPJC(2026)·3 citations
  10. 10*

    An -Symmetric Double Seesaw for Neutrino Masses and Mixing in Light of JUNO results

    Swaraj Kumar Nanda (SOA Univ.)🇮🇳 · Maibam Ricky Devi (Gauhati University)🇮🇳 · Chandini Dash (Utkal Univ.)🇮🇳 · R.N. Panda (SOA Univ.)🇮🇳 · Sudhanwa Patra (IIT Bhilai & IOPB)🇮🇳

    We discuss a double seesaw mechanism for generating light neutrino masses within the Standard Model extensions that include both right-handed neutrinos and extra gauge-singlet sterile fermions. The flavour structure of the double seesaw framework is invoked by an discrete symmetry which yields predictive textures for the Dirac neutrino mass matrix , the mixing matrix connecting right-handed and sterile neutrinos, and the bare Majorana mass matrix for the sterile neutrinos. The interesting feature of the present framework is that the combination of the double seesaw mechanism and flavour alignments yields a leading-order TBM structure, corrected by a single rotation in the (1-3) sector. We also derive analytic expressions for the heavy sterile eigenvalues and for the resulting light neutrino masses, thereby clarifying the role of the symmetry in shaping the neutrino mass hierarchy. We further incorporate the most recent JUNO measurements, which improve the precision of the solar mixing angle , along with updated constraints on . We show that these results significantly restrict the allowed parameter space of the model. In particular, the observed value of constrains the magnitude of the (1--3) rotation and the phases associated with the flavon couplings, while the value of sharpens these restrictions further. Overall, the interplay between double seesaw dynamics, flavour symmetry, and the recent JUNO constraints yields a highly predictive framework for neutrino masses and mixings, offering a coherent explanation for the generation of light neutrino masses and testable predictions for future experiments.

    hep-ph7 citations
  11. 11*

    Lepton-flavor violation in the MRSSMSeesaw

    Hao-Yi Liu (1,3,4)🇨🇳 · Jin-Lei Yang (1,3,4)🇨🇳 · Ke-Sheng Sun (6)🇨🇳 · Tai-Fu Feng (1,2,3,4,5) ((1) Hebei University, (2) Guangxi University,(3) Hebei Key Laboratory of High-precision Computation and Application of Quantum Field Theory,(4) Hebei Research Center of the Basic Discipline for Computational Physics, (5) Chongqing University,(6) Baoding University)🇨🇳

    The Minimal R-symmetric Supersymmetric Standard Model with Seesaw (MRSSMSeesaw) extends the MRSSM by incorporating right-handed neutrinos to generate neutrino masses via the Type-I seesaw mechanism. This work presents a detailed analysis of lepton flavor violation (LFV) processes, including , , and Higgs decays , Based on the current experimental limitations, we carry out detailed parameter scanning and numerical calculations to analyse the effects of different sensitive parameters on LFV.The numerical results show that the non-diagonal elements involving the initial and final leptons are main sensitive parameters and LFV sources.

    hep-ph0 citations
  12. 12*

    Sommerfeld Enhancement from Background Force and the Galactic Center GeV Excess

    Yu Cheng🇰🇷 · Shuailiang Ge🇰🇷

    We study the impact of background-induced forces on dark matter (DM) annihilation and their implications for indirect detection. In the presence of a finite number density of background particles, loop-level interactions can generate an effective force that is significantly enhanced relative to the vacuum case. We construct a two-component DM model in which the dominant component is a fermionic particle and the subdominant component is an ultralight pseudoscalar particle . The annihilation of proceeds through the p-wave channel and produces gamma-ray emission. The finite density of particles induces a background-enhanced force between particles, leading to a sizable Sommerfeld enhancement of the annihilation. We show that a viable region of parameter space in this model can account for the gamma-ray excess observed in the Galactic Center using Fermi-LAT data. The background-induced force substantially amplifies the Sommerfeld enhancement and thus enlarges the parameter space capable of explaining the excess, highlighting the importance of background effects in astrophysical environments.

    hep-phastro-ph.COastro-ph.HE0 citations
  13. 13*

    Neutrino Mass, Vacuum Stability and Higgs Inflation with Vector-Like Quarks and a Single Right-Handed Neutrino

    Canan Karahan🇹🇷

    We investigate a Standard Model extension containing degenerate down-type isosinglet vector-like quarks (VLQs) with masses and Yukawa couplings , supplemented by a single right-handed neutrino (RHN), aiming to simultaneously address neutrino mass generation, electroweak vacuum stability, and Higgs inflation. The VLQs play the dominant role in stabilizing the Higgs potential through their impact on the renormalization-group evolution, while the RHN generates light neutrino masses via a Type-I seesaw mechanism and smooths the high-scale running of the Higgs quartic coupling in the inflationary regime. We perform a two-loop Standard Model renormalization-group equation analysis supplemented by the one-loop contributions of the VLQs and the RHN, with proper matching across their mass thresholds. Using these RG trajectories, we identify the regions in that stabilize the Higgs potential up to the Planck scale while satisfying experimental constraints. Employing the RG-improved Higgs potential in the metric formulation of non-minimal Higgs inflation, we compute the inflationary observables and . The SM+VLQ+RHN framework yields predictions consistent with the latest Planck-LB-BK18 and ACT-LB-BK18 data, while simultaneously ensuring electroweak vacuum stability and phenomenologically viable neutrino masses within well-defined regions of parameter space. For comparison, we also investigate the SM+VLQ limit and present its vacuum stability and Higgs inflation predictions as a reference to quantify the stabilizing role of the VLQ sector.

    hep-phPTEP(2026)·0 citations
  14. 14*

    femtoscopy and the nature of

    Yi-Bo Shen🇨🇳 · Zhi-Wei Liu🇨🇳 · Ming-Zhu Liu · Rui-Xiang Shi🇨🇳 · Chu-Wen Xiao🇨🇳 · Wei-Hong Liang🇨🇳 · Li-Sheng Geng🇨🇳

    Over the past two decades, numerous exotic hadron states have been discovered, yet their underlying nature remains unclear. It is widely acknowledged that understanding hadron-hadron interactions is essential to unraveling their properties. Hadron spectroscopy is a powerful tool for this endeavor, providing rich experimental data that can shed light on exotic systems. Recently, the LHCb experiment analyzed the process and observed a narrow peak in the invariant mass spectrum, regarding it as a candidate for a pentaquark. In this work, we extract the coupled-channel potential based on the invariant mass spectrum. Our results indicate the existence of a bound state below the mass threshold, corresponding to the experimentally measured state . Furthermore, we predict the scattering lengths and momentum correlation functions for the and channels, which serve as theoretical references for future femtoscopy experiments.

    hep-phhep-exPRD(2026)·3 citations
  15. 15*

    interaction from the lineshape of in -decays

    Pedro Brandão🇧🇷 · Breno Agatão🇧🇷 · Luciano M. Abreu🇧🇷 · K. P. Khemchandani🇧🇷 · A. Martínez Torres🇧🇷

    We present a model calculation to reproduce the differential mass distribution for the system in the reactions and analyzed by the LHCb Collaboration, which shows a dominant signal for . %\textbf{We} (The idea is to) We consider a model based on coupled channel meson-meson interactions that can describe the properties of in terms of the underlying dynamics, use it to determine the invariant mass distribution of the system, and compare the results with the experimental data. We also determine the scattering length, for which different values are available from different sources, leading to a controversy. To our knowledge, this is the first attempt to reproduce the mentioned data using model calculations. Our formalism relies on the hadronization of different mesons through a weak decay, allowing for the final-state (strong) interactions among the relevant constituents. We benefit from our previous work when obtaining the amplitudes corresponding to the strong interactions. We hope that our findings can be useful in further investigations of the properties of .

    hep-phnucl-thPLB(2026)·3 citations
  16. 16*

    Probing compressed Higgsinos at the FASER experiment

    Shufang Su🇺🇸 · Wei Su🇨🇳 · Jin Min Yang🇨🇳 · Pengxuan Zhu🇦🇺 · Rui Zhu🇨🇳

    In the Minimal Supersymmetric Standard Model (MSSM), compressed Higgsinos spectrum ( GeV) occurs when and , which leads to a long-lived next-to-lightest neutralino. Such a long-lived neutralino could be copiously produced at the LHC, however escape the detection at the LHC main detectors. We examine the discovery potential at the FASER experiment and find that the FASER 2 could cover the neutral Higgsino mass up to about 130 GeV with mass splitting between 4 to 30 MeV. It is complementary to both the LHC Higgsino search in the GeV region, and displaced vertex and disappearing track searches of charginos with GeV.

    hep-ph0 citations
  17. 17*

    CoLoRFulNNLO for hadron collisions: integrating the iterated single unresolved subtraction terms

    L. Fekésházy🇩🇪 · G. Somogyi🇭🇺 · S. Van Thurenhout🇭🇺

    We present the analytic integration of the iterated single-unresolved subtraction terms in the extension of the CoLoRFulNNLO subtraction scheme to color-singlet production in hadron collisions. We exploit the fact that, in this scheme, subtraction terms are defined through momentum mappings which lead to exact phase space convolutions for real emissions. This allows us to write the integrated subtraction terms as parametric integrals, which can be evaluated using standard tools. Finally, we show that the integrated iterated single-unresolved approximate cross section can be written as a convolution of the Born cross section with an appropriately defined insertion operator.

    hep-phhep-thJHEP(2026)·5 citations
  18. 18*

    Clustering of cosmic string loops within a Milky-way like halo

    Itamar Allali🇺🇸 · Mudit Jain🇬🇧 · Shi Yan

    Loops of cosmic string experience a recoil from anisotropic gravitational radiation, known as the rocket effect, which influences the extent to which they are captured by galaxies during structure formation. Analytical studies have reached different conclusions regarding loop capture in galaxies: early treatments argued for efficient capture, while later analyses incorporating the loop rocket force throughout halo formation found that capture efficiency is reduced and strongly dependent on loop size. In this work, we employ the N-body simulation code GADGET-4, introducing non-backreacting tracer particles subject to a constant recoil force to model cosmic string loops with the rocket effect. We simulate the formation of a Milky-Way-like halo from redshift to , considering loop populations characterized by a range of length parameters , inversely proportional to the rocket acceleration. We find that the number of captured loops exhibits a pronounced peak at , arising from the competition between rocket-driven ejection at small and the declining intrinsic loop abundance at large . For fiducial string tensions, this corresponds to loops within the halo. We further find that loops with weak rocket forces closely trace the dark-matter distribution, while those subject to stronger recoil but still captured -- particularly the most abundant loops near -- are preferentially concentrated toward the central regions of the halo.

    astro-ph.COhep-ph0 citations
  19. 19*

    Towards a bottom-up formulation of spin kinetic theory

    Zonglin Mo🇨🇳 · Yi Yin🇨🇳

    We develop a bottom-up formulation of spin-kinetic theory for hot and/or dense plasmas. We introduce scalar and axial-vector phase-space functions as dynamical variables that parametrize both spin-averaged and spin-dependent distribution functions. Using spin-dependent Poisson brackets, we derive the corresponding kinetic equations and construct the associated Schwinger-Keldysh action. We further demonstrate how physical observables can be expressed in terms of these dynamical variables through constitutive relations. In the linear response regime, we establish a precise matching between the kinetic-theory and field-theory descriptions of vector and axial Wigner functions under electromagnetic and gravitational perturbations. Our framework provides a complementary approach to describing the dynamics of spin effects in a medium.

    nucl-thhep-phPRD(2026)·0 citations
  20. 20*

    Steinmann Violation and Minimal Cuts

    Holmfridur S. Hannesdottir🇺🇸 · Luke Lippstreu🇬🇧 · Andrew J. McLeod🇬🇧 · Maria Polackova🇬🇧

    The Steinmann relations are known to be violated with respect to some -- but not all -- two-particle momentum channels in massless Feynman integrals. We trace the source of this Steinmann violation to a special class of singularities, which arise from partially-overlapping minimal cuts. This allows us to propose an efficient graphical test for predicting which Steinmann relations will be violated by massless Feynman integrals of a given topology, which can be applied at any loop order. We provide evidence for this test by correctly predicting all instances of Steinmann violation in the complete set of known two-loop integrals that contribute to five-particle scattering with one or two external masses.

    hep-thhep-ph2 citations
  21. 21*

    Kinematic Anisotropies in PTA Observations: Analytical Toolkit

    Maximilian Blümke🇩🇪 · Kai Schmitz🇩🇪 · Tobias Schröder🇩🇪 · Deepali Agarwal🇺🇸 · Joseph D. Romano🇺🇸

    The reported evidence for an isotropic gravitational-wave background (GWB) from pulsar timing array (PTA) collaborations has motivated searches for extrinsic and intrinsic anisotropies. Kinematic anisotropies may arise as a consequence of a boosted observer moving with respect to the frame in which the GWB appears isotropic. In this work, we present an analytical toolbox to describe the effects of kinematic anisotropies on the overlap reduction function. Our analytical results differ from previous findings at the quadrupole order and are detailed in three appendices. For the first time, we also derive the corresponding auto-correlation using two approaches, taking the pulsar distances to be infinite or finite, respectively. Our formulas can be used in forecasts or Bayesian analysis pipelines.

    gr-qcastro-ph.COastro-ph.HEastro-ph.IM+1Symmetry(2026)·3 citations
  22. 22*

    Initial spin fluctuations as a probe of cluster spin structure in and nuclei

    Xiang Fan🇨🇳 · Jun-Qi Tao🇨🇳 · Ze-Fang Jiang · Ben-Wei Zhang🇨🇳

    We investigate the imprint of clustering on initial spin fluctuations in relativistic and collisions at ~TeV. Utilizing \textit{ab initio} configurations from Nuclear Lattice Effective Field Theory (NLEFT) and phenomenological -cluster models within a Monte-Carlo Glauber framework, we compute the event-by-event variance of the initial net spin polarization. We find that the strong short-range spin--isospin correlations characteristic of clusters lead to a significant suppression of spin fluctuations compared to a spherical Woods--Saxon baseline with uncorrelated spins. By constructing a scaled fluctuation observable that accounts for trivial finite-size effects, we demonstrate that this suppression exhibits a non-monotonic centrality dependence sensitive to the detailed cluster geometry. Furthermore, we propose the ratio of scaled spin fluctuations between and systems as a robust probe. Our results predict distinct percent-level deviations from the baseline for clustered nuclei, suggesting that measurements of final-state -hyperon spin correlations can provide novel constraints on the ground-state spin structure of light nuclei.

    nucl-thhep-ph1 citation
  23. 23*

    Jet Quenching in Anisotropic Holographic QCD: Probing Phase Transitions and Critical Regions

    Pavel Slepov🇷🇺

    The jet quenching phenomenon in an anisotropic quark-gluon plasma is studied using gauge-gravity duality. We consider a more general orientation of the contour of a lightlike Wilson loop in the boundary field theory. The Nambu-Goto action for a two-dimensional worldsheet, whose boundary is this contour, is evaluated in a five-dimensional bulk. We present the dependence of the jet quenching parameter on the orientation. Discontinuities of the jet quenching parameter occur at a first-order phase transition, and their magnitude depends on the orientation. These dependencies are observed in holographic models for both light and heavy quarks with nonzero temperature, chemical potential, magnetic field, and spatial anisotropy, supported by an Einstein-dilaton-three-Maxwell action.

    hep-thhep-phMoscow Univ.Phys.Bull.(2025)·1 citation
  24. 24*

    tension in a SI-ULDM scenario

    Jessica N. López-Sánchez🇨🇿

    We study the cosmological impact of a transient self-interaction phase in Ultra-Light Dark Matter (ULDM), focusing on its simultaneous effects on the sound horizon and the late-time growth of structure. In the presence of a quartic self-interaction, the scalar field undergoes a short-lived radiation-like phase before evolving into matter-like behaviour, inducing a localized modification of the expansion history at early times. We develop a perturbative and model-independent framework in which the self-interaction energy density is parametrized as a localized contribution to the total energy budget. Within this approach, the responses of the sound horizon and the linear growth factor can be expressed as weighted integrals over cosmic time, with distinct kernels encoding the temporal sensitivity of each observable. This structure leads to a simple analytic relation linking the corresponding early- and late-time responses, and naturally predicts correlated shifts in and whose sign and magnitude depend on the timing of the self-interaction episode. Our results show that a single transient modification of the expansion history can interpolate between early-time effects on the sound horizon and late-time suppression of structure growth within a unified physical framework, providing an analytical understanding of their joint response.

    astro-ph.COhep-ph1 citation
  25. 25*

    Total Gluon Helicity Contribution to the Proton Spin from Lattice QCD

    Dian-Jun Zhao🇨🇳 · Long Chen🇨🇳 · Hongxin Dong🇨🇳 · Xiangdong Ji🇺🇸 · Liuming Liu🇨🇳 · Zhuoyi Pang🇨🇳 · Andreas Schäfer🇩🇪 · Peng Sun🇨🇳 · Yi-Bo Yang🇨🇳 · Jian-Hui Zhang🇨🇳 · Shiyi Zhong🇨🇳

    We report a state-of-the-art lattice QCD calculation of the total gluon helicity contribution to the proton spin, . The calculation is done on ensembles with three different lattice spacings fm. By employing distillation and momentum smearing for proton external states, we extract the bare matrix elements of the topological current using 5-HYP smeared Coulomb gauge fixing configurations. Furthermore, we apply a non-perturbative renormalization scheme augmented by the Cluster Decomposition Error Reduction (CDER) technique to determine the renormalization constants of . The results obtained from different components (with being the direction of proton momentum or polarization) are consistent with Lorentz covariance within uncertainties. After extrapolating to the continuum limit, is found to be at the scale , which constitutes approximately of the proton spin.

    hep-lathep-phhep-thnucl-ex+13 citations
  26. 26*

    Self-Gravitating Scalar Field Configurations, Ultra Light Dark Matter and Galactic Scale Observations

    Bihag Dave🇮🇳

    In this thesis, we investigate the possibility that dark matter consists of ultra light spin-zero particles with mass . We focus on the role of self-interactions, assuming all other non-gravitational couplings to Standard Model particles are negligible. Such ultra light dark matter (ULDM) is expected to form stable self-gravitating scalar field configurations (solitons), whose properties depend on the particle mass and self-coupling . Using solutions of the Gross-Pitaevskii-Poisson equations, we explore how galactic-scale observations can constrain and . We show that observational upper limits on the mass enclosed in central galactic regions can probe both attractive and repulsive self-interactions with strengths . We further demonstrate that self-interactions can allow ULDM to describe observed rotation curves as well as satisfy an empirical soliton-halo mass relation in low surface brightness galaxies for and . We also study tidal effects in satellite dwarf galaxies and find that attractive self-interactions can extend their lifetimes over cosmological timescales, allowing ULDM to evade recent constraints derived for the non-interacting case. Finally, we explore machine learning based inference of dark matter and baryonic parameters from galaxy rotation curves, showing that neural networks can recover parameters consistent with observations.

    astro-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.