PaperPanorama

HEP Phenomenology·hep-ph

Thu·Dec 22, 2022

33 papers25 primary·8 cross-listed·reconstructed*

  1. 01*

    Soft and hard scales of the transverse momentum distribution in the Color String Percolation Model

    J. R. Alvarado García🇲🇽 · D. Rosales Herrera🇲🇽 · P. Fierro🇲🇽 · J. E. Ramírez🇲🇽 · A. Fernández Téllez🇲🇽 · C. Pajares🇪🇸

    In color string models, the transverse momentum distribution (TMD) is obtained through the convolution of the Schwinger mechanism with the string tension fluctuations distribution. Considering a -Gaussian distribution for these fluctuations, the TMD becomes a hypergeometric confluent function that adequately reproduces the characteristic scales at low and high values. In this approach, the hard scale of the TMD is a consequence of considering a heavy-tailed distribution for the string tension fluctuations whose width rises as , multiplicity or centrality increases. In this paper, we introduce the complete information of the TMD in the color string percolation model by means of the determination of the color suppression factor, which now also depends on the parameters of the -Gaussian. To this end, we analyze the reported data on pp and AA collisions at different center of mass energies, multiplicities, and centralities. In particular, for minimum bias pp collisions, we found that the -Gaussian parameters and the effective temperature are monotonically increasing functions of the center of mass energy. Similar results are found for AA collisions as a function of the centrality at fixed . We summarize these results in a phase diagram that indicates the -Gaussian parameters region allowing the quark-gluon plasma formation.

    hep-phcond-mat.stat-mechJ.Phys.G(2023)·12 citations
  2. 02*

    Comparing Point Cloud Strategies for Collider Event Classification

    Peter Onyisi🇺🇸 · Delon Shen🇺🇸 · Jesse Thaler🇺🇸

    In this paper, we compare several event classification architectures defined on the point cloud representation of collider events. These approaches, which are based on the frameworks of deep sets and edge convolutions, circumvent many of the difficulties associated with traditional feature engineering. To benchmark our architectures against more traditional event classification strategies, we perform a case study involving Higgs boson decays to tau leptons. We find a 2.5 times increase in performance compared to a baseline ATLAS analysis with engineered features. Our point cloud architectures can be viewed as simplified versions of graph neural networks, where each particle in the event corresponds to a graph node. In our case study, we find the best balance of performance and computational cost for simple pairwise architectures, which are based on learned edge features.

    hep-phhep-exphysics.data-anPRD(2023)·9 citations
  3. 03*

    Modular Symmetry With Three-Moduli and Flavor Problem

    Mohammed Abbas🇸🇦 · Shaaban Khalil🇪🇬

    The modular symmetry with three moduli is investigated. We assign different moduli to charged leptons, neutrinos, and quarks. We analyze these moduli at their fixed points where a residual symmetry exists. We consider two possibilities for right-handed neutrinos. First, they are assumed to be singlets under modular symmetry. In this case, we show that the lepton masses and mixing can be obtained consistently with experimental observations. Second, they are assigned non-trivially under modular symmetry. We emphasize that a small deviation from their fixed point is required in this case. Finally, the quark masses and mixing are generated correctly around the fixed point of their modulus. In our analysis, we only consider the simple case of weight 2.

    hep-phInt.J.Mod.Phys.A(2024)·11 citations
  4. 04*

    Prospects of a Strong first-order Electroweak Phase Transition in the -NMSSM

    Arindam Chatterjee🇮🇳 · AseshK Datta🇮🇳 · Subhojit Roy🇮🇳

    We have studied the viability and possible patterns of a strong first-order electroweak phase transition (SFOEWPT) within the -symmetric Next-to-Minimal Supersymmetric Standard Model (NMSSM), in view of the latest experimental results from the dark matter (DM) sector, Higgs sector and the searches of the lighter chargino and neutralinos at the Large Hadron Collider (LHC). We show that the region of parameter space with relatively small that favors an SFOEWPT has started to get excluded from the searches at the LHC and various DM experiments. However, there still remain phenomenologically much involved and compatible regions for an SFOEWPT that are yet not sensitive to the latest LHC and DM searches. We further estimate the production of stochastic gravitational waves (GW) from an SFOEWPT within and without the bag model and the prospects of detecting such signals at various future/proposed GW experiments.

    hep-phPoS(2022)·0 citations
  5. 05*

    Decay of the Mediator Particle at Threshold

    Shigeki Matsumoto🇯🇵 · Yu Watanabe🇯🇵 · Yuki Watanabe🇯🇵 · Graham White🇯🇵

    A light mediator particle is often predicted in the dark sector scenario, which weakly interacts with the standard model (SM) particles. The weakness of the interaction is usually described by a small coupling; however, the small coupling does not always guarantee the weakness of the interaction. When the mass of the mediator particle lies in a threshold region, the so-called threshold singularity may emerge, and then the perturbative calculation fails. This singularity causes several effects, e.g., the mixing between the mediator particle and bound states, the Sommerfeld effect on the final state of the mediator particle decay, etc. Taking the minimal model of the vector mediator particle decaying mainly into the SM particles as an example, we develop a method to describe the singularity quantitatively. We also calculate some physical quantities using this method, such as the lifetime of the mediator particle, and find that those could be significantly altered compared with the result of the perturbative calculation.

    hep-phcs.NAmath.NAJHEP(2023)·7 citations
  6. 06*

    The time-like electromagnetic kaon form factor

    A.S. Miramontes🇲🇽 · Adnan Bashir🇲🇽

    We compute the electromagnetic charged kaon form factor in the time-like region by employing a Poincaré covariant formalism of the Bethe-Salpeter equation to study quark-antiquark bound states in conjunction with the Schwinger-Dyson equation for the quark propagator. Following a recent kindred calculation of the time-like electromagnetic pion form factor, we include the most relevant intermediate composite particles permitted by their quantum numbers in the interaction kernel to allow for a decay mechanism for the resonances involved. This term augments the usual gluon mediated interaction between quarks. For a sufficiently low energy time-like probing photon, the electromagnetic form factor is saturated by the and resonances. We assume isospin symmetry throughout. Our results for the absolute value squared of the electromagnetic form factor agree qualitatively rather well and quantitatively moderately so with available experimental data.

    hep-phnucl-thPRD(2023)·14 citations
  7. 07*

    A Portal Dedicated to Higgs Bosons for Experts and the General Public

    Andre Sopczak (on behalf of the International Particle Physics Outreach Group)🇨🇿

    As an educational aid and source for expert information, a web portal dedicated to Higgs boson research is presented. A database is created with more than 1000 relevant articles using CERN Document Server API and web scraping methods. The database is automatically updated when new results on the Higgs boson become available. Using artificial intelligence and natural language processing, the articles are categorized according to properties of the Higgs boson and other criteria. The process of designing and implementing the Higgs Boson Portal (HBP) is described. The components of the HBP are deployed to CERN Web Services using the OpenShift cloud platform. The HBP is accessible within the Czech Particle Physics Project (CPPP) at http://cern.ch/cppp and directly at http://cern.ch/higgs.

    hep-phhep-exPoS(2023)·0 citations
  8. 08*

    Searching for axion streams with the echo method

    Ariel Arza🇷🇺 · Abaz Kryemadhi🇺🇸 · Konstantin Zioutas🇬🇷

    The axion dark matter echo technique, proposed in Ref. [1], aims to search for axion dark matter by detecting the electromagnetic echo coming from stimulated decay of ambient axion dark matter interacting with a radio-microwave outgoing beam. In this work we consider deviations from the standard halo model (SHM) in the form of fine grained streams that are present in the solar system and use them as a target for the axion echo method, which demonstrates to be very sensitive to particular local axion dark matter phase space distributions. We show that the extremely small dispersion of the streams works in favor of the echo method performance, improving its sensitivity in the axion-photon coupling up to two orders of magnitude, with respect to the isotropic SHM. We also discuss the possibility of targeting high density dark matter hairs formed when fine grained streams focus by the inner Earth's gravitational field.

    hep-phhep-exPRD(2023)·18 citations
  9. 09*

    Holographic Composite Higgs Model Building: Soft Breaking, Maximal Symmetry, and the Higgs Mass

    Simone Blasi🇧🇪 · Julian Bollig🇩🇪 · Florian Goertz🇩🇪

    We study the emergence and phenomenological consequences of recently proposed new structures, namely soft breaking of the Higgs shift symmetry and `maximal symmetry' of the composite sector, in holographic realizations of composite Higgs models. For the former, we show that soft breaking can also successfully be implemented in a full 5D warped model, where symmetry-restoring universal boundary conditions for the fermion fields allow to break the problematic connection between a realistically light Higgs and anomalously light top partners. For the latter, we demonstrate that the minimal incarnation of maximal symmetry in the holographic dual leads to a sharp prediction of GeV for GeV. We find that a viable implementation is possible with sizable negative gauge brane kinetic terms, allowing for GeV. Overall, both approaches offer promising directions to improve the naturalness also of holographic realizations of composite Higgs models.

    hep-phJHEP(2023)·8 citations
  10. 10*

    Top Yukawa Coupling at the Muon Collider

    Miranda Chen🇺🇸 · Da Liu🇺🇸

    We have presented a detailed study about the prospects for the measurement of the top Yukawa coupling in the vector boson fusion (VBF) production of a top quark pair at high energy muon colliders. By employing the effective approximation and the high energy limit for the helicity amplitudes of the subprocess , we have derived the energy scaling of the statistical signal significance in the presence of the anomalous couplings. The sensitivity on the top Yukawa coupling decreases as the bin energy increases. For the anomalous triple gauge boson couplings and the gauge-boson-fermion couplings with energy growing behavior for the interference term, the signal significance has mild increase at the beginning and start to decrease for . The 95\% C.L. on the anomalous top Yukawa coupling is projected to be 5.6\% (1.7\%) at a 10 (30) TeV muon collider, which is comparable to the sensitivity of 2\% at the 100 TeV collider.

    hep-phPRD(2024)·25 citations
  11. 11*

    in a Two-Higgs-Doublet Model with flavour-changing up-type Yukawa couplings

    Martin S. Lang🇩🇪 · Ulrich Nierste🇩🇪

    We present a Two-Higgs-Doublet Model in which the structure of the quark Yukawa matrices is governed by three spurions breaking the flavour symmetries of the quark Yukawa sector. The model naturally suppresses flavour-changing neutral current (FCNC) amplitudes in the down-type sector, but permits sizable FCNC couplings in the up sector. We calculate the branching ratio of to leading and next-to-leading order of QCD for the case with FCNC couplings of the heavy neutral Higgs bosons to up-type quarks and verify that all counterterms follow the pattern dictated by the spurion expansion of the Yukawa matrices. We find correlations between , , and the Higgs masses. The mixing amplitude is naturally suppressed in the model but can probe a portion of the parameter space with very heavy Higgs bosons.

    hep-phJHEP(2024)·7 citations
  12. 12*

    Supermassive black hole seeds from sub-keV dark matter

    Avi Friedlander🇨🇦 · Sarah Schon🇺🇸 · Aaron C. Vincent🇨🇦

    Quasars observed at redshifts are powered by supermassive black holes which are too large to have grown from early stellar remnants without efficient super-Eddington accretion. A proposal for alleviating this tension is for dust and metal-free gas clouds to have undergone a process of direct collapse, producing black hole seeds of mass around redshift . For direct collapse to occur, a large flux of UV photons must exist to photodissociate molecular hydrogen, allowing the gas to cool slowly and avoid fragmentation. We investigate the possibility of sub-keV mass dark matter decaying or annihilating to produce the UV flux needed to cause direct collapse. We find that annihilating dark matter with a mass in the range of can produce the required flux while avoiding existing constraints. A non-thermally produced dark matter particle which comprises the entire dark matter abundance requires a thermally averaged cross section of cms. Alternatively, the flux could originate from a thermal relic which comprises only a fraction of the total dark matter density. Decaying dark matter models which are unconstrained by independent astrophysical observations are unable to sufficiently suppress molecular hydrogen, except in gas clouds embedded in dark matter halos which are larger, cuspier, or more concentrated than current simulations predict. Lastly, we explore how our results could change with the inclusion of full three-dimensional effects. Notably, we demonstrate that if the self-shielding is less than the conservative estimate used in this work, the range of both annihilating and decaying dark matter models which can cause direct collapse is significantly increased.

    hep-phastro-ph.COastro-ph.GAJCAP(2023)·14 citations
  13. 13*

    50 Years of Quantum Chromodynamics

    Franz Gross🇺🇸 · Eberhard Klempt🇩🇪 · Stanley J. Brodsky🇺🇸 · Andrzej J. Buras🇩🇪 · Volker D. Burkert🇺🇸 · Gudrun Heinrich🇩🇪 · Karl Jakobs🇩🇪 · Curtis A. Meyer🇺🇸 · Kostas Orginos🇺🇸 · Michael Strickland🇺🇸 · Johanna Stachel🇩🇪 · Giulia Zanderighi🇩🇪 and 83 other authors

    This paper presents a comprehensive review of both the theory and experimental successes of Quantum Chromodynamics, starting with its emergence as a well defined theory in 1972-73 and following developments and results up to the present day. Topics include a review of the earliest theoretical and experimental foundations; the fundamental constants of QCD; an introductory discussion of lattice QCD, the only known method for obtaining exact predictions from QCD; methods for approximating QCD, with special focus on effective field theories; QCD under extreme conditions; measurements and predictions of meson and baryon states; a special discussion of the structure of the nucleon; techniques for study of QCD at high energy, including treatment of jets and showers; measurements at colliders; weak decays and quark mixing; and a section on the future, which discusses new experimental facilities or upgrades currently funded. The paper is intended to provide a broad background for Ph.D. students and postdocs starting their career. Some contributions include personal accounts of how the ideas or experiments were developed.

    hep-phhep-exhep-lathep-thEPJC(2023)·416 citations
  14. 14*

    Odderon as Regge oddball spin-3 in and elastic scattering

    Jingle B. Magallanes🇵🇭 · Prin Sawasdipol🇹🇭 · Chakrit Pongkitivanichkul🇹🇭 · Daris Samart🇹🇭

    In this work, we propose that the odderon is a Regge odd-glueball tensor spin-3. To demonstrate our proposal, we study the and elastic scattering by including contributions of the spin-3 odderon and spin-2 pomeron exchange in the processes. The phenomenological effective Lagrangian approach is used to calculate the and elastic scattering amplitudes at the tree level. In addition, a Donnachie-Landschoff ansatz of the odderon and pomeron propagators has been used in this work. We fit the theoretical results with the various experimental data of the and scattering at the TeV scale to determine the model parameters in the present work. By using the model parameters, the Chew-Frautschi plot of the tensor odderon Regge trajectory is evaluated. As a result, the odderon spin-3 mass is predicted to be 3.2 GeV. In addition, the total cross-section of our model is compatible with the results from TOTEM and its extrapolation from D0 collaboration. Moreover, the total cross-section also satisfies the Friossart bound at the Regge limit.

    hep-phnucl-thPRD(2024)·4 citations
  15. 15*

    Beyond oblique contributions: r and W-mass in models with scalar leptoquarks

    Carlo Marzo🇪🇪

    We study the dominant non-universal contributions to muon decay for the five scalar leptoquarks (LQs) allowed by the Standard Model gauge symmetries. By using a common computational framework, we isolate the new-Physics (NP) one-loop corrections over the observable and explore the connection with the boson mass. We highlight the role of non-universal terms considering, for the doublet and triplet LQs, a completely degenerate scenario, thus cancelling/moderating the effects of the oblique parameters S,T and U . We determine simple formulas that exhibit the leading non-universal behaviour generated by the introduction of extra Yukawa terms, and confront them against a present tension in and the projected FCC-ee accuracy.

    hep-phInt.J.Mod.Phys.A(2023)·2 citations
  16. 16*

    Non-strange quark stars within resummed QCD

    Tulio E. Restrepo🇧🇷 · Constança Providência🇵🇹 · Marcus Benghi Pinto🇧🇷

    The recently developed resummation technique known as {\it renormalization group optimized perturbation theory} (RGOPT) is employed in the evaluation of the EoS describing non-strange cold quark matter at NLO. Inspired by recent investigations, which suggest that stable quark matter can be made only of up and down quarks, the mass-radius relation for two flavor pure quark stars is evaluated and compared with the predictions from perturbative QCD (pQCD) at NNLO. This comparison explicitly shows that by being imbued with renormalization group properties, and a variational optimization procedure, the method allows for an efficient resummation of the perturbative series. Remarkably, when the renormalization scale is chosen so as to reproduce maximum mass stars with M=, one obtains a mass-radius curve compatible with the masses and radii of the pulsars PSR J0740+6620, PSR J0030+0451, and the compact object HESS J1731-347. Moreover, the scale dependence of the EoS (and mass-radius relation) obtained with the RGOPT is greatly improved when compared to that of pQCD. This seminal application to the description of quark stars shows that the RGOPT represents a robust alternative to pQCD when describing compressed quark matter.

    hep-phastro-ph.HEnucl-thPRD(2023)·24 citations
  17. 17*

    NNLO subtraction for any massless final state: a complete analytic expression

    Gloria Bertolotti🇮🇹 · Lorenzo Magnea🇮🇹 · Giovanni Pelliccioli🇩🇪 · Alessandro Ratti🇩🇪 · Chiara Signorile-Signorile🇩🇪 · Paolo Torrielli🇮🇹 · Sandro Uccirati🇮🇹

    We use the Local Analytic Sector Subtraction scheme to construct a completely analytic set of expressions implementing a fully local infrared subtraction at NNLO for generic coloured massless final states. The cancellation of all explicit infrared poles appearing in the double-virtual contribution, in the real-virtual correction and in the integrated local infrared counterterms is explicitly verified, and all finite contributions arising from integrated local counterterms are analytically evaluated in terms of ordinary polylogarithms up to weight three. The resulting subtraction formula can readily be implemented in any numerical framework containing the relevant matrix elements up to NNLO.

    hep-phJHEP(2023)·47 citations
  18. 18*

    Constraining scalar leptoquarks using COHERENT data

    Roberta Calabrese🇮🇹 · Jacob Gunn🇮🇹 · Gennaro Miele🇮🇹 · Stefano Morisi🇮🇹 · Samiran Roy🇮🇹 · Pietro Santorelli🇮🇹

    Neutrino-nucleus coherent scattering measurements by the COHERENT collaboration provide us with a unique capability to test various beyond the standard model scenarios. In this work, we constrain scalar leptoquarks (LQs) using the COHERENT data. LQs arise in many extensions of the Standard Model (SM). Generally, the mass of the LQs is assumed to be very high to avoid the bounds from proton decay. However, there are low-scale LQ models which prohibit proton decay by construction. We consider two electroweak doublet scalar LQ models with hypercharge Y=1/6, and Y=7/6 and provide the bounds in the plane of the Yukawa coupling and the mass of LQ. We also compare the bounds on LQs coming from various other experiments and find that the COHERENT one covers a wide range of LQ masses from MeV to TeV and in certain regions the constraints are competitive with the others.

    hep-phPRD(2023)·10 citations
  19. 19*

    Theoretical concepts and measurement prospects for BSM trilinear couplings: a case study for scalar top quarks

    Henning Bahl🇺🇸 · Johannes Braathen🇩🇪 · Georg Weiglein🇩🇪

    After the possible discovery of new heavy particles at the LHC, it will be crucial to determine the properties and the underlying physics of the new states. In this work, we focus on scalar trilinear couplings, employing as an example the case of the trilinear coupling of scalar partners of the top quark to the Higgs boson. We discuss possible strategies for experimentally determining the scalar top (stop) trilinear coupling parameter, which controls the stop--stop--Higgs interaction, and we demonstrate the impact of different renormalisation prescriptions for this parameter. We find that the best prospects for determining the stop trilinear coupling arise from its quantum effects entering the model prediction for the mass of the SM-like Higgs boson in comparison to the measured value. We point out that the prediction for the Higgs-boson mass has a high sensitivity to the stop trilinear coupling even for heavy masses of the non-standard particles. Regarding the renormalisation of the stop trilinear coupling we identify a renormalisation scheme that is preferred in view of the present level of accuracy and we clarify the source of potentially large logarithms that cannot be resummed with standard renormalisation group methods.

    hep-phEPJC(2023)·6 citations
  20. 20*

    Dilution of Dark Matter Relic abundance due to First Order Electroweak Phase Transition

    Subhojit Roy🇮🇳

    We investigate the effect of a first-order electroweak phase transition (FOEWPT), which is one of the prerequisites for electroweak baryogenesis, on the thermal relic abundance of the dark matter (DM) that freezes out before the occurrence of the phase transition in the complex singlet scalar extended -invariant type-II seesaw model that can simultaneously provide a DM candidate, explain the non-vanishing neutrino masses and the baryon asymmetry of the Universe. Such a phase transition around the electroweak scale leaves an impact on the relic density due to the release of entropy, particularly for a TeV-scale DM. We thus concentrate on the region of parameter space of the said model, which favors an FOEWPT in the early Universe and for which the DM is heavy such that its freeze-out temperature turns out to be larger than the phase transition temperature. We further study the dependencies of the dilution factor of the DM relic density on the model parameters, the nucleation temperature, the strength and the duration of the phase transition. Such a dilution might retrieve some of the regions of parameter space that were previously ruled out by the measured value of the DM relic density and/or the latest constraints from the DM direct-detection experiments. Furthermore, a direct connection is drawn between the dilution factor and the generation of stochastic gravitational waves as a result of an FOEWPT.

    hep-phPRD(2025)·18 citations
  21. 21*

    Sensitivity to Triple Higgs Couplings via Di-Higgs Production in the 2HDM at the (HL-)LHC

    F. Arco🇪🇸 · S. Heinemeyer🇪🇸 · M. Mühlleitner🇩🇪 · K. Radchenko🇩🇪

    An important task of the LHC is the investigation of the Higgs-boson sector. Of particular interest is the reconstruction of the Higgs potential, i.e. the measurement of the Higgs self-couplings. Based on previous analyses, within the 2HDMs type~I and~II, we analyze several two-dimensional benchmark planes that are over large parts in agreement with all theoretical and experimental constraints. For these planes we evaluate di-Higgs production cross sections at the (HL-)LHC with a center-of-mass energy of 13 TeV at NLO in the heavy top-quark limit with the code HPAIR. We investige in particular the process , with being the Higgs boson discovered at the LHC with a mass of about 125 GeV. The top box diagram of the loop-mediated gluon fusion process into Higgs pairs interferes with the -channel exchange of the two CP-even 2HDM Higgs bosons and involving the trilinear couplings and , respectively. Depending on the size of the involved top-Yukawa and triple Higgs couplings as well as on the mass of , the contribution of the -channel ~diagram can be dominating or be highly suppressed. We find regions of the allowed parameter space in which the di-Higgs production cross section can differ by many standard deviations from its SM prediction, indicating possible access to deviations in from the SM value and/or contributions involving . The sensitivity to is further analyzed employing the distributions. We demonstrate how a possible measurement of depends on the various experimenal uncertainties. Depending on the underlying parameter space, the HL-LHC may have the option not only to detect beyond-the-Standard-Model triple Higgs couplings, but also to provide a first rough measurement of their sizes.

    hep-phEPJC(2023)·25 citations
  22. 22*

    FETA: Flow-Enhanced Transportation for Anomaly Detection

    Tobias Golling🇨🇭 · Samuel Klein🇨🇭 · Radha Mastandrea🇺🇸 · Benjamin Nachman🇺🇸

    Resonant anomaly detection is a promising framework for model-independent searches for new particles. Weakly supervised resonant anomaly detection methods compare data with a potential signal against a template of the Standard Model (SM) background inferred from sideband regions. We propose a means to generate this background template that uses a flow-based model to create a mapping between high-fidelity SM simulations and the data. The flow is trained in sideband regions with the signal region blinded, and the flow is conditioned on the resonant feature (mass) such that it can be interpolated into the signal region. To illustrate this approach, we use simulated collisions from the Large Hadron Collider (LHC) Olympics Dataset. We find that our flow-constructed background method has competitive sensitivity with other recent proposals and can therefore provide complementary information to improve future searches.

    hep-phhep-exphysics.data-anPRD(2023)·62 citations
  23. 23*

    Magnetic Moments of Astrophysical Neutrinos

    Joachim Kopp (CERN)🇨🇭 · Toby Opferkuch (UC Berkeley)🇺🇸 · Edward Wang (TU Munich)🇩🇪

    We study the impact of neutrino magnetic moments on astrophysical neutrinos, in particular supernova neutrinos and ultra-high energy neutrinos from extragalactic sources. We show that magnetic moment-induced conversion of left-handed neutrinos into unobservable right-handed singlet states can substantially change the flux and flavour composition of these neutrinos at Earth. Notably, neutrinos from a supernova's neutronisation burst, whose flux can be predicted with O(10%) accuracy, offer a discovery reach to neutrino magnetic moments , up to one order of magnitude below current limits. For high-energy neutrinos from distant sources, for which no robust flux prediction exists, we show how the flavour composition at Earth can be used as a handle to establish the presence of non-negligible magnetic moments, potentially down to if the measurement can be performed on neutrinos from a single source. In both cases, the sensitivity strongly depends on the galactic resp. intergalactic magnetic field profiles along the line of sight. Therefore, while a discovery is possible down to very small values of the magnetic moment, the absence of a discovery does not imply an equally strong limit. We also comment on the dependence of our results on the right-handed neutrino mass, paying special attention to the transition from coherent deflection by a classical magnetic field to incoherent scattering on individual scattering targets. Finally, we show that a measurement of Standard Model Dirac neutrino magnetic moments, of order , could be possible under rather optimistic, but not completely outrageous, assumptions using flavour ratios of high-energy astrophysical neutrinos.

    hep-phastro-ph.HEJCAP(2024)·15 citations
  24. 24*

    Probing HNL-ALP couplings at colliders

    Arturo de Giorgi🇪🇸 · Luca Merlo🇪🇸 · Jean-Loup Tastet🇪🇸

    Axion-like particles (ALPs) and heavy neutral leptons (HNLs) are both well-motivated extensions of the Standard Model. As ALPs couple to on-shell fermions proportionally to their masses, processes involving both types of particles may give rise, for TeV HNLs, to relevant phenomenology at colliders. In this work, we point out a particularly clean process, whose final state consists of four jets and two charged leptons, and we estimate its current and future sensitivity at the LHC. For on-shell HNLs, i) there is no dependence on the overall scale of the mixing between HNLs and the active neutrinos, making this process sensitive down to the type-I Seesaw line; ii) the signal strength of the process is sizable only as far as the HNL masses are below a few TeVs, contrary to what the proportionality to masses of the ALP couplings may suggest. Although ALPs and HNLs have been mainly studied independently in the literature, considering their interplay may lead to joint limits that are much stronger than those on the individual particles taken separately. This concise study paves the way for similar searches at colliders and other experiments.

    hep-phhep-exFortsch.Phys.(2023)·26 citations
  25. 25*

    Dark Matter and Baryogenesis from Visible-Sector Long-Lived Particles

    Rouzbeh Allahverdi🇺🇸 · Ngo Phuc Duc Loc🇺🇸 · Jacek K. Osiński🇵🇱

    We present a minimal extension of the standard model that includes a long-lived fermion with weak-scale mass and an fermionic dark matter candidate both of which are coupled to quarks. Decays of a TeV-scale colored scalar in a radiation-dominated phase bring the former to a thermal abundance while also producing dark matter. The long-lived fermion then dominates the energy density of the Universe and drives a period of early matter domination. It decays to reheat the Universe, mainly through baryon-number-violating interactions that also generate a baryon asymmetry, with a small branching fraction to dark matter. We find the allowed parameter space of the model and show that it can be probed by proposed long-lived particle searches as well as next-generation neutron-antineutron oscillation experiments. This model provides a robust explanation of dark matter and baryogenesis as long as the Universe is in a radiation-dominated phase at .

    hep-phastro-ph.COhep-thPRD(2023)·13 citations
  26. 26*

    Dispersion Relations for Dislocation Modes and their Sensitivity to the Lattice Structure

    Jin-Yun Lin🇺🇸 · Shashin Pavaskar🇺🇸 · Ira Z. Rothstein🇺🇸

    In this letter we show that the dispersion relation for the dynamical modes of dislocations ("dislons") in solids is sensitive to the lattice symmetries. In particular, we show that in the IR, the dislon dispersion relation develops a logarithmic dependence on momenta for approximately isotropic lattices whereas for non-isotropic lattices, the linear term dominates. The renormalization group flows for dislocation tension are shown to be distinct for isotropic and anisotropic lattices.

    hep-thcond-mat.mtrl-scihep-phPRB(2025)·6 citations
  27. 27*

    Outreach Modules for New Particle Searches Using the ATLAS Forward Proton Detector and for Higgs Boson Physics

    Andre Sopczak (on behalf of the International Particle Physics Outreach Group)🇨🇿

    We present two modules as part of the Czech Particle Physics Project (CPPP). These modules are intended as learning tools in masterclasses aimed at high-school students (aged 15 to 18). The first module is dedicated to the detection of an Axion-Like-Particle (ALP) using the ATLAS Forward Proton (AFP) detector. The second module focuses on the reconstruction of the Higgs boson mass using the Higgs boson golden channel with four leptons in the final state. The modules are accessible at http://cern.ch/cppp.

    hep-exhep-phPoS(2023)·0 citations
  28. 28*

    Neutron Star versus Neutral Star: On the 90th anniversary of Landau's publication in astrophysics

    Renxin Xu (PKU)🇨🇳

    In the late age of developing quantum mechanics, Lev Landau, one of the distinguished players, made great efforts to understand the nature of matter, even stellar matter, by applying the quantum theory. Ninety years ago, he published his idea of "neutron" star, which burst upon him during his visit over Europe in the previous year. The key point that motivated Landau to write the paper is to make a state with lower energy for "gigantic nucleus", avoiding extremely high kinematic energy of electron gas due to the new Fermi-Dirac statistics focused hotly on at that time. Landau had no alternative but to neutronize/neutralize by "combining a proton and an electron", as electron and proton were supposed to be elementary before the discovery of neutron. However, our understanding of the Nature has fundamentally improved today, and another way (i.e., strangeonization) could also embody neutralization and thus a low-energy state that Landau had in mind, which could further make unprecedented opportunities in this multi-messenger era of astronomy. Strangeon matter in "old" physics may impact dramatically on today's physics, from compact stars initiated by Landau, to cosmic rays and dark matter. In this essay, we are making briefly the origin and development of neutron star concept to reform radically, to remember Landau's substantial contribution in astrophysics and to recall those peculiar memories.

    physics.hist-phastro-ph.HEhep-phnucl-thAstron.Nachr.(2023)·7 citations
  29. 29*

    Heavy quark diffusion coefficient with gradient flow

    Viljami Leino🇩🇪 · Nora Brambilla🇩🇪 · Julian Mayer-Steudte🇩🇪 · Peter Petreczky🇺🇸

    The heavy quark diffusion coefficient is encoded in the spectral functions of the chromo-electric and the chromo-magnetic correlators, of which the latter describes the T/M contribution. We study these correlators at two different temperatures and in the deconfined phase of SU(3) gauge theory. We use gradient flow for noise reduction. We perform both continuum and zero flow time limits to extract the heavy quark diffusion coefficient. Our results imply that the mass suppressed effects in the heavy quark diffusion coefficient are 20% for bottom quarks and 34% for charm quark at .

    hep-lathep-phPoS(2023)·3 citations
  30. 30*

    Unobservability of topological charge in nonabelian gauge theory

    Nodoka Yamanaka🇯🇵

    We show that the topological charge of nonabelian gauge theory is unphysical by using the fact that it always involves the unphysical gauge field component proportional to the gradient of the gauge function. The removal of Gribov copies, which may break the Becchi-Rouet-Stora-Tyutin symmetry, is irrelevant thanks to the perturbative one-loop finiteness of the chiral anomaly. The unobservability of the topological charge immediately leads to the resolution of the Strong CP problem. We also present important consequences such as the physical relevance of axial symmetry, the -independence of vacuum energy, the unphysicalness of topological instantons, and the impossibilities of realizing the sphaleron induced baryogenesis as well as the chiral magnetic effect. The unphysical vacuum angle and the axial symmetry also imply that the CP phase of the Cabibbo-Kobayashi-Maskawa matrix is the sole source of CP violation of the standard model.

    hep-thhep-lathep-phnucl-th17 citations
  31. 31*

    Domain wall annihilation -- a QFT perspective

    Oriol Pujolas🇪🇸 · George Zahariade🇪🇸

    Domain wall networks in the early universe, formed upon spontaneous breaking of a discrete symmetry, have a rich impact on cosmology. Yet, they remain somewhat unexplored. We introduce a new analytic strategy to understand better the domain wall epoch, from formation to annihilation. Our method includes a quantum field theoretical treatment of the initial state at domain wall formation, as well as of the time evolution. We find that the domain wall area density for a network with biased initial condition in dimensional flat spacetime evolves as . We comment on the relation between this and previous results obtained in condensed matter and in cosmology. The extrapolation of this law to an expanding universe applies to networks that are close to the domain wall `gas' limit.

    hep-thastro-ph.COcond-mat.dis-nncond-mat.other+1PRD(2023)·18 citations
  32. 32*

    Direct access to hadronic decay parameters with twisted boundary conditions

    Benoît Blossier🇫🇷 · Jochen Heitger🇩🇪 · Jan Neuendorf🇫🇷 · Teseo San José🇫🇷

    Our exploratory study looks for direct access to the resonant hadronic transition amplitude without resorting to the Lüscher formalism. We study the decay by applying partially twisted boundary conditions to the quenched charm quark, circumventing possible problems with final state interactions. If successful, we could compute the dependence of the transition amplitude on the charm-quark mass and test the predictions made by phenomenological quark-pair-creation models. Finally, we study if and to what extent an extraction of the excited state is necessary for this analysis.

    hep-lathep-phPoS(2023)·1 citation
  33. 33*

    High-Energy Neutrinos from Gamma-Ray-Faint Accretion-Powered Hypernebulae

    Navin Sridhar (1)🇺🇸 · Brian D. Metzger (1, 2)🇺🇸 · Ke Fang (3) ((1) Columbia University, (2) Flatiron Institute, (3) University of Wisconsin, Madison)🇺🇸

    Hypernebulae are inflated by accretion-powered winds accompanying hyper-Eddington mass transfer from an evolved post-main sequence star onto a black hole or neutron star companion. The ions accelerated at the termination shock -- where the collimated fast disk winds/jet collide with the slower, wide-angled wind-fed shell -- can generate high-energy neutrinos via hadronic () reactions, and photohadronic () interactions with the disk thermal and Comptonized nonthermal background photons. It has been suggested that some fast radio bursts (FRBs) may be powered by such short-lived jetted hyper-accreting engines. Although neutrino emission associated with the ms-duration bursts themselves is challenging to detect, the persistent radio counterparts of some FRB sources -- if associated with hypernebulae -- could contribute to the high energy neutrino diffuse background flux. If the hypernebula birth rate follows that of steller-merger transients and common envelope events, we find that their volume-integrated neutrino emission -- depending on the population-averaged mass-transfer rates -- could explain up to of the high-energy diffuse neutrino flux observed by the IceCube Observatory and the Baikal-Gigaton Volume Detector (GVD) Telescope. The time-averaged neutrino spectrum from hypernebula -- depending on the population parameters -- can also reproduce the observed diffuse neutrino spectrum. The neutrino emission could in some cases furthermore extend to >100 PeV, detectable by future ultra-high-energy neutrino observatories. The large optical depth through the nebula to Breit-Wheeler () interaction attenuates the escape of GeV-PeV gamma-rays co-produced with the neutrinos, rendering these gamma-ray-faint neutrino sources, consistent with the \textit{Fermi} observations of the isotropic gamma-ray background.

    astro-ph.HEhep-exhep-phphysics.plasm-phApJ·30 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.