PaperPanorama

HEP Phenomenology·hep-ph

Mon·Jun 24, 2024

20 papers9 primary·11 cross-listed·reconstructed*

  1. 01*

    Phase transition and gravitational waves in maximally symmetric composite Higgs model

    Avik Banerjee🇮🇳 · Marco Merchand🇸🇪 · Ignacy Nałęcz🇵🇱

    In this paper we study phase transitions in a maximally symmetric composite Higgs model with next-to-minimal coset, where a pseudoscalar singlet emerges alongside the Higgs doublet. The maximal symmetry guarantees the finiteness of the radiatively generated scalar potential. We explore the scenario involving an explicit source of CP violation in the strong sector, which induces a asymmetric scalar potential, and consequently leads to nonzero vacuum expectation value for the singlet. Current experimental bounds from the LHC are imposed on the masses of the composite resonances, while the CP violating interactions of the pseudo Nambu-Goldstone bosons are tightly constrained from the measurements of the electric dipole moment of the electron. We compute the finite temperature corrections to the potential, incorporating the momentum-dependent form factors in the loop integrals to capture the effect of the strong dynamics. The impact of the resonances from the strong sector on the finite temperature potential are exponentially suppressed. The presence of explicit CP violation leads to strong first-order phase transition from a false vacuum to the electroweak vacuum where the pseudoscalar singlet has a non-zero vacuum expectation value. We illustrate that, as a result of such phase transitions, the production of potentially observable gravitational waves at future detectors will offer a complementary avenue to probe the composite Higgs models, distinct from collider experiments.

    hep-phJHEP(2024)·5 citations
  2. 02*

    Double DVCS amplitudes including kinematic twist-3 and 4 corrections

    V. Martinez-Fernandez🇵🇱 · B. Pire🇫🇷 · P. Sznajder🇵🇱 · J. Wagner🇵🇱

    Generalized parton distributions (GPDs) are off-forward matrix elements of quark and gluon operators that work as a window to the total angular momentum of partons and their transverse imaging (nucleon tomography). To access GPDs one needs to look into exclusive processes which are usually studied in a kinematic regime known as the Björken limit. In this limit, the photon virtualities are much larger than the hadron mass , and the kick to the hadron measured by the Mandelstam's variable . It turns out that this is not enough for the purposes of a precise GPD extraction and, in particular, of nucleon tomography for which measurements in a sizable range of are required. Deviation with respect to the Björken limit induces kinematic higher-twist corrections which enter the amplitudes with powers of and , where denotes the scale of the process (basically, the sum of photon virtualities in the case of DDVCS). There are also corrections by the name of "genuine" higher twists which are a separate topic and are not the subject of this research study. In this manuscript, we present novel calculations of DDVCS amplitudes off a (pseudo-)scalar target including up to kinematic twist-4 corrections. These results are important for measuring DDVCS, DVCS and TCS through the Sullivan process and off helium-4 target at the future Electron-Ion Collider (EIC) and JLab experiments. Preliminary numerical estimates for the pion target are provided.

    hep-phPoS(2025)·1 citation
  3. 03*

    Electric Conductivity of QCD Matter and Dilepton Spectra in Heavy-Ion Collisions

    Ralf Rapp🇺🇸

    The electric conductivity, , is a fundamental transport coefficient of QCD matter that can be related to the zero-energy limit of the electromagnetic (EM) spectral function at vanishing 3-momentum in the medium. The EM spectral function is also the central quantity to describe the thermal emission rates and pertinent spectra of photon and dilepton radiation in heavy-ion collisions. Employing a model for dilepton rates that combines hadronic many-body theory with nonperturbative QGP emission constrained by lattice-QCD which describes existing dilepton measurements in heavy-ion collisions, we investigate the sensitivity of low-mass dilepton spectra in Pb-Pb collisions at the LHC to . In particular, we disentangle the contributions from QGP and hadronic emission, and identify signatures that can help to extract from high-precision experimental data expected to be attainable with future detector systems at the LHC.

    hep-phnucl-exnucl-thPRC(2024)·12 citations
  4. 04*

    The meson magnetic dipole moment from BaBar cross section measurement

    Antonio Rojas🇲🇽 · Genaro Toledo🇲🇽

    We obtain the value of the magnetic dipole moment of the meson, using data from the BaBar Collaboration for the process. The considered center of mass energy range is from 0.9 to 1.8 GeV. We describe the vertex using a vector meson dominance model, including the intermediate resonant contributions relevant at these energies. We find in units. We improve on the previous extracted value, where preliminary data from the same collaboration was used, by considering definite data, better grounded values of the parameters involved and explicit gauge invariant description of the process.

    hep-phhep-exnucl-thPRD(2024)·7 citations
  5. 05*

    Pentaquark molecular states with hidden bottom and double strangeness

    Jing Song🇨🇳 · Man-Yu Duan🇨🇳 · Luis Roca🇪🇸 · Eulogio Oset🇪🇸

    We investigate the meson-baryon interaction in coupled channels with the quantum numbers of the pentaquarks and . The interaction is derived from an extension of the local hidden gauge approach to the heavy quark sector, which has demonstrated accurate results compared to experiments involving , states, and pentaquarks and . In our study, we identify several molecular states with small decay widths within the chosen set of coupled channels. The spin-parity () of these states is as follows: for pseudoscalar-baryon () coupled channels, for pseudoscalar-baryon () coupled channels, and for vector-baryon () coupled channels, and , , for vector-baryon () coupled channels. We search for the poles of these states and evaluate their couplings to the different channels.

    hep-phEPJC(2024)·7 citations
  6. 06*

    Adler function, Bjorken polarized sum rule: confirmation of elements of the -expansion and the diagrams

    S. V. Mikhailov🇷🇺

    Different ways exist to obtain the elements of the -expansion for renormgroup invariant quantities. Here we consider independent confirmation within the standard QCD of a number of our results [1] for the values of elements of this expansion for the nonsinglet Adler -function, Bjorken polarized sum rules up to the order NLO. We suggest an approach to estimate the results of high order QCD calculations using a smaller number of diagrams of the specific type. This type is based on a proposed generalization of Naive NonAbelianization.

    hep-phJHEP(2024)·3 citations
  7. 07*

    Probing light sterile neutrinos in left-right symmetric models with displaced vertices and neutrinoless double beta decay

    Jordy de Vries🇳🇱 · Herbi K. Dreiner🇩🇪 · Jelle Groot🇳🇱 · Julian Y. Günther🇩🇪 · Zeren Simon Wang🇹🇼

    An investigation of relatively light (GeV-scale), long-lived right-handed neutrinos is performed within minimal left-right symmetric models using the neutrino-extended Standard Model Effective Field Theory framework. Light sterile neutrinos can be produced through rare decays of kaons, -mesons, and -mesons at the Large Hadron Collider (LHC) and the Long-Baseline Neutrino Facility (LBNF) of Fermilab. Their decays could result in displaced vertices, which can be reconstructed. By performing Monte-Carlo simulations, we assess the sensitivities of the future LHC far-detector experiments ANUBIS, CODEX-b, FACET, FASER(2), MoEDAL-MAPP1(2), MATHUSLA, the recently approved beam-dump experiment SHiP, and the upcoming neutrino experiment DUNE at the LBNF, to the right-handed gauge-boson mass as functions of neutrino masses. We find that DUNE and SHiP could be sensitive to right-handed gauge-boson masses up to TeV. We compare this reach to indirect searches such as neutrinoless double beta decay, finding that displaced-vertex searches are very competitive.

    hep-phhep-exJHEP(2025)·16 citations
  8. 08*

    Electric and Magnetic Tau Dipole Moments Revisited

    G.A. González-Sprinberg🇺🇾

    Precise measurements of magnetic and electric dipole moments are important tests of the Standard Model and beyond Standard Model physics, particularly for the electron and the muon. However, the situation presents distinctive challenges when dealing with the tau lepton due to its very short lifetime and relatively high mass. Here, we review the theoretical predictions and experimental measurements of both the anomalous magnetic and electric dipole moments of the tau lepton. Note: Contribution to the proceedings of the 17th International Workshop on Tau Lepton Physics, Louisville, USA, 4-8 December 2023

    hep-phSciPost Phys.Proc.(2025)·1 citation
  9. 09*

    The Sensitivity of DUNE in Presence of Off-Diagonal Scalar NSI Parameters

    Arnab Sarker🇮🇳 · Dharitree Bezboruah🇮🇳 · Abinash Medhi🇮🇳 · Moon Moon Devi🇮🇳

    Scalar non-standard interactions (NSI) presents an exciting pathway for probing potential new physics that extends beyond the Standard Model (BSM). The scalar coupling of neutrinos with matter can appear as a sub-dominant effect that can impact the neutrino oscillation probabilities. The uniqueness of these interactions is that it can directly affect the neutrino mass matrix. This makes oscillations sensitive to the absolute neutrino mass. The effects of scalar NSI scales linearly with matter density which motivates its exploration in long-baseline sector. The presence of scalar NSI can influence the key measurements in the field of neutrino physics, including the precise determination of the leptonic CP phase (), neutrino mass ordering and the octant of . The precise determination of is one of the major goals of DUNE, which is an upcoming long-baseline experiment. A better understanding of the impact of scalar NSI on CP measurement sensitivities is crucial for accurate interpretation of phase. In this work, we have explored the impact of the complex off-diagonal scalar NSI elements and their associated phases on the CP-measurement sensitivities at DUNE. We have explored the impact of the neutrino mass scale on these sensitivities. We look for constraining these off-diagonal elements for different neutrino mass scales. We also explore their correlation with , investigating potential degeneracies that can arise due to additional phases. We also perform a correlation study among different scalar NSI elements. We show that the inclusion of the complex scalar NSI elements can significantly modify the CP phase measurements.

    hep-phPRD(2025)·9 citations
  10. 10*

    Comprehensive survey of hybrid equations of state in neutron star mergers and constraints on the hadron-quark phase transition

    Sebastian Blacker🇩🇪 · Andreas Bauswein🇩🇪

    We perform an extensive study of equation of state (EoS) models featuring a phase transition from hadronic to deconfined quark matter in neutron star merger simulations. We employ three different hadronic EoSs, a constant speed of sound parameterization for the quark phase and a Maxwell construction to generate a large sample of hybrid EoS models. We systematically vary the onset density and density jump of the phase transition as well as the quark matter stiffness and simulate binary neutron star mergers to infer how the properties of the phase transition affect the gravitational-wave signal. In total we simulate mergers with 245 different hybrid EoS models. In particular, we explore in which scenarios a phase transition would be detectable by a characteristically increased postmerger gravitational-wave frequency compared to an estimate from the inspiral signal assuming a purely hadronic EoS. We find that the density jump at the transition (latent heat) has the largest impact on the gravitational-wave frequencies, while the influence of the stiffness of quark matter is smaller. We quantify which range of phase transition properties would be compatible with a certain magnitude or absence of the gravitational-wave postmerger frequency shift. By means of these dependencies, a future detection will thus directly yield constraints on the allowed features of the hadron-quark phase transition.

    astro-ph.HEhep-phPRD(2025)·17 citations
  11. 11*

    Gravitational Scattering and Beyond from Extreme Mass Ratio Effective Field Theory

    Clifford Cheung🇺🇸 · Julio Parra-Martinez🇫🇷 · Ira Z. Rothstein🇺🇸 · Nabha Shah🇺🇸 · Jordan Wilson-Gerow🇺🇸

    We explore a recently proposed effective field theory describing electromagnetically or gravitationally interacting massive particles in an expansion about their mass ratio, also known as the self-force (SF) expansion. By integrating out the deviation of the heavy particle about its inertial trajectory, we obtain an effective action whose only degrees of freedom are the lighter particle together with the photon or graviton, all propagating in a Coulomb or Schwarzschild background. The 0SF dynamics are described by the usual background field method, which at 1SF is supplemented by a "recoil operator" that encodes the wobble of the heavy particle, and similarly computable corrections appearing at 2SF and higher. Our formalism exploits the fact that the analytic expressions for classical backgrounds and particle trajectories encode dynamical information to all orders in the couplings, and from them we extract multiloop integrands for perturbative scattering. As a check, we study the two-loop classical scattering of scalar particles in electromagnetism and gravity, verifying known results. We then present new calculations for the two-loop classical scattering of dyons, and of particles interacting with an additional scalar or vector field coupling directly to the lighter particle but only gravitationally to the heavier particle.

    hep-thgr-qchep-phJHEP(2024)·52 citations
  12. 12*

    Brane-Like Solutions and Other Non-Supersymmetric Vacua

    J. Mourad (APC, U. Paris Cité)🇫🇷 · S. Raucci🇮🇹 · A. Sagnotti (Scuola Normale Superiore and INFN, Pisa)🇮🇹

    After recasting the standard charged and uncharged brane profiles in the harmonic gauge, we explore solutions with the same isometries where the potentials of ten-dimensional non-supersymmetric strings are taken into account. Combining a detailed catalog of the possible asymptotics with some numerical results suggests that these spherically symmetric backgrounds terminate at singularities within finite proper distances.

    hep-thgr-qchep-phmath-ph+1JHEP(2024)·21 citations
  13. 13*

    High energy neutrino production in gamma-ray bursts: dependence of the neutrino signal on the jet composition

    Valentin De Lia🇩🇰 · Irene Tamborra🇩🇰

    Heavy nuclei can be synthetized or entrained in gamma-ray bursts (GRBs) with implications on the high-energy neutrino emission. By means of a Monte-Carlo algorithm, we model nuclear cascades and investigate their impact on the neutrino production considering kinetic dominated jets (in the internal shock model, including a dissipative photosphere) as well as Poynting flux dominated jets (for a jet model invoking internal-collision-induced magnetic reconnection and turbulence, ICMART). We find that the ICMART model allows for efficient nuclear cascades leading to an overall larger neutrino fluence than in the other two jet models. The survival of nuclei and inefficient nuclear cascades lead to an overall reduction of the neutrino fluence up to one order of magnitude. However, if nuclei are disintegrated, the neutrino fluence may be comparable to the one emitted from a jet loaded with protons. Exploring the parameter space of jet properties, we conclude that the composition and the bulk Lorentz factor have significant impact on the efficiency of nuclear cascades as well as the spectral shape of the expected neutrino fluence. On the other hand, the neutrino spectral distribution is less sensitive to the power-law index of the accelerated population of protons or heavier nuclei. For what concerns the diffuse emission of neutrinos from GRBs, we find that the uncertainty due to the jet composition can be at most comparable to the one related to the GRB cosmological rate.

    astro-ph.HEhep-phJCAP(2024)·7 citations
  14. 14*

    Non-thermal particle production in Einstein-Cartan gravity with modified Holst term and non-minimal couplings

    Tomohiro Inagaki🇯🇵 · Naoki Yoshioka🇯🇵

    Non-thermal fermionic particle production is investigated in Einstein-Cartan modified gravity with a modified Holst term and non-minimal couplings between the spin connection and a fermion. By using the auxiliary field method, the theory is rewritten into a pseudoscalar-tensor theory with Einstein-Hilbert action and canonical kinetic and potential terms for a pseudoscalar field. The introduced field is called Einstein-Cartan pseudoscalaron. If the potential energy of the Einstein-Cartan pseudoscalaron dominates the energy density of the early universe, it causes inflationary expansion. After the end of inflation, the pseudoscalaron develops a large value and the non-minimal couplings destabilize the vacuum. Evaluating the non-thermal fermionic particle production process, we obtain the mass and the helicity dependences of the produced particle number density. We show the model parameters to enhance the preheating and reheating processes.

    gr-qchep-phPRD(2024)·5 citations
  15. 15*

    He spin-dependent structure functions within the relativistic Light-Front Hamiltonian dynamics

    Eleonora Proietti🇮🇹 · Filippo Fornetti🇮🇹 · Emanuele Pace🇮🇹 · Matteo Rinaldi🇮🇹 · Giovanni Salmè🇮🇹 · Sergio Scopetta🇮🇹

    He spin-dependent structure functions, and , which parametrize the hadronic tensor in polarized deep-inelastic scattering, were evaluated within the Poincaré covariant light-front framework. The Bakamjian-Thomas construction of the Poincaré generators allows us to make use of a realistic He wave function, obtained from refined nuclear phenomenological potentials. The same approach was already successfully applied to the He and He unpolarized deep-inelastic scattering. To investigate the neutron polarized structure functions, and , a readily implementable procedure, aimed at extracting the neutron spin structure functions from those of He, is shown to hold. Moreover, the first moment of was evaluated, aiming at providing a valuable check of the Bjorken sum rule. The present analysis is relevant for experiments nvolving polarized beams planned at the future facilities, like the Electron Ion Colliders.

    nucl-thhep-phPRC(2024)·1 citation
  16. 16*

    Electromagnetic isovector form factors of the transition from the to the nucleon

    Di An🇸🇪 · Stefan Leupold🇸🇪

    Dispersion theory is used to provide a model-independent low-energy representation of the three electromagnetic isovector transition form factors . At low energies the virtual photon couples dominantly to a pion pair. Taking the very well understood pion vector form factor and pion re-scattering into consideration, the determination of the transition form factors is traced back to the determination of pion-baryon scattering amplitudes. Their low-energy aspects are parametrized by baryon exchange, accounting for the main decay channels of the . Short-distance physics is encoded in subtraction constants that are fitted to data on space-like form factors and hadronic decays. It is shown that a limitation in the determination of the subtraction constants lies in the fact that isovector form factors require sufficient information about the differences between protons and neutrons. In particular, this calls for improvements in the form factor extraction from the electroproduction of the on the neutron. Via the dispersion relations, space- and time-like regions are naturally connected from first principles. This allows to predict the time-like form factors that enter the Dalitz decays and . Under the assumption of the dominance of the isovector over the isoscalar channel, the Dalitz decay distributions are predicted.

    nucl-thhep-ph6 citations
  17. 17*

    Universality of scaled particle spectra in ultrarelativistic heavy-ion collisions

    Cicero D. Muncinelli🇧🇷 · Fernando G. Gardim🇧🇷 · David D. Chinellato🇦🇹 · Gabriel S. Denicol🇧🇷 · Andre V. Giannini🇧🇷 · Matthew Luzum🇧🇷 · Jorge Noronha🇺🇸 · Tiago Nunes da Silva🇧🇷 · Jun Takahashi🇧🇷 · Giorgio Torrieri🇧🇷

    We study the transverse momentum spectra of identified particles in ultrarelativistic collisions of large and small collision systems. In order to isolate information contained in the momentum dependence, we propose to scale the spectra by the total particle number and mean transverse momentum -- global quantities which are already well studied. We observe an interesting, nearly universal, centrality-independent shape in the scaled spectra, similar to scalings that have been studied previously. This scaling behavior breaks down at large transverse momentum and for very small systems, such as those produced in p-p collisions. We perform hybrid hydrodynamic simulations and show that, in these simulations, a centrality-independent shape is a consequence of an event-by-event independence. Our results motivate further theoretical and experimental investigations of the regime of validity of this scaling phenomenon and their physical interpretation at different collision energies and systems.

    nucl-thhep-phPRC(2025)·7 citations
  18. 18*

    Spinodal slowing down and scaling in a holographic model

    Alessio Caddeo🇪🇸 · Oscar Henriksson🇫🇮 · Carlos Hoyos🇪🇸 · Mikel Sanchez-Garitaonandia🇫🇷

    The dynamics of first-order phase transitions in strongly coupled systems are relevant in a variety of systems, from heavy ion collisions to the early universe. Holographic theories can be used to model these systems, with fluctuations usually suppressed. In this case the system can come close to a spinodal point where theory and experiments indicate that the the behaviour should be similar to a critical point of a second-order phase transition. We study this question using a simple holographic model and confirm that there is critical slowing down and scaling behaviour close to the spinodal point, with precise quantitative estimates. In addition, we determine the start of the scaling regime for the breakdown of quasistatic evolution when the temperature of a thermal bath is slowly decreased across the transition. We also extend the analysis to the dynamics of second-order phase transitions and strong crossovers.

    hep-thcond-mat.stat-mechhep-phJHEP(2024)·5 citations
  19. 19*

    Hybrid Star Properties with NJL and MFTQCD Model: A Bayesian Approach

    Milena Albino🇵🇹 · Tuhin Malik🇵🇹 · Márcio Ferreira🇵🇹 · Constança Providência🇵🇹

    The composition of the core of neutron stars (NS) is still under debate. One possibility is that because of the high densities reached in their cores, matter could be deconfined into quark matter. We investigate the existence of hybrid stars, using microscopic models to describe different phases of matter. Within the adopted microscopic models we calculate properties of NS and properties of matter. We want to probe the pQCD calculations influence and analyze properties that identify a transition to deconfined matter. Bayesian approach is applied to generate 8 sets of equations of state (EOS). A Maxwell construction is adopted to describe the deconfinement transition. For the hadron phase, we consider a stiff and a soft EOS obtained from the Relativistic Mean Field model with nonlinear meson terms. For the quark phase, we use 2 different models: the Nambu-Jona-Lasinio model with multiquark interactions and the Mean Field Theory of QCD, a model similar to the vector MIT bag model. Bayesian inference was applied to determine the model parameters that satisfy the X-ray observations from NICER and have phase transition at densities between 0.15 - 0.40 fm. We also applied restrictions from the pQCD calculations to half of the sets. Hybrid stars are compatible with current observational data. The pQCD restrictions reduce the value of the . However, even applying this restriction, the models were able to reach values of . The conformal limit was still not attained at the center of the most massive stars. The vector interactions are essential to describe hybrid stars with a mass above . The multiquark interactions introduced may affect the limits of some quantities considered as indicators of the presence of a deconfined phase. It is possible to find a set of EOS, that predict that inside NS the renormalized matter trace anomaly is always positive.

    nucl-thastro-ph.HEgr-qchep-phPRD(2024)·29 citations
  20. 20*

    Spectral evolution of RX J0440.9+4431 during the 2022-2023 giant outburst observed with Insight-HXMT

    P. P. Li🇺🇸 · Peter A. Becker · L. Tao🇨🇳

    In 2022-2023, the X-ray pulsar RX J0440.9+4431 underwent a Type II giant outburst, reaching a peak luminosity L_x ~ 4*10^{37} erg/s. In this work, we utilize Insight-HXMT data to analyze the spectral evolution of RX J0440.9+4431 during the giant outburst. By analysing the variation of the X-ray spectrum during the outburst using standard phenomenological models, we find that as the luminosity approaches the critical luminosity, the spectrum became flatter, with the photon enhancement predominantly concentrated around ~ 2 keV and 20-40 keV. The same behavior has also been noted in Type II outbursts from other sources. While the phenomenological models provide good fits to the spectrum, this approach is sometimes difficult to translate into direct insight into the details of the fundamental accretion physics. Hence we have also analyzed spectra obtained during high and low phases of the outburst using a new, recently-developed physics-based theoretical model, which allows us to study the variations of physical parameters such as temperature, density, and magnetic field strength during the outburst. Application of the theoretical model reveals that the observed spectrum is dominated by Comptonized bremsstrahlung emission emitted from the column walls in both the high and low states. We show that the spectral flattening observed at high luminosities results from a decrease in the electron temperature, combined with a compactification of the emission zone, which reduces the efficiency of bulk Comptonization. We also demonstrate that when the source is at maximum luminosity, the spectrum tends to harden around the peak of the pulse profile, and we discuss possible theoretical explanations for this behavior. We argue that the totality of the behavior in this source can be explained if the accretion column is in a quasi-critical state when at the maximum luminosity observed during the outburst.

    astro-ph.HEhep-phAstron.Astrophys.(2024)·4 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.