PaperPanorama

HEP Phenomenology·hep-ph

Mon·May 6, 2024

23 papers17 primary·6 cross-listed·reconstructed*

  1. 01*

    Electric dipole moments of charged leptons in models with pseudo-Dirac sterile fermions

    Asmaa Abada🇫🇷 · Takashi Toma🇯🇵

    In this work, we address the impact of a small lepton number violation on charged lepton electric dipole moments - EDMs. Low-scale seesaw models protected by lepton number symmetry and leading to pseudo-Dirac pairs in the neutrino heavy spectrum provide a natural explanation for the smallness of neutrino masses with potentially testable consequences. Among which, it was thought that the small mass gap in each pair of pseudo-Dirac neutrinos may induce important contribution to the charged lepton EDMs. Recently, it has been shown that the contribution from some of the Feynman diagrams to charged lepton EDMs exactly cancel by virtue of the Ward-Takahashi identity in quantum electrodynamics. We thus consider here the Standard Model minimally extended with pairs of pseudo-Dirac sterile fermions and derive the complete analytical formula at two loops for the charged lepton EDMs. In addition, we numerically evaluate the order of the predicted EDMs consistent with the experimental bounds and constraints such as neutrino oscillation data, charged lepton flavour violating processes, sterile neutrino direct searches, meson decays, sterile neutrino decays, and cosmological and astrophysical observations. We find that, in the minimal setup accommodating neutrino data (masses and mixings) with only two pseudo-Dirac pairs, the predicted electron EDM is , at most, which is much smaller than the current experimental bound and even future sensitivity. Hopefully, the electron EDM might reach future sensitivity, once extra pseudo-Dirac neutrinos are taken into account. The analytical formulae we derive are generic to any model involving pseudo-Dirac pairs in the heavy neutrino spectrum.

    hep-phhep-exJHEP(2024)·10 citations
  2. 02*

    Enhanced primordial gravitational waves from a stiff post-inflationary era due to an oscillating inflaton

    Chao Chen🇨🇳 · Konstantinos Dimopoulos🇬🇧 · Cem Eröncel🇹🇷 · Anish Ghoshal🇵🇱

    We investigate two classes of inflationary models, which lead to a stiff period after inflation that boosts the signal of primordial gravitational waves (GWs). In both families of models studied, we consider an oscillating scalar condensate, which when far away from the minimum it is overdamped by a warped kinetic term, a la -attractors. This leads to successful inflation. The oscillating condensate is in danger of becoming fragmented by resonant effects when non-linearities take over. Consequently, the stiff phase cannot be prolonged enough to enhance primordial GWs at frequencies observable in the near future for low orders of the envisaged scalar potential. However, this is not the case for a higher-order scalar potential. Indeed, we show that this case results in a boosted GW spectrum that overlaps with future observations without generating too much GW radiation to de-stabilise Big Bang Nucleosynthesis. For example, taking , we find that the GW signal can be safely enhanced up to at frequency Hz, which will be observable by the Einstein Telescope (ET). Our mechanism ends up with a characteristic GW spectrum, which if observed, can lead to the determination of the inflation energy scale, the reheating temperature and the shape (steepness) of the scalar potential around the minimum.

    hep-phastro-ph.COgr-qchep-thPRD(2024)·22 citations
  3. 03*

    Multiplicity dependence of the -spectra for charged particles and its relationship with partonic entropy

    L.S. Moriggi🇧🇷 · G.S. Ramos🇧🇷 · M.V.T. Machado🇧🇷

    We investigate the multiplicity dependence of the transverse momentum spectra of hadrons produced in high-energy collisions. We propose that the partonic distribution be parameterized by its non-extensive entropy and the parton saturation scale . These two variables can be identified from the produced charged hadron distributions and provide important information on the gluon dynamics at the moment of interaction. From this perspective we interpret data from different ALICE multiplicity classes at TeV and TeV. A multiplicity dependent scaling function is presented and the dependence of the interaction area on multiplicity is also investigated.

    hep-phhep-exPRD(2024)·10 citations
  4. 04*

    Exploring hadronic de-excitation via Lepton Flavor Violation

    Fabiola Fortuna🇲🇽 · Leonardo Esparza🇲🇽 · Genaro Toledo🇲🇽

    In this work, we consider a hadronic de-excitation mechanism via lepton flavor violation (LFV). Namely, for vector and pseudoscalar meson decays of the form and , respectively. They are described considering effective dim-5 and dim-7 operators. Using the current bounds for the effective couplings obtained from direct processes, we exhibit the different features in the dilepton invariant mass distribution and the branching ratios, depending on the effective operator. We consider hadronic states, from light mesons to quarkonia. We show that the branching ratios of quarkonia system for LFV are comparable with the estimates in other hadronic systems. Our results show that the dilepton invariant mass may be useful to constrain individual contributions and help disentangle them, when complemented with observables from nuclei.

    hep-phInt.J.Mod.Phys.A(2025)·0 citations
  5. 05*

    Excited electron production at the SPPC-based ep colliders via contact interactions

    Abdullatif Çalışkan🇹🇷

    If a linear electron accelerator is installed into the SPPC (Super Proton-Proton Collider) complex, ep collision options will be available in addition to pp collisions. We consider the production of excited electrons with spin-1/2 at the future SPPC-based electron-proton colliders with center-of-mass energies of , , and TeV. In the signal process, excited electrons are produced by contact interactions and decay into the photon channel by gauge interactions. Taking into account the corresponding background process, the pseudorapidity and transverse momentum distributions of the final state particles are plotted. We reported the discovery, observation and exclusion mass limits of excited electrons by applying appropriate kinematical cuts best suited for amplify the signal of the excited electron signature. We also investigated the highest achievable values of the compositeness scale for the discovery of excited electrons at these colliders.

    hep-phActa Phys.Polon.B(2025)·0 citations
  6. 06*

    On the (in)consistency of perturbation theory at finite temperature

    Peter Lowdon🇩🇪 · Owe Philipsen🇩🇪

    A well-known difficulty of perturbative approaches to quantum field theory at finite temperature is the necessity to address theoretical constraints that are not present in the vacuum theory. In this work, we use lattice simulations of scalar correlation functions in massive theory to analyse the extent to which these constraints affect the perturbative predictions. We find that the standard perturbative predictions deteriorate even in the absence of infrared divergences at relatively low temperatures, and that this is directly connected to the analytic structure of the propagators used in the expansion. This suggests that the incorporation of non-perturbative thermal effects in the propagators is essential for a consistent perturbative formulation of scalar quantum field theories at finite temperature. By utilising the spectral constraints imposed on finite-temperature correlation functions, we explore how these effects manifest themselves in the lattice data, and discuss why the presence of distinct thermoparticle excitations provides a potential resolution to these issues.

    hep-phhep-lathep-thnucl-thJHEP(2024)·10 citations
  7. 07*

    Muon g-2, Long-Range Muon Spin Force, and Neutrino Oscillations

    Rundong Fang🇨🇳 · Ji-Heng Guo🇨🇳 · Jia Liu🇨🇳 · Xiao-Ping Wang🇨🇳

    Recent studies have proposed using a geocentric muon spin force to account for the anomaly, with the long-range force mediator being a light axion-like particle. The mediator exhibits a CP-violating scalar coupling to nucleons and a normal derivative coupling to muons. Due to the weak symmetry, this axion inevitably couples to neutrinos, providing potential impact on neutrino oscillations. By utilizing neutrino data from BOREXINO, IceCube DeepCore, Super-Kamiokande, and SNO, we have identified that both atmospheric and solar neutrino data can impose stringent constraints on the long-range muon spin force model and the parameter space. With optimized data analysis techniques and the potential from future experiments, such as JUNO, Hyper-Kamiokande, SNO+, and IceCube PINGU, there exists a promising opportunity to achieve even greater sensitivities. Indeed, neutrino oscillations offer a robust and distinctive cross-check for the model, offering stringent constraints on the parameter space.

    hep-phPRD(2024)·3 citations
  8. 08*

    Searching for a new light gauge boson with axial couplings in muon beam dump experiments

    Pierre Fayet🇫🇷 · María Olalla Olea-Romacho🇫🇷

    We present a formalism for new interactions involving weak hypercharge, baryon, and lepton numbers, and a possible axial symmetry generator in the presence of a second Brout-Englert-Higgs doublet. The resulting boson, after mixing with the , interpolates between a generalised dark photon, a dark , and an axially coupled gauge boson. We especially focus on the axial couplings originating from or from mixing with the , determined by the scalar sector via parameters like and the v.e.v. of an extra dark singlet. We explore the distinctive features of axially coupled interactions, especially in the ultrarelativistic limit, where the boson behaves much as an axion-like particle, with enhanced interactions to quarks and leptons. This enhancement is particularly relevant for future muon beam dump experiments, since the muon mass considerably increases the effective coupling, proportional to , compared to analogous experiments with electrons. We also analyse the shape of the expected beam dump exclusion or discovery regions, influenced by boson interactions and the experiment geometry. Different situations are considered, limited in particular by cases for which the decays before reaching the detector, or has too small couplings to produce detectable events. We also compare to vectorially coupled bosons and axion-like pseudoscalars, highlighting the importance of understanding the parameter space for future experiment design and optimisation.

    hep-phJHEP(2024)·5 citations
  9. 09*

    Intriguing aspects of light baryon resonances

    K. P. Khemchandani🇧🇷 · A. Martinez Torres🇧🇷 · Sang-Ho Kim🇰🇷 · Seung-il Nam🇰🇷 · A. Hosaka🇯🇵 · H. Nagahiro🇯🇵

    We discuss that some light baryon resonances exhibit properties which cannot be described when attributing a three-valence quark structure to them. Besides pointing out the hadron resonances which clearly require description beyond the quark model, we focus on the third state and its decay to final states consisting of the lightest hyperon resonances which have a partial width comparable to that for the decay to . Such properties of the mentioned nucleon resonance get manifested in the cross sections and other observables related to processes producing the lightest hyperon resonances. We show that all these findings arise from the strong association of the baryon resonances to the dynamics among the ground-state hadrons.

    hep-phnucl-thEPJ Web Conf.(2024)·0 citations
  10. 10*

    Pseudoscalar Higgs plus jet production at Next-to-Next-to-Leading Order in QCD

    Youngjin Kim🇰🇷 · Ciaran Williams🇺🇸

    We present a calculation of pseudoscalar Higgs production in association with a jet at Next-to-Next-to Leading Order (NNLO) accuracy in QCD. We work in an effective field theory in which resulting in effective operators which couple the pseudoscalar to gluons and (massless) quarks. We have calculated all of the relevant amplitudes for the two-loop, one-loop and tree-level contributions. As a cross-check of our calculation we have re-calculated all of the scalar Higgs plus parton amplitudes and perform a detailed comparison to the literature. In order to regulate the infra-red singularities present at this order we employ the jettiness slicing method. In addition to a detailed validation of our calculation at this order we investigate LHC phenomenology for a selection of pseudoscalar Higgs masses. Our results are implemented into the parton-level Monte Carlo code MCFM.

    hep-phJHEP(2024)·4 citations
  11. 11*

    Unitarity in the non-relativistic regime and implications for dark matter

    Marcos M. Flores🇫🇷 · Kalliopi Petraki🇫🇷

    Unitarity sets upper limits on partial-wave elastic and inelastic cross-sections, which are often violated by perturbative computations. We discuss the dynamics underlying these limits in the non-relativistic regime, namely long-range interactions, and show how the resummation of the 2-particle-irreducible diagrams arising from squaring inelastic processes unitarizes both elastic and inelastic cross-sections. We provide a simple prescription to obtain the unitarized cross-sections from those that do not include resummation of the squared inelastic processes. Our results are model-independent, apply to all partial waves, and affect elastic and inelastic cross-sections, with extensive implications for new physics scenarios, such as dark-matter freeze-out, indirect detection and self-interactions.

    hep-phastro-ph.COhep-thPLB(2024)·17 citations
  12. 12*

    QCD analysis of valence structure functions using deep inelastic lepton-nucleon scattering

    Javad Shahrzad🇮🇷 · Ali Khorramian🇮🇷

    A new '''' non-singlet QCD analysis of the structure functions at the NNLO approximation is performed, utilizing the global fit of the data from various charged lepton scattering experiments. We extract the valence parton distribution functions (PDFs) and provide a parametrization of them, along with the correlated errors for a wide range of and . We compare valence PDFs and their uncertainties with those from different PDF sets provided by various groups. We also obtain valence PDFs and the strong coupling constant , taking into account the nuclear correction concerning large as well as the target mass correction (TMC) and higher twist (HT) effects at the NNLO. In the large region, we extract the higher twist contributions of , , and . We determine without and with considering the TMC and HT corrections and perform a comparison with the world average of and other reported results. The extracted results concerning valence PDFs with their uncertainties and value agree with available theoretical models.

    hep-phhep-exPRD(2024)·1 citation
  13. 13*

    Is holographic quark-gluon plasma homogeneous?

    Tuna Demircik🇵🇱 · Niko Jokela🇫🇮 · Matti Jarvinen🇰🇷 · Aleksi Piispa🇫🇮

    We present evidence for a spatially modulated instability within the deconfined quark-gluon plasma phase of QCD. This evidence is based on robust predictions from generic holographic models, accurately fitted to lattice data, where the instability is driven by the Chern-Simons term mandated by the flavor anomalies of QCD. Such an instability occurs universally across holographic models at surprisingly low densities, within the crossover region amenable to lattice and experimental studies, therefore inviting further explorations of inhomogeneous phases in this region.

    hep-phhep-lathep-thPRD(2026)·13 citations
  14. 14*

    Dark Kinetic Heating of Exoplanets and Brown Dwarfs

    Javier F. Acevedo🇺🇸 · Rebecca K. Leane🇺🇸 · Aidan J. Reilly🇺🇸

    Dark kinetic heating of neutron stars has been previously studied as a promising dark matter detection avenue. Kinetic heating occurs when dark matter is sped up to relativistic speeds in the gravitational well of high-escape velocity objects, and deposits kinetic energy after becoming captured by the object, thereby increasing its temperature. We show that dark kinetic heating can be significant even in objects with low-escape velocities, such as exoplanets and brown dwarfs, increasing the discovery potential of such searches. This can occur if there is a long-range dark force, creating a "dark escape velocity", leading to heating rates substantially larger than those expected from neutron stars. We consequently set constraints on dark sector parameters using Wide-field Infrared Survey Explorer and JWST data on Super-Jupiter WISE 0855-0714, and map out future sensitivity to the dark matter scattering cross section below . We compare dark kinetic heating rates of other lower escape velocity objects such as the Earth, Sun, and white dwarfs, finding complementary kinetic heating signals are possible depending on particle physics parameters.

    hep-phastro-ph.EPastro-ph.HEastro-ph.SRJHEP(2025)·15 citations
  15. 15*

    Probing protoneutron stars with gamma-ray axionscopes

    Alessandro Lella🇮🇹 · Francesca Calore🇫🇷 · Pierluca Carenza🇸🇪 · Christopher Eckner🇫🇷 · Maurizio Giannotti🇪🇸 · Giuseppe Lucente🇮🇹 · Alessandro Mirizzi🇮🇹

    Axion-like particles (ALPs) coupled to nucleons can be efficiently produced in the interior of protoneutron stars (PNS) during supernova (SN) explosions. If these ALPs are also coupled to photons they can convert into gamma rays in the Galactic magnetic field. This SN-induced gamma-ray burst can be observable by gamma-ray telescopes like -LAT if the SN is in the field of view of the detector. We show that the observable gamma-ray spectrum is sensitive to the production processes in the SN core. In particular, if the nucleon-nucleon bremsstrahlung is the dominant axion production channel, one expects a thermal spectrum with average energy MeV. In this case the gamma-ray spectrum observation allows for the reconstruction of the PNS temperature. In case of a sizable pion abundance in the SN core, one expects a second spectral component peaked at MeV due to axion pionic processes. We demonstrate that, through a dedicated LAT analysis, we can detect the presence of this pionic contribution, showing that the detection of the spectral shape of the gamma-ray signal represents a unique probe of the pion abundance in the PNS.

    hep-phastro-ph.HEJCAP(2024)·26 citations
  16. 16*

    Fast and Accurate Algorithm for Calculating Long-Baseline Neutrino Oscillation Probabilities with Matter Effects: NuFast

    Peter B. Denton🇺🇸 · Stephen J. Parke🇺🇸

    Neutrino oscillation experiments will be entering the precision era in the next decade with the advent of high statistics experiments like DUNE, HK, and JUNO. Correctly estimating the confidence intervals from data for the oscillation parameters requires very large Monte Carlo data sets involving calculating the oscillation probabilities in matter many, many times. In this paper, we leverage past work to present a new, fast, precise technique for calculating neutrino oscillation probabilities in matter optimized for long-baseline neutrino oscillations in the Earth's crust including both accelerator and reactor experiments. For ease of use by theorists and experimentalists, we provide fast c++ and fortran codes.

    hep-phhep-exPRD(2024)·12 citations
  17. 17*

    Electroweak Axion Portal to Dark Matter

    Stephanie Allen🇺🇸 · Albany Blackburn🇺🇸 · Oswaldo Cardenas🇺🇸 · Zoe Messenger🇺🇸 · Ngan H. Nguyen🇺🇸 · Brian Shuve🇺🇸

    Axion-like particles (ALPs) are good candidates for mediators to the dark sector. We explore scenarios in which an ALP mediates interactions between dark matter and electroweak gauge bosons. These models yield testable electromagnetic signals in astrophysical, cosmological, and terrestrial probes. We find promising prospects for both indirect detection and accelerator tests, with interesting parameter space already constrained by current experiments. Our work provides concrete benchmarks for future tests of the electroweak ALP portal.

    hep-phPRD(2024)·18 citations
  18. 18*

    Ab initio calculation of hyper-neutron matter

    Hui Tong🇩🇪 · Serdar Elhatisari🇹🇷 · Ulf-G. Meißner🇩🇪

    The equation of state (EoS) of neutron matter plays a decisive role in our understanding of the properties of neutron stars as well as the generation of gravitational waves in neutron star mergers. At sufficient densities, it is known that the appearance of hyperons generally softens the EoS, thus leading to a reduction in the maximum mass of neutron stars well below the observed values of about 2 solar masses. Even though repulsive three-body forces are known to solve this so-called "hyperon puzzle", so far performing \textit{ab initio} calculations with a substantial number of hyperons has remained elusive. In this work, we address this challenge by employing simulations based on Nuclear Lattice Effective Field Theory with up to 232 neutrons (pure neutron matter) and up to 116 hyperons (hyper-neutron matter) in a finite volume. We introduce a novel auxiliary field quantum Monte Carlo algorithm, allowing us to simulate for both pure neutron matter and hyper-neutron matter systems up to 5 times the density of nuclear matter using a single auxiliary field without any sign oscillations. Also, for the first time in {\em ab initio} calculations, we not only include two-body and three-body forces, but also and interactions. Consequently, we determine essential astrophysical quantities such as the mass-radius relation, the speed of sound and the tidal deformability of neutron stars. Our findings also confirm the existence of the -Love- relation, which gives access to the moment of inertia of the neutron star.

    nucl-thastro-ph.HEastro-ph.SRgr-qc+2Sci.Bull.(2025)·31 citations
  19. 19*

    Bubble wall velocity and gravitational wave in the minimal left-right symmetric model

    Dian-Wei Wang🇨🇳 · Qi-Shu Yan🇨🇳 · Mei Huang🇨🇳

    The bubble wall velocity in the first order phase transition plays an important role in determining both the amplitude and the pivot frequency of stochastic gravitational wave background. In the framework of the minimal left-right symmetric model, we study the wall velocity when the first order phase transition can occur. The wall velocity can be determined by matching the distribution functions in the free particle approximation and the local thermal equilibrium approximation. It is found that the wall velocity can be determined in the range for the parameter space with the first order phase transition. It is also found that for the case when the wall velocity is close to the speed of sound, the peak amplitude of gravitational wave spectrum can be larger than that in the runaway case. Moreover, It is also found that there exists an approximate power law between the wall velocity and pressure difference between broken and symmetry phases, and the power index is equal to 0.41 or so.

    gr-qcastro-ph.COhep-phPRD(2024)·15 citations
  20. 20*

    Relic gravitons and non-stationary processes

    Massimo Giovannini🇨🇭

    Stationary processes do not accurately describe the diffuse backgrounds of relic gravitons whose correlations are homogeneous in space (i.e. only dependent upon the distance between the two spatial locations) but not in time. The symmetries of the autocorrelations ultimately reflect the quantum mechanical origin of the diffuse backgrounds and lead to non-stationary observables at late time. In particular, large oscillations are believed to arise in the spectral energy density that is customarily (but approximately) related to the tensor power spectrum. When the full expression of the spectral energy density is employed the amplitudes of oscillation are instead suppressed in the large-scale limit and the non-stationary features of the late-time signal practically disappear. For similar reasons the relations between the spectral energy density and the spectral amplitude are ambiguous in the presence of non-stationary features. While it is debatable if the non-stationary features are (or will be) directly detectable, we argue that the spectral amplitude following from the Wiener-Khintchine theorem is generally inappropriate for a consistent description of the relic signal. Nevertheless the strong oscillatory behaviour of the late-time observables is naturally smeared out provided the spectral energy density is selected as pivotal variable.

    gr-qcastro-ph.COhep-phhep-thJCAP(2024)·3 citations
  21. 21*

    Lectures on Resurgence in Integrable Field Theories

    Marco Serone🇮🇹

    There has been recently considerable progress in understanding the nature of perturbation theory in UV free and gapped integrable field theories with renormalon singularities. Thanks to Bethe ansatz and large techniques, non-perturbative corrections can also be computed and lead to the reconstruction of the trans-series for the free energy in presence of a chemical potential. This is an ideal arena to test resurgence in QFT and determine if and how the exact result can be reconstructed from the knowledge of the perturbative series only. In these notes we give a pedagogical introduction to this subject starting from the basics. In the first lecture we give an overview of applications in QFT of Borel resummations before the advent of resurgence. The second lecture introduces the key concepts of resurgence and finally in the third lecture we discuss a specific application in the context of the principal chiral field model. Extended version of three lectures given at IHES and review talks given at Les Diablerets and Mainz, in 2023.

    hep-thhep-lathep-ph14 citations
  22. 22*

    Flow harmonic correlations via multi-particle symmetric and asymmetric cumulants in Au+Au collisions at \(\sqrt{s_{NN}}\) = 200 GeV

    Kaiser Shafi🇮🇳 · Prabhupada Dixit🇮🇳 · Sandeep Chatterjee🇮🇳 · Md. Nasim🇮🇳

    We study multi-particle azimuthal correlations in Au+Au collisions at = 200 GeV. We use initial conditions obtained from a Monte-Carlo Glauber model and evolve them within a viscous relativistic hydrodynamics framework that eventually gives way to a transport model in the late hadronic stage of the evolution. We compute the multi-particle symmetric and asymmetric cumulants and present the results for their sensitivity to the shear and bulk viscosities during the hydrodynamic evolution. We also check their sensitivity to resonance decay and hadronic interactions. We demonstrate that while some of these observables are more sensitive to transport properties than traditional flow observables, others are less sensitive, making them suitable for studying different stages of the evolution.

    nucl-thhep-phnucl-exPRC·1 citation
  23. 23*

    Refining holographic models of the quark-gluon plasma

    Niko Jokela🇫🇮 · Matti Järvinen🇰🇷 · Aleksi Piispa🇫🇮

    We investigate quark-gluon plasma at nonzero density by using two holographic models for QCD based on either brane or Einstein-Maxwell-dilaton actions. We determine the parameters of these models through a systematic statistical fitting procedure to lattice QCD data, which encompasses the equation of state (through the entropy density) and the two lowest baryon number susceptibilities. The predictions from the two models for the higher-order susceptibilities and the equation of state at nonzero density are strikingly similar. In particular, both models suggest the presence of a critical point on the -phase diagram near . The results for the equation of state are in agreement with lattice data for higher-order susceptibilities and experimental data for the cumulants of the net-proton number from the Beam Energy Scan program at the Relativistic Heavy-Ion Collider.

    hep-thhep-phPRD(2024)·34 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.