PaperPanorama

HEP Phenomenology·hep-ph

Fri·Mar 29, 2024

21 papers14 primary·7 cross-listed·reconstructed*

  1. 01*

    Stau pairs from natural SUSY at high luminosity LHC

    Howard Baer🇺🇸 · Vernon Barger🇺🇸 · Kairui Zhang🇺🇸

    Natural supersymmetry (SUSY) with light higgsinos is perhaps the most plausible of all weak scale SUSY models while a variety of motivations point to (right) tau sleptons as the lightest of all the sleptons. We examine a SUSY model line with rather light right-staus embedded within natural SUSY. For light stau_1 of a few hundred GeV, then the decays stau_1 -> \tau\tchi_{1,2}^0 and \nu_\tau\tchi_1^- occur at comparable rates where the (higgsino-like) \tchi_1^\pm and \tchi_2^0 release only small visible energy: in this case, the expected \tau^+\tau^- +\eslt signature is diminished from usual expectations due to the presence of the nearly invisible decay mode \ttau_1 -> \nu_\tau\tchi_1^-. However, once m_{\ttau_1}> ~m(bino), then decays to binos such as \ttau_1 -> \tau\tchi_3^0 open up where \tchi_3^0 decays to higgsinos plus W^\pm, Z^0 and h at comparable rates. For these heavier staus, then stau pair production gives rise to diboson+\eslt events which may contain 0, 1 or 2 additional hard \tau leptons. From these considerations, we examine the potential for future discovery of tau-slepton pair production at high-luminosity LHC. While we do not find a 5\sigma HL-LHC discovery reach for 3000 fb^{-1}, we do find a 95\% CL exclusion reach, ranging between m_{\ttau_1}:100-450 GeV for m_{\tchi_1^0}~ 100 GeV. This latter reach disappears for m_{\tchi_1^0}>~ 200 GeV.

    hep-phPRD(2024)·6 citations
  2. 02*

    Analysis of data on decays into two light vector mesons

    Roy Aleksan🇫🇷 · Luis Oliver🇫🇷

    An important experimental effort has been accomplished in recent years in the measurement of rates, polarization and CP observables in decays into two light vector mesons. On the theoretical side, after a very consistent effort done within the framework of QCD Factorization, the comparison of the theory with the present experimental data has not been updated, to our knowledge. In the present paper we compare this wealth of data to the theory, in tree color-allowed, tree color-suppressed and pure penguin decays, and present predictions for the observables that have not yet been measured in these decays. In our fits we find acceptable values of for the branching ratios and for the direct CP asymmetries. However, this is not the case for the longitudinal polarization fractions, essentially due to disagreement between theory and experiment for the modes and . Although we rely on previous work by other authors, we summarize the formalism so that the paper is self-contained and its results can be checked.

    hep-ph1 citation
  3. 03*

    Note on Klein-Nishina effect in strong-field QED: the case of nonlinear Compton scattering

    Uwe Hernandez Acosta🇩🇪 · Burkhard Kämpfer🇩🇪

    Suitably normalized differential probabilities of one-photon emission in external electromagnetic fields are compared to quantify the transit of nonlinear Compton scattering to linear Compton scattering, described by the Klein-Nishina formula, and to constant crossed field treatment. The known Klein-Nishina suppression at large energies is further enforced by increasing field intensity. In view of the Ritus-Narozhny conjecture, we demonstrate that different paths in the field intensity vs. energy plane towards large values of the quantum non-linearity parameter facilitate significantly different asymptotic dependencies, both in the Klein-Nishina regime and the constant crossed field regime and in between.

    hep-phEur.Phys.J.D(2025)·0 citations
  4. 04*

    Introducing scalar leptoquarks into a 3-3-1 model to solve the puzzle

    A. Doff🇧🇷 · C. A. de S. Pires🇧🇷

    In this work we introduce scalar leptoquarks into the 3-3-1 model with right-handed neutrinos with the aim of solving the puzzle. We show that besides the model supports leptoquarks in the octet, sextet, triplet and singlet representations, we identified that only one specif leptoquark in the singlet representation leads to flip of chirality as required to generate positive and robust contribution to the . Then we calculate its contributions to and to the decay process and discuss the results.

    hep-phPLB(2024)·5 citations
  5. 05*

    Running Coupling and Running Quark Mass Effects on the Elastic Form Factors of Nucleons

    Bao-Yi Yang🇨🇳 · Hui-Hua Zhong🇨🇳 · Muyang Chen🇨🇳

    We study the elastic electric and magnetic form factors of the proton, neutron and the charged roper resonance (, , , , and ) systematically in a constituent quark model. Three ingredients are crucial in this study: i) the mixing between the pure S-wave and other components which produces a nonzero neutron electric form factor. ii) a running coupling constant that soften the form factors. iii) the running quark mass function, , which is responsible for the decreasing of the as increases. The produced elastic form factors of the proton and neutron match the corresponding observed values fairly well. Our study shows that upto . We give predictions on the elastic form factors of the roper resonance, the electric charge and the magnetic momentum radius ratios of the roper resonance to the proton are .

    hep-phhep-th0 citations
  6. 06*

    Impact of JLab data on the determination of GPDs at zero skewness and new insights from transition form factors

    The MMGPDs Collaboration · Muhammad Goharipour · Hadi Hashamipour · Fatemeh Irani · K. Azizi

    It is well established now that the generalized parton distributions (GPDs) at zero skewness are playing important roles in some physical process such as elastic electron-nucleon scattering, elastic (anti)neutrino-nucleon scattering, and wide-angle Compton scattering (WACS) via various types of form factors (FFs). In this study, we are going to utilize the recent JLab measurements of the elastic electron-nucleon scattering reduced cross-section, namely GMp12, as a touchstone to unravel the tension observed between the measurements of the WACS cross-section and the data of the proton magnetic FF . We also investigate the impact of GMp12 data on valence unpolarized GPDs and at zero skewness by performing some analyses of the related experimental data. By calculating the electric and scalar quadrupole ratios, and , and magnetic transition FF related to the nucleon-to-delta () transition using the extracted GPDs and comparing the results with corresponding experimental measurements, we show that our results are in an excellent consistency with experiments, indicating the universality property of GPDs. We emphasize that the inclusion of these data in the future analysis of GPDs can significantly affect the extracted GPDs especially their uncertainties at smaller values of .

    hep-phhep-exPRD(2024)·19 citations
  7. 07*

    Gaussian Formalism: Joint Measurement for Heisenberg's Uncertainty Relation for Errors by Squeezed Coherent States

    Kin-ya Oda🇯🇵 · Naoya Ogawa🇯🇵

    We point out that the Gaussian wave-packet formalism can serve as a concrete realization of the joint measurement of position and momentum, which is an essential element in understanding Heisenberg's original philosophy of the uncertainty principle, in line with the universal framework of error, disturbance, and their uncertainty relations developed by Lee and Tsutsui. We show that our joint measurement in the Gaussian phase space, being a Positive-Operator-Valued-Measure (POVM) measurement, smoothly interpolates between the projective measurements of position and momentum. We, for the first time, have obtained the Lee-Tsutsui (LT) error and the refined Lee error for the position-momentum measurement. We find that the LT uncertainty relation becomes trivial, 0 = 0, in the limiting case of projective measurement of either position or momentum. Remarkably, in contrast to the LT relation, the refined Lee uncertainty relation, which assesses errors for local representability, provides a constant lower bound unaffected by these limits and is invariably saturated, for a pure Gaussian initial state. The obtained lower bound is in agreement with Heisenberg's value.

    hep-phgr-qchep-thquant-phPTEP(2025)·1 citation
  8. 08*

    A partitioned dipole-antenna shower with improved transverse recoil

    Christian T Preuss🇩🇪

    The implementation of a new final-state parton-shower algorithm in the Pythia event generator is described. The shower algorithm, dubbed Apollo, combines central aspects of the Vincia antenna shower with the global transverse-recoil scheme of the Alaric framework in order to achieve formal consistency with next-to-leading logarithmic (NLL) resummation. The shower algorithm is constructed in such a way that it facilitates a straightforward combination with fixed-order calculations. As an explicit proof of concept, a general scheme for matrix-element corrections (MECs) and two separate multiplicative next-to-leading order (NLO) matching schemes are outlined. It is argued that both matching schemes retain the logarithmic accuracy of the shower. The improved modelling of radiation is examined by contrasting the new algorithm with existing leading-logarithmic parton showers in Pythia.

    hep-phhep-exJHEP(2024)·46 citations
  9. 09*

    Comment on "Do near-threshold molecular states mix with neighboring states?"

    George Rupp🇵🇹

    I comment on a paper by Christoph Hanhart and Alexey Nefediev, published in Phys. Rev. D 106, 114003 (2022). The authors discuss the interpretation of mesons close to their lowest decay threshold and present a mechanism for the formation of molecular states. The proposed formalism is then applied to the axial-vector mesons and , presenting two scenarios for the lighter meson, namely a molecule or a compact state. The authors argue that the latter hypothesis requires a fine-tuning of the mixing angle between the and -parity eigenstates. In this Comment I show that no such fine-tuning is needed, as demonstrated in an article published in Phys. Rev. D 84, 094020 (2011), where a unitarized quark model was applied to the two -parity eigenstates, coupled to several two-meson channels including . The coupled-channel dynamics naturally leads to a mixing angle very close to the required one. Moreover, I argue that the and axial-vectors, not considered by the authors, as well as a lattice simulation in Phys. Rev. D 90, 034510 (2014), also not mentioned by the authors, do not lend support to a molecular interpretation of the . I conclude with some more general remarks about mesons coupling to -wave thresholds.

    hep-phhep-lat0 citations
  10. 10*

    Implications of purity constraints on light higgsinos

    Stephen P. Martin🇺🇸

    The lightest supersymmetric particles could be higgsinos that have a small mixing with gauginos. If the lightest higgsino-like state makes up some or all of the dark matter with a thermal freezeout density, then its mass must be between about 100 and 1150 GeV, and dark matter searches put bounds on the amount of gaugino contamination that it can have. Motivated by the generally good agreement of flavor- and CP-violating observables with Standard Model predictions, I consider models in which the scalar particles of minimal supersymmetry are heavy enough to be essentially decoupled, except for the 125 GeV Higgs boson. I survey the resulting purity constraints as lower bounds on the gaugino masses and upper bounds on the higgsino mass splittings. I also discuss the mild excesses in recent soft lepton searches for charginos and neutralinos at the LHC, and show that they can be accommodated in these models if is small and is negative.

    hep-phPRD(2024)·26 citations
  11. 11*

    Angular dependence in transverse momentum dependent diffractive parton distributions at small-

    Yoshitaka Hatta🇺🇸 · Feng Yuan🇺🇸

    We discuss the angular dependence of the recently proposed transverse momentum dependent quark and gluon diffractive parton distributions at small-. We introduce the difractive versions of the Sivers function and the elliptic gluon Wigner distribution and evaluate them in simple models with gluon saturation and study their geometric scaling properties. We also show that the diffractive version of the linearly polarized gluon distribution identically vanishes to leading order. These distributions enrich the physics opportunities for measuring semi-inclsuive diffractive DIS processes at the future electron-ion colliders.

    hep-phhep-exnucl-exnucl-thPLB(2024)·14 citations
  12. 12*

    Detecting Light Dark Matter with Kinetic Inductance Detectors

    Jiansong Gao🇨🇳 · Yonit Hochberg🇮🇱 · Benjamin V. Lehmann🇺🇸 · Sae Woo Nam🇰🇷 · Paul Szypryt · Michael R. Vissers · Tao Xu🇺🇸

    Superconducting detectors are a promising technology for probing dark matter at extremely low masses, where dark matter interactions are currently unconstrained. Realizing the potential of such detectors requires new readout technologies to achieve the lowest possible thresholds for deposited energy. Here we perform a prototype search for dark matter--electron interactions with kinetic inductance detectors (KIDs), a class of superconducting detector originally designed for infrared astronomy applications. We demonstrate that existing KIDs can achieve effective thresholds as low as 0.2 eV, and we use existing data to set new dark matter constraints. The relative maturity of the technology underlying KIDs means that this platform can be scaled significantly with existing tools, enabling powerful new searches in the coming years.

    hep-phhep-exphysics.ins-det14 citations
  13. 13*

    A computation of two-loop six-point Feynman integrals in dimensional regularization

    Johannes M. Henn🇩🇪 · Antonela Matijašić🇩🇪 · Julian Miczajka🇩🇪 · Tiziano Peraro🇮🇹 · Yingxuan Xu🇩🇪 · Yang Zhang🇨🇳

    We compute three families of two-loop six-point massless Feynman integrals in dimensional regularization, namely the double-box, the pentagon-triangle, and the hegaxon-bubble family. This constitutes the first analytic computation of two-loop master integrals with eight scales. We use the method of canonical differential equations. We describe the corresponding integral basis with uniform transcendentality, the relevant function alphabet, and analytic boundary values at a particular point in the Euclidean region up to the fourth order in the regularization parameter . The results are expressed as one-fold integrals over classical polylogarithms suitable for fast and high-precision evaluation.

    hep-phhep-thJHEP(2024)·34 citations
  14. 14*

    Confronting CP symmetry of order 4 with experimental data

    Igor P. Ivanov🇨🇳 · Duanyang Zhao🇨🇳

    CP4 3HDM is a three-Higgs-doublet model based on a symmetry of order 4 (CP4). It is the minimal model incorporating CP4 without leading to accidental symmetries or running into immediate conflict with experiment. Imposing CP4 on the lagrangian induces remarkably tight connections between the scalar and Yukawa sectors, including the unavoidable tree-level flavor-changing neutral couplings (FCNC). Here, we explore whether it is at all possible in the CP4 3HDM to suppressed FCNC to a level compatible with the neutral meson oscillation constraints. We express the FCNC matrices in terms of physical quark observables and quark rotation parameters, and scan the Yukawa parameter space using the quark masses and mixing parameters as input. With this procedure, we find that only two out of the eight possible CP4 Yukawa sectors are compatible with the , , and, in particular, -meson oscillation constraints. The results clearly indicate a way how to construct phenomenologically viable benchmark CP4 3HDMs.

    hep-phPoS(2024)·0 citations
  15. 15*

    Constraints on Primordial Black Holes from -body simulations of the Eridanus II Stellar Cluster

    Julia Monika Koulen🇺🇸 · Stefano Profumo🇺🇸 · Nolan Smyth🇺🇸

    The evolution of old, compact stellar structures provides strong constraints on macroscopic dark matter candidates such as primordial black holes. In view of recent observational data for the Eridanus II dwarf galaxy, we perform the first -body simulations of its central stellar cluster to model dynamical heating by PBHs. We find evidence that such candidates must be lighter than about one solar mass if they constitute the totality of the dark matter. We additionally derive constraints on the fraction of the dark matter in macroscopic objects as a function of mass, by modeling the remainder of the dark matter as standard, fluid-like cold dark matter.

    astro-ph.COhep-phPRD(2026)·11 citations
  16. 16*

    Cosmic Neutrino Decoupling and its Observable Imprints: Insights from Entropic-Dual Transport

    J. Richard Bond🇨🇦 · George M. Fuller🇺🇸 · Evan Grohs🇺🇸 · Joel Meyers🇺🇸 · Matthew James Wilson🇩🇪

    Very different processes characterize the decoupling of neutrinos to form the cosmic neutrino background (CB) and the much later decoupling of photons from thermal equilibrium to form the cosmic microwave background (CMB). The CB emerges from the fuzzy, energy-dependent neutrinosphere and encodes the physics operating in the early universe in the temperature range to . This is the epoch where beyond Standard Model (BSM) physics may be influential in setting the light element abundances and the necessarily distorted fossil neutrino energy spectra. Here we use techniques honed in extensive CMB studies to analyze the CB as calculated in detailed neutrino energy transport and nuclear reaction simulations. Our moment method, relative entropy, and differential visibility approach can leverage future high precision CMB and primordial abundance measurements to provide new insights into the CB and any BSM physics it encodes. We demonstrate that the evolution of the energy spectrum of the CB throughout the weak decoupling epoch is accurately captured in the Standard Model by only three parameters per species, a non-trivial conclusion given the deviation from thermal equilibrium. Furthermore, we can interpret each of the three parameters as physical characteristics of a non-equilibrium system. The success of our compact description within the Standard Model motivates its use also in BSM scenarios. We demonstrate how observations of primordial light element abundances can be used to place constraints on the CB energy spectrum, deriving response functions that can be applied for general CB spectral distortions. Combined with the description of those deviations that we develop here, our methods provide a convenient and powerful framework to constrain the impact of BSM physics on the CB.

    astro-ph.COhep-phhep-thJCAP(2024)·7 citations
  17. 17*

    Extended Nambu--Jona-Lasinio model for quark and nuclear matters

    Gaoqing Cao🇨🇳

    In this work, we extend the two-flavor Nambu--Jona-Lasinio model to one capable of exploring quark and nuclear matter consistently. With an extra term standing for quark-nucleon interactions, nucleons could automatically emerge as color-singlet three-quark entities by following a process similar to mesons. Besides the quark part in mean field approximation, both mesons and nucleons could contribute to the thermodynamic potential thus possibly give rise to quarkyonic matter beyond mean field. In the study, two kinds of "confining" couplings are adopted for the new interaction term and two different quark masses are considered for comparison. It turns out that only confined nuclear matter or deconfined quark matter is possible for all the cases at zero temperature, thus quarkyonic matter is not favored at all. Even more strictly, only the case with stronger confinement effect and a smaller quark mass admits a physical first-order phase transition from nuclear matter to quark matter around twice saturation density.

    nucl-thcond-mat.supr-conhep-phPLB(2025)·2 citations
  18. 18*

    Polyadic sigma matrices

    Steven Duplij (University of Münster)🇩🇪

    We generalize -matrices to higher arities using the polyadization procedure proposed by the author. We build the nonderived -ary version of using cyclic shift block matrices. We define a new function, the polyadic trace, which has an additivity property analogous to the ordinary trace for block diagonal matrices and which can be used to build the corresponding invariants. The elementary -matrices introduced here play a role similar to ordinary matrix units, and their sums are full -matrices which can be treated as a polyadic analog of -matrices. The presentation of -ary in terms of full -matrices is done using the Hadamard product. We then generalize the Pauli group in two ways: for the binary case we introduce the extended phase shifted -matrices with multipliers in cyclic groups of order (), and for the polyadic case we construct the correspondent finite -ary semigroup of phase-shifted elementary -matrices of order , and the finite -ary group of phase-shifted full -matrices of order . Finally, we introduce the finite -ary group of heterogeneous full -matrices of order . Some examples of the lowest arities are presented.

    math.GRhep-phhep-thmath-ph+2J.Math.Phys.(2024)·1 citation
  19. 19*

    Spin couplings as witnesses of Planck scale phenomenology

    Pasquale Bosso🇮🇹 · Fabrizio Illuminati🇮🇹 · Luciano Petruzziello🇮🇹 · Fabian Wagner🇮🇹

    Modified dispersion relations (MDRs) and noncommutative geometries are phenomenological models of Planck-scale corrections to relativistic kinematics, motivated by several approaches to quantum gravity. High-energy astrophysical observations, while commonly used to test such effects, are limited by significant systematic uncertainties. In contrast, low-energy, nonrelativistic experiments provide greater control, with precision serving as an amplifier for Planck-suppressed corrections. We derive corrections to Pauli's equation for nonrelativistic spin-1/2 particles in a magnetic field, incorporating general MDRs and noncommutative geometries. Applying our framework to k-Poincaré symmetries and minimal-length quantum mechanics, we identify Planck-scale corrections accessible in the nonrelativistic regime. Using the electron's anomalous magnetic moment, we constrain model parameters, pushing the k-Poincaré scale in the bi-crossproduct representation beyond GeV. These results highlight the complementarity of low-energy precision tests and astrophysical observation in probing quantum gravity phenomenology.

    hep-thhep-phEPJC(2025)·1 citation
  20. 20*

    A search for super-imposed oscillations to the primordial power spectrum in Planck and SPT-3G 2018 data

    Akhil Antony🇰🇷 · Fabio Finelli🇮🇹 · Dhiraj Kumar Hazra🇮🇹 · Daniela Paoletti🇮🇹 · Arman Shafieloo🇰🇷

    We search for super-imposed oscillations linearly or logarithmically spaced in Fourier wavenumbers in Planck and South Pole Telescope (SPT-3G) 2018 temperature and polarization data. The SPT-3G temperature and polarization data provide a new window to test these oscillations at high multipoles beyond the Planck angular resolution and sensitivity. We consider linear and logarithmic oscillations with a constant amplitude, or with a power-law dependence or a Gaussian modulation, always in . These models correspond to three, four and five additional parameters beyond power-law primordial power spectrum for the templates considered, respectively. We find that each of the five models considered can provide an improved fit to Planck data, consistently with previous findings, and to SPT-3G data, always compared to power-law power spectrum. We find tighter constraints on the amplitude of the super-imposed oscillations from the combined Planck/SPT-3G data set than in each individual data sets. For linear oscillations, with the amplitude allowed to vary as a power-law in , as in the case of EFT, we find that the addition of SPT-3G data sets tighter constraints on the possibility that the amplitude increase at small scales. When the ranges of parameters which provide a better fit to Planck and SPT-3G data overlap, as in the case of Gaussian modulated oscillations, we find a larger for logarithmic (linear) oscillations - in a combined Planck/SPT-3G data set than in each individual data sets. These findings will be further tested with upcoming CMB temperature and polarization measurements at high multipoles provided by ongoing ground experiments.

    astro-ph.COhep-phhep-thJCAP(2026)·15 citations
  21. 21*

    More on Black Holes Perceiving the Dark Dimension

    Luis A. Anchordoqui🇺🇸 · Ignatios Antoniadis🇫🇷 · Dieter Lust🇩🇪

    In the last two years the dark dimension scenario has emerged as focal point of many research interests. In particular, it functions as a stepping stone to address the cosmological hierarchy problem and provides a colosseum for dark matter contenders. We reexamine the possibility that primordial black holes (PBHs) perceiving the dark dimension could constitute all of the dark matter in the universe. We re-assess limits on the abundance of PBHs as dark matter candidates from -ray emission resulting from Hawking evaporation. We re-evaluate constraints from the diffuse -ray emission in the direction of the Galactic center which offer the best and most solid upper limits on the dark matter fraction composed of PBHs. The revised mass range which allows PBHs to assemble all cosmological dark matter is estimated to be . We demonstrate that due to the constraints from -ray emission, quantum corrections due to the speculative memory burden effect do not modify this mass range. We also investigate the main characteristics of PBHs which are localized in the bulk. We show that PBHs localized in the bulk can make all cosmological dark matter if . Finally, we comment on the black holes that could be produced if one advocates a space with two boundaries for the dark dimension.

    hep-thastro-ph.HEhep-phPRD(2024)·35 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.