PaperPanorama

HEP Phenomenology·hep-ph

Mon·Mar 4, 2024

22 papers15 primary·7 cross-listed·reconstructed*

  1. 01*

    Collective excitations and low-energy ionization signatures of relativistic particles in silicon detectors

    Rouven Essig🇺🇸 · Ryan Plestid🇺🇸 · Aman Singal🇺🇸

    Solid-state detectors with a low energy threshold have several applications, including searches of non-relativistic halo dark-matter particles with sub-GeV masses. When searching for relativistic, beyond-the-Standard-Model particles with enhanced cross sections for small energy transfers, a small detector with a low energy threshold may have better sensitivity than a larger detector with a higher energy threshold. In this paper, we calculate the low-energy ionization spectrum from high-velocity particles scattering in a dielectric material. We consider the full material response including the excitation of bulk plasmons. We generalize the energy-loss function to relativistic kinematics, and benchmark existing tools used for halo dark-matter scattering against electron energy-loss spectroscopy data. Compared to calculations commonly used in the literature, such as the Photo-Absorption-Ionization model or the free-electron model, including collective effects shifts the recoil ionization spectrum towards higher energies, typically peaking around 4--6 electron-hole pairs. We apply our results to the three benchmark examples: millicharged particles produced in a beam, neutrinos with a magnetic dipole moment produced in a reactor, and upscattered dark-matter particles. Our results show that the proper inclusion of collective effects typically enhances a detector's sensitivity to these particles, since detector backgrounds, such as dark counts, peak at lower energies.

    hep-phastro-ph.COhep-exphysics.ins-detCommun.Phys.(2024)·20 citations
  2. 02*

    Pole properties of a resonance: When to subtract partial-decay widths to obtain the pole widths

    J. A. Oller🇪🇸

    When a resonance lies near the threshold of a heavier channel, an interesting feature can occur. The paradigmatic example employed here is the scalar isoscalar resonance that couples to the lighter and heavier channels. It is shown that the decay width is given by the sum or subtraction of the partial decay widths depending on whether the pole lies in the Riemann sheet that is contiguous with the physical one above or below the threshold, respectively. Next, we show that the usually disregarded renormalization of bare parameters in Flatté or energy-dependent Breit-Wigner parameterizations is essential to extract physical information. The compositeness of the by using a Flatté parameterization matched to reproduce the pole properties obtained from Roy equations and other analytic constraints is evaluated.

    hep-phnucl-thActa Phys.Polon.Supp.(2024)·0 citations
  3. 03*

    A Phenomenological Study of WIMP Models

    Shivam Gola🇮🇳

    In this thesis, we investigate various possibilities of Weakly Interacting Massive Particle (WIMP) dark matter (DM) and their implications. These possibilities are important because they challenge the viability of WIMP DM in light of tight constraints from experiments such as direct detection. We begin by analyzing a fermion dark matter possibility with an axion-like particle (ALP) portal. We consider theoretical and experimental limits related to neutrino and ALP data within a certain mass range, and we find the allowed parameter space. This possibility resolves the problem of the lack of direct detection of WIMP DM through the ALP portal. Furthermore, we examine the limits on photon signals from HESS and Fermi-LAT data. Next, we look at a two-component scalar and fermion dark matter possibility, following a similar approach to our previous work. This simple possibility requires only a few additional fields and symmetries to explain neutrino mass and dark matter candidates. By finding parameter space that satisfies various bounds, such as relic density, direct detection, and invisible Higgs width, we show that both scalar and fermion particles can serve as DM. This possibility is consistent and offers a rich spectrum of phenomenology that can be tested through collider-based experiments. In our final work, we removie the extra Z2 symmetry and added a new pseudoscalar particle in our two compoent model. We test this pseudoscalar particle against multiple DM and non-DM related bounds, including DM lifetime bound, Planck bound, direct-detection limits from various target materials, and invisible Higgs width. The possibility exhibits a significant parameter space for our pseudoscalar DM while being in agreement with theoretical and experimental limits.

    hep-ph0 citations
  4. 04*

    Dual symmetries of dense three and two-color QCD and some QCD-like NJL models

    T. G. Khunjua🇬🇪 · K. G. Klimenko🇷🇺 · R. N. Zhokhov🇷🇺

    In this paper the symmetry properties of the phase diagram of dense quark matter composed of and quarks with two or three colors has been investigated in the framework of massless (3+1)-dimensional Nambu--Jona-Lasinio (NJL) and QCD models. It turns out that in the presence of baryon , isospin , chiral and chiral isospin chemical potentials the Lagrangians of these models are invariant under the so-called dual transformations. Consequently, the entire NJL model (or QCD) thermodynamic potentials are dually symmetric. In particular, it means that in the total -phase portraits of these models the chiral symmetry breaking (CSB) and charged pion condensation (PC) phases are arranged dually conjugated (or symmetrical) to each other (in the case of three-color models). Whereas in the case of two-color quark matter, these models predict the entire phase structure in which there are dual symmetries between CSB, charged PC and baryon superfluid phases.

    hep-phhep-thPRD(2025)·6 citations
  5. 05*

    Charge-conjugation asymmetry and molecular content: the in matter

    Victor Montesinos🇪🇸 · Miguel Albaladejo🇪🇸 · Juan Nieves🇪🇸 · Laura Tolos🇪🇸

    We analyze the modifications that a dense nuclear medium induces in the and . In the vacuum, we consider them as isoscalar and -wave bound states, which are dynamically generated from effective interactions that lead to different Weinberg compositeness scenarios. Matter effects are incorporated through the two-meson loop functions, taking into account the self energies that the , , , and develop when embedded in a nuclear medium. Although particle-antiparticle [ versus ] lineshapes are the same in vacuum, we find extremely different density patterns in matter. This charge-conjugation asymmetry mainly stems from the very different kaon and antikaon interaction with the nucleons of the dense medium. We show that the in-medium lineshapes found for these resonances strongly depend on their / molecular content, and discuss how this novel feature can be used to better determine/constrain the inner structure of these exotic states.

    hep-phnucl-thPLB(2024)·9 citations
  6. 06*

    A test of strangeness quantum number conservation in proton-proton collisions

    Christian Bierlich🇸🇪 · Stefano Cannito🇮🇹 · Valentina Zaccolo🇮🇹

    The study delves into the production of (multi-)strange hadrons in proton-proton collisions at LHC. Novel observables are proposed to distinguish between EPOS4, based on core-corona separation between a thermalised QGP phase and a vacuum phase with global strangeness conservation, and PYTHIA8.3, based on microscopic interactions between Lund strings that conserve strangeness locally. Correlations between a meson and (multi-)strange hadrons are shown to be an excellent discriminator between the two types of models.

    hep-phEPJC(2024)·0 citations
  7. 07*

    The non-first-order-factorizable contributions to the three-loop single-mass operator matrix elements and

    J. Ablinger🇦🇹 · A. Behring🇨🇭 · J. Blümlein🇩🇪 · A. De Freitas🇦🇹 · A. von Manteuffel🇩🇪 · C. Schneider🇦🇹 · K. Schönwald🇨🇭

    The non-first-order-factorizable contributions (The terms 'first-order-factorizable contributions' and 'non-first-order-factorizable contributions' have been introduced and discussed in Refs. \cite{Behring:2023rlq,Ablinger:2023ahe}. They describe the factorization behaviour of the difference- or differential equations for a subset of master integrals of a given problem.) to the unpolarized and polarized massive operator matrix elements to three-loop order, and , are calculated in the single-mass case. For the -related master integrals of the problem, we use a semi-analytic method based on series expansions and utilize the first-order differential equations for the master integrals which does not need a special basis of the master integrals. Due to the singularity structure of this basis a part of the integrals has to be computed to in the dimensional parameter. The solutions have to be matched at a series of thresholds and pseudo-thresholds in the region of the Bjorken variable using highly precise series expansions to obtain the imaginary part of the physical amplitude for at a high relative accuracy. We compare the present results both with previous analytic results, the results for fixed Mellin moments, and a prediction in the small- region. We also derive expansions in the region of small and large values of . With this paper, all three-loop single-mass unpolarized and polarized operator matrix elements are calculated.

    hep-phPLB(2024)·35 citations
  8. 08*

    A new Wolfenstein-like expansion of lepton flavor mixing towards understanding its fine structure

    Zhi-zhong Xing🇨🇳

    Taking the tri-bimaximal flavor mixing pattern as a particular basis, we propose a new way to expand the unitary Pontecorvo-Maki-Nakagawa-Sakata (PMNS) lepton flavor mixing matrix in powers of the magnitude of its smallest element . Such a Wolfenstein-like parametrization of allows us to easily describe the salient features and fine structures of flavor mixing and CP violation, both in vacuum and in matter.

    hep-phhep-exPLB(2024)·2 citations
  9. 09*

    Neutrino phenomenology in the modular seesaw model

    Mitesh Kumar Behera🇹🇭 · Pawin Ittisamai🇹🇭 · Chakrit Pongkitivanichkul🇹🇭 · Patipan Uttayarat🇹🇭

    We have studied neutrino phenomenology in the supersymmetric type-I seesaw model endowed with the modular symmetry. We have identified different realizations of the modular symmetry, referred to as models A, B, C, and D. The 4 models are compatible with neutrino mass being inverted ordering (IO). Moreover, models A, B, and D can also accommodate normal ordering (NO) neutrino masses. We identify parameter space for each model compatible with neutrino oscillation at the 2- level. We then proceed to study the neutrino phenomenology of each model. We find that the lightest neutrino mass can be as light as 0.64 meV in the case of NO in model A and 50 meV in the case of IO in model D. The smallest effective electron neutrino mass attainable in our analysis is 8.8 meV in the case of NO (model A), and 50 meV for IO (model D). Finally, we note that the effective Majorana mass can be as small as 0.33 meV in the case of NO (model A) and 22 meV for IO (model D).

    hep-phPRD(2024)·10 citations
  10. 10*

    A Light-Front Model for the Transition Distribution Amplitudes for Backward Timelike Compton Scattering

    B. Pasquini🇮🇹 · A. Schiavi🇮🇹

    To access information on the internal structure of the nucleon, data from a variety of scattering experiments can be analyzed, in regimes where the information factorizes from an otherwise known scattering amplitude. A recent development, promising new insight, is the study of exclusive reactions in the backward kinematical region, where the information can be encoded in Transition Distribution Amplitudes (TDAs). We model the photon-to-nucleon TDAs, entering the factorized description of backward Timelike Compton Scattering, using techniques of light-front dynamics to integrate information from a quark model for the photon and the nucleon. We include the results of numerical predictions that could inform further experiments at Jefferson Lab and the future Electron--Ion Collider.

    hep-phnucl-exnucl-thPRD(2024)·4 citations
  11. 11*

    Hadron momentum spectra from analytical solutions of relativistic hydrodynamics

    Mahammad Sabir Ali🇮🇳 · Deeptak Biswas🇮🇳 · Amaresh Jaiswal🇮🇳 · Sushant K. Singh🇮🇹

    We present analytical solution of relativistic hydrodynamics for a system having cylindrical symmetry with boost-invariant longitudinal expansion and Hubble-like transverse expansion. We also consider analytical solution for Hubble-like spherically expanding system. For these two cases, we calculate analytical expression for transverse momentum spectra of hadrons, at constant temperature freeze-out hypersurface using Cooper-Frye prescription. We compare our results for transverse momentum spectra with experimental results from Large Hadron Collider and CERN SPS where one expects cylindrical and spherical geometry of the fireball, respectively. In the case of low-energy collisions with spherical geometry, we calculate rapidity spectra and compare with the results from CERN SPS.

    hep-phnucl-thEPJC(2025)·3 citations
  12. 12*

    Pseudoscalar Mesons and Emergent Mass

    K. Raya🇪🇸 · A. Bashir🇲🇽 · D. Binosi🇮🇹 · C. D. Roberts🇨🇳 · J. Rodríguez-Quintero🇪🇸

    Despite its role in the continuing evolution of the Universe, only a small fraction of the mass of visible material can be attributed to the Higgs boson alone. The overwhelmingly dominant share may/should arise from the strong interactions that act in the heart of nuclear matter; namely, those described by quantum chromodynamics. This contribution describes how studying and explaining the attributes of pseudoscalar mesons can open an insightful window onto understanding the origin of mass in the Standard Model and how these insights inform our knowledge of hadron structure. The survey ranges over distribution amplitudes and functions, electromagnetic and gravitational form factors, light-front wave functions, and generalized parton distributions. Advances made using continuum Schwinger function methods and their relevance for experimental efforts are highlighted.

    hep-phhep-latnucl-thFew Body Syst.(2024)·53 citations
  13. 13*

    J/psi-pair production at NLL in TMD factorisation at the LHC

    Alice Colpani Serri🇵🇱 · Jelle Bor🇳🇱 · Daniel Boer🇳🇱 · Jean-Philippe Lansberg🇫🇷

    J/psi-pair production at the LHC is currently one of the few tools available to probe gluon transverse momentum distributions (TMDs). In this context, data from LHCb in the collider mode have the potential to probe the evolution of the unpolarised-gluon TMDs and to measure the distribution of the linearly-polarised gluon in unpolarised protons for the first time. In this proceedings contribution, improved predictions obtained for the LHC (at sqrt(s) = 13 TeV) up to next-to-leading logarithm (NLL) in TMD factorisation are presented. We show the obtained predictions of transverse-momentum distributions at different invariant masses and rapidities computed in the LHCb acceptance along with PDF uncertainty. We predict the azimuthal modulations of the cross section that arise from linearly-polarised gluons.

    hep-phhep-exnucl-exnucl-thPoS(2024)·2 citations
  14. 14*

    Two-loop contributions of axion-like particles to electromagnetic and chromomagnetic form factors

    Matthias Neubert🇺🇸 · Marvin Schnubel🇺🇸

    Axions and axion-like particles emerge in many models for physics beyond the Standard Model. Thus, they have gained increasing research interest in both experimental and theoretical physics apart from their original proposition as a solution to the strong -problem. Among other aspects it has recently been shown that ALPs can potentially provide a solution to the long-lasting discrepancy between theory and experiment of the anomalous magnetic moment of the muon. Provided that the ALP has flavor-violating couplings to leptons, they can also mediate flavor-violating decays like . Both processes are mediated through related form factors that we compute to two-loop order. We further show numerical implications of our calculations and how they might affect constraints on ALP couplings derived from experiments.

    hep-phEPJC(2024)·4 citations
  15. 15*

    An exciting hint towards the solution of the neutron lifetime puzzle?

    Benjamin Koch🇦🇹 · Felix Hummel🇦🇹

    We revisit the neutron lifetime puzzle, a discrepancy between beam and bottle measurements of the weak neutron decay. Since both types of measurements are realized at different times after the nuclear production of free neutrons, we argue that the existence of excited states could be responsible for the different lifetimes. We elaborate on the required properties of such states and under what circumstances it is possible that they have not been experimentally identified yet.

    hep-phPRD(2024)·10 citations
  16. 16*

    The Odd 2D Bubbles, 4D Triangles, and Einstein and Weyl Anomalies in 2D Gravitational Fermionic amplitudes: The Role of Breaking Integration Linearity for Anomalies

    Luciana Ebani🇧🇷

    We investigated Relations Among Green Functions defined in an alternative strategy for coping with the divergences, also called the Implicit Regularization Method (IREG): the mathematical content (divergent and finite) will remain intact until the calculations end. The divergent part will be organized through standardized objects free of physical quantities. In contrast, the finite part is projected in a class of well-behaved functions that carry all the amplitudes' physical content. That relations arise in fermionic amplitudes in even space-time dimensions, where anomalous tensors connect to finite amplitudes as in the bubbles and triangles in two and four dimensions. Those tensors depend on surface terms, whose non-zero values arise from finite amplitudes as requirements of consistency with the linearity of integration and uniqueness. Maintaining these terms implies breaking momentum-space homogeneity and, in a later step, the Ward identities. Meanwhile, eliminating them allows more than one mathematical expression for the same amplitude. That is a consequence of choices related to the involved Dirac traces. Independently of divergences, it is impossible to satisfy all symmetry implications by simultaneously requiring vanishing surface terms and linearity. Then we approach the 1-loop level fermionic correction for the propagation of the graviton in a space-time D=1+1 through the action of a Weyl fermion in curved space-time. In this context, gravitational anomalies arise, and the amplitudes investigated have the highest degree of divergence quadratic. That imposes a substantial algebraic effort; however, the conclusions are in agreement with the non-gravitational amplitudes. At the end of the calculations, we show how it is possible to fix the value of the divergent part through the relations imposed for amplitudes.

    hep-thhep-phmath-phmath.MP2 citations
  17. 17*

    Angular bispectrum and trispectrum of scalar-induced gravitational waves: all contributions from primordial non-Gaussianity and

    Jun-Peng Li🇨🇳 · Sai Wang🇨🇳 · Zhi-Chao Zhao🇨🇳 · Kazunori Kohri🇯🇵

    Studying the primordial non-Gaussianity of inflationary perturbations is crucial for testing the inflation paradigm of the early universe. In this work, we conduct a comprehensive analysis of the angular bispectrum and trispectrum of scalar-induced gravitational waves (SIGWs) in the presence of local-type primordial non-Gaussianity parameterized by and , deriving their semi-analytical formulae for the first time. Our findings indicate that it is the presence of primordial non-Gaussianity that leads to a non-Gaussian SIGW background, suggesting that the angular bispectrum and trispectrum of SIGWs could serve as probes of the primordial non-Gaussianity. Our numerical results further illustrate that and exert significant impacts on the spectral amplitudes, potentially reaching up to for the former and for the latter. In particular, we demonstrate that the angular bispectrum and trispectrum exhibit characteristic dependence on the angular multipoles and frequency bands. They hold potentials to be measured by gravitational-wave detectors that may advance our understanding of the origin of the universe.

    astro-ph.COgr-qchep-phJCAP(2024)·19 citations
  18. 18*

    Neural Simulation-Based Inference of the Neutron Star Equation of State directly from Telescope Spectra

    Len Brandes🇩🇪 · Chirag Modi🇺🇸 · Aishik Ghosh🇺🇸 · Delaney Farrell🇺🇸 · Lee Lindblom🇺🇸 · Lukas Heinrich🇩🇪 · Andrew W. Steiner🇺🇸 · Fridolin Weber🇺🇸 · Daniel Whiteson🇺🇸

    Neutron stars provide a unique opportunity to study strongly interacting matter under extreme density conditions. The intricacies of matter inside neutron stars and their equation of state are not directly visible, but determine bulk properties, such as mass and radius, which affect the star's thermal X-ray emissions. However, the telescope spectra of these emissions are also affected by the stellar distance, hydrogen column, and effective surface temperature, which are not always well-constrained. Uncertainties on these nuisance parameters must be accounted for when making a robust estimation of the equation of state. In this study, we develop a novel methodology that, for the first time, can infer the full posterior distribution of both the equation of state and nuisance parameters directly from telescope observations. This method relies on the use of neural likelihood estimation, in which normalizing flows use samples of simulated telescope data to learn the likelihood of the neutron star spectra as a function of these parameters, coupled with Hamiltonian Monte Carlo methods to efficiently sample from the corresponding posterior distribution. Our approach surpasses the accuracy of previous methods, improves the interpretability of the results by providing access to the full posterior distribution, and naturally scales to a growing number of neutron star observations expected in the coming years.

    astro-ph.HEastro-ph.IMgr-qchep-ph+1JCAP(2024)·28 citations
  19. 19*

    Gravitational waves in a cyclic Universe: resilience through cycles and vacuum state

    Mariaveronica De Angelis🇬🇧 · Adam Smith🇬🇧 · William Giarè🇬🇧 · Carsten van de Bruck🇬🇧

    We present a generalised calculation for the spectrum of primordial tensor perturbations in a cyclic Universe, making no assumptions about the vacuum state of the theory and accounting for the contribution of tensor modes produced in the dark energy phase of the previous cycle. We show that these modes have minimal impact on the spectrum observed in the current cycle, except for corrections on scales as large as the comoving Hubble radius today. These corrections are due to sub-horizon modes produced towards the end of the dark energy phase, persisting into the ekpyrotic phase of the next cycle as additional quanta. In relation to the vacuum state, we argue that non-Bunch-Davies quanta can easily overwhelm the energy density driving the dark energy phase, potentially compromising the model. Therefore, avoiding backreaction effects sets restrictive constraints on deviations away from the Bunch-Davies vacuum during this phase, limiting the overall freedom to consider alternative vacua in the cyclic Universe.

    hep-thastro-ph.COhep-phJCAP(2024)·4 citations
  20. 20*

    Nonperturbative Collins-Soper Kernel from Chiral Quarks with Physical Masses

    Dennis Bollweg🇺🇸 · Xiang Gao🇺🇸 · Swagato Mukherjee🇺🇸 · Yong Zhao🇺🇸

    We present a lattice QCD calculation of the rapidity anomalous dimension of quark transverse-momentum-dependent distributions, i.e., the Collins-Soper (CS) kernel, up to transverse separations of about 1 fm. This unitary lattice calculation is conducted, for the first time, employing the chiral-symmetry-preserving domain wall fermion discretization and physical values of light and strange quark masses. The CS kernel is extracted from the ratios of pion quasi-transverse-momentum-dependent wave functions (quasi-TMDWFs) at next-to-leading logarithmic perturbative accuracy. Also for the first time, we utilize the recently proposed Coulomb-gauge-fixed quasi-TMDWF correlator without a Wilson line. We observe significantly slower signal decay with increasing quark separations compared to the established gauge-invariant method with a staple-shaped Wilson line. This enables us to determine the CS kernel at large nonperturbative transverse separations and find its near-linear dependence on the latter. Our result is consistent with the recent lattice calculation using gauge-invariant quasi-TMDWFs, and agrees with various recent phenomenological parametrizations of experimental data.

    hep-lathep-exhep-phnucl-ex+1PLB(2024)·40 citations
  21. 21*

    Numerical challenges for energy conservation in N-body simulations of collapsing self-interacting dark matter halos

    Moritz S. Fischer🇩🇪 · Klaus Dolag🇩🇪 · Hai-Bo Yu🇺🇸

    Dark matter (DM) halos can be subject to gravothermal collapse if the DM is not collisionless, but engaged in strong self-interactions. When the scattering can efficiently transfer heat from the centre to the outskirts, the central region of the halo collapses and reaches densities much higher than those for collisionless DM. This phenomenon is potentially observable in studies of strong lensing. Current theoretical efforts are motivated by observations of surprisingly dense substructures. A comparison with observations requires accurate predictions. One method to obtain such predictions is to use N-body simulations. Collapsed halos are extreme systems that pose challenges when applying state-of-the-art codes to model self-interacting dark matter (SIDM). We investigate the root of such problems, with a focus on energy non-conservation and discuss possible strategies to avoid them. We ran N-body simulations, with and without SIDM, of an isolated DM-only halo and we adjusted the numerical parameters to check the accuracy of the simulation. We find that not only the numerical scheme for SIDM can lead to energy non-conservation, but also the modelling of gravitational interaction and the time integration are problematic. The issues we find are: (a) particles changing their time step in a non-time-reversible manner; (b) the asymmetry in the tree-based gravitational force evaluation; and (c) SIDM velocity kicks breaking the time symmetry. Tuning the parameters of the simulation allows us to conserve energy not only at early stages of the evolution, but also later on. However, the cost of the simulations becomes prohibitively large. Some of the problems that make the simulations of the gravothermal collapse phase inaccurate can be overcome by choosing appropriate numerical schemes. However, other issues still pose a challenge. Our findings motivate further works on addressing these challenges.

    astro-ph.COastro-ph.GAhep-phAstron.Astrophys.(2024)·36 citations
  22. 22*

    The QCD theta-parameter in canonical quantization

    Wen-Yuan Ai🇬🇧 · Bjorn Garbrecht🇩🇪 · Carlos Tamarit🇩🇪

    The role of the QCD theta-parameter is investigated in pure Yang-Mills theory in the spacetime given by the four-dimensional Euclidean torus. While in this setting the introduction of possibly unphysical boundary conditions is avoided, it must be specified how the sum over the topological sectors is to be carried out. To connect with observables in real time, we perceive the partition function as the trace over the canonical density matrix. The system then corresponds to one of a finite temperature on a spatial three-torus. Carrying out the trace operation requires canonical quantization and gauge fixing. Fixing the gauge and demanding that the Hermiticity of the Hamiltonian is maintained leads to a restriction of the Hilbert space of physical wave functionals that generalizes the constraints derived from imposing Gauss' law. Consequently, we find that the states in the Hilbert space are properly normalizable under an inner product that integrates over each physical configuration represented by the gauge potential one time and one time only. The observables derived from the constrained Hilbert space do not violate charge-parity symmetry. We note that an exact hidden symmetry of the theory that is present for arbitrary values of theta in the Hamiltonian is effectively promoted to parity conservation in this constrained space. These results, derived on a torus in order to avoid the introduction of boundary conditions, also carry over to Minkowski spacetime when taking account of all possible gauge transformations.

    hep-thhep-lathep-ph15 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.