PaperPanorama

HEP Phenomenology·hep-ph

Fri·Nov 16, 2018

33 papers—23 primary·10 cross-listed·reconstructed*

  1. 01*

    Displaced Lepton Jet Signatures from Self-Interacting Dark Matter Bound States

    Yuhsin Tsai🇺🇸 · Tao Xu🇨🇳 · Hai-Bo Yu🇺🇸

    We study self-interacting dark matter signatures at the Large Hadron Collider. A light dark photon, mediating dark matter self-interactions, can bind dark matter particles to form a bound state when they are produced via a heavy pseduoscalar in collisions. The bound state can further annihilate into a pair of boosted dark photons, which subsequently decay into charged leptons through a kinetic mixing portal, resulting in striking displaced lepton jet signals. After adapting the analysis used in the ATLAS experiment, we explore the reach of the model parameters at the run with an integrated luminosity of . For heavy dark matter, the displaced lepton jet searches can surpass traditional monojet signals in setting the lower bound on the pseduoscalar mass. If a positive signal is detected, we can probe the dark matter mass and the dark coupling constant after combining both the displaced lepton jet and monojet searches. We further show the CMS dimuon search can be sensitive to the final state radiation of the dark photon. Our results demonstrate terrestrial collider experiments complement astronomical observations of galaxies in the search of the self-interacting nature of dark matter.

    hep-phJHEP(2019)·9 citations
  2. 02*

    Exploring first order phase transition in extended models by complementarity between collider measurements and cosmological observations

    Toshinori Matsui🇰🇷

    We consider models with the gauge symmetry, which is spontaneously broken by dark Higgs mechanism. We discuss patterns of the electroweak phase transition and detectability of gravitational waves (GWs) when strongly first order phase transition (1stOPT) occurs. It is pointed out that the collider bounds on the properties of the discovered Higgs boson exclude a part of parameter space that could otherwise generate detectable GWs. We find that GWs produced from multi-step PT can be detected at future observations such as LISA and DECIGO if the dark photon mass is GeV with the gauge coupling being . In addition, we show that most of the parameter regions can be covered by precision measurements of various Higgs boson couplings and direct searches for the singlet scalar boson at future collider experiments. Furthermore, we expect the complementarity of the detection of GW observations from the strongly 1stOPT, collider bounds and dark photon searches in the models of the dark gauge symmetry.

    hep-ph0 citations
  3. 03*

    Continuum Naturalness

    Csaba Csáki🇺🇸 · Gabriel Lee🇺🇸 · Seung J. Lee🇰🇷 · Salvator Lombardo🇺🇸 · Ofri Telem🇺🇸

    We present a novel class of composite Higgs models in which the top and gauge partners responsible for cutting off the Higgs quadratic divergences form a continuum. The continuum states are characterized by their spectral densities, which should have a finite gap for realistic models. We present a concrete example based on a warped extra dimension with a linear dilaton, where this finite gap appears naturally. We derive the spectral densities in this model and calculate the full Higgs potential for a phenomenologically viable benchmark point, with percent level tuning. The continuum top and gauge partners in this model evade all resonance searches at the LHC and yield qualitatively different collider signals.

    hep-phJHEP(2019)·36 citations
  4. 04*

    Top partners tackling vector dark matter

    Juan Yepes🇨🇱

    The WIMP-nucleon scattering cross section in a simple dark matter model and its constraints from the latest direct detection experiment are treated here at the loop level. We consider a scenario with an emerging vector dark matter field that interacts with the Standard Model quarks, via loop contributions that are sourced from a scalar mediator. The involved parameter space for the dark matter-mediator masses is constrained by the Xenon1T limit and the neutrino floor. The current direct detection bounds are eluded by invoking the top partners in a Composite Higgs model, whose scale mass helps us in suppressing the WIMP-nucleon cross section.

    hep-phPLB(2020)·11 citations
  5. 05*

    Understanding the energy resolution of liquid argon neutrino detectors

    Alexander Friedland🇺🇸 · Shirley Weishi Li🇺🇸

    Available estimates for the energy resolution of DUNE vary by as much as a factor of four. To address this controversy, and to connect the resolution to the underlying physical processes, we build an independent simulation pipeline for neutrino events in liquid argon, combining the public tools GENIE and FLUKA. Using this pipeline, we first characterize the channels of non-hermeticity of DUNE, including subthreshold particles, charge recombination, and nuclear breakup. Particular attention is paid to the role of neutrons, which are responsible for a large fraction of missing energy in all channels. Next, we determine energy resolution, by quantifying event-to-event stochastic fluctuations in missing energy. This is done for several sets of assumptions about the reconstruction performance, including those available in the literature. The resulting migration matrices, connecting true and reconstructed neutrino energies, are presented. Finally, we quantify the impact of different improvements on the experimental performance. For example, we show that dropping particle identification information degrades the resolution by a factor of two, while omitting charge deposits from de-excitation gammas worsens it by about 25%. In the future, this framework can be used to assess the impact of cross section uncertainties on the oscillation sensitivity.

    hep-phhep-exnucl-exnucl-thPRD(2019)·87 citations
  6. 06*

    Cosmological Helical Hypermagnetic Fields and Baryogenesis

    Kohei Kamada🇰🇷

    Recent gamma-ray observations of TeV blazars exhibits the deficits of the secondary GeV cascade photons. This suggests the existence of the intergalactic magnetic fields, which may have a primordial origin. One of the mechanisms that can produce primordial magnetic fields is so-called the chiral plasma instability, where the (hyper) magnetic fields are destabilized when a large chiral asymmetry exists in the high-temperature plasma in the early Universe. We argue that such a large chiral asymmetry can be produced through the GUT baryogenesis. Note that the chiral asymmetry is a good conserved quantity at high temperature when the Yukawa interaction is weak enough. We also point out that the generated hypermagnetic fields are maximally helical, and hence baryon and lepton asymmetry is inevitably produced through the chiral anomaly in the Standard Model through gauge interaction at the electroweak symmetry breaking. Consequently, the magnetic fields suggested by the blazar observations over-produce baryon asymmetry. Thus the chiral plasma instability alone cannot be responsible for the intergalactic magnetic fields but can be responsible for the baryon asymmetry of the Universe. In other words, GUT baryogenesis without - asymmetry generation is revived as a viable baryogenesis scenario, which otherwise has been thought to suffer from + washout by sphalerons. This presentation is based on the work [1].

    hep-phastro-ph.COhep-thPoS(2019)·2 citations
  7. 07*

    The radiative decays of the singly heavy baryons in chiral perturbation theory

    Guang-Juan Wang🇨🇳 · Lu Meng🇨🇳 · Shi-Lin Zhu🇨🇳

    In the framework of the heavy baryon chiral perturbation theory (HBChPT), we calculate the radiative decay amplitudes of the singly heavy baryons up to the next-to-next-to-leading order (NNLO). In the numerical analysis, we adopt the heavy quark symmetry to relate some low energy constants (LECs) with those LECs in the calculation of the magnetic moments. We use the results from the lattice QCD simulation as input. With a set of unified LECs, we obtain the numerical (transition) magnetic moments and radiative decay widths. We give the numerical results for the spin- sextet to the spin- antitriplet up to the next-to-leading order (NLO). The nonvanishing and solely arise from the U-spin symmetry breaking, and do not depend on the lattice QCD inputs up to NLO. We also systematically give the numerical analysis of the magnetic moments of the spin-, spin- sextet and their radiative decay widths up to NNLO. In the heavy quark limit, the radiative decays between the sextet states happen through the magnetic dipole (M1) transitions, while the electric quadrupole (E2) transition does not contribute. We also extend the same analysis to the single bottom baryons.

    hep-phPRD(2019)·38 citations
  8. 08*

    Magnetic Dipole Moment in Relativistic Quantum Mechanics

    Andrew Steinmetz🇺🇸 · Martin Formanek🇺🇸 · Johann Rafelski🇺🇸

    We investigate relativistic quantum mechanics (RQM) for particles with arbitrary magnetic moment. We compare two well known RQM models: a) Dirac equation supplemented with an incremental Pauli term (DP); b) Klein-Gordon equations with full Pauli EM dipole moment term (KGP). We compare exact solutions to the external field cases in the limit of weak and strong (critical) fields for: i) homogeneous magnetic field, and ii) the Coulomb -potential. For i) we consider the Landau energies and the Landau states as a function of the gyromagnetic factor (-factor). For ii) we investigate contribution to the Lamb shift and the fine structure splitting. For both we address the limit of strong binding and show that these two formulations grossly disagree. We discuss possible experiments capable of distinguishing between KGP and DP models in laboratory. We describe impact of our considerations in astrophysical context (magnetars). We introduce novel RQM models of magnetic moments which can be further explored.

    hep-phEPJA(2019)·35 citations
  9. 09*

    Highly predictive and testable flavor model within type-I and II seesaw framework and associated phenomenology

    Surender Verma🇮🇳 · Monal Kashav🇮🇳 · Shankita Bhardwaj🇮🇳

    We investigate neutrino mass model based on discrete flavor symmetry in type-I+II seesaw framework. The model has imperative predictions for neutrino masses, mixing and violation testable in the current and upcoming neutrino oscillation experiments. The important predictions of the model are: normal hierarchy for neutrino masses, a higher octant for atmospheric angle () and near-maximal Dirac-type phase ( or ) at C. L.. These predictions are in consonance with the latest global-fit and results from Super-Kamiokande(SK), NOA and T2K. Also, one of the important feature of the model is the existence of a lower bound on effective Majorana mass, eV(at 3) which corresponds to the lower part of the degenerate spectrum and is within the sensitivity reach of the neutrinoless double beta decay(0) experiments.

    hep-phNPB(2019)·16 citations
  10. 10*

    Pseudo-Dirac Higgsino dark matter in GUT scale supersymmetry

    V Suryanarayana Mummidi🇮🇳 · Ketan M. Patel🇮🇳

    We investigate a scenario in which supersymmetry is broken at scale GeV leaving only a pair of Higgs doublets, their superpartners (Higgsinos) and a gauge singlet fermion (singlino) besides the standard model fermions and gauge bosons at low energy. The Higgsino-singlino mixing induces small splitting between the masses of electrically neutral components of Higgsinos which otherwise remain almost degenerate in GUT scale supersymmetry. The lightest combination of them provides a viable thermal dark matter if the Higgsino mass scale is close to TeV. The small mass splitting induced by singlino turns the neutral components of Higgsinos into pseudo-Dirac fermions which successfully evade the constraints from the direct detection experiments if the singlino mass is GeV. We analyse the constraints on the effective framework, arising from the stability of electroweak vacuum, observed mass and couplings of Higgs, and the limits on the masses of the other scalars, by matching it with the next-to-minimal supersymmetric standard model at . It is found that the presence of singlino at intermediate scale significantly improves the stability of electroweak vacuum and allows a stable or metastable vacuum for almost all the values of while the observed Higgs mass together with the limit on the charged Higgs mass favours .

    hep-phJHEP(2019)·9 citations
  11. 11*

    Small- physics at the LHeC

    Heikki Mäntysaari🇫🇮

    The Large Hadron-electron Collider LHeC is a proposed upgrade of the LHC. It would add an electron beam to the LHC, and make it possible to study electron-proton and electron-nucleus collisions at very high energies. We present some of the highlights of the LHeC physics program related to the studies of partonic structure of protons and nuclei, and to the non-linear QCD phenomena visible at small .

    hep-phnucl-exnucl-thPoS(2018)·1 citation
  12. 12*

    Solutions of evolution equations for medium-induced QCD cascades

    K. Kutak🇵🇱 · W. Placzek🇵🇱 · R. Straka🇵🇱

    In this paper we present solutions of evolution equations for inclusive distribution of gluons as produced by jet traversing quark-gluon plasma. We reformulate the original equations in such a form that the virtual and unresolved-real emissions as well as unresolved collisions with medium are resummed in a Sudakov-type form factor. The resulting integral equations are then solved most efficiently with use of newly developed Markov Chain Monte Carlo algorithms implemented in a dedicated program called MINCAS. Their results for a gluon energy density are compared with an analytical solution and a differential numerical method. Some results for gluon transverse-momentum distributions are also presented. They exhibit interesting patterns not discussed so far in the literature, in particular a departure from the Gaussian behaviour - which does not happen in approximate analytical solutions.

    hep-phEPJC(2019)·25 citations
  13. 13*

    Damping rate of a fermion in ultradegenerate chiral matter

    Stefano Carignano🇪🇸 · Cristina Manuel🇪🇸

    We compute the damping rate of a fermion propagating in a chiral plasma when there is an imbalance between the densities of left- and right-handed fermions, after generalizing the hard thermal loop resummation techniques for these systems. In the ultradegenerate limit, for very high energies the damping rate of this external fermion approaches a constant value. Closer to the two Fermi surfaces, however, we find that the rate depends on both the energy and the chirality of the fermion, being higher for the predominant chirality. This comes out as a result of its scattering with the particles of the plasma, mediated by the exchange of Landau damped photons. In particular, we find that the chiral imbalance is responsible for a different propagation of the left and right circular polarised transverse modes of the photon, and that a chiral fermion interacts differently with these two transverse modes. We argue that spontaneous radiation of energetic fermions is kinematically forbidden, and discuss the time regime where our computation is valid.

    hep-phcond-mat.mes-hallPRD(2019)·15 citations
  14. 14*

    Neutrino flavor-mass uncertainty relations and an entanglement-assisted determination of the PMNS matrix

    Stefan Floerchinger🇩🇪 · Jan-Markus Schwindt🇩🇪

    As a result of a non-trivial mixing matrix, neutrinos cannot be simultaneously in a flavor and mass eigenstate. We formulate and discuss information entropic relations that quantify the associated quantum uncertainty. We also formulate a protocol to determine the Pontecorvo-Maki-Nakagawa-Sakata (PMNS) matrix from quantum manipulations and measurements on an entangled lepton-neutrino pair. The entangled state features neutrino oscillations in a conditional probability involving measurements on the lepton and the neutrino. They can be switched off by choosing a specific observable on the lepton side which is determined by the PMNS matrix. The parameters of the latter, including the CP-violating phase , can be obtained by guessing them and improving the guess by minimizing the remaining oscillations.

    hep-phquant-phPRD(2020)·7 citations
  15. 15*

    Dark Matter Theory

    Manuel Drees (Bonn U.)🇩🇪

    I begin by briefly reviewing the evidence for the existence of Dark Matter (DM), emphasizing that {\em many} observations, at length scales between kpc (the size of the smallest galaxies) and Gpc (the Hubble radius) can be described by the same simple model, CDM. I will then argue that primordial black holes, the only DM candidates that can be realized within the Standard Model (SM) of particle physics, are very unlikely to provide all of DM. After giving a (probably incomplete) list of possible DM candidates, I end by mentioning some recent developments in the theory of Weakly Interacting Massive Particles (WIMPs).

    hep-phPoS(2019)·22 citations
  16. 16*

    A modern guide to {\rm }-Poincaré

    A. Addazi🇨🇳 · A. Marciano🇨🇳

    Motivated by the recent interest in underground experiments phenomenology, we review the main aspects of one specific non-commutative space-time model, based on the Groenewold-Moyal plane algebra, the -Poincaré space-time. In the -Poincaré scenario, the Lorentz co-algebra is deformed introducing a non-commutativity of space-time coordinates. In such a theory, a new quantum field theory in non-commutative space-time can be reformulated. Tackling on several conceptual misunderstanding and technical mistakes in the literature, we will focus on several issues such: the construction of fields theories in -Poincaré; the unitarity of the S-matrix; the violation of locality, the violation of the spin statistic theorem and the Pauli principle; the observables for underground experiments.

    hep-phgr-qchep-thInt.J.Mod.Phys.A(2020)·23 citations
  17. 17*

    The spin parity of (4100), (4050) and (4250)

    Xu Cao🇨🇳 · Jian-Ping Dai🇨🇳

    We conjecture that (4100) found by LHCb group from a Dalitz plot analysis of decay is the charge conjugate of (4050) observed in distribution from Belle collaboration. Some interesting conclusions are inferred from this assumption. The (4250) would be assigned to be a or state because of its absence in invariant mass distribution, while (4050)/(4100) could be a or state but is unfavored because it would be coupled to in -wave. The null observation of , and production in annihilation and decay by Belle collaboration would further allocate the spin parity combination of (4050)/(4100) and (4250). Our deductions can be used to exclude a set of proposed models and could be further tested by future experiment, e.g. in collisions.

    hep-phnucl-thPRD(2019)·16 citations
  18. 18*

    Small-mass effects in heavy-to-light form factors

    T. Engel🇨🇭 · C. Gnendiger🇨🇭 · A. Signer🇨🇭 · Y. Ulrich🇨🇭

    We present the heavy-to-light form factors with two different non-vanishing masses at next-to-next-to-leading order and study its expansion in the small mass. The leading term of this small-mass expansion leads to a factorized expression for the form factor. The presence of a second mass results in a new feature, in that the soft contribution develops a factorization anomaly. This cancels with the corresponding anomaly in the collinear contribution. With the generalized factorization presented here, it is possible to obtain the leading small-mass terms for processes with large masses, such as muon-electron scattering, from the corresponding massless amplitude and the soft contribution.

    hep-phJHEP(2019)·68 citations
  19. 19*

    Systematical investigation on the stability of doubly heavy tetraquark states

    Chengrong Deng🇨🇳 · Hong Chen🇨🇳 · Jialun Ping🇨🇳

    We systematically investigate the stability of the doubly heavy tetraquark states ( and , , and ) within the framework of the color flux-tube model involving a multibody confinement potential, -exchange, one-gluon-exchange and one-Goldstone-boson-exchange interactions. Our numerical analysis indicates that the states with and with are the most promising stable states against strong interactions. The states with , with , , and , and with and as stable states are also predicted in the color flux-tube model. The dynamical mechanism producing those stable doubly heavy tetraquark states are discussed in the color flux-tube model.

    hep-phEPJA(2020)·75 citations
  20. 20*

    Photon collider search strategy for sleptons and dark matter at the LHC

    Lydia Beresford🇬🇧 · Jesse Liu🇬🇧

    We propose a search strategy using the LHC as a photon collider to open sensitivity to scalar lepton (slepton ) production with masses around 15 to 60 GeV above that of neutralino dark matter . This region is favored by relic abundance and muon arguments. However, conventional searches are hindered by the irreducible diboson background. We overcome this obstruction by measuring initial state kinematics and the missing momentum four-vector in proton-tagged ultraperipheral collisions using forward detectors. We demonstrate sensitivity beyond LEP for slepton masses of up to 220 GeV for GeV with 100 fb of 13 TeV proton collisions. We encourage the LHC collaborations to open this forward frontier for discovering new physics.

    hep-phPRL(2019)·43 citations
  21. 21*

    Dissociative production of vector mesons at electron-ion colliders

    D. Bendova🇨🇿 · J. Cepila🇨🇿 · J. G. Contreras🇨🇿

    We present predictions for the exclusive and dissociative production of vector mesons off protons in an electron-ion collider. The computation is based on the energy-dependent hot spot model that has successfully described the available photoproduction data. We find that the model also describes correctly all available electroproduction data. In addition, we find that the cross section for dissociative production as a function of the center-of-mass energy of the photon-proton system has a maximum, whose position depends on the virtuality of the photon and the mass of the vector meson. We use these maxima to define a geometrical saturation scale and find that it grows linearly with energy as a function of the scale of the process. This phenomenon can be studied at the proposed electron-ion colliders, JLEIC, eRHIC and LHeC.

    hep-phPRD(2019)·33 citations
  22. 22*

    Paper-boat relaxion

    Shao-Jiang Wang🇺🇸

    A new relaxion mechanism is proposed where a small electroweak scale is preferably selected earlier than the larger one due to a potential instability, which is different from previously proposed stopping mechanisms by either Hubble friction from an increasing periodic barrier or thermal friction from gauge boson production. The sub-Planckian field excursion of an axion can be achieved without violating the bound on the -folding number from a quantum gravity perspective; and our relaxion can be identified as a QCD axion, preserving the Peccei-Quinn solution to the strong problem as well as making up all the cold dark matter in our current Universe.

    hep-phastro-ph.COhep-thPRD(2019)·13 citations
  23. 23*

    Neutron Star Stability in Light of the Neutron Decay Anomaly

    Benjamin Grinstein🇺🇸 · Chris Kouvaris🇩🇰 · Niklas Grønlund Nielsen🇩🇰

    A recent proposal suggests that experimental discrepancies on the lifetime of neutrons can be resolved if neutrons decay to dark matter. At the same time it has been demonstrated that such a decay mode would soften the nuclear equation of state resulting in neutron stars with a maximum mass much below currently observed ones. In this paper we demonstrate that appropriate dark matter-baryon interactions can accommodate neutron stars with mass above 2 solar masses. We also show that dark matter self-interactions could also help neutrons stars reach 2 solar masses provided that dark matter is of asymmetric nature.

    hep-phastro-ph.COPRL(2019)·45 citations
  24. 24*

    Deep learning in the heterotic orbifold landscape

    Andreas Mütter🇩🇪 · Erik Parr🇩🇪 · Patrick K.S. Vaudrevange🇩🇪

    We use deep autoencoder neural networks to draw a chart of the heterotic -II orbifold landscape. Even though the autoencoder is trained without knowing the phenomenological properties of the -II orbifold models, we are able to identify fertile islands in this chart where phenomenologically promising models cluster. Then, we apply a decision tree to our chart in order to extract the defining properties of the fertile islands. Based on this information we propose a new search strategy for phenomenologically promising string models.

    ↳ hep-thhep-phNPB(2019)·57 citations
  25. 25*

    QCD at nonzero isospin asymmetry

    Bastian B. Brandt🇩🇪 · Gergely Endrodi🇩🇪 · Sebastian Schmalzbauer🇩🇪

    We study the phase diagram and the thermodynamic properties of QCD at nonzero isospin asymmetry at physical quark masses with staggered quarks. In particular, continuum results for the phase boundary between the normal and the pion condensation phases and the chiral/deconfinement transition are presented. Our findings indicate that the pion condensation phase is restricted to ~MeV for isospin chemical potentials up to 325~MeV. We also use the data to test the range of validity of the Taylor expansion method and show first results for the equation of state.

    ↳ hep-lathep-phnucl-thPoS(2018)·21 citations
  26. 26*

    Anisotropic flow in the few collisions regime: application to bottomonia

    Nina Kersting🇩🇪 · Nicolas Borghini🇩🇪 · Steffen Feld🇩🇪

    Considering the kinetic Boltzmann equation in the limit of very few collisions, we study the evolution of the phase space distribution of bottomonia interacting with an expanding gas of massless partons. We investigate the scaling of the anisotropic flow coefficients on the initial eccentricities and the inverse Knudsen number, and compute their transverse momentum dependence.

    ↳ nucl-thhep-phMDPI Proc.(2019)·8 citations
  27. 27*

    Baryogenesis with the Berry phase

    Seishi Enomoto🇺🇸 · Tomohiro Matsuda🇯🇵

    The spontaneous baryogenesis scenario explains how a baryon asymmetry can develop while baryon violating interactions are still in thermal equilibrium. However, generation of the chemical potential from the derivative coupling is dubious since the chemical potential may not appear after the Legendre transformation. The geometric phase (Pancharatnam-Berry phase) results from the geometrical properties of the parameter space of the Hamiltonian, which is calculated from the Berry connection. In this paper, using the formalism of the Berry phase, we show that the chemical potential defined by the Berry connection is consistent with the Legendre transformation. The framework of the Berry phase is useful in explaining the mathematical background of the spontaneous baryogenesis, and also is useful for calculating the asymmetry of the non-thermal particle production in time-dependent backgrounds. Using the formalism, we show that the mechanism can be extended to more complex situations.

    ↳ hep-thhep-phPRD(2019)·7 citations
  28. 28*

    Impact of Magnetic field on neutron star properties

    Tuhin Malik🇮🇳 · Debashree Sen🇮🇳 · T. K. Jha🇮🇳 · Hiranmaya Mishra🇮🇳

    We derive an equation of state for magnetized charge neutral nuclear matter relevant for neutron star structure. The calculations are performed within an effective chiral model based on generalization of sigma model with nonlinear self interactions of the sigma mesons along with vector mesons and a cross-coupling term. The effective chiral model is extended by introducing the contributions of strong magnetic field on the charged particles of the model. The contributions arising from the effects of magnetic field on the Dirac sea of charged baryons are also included. The resulting equation of state for the magnetized dense matter is used to investigate the neutron star properties, like, mass-radius relation and tidal deformability. The dimensionless tidal deformability of NS is found to be , which is consistent with recent observation of GW170817. The maximum mass of neutron star in presence of strong magnetic field is consistent with the observational constraints on mass of neutron star from PSR~ J0348 - 0432 and the radius at mass of the neutron star is within the empirical bounds.

    ↳ nucl-thhep-ph1 citation
  29. 29*

    Dark Energy and Modified Gravity in Degenerate Higher-Order Scalar-Tensor (DHOST) theories: a review

    David Langlois🇫🇷

    This article reviews scalar-tensor theories characterized by a Lagrangian that, despite the presence of second order derivatives, contain a single scalar degree of freedom. These theories, known as Degenerate Higher-Order Scalar-Tensor (DHOST) theories, include Horndeski and Beyond Horndeski theories. They propagate a single scalar mode as a consequence of the degeneracy of their Lagrangian and, therefore, are not plagued by an Ostrodradsky instability. They have been fully classified up to cubic order in second-order derivatives. The study of their phenomenological consequences restricts the subclass of DHOST theories that are compatible with observations. In cosmology, these theories can be described in the language of the unified effective approach to dark energy and modified gravity. Compact objects in the context of DHOST theories are also discussed.

    ↳ gr-qcastro-ph.COhep-phhep-thInt.J.Mod.Phys.D(2019)·327 citations
  30. 30*

    Derivation of spontaneously broken gauge symmetry from the consistency of effective field theory II: Scalar field self-interactions and the electromagnetic interaction

    D. Djukanovic🇩🇪 · J. Gegelia🇩🇪 · Ulf-G. Meißner🇩🇪

    We extend our study of deriving the local gauge invariance with spontaneous symmetry breaking in the context of an effective field theory by considering self-interactions of the scalar field and inclusion of the electromagnetic interaction. By analyzing renormalizability and the scale separation conditions of three-, four- and five-point vertex functions of the scalar field, we fix the two couplings of the scalar field self-interactions of the leading order Lagrangian. Next we add the electromagnetic interaction and derive conditions relating the magnetic moment of the charged vector boson to its charge and the masses of the charged and neutral massive vector bosons to each other and the two independent couplings of the theory. We obtain the bosonic part of the Lagrangian of the electroweak Standard Model as a unique solution to the conditions imposed by the self-consistency conditions of the considered effective field theory.

    ↳ hep-thhep-lathep-phnucl-thPLB(2019)·1 citation
  31. 31*

    HFLAV branching fractions fit and measurements of Vus with lepton data

    Alberto Lusiani🇮🇹

    We report the status of the Heavy Flavour Averaging Group (HFLAV) averages of the lepton measurements We then update the latest published HFLAV global fit of the lepton branching fractions (Spring 2017) with recent results by BABAR. We use the fit results to update the Cabibbo-Kobayashi-Maskawa (CKM) matrix element Vus measurements with the branching fractions. We combine the direct branching fraction measurements with indirect predictions using kaon branching fractions measurements to improve the determination of Vus using branching fractions. The Vus determinations based on the inclusive branching fraction of to strange final states are about lower than the Vus determination from the CKM matrix unitarity.

    ↳ hep-exhep-phSciPost Phys.Proc.(2019)·6 citations
  32. 32*

    Multi-Regge kinematics and the scattering equations

    Claude Duhr🇨🇭 · Zhengwen Liu🇧🇪

    We study the solutions to the scattering equations in various quasi-multi-Regge regimes where the produced particles are ordered in rapidity. We observe that in all cases the solutions to the scattering equations admit the same hierarchy as the rapidity ordering, and we conjecture that this behaviour holds independently of the number of external particles. In multi-Regge limit, where the produced particles are strongly ordered in rapidity, we determine exactly all solutions to the scattering equations that contribute to the Cachazo-He-Yuan (CHY) formula for gluon scattering in this limit. When the CHY formula is localised on these solutions, it reproduces the expected factorisation of tree-level amplitudes in terms of impact factors and Lipatov vertices. We also investigate amplitudes in various quasi-MRK. While in these cases we cannot determine the solutions to the scattering equations exactly, we show that again our conjecture combined with the CHY formula implies the factorisation of the amplitude into universal buildings blocks for which we obtain a CHY-type representation.

    ↳ hep-thhep-phJHEP(2019)·6 citations
  33. 33*

    The QCD critical point hunt: emergent new ideas and new dynamics

    Yi Yin🇺🇸

    The QCD critical point is a landmark point on the QCD phase diagram, with potential connections to a plethora of deep questions on the properties of thermal nuclear matter. Future heavy-ion collision experiments, in particular, the second phase of beam energy scan (BES-II), will explore the QCD phase diagram with an unprecedented precision and would potentially discover the QCD critical point. In this short review, I discuss and summarize recent new ideas, such as `rapidity scan', and new theoretical developments, in particular in the qualitative characterization and quantitative descriptions of the critical fluctuations in the expanding fireball. Those new ideas and developments together would enhance the prospect of locating the QCD critical point.

    ↳ nucl-thhep-ph30 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.