High Energy Physics  Phenomenology
New submissions
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New submissions for Fri, 23 Aug 19
 [1] arXiv:1908.08050 [pdf, ps, other]

Title: Effective Field Theory of Gravity to All OrdersComments: 30 pages + appendices and referencesSubjects: High Energy Physics  Phenomenology (hepph); General Relativity and Quantum Cosmology (grqc); High Energy Physics  Theory (hepth)
We construct the general effective field theory of gravity coupled to the Standard Model of particle physics, which we name GRSMEFT. Our method allows the systematic derivation of a nonredundant set of operators of arbitrary dimension with generic field content and gravity. We explicitly determine the pure gravity EFT up to dimension ten, the EFT of a shiftsymmetric scalar coupled to gravity up to dimension eight, and the operator basis for the GRSMEFT up to dimension eight. Extensions to all orders are straightforward.
 [2] arXiv:1908.08122 [pdf, other]

Title: The phase diagram of the Polyakov Nambu JonaLasinio approach for finite chemical potentialsSubjects: High Energy Physics  Phenomenology (hepph); High Energy Physics  Theory (hepth)
We extend the SU(3) (Polyakov) Nambu JonaLasinio in two ways: We introduce the next to leading order contribution (in $N_c$) in the partition function. This contribution contains explicit mesonic terms. We introduce a coupling between the gluon field and the quark degrees of freedom which goes beyond a simple rescaling of the critical temperature. With both these improvements we can reproduce, for vanishing chemical potentials, the lattice results for the thermal properties of a strongly interacting system like pressure, energy density, entropy density, interaction measure and the speed of sound. Also the expansion parameter towards small but finite chemical potentials agrees with the lattice results. Extending the calculations to finite chemical potentials (what does not require any new parameter) we find a first order phase transition up to a critical end point of $T_{CEP}= 110\ MeV$ and $\mu_q = 320\ MeV$. For very large chemical potentials, we find agreement with pQCD calculations. We calculate the mass of mesons and baryons as a function of temperature and chemical potential and the transition between the hadronic and the chirally restored phase. These calculations provide an equation of state in the whole $T,\mu$ plane an essential ingredient for dynamical calculations of ultrarelativistic heavy ion collisions but also for the physics of neutron stars and neutron star collisions.
 [3] arXiv:1908.08126 [pdf, other]

Title: Flavoured leptogenesis and ${\rm CP}^{μτ}$ symmetryComments: 31 pages, 14 figuresSubjects: High Energy Physics  Phenomenology (hepph)
We present a systematic study of leptogenesis in neutrino mass models with $\mu\tau$flavoured CP symmetry. In addition to the strong hierarchical $N_1$dominated scenario ($N_1$DS) in the `two flavour regime' of leptogenesis, we show that one may choose the righthanded (RH) neutrino mass hierarchy as mild as $M_2\simeq 4.7 M_1$ for a perfectly valid hierarchical $N_1$DS. This in turn reduces the lower bound on the allowed values of $M_1$, compared to what is stated in the literature. The consideration of flavour effects due to the heavy neutrinos also translate into an upper bound on $M_1$. It is only below this bound that the observed baryontophoton ratio can be realized for a standard ${ N_1}$ domination, else a substantial part of the parameter space is also compatible with $N_2$DS. We deduce conditions under which the baryon asymmetry produced by the second RH neutrino plays an important role. Finally, we discuss another interesting scenario where lepton asymmetry generated by $N_2$ in the two flavour regime faces washout by $N_1$ in the three flavour regime. Considering a hierarchical light neutrino mass spectrum, which is now favoured by cosmological observations, we show that at the end of $N_1$leptogenesis, the asymmetry generated by $N_2$ survives only in the electron flavour and around $33\%$ of the parameter space is consistent with a pure $N_2$leptogenesis.
 [4] arXiv:1908.08256 [pdf, other]

Title: Boosted $W/Z$ Tagging with Jet Charge and Deep LearningSubjects: High Energy Physics  Phenomenology (hepph)
We demonstrate that the classification of boosted, hadronicallydecaying weak gauge bosons can be significantly improved over traditional cutbased and BDTbased methods using deep learning and the jet charge variable. We construct binary taggers for $W^+$ vs. $W^$ and $Z$ vs. $W$ discrimination, as well as an overall ternary classifier for $W^+$/$W^$/$Z$ discrimination. Besides a simple convolutional neural network (CNN), we also explore a composite of two CNNs, with different numbers of layers in the jet $p_{T}$ and jet charge channels. We find that this novel structure boosts the performance particularly when considering the $Z$ boson as signal. The methods presented here can enhance the physics potential in SM measurements and searches for new physics that are sensitive to the electric charge of weak gauge bosons.
 [5] arXiv:1908.08263 [pdf, other]

Title: A generator of forward neutrons for ultraperipheral collisions: $\textbf{n$\mathbf{_O^O}$n}$Comments: 25 pages, 14 figuresSubjects: Nuclear Theory (nuclth); High Energy Physics  Phenomenology (hepph)
The study of photoninduced reactions in collisions of heavy nuclei at RHIC and the LHC has become an important direction of the research program of these facilities in recent years. In particular, the production of vector mesons in ultraperipheral collisions (UPC) has been intensively studied. Owing to the intense photon fluxes, the two nuclei participating in such processes undergo electromagnetic dissociation producing neutrons at beam rapidities. Here, we introduce the $\textbf{n$\mathbf{_O^O}$n}$ (pronounced noon) Monte Carlo program, which generates events containing such neutrons. $\textbf{n$\mathbf{_O^O}$n}$ is a ROOT based program that can be interfaced with existing generators of vector meson production in UPC or with theoretical calculations of such photonuclear processes. $\textbf{n$\mathbf{_O^O}$n}$ can also be easily integrated with the simulation programs of the experiments at RHIC and the LHC.
 [6] arXiv:1908.08330 [pdf, other]

Title: EWQCD interference in hadronic vector bosons at LHCComments: 10 pages, 16 figuresSubjects: High Energy Physics  Phenomenology (hepph)
The analysis of hadronic vector boson decays at LHC does not normally allow for interference with QCD production. These effects are studied here using the Sherpa package and can move by several GeV/c 2 the peak positions experiments would reconstruct. However, their impact depends strongly on the kinematics involved. The shifts expected in boosted W and Z bosons, which have been the subject of experimental study, are explored for the first time. The effects in the channels examined are all very small or negligible, but this may not true if lower transverse momenta are analysed, for example in the experimental trigger systems.
 [7] arXiv:1908.08333 [pdf, ps, other]

Title: Intrinsic threebody nuclear interaction from a constituent quark modelComments: 8 pages, 1 figureSubjects: High Energy Physics  Phenomenology (hepph); Nuclear Theory (nuclth)
We study the short distance part of the intrinsic threenucleon interaction in a constituent quark model with colorspin interaction. For that purpose we first calculate the transformation coefficient between the tribaryon configuration and their corresponding three baryon basis. Using a formula for the intrinsic threebody interaction in terms of a tribaryon configuration, we find that after subtracting the corresponding twobaryon contributions, the intrinsic threebody interaction vanishes in flavor SU(3) symmetric limit for all quantum numbers for the three nucleon states. We further find that the intrinsic threebody interaction also vanishes for flavorspin type of quark interaction.
 [8] arXiv:1908.08353 [pdf, other]

Title: CIMBA: fast Monte Carlo generation using cubic interpolationAuthors: Philip IltenComments: 16 pages, 6 figuresSubjects: High Energy Physics  Phenomenology (hepph); High Energy Physics  Experiment (hepex)
Monte Carlo generation of high energy particle collisions is a critical tool for both theoretical and experimental particle physics, connecting perturbative calculations to phenomenological models, and theory predictions to full detector simulation. The generation of minimum bias events can be particularly computationally expensive, where nonperturbative effects play an important role and specific processes and fiducial regions can no longer be well defined. In particular scenarios, particle guns can be used to quickly sample kinematics for single particles produced in minimum bias events. CIMBA (Cubic Interpolation for Minimum Bias Approximation) provides a comprehensive package to smoothly sample predefined kinematic grids, from any general purpose Monte Carlo generator, for all particles produced in minimum bias events. These grids are provided for a number of beam configurations including those of the Large Hadron Collider.
 [9] arXiv:1908.08355 [pdf, other]

Title: Towards the meV limit of the effective neutrino mass in neutrinoless doublebeta decaysAuthors: Jun Cao, Guoyuan Huang, YuFeng Li, Yifang Wang, LiangJian Wen, Zhizhong Xing, Zhenhua Zhao, Shun ZhouComments: 16 pages, 6 figuresSubjects: High Energy Physics  Phenomenology (hepph); High Energy Physics  Experiment (hepex)
In this paper, we emphasize why it is important for future neutrinoless doublebeta ($0\nu\beta\beta$) decay experiments to reach the sensitivity to the effective neutrino mass $m^{}_{\beta\beta} \approx 1~{\rm meV}$. Assuming such a sensitivity and the precisions on neutrino oscillation parameters after the JUNO experiment, we fully explore the constrained regions of the lightest neutrino mass $m^{}_1$ and two Majoranatype CPviolating phases $\{\rho, \sigma\}$. The implications for the neutrino mass spectrum, the effective neutrino mass $m^{}_\beta$ in beta decays and the sum of three neutrino masses $\Sigma \equiv m^{}_1 + m^{}_2 + m^{}_3$ relevant for cosmological observations are also discussed.
 [10] arXiv:1908.08363 [pdf, other]

Title: Renormalization group improved pressure for cold and dense QCDComments: 16 pages and 7 figuresSubjects: High Energy Physics  Phenomenology (hepph); High Energy Physics  Theory (hepth); Nuclear Theory (nuclth)
We apply the renormalization group optimized perturbation theory (RGOPT)to evaluate the QCD (matter) pressure at the twoloop level considering three flavors of massless quarks in a dense and cold medium. Already at leading order ($\alpha_s^0$), which builds on the simple one loop (RG resummed) term, our technique provides a nontrivial nonperturbative approximation which is completely renormalization group invariant. At the nexttoleading order the comparison between the RGOPT and the pQCD predictions shows that the former method provides results which are in better agreement with the stateoftheart $higher \, order$ perturbative results, which include a contribution of order $\alpha_s^3 \ln^2 \alpha_s$. At the same time one also observes that the RGOPT predictions are less sensitive to variations of the arbitrary $\overline {\rm MS}$ renormalization scale than those obtained with pQCD. These results indicate that the RGOPT provides an efficient resummation scheme which may be considered as an alternative to lattice simulations at high baryonic densities.
 [11] arXiv:1908.08387 [pdf, ps, other]

Title: Neutrino Mass Spectrum for CoBimaximal Mixings from Quantum GravityAuthors: Bipin Singh Koranga (Department of Physics, Kirori Mal college, University of Delhi, India)Comments: 10 pages. arXiv admin note: substantial text overlap with arXiv:1006.5553, arXiv:0810.4394Journalref: Int. J. Modern Theo. Physics, 2019, 8(1)Subjects: High Energy Physics  Phenomenology (hepph)
We consider nonrenormalizable interaction term as a perturbation of the conventional neutrino mass matrix. Quantum gravitational (Planck scale )effects lead to an effective $SU(2)_L\times U(1)$ invariant dimension5 Lagrangian involving neutrino and Higgs fields,On symmetry breaking, this operator gives rise to correction to the neutrino masses and mixing. The gravitational interaction $M_X=M_{pl}$ which gives rise to additional terms in neutrino mass matrix. We also assume that, just above the electroweak breaking scale, neutrino masses are nearly degenerate and their mixing is Cobimaximal mixing by assuming mixing angle $\theta_{13}\neq0 = 10^{o}$, $\theta_{23}=\frac{\pi}{4}$, $\tan\theta_{12}^ 2 = \frac{13sin\theta_{13}^2}{2} = 34^{o}$ and Dirac phase $\delta=\pm\frac{\pi}{2}$.There additional term can be considered to be perturbation of the GUT scale Cobimaximal neutrino mass matrix. The relation consider with solar and atmospheric neutrino oscillation data predicted above GUT scale $m_1' \simeq 0.00001eV0.00003eV$, $m_2' \simeq 0.00008eV0.00012$, and $m_3' \simeq 0.000207eV000320eV$.
 [12] arXiv:1908.08398 [pdf, other]

Title: How to include exclusive $J/ψ$ production data in global PDF analysesComments: 14 pages, 6 figuresSubjects: High Energy Physics  Phenomenology (hepph)
We compare the cross section for exclusive $J/\psi$ photoproduction calculated at NLO in the collinear factorization approach with HERA and LHCb data. Using the optimum scale formalism together with the subtraction of the low $k_t<Q_0$ contribution from the NLO coefficient function to avoid double counting we show that the existing global parton distribution functions (PDFs) are consistent with the data within their uncertainties. However, at low $x$ the uncertainties of the present global PDFs are large. On the other hand, the accuracy of the LHCb data are rather good. Therefore, these data provide the possibility to directly measure the gluon PDF over the very large interval of $x$, $10^{6}<x<10^{2}$, at a fixed low scale.
 [13] arXiv:1908.08409 [pdf, ps, other]

Title: Neutrino mass model with a modular $S_4$ symmetryComments: 13 pages, 3 figures, 2 tables. arXiv admin note: text overlap with arXiv:1908.07457, arXiv:1907.04716, arXiv:1907.13520Subjects: High Energy Physics  Phenomenology (hepph)
We propose a predictive lepton model under a modular $S_4$ symmetry, and the neutrino mass matrix arises from a combination of canonical seesaw at tree level and radiative seesaw at oneloop level. Supposing the Majorana neutrino to be embedded into doublet under $S_4$, the lightest neutrino mass is zero. In addition, we show predictions for phases, mixings, and masses such as the effective mass for the neutrinoless double beta decay and the total mass of neutrinos that originate from the specific textures due to the assignment of $S_4$ and its modular weight. The modular weight also plays an important role in stabilizing the DM candidate.
 [14] arXiv:1908.08417 [pdf, other]

Title: $keV$ scale dark matter, baryogenesis and neutrinoless double beta decay in minimal extended seesawComments: 34 pages, 10 figuresSubjects: High Energy Physics  Phenomenology (hepph)
We have studied $keV$ scale dark matter (DM), neutrinoless double beta decay (NDBD) and baryogenesis within minimal extended seesaw (MES). A generic model based on $A_4\times Z_4$ flavor symmetry is used to explain both normal and inverted hierarchy mass pattern of neutrino and also to accommodate the $keV$ ranged sterile netrino mass. Significant results on effective neutrino mass are observed in presence of $keV$ sterile neutrino in NDBD. In order to validate DM within this model, we have checked decay width and relic abundance of the heavy neutrino flavor and which constrained sterile neutrino DM mass. Baryogenesis is also studied simultaneously within this framework and Dirac CP phase get constrained with the results. Corelation among the observable and model parameters are also carried out within this framework.
 [15] arXiv:1908.08455 [pdf, other]

Title: Nucleonantinucleon annihilation at LEARAuthors: Claude AmslerComments: 27 pages, 29 figures, Invited talk at the ECT* workshop on Antiprotonnucleus interactions and related phenomenaSubjects: High Energy Physics  Phenomenology (hepph); Nuclear Experiment (nuclex); Nuclear Theory (nuclth)
This report is a historical review of the salient results in low energy antiprotonproton and antineutronproton annihilation obtained at the Low Energy Antiproton Ring (LEAR), which was operated at CERN between 1983 and 1996. The intention is to provide guidelines for future experiments at the CERN AD/ELENA complex and elsewhere. In the spirit of this workshop, hadron spectroscopy  one of the cornerstones at LEAR  is briefly mentioned, while emphasis is put on the annihilation mechanism on one and two nucleons, the final state multiplicity distributions and the contributions from quarks, in particular in annihilation channels involving strangeness.
 [16] arXiv:1908.08524 [pdf, other]

Title: Dynamical resolution scale in transverse momentum distributions at the LHCComments: 16 pages, 7 figuresSubjects: High Energy Physics  Phenomenology (hepph)
The QCD evolution of transverse momentum dependent (TMD) distribution functions has recently been formulated in a parton branching (PB) formalism. In this approach, softgluon coherence effects are taken into account by introducing the softgluon resolution scale and exploiting the relation between transversemomentum recoils and branching scales. In this work we investigate the implications of dynamical, i.e., branching scale dependent, resolution scales. We present both analytical studies and numerical solution of PB evolution equations in the presence of dynamical resolution scales. We use this to compare PB results with other approaches in the literature, and to analyze predictions for transverse momentum distributions in $Z$boson production at the Large Hadron Collider (LHC).
Crosslists for Fri, 23 Aug 19
 [17] arXiv:1908.08081 (crosslist from heplat) [pdf, ps, other]

Title: Particles propagation on a torusAuthors: Peng GuoSubjects: High Energy Physics  Lattice (heplat); Strongly Correlated Electrons (condmat.strel); High Energy Physics  Phenomenology (hepph)
Based on variational principle and Faddeev method, we present a general framework toward finding propagating solutions of multiple interacting particles on a torus. Two different versions of multiple particles secular equations are presented. Version one shows a close relation between propagating solutions on a torus and infinite volume dynamics. Second may be more suitable and robust for the task of lattice QCD data analysis. The proposed formalism may also be useful for the study of fewbody interaction effect on electronic band structure in condensed matter physics.
 [18] arXiv:1908.08149 (crosslist from astroph.HE) [pdf, ps, other]

Title: Xray Intraday Variability of the TeV Blazar Mrk 421 with SuzakuAuthors: Zhongli Zhang, Alok C. Gupta, Haritma Gaur, Paul J. Wiita, Tao An, Minfeng Gu, Dan Hu, Haiguang XuComments: 16 pages, 3 figures, 3 tables, accepted by ApJSubjects: High Energy Astrophysical Phenomena (astroph.HE); High Energy Physics  Phenomenology (hepph)
We present Xray flux and spectral analyses of the three pointed Suzaku observations of the TeV high synchrotron peak blazar Mrk 421 taken throughout its complete operational duration. The observation taken on 5 May 2008 is, at 364.6 kiloseconds (i.e., 101.3 hours), the longest and most evenly sampled continuous observation of this source, or any blazar, in the Xray energy 0.8  60 keV until now. We found large amplitude intraday variability in all soft and hard bands in all the light curves. The discrete correction function analysis of the light curves in soft and hard bands peaks on zero lag, showing that the emission in hard and soft bands are cospatial and emitted from the same population of leptons. The hardness ratio plots imply that the source is more variable in the harder bands compared to the softer bands. The source is harderwhenbrighter, following the general behavior of high synchrotron peak blazars. Power spectral densities of all three light curves are red noise dominated, with a range of power spectra slopes. If one assumes that the emission originates very close to the central super massive black hole, a crude estimate for its mass, of ~ 4 * 10^{8} M_{\odot}, can be made; but if the variability is due to perturbations arising there that are advected into the jet and are thus Doppler boosted, substantially higher masses are consistent with the quickest seen variations. We briefly discuss the possible physical mechanisms most likely responsible for the observed flux and spectral variability.
 [19] arXiv:1908.08189 (crosslist from quantph) [pdf, ps, other]

Title: Electronpositron pair production in frequency modulated laser fieldsComments: 8 pages, 6 figuresSubjects: Quantum Physics (quantph); High Energy Physics  Phenomenology (hepph)
The momentum spectrum and the number density of created electronpositron pairs in a frequency modulated laser field are investigated using quantum kinetic equation. It is found that the momentum spectrum presents obvious interference pattern. This is an imprint of the frequency modulated field on the momentum spectrum, because the momentum peaks correspond to the pair production process by absorbing different frequency component photons. Moreover, the interference effect can also be understood qualitatively by analyzing turning point structures. The study of the pair number density shows that the number density is very sensitive to modulation parameters and can be enhanced by over two orders of magnitude for certain modulation parameters, which may provide a new way to increase the number of created electronpositron pairs in future experiments.
 [20] arXiv:1908.08236 (crosslist from astroph.HE) [pdf, other]

Title: Dark matter searches with the IceCube UpgradeAuthors: Sebastian Baur (for the IceCube Collaboration)Comments: Presented at the 36th International Cosmic Ray Conference (ICRC 2019). See arXiv:1907.11699 for all IceCube contributionsSubjects: High Energy Astrophysical Phenomena (astroph.HE); High Energy Physics  Phenomenology (hepph)
Weakly Interacting Massive Particles (WIMPs) are wellmotivated candidates for Dark Matter (DM). WIMP models often include selfannihilation into Standard Model particles such as neutrinos which could potentially be detected by the IceCube Neutrino Observatory. Various searches for a dark matter induced signal have been performed with the existing IceCube detector. However, since there is so far no evidence for WIMPs at TeV scales, more attention is brought to DM candidates at GeV masses, for which the IceCube detector is not sensitive due to its energy threshold. The IceCube collaboration is currently preparing the construction of the IceCube Upgrade which is planned to be deployed in the 2022/2023 South Pole summer season. The IceCube Upgrade will consist of 7 new inice strings with about 700 additional optical sensors. This dense sensor array inside the IceCubeDeepCore volume will enhance the reconstruction capability of fewGeV neutrinos. We present first studies on the potential improvements of this upgrade on IceCube's sensitivity to Dark Matter annihilating in the Galactic Center.
 [21] arXiv:1908.08421 (crosslist from astroph.HE) [pdf, ps, other]

Title: Multimessenger tests of cosmicray acceleration in radiatively inefficient accretion flowsComments: 15 pages, 6 figures, 3 tablesSubjects: High Energy Astrophysical Phenomena (astroph.HE); High Energy Physics  Phenomenology (hepph)
The cores of active galactic nuclei (AGNs) have been suggested as the sources of IceCube neutrinos, and recent numerical simulations have indicated that hot AGN coronae of Seyfert galaxies and radiatively inefficient accretion flows (RIAFs) of lowluminosity AGNs (LLAGNs) may be promising sites of ion acceleration. We present detailed studies on detection prospects of highenergy multimessenger emissions from RIAFs in nearby LLAGNs. We construct a model of RIAFs that can reproduce the observational features of the current Xray observations of nearby LLAGNs. We then calculate the highenergy particle emissions from nearby individual LLAGNs, including MeV gamma rays from thermal electrons, TeVPeV neutrinos produced by nonthermal protons, and subGeV to subTeV gamma rays from protoninduced electromagnetic cascades. We find that, although these are beyond the reach of current facilities, proposed future experiments such as eASTROGAM and IceCubeGen2 should be able to detect the MeV gamma rays and the neutrinos, respectively, or else they can place meaningful constraints on the parameter space of the model. On the other hand, the detection of highenergy gamma rays due to the electromagnetic cascades will be challenging with the current and nearfuture experiments, such as Fermi and Cherenkov Telescope Array. In an accompanying paper, we demonstrate that LLAGNs can be a source of the diffuse soft gammaray and TeVPeV neutrino backgrounds, whereas in the present paper, we focus on the prospects for multimessenger tests which can be applied to reveal the nature of the highenergy neutrinos and photons from LLAGNs.
 [22] arXiv:1908.08437 (crosslist from heplat) [pdf, other]

Title: Thermal Broadening of Bottomonia: Lattice NonRelativistic QCD with Extended OperatorsSubjects: High Energy Physics  Lattice (heplat); High Energy Physics  Phenomenology (hepph); Nuclear Theory (nuclth)
We present lattice nonrelativistic QCD calculations of bottomonia correlation functions at temperatures $T \simeq 150350$ MeV. The correlation functions were computed using extended bottomonia operators, and on background gaugefield configurations for 2+1flavor QCD having physical kaon and nearlyphysical pion masses. We analyzed these correlation functions based on simple theoreticallymotivated parameterizations of the corresponding spectral functions. The results of our analyses are compatible with significant inmedium thermal broadening of the ground state S and Pwave bottomonia.
 [23] arXiv:1908.08477 (crosslist from astroph.CO) [pdf, other]

Title: Using SPTpol, Planck 2015, and nonCMB data to constrain tilted spatiallyflat and untilted nonflat $Λ$CDM, XCDM, and $φ$CDM dark energy inflation cosmologiesComments: 24 pages, 14 figures, 6 tablesSubjects: Cosmology and Nongalactic Astrophysics (astroph.CO); General Relativity and Quantum Cosmology (grqc); High Energy Physics  Phenomenology (hepph); High Energy Physics  Theory (hepth)
We use six tilted spatiallyflat and untilted nonflat dark energy cosmological models in analyses of South Pole Telescope polarization (SPTpol) cosmic microwave background (CMB) data, alone and in combination with Planck 2015 CMB data and nonCMB data. All bestfit cosmological models have CMB anisotropy power spectra that do not provide good fits to the SPTpol data, differing at the 2 to 3$\sigma$ level. In all models, there is no significant difference between the model that best fits the SPTpol data and the one that best fits the Planck CMB and nonCMB data. When the smaller angular scale SPTpol data are used jointly with either the Planck data alone or with the Planck CMB and the nonCMB data to constrain untilted nonflat models, spatiallyclosed models remain favored over their corresponding flat limits. When used in conjunction with Planck data, nonCMB data (baryon acoustic oscillation measurements in particular, from six experiments) have significantly more constraining power than the SPTpol data.
Replacements for Fri, 23 Aug 19
 [24] arXiv:1809.06385 (replaced) [pdf, ps, other]

Title: How high is the neutrino floor?Comments: 10 pages, 3 figures. Author addedSubjects: High Energy Physics  Phenomenology (hepph); Cosmology and Nongalactic Astrophysics (astroph.CO)
 [25] arXiv:1811.12612 (replaced) [pdf, other]

Title: An analytical approach to the field amplification and particle production by parametric resonance during inflation and reheatingComments: 6 pages, 3 figures; v2: some typos are corrected, added two references; v3: 10 pages, some discussions are largely expanded, version to appear at Physics of the Dark UniverseSubjects: High Energy Physics  Phenomenology (hepph); General Relativity and Quantum Cosmology (grqc); High Energy Physics  Theory (hepth)
 [26] arXiv:1812.11931 (replaced) [pdf, ps, other]

Title: Probing the seesaw mechanism at the 250 GeV ILCComments: 8 pages, 4 figures, the version published in Phys. Lett. B (typos in Table III & IV have been corrected after the publication)Subjects: High Energy Physics  Phenomenology (hepph); High Energy Physics  Experiment (hepex)
 [27] arXiv:1812.11968 (replaced) [pdf, other]

Title: New Higher Anomalies, SU(N) YangMills Gauge Theory and $\mathbb{CP}^{\mathrm{N}1}$ Sigma ModelComments: 53 pages, two columns. v4: Refinement. Sec IX provides the symmetryextended TQFTs; while the symmetrypreserving TQFTs actually become spontaneously symmetrybreaking, agreed with CordovaOhmori's work. See companions arXiv:1812.11967 and arXiv:1904.00994Subjects: High Energy Physics  Theory (hepth); Strongly Correlated Electrons (condmat.strel); High Energy Physics  Lattice (heplat); High Energy Physics  Phenomenology (hepph); Algebraic Topology (math.AT)
 [28] arXiv:1902.08187 (replaced) [pdf, other]

Title: When Primordial Black Holes from Sound Speed Resonance Meet a Stochastic Background of Gravitational WavesComments: 14 pages,5 figuresJournalref: Phys. Rev. D 100, 043518 (2019)Subjects: Cosmology and Nongalactic Astrophysics (astroph.CO); General Relativity and Quantum Cosmology (grqc); High Energy Physics  Phenomenology (hepph); High Energy Physics  Theory (hepth)
 [29] arXiv:1903.05931 (replaced) [pdf, ps, other]

Title: Semileptonic decays of the scalar tetraquark $Z_{bc;\overline{u} \overline{d}}^{0}$Comments: 10 Pages and 3 FiguresSubjects: High Energy Physics  Phenomenology (hepph); High Energy Physics  Experiment (hepex); High Energy Physics  Lattice (heplat)
 [30] arXiv:1904.09996 (replaced) [pdf, ps, other]

Title: Observing Supernova Neutrino Light Curves with SuperKamiokande: Expected Event Number over 10 sAuthors: Yudai Suwa (Kyoto Sangyo Univ. & YITP, Kyoto Univ.), Kohsuke Sumiyoshi (NIT, Numazu College), Ken'ichiro Nakazato (Kyushu Univ.), Yasufumi Takahira, Yusuke Koshio (Okayama Univ.), Masamitsu Mori, Roger A. Wendell (Kyoto Univ.)Comments: 16 pages, 14 figures, 2 tables, matched to published versionJournalref: The Astrophysical Journal, 881, 139 (2019)Subjects: High Energy Astrophysical Phenomena (astroph.HE); Solar and Stellar Astrophysics (astroph.SR); High Energy Physics  Phenomenology (hepph)
 [31] arXiv:1905.01291 (replaced) [pdf, other]

Title: Nucleon isovector charges and twist2 matrix elements with $N_f=2+1$ dynamical Wilson quarksAuthors: Tim Harris, Georg von Hippel, Parikshit Junnarkar, Harvey B. Meyer, Konstantin Ottnad, Jonas Wilhelm, Hartmut Wittig, Linus WrangComments: 35 pages, 13 figures; matching version accepted for publication in PRDJournalref: Phys. Rev. D 100, 034513 (2019)Subjects: High Energy Physics  Lattice (heplat); High Energy Physics  Phenomenology (hepph); Nuclear Theory (nuclth)
 [32] arXiv:1905.06299 (replaced) [pdf, other]

Title: Modelindependent formfactor constraints for electromagnetic spin1 currentsAuthors: Helmut HaberzettlComments: Slightly revised version, as published in PRD. This version corrects an erroneous statement in the first version based on a numerical errorJournalref: Phys. Rev. D 100, 036008 (2019)Subjects: Nuclear Theory (nuclth); High Energy Physics  Phenomenology (hepph)
 [33] arXiv:1905.06775 (replaced) [pdf, other]

Title: The onset of $ΛΛ$ hypernuclear bindingComments: v2  14 pages, 4 figures, 1 table, slightly revised, accepted for publication in PLBSubjects: Nuclear Theory (nuclth); High Energy Physics  Phenomenology (hepph); Nuclear Experiment (nuclex)
 [34] arXiv:1906.02677 (replaced) [pdf, other]

Title: A First Look on 3D Effects in Open Axion HaloscopesAuthors: Stefan Knirck, Jan SchütteEngel, Alexander J. Millar, Javier Redondo, Olaf Reimann, Andreas Ringwald, Frank D. SteffenComments: 41 pages, 20 figures; typos corrected, references updatedJournalref: JCAP08(2019)026Subjects: Instrumentation and Detectors (physics.insdet); High Energy Physics  Experiment (hepex); High Energy Physics  Phenomenology (hepph)
 [35] arXiv:1906.08768 (replaced) [pdf, other]

Title: Explaining electron and muon $g2$ anomaly in SUSY without leptonflavor mixingsComments: 14 pages, 4 figures, 2 tables, v2: version to appear in JHEPSubjects: High Energy Physics  Phenomenology (hepph)
 [36] arXiv:1906.09930 (replaced) [pdf, other]

Title: Dark matter as Planck relics without too exotic hypothesesSubjects: High Energy Physics  Phenomenology (hepph); Cosmology and Nongalactic Astrophysics (astroph.CO); General Relativity and Quantum Cosmology (grqc)
 [37] arXiv:1906.10890 (replaced) [pdf, other]

Title: Multiscale Mining of Kinematic Distributions with WaveletsComments: 21 pages, 8 figures. KWAK package available at this https URLSubjects: High Energy Physics  Phenomenology (hepph)
 [38] arXiv:1907.00413 (replaced) [pdf, other]

Title: Heavy ion anisotropies: a closer look at the angular power spectrumAuthors: Meera MachadoSubjects: High Energy Physics  Phenomenology (hepph)
 [39] arXiv:1907.11193 (replaced) [pdf, other]

Title: Searches for Connections Between Dark Matter and Neutrinos with the IceCube HighEnergy Starting Event SampleComments: Presented at the 36th International Cosmic Ray Conference (ICRC 2019). See arXiv:1907.11699 for all IceCube contributions, 6 pages, 2 figuresSubjects: High Energy Physics  Phenomenology (hepph); High Energy Physics  Experiment (hepex)
 [40] arXiv:1908.04740 (replaced) [pdf, other]

Title: Firstorder phase transition from hypernuclear matter to deconfined quark matter obeying new constraints from compact star observationsComments: 33 pages, 12 figures, 1 table, references added, text updatedSubjects: Nuclear Theory (nuclth); High Energy Astrophysical Phenomena (astroph.HE); High Energy Physics  Phenomenology (hepph)
 [41] arXiv:1908.07602 (replaced) [pdf, other]

Title: Quest for new physics using astrophysical neutrino flavor in IceCubeAuthors: Carlos A. Argüelles, Kareem Farrag, Teppei Katori, Shivesh Mandalia (for the IceCube Collaboration)Comments: Presented at the 36th International Cosmic Ray Conference (ICRC 2019). See arXiv:1907.11699 for all IceCube contributions. 8 Pages, 2 FiguresSubjects: High Energy Astrophysical Phenomena (astroph.HE); High Energy Physics  Experiment (hepex); High Energy Physics  Phenomenology (hepph)
 [42] arXiv:1908.07911 (replaced) [pdf, other]

Title: Consistent largescale shellmodel analysis of the twoneutrino $ββ$ and single $β$ branchings in $^{48}\rm Ca$ and $^{96}\rm Zr$Comments: 13 pages, 8 figuresSubjects: Nuclear Theory (nuclth); High Energy Physics  Phenomenology (hepph)
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