PaperPanorama

HEP Phenomenology·hep-ph

Tue·Apr 5, 2016

38 papers20 primary·18 cross-listed·reconstructed*

  1. 01*

    An Exponential Regulator for Rapidity Divergences

    Ye Li🇺🇸 · Duff Neill🇺🇸 · Hua Xing Zhu🇺🇸

    Finding an efficient and compelling regularization of soft and collinear degrees of freedom at the same invariant mass scale, but separated in rapidity is a persistent problem in high-energy factorization. In the course of a calculation, one encounters divergences unregulated by dimensional regularization, often called rapidity divergences. Once regulated, a general framework exists for their renormalization, the rapidity renormalization group (RRG), leading to fully resummed calculations of transverse momentum (to the jet axis) sensitive quantities. We examine how this regularization can be implemented via a multi-differential factorization of the soft-collinear phase-space, leading to an (in principle) alternative non-perturbative regularization of rapidity divergences. As an example, we examine the fully-differential factorization of a color singlet's momentum spectrum in a hadron-hadron collision at threshold. We show how this factorization acts as a mother theory to both traditional threshold and transverse momentum resummation, recovering the classical results for both resummations. Examining the refactorization of the transverse momentum beam functions in the threshold region, we show that one can directly calculate the rapidity renormalized function, while shedding light on the structure of joint resummation. Finally, we show how using modern bootstrap techniques, the transverse momentum spectrum is determined by an expansion about the threshold factorization, leading to a viable higher loop scheme for calculating the relevant anomalous dimensions for the transverse momentum spectrum.

    hep-phnucl-thNPB(2020)·173 citations
  2. 02*

    Polarization observables for millicharged particles in photon collisions

    Emidio Gabrielli🇮🇹 · Luca Marzola🇪🇪 · Edoardo Milotti🇮🇹 · Hardi Veermäe🇪🇪

    Particles in a hidden sector can potentially acquire a small electric charge through their interaction with the Standard Model and can consequently be observed as millicharged particles. We systematically compute the production of millicharged scalar, fermion and vector boson particles in collisions of polarized photons. The presented calculation is model independent and is based purely on the assumptions of electromagnetic gauge invariance and unitarity. Polarization observables are evaluated and analyzed for each spin case. We show that the photon polarization asymmetries are a useful tool for discriminating between the spins of the produced millicharged particles. Phenomenological implications for searches of millicharged particles in dedicated photon-photon collision experiments are also discussed.

    hep-phPRD(2016)·5 citations
  3. 03*

    Numerical multi-loop integrals and applications

    Ayres Freitas🇺🇸

    Higher-order radiative corrections play an important role in precision studies of the electroweak and Higgs sector, as well as for the detailed understanding of large backgrounds to new physics searches. For corrections beyond the one-loop level and involving many independent mass and momentum scales, it is in general not possible to find analytic results, so that one needs to resort to numerical methods instead. This article presents an overview over a variety of numerical loop integration techniques, highlighting their range of applicability, suitability for automatization, and numerical precision and stability. In a second part of this article, the application of numerical loop integration methods in the area of electroweak precision tests is illustrated. Numerical methods were essential for obtaining full two-loop predictions for the most important precision observables within the Standard Model. The theoretical foundations for these corrections will be described in some detail, including aspects of the renormalization, resummation of leading loop contributions, and the evaluation of the theory uncertainty from missing higher orders.

    hep-phPPNP(2016)·46 citations
  4. 04*

    Stop searches in flavourful supersymmetry

    Andreas Crivellin🇨🇭 · Ulrich Haisch🇬🇧 · Lewis C. Tunstall🇨🇭

    Natural realisations of supersymmetry require light stops , making them a prime target of LHC searches for physics beyond the Standard Model. Depending on the kinematic region, the main search channels are , and . We first examine the interplay of these decay modes with in a model-independent fashion, revealing the existence of large regions in parameter space which are excluded for any branching ratio. This effect is then illustrated for scenarios with stop-scharm mixing in the right-handed sector, where it has previously been observed that the stop mass limits can be significantly weakened for large mixing. Our analysis shows that once the LHC bounds from searches are taken into account, non-zero stop-scharm mixing leads only to a modest increase in the allowed regions of parameter space, with large areas excluded for arbitrary mixing angles.

    hep-phhep-exJHEP(2016)·3 citations
  5. 05*

    Adler function and Bjorken polarized sum rule: Perturbation expansions in powers of conformal anomaly and studies of the conformal symmetry limit

    Gorazd Cvetič🇨🇱 · A.L. Kataev🇷🇺

    We consider a new form of analytical perturbation theory expansion in the massless theory, for the non-singlet part of the -annihilation to hadrons Adler function and of the Bjorken sum rule of the polarized lepton-hadron deep-inelastic scattering , and demonstrate its validity at the -level at least. It is a two-fold series in terms of powers of the conformal anomaly and of coupling . Explicit expressions are obtained for the -expanded perturbation coefficients at level in scheme, for both considered physical quqantities. Comparisons of the terms in the -expanded coefficients are made with the corresponding terms obtained by using extra gluino degrees of freedom, or skeleton-motivated expansion, or -scheme motivated expansion in the Principle of Maximal Conformality. Relations between terms of the -expansion for the - and -functions, which follow from the conformal symmetry limit and its violation, are presnted. The relevance to the possible new analysis of the experimental data for the Adler function and Bjorken sum rule is discussed.

    hep-phhep-exhep-thPRD(2016)·20 citations
  6. 06*

    Reliability of the optimized perturbation theory in the 0-dimensional scalar field model

    Dérick S. Rosa🇧🇷 · R. L. S. Farias🇧🇷 · Rudnei O. Ramos🇧🇷

    We address the reliability of the Optimized Perturbation Theory (OPT) in the context of the 0-dimensional scalar field model. The effective potential, the self-energy and the 1PI four-point Green's function for the model are computed using different optimization schemes and the results contrasted to the exact results for the model. Our results are also compared to those obtained with the -expansion and with those from ordinary perturbation theory. The OPT results are shown to be stable even at large couplings and to have better convergence properties than the ones produced in the -expansion. It is also shown that the principle of minimal sensitive optimization procedure used in conjunction with the OPT method tends to always produce better results, in particular when applied directly to the self-energy.

    hep-phPhysica A(2016)·16 citations
  7. 07*

    Mass spectra of dimesonic states in light flavour sector

    D P Rathaud🇮🇳 · A K Rai🇮🇳

    Masses of the dimesonic (meson-antimeson) molecular states are calculated using Yukawa like and meson exchange potential in semi-relativistic approach. The digamma decay width of the dimesonic systems are evaluated using the spectroscopic parameters. Many states such as (980), (1380), (1450), (1500), (1525), (1565), (1700), (1710), (1810), (2010) have shown the signature of dimesonic molecules. Their masses and digamma widths are in good agreement with other theoretical results as well as experimental measurements.

    hep-phIndian J.Phys.(2016)·21 citations
  8. 08*

    Production of Heavy neutrino in next-to-leading order QCD at the LHC and beyond

    Arindam Das🇺🇸 · Partha Konar🇮🇳 · Swapan Majhi🇮🇳

    Majorana and pseudo-Dirac heavy neutrinos are introduced into the type-I and inverse seesaw models, respectively, in explaining the naturally small neutrino mass. TeV scale heavy neutrinos can also be accommodated to have a sizable mixing with the Standard Model light neutrinos, through which they can be produced and detected at the high energy colliders. In this paper we consider the Next-to-Leading Order QCD corrections to the heavy neutrino production, and study the scale variation in cross-sections as well as the kinematic distributions with different final states at TeV LHC and also in the context of TeV hadron collider. The repertoire of the Majorana neutrino is realized through the characteristic signature of the same-sign dilepton pair, whereas, due to a small lepton number violation, the pseudo-Dirac heavy neutrino can manifest the trileptons associated with missing energy in the final state. Using the TeV, fb and fb data at the ATLAS and CMS respectively, we obtain prospective scale dependent upper bounds of the light-heavy neutrino mixing angles for the Majorana heavy neutrinos at the TeV LHC and TeV collider. Further exploiting a recent study on the anomalous multilepton search by CMS at TeV with fb data, we also obtain the prospective scale dependent upper bounds on the mixing angles for the pseudo-Dirac neutrinos. We thus project a scale dependent prospective reach using the NLO processes at the TeV LHC.

    hep-phhep-exJHEP(2016)·120 citations
  9. 09*

    CP Violation in the scalar sector

    D. Emmanuel-Costa🇵🇹 · O. M. Ogreid🇳🇴 · P. Osland🇳🇴 · M. N. Rebelo🇵🇹

    Models with an extended scalar sector may in principle provide new sources of CP violation originating in the scalar potential. One of the simplest ways to implement this idea is to have CP violation in a two-Higgs-doublet model. Here, it leads to CP violation in trilinear weak gauge boson couplings. We discuss how these couplings are becoming constrained in the alignment limit. In a model with three Higgs doublets, subject to an symmetry, several complex vacua are possible. Some of these, but not all, may lead to spontaneous CP violation.

    hep-phPoS(2016)·2 citations
  10. 10*

    Nonrelativistic Effective Field Theory for Axions

    Eric Braaten🇺🇸 · Abhishek Mohapatra🇺🇸 · Hong Zhang🇺🇸

    Axions can be described by a relativistic field theory with a real scalar field whose self-interaction potential is a periodic function of . Low-energy axions, such as those produced in the early universe by the vacuum misalignment mechanism, can be described more simply by a nonrelativistic effective field theory with a complex scalar field whose effective potential is a function of . We determine the coefficients in the expansion of the effective potential to fifth order in by matching low-energy axion scattering amplitudes. In order to describe a Bose-Einstein condensate of axions that is too dense to expand the effective potential in powers of , we develop a sequence of systematically improvable approximations to the effective potential that include terms of all orders in .

    hep-phPRD(2016)·48 citations
  11. 11*

    Axionic domain wall number related to U(1) global symmetry

    Jihn E. Kim🇰🇷

    The QCD axion with at an intermediate scale, 10**9-10**12 GeV, seems in conflict with the gravity spoil of global symmetries and may face the axionic domain wall problem. We point out that the string compactifications with an anomalous U(1) gauge symmetry, allowing desirable chiral matter spectra, circumvent these two problems simultaneously.

    hep-phastro-ph.COhep-thPLB(2016)·11 citations
  12. 12*

    750 GeV Diphoton Resonance in a Vector-like Extension of Hill Model

    Ning Liu🇨🇳 · Wenyu Wang🇨🇳 · Mengchao Zhang🇨🇳 · Rui Zheng🇺🇸

    In this paper, we study the recent 750 GeV diphoton excess in the Hill Model with vector-like fermions, in which the singlet-like Higgs boson is chosen as 750 GeV resonance and is mainly produced by the gluon fusion through vector-like top and bottom quarks. Meanwhile its diphoton decay rate is greatly enhanced by the vector-like lepton. Under the current experimental and theoretical constraints, we present the viable parameter space that fits the 750 GeV diphoton signal strength at 13 TeV LHC. We find that the heavier vector-like fermion masses are, the smaller mixing angle is required. The mixing angle of singlet and doublet Higgs bosons is constrained within in the condition of the perturbative Yukawa couplings. In the allowed parameter space, the 750 GeV diphoton cross section can be maximally enhanced to about 6 fb at 13 TeV LHC.

    hep-phhep-exInt.J.Mod.Phys.A(2016)·11 citations
  13. 13*

    Gamma rays from muons from WIMPs: Implementation of radiative muon decays for dark matter analyses

    Andre Scaffidi🇦🇺 · Katherine Freese🇸🇪 · Jinmian Li🇦🇺 · Christopher Savage🇸🇪 · Martin White🇦🇺 · Anthony G. Williams🇦🇺

    Dark matter searches in gamma ray final states often make use of the fact that photons can be produced from final state muons. Modern Monte Carlo generators and DM codes include the effects of final state radiation from muons produced in the dark matter annihilation process itself, but neglect the O(1%) radiative correction that arises from the subsequent muon decay. After implementing this correction we demonstrate the effect that it can have on dark matter phenomenology by considering the case of dark matter annihilation to four muons via scalar mediator production. We first show that the AMS-02 positron excess can no longer easily be made consistent with this final state once the Fermi-LAT dwarf limits are calculated with the inclusion of radiative muon decays, and we next show that the Fermi-LAT galactic centre gamma excess can be improved with this final state after inclusion of the same effect. We provide code and tables for the implementation of this effect in the popular dark matter code micrOMEGAs, providing a solution for any model producing final state muons.

    hep-phastro-ph.HEPRD(2016)·10 citations
  14. 14*

    Hindered magnetic dipole transitions between P-wave bottomonia and coupled-channel effects

    Feng-Kun Guo🇨🇳 · Ulf-G. Meißner🇩🇪 · Zhi Yang🇩🇪

    In the hindered magnetic dipole transitions of heavy quarkonia, the coupled-channel effects originating from the coupling of quarkonia to a pair of heavy and anti-heavy mesons can play a dominant role. Here, we study the hindered magnetic dipole transitions between two -wave bottomonia, and , with . In these processes the coupled-channel effects are expected to lead to partial widths much larger than the quark model predictions. We estimate these partial widths which, however, are very sensitive to unknown coupling constants related to the vertices . A measurement of the hindered M1 transitions can shed light on the coupled-channel dynamics in these transitions and hence on the size of the coupling constants. We also suggest to check the coupled-channel effects by comparing results from quenched and fully dynamical lattice QCD calculations.

    hep-phPLB(2016)·9 citations
  15. 15*

    Seeking for the observational manifestation of de Sitter Relativity

    Daria A. Tretyakova🇷🇺

    The de Sitter invariant special relativity is a natural extension of the usual Einstein special relativity. Within this framework a generalization of special relativity (SR) for the de Sitter space-time introduces a new length scale , serving an origin of geometrical cosmological constant . De Sitter relativity predicts the departure from the Lorentz invariance due to spacetime curvature, related to the geometrical cosmological constant. In this paper the possible impact of de Sitter special relativity effects on threshold particle processes and equivalence principle violation is considered. The main conclusion is that constraints, coming from cosmological fine structure constant variations render this effects nowadays undetectable. A brief outlook is given thereafter.

    hep-phgr-qcGrav.Cosmol.(2016)·3 citations
  16. 16*

    Leading QCD-induced four-loop contributions to the -function of the Higgs self-coupling in the SM and vacuum stability

    K. G. Chetyrkin🇩🇪 · M. F. Zoller🇨🇭

    We present analytical results for the leading top-Yukawa and QCD contribution to the -function for the Higgs self-coupling of the Standard Model at four-loop level, namely the part independently confirming a result given in [1]. We also give the contribution of the anomalous dimension of the Higgs field as well as the terms to the top-Yukawa -function which can also be derived from the anomalous dimension of the top quark mass. We compare the results with the RG functions of the correlators of two and four scalar currents in pure QCD and find a new relation between the anomalous dimension of the QCD vacuum energy and the anomalous dimension appearing in the RG equation of the correlator of two scalar currents. Together with the recently computed top-Yukawa and QCD contributions to [2,3] the -functions presented here constitute the leading four-loop contributions to the evolution of the Higgs self-coupling. A numerical estimate of these terms at the scale of the top-quark mass is presented as well as an analysis of the impact on the evolution of up to the Planck scale and the vacuum stability problem.

    hep-phJHEP(2016)·56 citations
  17. 17*

    Effects of Tsallis distribution on parametric resonance in chiral phase transitions

    Masamichi Ishihara

    The parametric resonance was studied in chiral phase transitions when the momentum distribution is described by a Tsallis distribution. A Tsallis distribution has two parameters, the temperature and the entropic index . The amplification was estimated in two cases: 1) expansionless case and 2) one dimensional expansion case. In an expansionless case, the temperature is constant, and the amplified modes as a function of were calculated for various . In one dimensional expansion case, the temperature decreases as a function of the proper time, and the amplification as a function of the transverse momentum was calculated for various . In the expansionless case, the following facts were found: 1) the larger the value is, the softer the amplified modes are for the first and second resonance bands, 2) the amplified mode of the first resonance band decreases and vanishes, as the temperature increases, and 3) the amplified mode of the second resonance band decreases and approaches to zero, as the temperature increases. In one dimensional expansion case, the following facts were found: 1) the soft mode is amplified, 2) the amplification is extremely strong around the amplified mode of the first resonance band at , and 3) the magnitude of the amplification as a function of transverse momentum oscillates around the amplified mode of the first resonance band at .

    hep-phIJMPE(2016)·0 citations
  18. 18*

    Diphoton signal via Chern-Simons interaction in a warped geometry scenario

    Nabarun Chakrabarty🇮🇳 · Biswarup Mukhopadhyaya🇮🇳 · Soumitra SenGupta🇮🇳

    The Kalb-Ramond field, identifiable with bulk torsion in a five-dimensional Randall Sundrum (RS) scenario, has Chern-Simons interactions with gauge bosons, from the requirement of gauge anomaly cancellation. Its lowest Kaluza Klein (KK) mode on the visible 3-brane can be identified with a spin-0 CP-odd field, namely, the axion. By virtue of the warped geometry and Chern-Simons couplings, this axion has unsuppressed interactions with gauge bosons in contrast to ultra-suppressed interactions with fermions. The ensuing dynamics can lead to a peak in the diphoton spectrum, which could be observed at the LHC, subject to the prominence of the signal. Moreover, the results can be numerically justified when the warp factor is precisely in the range required for stabilization of the electroweak scale.

    hep-phPRD(2017)·6 citations
  19. 19*

    The role of flavon cross couplings in leptonic flavour mixing

    Silvia Pascoli🇬🇧 · Ye-Ling Zhou🇬🇧

    In models with discrete flavour symmetries, flavons are critical to realise specific flavour structures. Leptonic flavour mixing originates from the misalignment of flavon vacuum expectation values which respect different residual symmetries in the charged lepton and neutrino sectors. Flavon cross couplings are usually forbidden, in order to protect these symmetries. Contrary to this approach, we show that cross couplings can play a key role and give raise to necessary corrections to flavour-mixing patterns, including a non-zero value for the reactor angle and CP violation. For definiteness, we present two models based on . In the first model, all flavons are assumed to be real or pseudo-real, with 7 real degrees of freedom in the flavon sector in total. A sizable reactor angle associated with nearly maximal CP violation is achieved, and, as both originate from the same cross coupling, a sum rule results with a precise prediction for the value of the Dirac CP-violating phase. In the second model, the flavons are taken to be complex scalars, which can be connected with supersymmetric models and multi-Higgs models. The complexity properties of flavons provide new sources for generating the reactor angle. Models in this new approach introduce very few degrees of freedom beyond the Standard Model and can be more economical than those in the framework of extra dimension or supersymmetry.

    hep-phJHEP(2016)·18 citations
  20. 20*

    Neutrino spin-flavor oscillations derived from the mass basis

    Riccardo Fabbricatore🇷🇺 · Alexander Grigoriev🇷🇺 · Alexander Studenikin🇷🇺

    We consider neutrino mixing and oscillations in presence of an arbitrary constant magnetic field with nonzero transversal and longitudinal components with respect to the direction of neutrino propagation. The electromagnetic interaction of neutrinos is determined by diagonal and transition neutrino magnetic moments that are introduced for the neutrino mass states. Explicit expressions for the effective neutrino diagonal and transition magnetic moments for the flavor basis in terms of these values for the mass states are obtained. The effective evolution Hamiltonian for the flavor neutrino and the corresponding oscillation probability are derived. The role of the longitudinal magnetic field component is examined. In particular, it is shown that: 1) coupled to the corresponding magnetic moments shifts the neutrino energy, and 2) in case of nonvanishing neutrino transition magnetic moments produces an additional mixing between neutrino states, both in the mass and flavor neutrino bases.

    hep-phJ.Phys.Conf.Ser.(2016)·29 citations
  21. 21*

    A Proposed Experimental Search for Chameleons using Asymmetric Parallel Plates

    Clare Burrage🇬🇧 · Edmund J. Copeland🇬🇧 · James A. Stevenson🇬🇧

    Light scalar fields coupled to matter are a common consequence of theories of dark energy and attempts to solve the cosmological constant problem. The chameleon screening mechanism is commonly invoked in order to suppress the fifth forces mediated by these scalars, suficiently to avoid current experimental constraints, without fine tuning. The force is suppressed dynamically by allowing the mass of the scalar to vary with the local density. Recently it has been shown that near future cold atoms experiments using atom-interferometry have the ability to access a large proportion of the chameleon parameter space. In this work we demonstrate how experiments utilising asymmetric parallel plates can push deeper into the remaining parameter space available to the chameleon.

    astro-ph.COhep-phJCAP(2016)·17 citations
  22. 22*

    Cosmological Attractors and Asymptotic Freedom of the Inflaton Field

    Renata Kallosh🇺🇸 · Andrei Linde🇺🇸

    We show that the inflaton coupling to all other fields is exponentially suppressed during inflation in the cosmological -attractor models. In the context of supergravity, this feature is a consequence of the underlying hyperbolic geometry of the moduli space which has a flat direction corresponding to the inflaton field. A combination of these factors protects the asymptotic flatness of the inflaton potential.

    hep-thastro-ph.COgr-qchep-phJCAP(2016)·66 citations
  23. 23*

    Random-walk baryogenesis via primordial black holes

    İbrahim Semiz🇹🇷

    Gravitation violates baryon number : A star has a huge amount of it, while a black hole forming from the star has none. Consider primordial black holes before the hadronic annihiliation in the early universe, encountering and absorbing baryons and antibaryons: Each such absorption changes of the universe by one unit, up or down. But the absorption events are , hence they amount to a random walk in -space, leading to the expectation of a net at the end. While the scale of this effect is most uncertain, it must exist. We explore some ramifications, including the change of net with expansion, connection with universe topology, and possible observational signatures.

    gr-qchep-ph2 citations
  24. 24*

    A Green's function approach to the Casimir effect on topological insulators with planar symmetry

    A. Martín-Ruiz🇲🇽 · M. Cambiaso🇨🇱 · L. F. Urrutia🇲🇽

    We investigate the Casimir stress on a topological insulator (TI) between two metallic plates. The TI is assumed to be joined to one of the plates and its surface in front of the other is covered by a thin magnetic layer, which turns the TI into a full insulator. We also analyze the limit where one of the plates is sent to infinity yielding the Casimir stress between a conducting plate and a TI. To this end we employ a local approach in terms of the stress-energy tensor of the system, its vacuum expectation value being subsequently evaluated in terms of the appropriate Green's function. Finally, the construction of the renormalised vacuum stress-energy tensor in the region between the plates yields the Casimir stress. Numerical results are also presented.

    cond-mat.mes-hallhep-phhep-thEPL(2016)·40 citations
  25. 25*

    Consistent Perturbative Fixed Point Calculations in QCD and SQCD

    Thomas A. Ryttov🇩🇰

    We suggest how to consistently calculate the anomalous dimension of the operator in finite order perturbation theory at an infrared fixed point for asymptotically free theories. If the loop beta function and loop anomalous dimension are known then can be calculated exactly and fully scheme independently through where and is the number of flavors and is the number of flavors above which asymptotic freedom is lost. For a supersymmetric theory the calculation preserves supersymmetry order by order in . We then compute through for supersymmetric QCD in the scheme and find that it matches the exact known result. We find that is astonishingly well described in perturbation theory already at the few loops level throughout the entire conformal window. We finally compute through for QCD and a variety of other non-supersymmetric fermionic gauge theories. Small values of are observed for a large range of flavors.

    hep-thhep-lathep-phPRL(2016)·40 citations
  26. 26*

    Inflationary Birefringence and Baryogenesis

    Stephon H.S. Alexander🇺🇸

    A decade ago, the first leptogenesis model based on inflation was proposed, where the complex phase of the inflaton field carries lepton number. If the inflaton field is an axion, it can couple to gravitational waves and gauge fields via. Chern-Simons invariants. Due to these couplings, birefringent gravitational and gauge primordial perturbations are created during inflation to generate a lepton asymmetry, establishing a possible connection between non-vanishing TB-parity violating polarization cross-correlations and leptogenesis. We also discuss the prospect for a subset of these models can directly source circular (V-mode) polarization in the CMB.

    hep-thastro-ph.COgr-qchep-phInt.J.Mod.Phys.D(2016)·29 citations
  27. 27*

    The neutrino floor at ultra-low threshold

    Louis E. Strigari🇺🇸

    By lowering their energy threshold direct dark matter searches can reach the neutrino floor with experimental technology now in development. The 7Be flux can be detected with eV nuclear recoil energy threshold and 50 kg-yr exposure. The pep flux can be detected with ton-yr exposure, and the first detection of the CNO flux is possible with similar exposure. The pp flux can be detected with threshold of eV and only kg-yr exposure. These can be the first pure neutral current measurements of the low-energy solar neutrino flux. Measuring this flux is important for low mass dark matter searches and for understanding the solar interior.

    astro-ph.COhep-phPRD(2016)·26 citations
  28. 28*

    Anderson Localization in high temperature QCD: background configuration properties and Dirac eigenmodes

    Guido Cossu🇯🇵 · Shoji Hashimoto🇯🇵

    We investigate the properties of the background gauge field configurations that act as disorder for the Anderson localization mechanism in the Dirac spectrum of QCD at high temperatures. We compute the eigenmodes of the Möbius domain-wall fermion operator on configurations generated for the gauge theory with two flavors of fermions, in the temperature range . We identify the source of localization of the eigenmodes with gauge configurations that are self-dual and support negative fluctuations of the Polyakov loop , in the high temperature sea of . The dependence of these observations on the boundary conditions of the valence operator is studied. We also investigate the spatial overlap of the left-handed and right-handed projected eigenmodes in correlation with the localization and the corresponding eigenvalue. We discuss an interpretation of the results in terms of monopole-instanton structures.

    hep-latcond-mat.dis-nncond-mat.stat-mechhep-ph+1JHEP(2016)·34 citations
  29. 29*

    Evaluation of the forward Compton scattering off protons: II. Spin-dependent amplitude and observables

    Oleksii Gryniuk🇩🇪 · Franziska Hagelstein🇩🇪 · Vladimir Pascalutsa (JGU Mainz)🇩🇪

    The forward Compton scattering off the proton is determined by substituting the empirical total photoabsorption cross sections into dispersive sum rules. In addition to the spin-independent amplitude evaluated previously [Phys. Rev. D 92, 074031 (2015)], we obtain the spin-dependent amplitude over a broad energy range. The two amplitudes contain all the information about this process, and we, hence, can reconstruct the nonvanishing observables of the proton Compton scattering in the forward kinematics. The results are compared with predictions of chiral perturbation theory where available. The low-energy expansion of the spin-dependent Compton scattering amplitude yields the Gerasimov-Drell-Hearn (GDH) sum rule and relations for the forward spin polarizabilities (FSPs) of the proton. Our evaluation provides an empirical verification of the GDH sum rule for the proton, and yields empirical values of the proton FSPs. For the GDH integral, we obtain b, in agreement with the sum rule prediction: b. For the FSPs, we obtain: fm, and fm, improving on the accuracy of previous evaluations.

    nucl-thhep-phnucl-exPRD(2016)·22 citations
  30. 30*

    Liquid gas phase transition in hypernuclei

    S. Mallik🇮🇳 · G. Chaudhuri🇮🇳

    The fragmentation of excited hypernuclear system formed in heavy ion collisions has been described by the canonical thermodynamical model extended to three component systems. The multiplicity distribution of the fragments has been analyzed in detail and it has been observed that the hyperons have the tendency to get attached to the heavier fragments. Another important observation is the phase coexistence of the hyperons, a phenomenon which is linked to liquid gas phase transition in strange matter.

    nucl-thhep-exhep-phnucl-exPRC(2015)·6 citations
  31. 31*

    Effect of hyperons on phase coexistence in strange matter

    P. Das🇮🇳 · S. Mallik🇮🇳 · G. Chaudhuri🇮🇳

    The study of liquid gas phase transition in fragmentation of nuclei in heavy ion collisions has been extended to the strangeness sector using the statistical model for multifragmentation. Helmholtz's free energy, specific heat and few other thermodynamic observables have been analyzed in order to examine the occurence of phase transition in the strange matter. The bimodal behaviour of the largest cluster formed in fragmentation also strongly indicates coexistence of both the phases. The presence of hyperons strengthens the signals and also shifts the transition temperature to lower values.

    nucl-thhep-exhep-phnucl-exPRC(2017)·2 citations
  32. 32*

    The Potential of the Dwarf Galaxy Triangulum II for Dark Matter Indirect Detection

    Anna Genina🇬🇧 · Malcolm Fairbairn🇬🇧

    The recently discovered object Triangulum II appears to be an ultra faint dwarf spheroidal galaxy which may be one of the most dark matter dominated objects yet known. In this work we try to estimate the potential of this object for studies of the indirect detection of self-annihilating dark matter by obtaining its astrophysical J-factor. We perform a basic estimate of the velocity gradient to look for signs of the halo being tidally disrupted but show that the observed value is statistically compatible with zero velocity gradient. We solve the spherical Jeans equation using Markov Chain Monte Carlo (MCMC) engine GreAT and the Jeans analysis part of the CLUMPY package. We find the results point towards a very large J-factor, appearing to make Triangulum II one of the best targets in the search for dark matter. However we stress that the very small number of line of sight velocities currently available for this object make follow up studies essential.

    astro-ph.GAhep-phMNRAS(2016)·17 citations
  33. 33*

    Non-BPS exact solutions and their relation to bions in models

    Tatsuhiro Misumi🇯🇵 · Muneto Nitta🇯🇵 · Norisuke Sakai🇯🇵

    We investigate non-BPS exact solutions in sigma models on with twisted boundary conditions, by using the Din-Zakrzewski projection method. We focus on the relation of the non-BPS solutions to the ansatz of multi-instanton (bion) configurations and discuss their significance in the context of the resurgence theory. We find that the transition between seemingly distinct configurations of multi-instantons occur as moduli changes in the non-BPS solutions, and the simplest non-BPS exact solution corresponds to multi-bion configurations with fully-compressed double fractional instantons in the middle. It indicates that the non-BPS solutions make small but nonzero contribution to the resurgent trans-series as special cases of the multi-bion configurations. We observe a generic pattern of transitions between distinct multi-bion configurations (flipping partners), leading to the three essential properties of the non-BPS exact solution: (i) opposite sign for terms corresponding to the left and right infinities, (ii) symmetric location of fractional instantons, and (iii) the transition between distinct bion configurations. By studying the balance of forces, we show that the relative phases between the instanton constituents play decisive roles in stability and instability of the muli-instanton configurations. We discuss local and global instabilities of the solutions such as negative modes and the flow to the other saddle points, by considering the deformations of the non-BPS exact solutions within our multi-instanton ansatz. We also briefly discuss some classes of the non-BPS exact solutions in Grassmann sigma models.

    hep-thhep-phJHEP(2016)·32 citations
  34. 34*

    A new algebraic structure in the standard model of particle physics

    Latham Boyle🇨🇦 · Shane Farnsworth🇨🇦

    We introduce a new formulation of the real-spectral-triple formalism in non-commutative geometry (NCG): we explain its mathematical advantages and its success in capturing the structure of the standard model of particle physics. The idea, in brief, is to represent (the algebra of differential forms on some possibly-noncommutative space) on (the Hilbert space of spinors on that space), and to reinterpret this representation as a simple super-algebra with even part and odd part . is the fundamental object in our approach: we show that (nearly) all of the basic axioms and assumptions of the traditional real-spectral-triple formalism of NCG are elegantly recovered from the simple requirement that should be a differential graded -algebra (or "-DGA"). Moreover, this requirement also yields other, new, geometrical constraints. When we apply our formalism to the NCG traditionally used to describe the standard model of particle physics, we find that these new constraints are physically meaningful and phenomenologically correct. In particular, these new constraints provide a novel interpretation of electroweak symmetry breaking that is geometric rather than dynamical. This formalism is more restrictive than effective field theory, and so explains more about the observed structure of the standard model, and offers more guidance about physics beyond the standard model.

    hep-thhep-phmath-phmath.MPJHEP(2018)·20 citations
  35. 35*

    Lifshitz transitions, type-II Dirac and Weyl fermions, event horizon and all that

    Kuang Zhang🇨🇳 · G.E. Volovik🇫🇮

    The type-II Weyl and type-II Dirac points emerge in semimetals and also in relativistic systems. In particular, the type-II Weyl fermions may emerge behind the event horizon of black holes. In this case the horizon with Painleve-Gullstrand metric serves as the surface of the Lifshitz transition. This relativistic analogy allows us to simulate the black hole horizon and Hawking radiation using the fermionic superfluid with supercritical velocity, and the Dirac and Weyl semimetals with the interface separating the type-I and type-II states. The difference between such type of the artificial event horizon and that which arises in acoustic metric is discussed. At the Lifshitz transition between type-I and type-II fermions the Dirac lines may also emerge, which are supported by the combined action of topology and symmetry. The type-II Weyl and Dirac points also emerge as the intermediate states of the topological Lifshitz transitions. Different configurations of the Fermi surfaces, involved in such Lifshitz transition, are discussed. In one case the type-II Weyl point connects the Fermi pockets, and the Lifshitz transition corresponds to the transfer of the Berry flux between the Fermi pockets. In the other case the type-II Weyl point connects the outer and inner Fermi surfaces. At the Lifshitz transition the Weyl point is released from both Fermi surfaces. These examples reveal the complexity and universality of topological Lifshitz transitions, which originate from the ubiquitous interplay of a variety of topological characters of the momentum-space manifolds. For the interacting electrons, the Lifshitz transitions may lead to the formation of the dispersionless (flat) band with zero energy and singular density of states, which opens the route to room-temperature superconductivity.

    cond-mat.otherhep-phJETP Lett.(2017)·18 citations
  36. 36*

    Sound Speed and Viscosity of Semi-Relativistic Relic Neutrinos

    Lawrence M. Krauss (1,2)🇺🇸 · Andrew J. Long (3) ((1) Arizona State University, (2) Australian National University, (3) University of Chicago)🇺🇸

    Generalized fluid equations, using sound speed and viscosity as effective parameters, provide a convenient phenomenological formalism for testing the relic neutrino "null hypothesis," i.e. that that neutrinos are relativistic and free-streaming prior to recombination. In this work, we relax the relativistic assumption and ask "to what extent can the generalized fluid equations accommodate finite neutrino mass?" We consider both the mass of active neutrinos, which are largely still relativistic at recombination , and the effect of a semi-relativistic sterile component. While there is no one-to-one mapping between mass/mixing parameters and and , we demonstrate that the existence of a neutrino mass could induce a bias to measurements of and at the level of .

    astro-ph.COhep-exhep-phJCAP(2016)·2 citations
  37. 38*

    Recent developments in string model-building and cosmology

    Michele Cicoli🇮🇹

    In this talk I discuss recent developments in moduli stabilisation, SUSY breaking and chiral D-brane models together with several interesting features of cosmological models built in the framework of type IIB string compactifications. I show that a non-trivial pre-inflationary dynamics can give rise to a power loss at large angular scales for which there have been mounting observational hints from both WMAP and Planck. I then describe different stringy embeddings of inflationary models which yield large or small tensor modes. I finally argue that reheating is generically driven by the decay of the lightest modulus which can produce, together with Standard Model particles, also non-thermal dark matter and light hidden sector degrees of freedom that behave as dark radiation.

    hep-thastro-ph.COhep-ph3 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.