PaperPanorama

HEP Phenomenology·hep-ph

Mon·Jan 7, 2019

12 papers—9 primary·3 cross-listed·reconstructed*

  1. 01*

    Event Generation and Statistical Sampling for Physics with Deep Generative Models and a Density Information Buffer

    Sydney Otten🇳🇱 · Sascha Caron🇳🇱 · Wieske de Swart🇳🇱 · Melissa van Beekveld🇳🇱 · Luc Hendriks🇳🇱 · Caspar van Leeuwen🇺🇸 · Damian Podareanu🇺🇸 · Roberto Ruiz de Austri🇪🇸 · Rob Verheyen🇳🇱

    We present a study for the generation of events from a physical process with deep generative models. The simulation of physical processes requires not only the production of physical events, but also to ensure these events occur with the correct frequencies. We investigate the feasibility of learning the event generation and the frequency of occurrence with Generative Adversarial Networks (GANs) and Variational Autoencoders (VAEs) to produce events like Monte Carlo generators. We study three processes: a simple two-body decay, the processes and including the decay of the top quarks and a simulation of the detector response. We find that the tested GAN architectures and the standard VAE are not able to learn the distributions precisely. By buffering density information of encoded Monte Carlo events given the encoder of a VAE we are able to construct a prior for the sampling of new events from the decoder that yields distributions that are in very good agreement with real Monte Carlo events and are generated several orders of magnitude faster. Applications of this work include generic density estimation and sampling, targeted event generation via a principal component analysis of encoded ground truth data, anomaly detection and more efficient importance sampling, e.g. for the phase space integration of matrix elements in quantum field theories.

    hep-phhep-exphysics.data-anNature Commun.(2021)·132 citations
  2. 02*

    Behind the Standard Model

    Andrea Wulzer🇮🇹

    These lectures provide a concise introduction to the so-called "Beyond the Standard Model"' physics, with particular emphasis on the problem of the microscopic origin of the Higgs mass term and of the Electro-Weak symmetry breaking scale in connection with Naturalness. The standard scenarios of Supersymmetry and Composite Higgs are shortly reviewed. An attempt is made to summarise the implications of the LHC run- results on what we expect to lie beyond (or behind) the Standard Model.

    hep-phCERN-2018-008-SP, pp. 91-140·11 citations
  3. 03*

    Spin-flavor oscillations of Dirac neutrinos in matter under the influence of a plane electromagnetic wave

    Maxim Dvornikov (IZMIRAN)🇷🇺

    We study oscillations of Dirac neutrinos in background matter and a plane electromagnetic wave. First, we find the new exact solution of the Dirac-Pauli equation for a massive neutrino with the anomalous magnetic moment electroweakly interacting with matter under the influence of a plane electromagnetic wave with the circular polarization. We use this result to describe neutrino spin oscillations in the external fields in question. Then we consider several neutrino flavors and study neutrino spin-flavor oscillations in this system. For this purpose we formulate the initial condition problem and solve it accounting for the considered external fields. We derive the analytical expressions for the transition probabilities of spin-flavor oscillations for different types of neutrino magnetic moments. These analytical expressions are compared with the numerical solutions of the effective Schrödinger equation and with the findings of other authors. In particular, we reveal that a resonance in neutrino spin-flavor oscillations in the considered external fields cannot happen contrary to the previous claims. Finally, we briefly discuss some possible astrophysical applications.

    hep-phPRD(2019)·9 citations
  4. 04*

    Impact of unidentified light charged hadron data on the determination of pion fragmentation functions

    Maryam Soleymaninia🇮🇷 · Muhammad Goharipour🇮🇷 · Hamzeh Khanpour🇮🇷

    In this paper a new comprehensive analysis of parton-to-pion fragmentation functions (FFs) is performed for the first time by including all experimental data sets on single inclusive pion as well as unidentified light charged hadron production in electron-positron () annihilation. We determine the pion FFs along with their uncertainties using the standard "Hessian" technique at next-to-leading order (NLO) and next-to-next-to leading order (NNLO) in perturabative QCD. It is shown that the determination of pion FFs using simultaneously the data sets from pion and unidentified light charged hadron productions leads to the reduction of all pion FFs uncertainties especially for the case of strange quark and gluon FFs by significant factors. In this study, we have quantified the constraints that these data sets could impose on the extracted pion FFs. Our results also illustrate the significant improvement in the precision of FFs fits achievable by inclusion of higher order corrections. The improvements on both FFs uncertainties as well as fit quality have been clearly discussed.

    hep-phhep-exPRD(2019)·14 citations
  5. 05*

    Non-perturbative uncertainties on the transverse momentum distribution of electroweak bosons and on the determination of the boson mass at the LHC

    Giuseppe Bozzi (INFN, Pavia & Pavia U.)🇮🇹 · Andrea Signori (Argonne National Laboratory)🇺🇸

    In this contribution we present an overview of recent results concerning the impact of a possible flavour dependence of the intrinsic quark transverse momentum on electroweak observables. In particular, we focus on the spectrum of electroweak gauge bosons produced in proton-proton collisions at the LHC and on the direct determination of the boson mass. We show that these effects are comparable in size to other non-perturbative effects commonly included in phenomenological analyses, and should thus be included in precise theoretical predictions for present and future hadron colliders.

    hep-phhep-exAdv.High Energy Phys.(2019)·24 citations
  6. 06*

    Interplay of the CGC and TMD frameworks to all orders in kinematic twist

    Tolga Altinoluk🇵🇱 · Renaud Boussarie🇺🇸 · Piotr Kotko🇵🇱

    A framework for an improved TMD (iTMD) factorization scheme at small , involving off-shell perturbative subamplitudes, was recently developed as an interpolation between the TMD regime and the BFKL regime. In this article, we study the relation between CGC and iTMD amplitudes. We first show how the dipole-size expansion of CGC amplitudes resembles the twist expansion of a TMD amplitude. Then, by isolating kinematic twists, we prove that iTMD amplitudes are obtained with infinite kinematic twist accuracy by simply getting rid of all genuine twist contributions in a CGC amplitude. Finally we compare the amplitudes obtained via a proper kinematic twist expansion to those obtained via a more standard dilute expansion to show the relation between the iTMD framework and the dilute low framework.

    hep-phJHEP(2019)·79 citations
  7. 07*

    Fully constrained mass matrix: Can symmetries alone determine the flavon vacuum alignments?

    R. Krishnan🇮🇳

    In the framework of the representation theory of finite groups, it was recently shown that a fully constrained complex-symmetric mass matrix can be conveniently mapped into a sextet of . In this paper, we introduce an additional flavor group in the model so that the vacuum alignment of the sextet is determined not only by the symmetries of but also by that of . We define several flavons which transform as multiplets under as well as . The vacuum alignment of each of these flavons is obtained as a simultaneous invariant eigenstate of specific elements of the groups and ; i.e.,~the vacuum alignment is fully determined by its residual symmetries. These flavons couple together uniquely resulting in the fully constrained sextet of . Through this work we propose a general formalism in which the flavor symmetry group () is obtained as the direct product, . Fermions transform nontrivially only under while they remain invariant under . Flavons, on the other hand, transform nontrivially under both and . The vacuum alignment of each flavon multiplet transforming irreducibly under is uniquely identified by its corresponding residual symmetry (a subgroup of ). Several such flavons couple together to form an effective multiple of which remains invariant under . This effective multiplet couples to the fermions.

    hep-phPRD(2020)·9 citations
  8. 08*

    Relaxing the Cosmological Moduli Problem by Low-scale Inflation

    Shu-Yu Ho🇯🇵 · Fuminobu Takahashi🇯🇵 · Wen Yin🇰🇷

    We show that the cosmological abundance of string axions is much smaller than naive estimates if the Hubble scale of inflation, , is sufficiently low (but can still be much higher than the axion masses) and if the inflation lasts sufficiently long. The reason is that the initial misalignment angles of the string axions follow the Bunch-Davies distribution peaked at the potential minima. As a result, the cosmological moduli problem induced by the string axions can be significantly relaxed by low-scale inflation, and astrophysical and cosmological bounds are satisfied over a wide range of the mass without any fine-tuning of the initial misalignment angles. Specifically, the axion with its decay constant \,GeV satisfies the bounds over for \,{\rm GeV}. We also discuss cases with multiple axions and the QCD axion.

    hep-phastro-ph.COgr-qchep-thJHEP(2019)·59 citations
  9. 09*

    Mono-Neutrino at DUNE: New Signals From Neutrinophilic Thermal Dark Matter

    Kevin J. Kelly🇺🇸 · Yue Zhang🇺🇸

    We introduce the mono-neutrino signal at neutrino detectors as a smoking gun of sub-GeV scale dark matter candidates that mainly interact with standard model neutrinos. In a mono-neutrino process, invisible particles, either dark matter themselves or the mediator particle, are radiated off a neutrino when it undergoes the charged-current weak interaction. The associated signals include a missing transverse momentum with respect to the incoming neutrino beam direction and the production of wrong-sign charged leptons. We demonstrate the potential leading role of the future DUNE experiment, using its proposed liquid and gas argon near detectors, in probing these new signals and the thermal origins of neutrinophilic dark matter.

    hep-phhep-exPRD(2019)·75 citations
  10. 10*

    Cosmic Ferromagnetism of Magninos

    R. B. MacKenzie🇨🇦 · M. B. Paranjape🇨🇦 · U. A. Yajnik🇮🇳

    We study the physical conditions for the occurrence of ferromagnetic instability in a neutral plasma of fermions. We consider a system of two species and which are oppositely charged under a local , with much lighter than . The leading correction to free quasiparticle behaviour for the lighter species arises from the exchange interaction, while the heavier species remain spectators. This plasma, which is abelian, asymmetric and idealised, is shown to be naturally susceptible to the formation of a completely spin-imbalanced ferromagnetic state for the lighter species (dubbed a magnino) in large parts of parameter space. It is shown that the domain structure formed by this ferromagnetic state can mimic Dark Energy, determining the masses of the two fermion species involved, depending on their abundance relative to the standard photons. Incomplete cancellation of the X-magnetic fields among the domains can give rise to residual long range -magnetic fields. Under the assumption that this mixes with Maxwell electromagnetism, this provides a mechanism for the seed for cosmic-scale magnetic fields. An extended model with several flavours and of the species can incorporate Dark Matter. Thus the scenario shows the potential for explaining the large scale magnetic fields, and what are arguably the two most important outstanding puzzles of cosmology: Dark Matter and Dark Energy.

    ↳ astro-ph.COcond-mat.str-elhep-phhep-th2 citations
  11. 11*

    T-Dual Cosmological Solutions of Double Field Theory II

    Heliudson Bernardo🇨🇦 · Robert Brandenberger🇨🇦 · Guilherme Franzmann (McGill Univ. and IFT, UNESP)🇨🇦

    In this paper we present cosmological solutions of Double Field Theory in the supergravity frame and in the winding frame which are related via T-duality. In particular, we show that the solutions can be viewed without the need of complexifying the cosmological scale factor.

    ↳ hep-thastro-ph.COgr-qchep-phPRD(2019)·29 citations
  12. 12*

    New Constraints on Sterile Neutrino Dark Matter from M31 Observations

    Kenny C. Y. Ng🇮🇱 · Brandon M. Roach🇺🇸 · Kerstin Perez🇺🇸 · John F. Beacom🇺🇸 · Shunsaku Horiuchi🇺🇸 · Roman Krivonos🇷🇺 · Daniel R. Wik🇺🇸

    We use a combined 1.2 Ms of observations of M31 to search for X-ray lines from sterile neutrino dark matter decay. For the first time in a analysis, we consistently take into account the signal contribution from both the focused and unfocused fields of view. We also reduce the modeling systematic uncertainty by performing spectral fits to each observation individually and statistically combining the results, instead of stacking the spectra. We find no evidence of unknown lines, and thus derive limits on the sterile neutrino parameters. Our results place stringent constraints for dark matter masses keV, which reduces the available parameter space for sterile neutrino dark matter produced via neutrino mixing (, in the MSM) by approximately one-third. Additional observations, together with improved low-energy background modeling, could probe the remaining parameter space in the future. Lastly, we also report model-independent limits on generic dark matter decay rates and annihilation cross sections.

    ↳ astro-ph.HEastro-ph.COhep-phPRD(2019)·206 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.