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NTN Workshop on Neutrino Non-Standard Interactions

29–31 May 2019
Washington University in St Louis
US/Central timezone

Contribution List

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  1. 26. Welcome Address by the Chair of Physics
    Mark Alford (Washington University in St Louis)
    29/05/2019, 08:55
  2. 8. Overview of Neutrino Flavor Models
    Mu-Chun Chen (UC Irvine)
    29/05/2019, 09:00

    I will review current state of models of neutrino masses. I will discuss the models' implications for particle physics phenomenology and for cosmology.

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  3. 11. Overview of Neutrino Physics at Colliders
    Tao Han (Univ. Pittsburgh)
    29/05/2019, 09:45
  4. 13. Global Fit Constraints on NSI
    Ivan Martinez-Soler (Northwestern/Fermilab)
    29/05/2019, 11:00
  5. 12. Testing NSI at Colliders
    Dorival Goncalves (Univ. Pittsburgh)
    29/05/2019, 11:45
  6. 14. Dark Matter direct detection and NSI
    Yuber Perez-Gonzalez (Northwestern/Fermilab)
    29/05/2019, 14:00
  7. 15. Large NSI in a Radiative Neutrino Mass Model
    Anil Thapa (Oklahoma State Univ.), Sudip Jana (Oklahoma State University)
    29/05/2019, 14:45
  8. 10. Confronting Neutrino Mass Generation Mechanism with MiniBooNE Anomaly
    SUDIP JANA (OKLAHOMA STATE UNIVERSITY)
    29/05/2019, 16:00

    We present a novel framework that provides an explanation to the long-standing excess of electronlike events in the MiniBooNE experiment at Fermilab. We suggest a new dark sector containing a dark neutrino and a dark gauge boson, both with masses between a few tens and a few hundreds of MeV. Dark neutrinos are produced via neutrino-nucleus scattering, followed by their decay to the dark gauge...

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  9. 16. Testing MiniBooNE Anomaly at Neutrino Scattering Experiments
    Carlos Arguelles (MIT)
    29/05/2019, 16:45
  10. 23. Leptogenesis from Low Energy CP Violation
    Jessica Turner (Fermilab)
    29/05/2019, 17:30
  11. 18. Dark Tridents
    Andre de Gouvea (Northwestern)
    30/05/2019, 09:00
  12. 2. Light Dark Matter with DUNE-PRISM
    Kevin Kelly (Fermilab)
    30/05/2019, 09:45

    The upcoming DUNE Experiment will depend on precision measurement of neutrino fluxes and cross sections at its near detector in order to deliver on its stated neutrino physics goals, such as measurements of CP violation and the neutrino mass ordering, using its far detector. To this end, the DUNE-PRISM concept has been proposed -- it consists of moving the near detector up to 36 m off-axis,...

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  13. 19. Light Mediators
    Bhaskar Dutta (Texas A&M)
    30/05/2019, 11:00

    In this talk, I will discuss light mediator models and various experimental constraints with particular emphasis on the recent results from the COHERENT experiment. I will show one particular example of such a model which contains sub-GeV dark matter.

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  14. 4. Effective Field Theory for NSI in Elastic Neutrino - Nucleus Scattering
    Michele Tammaro
    30/05/2019, 11:45

    We formulate an Effective Field Theory (EFT) for Non Standard neutrino Interactions (NSI) in elastic scattering with light quarks, leptons, gluons and photons, including all possible operators of dimension 5, 6 and 7. We constrain the respective Wilson coefficient using the measurements by the COHERENT and CHARM collaborations. We also point out the constraining power of future elastic...

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  15. 3. New physics in coherent neutrino scattering
    Xun-Jie XU (Max-Planck-Institut fuer Kernphysik)
    30/05/2019, 14:00

    In this talk, I am going to review the recent progress of coherent neutrino-nucleus scattering experiments and summarize the constraints on various BSM physics, including NSI, SPVAT (Scalar Pseudoscalar, Vector, Axialvector, Tensor) interactions, sterile neutrinos, light mediators, neutrino magnetic moments, dark matter, etc.

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  16. 6. New physics in rare neutrino scattering
    Matheus Hostert (IPPP, Durham University)
    30/05/2019, 14:45

    Rare and unique neutrino scattering processes can serve as an ideal tool in the search for new physics. In this context, I will present the sensitivity of the DUNE near detector to leptophilic Z' models, using neutrino-electron and neutrino trident scattering. I will conclude illustrating how similar signatures can also arise in more exotic models and motivating the need for a program to...

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  17. 5. Octant of theta23 and NSI degeneracy at DUNE
    Sabya Sachi Chatterjee (Institute for Particle Physics Phenomenology, Durham University)
    30/05/2019, 16:00

    We expound in detail the degeneracy between the octant of θ23 and flavor-changing neutral-current non-standard interactions (NSI’s) in neutrino propagation, considering DUNE as a case study. In the presence of such NSI parameters involving the e − µ (εeµ) and e − τ (εeτ) flavors, the νµ → νe and νµ → νe bar appearance probabilities in long-baseline experiments acquire an additional...

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  18. 9. Beginnings of Quantum Monte Carlo Short-Time Approximation Implementations for electron and neutrino scattering from He4 and C12 in GENIE
    Joshua Barrow (The University of Tennessee, FNAL)
    30/05/2019, 16:45

    The study of inclusive neutrino ($\nu$) cross sections and total fluxes for signs of (beyond) Standard Model interactions is critically dependent upon accurate theoretical modeling for consistent reconstruction of a $\nu$'s energy. Given the continuum of final state topologies available to such processes, the most popular form of this modeling within the experimental community generally occurs...

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  19. 7. Liquid Argon Technology for Theorists
    Shirley Li (SLAC)
    30/05/2019, 17:30

    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,...

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  20. 17. NSI with DUNE Alternative Configurations
    Poonam Mehta (JNU, New Delhi)
    31/05/2019, 09:00
  21. 21. NSI with IceCube
    Jordi Salvado (Barcelona)
    31/05/2019, 09:45
  22. 22. Inflation and NSI
    Peter Denton (Brookhaven)
    31/05/2019, 11:00
  23. 25. Summary
    Pedro Machado (Fermilab)
    31/05/2019, 11:45