Login

CIPANP 2018 - Thirteenth Conference on the Intersections of Particle and Nuclear Physics

29 May 2018 to 3 June 2018
Hyatt Regency Indian Wells Conference Center
US/Pacific timezone

Session

NMNM / TSEI

NMNM/TSEI
1 Jun 2018, 16:10
Hyatt Regency Indian Wells Conference Center

Hyatt Regency Indian Wells Conference Center

44600 Indian Wells Lane, Indian Wells, CA 92210, USA

Conveners

NMNM / TSEI: Parallel 8 — Neutrinos and Symmetries

  • Daniel Dwyer
  • Andre de Gouvea (Northwestern University)
  • Brad Filippone (caltech)

Presentation materials

There are no materials yet.

  1. 253. Sterile Neutrinos in the Early Universe
    Prof. George Fuller (University of California, San Diego)
    01/06/2018, 16:10
    TSEI
    Parallel
    I will give an overview of sterile neutrino physics in the early universe and in cosmology, especially as regards dark matter. This will include a discussion of production mechanisms, relic densities, the relationship of these to lepton and baryon numbers, and associated high energy scale physics issues. I will also discuss the status of X-ray observational constraints on sterile neutrino and...
    Go to contribution page
  2. 294. Non-Standard Neutrino Interactions
    Prof. Andre de Gouvea (Northwestern University)
    01/06/2018, 16:35
    NMNM
    Parallel
    I discuss the status of non-standard neutrino interactions, especially their impact on next-generation neutrino oscillation experiments.
    Go to contribution page
  3. 25. Detecting CP Violation in the Presence of Non-Standard Neutrino Interactions
    Jeffrey Hyde (Goucher College)
    01/06/2018, 17:00
    NMNM
    Parallel
    New physics beyond the Standard Model could appear at long baseline oscillation experiments as non-standard interactions (NSI) between neutrinos and matter. If so, determination of the CP-violating phase $\delta_{13}$ is ambiguous due to interference with additional complex phases. I'll present my work using both numerical solutions and a perturbative approach to study oscillation...
    Go to contribution page
  4. 217. Neutrino Oscillations and Supernova Nucleosynthesis
    Prof. Akif Baha Balantekin (University of Wisconsin-Madison)
    01/06/2018, 17:25
    NMNM
    Parallel
    A good fraction of the heavier nuclei were formed in the rapid neutron capture (r-process) nucleosynthesis scenario. Although an astrophysical site of the r-process is not yet identified, one expects such sites to be associated with explosive phenomena since a large number of interactions are required to take place during a rather short time interval. Candidate sites include core-collapse...
    Go to contribution page
  5. 151. Collective Neutrino Oscillations in the Presence of Collisions
    Dr Shashank Shalgar (Los Alamos National Laboratory)
    01/06/2018, 17:50
    NMNM
    Parallel
    In dense astrophysical environments, the evolution of neutrino flavor is non-linear which can lead to many interesting phenomena. However, this non-linear evolution of neutrino flavor also called the "collective neutrino oscillations" is only beginning to be understood, especially in conjunction with collisions. I will discuss the effect of neutrino back-scattering in the interior of a...
    Go to contribution page
  6. 340. Neutrino Flavor Transformation and the Cosmic Lepton Asymmetry
    Luke Johns (UC San Diego)
    01/06/2018, 18:10
    NMNM
    Parallel
    Observational constraints permit a cosmic lepton asymmetry that is orders of magnitude larger than its baryonic counterpart, a possibility of great relevance for leptogenesis, sterile neutrino dark matter, and the flavor evolution of Standard Model neutrinos. It is this last connection that we focus on here: the flavor states of neutrinos in the early universe are coupled to each other,...
    Go to contribution page
Building timetable...