'Mass eigenstates' presentation slideshows

NASA Hubble Photo

Neutrino Oscillation Phenomenology. Boris Kayser Pontecorvo School September, 2019. NASA Hubble Photo. 1. Spin:. 1. 1. 1. 1. Without the neutrino, angular momentum would not be conserved. 2. 2. 2. 2. What Are Neutrinos Good For?.

1.34k views • 134 slides

Neutrinos: Results and Future

Neutrinos: Results and Future. Boris Kayser DESY March 4, 2008. Evidence For ? Flavor Change. Neutrinos Solar Reactor (L ~ 180 km) Atmospheric Accelerator (L = 250 and 735 km) Stopped ? + Decay LSND L ? 30 m. Evidence of Flavor Change Compelling Compelling Compelling

1.18k views • 108 slides

H. Fritzsch LMU Munich

Flavor Mixing and Neutrino Masses. H. Fritzsch LMU Munich. mixing of mass eigenstates by weak interaction. (Cabibbo angle). mass matrices:. texture 0. u,c - d,s. F., Weinberg. (beyond Standard Model). texture zero:. SU(2) x SU(2). L. R. Reflection symmetries (~parity).

647 views • 64 slides

1.18k views • 50 slides

The role of the tetraquark at nonzero temperature

480 views • 40 slides

Overview of flavour physics

Overview of flavour physics. Probes for New Physics. Example from the past:. Probes for New Physics searches. The aim of heavy flavour physics is to study B and D decays and to look for anomalous effects beyond the Standard Model. Requirements to look for New Physics effects:

525 views • 38 slides

Gennaro Corcella 1 , Simonetta Gentile 2 1. Laboratori Nazionali di Frascati, INFN

453 views • 33 slides

Gennaro Corcella 1 , Simonetta Gentile 2 1. Laboratori Nazionali di Frascati, INFN

379 views • 27 slides

Gennaro Corcella 1 , Simonetta Gentile 2 1. Laboratori Nazionali di Frascati, INFN

422 views • 27 slides

Neutrino Physics

442 views • 23 slides

Dimuon CP asymmetry and new physics in Bs-Bsbar mixing

324 views • 20 slides

The NOvA Experiment

The NOvA Experiment. Ji Liu On behalf of the NOvA collaboration College of William and Mary APS April Meeting April 1, 2012. NOvA. L ong -baseline neutrino oscillation experiment currently under construction Off-axis neutrinos from NuMI beam

340 views • 18 slides

278 views • 15 slides

Matter effects in a rank-1 see-saw model of neutrino masses

Matter effects in a rank-1 see-saw model of neutrino masses. G. J. Stephenson Jr University of New Mexico with T. Goldman, LANL B. H. J. McKellar, Melbourne. dpf-06, Hawaii. Direction of single massive sterile eigenstate in space defined by Dirac mass eigenstates.

71 views • 7 slides

Search for B s oscillations at D ?

Search for B s oscillations at D ?. Constraining the CKM matrix. What is mixing ?. SM or NP ?. Neutral B meson transition from particle to anti-particle state, and vice-versa Weak eigenstates ? mass eigenstates Caused by higher order flavor changing weak interactions:

11 views • 1 slides