7–8 Nov 2016
Max Planck Institute for Astrophysics (MPA)
Europe/Berlin timezone

Contribution List

15 out of 15 displayed
  1. 07/11/2016, 11:15
  2. Andrzej Czarnecki (U. Alberta)
    07/11/2016, 11:30
    The mass of the electron is best determined with hydrogen-like ions in a Penning trap. Binding in an ion removes the error due to the thermal motion of the electron. However, the price is that some properties of the electron are modified by the binding. These changes can be computed in QED but there are interesting complications. We present recent progress in the determination of the g-factor...
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  3. Dr Mario Pitschmann (TU Wien)
    07/11/2016, 13:30
    The qBounce experiment will be presented: ultracold neutrons fall in the gravity potential of the earth and are re ected from a mirror. As a bound quantum system, the neutrons have discrete energy eigenstates and are found in a coherent superposition of particular levels. The lowest discrete states are in the range of several pico-eVs. This opens the way to probe theories of gravitational...
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  4. Prof. Bastian Märkisch (TUM)
    07/11/2016, 14:00
    In the upcoming years next generation experiments on neutron beta decay will provide an increased sensitivity by an order of magnitude or more and will allow to asses previously inaccessible observables. In this talk I will present an overview on observables in neutron beta decay and the measurement principles used. In particular the reach of the new instrument PERC, which is currently under...
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  5. Martín González-Alonso (Lyon Institute of Origins, Institut de Physique Nucléaire de Lyon)
    07/11/2016, 14:45
  6. Prof. Andrey Ivanov (Atominstitut TU Wien)
    07/11/2016, 16:00
    We give a precision analysis of the correlation coefficients of the electron-energy spectrum and angular distribution of the Beta-decay and radiative Beta-decay of the neutron with polarized neutron and electron to order 10^(-3). The calculation of correlation coefficients is carried out within the Standard model with the contributions of order 10^(-3), caused by the ``weak...
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  7. Dr Simon Eidelman (Budker Institute of Nuclear Physics)
    07/11/2016, 16:30
  8. Susan Gardner (University of Kentucky)
    07/11/2016, 17:00
    I offer a snapshot summary of the new physics searches possible via precision measurements of heavy meson and neutron decays, emphasizing probes of the violation of discrete symmetries. In some cases the tests in systems of light and heavy flavor are complementary, in others they are disjunct. I consider examples of each class, noting the broader complementary of such work with...
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  9. David Straub (TUM)
    08/11/2016, 09:00
    Effective field theory methods allow to analyze the impact of physics beyond the Standard Model on precision observables in low-energy experiments, e.g. flavour physics, in a model-independent way and also allow to correlate effects in different types of experiments. I will discuss the general framework and some examples of current interest, e.g. concerning tensions between B decay...
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  10. Dr Christoph Bobeth (TUM)
    08/11/2016, 10:00
    Given a particular UV completion beyond the SM, flavor constraints from various low-energy flavor observables can provide combined powerful constraints on the new physics parameter space, depending on the model at hand. But even with EFT-methods, correlations between various flavor sectors exist due to operator mixing. A particular example from the literature (arXiv:1605.00524) will be...
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  11. Prof. Eberhard WIDMANN (Stefan Meyer Institute)
    08/11/2016, 11:00
    The CPT symmetry is one of the cornerstones of the Standard Model of Particle Physics. It's consequence that properties of particles and antiparticles are either exactly equal or exctly opposite is being tested using antihydrogen spectroscopy at the Antiproton Decelerator of CERN. The ASACUSA collaboration is pursuing a meansurement of the ground-state hyperfine splitting GS-HFS of...
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  12. Sebastian Jaeger (TUM)
    08/11/2016, 11:30
  13. Martin Bauer (Universität Heidelberg)
    08/11/2016, 12:00
  14. Ikaros Bigi (TUM)
    For long time we know that probing EDMs for baryons and leptons give us hunting region, where we have not to worry about background from the SM (except the well-known problem with strong CP violation). The landscape is actually more complex as said before. We have now much more actors in the stage beyond EDM of neutrons and EDM of electrons coming from atoms. On one side we should probe EDMs...
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  15. Ikaros Bigi (TUM)
    At least in the early 1990's we had realized that the SM cannot produce sizable contribution to the huge asymmetry in matter vs. anti-matter known in our Universe; now we known that known matter is only around 4.5 % there. We have to think and follow unusual `roads'. There are three obvious candidates: (i) CP asymmetries in neutrino oscillations; (ii) EDMs of baryons & leptons and - (iii)...
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