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6th IDPASC/LIP PhD Students Workshop

25–27 Jun 2020
Europe/Lisbon timezone

Session

Session 5

26 Jun 2020, 09:30

Conveners

Session 5

  • Orlando Oliveira (UC)

Presentation materials

There are no materials yet.

  1. 17. Keynote talk 4: A (brief) Introduction to Non-perturbative Quantum Field Theory
    Peter Lowdon (École Polytechnique, Paris)
    26/06/2020, 09:30
  2. 47. A Taste of the Flavour Problem - Is Symmetry the Missing Ingredient
    Miguel Levy (CFTP, Instituto Superior Técnico)
    26/06/2020, 10:10
    PhD student talk

    In this talk I will present some generalities on the paradigm of flavour symmetries, and the benefits that it encompasses. Given the large multiplicity of scenarios in which this paradigm is included, I will focus on two specific works (in progress): approximate Yukawa symmetries in the context of 2HDMs; and subgroup-preserving points (stabilizers) in the context of discrete modular symmetries...

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  3. 57. Constraints on the chi_c1 and chi_c2 polarizations
    Mariana Araújo
    26/06/2020, 10:25
    PhD student talk

    Hadron formation is a rather complex problem in the realm of non-perturbative QCD and remains an open question in HEP, despite the significant progress recently made through detailed phenomenological studies of several quarkonium production measurements made at the LHC. A new piece in the global panorama of quarkonium production data has recently been added by CMS: the first measurement of the...

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  4. 46. Functional renormalization group study of the critical region of the quark-meson model with vector interactions
    Renan Pereira (Centre for Physics of the University of Coimbra)
    26/06/2020, 10:40
    PhD student talk

    The critical region of the two flavour quark-meson model with vector interactions is explored using the Functional Renormalization Group, a non-perturbative method that takes into account quantum and thermal fluctuations. Special attention is given to the low temperature and high density region of the phase diagram, which is very important to construct the equation of state of compact stars....

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