21–29 Aug 2019
Europe/Athens timezone
ICNFP 2019 follows HiX 2019 (also at the OAC), Int. Workshop devoted to Nucleon Structure at Large Bjorken-x (https://indico.cern.ch/event/799284/overview). Related ICNFP Session organized with HiX 2019 convenors will take place the 22-23 August

Session

Workshop on New physics paradigms after Higgs and gravitational wave discoveries

27 Aug 2019, 10:00

Conveners

Workshop on New physics paradigms after Higgs and gravitational wave discoveries

  • Ignatios Antoniadis (CERN)

Workshop on New physics paradigms after Higgs and gravitational wave discoveries

  • Ignatios Antoniadis (CERN)

Workshop on New physics paradigms after Higgs and gravitational wave discoveries

  • Elena Arbuzova (Dubna State University and Novosibirsk State University)

Workshop on New physics paradigms after Higgs and gravitational wave discoveries

  • Peter Minkowski (Universitaet Bern (CH))

Presentation materials

There are no materials yet.

  1. Karim Benakli (Centre National de la Recherche Scientifique (FR))
    27/08/2019, 10:00

    Stochastic gravitational waves can be produced during the preheating when out-of-equilibrium particles are produced with an anisotropic stress-tensor. We discuss the case where these particles carry spin 3/2. We compute the spectrum of the gravitational waves generated by the transverse and longitudinal components. We find a different scaling of the spectrum near the peak and the longitudinal...

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  2. Mark Dayvon Goodsell (Univ. P. et Marie Curie Paris VI (FR))
    27/08/2019, 11:00

    Since new coloured states have been strongly constrained by LHC searches, extended electroweak sectors have become of paramount interest. However, the quantum corrections to these sectors can be very large; in the classic example of the MSSM, the Higgs mass has very large corrections at two loop order. On the other hand, in the MSSM, or even in the Two Higgs Doublet Model, the electroweak...

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  3. Dr Eugenio Megias (University of Granada)
    27/08/2019, 11:30
    Oral Presentation

    In this work we consider a warped five-dimensional model with an ultraviolet (UV) brane and, on top of the Standard Model zero modes, continua of KK modes with different mass gaps for all particles: gauge bosons, fermions, graviton, radion and Higgs boson. The model can be considered as a modelization in five dimensions of gapped unparticles. It has a singularity, at a finite (infinite) value...

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  4. Alexander Dolgov (NSU)
    27/08/2019, 12:00
  5. Paul Frampton (University of Salento)
    27/08/2019, 12:30
    Oral Presentation

    Primordial Intermediate Black Holes as Dark Matter

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  6. Dr Silvia Nagy (Silvia)
    27/08/2019, 13:00
    Oral Presentation

    It is known that de Sitter solutions in supergravity require supersymmetry breaking. I will present a new construction that allows the inclusion of the goldstino into supergravity, based on applying the Stueckelberg trick to a novel superfield formulation of unimodular supergravity. I will show the existence of de Sitter solutions and also the connection to the Volkov-Akulov model in the flat...

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  7. Ignatios Antoniadis (CERN)
    28/08/2019, 08:30
  8. Prof. Alexander Sorin (Joint Institute for Nuclear Research (RU))
    28/08/2019, 09:00

    For an isotropic cosmological model with a spatial curvature supported by a self-interacting scalar field minimally coupled to gravity, we construct and analyze a special integrable potential which approximates the potential of the Starobinsky R+R^2 inflationary model in the Einstein frame, and derive the general analytic solution of the corresponding Einstein–Friedmann equations. We...

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  9. Andrei Smilga
    28/08/2019, 11:00
    Oral Presentation

    Classical and quantum dynamics of higher derivative systems

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  10. Mariusz Dabrowski (University of Szczecin)
    28/08/2019, 11:30
    Oral Presentation

    I will briefly present the main ideas of the Generalized Uncertainty Principle (GUP) and the Extended Uncertainty Principle (EUP). Then, first I will discuss the impact of GUP onto the Bekenstein entropy and the Hawking temperature and show how GUP influences the Hawking radiation leaving a remnant of a radiating black hole. I will also show that when GUP is applied, the Hawking radiation does...

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  11. Elena Arbuzova (Dubna State University and Novosibirsk State University)
    28/08/2019, 12:00
    Oral Presentation

    Deviations of R^2 cosmology from the Einstein's General Relativity

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  12. Dmitry Gorbunov (Russian Academy of Sciences (RU))
    28/08/2019, 12:30

    Inflation can explain why the Universe is flat and homogeneous at large scales. However, it is not falsifiable unless also responsible for the matter perturbations sourcing the cosmic structure formation and anisotropy of cosmic microwave background. Moreover, even in that case different models often give (almost) the same predictions for the cosmological spectra, and it would be nice to test...

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  13. Herve Partouche
    28/08/2019, 13:00

    Phase transitions can occur in string theory, when the scale of spontaneous breaking of supersymmetry is of the order of the string scale. We describe these instabilities at the level of the effective supergravity at low energy. In this framework, infinitely many scalars that can become tachyonic are taken into account. They play the role of order parameters whose condensations yield various...

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