Theoretical Physics Division seminar

  • English translation unavailable for DEEP LEARNING AND ITS BIGGEST ACHIEVEMENTS.
  • English translation unavailable for COHERENT STATES IN QUANTUM OPTICS: AN ORIENTED OVERVIEW.
  • English translation unavailable for RELATIVISTIC COSMOLOGY AND BACK-REACTION CONJECTURE .
  • English translation unavailable for ASYMPTOTIC SAFETY IN THE LIMIT OF LARGE N.
  • English translation unavailable for "Three examples of quantum dynamics on the half-line with smooth bouncing".
  • English translation unavailable for Reconstruction of light-cone parton distribution functions from lattice QCD simulations at the physical point.
  • English translation unavailable for DENSITY PERTURBATIONS IN THE COSMOLOGICAL SCENARIOS WITH SINGULARITIES.
  • English translation unavailable for EXACT QUANTUM DYNAMICS OF BOSE-FERMI SYSTEMS (QCD FOR EXAMPLE) VIA CLASSICAL FIELD STOCHASTIC EQUATIONS.

  • HARD PHOTOPRODUCTION OF A DIPHOTON WITH A LARGE INVARIANT MASS

    2017.12.08 7:40 - Anna Rędaszek

    The electromagnetic probe has proven to be a very efficient way to access the 3−dimensional structure of the nucleon, particularly thanks to the exclusive Compton processes. We explore the hard photoproduction of a large invariant mass diphoton in the kinematical regime where the diphoton is nearly forward and its invariant mass is the hard scale enabling to factorize the scattering amplitude in terms of generalized parton distributions. Our results include calculated unpolarized cross sections and the angular asymmetry, triggered by a linearly polarized photon beam.

  • CONNECTING LIGHT AND DARK SIDE OF THE UNIVERSE

    2017.11.16 14:45 - Anna Rędaszek

    Studies at low and intermediate redshift ranges show that the relation between the luminous structure and underlying dark matter distribution is not straightforward and depend on the various properties of galaxy population. Naturally one would like to extend these studies of the luminous-dark matter relations to the high redshift ranges (z>2) in order to improve our understanding of the evolution of the universe structure.

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