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J.E. Horvath, IAG – USP São Paulo, Brazil

Concluding Remarks t o the 6 th IWARA . J.E. Horvath, IAG – USP São Paulo, Brazil. Olinto : colorful panorama of (non-accelerator) high-energy physics/astrophysics 10 6 x higher than a TeV scale (Higgs) !!.

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J.E. Horvath, IAG – USP São Paulo, Brazil

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  1. Concluding Remarks to the 6th IWARA J.E. Horvath, IAG – USP São Paulo, Brazil

  2. Olinto: colorful panorama of (non-accelerator) high-energy physics/astrophysics 106 x higher than a TeV scale (Higgs) !! R. Negreiros: discussion non-spherical effects (Cas A?) general scope G. Contrera: beyond simple models , non-local NJL confines, yet mean field solution developed C. Vasconcellos: “genuine” vs. “effective” 3 body forces. Mean field solution again !!!

  3. H. Stocker: a FAIR opportunity for extreme matter physics! FLAIR (antimatter) CMB, PANDA, NuStar neutron star physics Vacuum instability probed

  4. M. Malheiro: it is not easy to violate virial relations, no massive white dwarfs (B2 blows them away!) The Golden Age of ITA

  5. M. Alford: deep into the physical reasons of QCD pairing and its effects in NS Surface effects drive ‘crusts” in SS However… a few quark system sits probably in shell states, hence “strangelets” could be structured, not just “drops” S. Schramm: SU(3) grounded approach + excluded volume+ non-linear extra repulsion D. ManrezaParets: giving up spherical symmetry prolate “stars” (cuban cigars?), still problems with metric matching & EoS

  6. M. de Avellar: entropy as a tool to investigate composition H. Montoya: strong lensing reconstruction of mass distributions, cute but difficult M.E. Pereira: CFHT/MegaCam Stripe 82 Survey Galaxy morphology

  7. S. Perez Bergliaffa: relativistic Bondi-Hoyle accretion easier handling, still quite ideal L. Pellizza: the devilish details of supposedly known physics  our Universe in a simulation The concept of INFINITELY WRONG things D. Rodrigues: quantum effects at large scales G(μ) running constant, DM still needed

  8. M.E. Guimaraes/Xico: what is the true nature of Hawking radiation? M. Dvornikov: neutrinos in a gravitational field, explicit calculation of oscillations M. Reintjes: dealing with discontinuities in GR New observables? (distortion of GW?) R. Rosenfeld (a Very High Frequency guy): DES (dark energy + spinoffs) A. Perez Martinez: anomalous MM V. Pagura: more on non-local PNJL comparison with lattice

  9. Highlights * A truly dedicated organization, pro level * The quality of most poster presentations, highly rated by the organizers So long IWARA !!!

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