XI School of Cosmology 17-22 September IESC, Cargese

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Translations in Relative Locality. Niccolò Loret with Giovanni Amelino-Camelia and Leonardo Barcaroli Università “La Sapienza” Roma. XI School of Cosmology 17-22 September IESC, Cargese. THE LOCALIZATION PROBLEM. PLANCK LENGTH. κ -MINKOWSKI. κ -POINCARE'. - PowerPoint PPT Presentation

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  • XI School of Cosmology17-22 September IESC, CargeseTranslations in Relative LocalityNiccol Loret

    with Giovanni Amelino-Camelia and Leonardo Barcaroli

    Universit La Sapienza Roma

  • THE LOCALIZATION PROBLEM-MINKOWSKIPLANCK LENGTH

  • -POINCARE'DEFORMED TRANSLATION GENERATORSCOALGEBRIC SECTORDEFORMED SIMPLETIC SECTOR

  • 1/cQuantum MechanicsGalilean RelativityQuantum Field TheorySpecial RelativityGeneral RelativityNewtonian GravityChandrasekhar RegimeQuantum GravityLOOPSSTRINGSBLACKHOLETHERMOD.BRONSTEIN-ZELMANOV-OKUN CUBE

  • RELATIVE LOCALITY LIMITWE STILL HAVE A DEFORMED MOMENTUM SPACE ATBUT NO WEIRD PLANCK LENGTH EFFECTS RELATED TO SPACETIME QUANTIZATIONDINSTANT NONLOCALITIES- What we really see in our telescopes and particle detectors are quanta arriving at different angles with different momenta and energies.

    - As naive observers looking out at the world, and no less as particle physicists and astronomers, we are basically calorimeters with clocksSPACETIME IS AN INFERENCE THAT WE BUILD ON MOMENTUM SPACE

  • CURVED MOMENTUM SPACESPACETIME TRANSLATIONS AS THE ACTION OF TOTAL MOMENTUM ON COORDINATESWE CAN EXPRESS NONLOCALITIES AS SOME SORT OF CURVATURE OF MOMENTUM SPACE:

  • WORDLINES IN RELATIVE LOCALITYMOMENTUM-DEPENDENT COORDINATES

  • RAINBOW METRICSCAN WE FORMALIZE SUCH EFFECTS INTO A METRIC? - We notice that a pointlike observer has to perform a translation in order to study the shape of the spacetime he is inIN THE MINKOWSKIAN LIMIT FROM -POINCARE' MODEL WE OBTAIN:

  • PHENOMENOLOGY ?FOCUSING IN THE DE SITTER CASE WE CAN EASELY CALCULATE THE RATIO BETWEEN THE OBSERVED WAVELENGTH IN ALICE AND BOB:

  • REFERENCES[1]G.Amelino-Camelia, J.Lukierski, A.Nowicki, Act.Phys.Pol. 4, Vol 29 (1998)[2]G.Amelino-Camelia, L.Freidel, J.Kowalski-Glikman, L.Smolin, Phys. Rev. D 84, 084010 (2011)[3]J. Magueijo, L.Smolin, Class. Quantum Grav. 21, 1725 (2004)[4]G.Amelino-Camelia, N.Loret, G.Rosati, Phys. Lett. B 700, 150-156 (2011)[5]G.Amelino-Camelia, N.Loret, G.Mandanici, F.Mercati, Int J. Mod. Phys. D 19, 2385-2392 (2010).[6]G.Amelino-Camelia, N.Loret, L.Barcaroli, in preparation[1] G.Amelino-Camelia, J.Lukierski, A.Nowicki, Act.Phys.Pol. 4, Vol 29 (1998)

    [2] G.Amelino-Camelia, L.Freidel, J.Kowalski-Glikman, L.Smolin, Phys. Rev. D 84, 084010 (2011)

    [3] J. Magueijo, L.Smolin, Class. Quantum Grav. 21, 1725 (2004)

    [4] G.Amelino-Camelia, N.Loret, G.Rosati, Phys. Lett. B 700, 150-156 (2011)

    [5] G.Amelino-Camelia, N.Loret, G.Mandanici, F.Mercati, Int J. Mod. Phys. D 19, 2385-2392 (2010)

    [6] G.Amelino-Camelia, N.Loret, L.Barcaroli, in preparation