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Search for the Mini Black Hole in the Multijet Final State in pp Collisions at √ s = 7 TeV
A mini black hole search is motivated by theories of extra dimensions. ADD model is one of extra dimensions theories in which all extra dimen- sions are compactified in cylinder shape. In the model, only gravitational field can propagate into additional n dimensions. Hence, the fundamental gravitati...
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Lenguaje: | eng |
Publicado: |
2015
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Materias: | |
Acceso en línea: | http://cds.cern.ch/record/2041419 |
Sumario: | A mini black hole search is motivated by theories of extra dimensions. ADD model is one of extra dimensions theories in which all extra dimen- sions are compactified in cylinder shape. In the model, only gravitational field can propagate into additional n dimensions. Hence, the fundamental gravitational force is stronger than that measured in 3+1 space-time dimen- sions. This could lead the fundamental Planck scale, M D , of O (1) TeV in n + 4 dimensions, and solve the hierarchy problem where the Planck scale is vastly large compared with the electroweak scale. On the assumption of M D ∼ O (1) TeV, mini black holes with masses of O (1) TeV could be pro- duced at the Large Hadron Collider (LHC) at CERN. In this thesis, mini black holes were searched for in a multijet final state in proton-proton collisions at center of mass energy of 7TeV, produced by LHC. The collision data collected by the ATLAS detector in 2010, corresponding to the integrated luminosity of 36 . 3pb − 1 , were used in the search. The mini black hole signals for n = 2 to 7 and M D = 0 . 8 GeV to 2 TeV are searched for. For each n and M D , the mass thresholds of the mini black holes were set by the assumptions that colliding particles collapse in a black hole if the Compton wavelength is equal to or less than the Schwarzschild radius or horizon radius. In case M D = 1 TeV, the assumption with Schwarzschild (horizon) radius gives mass thresholds of about 2(3) TeV to 4(5) TeV for n = 7 to 2. Mini black holes are decaied mainly by the Hawking radiation. The model of no graviton emission is used for the decay of mini black holes. The burst model, in which mini black hole decay into multi-body, is adopted for the Planck Phase when the mass of mini black holes become smaller than the Planck Scale. Observed events are consistent with Standard Model predictions and up- per limits on the mini black hole production cross sections are set. This result can be interpreted to the lower limits on M D for each n by comparing with theoretical cross sections. On the assumption using Schwarzschild (horizon) radius, a lower limit on M D for n = 4 (5) is placed as M D > 1 . 26(1 . 06) TeV , at 95% confidence level, which is the most stringent limit obtained by the collider experiments |
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