@Article{ATLASCollaborationAad_etal2013,
author="ATLAS Collaboration (Aad, G. et al
and Cabrera Urban, S.
and Castillo Gimenez, V.
and Costa, M. J.
and Fassi, F.
and Ferrer, A.
and Fiorini, L.
and Fuster, J.
and Garcia, C.
and Garcia Navarro, J. E.
and Gonzalez de la Hoz, S.
and Hernandez Jimenez, Y.
and Higon-Rodriguez, E.
and Irles Quiles, A.
and Kaci, M.
and Lacasta, C.
and Lacuesta, V. R.
and March, L.
and Marti-Garcia, S.
and Mi{\~A}{\textpm}ano, M.
and Mitsou, V. A.
and Moles-Valls, R.
and Moreno Llacer, M.
and Oliver Garcia, E.
and Pedraza Lopez, S.
and Perez Garcia-Esta{\~A}{\textpm}, M. T.
and Romero Adam, E.
and Ros, E.
and Salt, J.
and Sanchez Martinez, V.
and Soldevila, U.
and Sanchez, J.
and Torro Pastor, E.
and Valero, A.
and Valladolid Gallego, E.
and Valls Ferrer, J. A.
and Villaplana Perez, M.
and Vos, M.",
title="Search for microscopic black holes in a like-sign dimuon final state using large track multiplicity with the ATLAS detector",
journal="Physical Review D",
year="2013",
volume="88",
number="7",
pages="072001--22pp",
abstract="A search is presented for microscopic black holes in a like-sign dimuon final state in proton-proton collisions at root s = 8 TeV. The data were collected with the ATLAS detector at the Large Hadron Collider in 2012 and correspond to an integrated luminosity of 20.3 fb(-1). Using a high track multiplicity requirement, 0.6 +/- 0.2 background events from Standard Model processes are predicted and none observed. This result is interpreted in the context of low-scale gravity models and 95{\%} C.L. lower limits on microscopic black hole masses are set for different model assumptions.",
optnote="WOS:000325169600002",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=1614), last updated on Fri, 08 Nov 2013 11:38:05 +0000",
issn="1550-7998",
doi="10.1103/PhysRevD.88.072001",
opturl="http://arxiv.org/abs/arXiv:1308.4075",
opturl="https://doi.org/10.1103/PhysRevD.88.072001",
archivePrefix="arXiv",
eprint="arXiv:1308.4075"
}